yego.me
💡 Stop wasting time. Read Youtube instead of watch. Download Chrome Extension

The Last Light Before Eternal Darkness – White Dwarfs & Black Dwarfs


4m read
·Nov 2, 2024

Humans can survive in this universe as long as we have an energy source. Unfortunately, the universe will die. It will happen slowly, over many billions of years, but it will happen. On a universal time scale, stars like our sun will be gone in no time.

Luckily, there are places that will exist practically forever from a human perspective: the corpses of dead stars... white dwarfs. They could be humanity's last home right before the death of the universe. What are these strange things and what happens when they finally die? How long stars live varies drastically, depending on how massive they are. For example, really massive stars burn hot and fast, dying violently in supernovae a few million years after birth. But they're the exception.

97% of all stars will end their existence as white dwarfs. There are two ways this can happen: Small stars - so-called red dwarfs - burn out over trillions of years until they eventually quietly turn into white dwarfs. Medium-sized stars like our Sun are more interesting. Imagine the sun as a huge pressure cooker that fuses hydrogen into helium in its core through its gravity. The fusion of elements releases extreme amounts of energy, that pushes outwards and stabilizes the star, keeping it in a delicate balance.

When the Sun is old, the hydrogen in the core is exhausted, and the Sun will begin to burn helium into heavier elements. While doing so, it will shed its outer layers. When this process is over, more than half of the Sun's mass will be lost into space as a spectacular planetary nebula millions of kilometers across. What remains will be its former core: A white dwarf is born, a star corpse. While its former self was about 100 times its diameter, now it's only about as big as Earth, but still with about half of its former mass.

This means it's extremely dense; a teaspoon of white dwarf is about as massive as a car. Its surface gravity is over 100,000 times higher than Earth's. If you tried to land on it, you'd immediately be compressed into a steaming puddle. Life around a white dwarf is very unlikely, but possible. Most of them that exist now were former stars that, well, died, which probably ruined any planets they once had.

But that's not all: since they are so small, a planet would need to orbit them about 75 times closer than Earth is to the Sun to have liquid water. This proximity has up- and downsides: for one, it would tidally lock the planet, giving it a permanent day and permanent night. At the edges of these day and night zones, life could be possible. But white dwarfs have a very stable energy output, so they might actually be safer to live around than many red dwarfs. This is still speculation at this point, but if we could find the white dwarf with the right conditions to settle around, we could have a home for many billions of years.

But why do they shine so much longer than other star types? White dwarfs are very, very hot - up to 40 times hotter than our Sun - ranking among the hottest objects in the universe. But they are not incredibly active. All the heat inside of them is trapped and has nowhere to go. Only on its outer layer can it escape into space. But space is mostly empty, so heat can't be transferred by conduction.

The only way energy can escape is by radiation. This is so inefficient that white dwarfs will take trillions of years to cool down, which may make them humanity's last refuge. They might be the last sources of light and energy in a dying universe. According to some estimates, white dwarfs might shine as long as 100 billion billion years, ten billion times longer than the universe has existed. So far into the future that no regular stars will shine anymore, galaxies will have evaporated, and only then will the first white dwarf turn into the first black dwarf.

When this happens, the last hope for life will die off. Black dwarfs will be inactive spheres with no energy left to give, still massive enough to kill you if you get too close. So cold that they'll be near the coldest possible temperature in the universe, so dark that they are practically invisible.

The universe will enter its last stage - heat death - which will leave the universe unrecognizable, an absolutely dark and cold graveyard, with black holes and black dwarfs scattered over trillions of lightyears. We don't know for sure what will happen with black dwarfs in the end. If the proton - one of the fundamental parts of atoms - has a limited lifespan, black dwarfs will slowly evaporate over many trillions of years. If the proton does not decay, black dwarfs will probably turn into spheres of pure ion via quantum tunneling, over a timespan so obscenely gigantic that calling it forever is okay.

These ion spheres will then travel completely alone through a dark universe. Nothing new will happen anymore... forever. While this may sound kind of dark, this is so far away that for our purposes today, it might as well not happen at all. It doesn't matter what happens in a billion trillion years.

Right now, we happen to exist at an excellent time, able to be in awe about a universe filled with endless stars and light and planets. And enough time to visit them one day. Our music is finally available on Spotify and iTunes. It's composed by our good friends at Epic Mountain, two guys with a studio who make music for a living. You can check them out here, and follow them on Facebook and Twitter. And if you like our videos, please consider supporting us on Patreon. It really would be extremely helpful. If you need an excuse to delay work a little bit longer, here's a playlist with more space videos.

More Articles

View All
Payment methods | Consumer credit | Financial Literacy | Khan Academy
Hi everyone! I’m here, and in this video, we’re going to talk a little bit about how you pay for things. You’re probably already familiar with this, but maybe we’ll get into a little bit more detail than you might have fully realized. So, the most basic …
Impostor Syndrome: What Is Your Worth?
Hi there. We’ve been looking for you. Yes, you. We know everything about you: how you’ve pretended to know things you have no idea about, how you’ve slept through years of your education, how you’ve received awards that you never deserved, and how you’ve …
Geoengineering: A Horrible Idea We Might Have to Do
By the end of the 21st century, humanity is becoming desperate. Decades of heat waves and droughts have led to unusually poor harvests, while the warming oceans yield fewer fish each year in the tropical zones. Millions suffer from famines, and resource w…
Elevator Thought Experiment | Genius
I’d like to continue our work together. So why don’t you come to Prague with me, Jakob? Maybe I could get you a position at the University. We’d have time to work on accelerated motion. Albert, I am flattered. But I’ve received another offer. A [inaudi…
Identifying constant of proportionality graphically
We’re asked what is the constant of proportionality between y and x in the graph. Just as a reminder, when we’re talking about the constant of proportionality, it sounds like a very fancy thing, but it’s not too bad. If we’re thinking about any xy pair o…
YC SUS: Kat Mañalac and Eric Migicovsky discuss Week 2 SUS Lectures
Good morning everyone, and good evening. It could be anywhere actually. I’d like to start somewhere. My name is Eric, and I’m the facilitator, of course, facilitator here at Startup School. It’s a pleasure to be joined by Kat. “Hi everyone, I’m Kat, a pa…