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  1. en.wikipedia.org › wiki › White_dwarfWhite dwarf - Wikipedia

    In 1917, Adriaan van Maanen discovered van Maanen's Star, an isolated white dwarf. These three white dwarfs, the first discovered, are the so-called classical white dwarfs.

  2. Jun 14, 2024 · White dwarf star, any of a class of faint stars representing the endpoint of the evolution of intermediate- and low-mass stars. White dwarf stars are characterized by a low luminosity, a mass on the order of that of the Sun, and a radius comparable to that of Earth.

  3. Apr 25, 2023 · White dwarfs are the hot, dense remnants of long-dead stars. They are stellar cores, left behind when stars exhaust their fuel supplies and blow their gases into space.

  4. Mar 4, 2022 · White dwarfs are what is left when stars like our sun have exhausted all of their fuel. They are dense, dim, stellar corpses — the last observable stage of evolution for low- and medium-mass...

  5. Ancient white dwarf stars shine in the Milky Way galaxy. Stars like our sun fuse hydrogen in their cores into helium. White dwarfs are stars that have burned up all of the hydrogen they...

  6. Jun 12, 2020 · A white dwarf star, also called a degenerate dwarf, is a stellar core remnant composed mostly out of electron-degenerate matter. A white dwarf is quite dense, its mass may be comparable to that of the Sun, while its volume could be comparable to that of Earth.

  7. www.nasa.gov › universe › starsWhite Dwarfs - NASA

    Learn about the fascinating properties and evolution of white dwarfs, the final stage of most stars in the universe, from NASA experts.

  8. imagine.gsfc.nasa.gov › science › objectsImagine the Universe!

    Sep 23, 2021 · White Dwarf Stars. A white dwarf is what stars like the Sun become after they have exhausted their nuclear fuel. Near the end of its nuclear burning stage, this type of star expels most of its outer material, creating a planetary nebula. Only the hot core of the star remains.

  9. www.nasa.gov › image-article › white-dwarf-starsWhite Dwarf Stars - NASA

    Mar 23, 2008 · Pushing the limits of its powerful vision, NASA’s Hubble Space Telescope uncovered the oldest burned-out stars in our Milky Way Galaxy. These extremely old, dim “clockwork stars” provide a completely independent reading on the age of the universe. The ancient white dwarf stars, as seen by Hubble, are 12-13 billion years old.

  10. Sep 6, 2021 · New evidence from NASA's Hubble Space Telescope suggests that white dwarf stars could continue to burn hydrogen in the final stages of their lives, causing them to appear more youthful than they actually are.

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