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  2. White dwarf - Wikipedia

    en.wikipedia.org/wiki/White_dwarf

    The first white dwarf discovered was in the triple star system of 40 Eridani, which contains the relatively bright main sequence star 40 Eridani A, orbited at a distance by the closer binary system of the white dwarf 40 Eridani B and the main sequence red dwarf 40 Eridani C.

  3. 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 ...

  4. 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 ]

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

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

    A light-year is the distance light travels in a year, 5.9 trillion miles (9.5 trillion km). ... eventually leaving behind a compact core roughly the diameter of Earth - the white dwarf. This one ...

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

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

    A light year is the distance light travels in a year, 5.9 trillion miles (9.5 trillion km). Like all white dwarfs, it is incredibly dense, packing about 70% of the sun's mass into an Earth-sized ...

  7. Sirius - Wikipedia

    en.wikipedia.org/wiki/Sirius

    Sirius is a binary star system consisting of two white stars orbiting each other with a separation of about 20 AU [e] (roughly the distance between the Sun and Uranus) and a period of 50.1 years. The brighter component, termed Sirius A, is a main-sequence star of spectral type early A , with an estimated surface temperature of 9,940 K . [ 14 ]

  8. BPM 37093 - Wikipedia

    en.wikipedia.org/wiki/BPM_37093

    BPM 37093 (V886 Centauri) is a variable white dwarf star of the DAV, or ZZ Ceti, type, with a hydrogen atmosphere and an unusually high mass of approximately 1.1 times the Sun's. It is 48 light-years (15 parsecs) from Earth in the constellation Centaurus and vibrates; these pulsations cause its luminosity to vary.

  9. LP 658-2 - Wikipedia

    en.wikipedia.org/wiki/LP_658-2

    LP 658-2 is a degenerate (white dwarf) star in the constellation of Orion, [3] the single known object in its system. It has an apparent visual magnitude of approximately 14.488. [ 2 ]

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