
while we've got the chance."
Planning and a sketchy run-through had gone before, and the business went more
smoothly than might have been awaited. But then, it offered a brief escape from what
was outside.
After the cameras had scanned the book-lined room, the battered desk, the portrait
of Einstein, while Fleury gave her introduction, " — scientist, mathematical physicist, as
famous as he is modest — We'll discuss his latest and greatest achievement . . ." they
moved in on her and him, seated in swivel chairs. A projector spread a representation of
the galaxy behind them, ruddy nucleus and outcurving blue-tinged spiral arms,
awesome athwart blackness. Somehow his slight frame belonged in front of it.
She gestured at the grandeur. "Alien spacecraft traveling there, almost at the speed
of light," she said. "Incredible. Perhaps you, Dr. Olivares, can explain to us why it took
so long to convince so many experts that this must be the true explanation."
"Well," he replied, "if the X-ray sources are material objects, the radiation is due to
their passage through the gas in interstellar space. That's an extremely thin gas, a hard
vacuum by our standards here on Earth, but when you move close to
c
— we call the
velocity of unimpeded light
c
— then you slam into a lot of atoms every second. This
energizes them, and they give back the energy in the form of hard X-rays."
For a minute, an animated diagram replaced the galaxy. Electrons tore free of atoms,
fell back, spat quanta. The star images returned as Olivares finished: "To produce the
level of radiation that our instruments measure, those masses must be enormous."
"Mostly due to the speed itself, am I right?" Fleury prompted.
Olivares nodded. "Yes. Energy and mass are equivalent. As a body approaches
c,
its
kinetic energy, therefore its mass, increases without limit. Only such particles as
photons, which have no rest mass, can actually travel at that velocity. For any material
object, the energy required to reach c would be infinite. This is one reason why nothing
can move faster than light.
"The objects, the ships, that we're talking about are moving so close to
c
that their
masses must have increased by a factor of hundreds. Calculating backward, we work
out that their rest masses — the masses they have at ordinary speeds — must amount
to tens of thousands of tonnes. In traditional physics,
this
means that to boost every
such vessel, you would have to annihilate millions of tonnes of matter, and an equal
amount to slow down at journey's end. That's conversion on an astrophysical scale.
Scarcely sounds practical, eh? Besides, it should produce a torrent of neutrinos; but we
have no signs of any."
Fleury picked up her cue. "Also, wouldn't the radiation kill everybody aboard? And if
you hit a speck of dust, wouldn't that be like a nuclear warhead exploding?"
A jet snarled low above the roof. Thunder boomed through the building. Cameras
shivered in men's hands. Fleury tensed. The noise passed, and she found herself
wondering whether or not to edit this moment out of the tapes.
"Go on, please," she urged.
Olivares had glanced at the galaxy, and thence at Einstein. They seemed to calm him.
"Yes," he told the world. "There would have to be some kind of — I'm tempted to say
streamlining. The new spaceborne instruments have shown that this is indeed the case.