Today's science news involves something called the Chandrasekhar Limit.
Stars live for most of their lives in an equilibrium between two forces; the inward pull of their own gravity, and the outward pressure from the heat generated by fusion in their cores. As long as there is plenty of hydrogen left to power fusion, those forces are equal and opposing, and the star is stable.
When the hydrogen is depleted, though, the balance shifts. The core cools, and the gravitational collapse resumes. This, however, heats things up -- recall the "ideal gas law" from high school chemistry, and that temperature and pressure are inversely proportional -- and the star begins to fuse the helium "ash" left over from hydrogen burning into carbon. Eventually that runs out, too, and the process repeats -- carbon to oxygen and silicon, and on up the scale until finally it gets to iron. At that point, there's nowhere to go; after iron, fusion begins to be an endothermic (energy-requiring) reaction, and the star is pretty much out of gas.
What happens at this point depends on one thing: the star's initial mass. For a star the size of the Sun, the later stages liberate enough energy to balloon the outer atmosphere into a red giant, and when the final collapse happens, it blows off that atmosphere into a wispy bubble called a planetary nebula.
What's left at the center is the exposed core of the star -- a white dwarf, still glowing from its residual heat. It doesn't collapse further because its mass is held up by electron degeneracy pressure -- the resistance of electrons to occupying the same quantum state, something known as the Pauli Exclusion Principle. But it's no longer capable of fusion, so it will simply cool and darken over the next few billion years.
For heavier stars -- between two and ten times the mass of the Sun -- electron degeneracy is not sufficient to halt the collapse. The electrons are forced into the nuclei of the atoms, and what's left is a densely-packed glob of neutrons called, appropriately enough, a neutron star. So much energy is liberated by this process that the result is a supernova; the atmosphere is blown away completely, and the collapsed core, which is made of matter dense enough that a teaspoonful would weigh as much as Mount Everest, spins faster and faster because of the Law of Conservation of Angular Momentum, in some cases reaching speeds of thirty rotations per second. This whirling stellar core is called a pulsar.
For stars even larger than that, though, the pressure of neutron star matter isn't enough to stop the gravitational collapse. In fact, nothing is. The supernova and subsequent collapse lead to the formation of a singularity -- a black hole.
So that's the general scheme of things, but keep in mind that this is the simplest case. Like just about everything in science, reality is more complex.
Suppose you had an ordinary star like the Sun, but it was in a binary system. The Sun-like star reaches the end of its life as a white dwarf, as per the above description. Its partner, though, is still in stable middle age. If it's close enough, the dense, compact white dwarf will begin to funnel material away from its partner, siphoning off the outer atmosphere, and -- this is the significant part -- gaining mass in the process.
The brilliant Indian physicist Subrahmanyan Chandrasekhar figured out that this process can only go on so long -- eventually the white dwarf gains enough mass that its gravity exceeds the outward pressure from electron degeneracy. At a mass of 1.4 times that of the Sun -- the Chandrasekhar Limit -- the threshold is reached, and the result is a sudden and extremely violent collapse and explosion called a type 1a supernova. This is one of the most energetic events known -- in a few seconds, it liberates 10^44 Joules of energy (that's 1, followed by 44 zeroes).
So this is why I got kind of excited when I read a paper in Nature Astronomy about a binary star system only 150 light years away made of two white dwarf stars, which are spiraling inward and will eventually collide.
Because that would be the type 1a supernova to end all type 1a supernovas, wouldn't it? No gradual addition of little bits of mass at a time until you pass the Chandrasekhar Limit; just a horrific, violent collision. And 150 light years is close enough that it will be a hell of a fireworks show. Estimates are that it will be ten times brighter than the full Moon. But at that distance, it won't endanger life on Earth, so it'll be the ideal situation -- a safe, but spectacular, event.
The two stars are currently orbiting their common center of mass at a distance of about one-sixtieth of that between the Earth and the Sun, completing an orbit every fourteen hours. Immediately before collision, that orbital period will have dropped to the frantic pace of one revolution every thirty seconds. After that...
... BOOM.
But this was the point where I started thinking, "Hang on a moment." Conservation of energy laws suggest that to go from a fourteen-hour orbit with a radius of around 2.5 million kilometers, to a thirty-second orbit with a radius of close to zero, would require an enormous loss of energy from the system. That kind of energy loss doesn't happen quickly. So how long will this process take?
And there, in the paper, I found it.
This spectacular supernova isn't going to happen for another 23 billion years.
This was my expression upon reading this:
I don't know about you, but even in my most optimistic moments I don't think I'm going to live for another 23 billion years. So this whole thing gives new meaning to the phrase "advance notice."
You know, I really think y'all astrophysicists need to step up your game, here. You get our hopes up, and then say, "Well, of course, you know, astronomical time scales..." Hell, I've been waiting for Betelgeuse to blow up since I was like fifteen years old. Isn't fifty years astronomical enough for you?
And now, I find out that this amazing new discovery of two madly-whirling white dwarf stars on an unavoidable collision course is going to take even longer. To which I say: phooey.
I know your priority isn't to entertain laypeople, but c'mon, have a heart. Down here all we have to keep our attention is the ongoing fall of civilization, and that only gets you so far. Back in the day, stuff like comets and supernovas and whatnot were considered signs and portents, and were a wonderful diversion from our ancestors' other occupations, such as starving, dying of the plague, and being tortured to death by the Inquisition. Don't you think we deserve a reason to look up, too? In every sense of the phrase?
So let's get a move on, astrophysicists. Find us some imminent stellar hijinks to watch. I'll allow for some time in the next few months. A year at most. I think that's quite generous, really.
And if you come up with something good, I might even forgive you for getting my hopes up about something amazing that won't happen for another 23 billion years.