‘We think the impact actually
created -
or at any rate widened - more, branching wormholes, which carried the
Crab
further into the future. Perhaps much further.
‘We have simulations which show how this could happen, given the right form of hyperdrive physics - particularly if there were other cross-time wormholes already extant in the Solar System of the occupation era - perhaps set up by the Qax. In fact, the assumption that the branching
did
occur is allowing us to rule out classes of hyperdrive theory . . .’
The Virtual stood, and paced slowly across the transparent floor. ‘I was determined to close off the time bridge - to remove the threat of invasions from the future. But - I have to tell you - Paradoxa thinks this was a mistake.’ The Virtual twisted his hands together. ‘After all, we had already beaten off one Spline incursion. After Poole’s departure the study of the Qax incident became the prime focus of Paradoxa. But because the wormhole is closed, Paradoxa is reduced to
inferring
the truth about the future of our species from fragments, from indirect shards of evidence . . .’
Louise said, ‘You don’t believe it was a mistake, Michael.’
Poole looked haunted; again, Louise realized with an inner ache, his personality was conflicting with the programming imposed on it by Paradoxa.
Mark peered up at the dying stars. ‘So. Did Poole survive?’
Louise said, ‘I’d like to think he did. Even just for a short while, so that he could understand what he saw.’
Milpitas lay back in her couch and stared up at the scattering of dim, reddened stars. ‘I’m no cosmologist . . . but those stars look so
old
. How far in time did he come?’
The Virtual did not reply.
Uvarov said, ‘Why have you shown us all this? What do you want?’
Virtual-Poole raised his thin arms to the desolate sky. ‘Look around you, Uvarov. Perhaps this is the end of time; it is certainly the end of the stars, of baryonic life. Perhaps there are other life forms out there, not perceived by us - creatures of dark matter, the non-baryonic stuff which makes up nine-tenths of the Universe. But -
where is man?
In fact there’s no evidence of life at all here, human or otherwise.
‘Paradoxa has pieced together some fragments of the history of the future, from the rubble the
Crab
left behind. We know about the Xeelee, for example. We even know - we think - the name of the Xeelee’s greatest project: the
Ring
. But -
what happens to us?
What happens to the human species? What destroys us, even as it extinguishes the stars?
‘And - Paradoxa asks - is there anything we can do to avert this, the final catastrophe?’
Louise looked up at the dying stars. ‘Ah. I think I understand why I’m here. Paradoxa wants me to follow the
Hermit Crab
. To take the
Great Northern
- not to Tau Ceti - but on a circular trip, like Poole’s
Cauchy
, to establish a time bridge. Paradoxa wants to set up a way - a stable way - of reaching
this
era: the end of time.
‘I get it. We’ve long since taken responsibility for the management of our planets - for the survival of their ecologies. Why, now, should we not take responsibility for our own long term survival as a species?’ She felt like laughing. ‘Paradoxa really does think big, doesn’t it?’
Milpitas sat on the edge of her couch. ‘But what does
survival
mean, on such timescales? Surely even with AS treatments, survival of individuals - of us - into the indefinite future is impossible. What, then? Survival of the genotype? Or of the culture of our species - the memes, the cultural elements, perhaps, preserved in some form—’
Uvarov looked fascinated now, Louise thought; all his impatience and irritability gone, he stared up at the Virtual rendition of the future hungrily. ‘Either, or both, perhaps. Speaking as a flesh-and-blood human, I share a natural human bias to the survival of the actual genotype in some form. The preservation of mere information appears a sterile option to me.
‘But, whatever survival means,
it doesn’t matter
. Look beyond the dome. In this time to which Michael Poole travelled,
nothing
of us has survived,
in any form
. And
that’s
the catastrophe Paradoxa is determined - clearly - we must work to avert.’
Louise pulled her lip. ‘If this is such a compelling case, why is Paradoxa a small, covert operation? Why shouldn’t Paradoxa’s goals motivate the primary activity of the race?’
