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  2. White dwarf - Wikipedia

    en.wikipedia.org/wiki/White_dwarf

    It is thought that, over a lifespan that considerably exceeds the age of the universe (c. 13.8 billion years), [129] such a star will eventually burn all its hydrogen, for a while becoming a blue dwarf, and end its evolution as a helium white dwarf composed chiefly of helium-4 nuclei. [130]

  3. Stellar evolution - Wikipedia

    en.wikipedia.org/wiki/Stellar_evolution

    For a star of 1 M ☉, the resulting white dwarf is of about 0.6 M ☉, compressed into approximately the volume of the Earth. White dwarfs are stable because the inward pull of gravity is balanced by the degeneracy pressure of the star's electrons, a consequence of the Pauli exclusion principle. Electron degeneracy pressure provides a rather ...

  4. List of white dwarfs - Wikipedia

    en.wikipedia.org/wiki/List_of_white_dwarfs

    Van Maanen's star is also the nearest solitary white dwarf [5] First white dwarf with a planet WD B1620−26: 2003 PSR B1620-26 b (planet) This planet is a circumbinary planet, which circles both stars in the PSR B1620-26 system [6] [7] First singular white dwarf with a transiting object WD 1145+017: 2015 Known object is a disintegrating ...

  5. Astronomers observe scar on white dwarf 'cannibal' star - AOL

    www.aol.com/news/astronomers-observe-scar-white...

    This white dwarf started its life as a star about twice the sun's mass, living a lifespan of perhaps 1.2 billion years before entering its death throes. Many white dwarfs have a debris disk ...

  6. van Maanen 2 - Wikipedia

    en.wikipedia.org/wiki/Van_Maanen_2

    Van Maanen 2, or van Maanen's Star, is the closest known solitary white dwarf to the Solar System. It is a dense, compact stellar remnant no longer generating energy and has equivalent to about 68% of the Sun's mass but only 1% of its radius. [ 9 ]

  7. Straight out of 'Star Wars,' NASA discovers a real 'death ...

    www.aol.com/article/2015/10/22/straight-out-of...

    The star is ending its life by casting off its outer layers of gas, which formed a cocoon around the star's remaining core. Ultr. What exactly is a white dwarf star, you ask?

  8. K-type main-sequence star - Wikipedia

    en.wikipedia.org/wiki/K-type_main-sequence_star

    A K-type main-sequence star, also referred to as a K-type dwarf, or orange dwarf, is a main-sequence (hydrogen-burning) star of spectral type K and luminosity class V. These stars are intermediate in size between red M-type main-sequence stars ("red dwarfs") and yellow/white G-type main-sequence stars.

  9. Intrepid white dwarf has a close encounter with a massive ...

    www.aol.com/news/intrepid-white-dwarf-close...

    Scientists have detected emanating from the nucleus of a galaxy relatively close to our Milky Way flashes of X-rays gradually increasing in frequency that seem to be coming from a white dwarf - a ...