Arthur
C. Clarke
Profiles
of the Future:
An
Inquiry into the Limits of the Possible
Indigo,
Paperback, 2000.
8vo. ix+211 pp. Millennium Edition.
New Foreword by the author, April 1999 [1-3].
First published, 1962.
Second Revised Edition, 1973.
Third Revised Edition, 1982.
Millennium Edition by Gollancz, 1999.
Paperback reprint by Indigo, 2000.
Foreword to
Millennial Edition
This book began, in 1961, as a series
of essays for the Playboy magazine. They
were assembled in one volume the following year, and a revised edition was
published in 1982. It is hard to remember that the later date was two years
pre-Orwell, while the earlier one now seems halfway back to the Jurassic. What,
no VCRs, no laptops, no Internet, no World Wide Wait – sorry, Web – no CDRoms! How
did people manage to live in those primitive times?
Quite apart from the technological
revolution, largely due to the invention of the microchip, the last four
decades of the twentieth century also witnessed the greatest age of exploration
in human history. Although the landings on the Moon were the undoubted
highlights, equally important was the reconnaissance of all the planets (except
Pluto – whose status as a genuine planet is now being challenged!) by robot
probes. Though I had no doubt that all these events would occur, I never
expected to see them in my lifetime. Still less did I imagine that, after
reaching the Moon, we would abandon it for – how long? Your guess is as good as
mine, for the answer depends on politics and economics as much as on
technology.
This book’s subtitle is still an
accurate description of its intention: ‘An Inquiry into the Limits of the
Possible’. Not, be it noted, the probable – still less the desirable; in fact,
it will mention many very undesirable possibilities, as well as some desirable
impossibilities.
As the examples quoted in the opening
chapters amply demonstrate, ‘Impossible’ is an extremely dangerous word, and I
have tried to defined its sphere of application by Three Laws which were
originally enunciated in this book (the first now updated for Political
Correctness, though I do not guarantee continuing to do so):
1.
When
a distinguished but elderly scientist says that something is possible, (s)he is
almost certainly right. When (s)he says it is impossible, (s)he is very
probably wrong.
2.
The
only way of finding the limits of the possible is by going beyond them into the
impossible.
But perhaps the best-known, and most
often quoted, of the Laws is the Third:
3.
Any
sufficiently advanced technology is indistinguishable from magic.
Nowadays, there are innumerable proofs
of the Third Law, but here is my favourite: if anyone had told me, in 1962, that
one day there would be book-sized objects that would hold the contents of an
entire library, I would have believed him. But if they had said that I could
find any page – or even word – in an instant, and then display it in scores of
different typefaces ranging Albertus Extra Bold to Zurich Calligraphic, any
font size from 8 to 72, I would have protested that no imaginable technology
could perform such a feat. I can still remember seeing – and hearing! –
Linotype machines slowly converting molten lead into front pages that required
two strong men to lift them. Now, of course, Microsoft Word performs far
greater miracles, every day, in millions of homes all over the world.
And while we’re on the subject of the
word-processing revolution – how would a mid-century typist have reacted to the
prediction that within twenty years she’s spend most of her working hours
fondling a mouse?
[...]
Introduction
It is impossible to predict the
future, and all attempts to do so in any detail appear ludicrous within a very
few years. This book has a more realistic, yet at the same time more ambitious,
aim. It does not try to describe the
future, but to define the boundaries within which possible futures must lie. If
we regard the ages which stretch ahead of us as an unmapped and unexplored
country, what I am attempting to do is to survey its frontiers and get some
idea of its extent. The detailed geography of the interior must remain unknown
– until we reach it.
With a few exceptions, I am limiting
myself to a single aspect of the future – its technology, not the society that
will be based upon it. This is not such a limitation as it may seem, for
science will dominate the future even more than it dominates the past.
Moreover, it is only in this field that prediction is at all possible; there
are some general laws governing scientific extrapolation, as there are not (pace Marx) in the case of politics and
economics.
I also believe – and hope – that
politics and economics will cease to be as important in the future as they have
been in the past; the time will come when most of our present controversies on
these matters will seem as trivial, or as meaningless, as the theological
debates in which the keenest minds of the Middle Ages dissipated their
energies. Politics and economics are concerned with power and wealth, neither
of which should be the primary, still less the exclusive, concern of adult
human beings.
[...]
Over the last half century, tens of
thousands of stories have explored all the conceivable, and many of the
inconceivable, possibilities of the future; there are few things that can happen that have not been described
somewhere, in books or magazines. A critical – the adjective is important –
reading of science fiction is essential training for anyone wishing to look
more than ten years ahead. The facts of the future can hardly be imagined ab initio by those who are unfamiliar
with the fantasies of the past.
This claim may produce indignation,
especially among those second-rate scientists who sometimes make fun of science
fiction (I have never known a first-rate one to do so – and I knew several who
wrote it). But the simple fact is that anyone with sufficient imagination to
assess the future realistically would, inevitably, be attracted to this form of
literature. I do not for a moment suggest that more than one per cent of
science fiction readers would reliable prophets; but I do suggest that almost
one hundred per cent of reliable prophets will be science fiction readers – or
writers.
As for my own qualifications for the
job, I am content to let the published record speak for itself. Although, like
all other propagandists for space flight, I overestimated the time scale and
underestimated the cost, I am not in the least contrite about this error. Had
we known, back in the 1930s, that it was going to cost billions of dollars to
develop space vehicles, we would have been completely discouraged; in those
days no one could have believed that such sums would ever be available.
The speed with which space exploration
actually progressed would have seemed equally unlikely. When Hermann Oberth’s
pioneering book Die Rakete zu den Planetenraumen was reviewed by Nature in 1924, that journal remarked,
with great daring, ‘In these days of unprecedented achievements one cannot
venture to suggest that even Herr Oberth’s ambitious scheme may not be realised
before the human race becomes extinct.’ It had been realised, in large measure,
before Professor Oberth became extinct in 1989 – twenty years after the first
Moon landing!
I can claim a slightly better record
than Nature’s reviewer. On glancing
into my first novel Prelude to Space (written in 1947) I am amused to see that
I scored a direct hit by giving 1959 as the date of the first lunar impact, I
put manned satellites in 1970 and the landing on the Moon in 1978. This seemed
wildly optimistic to most people at the time, but now demonstrates my innate
conservatism. A still better proof of this is provided by the fact that I made
no attempt whatsoever, in 1945, to patent the communication satellite. I
couldn’t have done so, as it happens; but at least I would have made the
effort, had I dreamed that the first experimental models would be operating
while I was still in my forties.
In any event, this book is not
concerned with time scales – only with ultimate goals. At the present rate of
progress, it is impossible to imagine any technical feat that cannot be
achieved, if it can be achieved at
all, within the next hundred years. But for the purposes of this inquiry, it is
all the same whether the things discussed can be done in ten years, or in ten
thousand. My only concern is with what, not with when.
For this reason, many of the ideas
developed in this book will be mutually contradictory. To give an example, a
really perfect system of communication would have an extremely inhibiting
effect on transportation. Less obvious is the converse; if travel became
effortless and instantaneous, would anyone bother to communicate? The future
will have to choose between many competing superlatives; in such cases, I have
described each possibility as if the other did not exist.
In a similar manner, some chapters end
on an optimistic note, others on a pessimistic. According to the point of view,
both unlimited optimism and unlimited pessimism about the future are equally
justified. In the final chapter, I have tried to reconcile both.
It has been said that the art of
living lies in knowing where to stop, and going a little further (an early
version of my Second Law!). In Chapters 14 and 15 I have attempted to do this
by discussing conceptions which are almost certainly not science-fact, but
science-fantasy. Some people may regard a serious treatment of such ideas as
invisibility and the Fourth Dimension as a waste of time, but in this context
it is fully justified. It is as important to discover what cannot be done as
what can be done; and it is sometimes considerably more amusing.
While writing this introduction, I
came across a review of a somewhat pedestrian Russian book about the
twenty-first century. The distinguished British scientist writing the review
found the work extremely reasonable and the author’s extrapolations quite
convincing.
I hope this charge will not be
levelled against me. If this book seems completely reasonable and all my
extrapolations convincing, I will not have succeeded in looking very far ahead;
for the one fact about the future of which we can be certain is that it will be
utterly fantastic.
1. Hazards of
Prophecy: The Failure of Nerve
Before one attempts to set up in
business as a prophet, it is instructive to see what success others have made
in this dangerous occupation – and it is even more instructive to see where
they have failed.
With monotonous regularity, apparently
competent men have laid down the law about what is technically possible or
impossible – and have been proved utterly wrong, sometimes while the ink was
scarcely dry from their pens. On careful analysis, it appears that these débâcles
fall into two classes, which I will call Failures of Nerve and Failures of
Imagination.
The Failure of Nerve seems to be the
more common; it occurs when even given
all the relevant facts the would-be prophet cannot see that they point to
an inescapable conclusion. Some of these failures are so ludicrous as to be
almost unbelievable, and would form an interesting subject for psychological
analysis. ‘They said it couldn’t be done’ is a phrase that occurs throughout
the history of invention; I do not know if anyone has ever looked into the reasons
why ‘they’ said so, often with quite
unnecessary vehemence.
It is now impossible for us to recall the
mental climate which existed when the first locomotives were being built, and
critics gravely asserted that suffocation lay in wait for anyone who exceeded
the awful speed of twenty miles an hour. It is equally difficult to believe
that the idea of the domestic electric light was pooh-poohed by all the
‘experts’ – with the exception of a thirty-one-year-old American inventor
Thomas Alva Edison. When gas securities nose-dived in 1878 because Edison
(already a formidable figure, with the phonograph and the carbon microphone to
his credit) announced that he was working on the incandescent lamp, the British
Parliament set up a committee to look into the matter. (Westminster can beat
Washington hands down at this game.)
The distinguished witnesses reported,
to the relief of the gas companies, that Edison’s ideas were ‘good enough for
our transatlantic friends... but unworthy of the attention of practical or
scientific men.’ And Sir William Preece, engineer-in-chief of the British Post
Office, roundly declared that ‘Subdivision of the electric light is an absolute
ignis fatuus.’ One feels that the
fatuousness was not in the ignis.
The scientific absurdity being
pilloried, be it noted, is not some wild-and-woolly dream like perpetual
motion, but the humble little electric bulb, which for more than a century has
been part of everyday life, completely taken for granted, except when it burns
out...
Yet although in this matte Edison saw
far beyond his contemporaries, in later life he was also guilty of the same
short-sightedness that afflicted Preece, for he furiously opposed the
introduction of alternating current. However, his often unscrupulous campaign –
which included electrocuting animals to demonstrate the lethal properties of
a/c as opposed to d/c! – was probably dictated by economics rather than genuine
conviction. Edison’s direct-current system was engaged in a desperate battle
with the rival Westinghouse a/c network. It lost: but the Electric Chair is one
of Edison’s less-heralded bequests to the world.[1]
The most famous, and perhaps the most
instructive, failures of nerve have occurred in the fields of aero- and
astronautics. At the beginning of the twentieth century, scientists were almost
unanimous in declaring that heavier-than-air flight was impossible, and that
anyone who attempted to build aeroplanes was a fool. The great American
astronomer, Simon Newcomb, wrote a celebrated essay which concluded:
The demonstration that no
possible combination of known substances, known forms of machinery and known
forms of force, can be united in a practical machine by which man shall fly
long distances through the air, seems to the writer as complete as it is
possible for the demonstration of any physical fact to be.
Oddly enough, Newcomb was sufficiently
broadminded to admit that some wholly new discovery might make flight
practical. He even wrote a science fiction novel, incorporating the invention
of antigravity, so he certainly cannot be accused of lacking imagination; his error
was attempting to marshal the facts of aerodynamics, when he clearly did not
understand its basic principles. His failure of nerve lay in not realising that
the means of flight were already at hand.
For Newcomb’s article received wide
publicity at just about the time that the Wright brothers, not having a
suitable antigravity device in their bicycle shop, were mounting a gasoline
engine on wings. When news of their success reached the astronomer, he was only
momentarily taken aback. Flying machines might
be a marginal possibility, he conceded – but they were certainly of no
practical importance, for it was quite out of the question that they could
carry the extra weight of a passenger as well as that of a pilot.
[...]
Closer to the present, the opening of
the Space Age has produced a mass vindication (and refutation) of prophecies on
a scale and at a speed never before witnessed. Having taken some part in this
myself, and being no more immune than the next man to the pleasures of saying
‘I told you so,’ I would like to recall a few of the statements about space
flight that have been made by prominent scientists in the past. It is necessary
for someone to do this, and to jog
the remarkably selective memories of the pessimists. The speed with which those
who once declaimed ‘It’s impossible’ can switch to ‘I said it could be done all
the time’ is really astounding. (There is sometimes a third stage: ‘I thought
of it first.’)[2]
As far as the general public is
concerned, the idea of space flight as a serious possibility first appeared on
the horizon in the 1920s, largely as a result of newspaper reports of the work
of the American, Robert Goddard, and the Rumanian, Hermann Oberth (the much
earlier studies of Tsiolkovsky in Russia then being almost unknown outside his
own country). When the ideas of Goddard and Oberth, usually distorted by the
press, filtered through to the scientific world, they were received with hoots
of derision. For a sample of the kind of criticism the pioneers of astronautics
had to face, I present this masterpiece from a paper published by one Professor
A. W. Bickerton in 1926. It should be read carefully, for as an example of
cocksure thinking it would be very hard to beat.
This foolish idea of
shooting at the moon is an example of the absurd length to which vicious
specialisation will carry scientists working in thought-tight compartments. Let
us critically examine the proposal. For a projectile entirely to escape the
gravitation of the earth, it needs a velocity of 7 miles a second. The thermal
energy of a gramme at this speed is 15,180 calories... The energy of our most
violent explosive – nitroglycerine – is less than 1,500 calories per gramme. Consequently,
even had the explosive nothing to carry, it has only one-tenth of the energy
necessary to escape the earth... Hence the proposition appears to be basically
impossible...
Indignant readers in the Colombo
Public Library pointed angrily to the SILENCE notices when I discovered this
little gem. It is worth examining it in some detail to see just where ‘vicious
specialisation’, if one may coin a phrase, led the professor so badly astray.
His first error lies in the sentence:
‘The energy of our most violent explosive – nitroglycerine...’ One would have
thought it obvious that energy, not
violence, is what we want from a rocket fuel; and as a matter of fact
nitroglycerine and similar explosives contain much less energy, weight for
weight, that such mixtures as kerosene and liquid oxygen. This had been
carefully pointed out by Tsiolkovsky and Goddard years before.
Bickerton’s second error is even more
culpable. What does it matter if nitroglycerine has only a tenth of the energy
necessary to escape from the Earth? That merely means that you have to use at
least ten pounds of nitroglycerine to launch a single pound of payload.*
For the fuel
itself has
not got to escape from Earth; it can all be burned quite close to our planet,
and as long as it imparts its energy to the payload, this is all that matters. When
Lunik II lifted thirty-three years after Professor Bickerton said it was
impossible, most of its several hundred tons of kerosene and liquid oxygen
never climbed more than a few miles above Russia – but the half-ton payload
reached the Mare Imbrium.
As a comment on the above, I might add
that Professor Bickerton, who was an active populariser of science, numbered
among his published books one with the intriguing title Perils of a Pioneer. Of the perils that all pioneers must face, few
are more disheartening than the Bickertons.
Right through the 1930s and 1940s,
eminent scientists continued to deride the rocket pioneers – when they bothered
to notice them at all.
[...]
The lesson to be learned from these
examples is one that can never be repeated too often, and is one that is seldom
understood by laymen – who have an almost superstitious awe of mathematics. But
mathematics is only a tool, though an immensely powerful one. No equations,
however impressive and complex, can arrive at the truth if the initial
assumptions are incorrect. It is really quite amazing by what margins competent
but conservative scientists and engineers can miss the mark, when they start
with the preconceived idea that what they are investigating is impossible. When
this happens, the most well-informed men become blinded by their prejudices and
are unable to see what lies directly ahead of them. What is even more
incredible, they refuse to learn from experience and will continue to make the
same mistake over and over again.
Some of my best friends are
astronomers, and I am sorry to keep throwing stones at them – but they do seem
to have an appalling record as prophets. If you doubt this, let me tell you a
story so ironic that you might well accuse me of making it up. But I am not
that much of a cynic; the facts are on file for anyone to check.
Back in the dark ages of 1935, the
founder of the British Interplanetary Society, P. E. Cleator, was rash enough
to write the first book on astronautics published in England. His Rockets through Space gave an
(incidentally highly entertaining) account of the experiments that had been
carried out by the German and American rocket pioneers, and their plans for
such commonplaces of today as giant multi-stage boosters and satellites. Rather
surprisingly, the staid scientific journal Nature
reviewed the book in its issue for March 14, 1936, and summed up as follows:
It must be said at once
that the whole procedure sketched in the present volume presents difficulties
of so fundamental a nature that we are forced to dismiss the notion as
essentially impracticable, in spite of the author’s insistent appeal to put
aside prejudice and to recollect the supposed impossibility of heavier-than-air
flight before it was actually accomplished. An analogy such as this may be
misleading, and we believe it to be so in this case...
The reviewer, as was normal procedure,
was identified only by the unusual initials R.v.d.R.W.
In 1956 – the year after President Eisenhower had announced
the United States satellite program! – a
new Astronomer Royal arrived in England to take up his appointment. The press
asked him to give his views on space flight, and after two decades Dr Richard
van der Riet Woolley had seen no reason to change his mind. ‘Space travel’, he
snorted, ‘is utter bilge.’
The newspapers did not allow him to
forget this when Sputnik I went up the very next year. And later – irony piled
upon irony – Dr Woolley became, by virtue of his position as Astronomer Royal,
a leading member of the committee advising the British government on space
research. The feelings of those who had been trying, for a generation, to get
the United Kingdom interested in space can well be imagined.**[3]
Even those who suggested that rockets
might be for more modest, though much more reprehensible, purposes were
overruled by the scientific authorities – except in Germany and Russia.
In late 1944, when the existence of
the 200-mile-range V-2 was disclosed to an astonished world, there was
considerable speculation about intercontinental missiles. This was firmly
squashed by Dr Vannevar Bush, the civilian general of the United States
scientific war effort, in evidence before a Senate committee on December 3,
1945. Listen:
There has been a great deal
said about a 3,000 mile high-angle rocket. In my opinion such a thing is
impossible for many years. The people who have been writing these things that
annoy me, have been talking about a 3,000 mile high-angle rocket shot from one
continent to another, carrying an atomic bomb and so directed as to be a
precise weapon which would land exactly on a certain target, such as a city.
I say, technically, I don’t
think anyone in the world knows how to do such a thing, and I feel confident
that it will not be done for a very long period of time to come... I think we
can leave that out of our thinking. I wish the American public would leave that
out of their thinking.
A few months earlier (in May 1945)
Prime Minister Churchill’s scientific advisor Lord Cherwell had expressed
similar views in a House of Lords debate. This was only to be expected, for
Cherwell was an extremely conservative and opinionated scientist who had
advised the government that the V-2 itself was only a propaganda rumour.
In the May 1945 debate on defence,
Lord Cherwell impressed his peers by a dazzling display of mental arithmetic
from which he correctly concluded that a very long-range rocket must consist of
more than 90 per cent fuel, and thus would have a negligible payload. The
conclusion he let his listeners draw from this was that such a device would be
wholly impracticable.
This was true enough in the spring of
1945, but it was no longer true in the summer. One astonishing feature of the
House of Lords debate is the casual way in which much-too-well-informed peers
used the words ‘atomic bomb’, at a time when this was the best kept secret of
the war. (The New Mexico test was still two months in the future!) Security
must have been horrified, and Lord Cherwell – who of course knew all about the
Manhattan Project – was quite justified in telling his inquisitive colleagues
not to believe everything they heard, even though in this case it happened to
be perfectly true.
When Dr Bush spoke to the Senate
committee in December of the same year, the only important secret about the
atomic bomb was that it weighed five tons. Anyone could then work out in his
head, as Lord Cherwell had done, that a rocket to deliver it across
intercontinental ranges would have to weigh about 200 tons – as against the
mere fourteen tons of then awe-inspiring V-2.
