White dwarf
Adapted from Wikipedia · Explorer experience
White Dwarfs
A white dwarf is a small, very dense star. Imagine a star that could fit inside a space about the size of the Earth, but it holds as much mass as our Sun! These stars are like tiny, strong lights in the sky.
Many stars, including ones like our Sun, will become white dwarfs after they run out of fuel. They cannot turn into denser objects like a neutron star or a black hole because they do not have enough mass. The closest known white dwarf to us is Sirius B, which is part of the bright binary star system called Sirius.
White dwarfs are made of a special kind of matter. Once they form, they stop all reactions that make stars shine and stay standing because of something called electron pressure. This makes them extremely dense. Even though they start very hot, white dwarfs cool down slowly over a very long time, sending their energy out into space.
Scientists have found many white dwarfs close to our solar system. Studying them helps us learn more about these interesting objects and how stars change over time. White dwarfs remind us that even after stars stop shining, they still have a lot to teach us about the universe.
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