Poole sighed. ‘Because the case
isn’t
so compelling. Obviously. Louise, as a species we aren’t used to thinking on such timescales. Not yet. There is talk of hubris: of comparisons with the Friends of Wigner, who came back through time - evidently - to manipulate history, to avert the Qax occupation.’ He looked at Louise wearily. ‘There isn’t even agreement about what you’re seeing here. I’ve shown you just one scenario, reconstructed from the Interface incident evidence. Maybe, it’s argued, we’re addressing problems that don’t really exist.’
Louise folded her arms. ‘And what if that’s true?’
Uvarov said, ‘But if there’s even the smallest chance that this interpretation is correct - then isn’t it worth some investment, against the possibility?’
Mark frowned. ‘So we use the
Northern
to fly to the future. The flight to Tau Ceti is only supposed to take a century.’
Poole nodded. ‘With modern technology, the flight of the
Northern
into the future should last no more than a thousand subjective years—’
Mark laughed. ‘Poole, that’s impossible. No ship could last that long, physically. No closed ecology could survive. A closed society would tear itself apart . . . We don’t even know if AS treatment can keep humans alive over such periods.’
Louise stared up at the simulated stars.
A thousand years?
Mark was right; it was inhumanly long - but she had the feeling
it wasn’t long enough . . .
Uvarov nodded. ‘But that is clearly why you have been chosen: Louise, the best engineer of the day,
and
with will enough to sustain immense projects. You, Mark Wu, a good social engineer—’
‘There are better ones,’ Mark said.
‘Not married to Louise.’
‘Formerly married.’
Poole turned to Milpitas. ‘The proposal is that you, Serena, will make the
Great Northern
herself viable for its unprecedented thousand-year flight. And you, Dr Uvarov, have a deep understanding of the strengths and limitations of the engineering of the
human
form; you will help Mark Wu keep the people - the species - alive.’
Louise saw Uvarov’s eyes gleam.
‘I’ve no intention of going on this flight,’ Mark said. ‘And besides, the
Northern
already has a ship’s engineer. And a damn doctor, come to that.’
Poole smiled. ‘Not for this mission.’
‘Hold it,’ Louise said. ‘There’s something missing.’ She thought over what she had to say: relativistic math, done in the head, was chancy. But still . . . ‘Poole, a thousand-year trip can’t be long enough.’ She looked up at the decaying stars. ‘I’m no cosmologist. But I see no Main Sequence stars up there at all. I’d guess we’re looking at a sky from far into the future - tens of billions of years, at least.’
Poole shook his head. His Virtual face was difficult to see in the faded starlight. ‘No, Louise. You’re wrong. A thousand-subjective-year trip is quite sufficient.’
‘How can it be?’
‘Because the sky you’re seeing isn’t from tens of billions of years hence. It’s from
five million years
ahead. That’s all - five megayears,
nothing
in cosmological time . . .’
‘But how—’
‘More than time will ruin the stars, Louise. If this reconstruction is anything like accurate, there’s an agency at large - which must be acting
even now -
systematically destroying the stars . . .
‘And, as a consequence, us.’
Uvarov turned his face, expressionless, up to the darkling sky.
Virtual-Poole said, ‘We have reason to believe that even our own Sun is subject to this mysterious assault.’ He stood before Louise. ‘Look, Louise, you know I don’t advocate cosmic engineering - I was the one who opposed the Friends of Wigner, who did my damnedest to close my own bridge to the future.
But this is different
. Even I can sympathize with what Paradoxa is attempting here.
Now
can you see why they want you to follow the
Crab
?’
The light show began to fade from the dome; evidently the display was over.
Poole still stood before Louise, but his definition was fading, his outlines growing blocky in clouds of pixels. She reached out a hand to him, but his face had already grown smooth, empty; long before the final pixels of his image dispersed, she realized, all trace of consciousness had fled.
Lieserl soared through her convective cavern, letting her sensory range expand and contract, almost at random.
She thought about the Sun.