The outcome was the greatest Failure
of Nerve in all history, which changed the future of the world – indeed,
perhaps of many worlds. Faced with the same facts and the same conclusions,
American and Russian technology took two separate roads. The Pentagon –
accountable to the taxpayer – virtually abandoned long-range rockets for almost
half a decade, until the development of thermonuclear bombs made it possible to
build warheads five times lighter yet several hundred times more powerful than
the low-powered and now obsolete device that was dropped on Hiroshima.
The Russians had no such inhibitions.
Faced with the need for a 200-ton rocket, they went right ahead and build it.
By the time it was perfected, it was no longer required for military purposes,
for Soviet physicists had bypassed the United States’ billion-dollar tritium cul-de-sac and gone straight to the far
cheaper and simpler lithium-hydride bomb. Having backed the wrong horse in
rocketry, the Russians then entered it for a much more important event – and
won the race into space.
Of the many lessons to be drawn from
this slice of history, the one that I wish to emphasise is this. Anything that
is theoretically possible will be achieved in practice, no matter what the
technical difficulties, if it is desired greatly enough. It is no argument
against any project to say: ‘The idea’s fantastic!’ Most of the things that
have happened in the last fifty years have been fantastic, and it is only by
assuming that they will continue to be so that we have any hope of anticipating
the future.
To do this – to avoid that Failure of
Nerve to which history exacts so merciless a penalty – we must have the courage
to follow all technical extrapolations to their logical conclusion. Yet even
this is not enough, as I shall now demonstrate. To predict the future we need
logic; but we also need faith and imagination which can sometimes defy logic itself.
______________________________
*The dead weight of the rocket
(propellant tanks, motor, etc.) would actually make the ratio very much higher,
but that does not affect the argument.
**In all fairness to Dr Woolley, I
would like to record that his 1936 review contained the suggestion – probably
for the first time – that rockets could contribute to astronomical knowledge by
making observations in ultra violet light beyond the absorbing screen of the
Earth’s atmosphere. Thanks to the orbiting astronomical observatories, this
idea has been overwhelmingly realised.
2. Hazards of
Prophecy: The Failure of Imagination
In the last chapter, I suggested that
many of the negative statements about scientific possibilities, and the gross
failures of past prophets to predict what lay immediately ahead of them, could
be described as Failures of Nerve. All the basic facts of aeronautics were
available – in the writings of Cayley, Stringfellow, Chanute, and others – when
Simon Newcomb ‘proved’ that flight was impossible. He simply lacked the courage
to face those facts. All the fundamental equations and principles of space
travel had been worked out by Tsiolkovsky, Goddard and Oberth for years – often
decades – when distinguished scientists were making fun of would-be astronauts.
Here again, the failure to appreciate the facts was not so much intellectual as
moral. The critics did not have the courage that their scientific convictions
should have given them; they could not believe the truth even when it had been
spelled out before their eyes, in their own language of mathematics. We all
know this type of cowardice, because at some time or other we all exhibit it.
The second kind of prophetic failure
is less blameworthy, and more interesting. It arises when all the available
facts are appreciated and marshalled
correctly – but when the really vital facts are still undiscovered, and the
possibility of their existence is not admitted.
A famous example of this is provided
by the philosopher Auguste Comte, who in his Cours de Philosophie Positive (1835) attempted to define the limits
within which scientific knowledge must lie. In his chapter on astronomy (Book
2, Chapter 1) he wrote these words concerning the heavenly bodies:
We see how we may determine
their forms, their distances, their bulk, their motions, but we can never know
anything of their chemical or mineralogical structure; and much less, that of
organised beings living on their surface.
We must keep carefully
apart the idea of the solar system and that of the universe, and be always
assured that our only true interest is in the former. Within this boundary
alone is astronomy the supreme and positive science that we have determined it
to be... the stars serve us scientifically only as providing positions with
which we may compare the interior movements of our system.
In other words, Comte decided that the
stars could never be more than celestial reference points, of no intrinsic
concern to the astronomer. Only in the case of the planets could we hope for
any definite knowledge, and even that knowledge would be limited to geometry
and dynamics. Comte would probably have decided that such a science as
‘astrophysics’ was a priori
impossible.
Yet within half a century of his
death, almost the whole of astronomy was astrophysics,
and very few professional astronomers had much interest in the planets. Comte’s
assertion had been utterly refuted by the invention of the spectroscope, which
not only revealed the ‘chemical structure’ of the heavenly bodies but also told
us far more about the distant stars than we knew of our planetary neighbours –
at least until recently.
Comte cannot be blamed for not
imagining the spectroscope; no one could
have imagined it, or the still more sophisticated instruments that have now
joined it in the astronomer’s armoury. But he provides a warning that should
always be borne in mind: even things that are undoubtedly impossible with
existing or foreseeable techniques may prove to be easy as a result of new
scientific breakthroughs. From their very nature, these breakthroughs can never
be anticipated; but they have enabled us to bypass so many insuperable
obstacles in the past that no picture of the future can hope to be valid if it
ignores them.
Another celebrated Failure of
Imagination was that persisted in by Lord Rutherford, who, more than any other
man, laid bare the internal structure of the atom. Rutherford frequently made
fun of those sensation-mongers who predicted that we would one day be able to
harness the energy locked up in matter. Yet only five years after his death in
1937, the first chain reaction was started in Chicago. What Rutherford, for all
of his wonderful insight, had failed to take into account was that a nuclear
reaction might be discovered that would release more energy than that required
to start it. To liberate the energy of matter, what was wanted was a nuclear
‘fire’ analogous to chemical combustion, and the fission of uranium provided
this. Once that was discovered, the harnessing of atomic energy was inevitable,
though without the pressures of war it might well have taken the better part of
a century.
The example of Lord Rutherford
demonstrates that it is not the man who knows most about a subject, and is the
acknowledged master of his field, who can give the most reliable pointers to
its future. Too great a burden of knowledge can clog the wheels of imagination;
I have tried to embody this fact in Clarke’s Third Law, which I make no excuse
for repeating here:
When a distinguished but
elderly scientist states that something is possible, he is almost certainly
right. When he states that something is impossible, he is very probably wrong.
Perhaps the adjective ‘elderly’
requires definition. In physics and mathematics it means over thirty; in other
disciplines, senile decay is sometimes postponed to the forties. There are, of
course, glorious exceptions; but as every researcher just out of college knows,
scientists of over fifty are good for nothing but board meetings, and should at
all costs be kept out of the laboratory...
[...]
One can only prepare for the
unpredictable by trying to keep an open and unprejudiced mind – a feat which is
extremely difficult to achieve, even with the best will in the world. Indeed, a
completely open mind would be an empty one, and freedom from all prejudices and
preconceptions is an unattainable ideal. Yet there is one form of mental
exercise that can provide good basic training for would-be prophets: anyone who
wishes to cope with the future should travel back in imagination to 1900 – and
ask just how much of today’s technology would be not merely incredible, but incomprehensible to the keenest
scientific brains of that time. 1900 is a good round date to choose, because it
was just about then that all hell started break loose in science.
[...]
The collapse of ‘classical’ science
actually began with Roentgen’s discovery of X-rays in 1895; here was the first
clear indication, in a form that everyone could appreciate, that the
commonsense picture of the universe was not sensible after all. X-rays – the
very name reflects the bafflement of scientists and laymen alike – could travel
through solid matter, like light through a sheet of glass. No one had ever
imagined or predicted such a thing; that one would be able to peer into the
interior of the human body – and thereby revolutionise medicine and surgery –
was something that the most daring prophet had never suggested. Indeed, the
titan of British physics, Lord Kelvin, roundly declared it was all a hoax...
The discovery of X-rays was the first
great breakthrough into the realms where no human mind had ever ventured
before. Yet it gave scarcely a hint of still more astonishing developments to
come – radioactivity, the internal structure of the atom, Relativity, the
Quantum Theory, the Uncertainty Principle...
As a result of this, the inventions
and technical devices of our modern world can be divided into two sharply
defined classes. On the one hand there are those machines whose would have been
fully understood by any of the great thinkers of the past; on the other, there
are those that would be utterly baffling to the finest minds of antiquity. And
not merely of antiquity; there are devices now in common use that might well
have driven Edison or Marconi insane had they tried to fathom their operation.
Let me give some examples to emphasise
this point. If you showed a modern diesel engine, an automobile, a steam
turbine, or a helicopter to Benjamin Franklin, Galileo, Leonardo da Vinci, and
Archimedes – a list spanning a time period of two thousand years – not one of
them would have any difficulty in understanding how these machines worked.
Leonardo, in fact, would recognise several from his notebooks! All four men
would be astonished at the materials and the workmanship, which would have
seemed magical in its precision, but once they had got over that surprise they
would feel quite at home – as long as they did not delve too deeply into the
auxiliary control and electrical systems.
But now suppose that they were
confronted by an electronic computer, a nuclear reactor, a radar set, a VCR.[4]
Quite apart from the complexity of these devices, the individual elements of
which they are composed would be incomprehensible to any man born before this
century. Whatever his degree of education or intelligence, he would not possess
the mental framework that could accommodate electron beams, transistors, atomic
fission, microchips and cathode-ray tubes.
The difficulty, let me repeat, is not
one of complexity; some of the – apparently – simplest modern devices, such as
the featureless silver platter of a DVD, would be the most difficult to
explain. A more dramatic example is the atomic bomb...[5]
[...]
The wholly unexpected discovery of
uranium fission in 1939 made possible such absurdly simple (in principle, if
not in practice) devices as the atomic bomb and the nuclear chain reactor. No
scientist could ever have predicted them; if he had, all his colleagues would
have laughed at him.
It is highly instructive, and
stimulating to the imagination, to make a list of the inventions and
discoveries that have been anticipated – and those that have not. Here is my
attempt to do so. All the items on the left have already been achieved or
discovered, and all have an element of the unexpected or the downright
astonishing about them. To the best of my knowledge, not one was foreseen very
much in advance of the moment of revelation.
On the right, however, are concepts
that have been around for hundreds or thousands of years. Some have been
achieved; others will be achieved; others may be impossible. But which?
|
The
Unexpected |
The
Expected |
|
X-rays |
Automobiles |
|
Nuclear energy |
Flying machines |
|
Radio, TV |
Steam engines |
|
Electronics |
Submarines |
|
Photography |
Spaceships |
|
Sound recording |
Telephones |
|
Quantum mechanics |
Death rays |
|
Relativity |
Transmutation |
|
Transistors |
Artificial life |
|
Masers; lasers |
Immortality |
|
Superconductors; superfluids |
Invisibility |
|
Atomic clocks; Mössbauer effect |
Levitation |
|
Determining composition of celestial
bodies |
Teleportation |
|
Dating the past (Carbon 14, etc.) |
Communication with dead |
|
Detecting invisible planets |
Observing the past and the future |
|
The ionosphere; van Allen belts |
Telepathy |
The right-hand list is deliberately provocative;
it includes sheer fantasy as well as serious scientific speculation. But – to
repeat my Second Law – the only way of discovering the limits of the possible
is to venture a little way past them into the impossible. In the chapters that
follow, this is exactly what I propose doing; yet I am very much afraid that
from time to time I too will exhibit Failure of Imagination – if not Failure of
Nerve. For as I glance down the left-hand column I am aware of a few items
which, not many years ago, I would have thought were impossible...
3. The Future
of Transport
Most of the energy expended in the
history of the world has been used to move things from one place to another. For
thousands upon thousands of years, the rate of movement was very slow – about
two or three miles an hour, the pace of a walking man. Even the domestication
of the horse did not raise this figure appreciably, for though a racehorse can
exceed forty miles an hour for very short periods, the main use of the horse
has always been as a slow-moving beast of burden or hauler of vehicles. The
fastest of these – the stagecoaches immortalised by Dickens – could seldom have
travelled at more than ten miles an hour on the roads that existed before the
nineteenth century.
For almost the whole of history and
prehistory, therefore, humanity’s thoughts and ways of life have been
restricted to the tiny band of the speed spectrum between one and ten miles an
hour. Yet within the span of a few generations, the velocity of travel has been
multiplied more than a thousandfold; indeed, there are good grounds for
thinking that the acceleration that took place round the mid-twentieth century
will never again be matched.
Speed, however, is not the only
criterion of transport, and there are times when it is positively undesirable –
especially if it conflicts with safety, comfort or economics. As far as
transportation at ground level is concerned, we may well have reached (if not
passed) the practical limit of speed, and future improvements must lie in other
directions. No one wants to travel down Fifth Avenue at the velocity of sound,
but most New Yorkers would be very happy if they could always be sure of doing
so at the speed of a stagecoach.
[...]
Yet, it is becoming obvious that vehicles
– except public utility ones – cannot be permitted much longer in urban areas.
We have taken some time to face this fact; more than two thousand years have
passed since increasing traffic congestion in Rome compelled Julius Caesar to
ban all wheeled vehicles during the hours of daylight, and the situation has
become slightly worse since 46 BC. If private cars are to continue operating inside
cities, we will have to put all the buildings on stilts so that the entire
ground area can be used for highways and parking lots – and even this may not
solve the problem.
[...]
Even if they are banned from the city,
motor vehicles are likely to dominate the short (10–100 mile) range of
transportation for a long time to come. There is no one now alive who can remember
when it was otherwise – the automobile has become so much a part of our
existence. Though it was conceived in the late Nineteenth, it is essentially a
child of the Twentieth Century.
Looked at dispassionately, it is an
incredible device, which no sane society would tolerate. If anyone before 1900
could have seen the approaches to a modern city on a Monday morning or a Friday
evening, he might have imagined that he was in hell – and he would not be far
wrong. Here we have a situation in which millions of vehicles, each miracle of
(often unnecessary) complication, are hurtling in all directions under the
impulse of anything up to two hundred horsepower. Many of them are the size of
small houses and contain a couple of tons of sophisticated alloys – yet often
carry only a single passenger. They can travel at a hundred miles an hour, but
are lucky if they average forty. In one lifetime they have consumed more
irreplaceable fuel than has been used in the whole previous history of mankind.
The roads to support them, inadequate though they are, cost as much as a small war;
the analogy is a good one, for the casualties are on the same scale.
Yet despite the appalling expense in
spiritual as well as material values (look what Detroit has done to aesthetics)
our civilisation could not survive for ten minutes without the automobile.
Though it can obviously be improved, it seems hard to believe that it can be
replaced by anything fundamentally different. The world has moved on wheels for
six thousand years, and there is an unbroken sequence from of cart to
Rolls-Royce and Mercedes-Benz.[6]
Yet one day the sequence will be broken – perhaps by ground effect
vehicles riding on air blasts, perhaps by gravity control, perhaps by still
more revolutionary means. I shall discuss these possibilities elsewhere;
meanwhile, let us take a brief glance at the future of the automobile as we
know it.
It will become much lighter – and
hence more efficient – as materials improve. Its complicated and toxic gasoline
engine (which has probably killed as many people by air pollution as by direct
physical impact) will be replaced by clean and silent electric motors, built into
the wheels themselves and so wasting no body space. This implies, of course, the
development of a really compact and lightweight method of storing or producing
electricity, at least an order of magnitude better than our present clumsy
batteries. Such an invention has been overdue for the best part of a century;
it may be made possible either through improvements in fuel cells, or as a
by-product of solid-state physics. An alternative that has attracted much
attention is fly-wheel energy storage, already used in some buses.[7]
These improvements, however, will be
much less important than the fact that the automobile of the day-after-tomorrow
will not be driven by its owner, but by itself; indeed, it may one day be a
serious offence to drive an automobile on a public highway. I would not care to
say how long it will take to introduce completely computerised motoring, but
dozens of techniques already developed by airlines and railroads already point
the way to it. Automatic spacing, electronic road signs, radar obstacle
detectors, navigational grids – already we have the basic elements required, and
many have been tested experimentally, especially in Japan. An automatic highway
system will, of course, be fabulously expensive to install and maintain – but
in the long run it will be much cheaper, in terms of time, frustration, and
human lives, than the present manual one.
The automobile of the future will
really live up to the first half of its name; you need merely tell it your
destination – by dialling a code, or perhaps even verbally – and it will travel
there by the most efficient route, after first checking with the highway
information system for blockages and traffic jams. As a mere incidental, this
would virtually solve the parking problem. Once your car had delivered you to
the office, you could instruct it to head out of town again. It would then
report for duty in the evening when summoned by radio, or at a prearranged
time. This is only one of the advantages of having a built-in chauffeur.
Some people, I know, enjoy driving,
for reasons which are simple and perhaps[8]
Freudian, though none the worse for that. Their desires could easily be
fulfilled at dedicated race-tracks – but not
on the public highways.
The most revolutionary – indeed, from
the viewpoint of all earlier ages the most incredible – event in the history of
transport has been the rise of aviation. Eventually all passenger traffic will
go by air when stage-lengths of more than a couple of hundred miles are
concerned; the railroads recognised this long time ago, as is proved by their
often unconcealed efforts to discourage customers. They would much prefer to
concentrate on freight, which is more profitable and far less troublesome, for
it is seldom in a frantic hurry and does not object to being parked in sidings
for a few hours. Nor does it insist that its feet be warmed and its martinis
chilled – vide Peter Arno’s once-famous cartoon, which showed an irate
passenger in the club car, holding up an unsatisfactory drink and complaining,
‘This is a hell of a way to run a railroad.’[9]
The story of the railroads, which have
served mankind so well for almost a century and a half, is now entering its
final chapter. As industry becomes decentralised, as the use of coal for fuel
diminishes and self-contained power sources enable factories to move nearer to
their sources of supply, so the very need for shifting megatons of raw
materials over thousands of miles will dwindle away.
Already some young countries –
Australia, to give a middle-aged example – have virtually bypassed the railroad
age and are building transportation systems based on highways and airlines. The
day will come, if it has not already, when Pullmans and diners and roomettes
will be as much period pieces as the Mississippi paddle-boats, and will evoke
equal nostalgia.
Nevertheless, by a strange paradox it
is quite possible that the heroic age of railroads still lies ahead. On airless
worlds like the Moon, Mercury, and the satellites of the giant planets,
alternative forms of transport may be impracticable, and the absence of
atmosphere will permit very high speeds even at ground level. Such a situation
almost demands railroads, or equivalent systems. On rugged, low-gravity worlds
there is a good deal to be said for cars suspended from overhead monorails or
cables, which could be slung across valleys and chasms and craters, with
complete indifference to the geography below them. A century from now, the face
of the Moon may be covered with such a network, linking together the
pressurised cities of the first extraterrestrial colony.
[...]
When this chapter was first written,
the Mach 2 (1,200 mph) Concorde was still fourteen years in the future. A
technological triumph, but an economic disaster (like that other one-off
product, the Space Shuttle!), it now appears that it will have no successors,
for commercial and environmental reasons rather than engineering ones. After
much initial optimism, and the expenditure of millions of dollars, dreams of
hypersonic – say Mach 10 – flight for paying passengers seem to have faded out.
To mix metaphors slightly, has commercial aviation come to the end of the line?
Before we jump to that conclusion, here is another cautionary tale from the
past, almost matching the Pickering débâcle
quoted in Chapter One.[10]
Back in 1929 a leading aeronautical
engineer, who later became a famous author (I’ll give his name in a moment, he
was the Tom Clancy of his day[11])
wrote a paper on the future of aviation which opened with the words: ‘The
forecast is freely made that within a few years passengers-carrying aeroplanes
will be travelling at over 300 mph, the speed record today.’ This, he stated
pontifically, was gross journalistic exaggeration, as ‘the commercial aeroplane
will have a definite range of development ahead of it beyond which no further
advance can be anticipated.’
Here are the advances this farsighted
prophet anticipated when the aeroplane had reached the limit of its
development, probably by the year 1980:
Speed: 110–130 mph
Range: 600 miles
Payload: 4 tons
Total weight: 20 tons
Well, every one of these figures had
been multiplied by more than five by the time their proponent died in 1960,
mourned by thousands of readers in many countries. For in 1929 he was N. S.
Norway, chief calculator on the R100 airship design; but in 1960 he was famous
as Nevil Shute. One can only hope, as he himself must have done, that his
post-nuclear-war novel On the Beach
turns out to be as wide of the mark as this earlier and lesser-known
prediction.
[...]
4.
Riding on Air
Re-reading this chapter, after almost
forty years, has been a chastening – even embarrassing – experience. Despite
the obvious temptation, I have left the original text unchanged, apart from
minor editorial corrections, as a splendid example of the Perils of Prediction.
Apologies and excuses will be found in
the postscript.
