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  2. List of white dwarfs - Wikipedia

    en.wikipedia.org/wiki/List_of_white_dwarfs

    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 [5] [6] First singular white dwarf with a planet WD 1145+017: 2015 WD 1145+017 b: Planet is extremely small and is disintegrating. First white dwarf that is a pulsar: AR Scorpii A ...

  3. White dwarf - Wikipedia

    en.wikipedia.org/wiki/White_dwarf

    Image of Sirius A and Sirius B taken by the Hubble Space Telescope. Sirius B, which is a white dwarf, can be seen as a faint point of light to the lower left of the much brighter Sirius A. A white dwarf is a stellar core remnant composed mostly of electron-degenerate matter. A white dwarf is very dense: its mass is comparable to the Sun 's ...

  4. List of smallest known stars - Wikipedia

    en.wikipedia.org/wiki/List_of_smallest_known_stars

    Part of a symbiotic binary star system containing a red giant and a white dwarf. As in 2019, with mass 67.54±12.79MJ (0.0523-0.0767 M☉) is the lowest known mass hydrogen-burning star. Luhman 16 B and Luhman 16 A are the closest brown dwarf stars to Earth, and the third-nearest star system to the Solar System.

  5. Category:White dwarfs - Wikipedia

    en.wikipedia.org/wiki/Category:White_dwarfs

    Stars by spectral type. Hertzsprung–Russell classifications. White. Hidden categories: Commons category link is on Wikidata. Template Category TOC via Automatic category TOC on category with 101–200 pages. Automatic category TOC generates standard Category TOC.

  6. GRW +70 8247 - Wikipedia

    en.wikipedia.org/wiki/GRW_+70_8247

    GRW +70 8247. GRW +70 8247 is a white dwarf star located 42 light-years from Earth [1] in the constellation Draco. With a magnitude of about 13 it is visible only through a large telescope.

  7. Timeline of white dwarfs, neutron stars, and supernovae

    en.wikipedia.org/wiki/Timeline_of_white_dwarfs...

    1910 – the spectrum of 40 Eridani B is observed, making it the first confirmed white dwarf. 1926 – Ralph Fowler uses Fermi–Dirac statistics to explain white dwarf stars. 1930 – Subrahmanyan Chandrasekhar discovers the white dwarf maximum mass limit. 1933 – Fritz Zwicky and Walter Baade propose the neutron star idea and suggest that ...

  8. Category:Main-sequence stars - Wikipedia

    en.wikipedia.org/wiki/Category:Main-sequence_stars

    Category. : Main-sequence stars. Wikimedia Commons has media related to Main-sequence stars. Main-sequence stars, also called dwarf stars, are stars that fuse hydrogen in their cores. These are dwarfs in that they are smaller than giant stars, but are not necessarily less luminous. For example, a blue O-type dwarf star is brighter than most red ...

  9. List of nearest stars - Wikipedia

    en.wikipedia.org/wiki/List_of_nearest_stars

    Additionally, astronomers have found 6 white dwarfs (stars that have exhausted all fusible hydrogen), 21 brown dwarfs, as well as 1 sub-brown dwarf, WISE 0855−0714 (possibly a rogue planet). The closest system is Alpha Centauri, with Proxima Centauri as the closest star in that system, at 4.2465 light-years from Earth.