For all its grandeur, the Sun, as a machine, was simple. When she looked down and
opened
her eyes she could see evidence of the fusing core, a glow of neutrino light beneath the radiative plasma ocean. If that core were ever extinguished, then the flood of energetic photons out of the core and into the radiative and convective layers would be staunched. The Sun was in hydrostatic equilibrium - the radiation pressure from the photons balanced the Sun’s tendency to collapse inwards, under gravity. And if the radiation pressure were removed the outer layers would implode, falling freely, within a few hours.
The Sun hadn’t always been as stable as this . . . and it wouldn’t always remain so.
The Sun had formed from a contracting cloud of gas - a
protostar
. At first the soft-edged, amorphous body had shone by the conversion of its gravitational energy alone.
When the central temperature had reached ten million degrees, hydrogen fusion had begun in the core.
The shrinkage had been halted, and stability reached rapidly. The fusion was restricted to an inner core, surrounded by the plasma sea and the convective ‘atmosphere’. The Sun, stable, burning tranquilly, had become a
Main Sequence
star; by the time Lieserl entered the convective zone, the Sun had burned for five billion years.
But the Sun would not remain on the Main Sequence forever.
The mass converted to energy was millions of tons per second. The Sun’s bulk was so huge that this was a tiny fraction; in all its five-billion-year history so far the Sun had burned only five per cent of its hydrogen fuel . . .
But, relentlessly, the fuel in the core would be exhausted. Gradually an ash of helium would accumulate in the core, and the central temperature would drop. The delicate balance between gravity and radiation pressure would be lost, and the core would implode under the weight of the surrounding, cooler layers.
Paradoxically, the implosion would cause the core temperature to
rise
once more - so much so that new fusion processes would become possible - and the star’s overall energy output would rise.
The outer layers would expand enormously, driven out by the new-burning core. The Sun would engulf Mercury, and perhaps more of the inner planets, before reaching a new gravity-pressure equilibrium - as a
red giant
. This hundred-million-year phase would be spectacular, with the Sun’s luminosity increasing by a factor of a thousand.
But this profligate expansion was not sustainable. Complex elements would be burned with increasing desperation in the expanding, clinker-ridden core, until at last all the available fuel was exhausted.
As the core’s temperature suddenly fell, equilibrium would be lost with sudden abandon. The Sun would implode once more, seeking a new stability. Finally, as a
white dwarf
, the Sun would consist of little more than its own dead core, its density a million times higher than before, with further contraction opposed by the pressure of high-speed electrons in its interior.
Slowly, the remnant would cool, at last becoming a
black dwarf
, surrounded - as if by betrayed children - by the charred husks of its planets.
. . . At least, Lieserl thought, that was the theory.
If the laws of physics were allowed to unravel, following their own logic unimpeded, the Sun’s red giant stage was still billions of years away . . . not mere
millions
of years, as Paradoxa’s evidence suggested was the case.
Lieserl’s brief was to find out what was damaging the Sun.
Lieserl. Try to pick up the p-modes; we want to see if that sensory mechanism works . . .
‘Absolutely. Helioseismology, here I come,’ she said flippantly.
She
opened
her eyes once more.
A new pattern was built up by her processors, a fresh overlay on top of the images of convective cells and tangled flux tubes: gradually, she made out a structure of ghostly-blue walls and spinning planes that propagated through the convective cavern. These were
p-modes:
sound waves, pressure pulses fleeing through the Solar gas from explosive events like the destruction of granules on the surface. The waves were trapped in the convective layer, reflected from the vacuum beyond the photosphere and bent away from the core by the increasing sound speed in the interior. The waves cancelled and reinforced each other until only standing waves survived, modes of vibration which matched the geometry of the convective cavern.
The modes filled the space around her with ghostly, spinning patterns; their character varied as she surveyed the depth of the cavern, with length scales increasing as she looked into the interior. Looking up with her enhanced vision Lieserl could see how patches - thousands of miles wide - of the Sun’s surface
oscillated
as the waves struck, with displacements of fifty miles and speeds of half a mile a second.