[...]
Postscript,
30 years later...
Well, it hasn’t worked out quite that
way – yet...
However, some of my less optimistic
extrapolations have come true. GEMs are in widespread use for tourism (e.g.
Channel crossing, the Adriatic) and very large models have been built for
military applications. There is one Russian monster in the multi-thousand ton
class, which caused great apprehension in Western intelligence circles when
first spotted by reconnaissance satellites. It’s probably moth-balled now,
while its rouble-starved owners wait for some Hollywood producer willing to pay
the fuel bills.
And that may be one of several reasons
why family-sized, private GEMs never became popular, except with more affluent
members of the sporting-car set. They are gas-guzzlers – as well as being
noisy, and prone to rearranging the ground over which they float.
I discovered this when, during my
initial enthusiasm, I imported a four-seater ‘Hover Hawk’ into Sri Lanka. It
was great fun to drive, but only in large open spaces: because steering
depended on rudders, it had poor lateral control. I would never have dared to
take it on a busy highway, and on water, visibility was liable to be obscured
by clouds of spray.
My final excursion was on a wide
beach, which seemed a safe enough venue. However, I failed to notice a small
pile of brushwood in time to avoid it, and the flexible rubber skirt which
trapped the supporting bubble of air was torn open. With a mournful sigh, my
Hover Hawn sank on to the sand.
It would have been easy enough to
repair the trivial damage, but I decided not to bother, and presented the
vehicle to the University of Moratuwa’s Engineering Department.
That was twenty years ago. I have
never driven anything since, without or without wheels.
5. Beyond
Gravity
Of all the natural forces, gravity is
the most mysterious and the most implacable. It controls our lives from birth
to death, killing or maiming us if we make the slightest slip. No wonder that,
conscious of their earthbound slavery, men have always looked wistfully at
birds and clouds, and have pictured the sky as the abode of the gods. The very
expression ‘heavenly being’ implies a freedom from gravity which, until the
present, we have known only in our dreams.
There have been many explanations of
those dreams, some psychologists trying to find their origin in our assumed
arboreal past – though it is unlikely that many of our ancestors spent their
lives jumping from tree to tree, and any who experienced more than one second
of free fall could have made no further contribution to the human gene – or
meme – bank. One could argue almost as convincingly that the familiar
levitation dream is not a memory from the past, but a premonition of the
future. Some day ‘weightlessness’ or reduced gravity will be a common, and
perhaps even a normal, state of mankind. The day may come when there are more
people living on space stations and worlds of low gravity than on the Mother
Planet; indeed, when the history of our race is written, the estimated one
hundred billion humans who have already spent laborious lives struggling against
gravitation may turn out to be a tiny minority. Perhaps our space-faring
descendants will be as little concerned with gravity as were our first
ancestors when they floated effortlessly in the buoyant sea.
Even now, most of the creatures on
this planet are hardly aware that gravity exists. Though it dominates the lives
of large land animals such as elephants, horses, H. sapiens and dogs, to anything much smaller than a mouse it is
seldom more than a mild inconvenience. To insects it is not even that; flies
and mosquitoes are so light and fragile that the air itself buoys them up, and
gravity bothers them no more than it does a fish.
But it bothers us a great deal,
especially now that we are making determined efforts to escape from it. Quite
apart from its relevance to space flight, the problem of gravitation has always
worried physicists. It seems to stand completely
apart from all the other forces – light, heat, electricity, magnetism – which
can be generated in many different ways, and are freely interconvertible. Indeed,
most of modern technology is based upon such conversions – of heat into
electricity, electricity into light, and so on.
Yet we cannot generate gravity at all,
and it appears completely indifferent to all the influences which we may bring
to bear on it. As far as we know, the only way a gravitational field can be
produced is by the presence of matter. Every particle of matter has an
attraction for every other particle of matter in the universe, and the sum
total of those attractions, in any one spot, is the local gravity. Naturally,
this varies from world to world, since some planets contain large amount of
matter and others very little. In our solar system the three giant planets
Jupiter, Saturn and Neptune all have surface gravities greater than Earth’s –
two and a half times greater, in the case of Jupiter. At the other extreme,
there are moons and asteroids where gravity is so low that one would have to
look at a falling object for several seconds to be certain that it was moving.
Gravitation is an incredibly, almost
unimaginably, weak force. This may
seem to contradict both common sense and everyday experience, yet when we
consider the statement it is obviously true. Really gigantic quantities of
matter – the six thousand million million million tons of the Earth – are
required to produce the rather modest gravity field in which we live. We can
generate magnetic or electric forces hundreds of times more powerful with a few
pounds of iron or copper. When you lift a piece of iron with a simple horseshoe
magnet, the amount of metal the magnet contains is outpulling the whole Earth. The
extreme weakness of gravitational forces makes our total inability to control
or modify them all the more puzzling and exasperating.
From time to time, one hears rumours
that research teams are working on the problem of gravity control, or
‘anti-gravity’, but these stories usually turn out to be misinterpretations. No
competent scientist, at this stage of our ignorance, would deliberately set out
to look for a way of overcoming gravity. What a number of physicists and
mathematicians are doing, however, is something less ambitious: they are simply
trying to uncover basic knowledge about gravity. If this plodding, fundamental
work does lead to some form of gravity control, that will be wonderful, but I
doubt if many people in the field believe that it will. The opinion of most
scientists is well summed up by a remark once made by Dr John Peerce, Father of
Telstar and part-time science fiction writer: ‘Anti-gravity,’ he said, ‘is
strictly for the birds.’ But the birds don’t need it – and we do.
We still know so little about
gravitation that we are not even sure if it travels through space at a definite
speed – like radio or light waves – or whether it is ‘always there’. Until the
time of Einstein, scientists thought that the latter was the case, and that
gravitation was propagated instantaneously. Today, the general opinion is that
it travels at the speed of light and that, also like light, it has some kind of
wave structure.
Gravitational waves will be
fantastically difficult to detect, because they carry very little energy. It
has been calculated that the gravity waves radiated by the whole Earth have an
energy of about a millionth of a horsepower, and the total emission from the
entire solar system – the Sun and all the planets – is only half a horsepower. There
is good evidence that gravitational radiation has been detected from very
dense, rapidly moving stars, but any conceivable man-made generator would be
billions of billions of times feebler than this.
[...]
It is also probable that we will not
make much progress in understanding gravity until we are able to isolate
ourselves and our instruments from it by establishing laboratories in space. Attempting
to study it on the Earth’s surface is rather like testing hi-fi equipment in a
boiler factory; the effects we are looking for may be swamped by the
background. Only in a satellite laboratory will we be able to investigate the
properties of matter under weightless conditions.
The reason why objects are – usually –
weightless in space is one of those elusive simplicities that is almost
invariably misunderstood. Most people are probably still under the impression
that astronauts are weightless because they are ‘beyond the pull of gravity’.
This is completely wrong. Nowhere in
the universe – not even in the remotest galaxy that appears as a faint smudge
on a Hubble Telescope image – would one be literally beyond the pull of Earth’s
gravity, though a few million miles away it is completely negligible. It falls
off slowly with distance, and at the modest altitudes reached by the first
astronauts it was still almost as powerful as at sea level. When Yuri Gagarin
looked down on Earth from a height of nearly two hundred miles, the gravity
field in which he was moving still had ninety percent of its normal value. Yet,
despite that, he weighed exactly nothing.
If this seems confusing, it is largely
due to poor semantics. The trouble is that we dwellers on the Earth’s surface
have grown accustomed to using the words ‘gravity’ and ‘weight’ almost
interchangeably. In ordinary terrestrial situations, this is safe enough; whenever
there’s weight there’s gravity, and vice
versa. But they are really quite separate entities, and either can occur independently
of the other. In space, they normally do.
On occasion, they can do so on Earth,
as the following experiment will prove. I suggest you think about it rather
than actually conducting it, but if you are unconvinced by my logic, go right
ahead. You will have the tremendous precedent of Galileo, who also refused to
accept argument but appealed to experimental proof. However, I disclaim all
responsibility for any damage.
You will need a quick-acting trapdoor
(one of those used by hangmen will do admirably) and a pair of bathroom scales.
Put the scales on the trapdoor and stand on them. They will, of course,
register your weight.
Now, while your eyes are fixed on the
scale, get one of your acquaintances (‘That’s not an office for a friend, my
lord,’ as Volumnius said to Brutus on a slightly similar occasion) to spring
the trapdoor. At once the needle will drop to zero; you will be weightless. But
you will certainly not be beyond the pull of gravity; you will be one hundred
per cent under its influence, as you will discover a fraction of a second
later.
Why are you weightless in these
circumstances? Well, weight is a force,
and a force cannot be felt if it has no point of application – if there is
nothing for it to push against. You cannot feel any force when you push against
a freely swinging door; nor can you feel any weight when you have no support
and are falling freely. An astronaut, except when the spaceship’s rockets are
firing, is always falling freely. The ‘fall’ may be downwards or upwards or
sideways – as in the case of an orbital satellite, which is in an eternal fall
around the world. The direction does not matter; as long as the fall is free
and unrestrained, anyone experiencing it will be weightless.
You can be weightless, therefore, even
if there is plenty of gravity. The reverse is also true; you don’t need gravity
to give you weight. A change of speed – in other words, an acceleration – will
do just as well.
[...]
It is conceivable that by some
treatment we might permanently ‘degravitise’ ordinary substances, in much the
same way that we can turn a piece of iron into a permanent magnet. (Less
well-known is the fact that continuously charged bodies – ‘permanent electrets’
– can also be made.) To do so would require a great expenditure of energy, for
to degravitise one ton of matter is equivalent of lifting it completely away
from the Earth. As any rocket engineer will tell you, this requires as much
energy as raising four thousand tons a height of one mile. That four thousand
mile-tons of energy is the price of weightlessness – the entrance fee to the
universe. There are no concession and no cheap rates. You may have to pay more,
but you can never pay less.
On the whole, a permanently
degravitised or weightless substance seems less plausible than the gravity
neutraliser or ‘gravitator’. This would be a device, supplied with energy from
some external power source, which will cancel gravity as long as it was
switched on. It is important to realise that such a machine would give not only
weightlessness, but something even more valuable – propulsion.
For if we exactly neutralised weight,
we would float motionless in midair; but if we over-neutralised it, we would shoot upwards with steadily
increasing speed. Thus any form of
gravity control would also be a propulsion system; we should expect this,
as gravity and acceleration are so intimately linked. It would be a wholly
novel form of propulsion, and it is difficult to see what it would ‘push
against’. Every prime mover must have some point of reaction; even the rocket,
the only known device that can give us a thrust in vacuum, pushes on its own
burned exhaust gases. (We premature Space Cadets spent much of our youth explaining
this to sceptics: in 1920 the New York
Times published an editorial – for which it apologised in 1969 –
castigating Goddard for his apparent ignorance of this elementary law of
physics.)
The term ‘space drive’, or just plain
‘drive’, has been coined for such nonexistent but highly desirable propulsion
systems. It is an act of faith among science fiction writers, and an increasing
number of people in the astronautics business, that there must be some quieter,
cheaper and safer way of getting to the planets than the rocket. The tanks of the
Space Shuttle contain as much energy as an atomic bomb – and as ‘Challenger’
demonstrated so tragically, it is not always reliably controlled.
It may seem a little premature to
speculate about the uses of a device which may not even be possible, and is certainly
beyond the present horizon of science. But it is a general rule that whenever
there is a technical need, something always comes along to satisfy it – or to
bypass it. For this reason, I feel sure that eventually we will have some means
of either neutralising gravity or overpowering it by brute force. In any event,
it will give us both levitation and propulsion, in amounts determined only by
the available power.
[...]
The value of gravity control for space
vehicles, both for propulsion and the comfort of their occupants, needs no
further discussion – but there are other astronautical uses that are not so
obvious. Jupiter, the largest of the planets, appears barred from direct human
exploration by its high gravity, two and a half times that of Earth. This giant
world has so many other unpleasant characteristics (an enormously dense,
turbulent and poisonous atmosphere, for example) that few would take very
seriously the idea that we will ever attempt personal exploration; surely we
will always rely on robots...
I doubt this; in any event, there will
often be cases when robots run into trouble and humans will have to get them
out of it, as has already been demonstrated in near-Earth orbit. Sooner or
later scientists – even tourists! – will wish to visit Jupiter – perhaps in
‘hot hydrogen’ balloons. (See my novella ‘A Meeting with Medusa’ for the
technology – and dangers – involved.*)
Before it was known that Jupiter had
no solid surface, John W. Campbell, the famed editor of Analog Magazine, suggested that we might have to breed a special
class of Jovian colonists with the physiques of gorillas. Though this won’t
happen, much closer to home there is an even more important example of a
high-gravity planet which, perhaps less than fifty years from now, humans may
not be able to visit. That planet is our own Earth.
Without gravity control, we may be
condemning the space travellers and settlers of the future to perpetual exile.
Anyone who had lived for a few years on the Moon, at only a sixth of
terrestrial ‘g’, would be a helpless cripple back on Earth. It might take him
months of painful practice before they could walk again, and children born on
the Moon (as they soon will be[12])
might never be able to make the adjustment. One can think of few things more
likely to breed bitterness and interplanetary discord than such gravitational
expatriation.
To avoid this we need a really
portable gravity-control unit, so compact that it could be strapped it on the
shoulders or round the waist. Indeed, it might even be a permanent article of
clothing, taken as much for granted as the wristwatch or the personal communication
device. It could use it to reduce one’s apparent weight down to zero, and also
to provide propulsion.
Anyone who is prepared to admit that
gravity control is possible at all should not boggle at this further
development. Miniaturisation is one of the everyday miracles of our age, for
better or for worse. The first thermonuclear bomb was as big as a house;
today’s economy-sized warheads are the size of a wastepaper basket – and one of
those baskets contains enough energy to carry a large ocean liner to the Moon,
though not in one piece. This everyday fact of modern missilery is, I submit, is
just as fantastic as the possibility of personal gravity control.[13]
The one-person gravitator, if it could
be made cheaply enough, would be among the most revolutionary inventions of all
times. Like birds and fish, we would have escaped from the tyranny of the
vertical – we would have gained the freedom of the third dimension. In the
city, no one would use the elevator if there was a convenient window. The
degree of effortless mobility that would be attained would demand re-education
to an entire new way of life – an almost avian order of existence. By the time
it arrives, it will not be unfamiliar, for countless films of spacemen in orbit
will have made everyone accustomed to the idea of weightlessness, and eager to
share its pleasures. Perhaps the levitator may do for the mountains what the
aqualung had done for the sea. The Sherpas and Alpine guides will, of course,
be indignant; but progress is inexorable. It is only a matter of time before
tourists are floating all over the Himalayas, and the summit of Everest is as
crowded as the seabed round the Florida Keys or off Cannes.**
[...]
_________________________________
*In the collection The
Wind From the Sun.
**See my short story ‘The Cruel Sky’
in The
Wind From the Sun.
8. Rocket to
the Renaissance
Foreword
This essay originally appeared in a
1960 Playboy magazine, and summarises my hopes and expectations in the first
dawn of the Space Age, which had opened just three years earlier.
I am not ashamed of what some may
consider my naïve optimism: surely it is preferable to the all-too-common
alternative, naïve pessimism.
Five centuries ago, European
civilisation started expanding into the unknown, in a slow but irresistible
explosion fuelled by the energies of the Renaissance. After a thousand years of
huddling round the Mediterranean, Western man had discovered a new frontier
beyond the sea. We know the very day when he found it – and the day when he
lost it. The American frontier opened on October 12, 1492; it closed on May 10,
1869, when the last spike was driven in the intercontinental railway.
In all the long history of mankind,
ours is the first age with no new frontiers on land or sea, and many of our
troubles stem from this fact. It is true that, even now, there are vast areas
of the Earth still unexploited and even unexplored, but dealing with them will
only be a mopping-up operation. Though the oceans will keep us busy for centuries
to come, the countdown started even for them, when the bathyscaphe Trieste descended into the ultimate deep
of the Marianas [sic] Trench.
There are no more undiscovered
continents; set out toward any horizon, and on its other side you will find
someone already waiting to check your visa and your vaccination certificate.
[...]
The road to the stars has been
discovered none too soon. Civilisation cannot exist without new frontiers; it
needs them both physically and spiritually. The physical need is obvious – new
lands, new resources, new materials. The spiritual need is less apparent, but
in the long run it is more important. We do not live by bread alone; we need
adventure, variety, novelty, romance. As the psychologists have shown by
sensory deprivation experiments, a man goes swiftly mad if he is isolated in a
silent, darkened room, cut off completely from the external world. What is true
of individuals is also true of societies; they too can become insane without
sufficient stimulus.
It may seem overoptimistic to claim
that our escape from Earth, and the crossing of interplanetary Space, will
trigger a new Renaissance and break the patterns into which our society, and
our arts, must otherwise freeze. Yet this is exactly what I propose to do;
first, however, it is necessary to demolish some common misconceptions.
[...]
Whatever the eventual outcome of our
exploration of Space, we can be reasonably certain of some immediate benefits –
and I am deliberately ignoring such ‘practical’ returns as the multibillion
dollar improvements in weather forecasting and communications, which may in
themselves put space travel on a paying basis. The creation of wealth is
certainly not to be despised, but in the long run the only human activities
really worthwhile are the search for knowledge and the creation of beauty. This
is beyond argument; the only point of debate is which comes first.
Only a small part of mankind will ever
be thrilled to learn the composition of the Jovian atmosphere, the strength of
Mercury’s magnetic field or the exact length of the Venusian day. Though the
time may come when the existence of whole nations may be determined by such
facts, and others still more esoteric, these are matters which concern the
mind, and not the heart. Civilizations are respected for their intellectual
achievements; they are loved – or despised – for their works of art. Can we
even guess, today, what art will come from Space?
Let us first consider literature, for
the trajectory of any civilisation is most accurately traced by its writers. To
quote again from Professor Webb’s The
Great Frontier: ‘We find that in general each nation’s Golden Age coincides
more or less with that nation’s supremacy in frontier activity... It seems that
as the frontier boom got under way in any country, the literary genius of that
nation was liberated.’
Writers cannot escape from his
environment, however hard they try. When the frontier is open we have Homer and
Shakespeare – or, to choose less Olympian examples nearer to our own age, Melville,
Conrad, and Kipling. When it is closed, the time has come for – well, quite a
few contemporaries come to mind, but perhaps the best example is Proust, whose
last horizon was a cork-lined room.[14]
It is too naïve to imagine that
astronautics will restore the epic and the saga in anything like their original
forms; space flight will be too well documented, and Homer started off with the
great advantage of being untrammelled by too many facts. But surely the discoveries
and adventures, the triumphs and inevitable tragedies that must accompany our
drive towards the stars will one day inspire a new heroic literature, and bring
forth latter-day equivalents of The
Golden Fleece, Gulliver’s Travels, Robinson Crusoe, The Lusiads
and Moby Dick.[15]
[...]
It is perhaps too early to speculate
about the impact of space-flight on music and the visual arts. Here again one
can only hope – and hope is certainly needed, when one looks at the canvases
upon which some contemporary painters all too accurately express their psyches.
The prospect for modern music is a little more favourable; now that electronic
computers have been taught to compose it, we may confidently expect that before
long some of them will learn to enjoy it, thus saving us the trouble.
Maybe these ancient art forms have
come to an end of the line, and the still unimaginable experiences that await
us beyond the atmosphere will inspire new forms of expression. The low or
nonexistent gravity, for example, will certainly give rise to a strange,
other-worldly architecture, fragile and delicate as a dream. And what, I
wonder, will Swan Lake be like on
Mars, when the dancers have only a third of their terrestrial weight – or on
the Moon, where they will have merely a sixth?
[...]
Contact with a contemporary, nonhuman
civilisation will be the most exciting thing that has ever happened to our
race; the possibilities for good and evil are endless. In the Twenty-First
Century, some of the classic themes of science fiction may enter the realm of
practical politics. It is much more likely, however, that if our Solar System[16]
ever produced intelligent life, we have missed it by geological ages. Since all
the planets have been in existence for at least five billion years, the probability of cultures flourishing on two of
them at the same time must be extremely small.
