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3001 The final Odissey Печать
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3001 The final Odissey
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mission before the final disaster. Though he and Bowman were perfectly aware
that 7794 was merely a lifeless, airless chunk of rock, that knowledge
scarcely affected their feelings. It was the only solid matter they would
meet this side of Jupiter, and they had stared at it with the emotions of
sailors on a long sea voyage, skirting a coast on which they could not land.
It was turning slowly end over end, and there were mottled patches of
light and shade distributed at random over its surface. Sometimes it
sparkled like a distant window, as planes or outcroppings of crystalline
material flashed in the Sun...
He remembered, also, the mounting tension as they waited to see if
their aim had been accurate. It was not easy to hit such a small target, two
thousand kilometres away, moving at a relative velocity of twenty kilometres
a second.
Then, against the darkened portion of the asteroid, there had been a
sudden, dazzling explosion of light. The tiny slug -- pure Uranium 238 --
had impacted at meteoric speed: in a fraction of a second, all its kinetic
energy had been transformed into heat. A puff of incandescent gas had
erupted briefly into space, and Discovery`s cameras were recording the
rapidly fading spectral lines, looking for the tell-tale signatures of
glowing atoms. A few hours later, back on Earth, the astronomers learned for
the first time the composition of an asteroid`s crust. There were no major
surprises, but several bottles of champagne changed hands.
Captain Chandler himself took little part in the very democratic
discussions around his semi-circular table: he seemed content to let his
crew relax and express their feelings in this informal atmosphere. There was
only one unspoken rule: no serious business at mealtimes. If there were any
technical or operational problems, they had to be dealt with elsewhere.
Poole had been surprised -- and a little shocked -- to discover that
the crew`s knowledge of Goliath`s systems was very superficial. Often he had
asked questions which should have been easily answered, only to be referred
to the ship`s own memory banks. After a while, however, he realized that the
sort of in-depth training he had received in his days was no longer
possible: far too many complex systems were involved for any man or woman`s
mind to master. The various specialists merely had to know what their
equipment did, not how. Reliability depended on redundancy and automatic
checking, and human intervention was much more likely to do harm than good.
Fortunately none was required on this voyage: it had been as uneventful
as any skipper could have hoped, when the new sun of Lucifer dominated the
sky ahead.

III THE WORLDS OF GALILEO


(Extract, text only, Tourist`s Guide to Outer Solar System, v 219.3)

Even today, the giant satellites of what was once Jupiter present us
with major mysteries. Why are four worlds, orbiting the same primary and
very similar in size, so different in most other respects?
Only in the case of Io, the innermost satellite, is there a convincing
explanation. It is so close to Jupiter that the gravitational tides
constantly kneading its interior generate colossal quantities of heat -- so
much, indeed, that Io`s surface is semi-molten. It is the most volcanically
active world in the Solar System; maps of Io have a half-life of only a few
decades.
Though no permanent human bases have ever been established in such an
unstable environment, there have been numerous landings and there is
continuous robot monitoring. (For the tragic fate of the 2571 Expedition,
see Beagle 5.)
Europa, second in distance from Jupiter, was originally entirely
covered in ice, and showed few surface features except a complicated network
of cracks. The tidal forces which dominate Io were much less powerful here,

 
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