been absent—but he would have forged new friendships, he was sure.
Four chimes would have signaled the discovery of intelligent aliens. Five,
a technological civilization. Six, spacefarers.
Three chimes, though, meant that the scout probes had detected unambiguous
signs of life—and that was reason enough for jubilation. Up until the
moment of the pre-launch cloning—a subjective instant before the chimes had
sounded—no reports of alien life had ever reached Earth. There'd been no
guarantee that any part of the diaspora would find it.
Paolo willed the polis library to brief him; it promptly rewired the
declarative memory of his simulated traditional brain with all the
information he was likely to need to satisfy his immediate curiosity. This
clone of C-Z had arrived at Vega, the second closest of the thousand target
stars, twenty-seven light-years from Earth. Paolo closed his eyes and
visualized a star map with a thousand lines radiating out from the sun,
then zoomed in on the trajectory which described his own journey. It had
taken three centuries to reach Vega—but the vast majority of the polis's
twenty thousand inhabitants had programmed their exoselves to suspend them
prior to the cloning, and to wake them only if and when they arrived at a
suitable destination. Ninety-two citizens had chosen the alternative:
experiencing every voyage of the diaspora from start to finish, risking
disappointment, and even death. Paolo now knew that the ship aimed at
Fomalhaut, the target nearest Earth, had been struck by debris and
annihilated en route. He mourned the ninety-two, briefly. He hadn't been
close to any of them, prior to the cloning, and the particular versions
who'd willfully perished two centuries ago in interstellar space seemed as
remote as the victims of some ancient calamity from the era of flesh.
Paolo examined his new home star through the cameras of one of the scout
probes—and the strange filters of the ancestral visual system. In
traditional colors, Vega was a fierce blue-white disk, laced with
prominences. Three times the mass of the sun, twice the size and twice as
hot, sixty times as luminous. Burning hydrogen fast—and already halfway
through its allotted five hundred million years on the main sequence.
Vega's sole planet, Orpheus, had been a featureless blip to the best lunar
interfer-ometers; now Paolo gazed down on its blue-green crescent, ten
thousand kilometers below Carter-Zimmerman itself. Orpheus was terrestrial,
a nickel-iron-silicate world; slightly larger than Earth, slightly warmer—a
billion kilometers took the edge off Vega's heat—and almost drowning in
liquid water. Impatient to see the whole surface firsthand, Paolo slowed
his clock rate a thousandfold, allowing C-Z to circumnavigate the planet in
twenty subjective seconds, daylight unshrouding a broad new swath with each
pass. Two slender ocher-colored continents with mountainous spines
bracketed hemispheric oceans, and dazzling expanses of pack ice covered
both poles—far more so in the north, where jagged white peninsulas radiated
out from the midwinter arctic darkness.
The Orphean atmosphere was mostly nitrogen—six times as much as on Earth;
probably split by UV from primordial ammonia—with traces of water vapor and
carbon dioxide, but not enough of either for a runaway greenhouse effect.
The high atmospheric pressure meant reduced evaporation—Paolo saw not a
wisp of cloud— and the large, warm oceans in turn helped feed carbon
dioxide back into the crust, locking it up in limestone sediments destined
for subduction.
The whole system was young, by Earth standards, but Vega's greater mass,
and a denser protostellar cloud, would have meant swifter passage through
most of the traumas of birth: nuclear ignition and early luminosity
fluctuations; planetary coalescence and the age of bombardments. The
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