Yet the impact of even an extinct
civilisation could be overwhelming; the European Renaissance, remember, was
triggered by the rediscovery of advanced societies that flourished more than a
thousand years earlier. When our archaeologists reach Mars, they may find
waiting for us a heritage as great as that which we owe to Greece and Rome. The
Chinese scholar Hu Shih has remarked: ‘Contact with strange civilisations
brings new standards of value, with which the native culture is re-examined and
re-evaluated, and conscious reformation and regeneration are the natural
outcome.’[17]
[...]
Until a few years ago, even the most
optimistic scientists though it impossible that we could ever span this
frightful abyss, which light itself takes years to cross at a tireless
670,000,000 miles an hour. Yet now, by one of the most extraordinary and
unexpected breakthroughs in the history of technology, there is a good chance
that we may make contact with intelligence outside
the Solar System before we discover the humblest mosses or lichens inside it.
This breakthrough has occurred in
electronics. It now appears that by far the greater part of our exploration of
space will be by radio, which can put us in touch with worlds that we can never
visit – even with worlds that have long ceased to exist. The radio telescope,
and not the rocket, may be the instrument that first discovers intelligence beyond
the Earth.
Even a few decades ago, this idea
would have seemed absurd. But now we have receivers of such sensitivity and
antennae of such enormous size, that we can hope to pick up radio signals from
the nearest stars – if there is anyone out there to send them. The search for
such signals began early in 1960 at the National Radio Astronomy Observatory,
Greenbank, West Virginia, and many other observatories have now followed suit.
This is perhaps the most momentous quest upon which men have ever embarked,
sooner or later, it will surely[18]
be successful.
From the background of cosmic noise,
the hiss and crackle of exploding stars and colliding galaxies, we will some
day filter out the faint, rhythmic pulses which are the voice of intelligence.
At first we will know only (only!) that there are other minds than ours in the
universe; later we will learn to interpret these signals. Some of them, it is
fair to assume, will carry images – the equivalent of picture telegraphy, or
even television. It will be fairly easy to deduce the coding and reconstruct
these images. One day, perhaps not far in the future, some cathode-ray screen
will show pictures from another world.
Let me repeat that this is no fantasy.
At this very moment millions of dollars’ worth of electronic equipment are
engaged upon the search. It may not be successful until the radio astronomers
can get into orbit, where they can build antennae miles across and can screen
them from the incessant din of the Earth: the Far Side of the Moon would be an excellent
location. We may have to wait ten – or a hundred – years for the first results;
no matter. The point I wish to make is that even if we can never leave the Solar
System in a physical sense, we may yet learn something about the civilisations
circling other stars – and they may learn about us. For as soon as we detect
messages from Space, we will attempt to answer them.
[...]
Radio prehistory – electronic
archaeology – may have consequences at least as great as the classical studies
of the past. The races whose messages we interpret and whose images we
reconstruct will obviously be of a very high order, and the impact of their art
and technology upon our own culture will be enormous. The rediscovery of Greek
and Latin literature in the fifteenth century, the avalanche of knowledge when
the Manhattan Atomic Bomb Project was revealed, the glories uncovered at the
opening of Tutankhamen’s tomb, the excavation of Troy, the publication of the Principia and The Origin of Species – these widely dissimilar examples may hint
at the stimulus and excitement that may come when we have learnt to interpret
the messages which for ages have fallen upon the heedless Earth.
Not all of these messages – not many,
perhaps – will bring us comfort. The proof, which is now only a matter of time,
that this young species of ours is low in the scale of cosmic intelligence will
be a shattering blow to our pride. Few of our current religions can be expected
to survive it, contrary to the optimistic forecasts from certain quarters. The
assertion that ‘God created man in his own image’ is ticking like a time bomb
in the foundations of Christianity. As the hierarchy of the Universe is slowly
disclosed to us, we will have to face this chilling fact: If there are any gods
whose chief concern is man, they cannot be very important gods.
The examples I have given, and the
possibilities I have outlined, should be enough to prove that there is rather
more to Space exploration than walking on the Moon, or even landing on Mars.
These are merely the preliminaries to the age of discovery that is now about to
dawn. Though that age will provide the necessary ingredients for a Renaissance,
we cannot be sure than one will follow. The present situation has no exact
parallel in the history of mankind; the past can provide hints, but no firm
guidance. The find anything comparable with our forthcoming ventures into
space, we must go back far beyond Columbus, far beyond Odysseus – far, indeed,
beyond the first ape-man. We must contemplate the moment, now irrevocably lost
in the mists of time, when the ancestors of all of us came crawling out of the
sea.
For this is where life began, and
where most of this planet’s life remains to this day, trapped in a meaningless
cycle of birth and death. Only the creatures who dared the hostile, alien land
were able to develop intelligence; now that intelligence is about to face a
still greater challenge. It may even be that this beautiful planet Earth of
ours is no more than a brief resting place between the sea of salt where we
were born, and the sea of stars on which we must now venture forth.
There are, of course, many who would
deny this, with varying degrees of indignation or even fear. Consider the
following extract from Lewis Mumford’s The
Condition of Man (1944):
Post-historic man’s
starvation of life would reach its culminating point in interplanetary
travel... Under such conditions, life would again narrow down to the
physiological functions of breathing, eating and excretion... By comparison,
the Egyptian cult of the dead was overflowing with vitality; from a mummy in
his tomb one can still gather more of the attributes of a full human being than
from a spaceman.
I sincerely hope that Dr Mumford (who
died in 1990 at the ripe age of 95) listened to some of the ecstatic broadcasts
of the Gemini, Apollo and Skylab astronauts as they described the wonders of
Space and weightlessness. But when he wrote: ‘No one can pretend... that
existence on a space satellite or on the barren face of the Moon would bear any
resemblance to human life’, he may well be expressing a truth he had not
intended. ‘Existence on dry land’, the more conservative fish may have said to
their amphibious relatives, a billion years ago, ‘will bear no resemblance to
piscatorial life. We will stay where we are.’
They did. They are still fish.[19]
9. You Can’t
Get There From Here
There is a striking though clumsy phrase
from the autobiography of the Nineteenth Century writer Richard Jefferies that
has stuck in my mind for many years: ‘The unattainable blue of the flower of
the sky.’ Unattainable: that is a
word we seldom use these days, now that we have reached the greatest heights
and depths on Earth and have even set foot upon the Moon. Yet only a century
ago the Poles were utterly unknown, much of Africa was still as mysterious as
in the time of King Solomon, and no human being had descended a hundred feet
into the sea or risen more than a mile in the air. We have gone so far in so
short a time, and will obviously go so much further if our species survives its
adolescence, that I would like to pose a question: Is there any place which will always remain
inaccessible to us, whatever scientific advances the future may bring?
[...]
There is one useful trick we may
employ to get quite close to the Sun in (almost) perfect safety. This is to use
a convenient asteroid or comet as a sunshade; a good choice is the little
flying mountain appropriately named Icarus.
This minor planet travels on an orbit
that every thirteen months brings it within a mere 17 million miles of the Sun.
Occasionally, it also passes quite close to Earth; it was within 4 million
miles of us in 1968: now we know that other asteroids NEOs (or Near Earth
Objects) come much closer.
Icarus is an irregular chunk of rock
one or two miles in diameter, and at perihelion, beneath a sun that appears
thirty times as big in the sky as it does from Earth, the surface of this
little world may reach temperatures not far short of 1,000°F. But it casts a
cone of shadow into space; and in the cold shelter of that shadow, a ship could
ride safely around the Sun.
In a short story called ‘Summertime on
Icarus’,* I described how scientists might embark on such a somewhat
hair-raising sleigh ride to get themselves and their instruments close to the
Sun, which would be unable to touch them as long as they remained on the night
side of their mile-thick shield of rock. Though it would be possible to
construct artificial heat shields, like today’s re-entry nose cones, it will be
a long time before we can give ourselves the protection that Icarus would
provide for nothing. Small though it is, this minor planet must weigh about 10
billion tons.
There may be other asteroids that go
even closer to the Sun; if there are not, we may one day make them do so by a
nudge at the right point of the orbit. And then, dug well in below the surface,
scientists would be able to skim the atmosphere of the Sun, whipping across it
and out again into Space on a tight hairpin bend.
It is interesting to work out how long
the ride would take. Being a rather small star, the Sun is ‘only’ three million
miles in circumference. A satellite just outside its atmosphere would move at
about a million miles an hour, so would circle it every three hours.
A comet or asteroid falling toward the
Sun from the distance of Earth would be moving somewhat faster than this at its
point of closest approach. It would flash across the surface of the Sun at a
million and a quarter miles an hour, before heading off into space again. Even
if a few megatons of rock boiled away in the process, the instruments and
observers deep inside the asteroid would be safe – unless, of course, there was
a navigational error and they plunged too deeply into the solar atmosphere, to
burn up through friction as so many artificial satellites on Earth already
done.
What a ride that would be! Imagine
flashing high above the centre of a giant sunspot, a gaping crater a hundred
thousand miles across, spanned by bridges of fire over which our planet Earth
could roll like a child’s hoop along a pavement. The explosion of the most
powerful hydrogen bomb would pass unnoticed in that inferno, where whole
continents of incandescent gas leap skyward at hundreds of miles a second,
sometimes escaping completely into space.
[...]
I have already mentioned dwarf stars,
which are tiny suns in the last stages of stellar evolution. Some of them are smaller
than Earth, yet they contain, packed within their few thousand miles of radius,
as much matter as goes to make up a normal star. The very atoms of which they
are composed are crushed beneath the enormous pressures in their interiors, to
densities which may rise to many millions of times that of water. A cubic inch
of matter from such a star may weigh more than a hundred tons.
Though most dwarfs are red or
white-hot, cool ‘black dwarfs’ are a theoretical possibility. They would be the
very end of the evolutionary line, and would be extremely difficult to detect
because, like planets, they would radiate no light of their own, but could be
observed only by reflection, or when they eclipsed some other body. Since our
Galaxy is still quite young – not much more than 15 billion years old! – it is
probable that none of its stars has yet reached the final black dwarf stage;
but their time will come.
These stellar corpses will be among
the most fascinating (and sinister) objects in the universe. Their combination
of great mass and tiny size would give them enormous gravitational fields – up
to a million times as powerful as Earth’s. A world with such a gravity would
have to be perfectly spherical; no hills or mountains could rear themselves
more than a fraction of an inch above its surface, and its atmosphere would be
only a few feet in depth.
At million gravities, all objects –
even if made of the strongest metal – would flow under their own weight until
they had flattened themselves into a thin film. A man could weigh as much as
the Queen Elizabeth and would
collapse so quickly that his disintegration could not be followed by the naked
eye, for it would take less than a thousandth of a second. A fall through a
distance of a third of an inch would be equivalent to falling, on Earth, from
the top of Mount Everest to sea level.
Yet despite the enormous gravitational
field, it would be possible to approach within a few miles of such a body. A
spaceship or a space-probe aimed into a sufficiently precise orbit could, in
theory at least, swing past it like a comet whipping round the Sun. If you were
in such a ship you would feel nothing, even at the moment of closest approach.
At an acceleration of a million gravities, you would still be completely
weightless, for you would be in free fall. The ship would reach a maximum speed
of some 25 million miles an hour as it raced low over the surface of the dying
star; then it would recede into space once more, escaping beyond its reach.
In 1967, just five years after the
first edition of this book was published, the next – though probably not final
– stage in stellar evolution was discovered, to the delighted amazement of
astronomers: I refer, of course, to the now famous ‘pulsars’. And far from
being ‘difficult to detect’, they announced their existence so loudly that any
well-equipped radio amateur can listen to their exquisitely precise time
signals.
Pulsars were quickly identified (by
the ubiquitous Dr Gold) as ‘neutron stars’ whose existence had been predicted
decades earlier on theoretical grounds by the brilliant Swiss astrophysicist
Fritz Zwicky. Little more than ten miles in diameter, yet containing the mass
of a whole sun, their average density is some 100,000,000,000,000 times that of
water, so a thimble-full would have a mass of – fasten your seat-belt – about a hundred thousand super-tankers! Their
surface temperature is around a million degrees, and the idea that any
organisms could exist under such conditions is so absurd as to be unworthy of
serious consideration.
[...]
As in the case of a white dwarf
already discussed, it would be safe (ignoring its lethal outpouring of
radiation!) to approach a neutron star by going into free fall around it. At
distances of a few thousand miles you would still feel weightless, but if you
were foolish enough to get closer, conditions would change rapidly. The
intensity of the gravitational field might be so different between your head
and your feet that you would be swiftly pulled apart by the same kind of tidal
force that rules the oceans of Earth. Even the strongest metals would flow like
liquid, a hundred miles above a neutron star.
This fact prompted me to make an entry
into the fierce-fought contest for the worst pun in science fiction. My
deplorable squib ‘Neutron Tide’** describes the tragic fate of the United
States Space Fleet’s supercruiser Flatbush,
which was unlucky enough to approach a neutron star too closely. The only recognisable
piece of the resultant debris was ‘one star-mangled spanner’.
Sorry about that...
But what of an actual landing on a white dwarf – or even a
neutron star? Such a feat is conceivable if we make two assumptions, neither of
which violates any known physical laws. We would need propulsion systems
billions of times more powerful than any known today, and we would require an
absolutely complete and reliable means of neutralising gravity, so that the
crushing external field could be cancelled a dozen to a dozen decimal places. If
even a microscopic – no, nanoscopic – fraction of that appalling gravity
‘leaked’ into the ship, its occupants would be pulped. They would never feel
anything, of course, if the compensating field failed; it would all be over so
quickly that nerve fibres would have no time to react.
In our own time, men have peered
through the portholes of a bathyscaphe into a region, only inches away, where
they would be crushed in a fraction of a second by a pressure of a thousand
tons on every square foot of their bodies. That was a wonderful achievement – a
triumph of courage and engineering skill. Centuries in the future, and
light-years from Earth, there may be men peering out of portholes into the
still more ferocious environment of a dwarf star.
How strange it will be, to look down
upon the smooth, geometrically perfect surface on the other side of the ship’s
compensating field – and to realise that, measured in terms of Earth’s feeble
gravity, your head is the equivalent of thousands – even millions – of miles
above your feet.
_________________________________________
*In the collection Tales
of Ten Worlds.
**In the collection The
Wind From the Sun.
10. Space,
the Unconquerable
Man will never conquer Space. After
all that has been said in the last two chapters, this statement sounds ludicrous.
Yet it expresses a truth which our forefathers knew, which we have forgotten –
and which our descendants must learn again, in heartbreak and loneliness.
Our age is in many ways unique, full
of events and phenomena which never occurred before and can never happen again.
They distort our thinking, making us believe that what is true now will be true
for ever, though perhaps on a larger scale. Because we have annihilated
distance on this planet, we imagine that we can do it once again. The truth is far
otherwise, and we will see it more clearly if we forget the present and turn
our minds towards the past.
To our ancestors, the vastness of the
Earth was a dominant fact controlling their thoughts and lives. In all earlier
ages than ours, the world was wide indeed and no man could ever see more than a
tiny fraction of its immensity. A few hundred miles – a thousand, at the most –
was infinity. Great empires and cultures could flourish on the same continent,
knowing nothing of each other’s existence save fables and rumours as faint as though
from a distant planet. When the pioneers and adventurers of the past left their
homes in search of new lands, they said goodbye for ever to the places of their
birth and the companions of their youth. Only a lifetime ago, parents waved
farewell to their emigrating children in the virtual certainty that they would
never meet again. Those they loved would be almost as good as dead.
And now, within little more than one
generation, all this has changed. Over the seas where Odysseus wandered for a
decade, the jumbo jets hurtle within the hour. And far higher, orbiting
astronauts span the distance between Troy and Ithaca in less than a minute.
Psychologically as well as physically,
there are no longer any remote places on Earth. When a friend leaves for what
was once a far country, even with no intention of returning, we cannot feel
that same sense of irrevocable separation that saddened our forefathers. We
know that we are only hours apart by jet, and that we have merely to touch a
keyboard to hear a familiar voice – or, better still, to see a beloved face.
The world can shrink no more: it has become a dimensionless point.
But the new stage that is opening up
for the human drama will never shrink as the old one has done. We have
abolished space here on this little Earth; we can never abolish the Space that
yawns between the stars. Once again, as in the days when Homer sang, we are
face to face with immensity and must accept its grandeur and terror, its
inspiring possibilities and its dreadful restraints. From a world that has
become too small, we are moving out into one that that will be for ever too
large, whose frontiers will recede from us as always more swiftly than we can
reach out towards them.
Consider first the fairly modest Solar
System distances which we are now challenging. Though the Moon is only a few
days away, our space probes take months to reach Mars and Venus – years to
reach the outer planets. However, when we have harnessed nuclear – or
alternative – energy for space flight, the empire of the Sun will contract
until it will seem little larger than the Earth today. The remotest of the
planets will be no more than a week away – Mars and Venus, only a few hours.
This achievement, which will be
witnessed within a century, might appear to make even the Solar System a
comfortable, homely place, with such giant planets as Saturn and Jupiter
playing much the same role in our thoughts as do Africa or Asia today. (Their
qualitative differences of climate, atmosphere, and gravity, fundamental though
they are, do not concern us at the moment.) To some extent this may be true,
yet as soon as we pass beyond the orbit of the Moon, a mere quarter-million
miles away, we will meet the first of the barriers that will sunder Earth from
her scattered children.
The marvellous telephone and
television networks that now enmesh our planet, making all men and women
neighbours, cannot be extended into space. It
will never be possible to converse with anyone on another world.
Please do not misunderstand this
statement! Even with amateur radio equipment, the problem of sending speech to
the outer planets is almost trivial. But the message will take minutes –
sometimes hours – on their journey, because radio and light waves travel at the
same limited speed of 186,000 miles a second. Twenty years from now you will be
able to listen to a friend on Mars, but the words you hear will have been
spoken at least three minutes earlier, and your reply will take a corresponding
time to return. In such circumstances, an exchange of verbal messages is
possible – but not a conversation. Even
in the case of the nearby Moon, the two-and-a-half second time lag is slightly
annoying. At distances of more than a million miles, it will be intolerable.
To a culture which has come to take
instantaneous communication for granted, as part of the very structure of
civilised life, this ‘time barrier’ may have a profound psychological impact. It
will be a perpetual reminder of universal laws and limitations against which
not all our technology can ever prevail. For it seems as certain as anything
can be that no signal – still less any material object – can ever travel faster
than light.
The velocity of light is the ultimate
speed limit, being part of the very structure of space and time. Within the
narrow confines of the Solar System, it will not handicap us too severely, once
we have accepted the delays in communication which it involves. At the worst,
these will amount to eleven hours – the time it takes a radio signal to span
the orbit of Pluto, the outermost planet. Between the three inner worlds Earth,
Mars, and Venus, it will never be more than twenty minutes – not enough to
interfere seriously with commerce or administration, but more than sufficient
to shatter those personal links of sound and vision that can give us a sense of
direct contact with friends on Earth, wherever they may be.
It is when we move out beyond the
confines of the Solar System that we come face to face with an altogether new
order of cosmic reality. Even today, many otherwise educated men – like those
savages who can count up to three but lump together all numbers beyond four – cannot
grasp the profound distinction between solar
and stellar space. The first is the
space enclosing our neighbouring worlds, the planets; the second is that which
embraces those distant suns, the stars. And
it is literally millions of times greater.
There is no such abrupt change of scale
in terrestrial affairs. To obtain a mental picture of the distance to the
nearest star, as compared with the distance to the nearest planet, you must
imagine a world in which the closest object to you is only five feet away – and
then there is nothing else to see until you have travelled a thousand miles.
Many conservative scientists, appalled
by these cosmic gulfs, have denied that they can ever be crossed. Some people
never learn; those who a century ago scoffed at the possibility of flight, and
– halfway between today and the Wright brothers! – pooh-poohed the idea of
travel to the planets, are quite sure that the stars will always be beyond our
reach. And again they will be wrong, for they have failed to grasp the great
lesson of our age – that if something is possible in theory, and no fundamental
scientific laws oppose its realisation, then sooner or later it will be
achieved.
One day – it may be within the next
few decades, or it may be a thousand years from now – we shall discover a
really efficient means of propelling our space vehicles. Every technical device
is always developed until its limits (unless it is superseded by something
better) and the ultimate speed for spaceships is the velocity of light. They
will never reach that goal, but they will get very close to it. And then the
nearest star will be less than five years’ voyaging from Earth.
