A Googol Years From Now

If humanity makes it the next few years and decades without destroying itself and the planet, we can ponder the broader fate of our universal home. Assuming humanity escapes the death of our beautiful local star (in 4-5 billion years or so) and the merging of our very own Milky Way and the Andromeda galaxy (around 7-10 billion years), we’ll be toast in a googol years. Actually, we and everything else in the cosmos will be more like a cold, dark particle soup. By the way, a googol is a rather large number — 10100. That gives us plenty of time to fix ourselves.

From Space:

Yes, the universe is dying. Get over it.

 Well, let’s back up. The universe, as defined as “everything there is, in total summation,” isn’t going anywhere anytime soon. Or ever. If the universe changes into something else far into the future, well then, that’s just more universe, isn’t it?

But all the stuff in the universe? That’s a different story. When we’re talking all that stuff, then yes, everything in the universe is dying, one miserable day at a time.

You may not realize it by looking at the night sky, but the ultimate darkness is already settling in. Stars first appeared on the cosmic stage rather early — more than 13 billion years ago; just a few hundred million years into this Great Play. But there’s only so much stuff in the universe, and only so many opportunities to make balls of it dense enough to ignite nuclear fusion, creating the stars that fight against the relentless night.

The expansion of the universe dilutes everything in it, meaning there are fewer and fewer chances to make the nuclear magic happen. And around 10 billion years ago, the expansion reached a tipping point. The matter in the cosmos was spread too thin. The engines of creation shut off. The curtain was called: the epoch of peak star formation has already passed, and we are currently living in the wind-down stage. Stars are still born all the time, but the birth rate is dropping.

At the same time, that dastardly dark energy is causing the expansion of the universe to accelerate, ripping galaxies away from each other faster than the speed of light (go ahead, say that this violates some law of physics, I dare you), drawing them out of the range of any possible contact — and eventually, visibility — with their neighbors. With the exception of the Andromeda Galaxy and a few pathetic hangers-on, no other galaxies will be visible. We’ll become very lonely in our observable patch of the universe.

The infant universe was a creature of heat and light, but the cosmos of the ancient future will be a dim, cold animal.

The only consolation is the time scale involved. You thought 14 billion years was a long time? The numbers I’m going to present are ridiculous, even with exponential notation. You can’t wrap your head around it. They’re just … big.

For starters, we have at least 2 trillion years until the last sun is born, but the smallest stars will continue to burn slow and steady for another 100 trillion years in a cosmic Children of Men. Our own sun will be long gone by then, heaving off its atmosphere within the next 5 billion years and charcoaling the Earth. Around the same time, the Milky Way and Andromeda galaxies will collide, making a sorry mess of the local system.

At the end of this 100-trillion-year “stelliferous” era, the universe will only be left with the … well, leftovers: white dwarves (some cooled to black dwarves), neutron stars and black holes. Lots of black holes.

Welcome to the Degenerate Era, a state that is as sad as it sounds. But even that isn’t the end game. Oh no, it gets worse. After countless gravitational interactions, planets will get ejected from their decaying systems and galaxies themselves will dissolve. Losing cohesion, our local patch of the universe will be a disheveled wreck of a place, with dim, dead stars scattered about randomly and black holes haunting the depths.

The early universe was a very strange place, and the late universe will be equally bizarre. Given enough time, things that seem impossible become commonplace, and objects that appear immutable … uh, mutate. Through a process called quantum tunneling, any solid object will slowly “leak” atoms, dissolving. Because of this, gone will be the white dwarves, the planets, the asteroids, the solid.

Even fundamental particles are not immune: given 10^34 years, the neutrons in neutron stars will break apart into their constituent particles. We don’t yet know if the proton is stable, but if it isn’t, it’s only got 10^40 years before it meets its end.

With enough time (and trust me, we’ve got plenty of time), the universe will consist of nothing but light particles (electrons, neutrinos and their ilk), photons and black holes. The black holes themselves will probably dissolve via Hawking Radiation, briefly illuminating the impenetrable darkness as they decay.

After 10^100 years (but who’s keeping track at this point?), nothing macroscopic remains. Just a weak soup of particles and photons, spread so thin that they hardly ever interact.

Read the entire article here.

In case, you’ve forgotten, a googol is 10100 (10 to the power of 100) or 10 followed by 100 zeros. And, yes, that’s how the company Google derived its name.