Our exploring ships will spread
outwards from their home over an ever-expanding sphere of space. It is a sphere
which will grow at almost – but never quite – the speed of light. Five years to
the triple system Alpha Centauri, ten to that strangely matched double Sirius A
and B, eleven to 61 Cygni, the first star suspected of possessing a planet.
(Today, we are certain of many more.) These journeys are long, but they are not
impossible. Our species has always accepted whatever price was necessary for
its explorations and discoveries, and the price of Space is Time.
Even voyages which may last for
centuries or millenniums will one day be attempted. Suspended animation, an
undoubted possibility, may be the key to interstellar travel. Self-contained
cosmic arks which will be tiny travelling worlds in their own right may be
another solution, for they would make possible journeys of unlimited extent,
lasting generation after generation. The famous time-dilation effect predicted
by the Theory of Relativity, whereby time appears to pass more slowly for a
traveller moving at almost the speed of light, may be yet a third. And there
are others.
With so many theoretical possibilities
for interstellar flight, we can be sure that at least one will be realised in
practice.
[...]
I will not argue the point, or give
the reasons scientists believe that light can never be outraced by any form of
radiation or any material object. Instead, let us assume the contrary and see
just where it gets us. We will even take the most optimistic possible case, and
imagine that the speed of transportation may eventually become infinite.
Picture a time when, by the
development of techniques as far beyond our present engineering as the
microchip is beyond a stone axe, we can reach anywhere we please instantaneously, with no more effort
than by dialling a number. This would indeed cut the Universe down to size, and
reduce its physical immensity to nothingness. What would be left?
Everything that really matters. For
the Universe has two aspects – its scale, and its overwhelming, mind-numbing
complexity. Having abolished the first, we must now confront the second. We
must try to visualise not size, but quantity.
[...]
The number of other suns in our own
Galaxy (that is, the whirlpool of stars and cosmic dust of which our Sun is an
out-of-town member, lying in one of the remoter spiral arms) is estimated at
about 1011 or, written in full, 100,000,000,000. Our present
telescopes can observe something like 109 other galaxies, and they
show no sign of thinning out even at the extreme limit of vision. There are
probably at least as many galaxies in the whole of creation as there are stars
in our own Galaxy, but let us confine ourselves to those we can see. They must
contain a total of about 1011 times 109 stars, or 1020
stars altogether.
One followed by twenty other digits
is, of course, a number beyond all understanding. There is no hope of ever
coming to grips with it, but there are ways of hinting at its implications.
Just now we assumed that the time
might come when we could dial ourselves, by some miracle of matter
transmission, effortlessly and instantly round the Cosmos, as today we call a
number in our local exchange. What would the Cosmic Telephone Directory look
like, if its contents were restricted only to suns and it made no effort to
list individual planets, still less the millions of places and entities on each
planet?
The directories of such cities as
London and New York are already getting somewhat out of hand, but they list
only about a million – 106 – or so numbers. The cosmic directory would be 1014
times bigger, to hold its 1020 numbers. It would contain more pages
than all the books that have ever been
produced since the invention of the printing press.
[...]
Before such numbers, even spirits
brave enough to face challenge of the light-years must quail. The detailed
examination of all the grains of sand on all the beaches of the world is a far
smaller task than the exploration of the Universe.
And so return to our opening
statement. Space can be mapped and crossed and occupied without definable
limit; but it can never be conquered. When our race has reached its ultimate
achievements, scattered far and wide across the stars, we will still be like
ants crawling on the face of the Earth. The ants have covered the world, but
have they conquered it – for what do their countless colonies know of it, or of
each other?
So it will be with us as we spread
outwards from Mother Earth, loosening the bonds of kinship and understanding,
hearing faint and belated rumours at second – of third – of thousandth-hand of
an ever-dwindling fraction of the entire human race. Though Earth will try to
keep in touch with her children, in the end all the efforts of her archivists
and historians will be defeated by time and distance, and the sheer bulk of
material. For the number of distinct societies or nations, where our race is
twice its present age, may be far greater than the total number of all men who
have ever lived up to the present time.
[...]
11. About
Time
Man is the only animal to be troubled
by time, and from that concern comes much of his finest art, a great deal of his
religion, and almost all his science. For it was the temporal regularity of
Nature – the rising of sun and stars, the slower rhythm of the seasons – which
led to the concept of law and order and in turn to astronomy, the first of all
sciences. Changeless environments like the deep ocean or the cloud-wrapped
surface of Venus provide little stimulus to intelligence, and in such places it
may never be able to arise.
It is not surprising, therefore, that
cultures which existed in regions of negligible climatic variation, like
Polynesia and tropical Africa, often had little conception of time. Other
societies, forced by their surroundings to be aware of it, have become obsessed
by time. Perhaps the classic example is that of ancient Egypt, where life was
regulated by the annual flooding of the Nile. No other civilisation, before or
since, has made such determined efforts to challenge eternity, and even to deny
the existence of death.
Time has been a basic element in all
religions, where it has been combined with such ideas as reincarnation,
foretelling the future, resurrection, and the worshipping of the heavenly
bodies – as shown by the monolithic calendar of Stonehenge, the zodiac from the
Dendera Temple, and the ecclesiastical architecture of the Mayas. Some faiths
(Christianity, for instance) have placed Creation and the Beginning of Time at
very recent dates in the past, and have anticipated the end of the Universe in
the near future. Other religions, such as Hinduism, have looked back through
enormous vistas of time and forward to even greater ones. It was with
reluctance that Western astronomers realised that the East was right, and that
the age of the universe is to be measured in billions rather than thousands of
years – if it can be measured at all.
And it was only in the Twentieth
Century that we learned something about the true nature of Time, and were even
able to influence its progress – though, so far, merely by nanoseconds. Now we
know that Time is neither absolute nor inexorable, and that tyranny of the
clock may not last forever.
It is hard not to think of Time as an
adversary, and in a sense, all the achievements of human civilisation are small
victories in the war against Time. Whatever their motives may have been, the
cave artists of Lascaux were the first to win any gains for mankind. About a
thousand generations ago, when the mammoth and saber-toothed tiger still walked
the Earth, they discovered a way of sending not merely their bones but some at
least of their thoughts and feelings into the future. We can look through their
eyes, across the gulfs of time, and see the animals that shared their world.
But we can see little more than that.
The invention of poetry, perhaps as
part of religious rituals, was the next advance. Ordinary words and phrases are
fleeting, forgotten as soon as uttered. However, once they are arranged in a
pattern, something magical happens. Shakespeare (most time-obsessed of writers)
truly remarked:
Not marble, nor the gilded
monuments
Of princes, shall outlive
this powerful rhyme.
Bards and minstrels like Homer carried
in their heads the only record of prehistory we possess, though until the
invention of writing it was always liable to distortion or total loss. Writing
– perhaps the most important single invention of mankind – changed all that.
Plato and Caesar speak to us across the ages more clearly than most of our
fellow men. And with the invention of the printing press, the written word
became virtually immortal. Manuscripts and scrolls and papyri are vulnerable
and easily destroyed, but since the time of Gutenberg, very few works of
permanent value can have vanished into oblivion.
[...]
The most convincing argument against
time travel is the remarkable scarcity of time travellers. However unpleasant
our age may appear to the future, surely one would expect scholars and students
to visit us, if such a thing was possible at all. Though they might try to
disguise themselves, accidents would be bound to happen – just as they would if
we went back to imperial Rome with cameras and tape recorders concealed under
our nylon togas. Time travelling could never be kept secret for very long; over
and over again down the ages, chronic argonauts (to use the original and
singularly uninspiring title of Wells’ The
Time Machine) would get into trouble and inadvertently disclose themselves.
As it is, the chief evidence of a security leak from the future appears to be
the notebooks of Leonardo da Vinci. Their parade of inventions from the
succeeding centuries is astonishing, but hardly conclusive proof that Fifteenth
Century Italy had visitors from Elsewhen.
[...]
Yet we know so little about Time, and
have made such scanty progress in understanding and controlling it, that we
cannot rule out even such outrageous possibilities as limited access to the
future. Professor J. B. S. Haldane once shrewdly remarked: ‘The Universe is not
only queerer than we imagine – it is queerer than we can imagine.’ Even the Theory of Relativity may only hint at the
ultimate queerness of Time.
In his poem The Future, Matthew Arnold described man as a wanderer ‘born in a
ship, On the breast of the river of Time’. Through all history, that ship has
been drifting, rudderless and uncontrolled; now, perhaps, we are learning how
to start the engines. They will never be powerful enough to overcome the
current; at the best, we may delay our departure, and get a better view of the
lands around us, and the ports we have left for ever. Or we may speed up our
progress, and dart downstream more swiftly than the current would otherwise
bear us. What we can never do is to turn back and revisit the upper reaches of
the river.
And in the end, for all our efforts, it
will sweep us with our hopes and dreams out into the unknown ocean:
As the pale waste widens
around him –
As the banks fade dimmer
away –
As the stars come out, and
the night-wind
Brings up the
stream
Murmurs and scents of the
infinite Sea.
12. Ages of
Plenty
[...]
Whatever new reserves may be
discovered, ‘fossil fuels’ such as coal and oil can last for only a few more
centuries; then they will be gone forever. They will have served to launch our
technological culture into its trajectory, by providing easily available sources
of energy, but they cannot sustain civilisation over thousands of years. For
this, we need something more permanent.
Until recently, there seemed little
doubt that the long-term (and perhaps the short-term) answer to the fuel
problem would be nuclear energy. The weapons now stockpiled by the major powers
could run all the machines on Earth for several years, if their energies could
be used constructively. The warheads in the American arsenals alone are
equivalent to thousands of millions of tons oil or coal.
It is not likely that fission
reactions (those involving such heavy elements as thorium, uranium and
plutonium) will play more than a temporary role in terrestrial affairs. One
hopes they will not, for fission is the dirtiest and most unpleasant method of
releasing energy that man has ever discovered. Some of the radioisotopes from
today’s reactors will still be causing trouble, and perhaps injuring unwary
archaeologists, a thousand years from now.
But beyond fission lies fusion – the
welding together of light atoms such as hydrogen and lithium. This is the
reaction that drives the stars themselves; we have reproduced it on Earth, but
have not yet tamed it. When we have done so, our power problems will have been
solved for ever – and there will no poisonous by-products but only the clean
ash of helium.
Controlled fusion is the supreme
challenge of applied nuclear physics; some scientists believe it will be
achieved in ten years, some in fifty. But almost all of them are sure that we
will have fusion power long before our oil and coal run out, and will be able
to draw fuel from the sea in virtually unlimited amounts.
[...]
The Earth’s magnetic field is so
extremely feeble (a toy magnet is a thousand times stronger) that it is not
even worth considering. From time to time one hears optimistic talk of
‘magnetic propulsion’ for space vehicles, but this is a project somewhat
comparable to escaping from Earth via
a ladder made of cobwebs. Terrestrial magnetic forces are just about as tough
as gossamer.
Yet so much of the universe is
indetectable to our senses, and so many of its energies have been discovered
only during the last few moments of historic time, that it would be rash to
discount the idea of still unknown cosmic forces. The concept of nuclear energy
seemed nonsense only a lifetime ago, and even when it was proved to exist, most
scientists denied that it could be tapped. There is considerable evidence that
a flood of energy is sweeping through all the stars and planets in the form
known as neutrino radiation (discussed in more detail in Chapter Nine) which
challenges our powers of observation. So might Isaac Newton, for all his
genius, have failed to detect anything emerging from a radio antenna.
For terrestrial projects, it does not
greatly matter whether or not the Universe contains unknown and untapped energy
sources. The heavy hydrogen in the seas can drive all our machines, heat all
our cities, for as far ahead as we can imagine. If, as is perfectly possible,
we are short of energy two generations from now, it will through our own
incompetence. We will be like Stone Age men freezing to death on top of a coal
bed.
For most of our raw materials, as for
our power sources, we have been living on capital. We have been exploiting the
easily available resources – the high-grade ores, the rich lodes where natural
forces have concentrated the metals and minerals we need. These processes took
a billion years or more; in mere centuries, we have looted treasures stored up
over aeons. When they are gone, our civilisation cannot mark time for a few
hundred million years until they are restored.
Once more, we will be forced to use
our brains instead of our muscles. When all the ores are exhausted we can turn
to ordinary rocks and clays: one hundred tons of average igneous rock such as
granite contains: 8 tons of aluminium, 5 tons of iron, 1,200 pounds of
titanium, 180 pounds of manganese, 70 pounds of chromium, 40 pounds of nickel,
30 pounds of vanadium, 20 pounds of copper, 10 pounds of tungsten and 4 pounds
of lead.
To extract these elements would
require not only advanced chemical techniques, but very considerable amounts of
energy. The rock would first have to be crushed, then treated by heat,
electrolysis and other means. However, a ton of granite contains enough uranium
and thorium to provide energy equivalent to fifty ton of coal. All the energy
we need for the processing is there in the rock itself.
Another almost limitless source of
basic raw materials is the sea. A single cubic mile of seawater contains,
suspended or dissolved, about 150 million tons of solid material. Most of this
(120 million tons) is common salt, but the remaining 30 million tons contains
almost all the elements in impressive quantities. The most abundant is
magnesium (about 18 million tons) and its large-scale extraction from the sea
during the Second World War was a great, and highly significant, triumph of chemical
engineering. It was not, however, the first element to be obtained from
seawater, for the extraction of bromine in commercial quantities started as
early as 1924.
The difficulty with ‘mining’ the sea
is that the materials we wish to win from it are present in very low
concentrations. The 18 million tons of magnesium per cubic mile sounds an
enormous figure, but it is dispersed in 4 billion
tons of water. Regarded as an ore, therefore, seawater contains only four parts
of magnesium per million; on land, it is seldom profitable to work rocks
containing less than one part in a hundred of the commoner metals. Many people
have been hypnotised by the fact that a cubic mile of seawater contains about
twenty tons of gold, but they would probably find richer pay dirt in their own
back gardens.
[...]
In view of the present astronomical
cost of space travel (several thousand dollars per pound of payload for even
the simplest orbital missions) it may seem fantastic to suggest that we will
ever be able to mine and ship megatons of raw materials across the Solar
System. Even gold could hardly pay its way, and only diamonds would show a
profit.
This view, however, is coloured by
today’s primitive state of the art, which depends upon hopelessly inefficient
techniques. It is something of a shock to realise that, if we could use the
energy really efficiently, it would require only about a dollar’s worth of
chemical fuel to lift a pound of payload completely clear of Earth – and a few
cents more to carry it to the Moon. For a number of reasons, these figures represent
unattainable ideals, but they do indicate how much room there is for
improvement. Some studies of nuclear propulsion systems suggest that, even with
technique we can imagine today, space flight need be no more expensive that jet
transportation; as far as inanimate cargoes are concerned, it may be very much
cheaper.
When those somewhat optimistic words
were written, I was unaware that an amazing idea had already surfaced, which
could turn them into reality sooner
than I dared to imagine. In the July 31, 1960 issues of Komsomlskaya [sic] Pravda[20],
Yuri Artsutanov, a Leningrad (now St Petersburg) engineer, published an article
describing a ‘heavenly funicular’, to use his engaging term, which could lift
12,000 tons of payload a day to synchronous orbit. The basic idea could hardly
be simpler: merely a system of cables linking a point on Earth’s equator to a
geostationary satellite poised 22,000 miles above it. Goods and passengers
could be carried up it purely by electrical energy; it would be the exact analogy
of the elevator familiar in every high-rise building – but a million times
taller.
The concept received little publicity
outside the USSR and quite independently discovered by Isaacs, Bradner and
Backus, of Scripps Institute of Oceanography, and Vine, of Wood’s Hole
Oceanographic Institute, who published a paper, ‘Satellite Elongation into a
True “Sky-Hook”’ in Science (February
11, 1966). When it was pointed out to them that Yuri had been there six years
earlier, they immediately acknowledged his priority.
The ‘space elevator’ was quite clearly
an idea whose time had come: as is demonstrated by the fact that within a
decade it was independently re-invented by several different groups. A very
detailed treatment, containing many new ideas, was published by Jerome Pearson
in Acta Astronautica for
September-October 1975 (‘The Orbital Tower: a spacecraft launcher using the
Earth’s rotational energy’). Dr Pearson was astonished to hear of the earlier
studies, which his computer survey had failed to locate; he discovered them
through reading my own testimony to the House of Representatives Space
Committee in July 1975! (See The
View From Serendip.[21])
Though the space elevator was a
delightful idea in theory, for the first few decades it seemed likely to remain
there, because the only material strong enough to build it was the crystalline
form of carbon – better known as diamond, and scarcely available in the megaton
qualities required. However, this did not stop me from assuming in The
Fountains of Paradise that this minor problem could be overcome when we had
zero-gee manufacturing facilities in orbit.
And now for a truly extraordinary
coincidence: I swear I’m not making this up...
In 1978, the year before Fountains was published, I had the great
pleasure of flying Buckminster Fuller over the places in Sri Lanka that I had
chosen as key locations for the story. The next years, when I recorded extracts
from the novel on a 12’’ LP (remember them, anyone? It was Caedmon TC 1606) Bucky very kindly wrote
the sleeve-notes, and drew a picture of the elevator reaching from Ceylon up to
orbit. He also made this astonishing comment:
‘In 1951, I designed a free-floating
tensegrity ring-bridge to be installed way out from and around the Earth’s
equator. Within this “halo” bridge, the Earth would continue its spinning while
the circular bridge would revolve at its own rate. I foresaw Earthian traffic vertically
ascending to the bridge, revolving and descending at preferred Earth loci.’
It appears, therefore, that Bucky
anticipated Artsutanov by almost a decade! But that’s the beginning of the
story.
In 1985, two years after Bucky’s death
at the age of 88, a new form of carbon was discovered, in which sixty atoms are
arranged in a structure exactly like the geodesic domes for which he is most
famous. It was, of course, instantly named Buckminsterfulleren, or Fullerene
for short, and the three co-discovers were awarded a Nobel Prize. Needless to
say, chemists all over the world quickly started to investigate the properties
of this remarkable substance.
Now for the eerie coincidence...
It was soon found that C60 could also
occur in the form of minute tubes –
Buckytubes, of course – which possess extraordinary strength. The
discoverers claimed that this is not only the strongest material known, but the strongest material that could ever
exist (I don’t know if they’ve given any thought to choice pieces of
neutron star). And they immediately added that it would make the space elevator
possible.
If Buckytubes
could be made in quantity, they would revolutionise almost every aspect of life
here on Earth as well as in Space. Just imagine what a material hundreds of
times stronger times stronger than steel, and far lighter, would do to all the
industries involved in building and transportation! The furniture of the
average house might weigh virtually nothing: chairs and tables would seem like
frozen soap-bubbles.
What a tragedy that Bucky missed, by
only two years, the amazing molecule that has now contributed greatly to his
posthumous fame – and has perhaps heralded the dawn of what future historians
may call the Carbon Age...
[...]
Having, in imagination, raided the
Solar System in the search for raw materials, let us come back to Earth and
explore a completely different line of thought. It may never be really
necessary to go beyond our own planet for anything we need – for the time will
come when we can create any element, in any quantity, by nuclear transmutation.
Until the discovery of uranium fission
in 1939, practical transmutation remained as much as a dream as it had been in
the days of the old alchemists. Since the first reactors started operating in
1942, substantial amounts (to be measured in hundreds of tons) of the synthetic
metal plutonium have been manufactured, and vast quantities of other elements have
been created as often unwanted and embarrassingly radioactive by-products.
But plutonium, with its overwhelmingly[22]
important military applications, is a very special case, and everyone is aware
of the cost and complexity of the plants needed to manufacture it. Gold is
cheap by comparison, and synthesising common metals like lead or copper or iron
seems about as probable as mining them from the Sun.
We must remember, however, that
nuclear engineering is in roughly the same position as chemical engineering at
the beginning of the Nineteenth Century, when the laws governing reactions
between compounds were just beginning to be understood. We now synthesise, on
the largest scale, drugs and plastics which yesterday’s chemists could not even
have produced in their laboratories. Within a few generations, we will surely
be able to do the same thing with the elements.
Starting with the simplest element
hydrogen (one electron revolting around one proton) or its isotope deuterium
(one electron revolving round a nucleus of a proton and a neutron) we can
‘fuse’ atoms together to make heavier and heavier elements. This is the process
operating in the Sun, as well as in the H-bomb; by various means, four atoms of
hydrogen are combined to make one of helium, and in the reaction enormous
quantities of energy are released. (In practice, the third element in the
periodic table, lithium, is also employed.) The process is extremely difficult
to start, and still harder to control – but it is only the very first step in
what might be christened ‘nuclear chemistry’.
At even higher pressures and
temperatures than those produced in today’s thermonuclear explosions or fusion
devices, the helium atoms will themselves combine to form heavier elements;
this is what happens in the cores of stars. At first, these reactions release
additional energy, but when we reach elements as heavy as iron or nickel the
balance shifts and extra energy has to be supplied to create them. This is the
consequence of the fact that the heaviest elements tend to be unstable and
break down more easily than they fuse together. Building up elements is rather
like piling up a column of bricks; the structure is stable at first, but after
a while it is liable to spontaneous collapse.
Inside the stars, nuclear synthesis is
produced by temperatures of between 1,000 and 5,000 millions degrees, and the
pressures millions of billions of
atmospheres. But there are other ways of starting reactions, besides heat and
pressure. The chemists have known this for many years; they employ catalysts
which speed up reactions or make them take place at far lower temperatures than
they would otherwise do. Much of modern industrial chemistry is founded on
catalysts (vide the ‘cat crackers’ of the oil refineries)
and the actual composition of these is often a closely guarded trade secret.
Are there nuclear, as well as
chemical, catalysts? Yes: in the Sun, carbon and nitrogen play this role. There
may be many other nuclear catalysts, not necessarily elements. Among the
legions of misnamed fundamental particles which now perplex the physicist – the
mesons and positrons and neutrinos – there may be entities that can bring about
fusion at temperatures and pressures that we can handle.
Or there may be completely different
ways of achieving nuclear synthesis, as surprising today as was the uranium
reactor half a century ago. In 1958 Luis Alvarez and his colleagues discovered
a rare form of nuclear catalysis,
involving particles known as negative muons. As he remarked rather sadly in his
autobiography Alvarez: Adventures of a Physicist
(1987):
For a few exhilarating
hours we thought we had solved mankind’s energy problem for ever. Our first
hasty calculations indicated that in liquid hydrogen-deuterium a single
negative muon should catalyse enough fusion reactions before it decayed to
supply enough energy to operate the accelerator to make more muons, to extract
the necessary hydrogen and deuterium from the sea, and to feed the power grid.
While everyone else had been trying to control thermonuclear fusion by heating
hydrogen plasmas to million of degrees, we seemed to have stumbled upon a
better than break-even reaction that operated at minus 250 degrees Celsius.
More realistic calculations
showed us we were short of the mark by several orders of magnitude... In
physics that’s a near miss. In recent years there has been a great resurgence
of interest in fusion catalysed by muons...
In 1989, only two years after Louie
wrote those words, there was indeed a great resurgence in fusion, when Pons and
Fleischman reported the generation of energy apparently at room temperature
with very simple equipment. After the initial excitement, when several leading
laboratories failed to reproduce the so-called ‘Cold Fusion’ effect, their
results were almost universally dismissed as erroneous.
However, during the last decade scores
of independent groups, many led by competent and experienced scientists, have
also claimed to have detected anomalous sources of energy – some of which can
have nothing to do fusion, hot or cold. Despite announcements from numerous
authorities that the whole matter is closed, this is far from being the case.
Whatever the final outcome, the ‘Cold
Fusion’ story is the biggest scandal in the history of science, and has
prompted me to frame my Fourth Law: ‘For every expert there is an equal and
opposite expert.’
So there is a real possibility that
the most important event of the early Twenty-First Century will be the advent
of unlimited amounts of clean, cheap energy. This would change our world beyond
recognition: it would mean the end of the fossil fuel age, the air pollution of
our cities, the fear of global warming – in fact, it seems too good to be true.
(In that case, as some of my more sceptical friends keep reminding me, it
probably is.)
Whatever type of energy technology
evolves – fusion, or something completely different – there will be no shortage
of raw material. The seas of this planet contain 100,000,000,000,000,000 tons
of hydrogen and 20,000,000,000,000,000 tons of deuterium – the fundamental
building blocks of all matter. One day we will learn to join these together to
create any element we please.
This survey should be enough to
indicate – though not to prove – that there need never be any permanent
shortages. Yet Sir George Darwin’s prediction that ours would be a Golden Age
compared with the aeons of poverty to follow, may well be perfectly correct. In
this inconceivably enormous universe, we can never run out of energy or matter.
But we can all too easily run out of brains.
13. Aladdin’s
Lamp
[...]
In Chapter Seven, when discussing the
possibility of instantaneous transportation, we considered a device that would
scan solid objects atom by atom to make a ‘recording’ that could ultimately be
played back, either at the spot or at a distance. Though such device cannot be
realised, or even remotely envisaged, in terms of today’s science, no
philosophical contradictions or absurdities are raised if we suppose its
operations limited to fairly simple, inanimate objects. It is worth remembering
that an ordinary camera can, in a thousandth of a second, make a ‘copy’ of a
picture containing millions of details. This would indeed have been a miracle
to an artist of the Middle Ages. The camera is a general-purpose machine for
reproducing, with considerable, though not complete, degree of accuracy, any pattern of light, shade, and colour.
[...]
Leaping lightly across some centuries
of intensive development and discovery, let us consider how the replicator
would operate. It would consist of three basic parts – which we might call
store, memory and organiser. The store would contain, or would have access to,
all the necessary raw materials. The memory would contain the instructions
specifying the manufacture (a word which would then be even more misleading
than it is today!) of all the objects within the size, mass, and complexity
limitations of the machine. Within these limits, it could make anything – just
as a tape-recorder can play any conceivable piece of music that is presented to
it. The physical size of the memory could be quite small, even if it had a
large built-in library of instructions for the most commonly needed artefacts.
One can envision a sort of directory or catalogue, with each item indicated by
a code number which could be punched as required.
The organiser would apply the
instructions to the raw material, presenting the finished product to the
outside world – or signalling its distress if it had run out of some essential
ingredient. Even this might never happen, if the transmutation of matter ever
becomes possible as a safe, small-scale operation, for then the replicator
might operate on nothing but water and air. Starting with the simple elements,
hydrogen, nitrogen and oxygen, the machine would first synthesis higher ones,
then organise these as requested. A rather delicate and fail-safe
mass-balancing procedure would be necessary, otherwise the replicator would
produce, as a highly unwanted by-product, rather more energy than an H-bomb. This
could be absorbed in the production of some easily disposable ‘ash’ such as
lead – or gold.
[...]
Despite what has been said earlier
about the appalling difficulty of synthesising higher organic structures, it is
absurd to suppose that machines cannot eventually create any material made by
living cells. Any last-ditch vitalists who still doubt this are referred to
Chapter Eighteen, where they will discover why inanimate devices can be
fundamentally more efficient and more versatile than living ones – though they
are very far from being so at the present stage of our technology. There is no
reason to suppose, therefore, that the ultimate replicator would not be able to
produce any food that men have ever desired or imagined. The creation of an
impeccably prepared filet mignon
might take a few seconds longer, and require a little more material, than a
paper-clip, but the principle is the same. If this seems astonishing, no one
today is surprised that a hi-fi set can reproduce the sound of a massed choir
as easily as the twang of a tuning fork.
The advent of the replicator would
mean the end of all factories, and perhaps all transportation of raw materials
and all farming. The entire structure of industry and commerce, as it is now
organised, would cease to exist. Every family would produce all that is needed
on the spot – as, indeed, it has had to do throughout most of human history. The
present machine era of mass production would then be seen as a brief
interregnum between two far longer periods of self-sufficiency, and the only
valuable items of exchange would be the matrices, or recordings, which had to
be inserted in the replicator to control its operations.
No one who has read thus far will, I
hope, argue that the replicator would itself be so expensive that nobody could
possibly afford it. The prototype, it is true, might cost trillions, spread
over a few centuries of time. The second model would cost nothing, because the
replicator’s first job would be to produce other replicators. It is perhaps
relevant to point out that in 1951 the great mathematician John von Neumann
established the important principle that a machine could always be designed to
build any desirable machine – including
itself. The human race has squeaking proof of this more than a hundred
thousand times a day.
A society based on the replicator
would be so completely different from ours that the Twentieth Century’s debates
between capitalism and communism would seem quite meaningless. All material
possessions would be literally as cheap as dirt. Soiled handkerchiefs, diamond
tiaras, Mona Lisas totally indistinguishable from the original, once-worn mink
stoles, half-consumed bottles of the most superb champagnes – all would go back
into the hopper when they were no longer required. Even the furniture of the
future might cease to exist when it was not actually in use.
At first sight, it might seem that
nothing could be of any real value in this utopia of infinite riches – this
world beyond the wildest dreams of Aladdin or Croesus. This is a superficial
reaction, such as might be expected from a Tenth Century monk if you told him
that one day every man could own far more books than he could read in a
lifetime. Yet the invention of the printing press has not made books less
valuable, or less appreciated, because they are now amongst the commonest
instead of the rarest of objects. Nor has music lost its charms, now that any
amount can be obtained at the turn of a switch.
When material objects are all
intrinsically worthless, perhaps only then will a real sense of values arise. Works
of art would then be cherished because they were beautiful, not because they
were rare. Nothing – no ‘things’ – would be as priceless as craftsmanship,
personal skills, professional services. One of the charges often made against
our culture is that it is materialistic. How ironic it will be, therefore, if
science give us such total and absolute control over the material universe that
its products no longer tempt us, because they can be too easily obtained.
It is certainly fortunate that the
replicator, if it can ever be built at all, lies far in the future, at the end
of many social revolutions. Confronted by it, our own culture would collapse
speedily into sybaritic hedonism, followed immediately by the boredom of
absolute satiety. Some cynics may doubt if any
society of human beings could adjust itself to unlimited abundance and the
lifting of the curse of Adam – a curse which may be a blessing in disguise.
Yet in every age, a few men have known
such freedom, and not all of them have been corrupted by it. Indeed, I would
define a civilised man as one who can be happily occupied for a lifetime even
if he has no need to work for a living. This means that the greatest problem of
the future is civilising the human race; but we knew that already.
So we may hope, therefore, that one
day our age of roaring factories and bulging warehouses will pass away, as the
spinning wheel and the home loom and the butter church passed before them. And
then our descendants, no longer cluttered up with possessions, will remember
what many of us have forgotten – that the only things in the world that really
matter are such imponderables as beauty and wisdom, laughter and love.
16. Voices
from the Sky
Foreword
After a good deal of heart-searching,
I decided that (apart from minor editorial corrections) this chapter should be
reprinted exactly as it appeared in 1962, because it started to become history
three years later.
For its occasional Failures of
Imagination, see the Postscript...
In the closing days of 1958, a human
voice spoke for the first time from space. It was the President of the United
States, broadcasting a Christmas message to the world. Yet that friendly
greeting from an orbiting Atlas satellite, leaping across all barriers of
geography and nationality, was as fateful a sound as any in the history of
mankind. It marked the dawn of a new age of communication, which will transform
the cultural, political, economic and even linguistic patterns of our world.
It is simple enough to demonstrate
this logically – as I hope to do – but very difficult to grasp its full
meaning. So wonderful are today’s techniques of communication, so integrated
into the very fabric of our society, that we overlook their gross limitations,
and find it hard to imagine any substantial improvements. We are like the early
Victorians who saw no value in the electric telegraph; semaphores or flashing
lights were quite adequate, for anyone who wanted something faster than the
mail coach.
We may laugh at this attitude; yet we
are still, for all our ability to pluck sound and vision from the empty air,
scarcely out of the Morse Code age. Within a few years, communications
satellites beyond the atmosphere will make our present facilities seem as
primitive as Indian smoke signals, and we as blind and deaf as our grandparents
before the coming of the electron tube.
[...]
Perhaps at this point I may be
permitted what has been called the modest cough of the minor poet. To the best
of my knowledge, the use of artificial satellites to provide global TV was
first proposed by myself in the October 1945 issue of the British radio journal
Wireless World. The scheme then put
forward, under the snappy title ‘Extraterrestrial Relays’[23],
envisaged the use of three satellites 22,000 miles above the Equator. At this
particular height, a satellite takes exactly twenty-four hours to complete one
orbit, and thus stays fixed for ever over the same spot on the Earth. The laws
of celestial mechanics can thus provide us with the equivalent of invisible TV towers
22,000 miles high. Even as I write these words, preparations are being made by
the Hughes Aircraft Company and the United States Army to launch communications
satellites into this twenty-four-hour orbit.
At first sight, global TV may hardly
seem a revolutionary force capable of transforming our civilisation. Let us,
therefore, look at some of its consequences in more detail.
In a few years every large nation will
be able to establish (or rent) its own space-born radio and TV transmitters,
able to broadcast really high-quality programmes to the entire planet. There
will be no shortage of wavelengths – as there is today even for local services.
One of the incidental advantages of satellite relays is that they will make
available vast new bands of the radio spectrum, providing ‘ether space’ for at
least a million simultaneous TV channels, or a billion radio circuits!
This will mean the end of all distance
barriers to sound and vision alike. New Yorkers and Londoners will be able to
tune in to Moscow or Peking as easily as to their local station. And, of
course, vice versa.
Think what this will mean. Until
today, even radio has been parochial, except to the shortwave fan willing to
put up with the fades and crackles and banshee wailings of the ionosphere. Yet
now the great highway of the ether will be thrown open to the whole world, and
all men will become neighbours – whether they like it or not. Any form of
censorship, political or otherwise, would be impossible; to jam signals coming
down from the heavens is almost as difficult as blocking the light of the
stars. The Russians could do nothing to stop their people from seeing the
American way of life; on the other hand, Madison Avenue agencies and censorship
committees might be equally distressed – though for different reasons – at a
nationwide switch to uninhibited telecasts from Montmartre.
Such freedom of communication will
have an ultimately overwhelming effect on the cultural, political and moral
climate of our planet. It holds danger as well as promise. If you doubt this,
consider the following quite unimaginative extrapolation, which might be
entitled ‘How to Conquer the World without Anyone Noticing.’
By 1970 the USSR has established the
first high-powered satellite TV relay above Asia, broadcasting in several
languages so that more than a billion viewers can understand the programmes. At
the same time, in a well-organised sales campaign spearheaded by
demonstrations, Russian trade missions have been flooding the East with cheap,
transistorised battery-powered receivers. There is scarcely a village which
cannot afford one and it doesn’t cost the USSR a thing; it even makes a small
profit on the deal.
And so millions who have never learned
to read, who have never seen a movie, who have no rival distractions, fall
under the hypnotic spell which even ostensibly educated nations have been
unable to resist. Good entertainment, rapid (if slanted) news reporting, Russian language lessons,
instructional programmes of a ‘Do It Yourself’ type useful to backwards
communities, quiz shows in which the first prizes are usually trips to the
Soviet Union – it takes little imagination to see the pattern. In a few years
of skilful propaganda, the uncommitted nations would be committed.
But let us turn aside from the
political aspects of the TV satellites and look in more detail at their
domestic effects.
[...]
The effect on the cultural content of
our local TV and radio programmes, when faced with direct competition from the
whole world, is a subject for lively speculation. Some cynics maintain that the
TV relay system is the best argument against
space travel that has ever been conceived; they shudder at the thought of
hundreds of simultaneous Westerns, thousands of rock-and-rolling disc jockeys.
Yet the very profusion of available channels, each capable of being received by
most of the human race, will make possible services of a quality and
specialised nature quite out of the question today. There are probably enough
viewers on Earth to make channels carrying nothing but Greek plays, lectures on
symbolic logic or championship chess an economic possibility.
[...]
The advent of global TV and radio
coverage will end, for better or worse, the cultural and political isolation
which still exists over the whole world, outside the great cities. As one who
has travelled widely throughout the United States, I have long been appalled by
the intellectual vacuum into which you are plunged as soon as you get out of
range of New York, San Francisco, Boston, Chicago, and a handful of other
cities. This applies both to newspapers and to radio/TV; how often have I spent
fruitless hours in places like Skunksville, Ugh., searching for a copy of the
New York Times so that I could find out what was happening to the planet Earth.
And as far as the ether waves are concerned, there are few more harrowing
experiences than a sweep across the radio bands in the Deep South, especially
on a Sunday morning. In England, at least, one is never far from civilisation
(ie the BBCs Third Programme).
The abolition of all barriers to free
intellectual and cultural intercourse will complete the revolution started by
the automobile half a century ago and timidly continued by today’s short-range
electronics. It will mean the eventual end of the limited, small-town mentality
which, it is true, has a certain charm (especially to nostalgic novelists, and
especially from a distance). When all men, wherever they may be, have equal
access to the same vast communications network, they will inevitably become
citizens of the world, and a major problem of the future will be the
preservation of regional characteristics of value and interest. There is grave
danger of global levelling-down; the troughs in man’s cultural heritage must
not be filled at the price of demolishing the peaks.
[...]
All that has been described so far –
even this last development [two or three dominant world languages – Ed.] – will
result from the application of existing techniques, merely made worldwide by
the use of satellite relays. It is time to consider some of the wholly new series
which will become feasible, if we wish to exploit them.
The most obvious is the personal
transceiver, so small and compact that every man carries one with no more
inconvenience than a wristwatch. This, of course, is an old dream, and anyone
who doubts that it can be realised is simply unaware of current achievements in
electronics. Radio receivers have now been built which make the most compact
transistor portables look like the 1925 cabinet models. The smallest so far
revealed by the micro-miniaturisation experts is about the size of a lump of
sugar.
Without going into technical details
(of interest largely to those who can already think of the answers) the time
will come when we will be able to call a person anywhere on Earth, merely by
dialing a number. He will be located automatically, whether he is in mid-ocean,
in the heart of a great city, or crossing the Sahara. This device alone may
change the patterns of society and commerce as greatly as the telephone, its
primitive successor, has already done.
Its peril and disadvantages are
obvious; there are no wholly beneficial inventions. Yet think of the countless
lives it would save, the tragedies and heartbreaks it would aver. (Remember
what the telephone has meant to lonely people everywhere.)
No one need ever again be lost, for a
simple position-and-direction-finding device could be incorporated in the
receiver, based on the principle of today’s radar navigational aids. And in
case of danger or accident, help could be summoned merely by pressing an
‘Emergency’ button.
If you think that this will make the
world a claustrophobically small place, in which you can never escape from
friends and family, or even run any stimulating risks, you are quite correct. But
you need not worry; there is more than enough danger and distance in the
bottomless chasm of Space. Earth is home now; let us make it cosy and
comfortable and safe. The pioneers will be elsewhere.
As communications improve, so the need
for transportation will decrease. Our grandchildren will scarcely believe that
millions once spent hours of every day fighting their way into city offices –
where, as often as not, they did nothing that could not have been achieved over
telecommunication links.
For global phone and vision services,
enabling men to confer with each other anywhere on the planet, are only a
beginning. Even now we have data-handling systems linking together factories
and offices miles apart, controlling nationwide industrial empires. Electronics
is already permitting the decentralisation which rising rents and transport
costs – not to mention the threat of the mushroom cloud – encourage more
strongly than ever before.
The business of the future may be run
by executives who are scarcely ever in each other’s physical presence. It will
not even have an address or a central office – only the equivalent of a
telephone number. For its files and records will be space rented in the memory
units of computers that could be located anywhere on Earth: the information
stored in them could read off on high-speed printers whenever any of the firm’s
offices needed it.
The time may come when half the
world’s business will be transacted through vast memory banks beneath the
Arizona desert, the Mongolian steppes, the Labrador muskeg, or whatever land is
cheap and useless for any other purpose. For all spots on Earth, of course, would
be equally accessible to the beams of the relay satellites: to sweep from Pole
to Pole would mean merely turning the directional antennae through seventeen
degrees.
And so the captains of industry of the
Twenty-First Century may live where they please, running their affairs through
computer keyboards and information-handling machines in their homes. Only on
rare occasions would there be any need for more of the personal touch than
could be obtained via wide-screen full-colour TV. The business lunch of the
future could be conducted perfectly well with the two halves of the table ten
thousand miles apart; all that would be missing would be the handshakes and
exchange of cigars.
Administrative and executive skills
are not the only ones which would thus become independent of geography. Distance
has already been abolished for the three basic senses of sight, hearing, and
touch – the latter, thanks to the development of remote-handling devices in the
atomic energy field. Any activity
which depends on these senses can, therefore, be carried out over radio
circuits. The time will certainly come when surgeons will be able to operate a
world away from their patients, and every hospitable will be able to call on
the services of the best specialists, wherever they may be.
An application of satellites which has
already been considered in some detail by the astronautical engineers is what
has been called the orbital post office, which will probably make airmail
obsolete in the quite near future. Modern facsimile systems can automatically
transmit and reproduce the equivalent of an entire book in less than a minute. By
using these techniques, a single satellite could handle the whole of today’s
transatlantic correspondence.
[...]
Perhaps a decade beyond the orbital
post office lies something even more startling – the orbital newspaper. This
will be made possible by more sophisticated descendants of the reproducing and
facsimile machines now found in most up-to-date offices. One of these, working
in conjunction with the TV set, will be able on demand to make a permanent
record of the picture flashed on the screen. Thus when you want your daily
paper, you will switch to the appropriate channel, press the right button – and
collect the latest edition as it emerges from the slot. It may be merely a
one-page news sheet; the editorials will be available on another channel –
sport, book reviews, drama, advertising, on others. We will select what we need
and ignore the rest, thus saving whole forests for posterity. The orbital
newspaper will have little more than the name in common with the newspaper of
today.
Nor will the matter end here. Over the
same circuits we will be able to conjure up, from central libraries and
information banks, copies of any document we desire, from Magna Carta to the
current Earth-Moon passenger schedules. Even books may one day be ‘distributed’
in this manner, though their format will have to be changed drastically to make
this possible.
All publishers would do well to
contemplate these really staggering prospects. Most affected will be newspapers
and paperbacks; practically untouched by the coming revolution will be art
volumes and quality magazines, which involve not only fine printing but
elaborate manufacturing process. The dailies may well tremble; the glossy
monthlies have little to fear.
How mankind will cope with the
avalanche of information and entertainment about to descend upon it from the
skies, only the future can show. Once again science, with its usual cheerful
irresponsibility, has left another squalling infant on civilisation’s doorstep.
It may grow up to be as big a problem child as the one born amid the clicking
Geiger counters beneath the Chicago University squash court, back in 1942.
For will there be time to do any work
at all on a planet saturated from Pole to Pole with fine entertainment,
first-class music, brilliant discussions, superbly executed athletics, and
every conceivable type of information service? Even now, it is claimed, our
children spent a sixth of their waking lives glued to the cathode-ray tube. We
are becoming a race of watchers, not of doers. The miraculous powers that are yet
to come may well prove more than our self-discipline can withstand.
If this is so, then the epitaph of our
race should read, in fleeting, fluorescent letters: Whom the Gods would destroy, they first give TV.
Postscript
Well...
Virtually everything in the above
chapter has happened, far sooner than I imagined, though sometimes in a
slightly different form. Thus I never imagined – who did? – that the fax
machine, and the even more ubiquitous personal computer, would bring most of
the services described above into every home. And the Information Technology
revolution is still gathering momentum...
But one promised benefit of electronic
data storage has still failed to materialise.
Have you seen any ‘paperless office’
yet? We are chopping down the world’s forests faster than ever...
17. Brain and
Body
[...]
A safe and practical form of suspended
animation – which involves no medical impossibility and may indeed be regarded
as an extension to anaesthesia – could have major effects upon society. Men
suffering from incurable diseases might choose to leapfrog ten or twenty years,
in the hope that medical science might have caught up with their condition. The
insane, and criminals beyond our present powers of redemption, might also be
sent forwards in time, in the expectation that the future could salvage them.
Out descendants might not appreciate this legacy, of course, but at least they
could not send it back.
All this assumes – though no one has
yet proved it – that the legend of Rip van Winkle is scientifically sound, and
that the processes of ageing would be slowed down, or even checked, during
suspended animation. Thus a sleeping man could travel down the centuries,
stopping from time to time and exploring the future as today we explore space. There
are always misfits in every age who might prefer to do this, if they were given
the opportunity, so that they could see the world that will exist far beyond
their normal span of life.
And this brings us to what is,
perhaps, the greatest enigma of all. Is
there a normal span of life, or do all creatures really die by ‘accident’? Though
we now live, on the average, far longer than our ancestors, the absolute limit
does not seem to have altered since records became available. The Biblical
limit three-scores-years-and-ten is still as valid today as it was four
thousand years ago.
No human being has been proved to have
lived more than about 120 years; the much higher figures often quoted are
almost certainly due to fraud or error. Man, it seems, is the longest lived of
all the mammals, but some fishes and tortoises may attain their second century.
And trees, of course, have incredible life-spans; the oldest known living
organism is a small and unprepossessing bristlecone pine in the foothills of
Sierra Nevada. It has been growing, though hardly flourishing, for 4,600 years.
Death (not ageing) is obviously
essential for progress, both social and biological. Even if it did not perish
from overpopulation, a world of immortals would soon stagnate. In every sphere
of human activity, one can find examples of the stultifying influence of men
who have outlived their usefulness. Yet death – like sleep – does not appear to
be biologically inevitable, even if it is an evolutionary necessity.
Our bodies are not like machines; they
never wear our, because they are continually rebuilt from new materials. If
this process were uniformly efficient, we would be immortal. Unfortunately,
after a few decades something seems to go wrong in the repair-and-maintenance
department; the materials are as good as ever, but the old plans get lost or
ignored, and vital services are not properly restored when they break down. It
is as if the cells of the body can no longer remember the jobs they once did so
well.
The way of avoiding a failure of
memory is to keep better records, and perhaps one day we will be able to help
our bodies to do just that. The invention of the alphabet made mental
forgetfulness no longer inevitable; the more sophisticated tools of future
medicine may cure physical forgetfulness by allowing us to preserve, in some
suitable storage device, the ideal prototypes of our bodies. Deviations from
the norm could then be checked from time to time and corrected, before they
became serious.
Because biological immortality and the
preservation of youth are such potent lures, men will never cease to search for
them, tantalised by the examples of creatures who live for centuries and
undeterred by the unfortunate experience of Dr Faust. It would be foolish to
imagine that this search will never be successful, down all the ages that lie
ahead. Whether success would be desirable is quite another matter.
(In The Last Mortal Generation (1999), the Australian polymath and
science fiction writer Damien Broderick has suggested that immortality is not
merely desirable – but inevitable. My recommendation of this truly
mind-stretching book was not in the least affected by its dedication: ‘For
Arthur C. Clarke, who profiled the future and dreamed a future of advanced
sciences indistinguishable from magic.’)
The body is the vehicle of the brain,
and the brain is the seat of the mind. In the past, this triad has been
inseparable, but it will not always be so. If we cannot prevent our bodies from
disintegrating, we may replace them while there is yet time.
The replacement need not be another
body of flesh and blood; it could be a machine, and this may represent the next
stage of evolution. Even if the brain is not immortal, it could certainly live
much longer than the body whose diseases and accidents eventually bring it low.
More than half a century ago, in a famous series of experiments, Russian
surgeons kept a dog’s head alive for some days by purely mechanical means. I do
not know if they have yet succeeded with humans, but I shall be surprised if
they have not tried.
If you think that immobile brain would
lead a very dull sort of life, you have not fully understood what has already
been said about the senses. A brain connected by wire or radio links to
suitable organs could participate in any conceivable experience, real or
imaginary. When you touch something, are you really aware that your brain is not at your fingertips, but three
feet away? And would you notice the difference if that three feet were three
thousand miles? Radio waves make such a journey more swiftly than the nervous
impulses can travel along your arm.
One can imagine a time when men who
still inhabit organic bodies are regarded with pity by those who have passed on
to an infinitely richer mode of existence, capable of throwing their
consciousness or sphere of attention instantaneously to any point on land, sea,
or sky where there is a suitable sensing organ. In adolescence we leave
childhood behind; one day there may be a second and more portentous
adolescence, when we bid farewell to the flesh. (Carnivale, in the literal sense!)
But even if we can keep the brain
alive indefinitely, surely in the end it would be clogged with memories,
overlaid like a palimpsest with so many impressions and experiences that there
was no room for more? Eventually, perhaps yes, though I would repeat again that
we have no idea of the ultimate capacity of a well-trained mind, even without
the mechanical aids which will certainly become available. As a good round
figure, a thousand years would seem to be about the ultimate limit for
continuous human existence – though suspended animation might spread this
millennium across far longer vistas of time.
Yet there may be a way past even this
barrier, as I suggested in The City and
the Stars (1956). This was an
attempt to envisage a virtually eternal society, in the closed city of Diaspar,
a billion years from now. I would like to end by quoting the words in which my
hero learns the facts of life from his old tutor, Jeserac:
A human being, like any other
object, is defined by its structure – its pattern. The pattern of a man is
incredibly complex; yet Nature was once able to pack that pattern into a tiny
cell, too small for the eye to see.
What Nature can do, Man can
do also, in his own way. We do not know how long the task took. A million
years, perhaps – but what is that? In the end our ancestors learned to analyse
and store the information that would define any specific human being – and to
use that information to recreate the original.
The way in which
information is stored is of no importance; all that matters is the information
itself. It may be in the form of written words on paper, or varying magnetic
fields, or patterns of electric charge. Men have used all these methods of
storage, and many others. Suffice to say that long ago they were able to store
themselves – or, to be more precise, the disembodied patterns from which they
could be called back into existence.
In a little while, I shall
prepare to leave this life. I shall go back through my memories, editing them
and cancelling those I do not wish to keep. Then I shall walk into the Hall of
Creation, but through a door that you have never seen. This old body will cease
to exist, and so will consciousness itself. Nothing will be left of Jeserac but
a galaxy of electrons frozen in the heart of a crystal.
I shall sleep, and without
dreams. Then one day, perhaps a hundred thousand years from now, I shall find
myself in a new body, meeting those who have been chosen to be my guardians...
At first I will know nothing of Diaspar and will have no memories of what I was
before. Those memories will slowly return, at the end of my infancy, and I will
build upon them as I move forward into my new cycle of existence.
This is the pattern of our
lives... We have all been here many, many times before, though as the intervals
of nonexistence vary according to random laws, this present population will
never repeat itself. The new Jeserac will have new and different friends and
interests, but the old Jeserac – as much of him as I wish to save – will still
exist.
So at any moment only a
hundredth of the citizens of Diaspar live and walk in its streets. The vast
majority slumber in the memory banks, waiting for the signal that will call
them forth on to the stage of existence once again. And so we have continuity,
yet change – immortality, but not stagnation...[24]
Is this fantasy? I do not know; but I
suspect that the truths of the far future will be stranger still.
Another possibility which has quite
suddenly come to the attention of the world (largely through Dolly, the most
famous sheep in history) is that of cloning. After denying for years that it
could be done with mammals, biologists are now arguing whether it should be done with humans. I would not
be in the least surprised to hear that it has already happened.
And now, to my considerable amusement,
there is a remote (in all senses of the word) possibility that it may happen to
me. I recently sacrificed some of my
few remaining hairs, to be launched into space as part of the AERO Astro
Corporation’s ‘Encounter Project’. If all goes well, they will leave the Solar
System (after a boost from Jupiter) and the hope is that, maybe a million years
from now, some super-civilisation will capture this primitive artefact from the
past. Recreating its biological contents might be an amusing exercise for their
equivalent of an infants’ class.
Of course, I’ll never know – unless
the experimenters are both very considerate – and Masters of Time.
18. The
Obsolescence of Man[25]
About a million years ago, an
unprepossessing primate discovered that his forelimbs could be used for other
purposes besides locomotion. Objects like sticks and stones could be grasped –
and, once grasped, were useful for killing game, digging up roots, defending or
attacking, and a hundred other jobs. On the third planet of the Sun, tools had
appeared; and the place would never be the same again.
The first users of tools were not men – a fact appreciated only
recently – but prehuman anthropoids; and by their discovery they doomed
themselves. For even the most primitive of tools, such as a naturally pointed
stone that happens to fit the hand, provides a tremendous physical and mental
stimulus to the user. He has to walk erect; he no longer needs huge canine
teeth – since sharp flints can do a better job – and he must develop manual
dexterity of a high order. These are the specifications of Homo sapiens; as soon as they start to be filled, all earlier
models are headed for rapid obsolescence. The quote Professor Sherwood Washburn
of the University of California’s Anthropology Department: ‘It was the success
of the simplest tools that started the whole trend of human evolution and led to
the civilisations of today.’
Note that phrase – ‘the whole trend of
human evolution’. The old idea that man invented tools is therefore a
misleading half-truth; it would be more accurate to say that tools invented man. They were very
primitive tools, in the hands of creatures who were little more than apes. Yet
they led to us – and to the eventual extinction of the ape-men who first
wielded them.
Now the cycle is about to begin again;
but neither history nor prehistory ever exactly repeats itself, and this time
there will be a fascinating twist in the plot. The tools the ape-men invented
caused them to evolve into their successor, H.
sapiens. The tool we have invented is
our successor. Biological evolution has given way to a far more rapid process –
technological evolution. To put it bluntly and brutally, the machine is going
to take over.
This, of course, is hardly an original
idea. That the creations of man’s brain might one day threaten and perhaps
destroy him is such a tired old cliché that no self-respecting science fiction
writer would dare to use it. It goes back, through Capek’s RUR, Samuel Butler’s Erewhon,
Mary Shelley’s Frankenstein and the
Faust legend to the mysterious but perhaps not wholly mythical figure of
Daedalus, King Minos’ one-man Office of Scientific Research. For at least three
thousand years, therefore, a vocal minority of mankind has had grave doubts
about the ultimate outcome of technology. From the self-centred, human point of
view, these doubts are justified. But that, I submit, will not be the only – or
even the most important – point of view for much longer.
When the first large-scale electronic
computers appeared in the late 1940s, they were promptly nicknamed ‘Giant
Brains’ – and the scientific community, as a whole, took a poor view of the
designation. But the scientists objected to the wrong word. The electronic
computers were not giant brains; they
were dwarf brains, and they still are, though they have now grown a
millionfold. Yet even in their present flint-axe stage of evolution, they have
done things which not long ago almost everyone would have claimed to be
impossible – such as translating from language to another, composing music, and
playing a good game of chess. (The moment when IBM’s Deep Blue beat Kasparov is
already regarded as a turning point in history.) And much more important than
any of these infant jeux d’esprit is
the fact that they have breached the barrier between brain and machine.
This is one of the greatest – and
perhaps one of the last – breakthroughs in the history of human thought, like
the discovery that the Earth moves round the Sun, or that man is part of the
animal kingdom, or that E = mc2. All these ideas took time to sink
in, and were frantically denied when first put forward. In the same way, it
will take a little while for humankind to realise that machines can not only
think, but may one day think it off the face of the Earth.
[...]
The fact that most of today’s
computers are still high-sped morons, capable of doing nothing beyond the scope
of the instructions carefully programmed into them, has given many people a
spurious sense of security. No machine, they argue, can possibly be more
intelligent than its makers – the men who designed it, and planned its
functions. It may be a million times faster in operation, but that is quite
irrelevant. Anything and everything that an electronic brain can do must also
be within the scope of a human brain, if it had sufficient time and patience. Above
all, it is maintained, no machine can show originality or creative power or the
other attributes which are fondly labeled ‘human’.
The argument is wholly fallacious;
those who still bring it forth are like the buggy-whip makers who used to poke
fun at stranded Model Ts. Even if it was true, it should give no comfort, as a
careful reading of these remarks by Dr Norbert Wiener (the father of
Cybernetics) will show:
The attitude (the
assumption that machines cannot posses any degree of originality) in my opinion
should be rejected entirely... It is my thesis that machines can and do
transcend some of the limitations of their designers... It may well be that in
principle we cannot make any machine, the elements of whose behaviour we cannot
comprehend sooner or later. This does not mean in any way that we shall be able
to comprehend them in substantially less time than the operation of the machine,
nor even within any given number of years or generations...
This means that though they
are theoretically subject to human criticism, such criticism may be ineffective
until a time long after it is relevant.
In other words, even machines less intelligent than us might escape
from our control by sheer speed of operation. And in fact, there is every
reason to suppose that machines will become much more intelligent than their
builders, as well as incomparably faster.
[...]
All speculations about intelligent
machines are inevitably conditioned – indeed, inspired – by our knowledge of
the human brain, the only thinking device currently on the market. No one, of
course, pretends to understand the full workings of the brain, or expects that
such knowledge will be available in any foreseeable future. (It is a nice
philosophical point as to whether the brain can ever, even in principle,
understand itself.) But we do know enough about its physical structure to draw
many conclusions about the limitations of ‘brains’ – whether organic or
inorganic.
There are approximately ten billion
separate switches – or neurons – inside your skull, ‘wired’ together in
circuits of unimaginable complexity. Ten billion is such a large number that,
until recently, it could be used as an argument against the achievement of
mechanical intelligence. In the 1950s a famous neurophysiologist made a
statement (chanted briefly like some protective incantation by the advocates of
cerebral supremacy) to the effect that an electronic model of the human brain
would have to be as large as the Empire State Building, and would need Niagara
Falls to keep it cool when it was running.
This must now be classed with such
interesting pronouncements as: ‘No heavier-than-air machine will ever be able
to fly.’ For this calculation was made in the days of the vacuum tube, and the
transistor promptly altered the picture. Indeed – such was the rate of
technological progress – the transistor itself was quickly replaced by the
microchip. If the problem was merely one of space, today’s electronic
techniques would allow us, at least in theory, to pack a computer as complex as
the human brain – inside a human skull. (Stop Press: now read ‘matchbox’.)[26]
[...]
During the 1950s, the electronic
engineers learned to pack up to a hundred thousand components into one cubic
foot. (To give a basis of comparison, a good hi-fi set may contain two or three
hundred components, a domestic radio about a hundred.) In the ‘60s, the
attainable figure was around a million components per cubic foot; by the 1970s,
it was in the hundred millions.
Fantastic though this last figure is,
the human brain surpasses it by a thousandfold, packing its ten billion neurons
into a tenth of a cubic foot. And
although smallness is not necessarily a virtue, even this may be nowhere near
the limit of possible compactness.
For the cells composing our brains are
slow-acting, bulky, and wasteful of energy – compared with the scarcely more
than atom-sized computer elements that are theoretically possible. The
mathematician John von Neumann once calculated that electronic cells could be
ten billion times more efficient than protoplasmic ones; already they are a
million times swifter in operation, and speed can often be traded for size. If
we take these ideas to their ultimate conclusion, it appears that a computer
equivalent in power to one human brain need be no bigger than a matchbox.
This slightly shattering thought
becomes more reasonable when we take a critical look at flesh and blood and
bone as engineering materials. All living creatures are marvellous, but let us
keep our sense of proportion. Perhaps the most wonderful think about Life is that
it works at all, when it has to employ such extraordinary materials, and has to
tackle its problems in such roundabout ways.
As a perfect example of this, consider
the eye. Suppose you were given the
problem of designing a camera – for that, of course, is what the eye is – which
has to be constructed entirely of water
and jelly, without using a scrap of glass, metal or plastic. Obviously it
can’t be done.
You’re quite right; the feat is
impossible. The eye is an evolutionary miracle, but it’s a lousy camera. You
can prove this while you’re reading the next sentence.
Here is a medium-length word: –
PHOTOGRAPHY. Close one eye and keep the other fixed – repeat, fixed – on that centre ‘G’. You may be
surprised to discover that – unless you cheat by altering the direction of your
gaze – you cannot see the whole word clearly. It fades out three or four
letters to the right and left.
No camera ever built – even the
cheapest ‘disposable’ – has as poor an optical performance as this. For colour
vision also, the human eye is nothing to boast about; it can operate only over
a small band of the spectrum. To the worlds of the infrared and ultraviolet,
visible to bees and other insects, it is completely blind.
We are not conscious of these
limitations because we have grown up with them, and indeed, if they were
corrected, the brain would be quite unable to handle the vastly increased flood
of information. But let us not make a virtue of a necessity; if our eyes had
the optical performance of even the cheapest camera, we would live in an
unimaginably richer and more colourful world.
These defects are due to the fact that
precision scientific instruments simply cannot be manufactured from living
materials. With the eye, the ear, the nose – indeed, all the sense organs –
evolution has performed a truly incredible job against fantastic odds. But it
will not be good enough for the future; indeed, it is not good enough for the
present.
There are some senses that do not
exist, that can probably never be provided by living structures, and that we
need in a hurry. On this planet, to the best of our knowledge, no creature has
ever developed organs that can detect radio waves or radioactivity. Though I
would hate to lay down the law and claim that nowhere in the Universe can there
be organic Geiger counters or living TV sets, I think it highly improbable. There
are some jobs that can be done only by transistors or magnetic fields or
electron beams, and are therefore beyond the capability of purely organic
creatures.
There is another fundamental reason
living machines such as you and I cannot hope to compete with non-living ones. Quite
apart from our poor materials, we are handicapped by one of the toughest
engineering specifications ever issued. What sort of performance would you
expect from a machine which has to grow several billionfold during the course
of manufacture – and which has to be completely and continuously rebuilt,
molecule by molecule, every few weeks? This is what happens to all of us, all
the time; you are – quite literally – not the person you were last year.
Most of the energy and effort required
to run the body goes into its perpetual tearing down and rebuilding – a cycle
completed every few weeks. New York City, which is a very much simpler
structure than a human being, takes hundreds of times longer to remake itself. When
one tries to picture the body’s myriads of building contractors and utility
companies all furiously at work tearing up arteries, nerves and even bones, it
is astonishing that there is any energy left over for the business of thinking.
Now I am perfectly well aware that
many of the ‘limitations’ and ‘defects’ just mentioned are nothing of the sort,
looked at from another point of view; living creatures, because of their very
nature, can evolve from simple to complex organisms. They may well be the only
path by which intelligence can be obtained, for it is a little difficult to see
how a lifeless planet can progress directly from metal ores and mineral
deposits to electronic computers by its own unaided efforts.
Though intelligence can arise only
from life, it may then discard it. Perhaps at a later stage, as the mystics
have suggested, it may also discard matter; but this leads us in realms of
speculations where an unimaginative person like myself would prefer to avoid.
One often-stressed advantage of living
creatures is that they are self-repairing and reproduce themselves with ease –
indeed, with enthusiasm. This superiority over machines will be short-lived;
the general principles underlying the construction of self-repairing and self-reproducing
machines have already been worked out.
The greatest single stimulus in the
evolution of mechanical – as opposed to organic – intelligence is the challenge
of Space. Only a vanishingly small fraction of the Universe is directly
accessible to mankind, in the sense that we can live there without elaborate
protection or mechanical aids. [...] If we reduced the known Universe to the
size of the Earth, then the portion in which we can live without space suits and pressure cabins is about the
size of a single atom.
It is true that, one day, we are going
to explore and colonise many other atoms in this Earth-sized volume, but it
will be at the cost of tremendous technical efforts, for most of our energies
will be devoted to protecting our frail and sensitive bodies against the
extremes of temperature, pressure or gravity found in Space and on other
worlds. Within very wide limits, machines are indifferent to these extremes. Even
more important, they can wait patiently through the years and the centuries that
will be needed for travel to the far reaches of the Universe.
Creatures of flesh and blood such as
ourselves can explore Space and win control over infinitesimal fractions of it.
But only creatures of metal and plastic can ever really conquer it, as indeed
they have already started to do. The tiny brains of our Voyagers and
Pathfinders[27] barely hint at the
mechanical intelligence that will one day be launched at the stars.
It may well be that only in Space,
confronted with environments fiercer and more complex than any to be found upon
this planet, will intelligence be able to reach its fullest stature. Like other
qualities, intelligence is developed by struggle and conflict; in the ages to
come, the dullards may remain on placid Earth, and real genius will flourish
only in Space – the realm of the machine, not of flesh and blood.
A striking parallel to this situation
can already be found on our planet. Some millions of years ago, the most
intelligent of the mammals withdrew from the battle of the dry land and
returned to their ancestral home, the sea. They are still there, with brains
larger and potentially more powerful than ours. But (as far as we know) they do
not use them; the static environment of the sea makes little call upon
intelligence. The porpoises and whales, which might have been our equals and
perhaps our superiors had they remained on land, now race in simpleminded and
innocent ecstasy beside the new sea monsters carrying a hundred megatons[28]
of death. Perhaps they, not we, made the right choice; but it is too late to
join them now.
If you have followed me so far, the
protoplasmic computer inside your skull should now be programmed to accept the
idea – at least for the sake of argument – that machines can be both more
intelligent and more versatile than men, and may well be so in the very near
future. So it is time to face the question: Where does that leave Man?
I suspect that this is not a question
of very great importance – except, of course, to Man. Perhaps the
Neanderthalers made similar plaintive noises, around 100,000 BC, when H. sapiens appeared on the scene, with
his ugly vertical forehead and ridiculous protruding chin. Any Paleolithic
philosopher who gave his colleagues the right answer would probably have ended
up in the cooking pot; I am prepared to take that risk.
The short-term answer may indeed be
cheerful rather than depressing. There may be a brief Golden Age when men will
glory in the power and range of their new partners.
[...]
And this is perhaps the moment to deal
with a conception which many people find even more horrifying than the idea
that machines will replace or supersede us. It is the idea, already mentioned
in the last chapter, that they may combine with us.
I do not know who first thought of
this; probably the physicist J. D. Bernal (1901–71), who in 1929 published an
extraordinary book of scientific predictions called The World, the Flesh and the Devil. In this slim volume (reprinted
in 1968, after considerable bullying from me[29])
Bernal decided that the numerous limitations of the human body could be
overcome only by the use of mechanical attachments or substitutes – until,
eventually, all that might be left of man’s original organic body would be the
brain.
This idea is already far more
plausible than when Bernal advanced it, for now we have seen the development of
mechanical hearts, kidneys, lungs and other organs, and the wiring of
electronic devices directly into the human nervous system.
[...]
The now familiar word ‘Cyborg’
(cybernetic organism) was coined to describe the machine-animal of the type we
have been discussing. Doctors Manfred Clynes and Nathan Kline of Rockland State
Hospital, Orangeburg, New York, who invented the name in the 1960s, defined a
Cyborg in these stirring words: ‘an exogenously extended organisational complex
functioning as a homeostatic system.’ So now you know...
To translate, it means a body which
has machines hitched to it, or built into it, to take over or modify some of
its functions. I suppose one could call a man in an iron lung a Cyborg, but the
concept has far wider implications than this. One day we may be able to enter
into temporary unions with any sufficiently sophisticated machines, thus being
able not merely to control but to become
a spaceship or a submarine or a TV network. This would give far more than
purely intellectual satisfaction; the thrill that can be obtained from driving
a racing car or flying an aeroplane may be only a pale ghost of the excitement
our great-grandchildren may know when the individual human consciousness is
free to roam at will from machine to machine, through all the reaches of sea
and sky and space.
But how long will this partnership
last? Can the synthesis of man and machine ever be stable, or will the purely
organic component become such a hindrance that it has to be discarded? If this
eventually happens – and I have given good reasons for thinking that it must –
we have nothing to regret, and certainly nothing to fear.
The popular idea, fostered by comic
strips and the cheaper forms of science fiction, that intelligent machines must
be malevolent entities hostile to man, is so absurd that it is hardly worth
wasting energy to refute it. I am almost tempted to argue that only unintelligent machines can be
malevolent; anybody who has tried to start a baulky outboard motor will
probably agree. Those who picture machines as active enemies are merely
projecting their own aggressive instincts, inherited from the jungle, into a
world where such things do not exist. The higher the intelligence, the greater
the degree of cooperativeness. If there is ever a war between men and machines,
it is easy to guess who will start it.
Yet however friendly and helpful the
machines of the future may be, most people will feel that it is a rather bleak
prospect for humanity if it ends up as a pampered specimen in some biological
museum – even if that museum is the whole planet Earth. This, however, is an
attitude I find hard to share.
No individual exists for ever; why
should we expect our species to be immortal? Man, said Nietzsche, is a rope stretched
between the animal and the superhuman – a rope across an abyss. That will be a
noble purpose to have served.
Postscript
The above chapter was written in the
year 6 BH (Before HAL) and many of the concepts in it are now taken for
granted.
[...]
Although even 1992 seemed a reasonable
date when we were working on the script in 1964–8, creating a computer with
anything like Hal’s capabilities has proved far more difficult than any of the
enthusiasts for artificial intelligence imagined: some of their predictions now
make embarrassing reading. Ironically, one key incident in the movie which I
thought somewhat improbable - Hal’s
lip-reading exploit – is now the subject of intensive research.
[...]
19. The Long
Twilight
Looking back over the preceding
chapters, I am aware of numerous inconsistencies and some omissions. As for the
first, I am unrepentant, for the reasons given in the introduction. In
attempting to explore rival and indeed contradictory possibilities, I have
tried to go to the end of the line in each case; sometimes this has lead to a
sense of pride in Man’s past and possible future achievements – sometimes to a
conviction that we present only a very early stage in the story of evolution,
destined to pass away leaving little mark on the universe.
Concerning the omissions, some are due
to a frank lack of interest on my part, others to a feeling that I did not have
the necessary qualifications to discuss them. The last reason accounts for the
fact that medical and biological themes were not developed in much more detail.
It seems perfectly possible that many future achievements of production,
sensing, data-processing, and manufacture may be based on living or
quasi-living creatures, rather than inorganic devices. Nature provides, at zero
cost, so many marvellous mechanisms that it seems foolish not to employ them to
the utmost. I have little doubt that our descendants will use many intelligent
animals to do jobs that could otherwise be performed only by very expensive and
sophisticated robots.
In this connection, I might have
discussed the attempts that have been made to establish communication with
dolphins. I might have said a good deal more about the possibility of
contacting extraterrestrial intelligences by radio or laser (coherent light)
beams. One or both of these objectives will be achieved, sooner or later, but
both open up vistas so unlimited that it is fruitless to speculate about them;
there are no boundary posts here, as yet, to mark the border between science
and fantasy.
[...]
Certain types of symmetrical or
ordered structure, certain kinds of energy release, are so abnormal that they
point to an intelligent origin. Thus on our planet, when the energy equivalent
to several megatons appears in an area a few miles across, it can be a volcano;
when it appears at a point source, it can only be a bomb.
The radio astronomers are now
discovering some most extraordinary phenomena in other galaxies; Virgo A
(Messier 87), for example, has a brilliant jet extending from its nucleus, like
a searchlight beam hundred of light-years long. What is so peculiar about this
jet is the concentration of energy it contains – perhaps equivalent to that of
millions of supernovae, or the radiation from millions of millions of ordinary stars. In fact, to power this jet, a mass
equivalent to about a hundred suns would have to be completely annihilated!
This is hard to explain in terms of
any known natural process; it is like comparing an H-bomb to a geyser. Almost
certainly there is a natural
explanation, which we have not yet discovered – though there are plenty of
theories – but it is tempting to speculate about the alternative. Given
sufficient time, rational beings might attain the power to manipulate not
merely planets, not merely stars, but the galaxies themselves. If the jet from
M.87 is artificial, what is its purpose? Is it an attempt to signal across
intergalactic space? A tool of cosmic engineers? A weapon? Or some by-product
of incomprehensible religions and philosophies – as on our own planet, the
Great Pyramid is a gigantic symbol of a now almost wholly alien mentality?
Such projects would demand vistas of
time, and continuity of cultures, on a scale inconceivable to us. The time is
there; of that there is no doubt. Each generation of astronomers multiplies the
age of the universe by ten; the current estimate appears to be about
twenty-five billion years. If we say that human civilisation has existed for
about a millionth of the age of this Galaxy, we may not be far wrong.
But it also appears that the past
duration of the Galaxy is a mere flicker of time, compared to aeons that may
lie ahead. At their present lavish rate of radiation, stars such as the Sun can
continue to burn for billions of years; then, after various internal
vicissitudes, they settle down to a more modest mode of existence as dwarf
stars. The reformed stellar spendthrifts can then shine steadily for periods of
time measured not in billions but in trillions (millions of millions) of years.
The planets of such stars, if at the same distance from their primary as Earth
(or even Mercury) would be frozen at temperatures hundreds of degrees below
zero. But by the time we are considering, natural or artificial planets could
have been moved sunwards to huddle against the oncoming Ice Age as, long ago,
our savage ancestors must have gathered around their fires to protect
themselves from the cold and the creatures of the night.
In a famous elegiac passage, Bertrand
Russell once remarked:
...that all the labours of
the ages, all the devotion, all the inspiration, all the noonday brightness of
human genius, are destined to extinction in the vast death of the solar system,
and that the whole temple of Man’s achievement must inevitably be buried
beneath the debris of a universe in ruin – all these things, if not quite
beyond dispute, are yet so nearly certain, that no philosophy which rejects
them can hope to stand.[30]
Even if this is true, the ruin of the
universe is so inconceivably far ahead that it can never be any direct concern
of our species. Or, perhaps, of any species that now exists, anywhere in the
spinning whirlpool of stars we call the Milky Way.
[...]
In that case, our Galaxy is now in the
brief springtime of its life – a springtime made glorious by such brilliant
blue-white stars as Vega and Sirius, and, on a more humble scale, our own Sun. Not
until all these have flamed through their incandescent youth, in a few fleeting
billions of years, will the real
history of the Universe begin.
It will be a history illuminated only
by the reds and infrareds of dully glowing stars that would be almost invisible
to our eyes; yet the sombre hues of that all-but-eternal Universe may be full
of colour and beauty to whatever strange beings have adapted to it. They will
know that before them lie, not the millions of years in which we measure eras
of geology, nor the billions of years which span the past lives of the stars, but
years to be counted literally in trillions.
They will have time enough, in those
endless aeons, to attempt all things, and to gather all knowledge. They will not
be like gods, because no gods imagined by our minds have ever possessed the
powers they will command. But for all that, they may envy us, basking in the
bright afterglow of Creation; for we knew the universe when it was young.
[1] The electrocution experiments and the
Electric Chair reference are not in the original 1962 edition.
[2] This addition in brackets is not in
the original 1962 edition.
[3] Woolley has been somewhat vindicated
in recent years. Apparently he was misquoted, having referred to sensational
newspaper articles about space travel and moon colonisation with “All this talk
about space travel is utter bilge, really”. (See the Omniscient
Entity.) That may be so. Indeed, Arthur himself at least twice in later
essays, “When Will the Real Space Age Begin?” (1996) and “Science and Society”
(1998), both reprinted in Greetings,
Carbon-Based Bipeds! (1999), admitted the misquotation. But if Mr
Woolley, who died in 1986 at the age of 80, ever contributed anything to the
British or any other space effort, history appears very silent about it.
Arthur’s footnote in this book may be the only evidence.
[4] The original 1962 edition doesn’t, of
course, mention VCR. The other machines are the same though, with the addition
of “a television set” – still cutting-edge stuff in those days, rapidly
becoming obsolete in ours.
[5] The fantasy of explaining to the
scientist before 1900 the secrets of the atomic bomb is the same as in the 1962
edition. The latter, however, contains a charming example from much farther
back in time which was later omitted: “What could be simpler than banging two
lumps of metal together? Yet how could one explain to Archimedes that the
result could be more devastating than that produced by all the wars between the
Trojans and the Greeks?”
[6] The 1962 edition reads “from the ox
cart to the Cadillac”, a more elegant alternative.
[7] The last sentence not in the 1962
edition.
[8] That “perhaps” charmingly skipped in
the 1962 edition.
[9] In the 1962 edition the cartoon is
just “famous” and remains unexplained.
[10] The Pickering “débâcle” is omitted in this selection of
quotes. William Pickering was an astronomer who, a few years after the first
airplanes flew, derided the idea of “gigantic flying machines speeding across
the Atlantic and carrying innumerable passengers” as “wholly visionary”. Mr
Pickering, in general not an unimaginative fellow, could only conceive of
planes carrying one or two passengers at exorbitant expense and speeds that
cannot compete with trains and cars. Arthur gleefully remarks that Mr
Pickering, before his death in 1938, managed to see planes travelling at 400
mph and carrying quite a few passengers more than “one or two”.
[11] The Tom Clancy quip –
shattering both him and Shute – was naturally not in the 1962 edition. Neither,
of course, was the previous paragraph.
[12] The 1962 edition has
“within another generation” instead of “soon”.
[13] The 1962 edition has “Queen Elizabeth to Mars” instead of a
nameless liner to the Moon. The next sentence is also made more reasonable; the
fact of “everyday missilry” is not “far more” but “just as” fantastic as
personal antigravity devices.
[14] This paragraph is
considerably different in the 1962 edition. Mark Twain has lost the battle with
Kipling, Tennessee Williams is not mentioned by name at all and neither are
Nabokov or Carroll referred to by their most famous works.
Writers
cannot escape from his environment, however hard they try. When the frontier is
open we have Homer and Shakespeare – or, to choose less Olympian examples
nearer to our own age, Melville, Conrad, and Mark Twain. When it is closed, the
time has come from Tennessee Williams and the Beatniks – and for Proust, whose
horizon toward the end of his life was a cork-lined room. (If Lewis Carroll had
lived today, he might have given us not Alice
but Lolita.)
[15] This list is slightly different in the 1962 edition. The Ancient Mariner was originally included instead of The Lusiads.
[16] Mars in the 1962 edition.
[17] The 1962 edition has one
sentence more here: “Hu Shih was speaking of the Chinese literary renaissance, circa 1915. Perhaps these words may
apply to a terrestrial renaissance a century hence.”
[18] This “surely” is not in
the 1962 edition. It seems Arthur’s notorious optimism, far from diminishing,
grew stronger in his old age.
[19] Some interesting changes
with the 1962 edition. The original, to begin with, contains almost two full
pages more after Mr Mumford was reduced to fish; I suppose it was removed
because references to the Soviet Union and articles in the Life magazine make it rather more dated than usual. Instead of hope
that he listened to space broadcasts, Mumford’s view of space is dismissed as
“slightly myopic, and conditioned by the present primitive state of the art.”
The Mumford quote comes from The
Transformation [sic] of Man
[1954] in the original: I do not know which the correct reference is. Last and
least, Arthur is slightly inaccurate that Mumford died at the age of 95. He
actually passed away some four months after his 94th birthday.
[20] Arthur’s Russian was a little
rusty there. He skipped an ‘o’ in Komsomolskaya
Pravda (Комсомольская Правда).
[21] “To the Committee on Space
Science”, hearing on 24 July 1975, also published in a volume with the juicy title
page:
Future
Space Programs 1975
Hearings
before the
Subcommittee
on Space Science and
Applications
of the
Committee
on
Science
and Technology
U.S.
House of Representatives
Ninety-fourth Congress
First session
July 22, 23, 24, 29, AND 30, 1975
[22] Here, as well as silently
in many other places, the 1962 edition was used to correct rather obvious
typos. The 2000 Indigo paperback, alas, contains a rich crop of these.
[23] This legendary paper has
been reprinted at least thrice in Arthur’s books. The original version,
figures, equations and all, appears as an appendix in one of his essay
collections, Voices from the Sky (1965), and of
course in his collected papers, Ascent to Orbit (1984). A simplified
version is reprinted in Arthur’s collected essays entitled Greetings, Carbon-Based Bipeds!
(1999).
[24] From Chapter 2, although
heavily edited.
[25] Interesting companion
pieces to this chapter are the essays “Of Mind and Matter”, first published in The Magazine of Fantasy and Science Fiction
(Oct 1958) and later collected in The Challenge of the Spaceship (1958),
and “The Mind of the Machine”, first published in Playboy (Dec 1968) and later collected in Report on Planet Three (1972).
Compare also this passage from 2010: Odyssey Two (1982):
‘Hell, Chandra – he’s only
a machine!’
Chandra looked at Max with
such a steady, confident gaze that the younger man quickly dropped his eyes.
‘So are we all, Mr
Brailovsky. It is merely a matter of degree. Whether we are based on carbon or
on silicon makes no fundamental difference; we should each be treated with
appropriate respect.’
[26] The 1962 version is basically the same, but with some sweet adjustments of scale. No mention of microchip and the computer-as-complex-as-human-brain is squeezed on a single floor of the Empire State Building. But the matchbox equivalent is mentioned later in the text – only the first mention, in the brackets, belongs to the 1999 edition alone.
[27] “Prospectors and Rangers” in the 1962 edition.
[28] Only “sixteen megatons” in the 1962 edition. Such is progress, Arthur might have quipped.
[29] The 1962 edition has very different contents in these brackets: “I sometimes wonder what the sixty-year-old Fellow of the Royal Society now thinks of his youthful indiscretion, if he ever remembers it”.
[30] From “A Free Man’s Worship”
(1903), one of Russell’s earliest and least characteristic writings.