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  2. White dwarf - Wikipedia

    en.wikipedia.org/wiki/White_dwarf

    A search has been proposed for transits of hypothetical Earth-like planets around white dwarfs with surface temperatures of less than 10 000 K. Such stars that could harbor a habitable zone at a distance of c. 0.005 to 0.02 AU that would last upwards of 3 billion years. This is so close that any habitable planets would be tidally locked.

  3. List of white dwarfs - Wikipedia

    en.wikipedia.org/wiki/List_of_white_dwarfs

    First double white dwarf system LDS 275: 1944 L 462-56 system [4] First solitary white dwarf Van Maanen 2: 1917 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]

  4. White dwarf cooling anomaly - Wikipedia

    en.wikipedia.org/wiki/White_dwarf_cooling_anomaly

    Gaia-based HR diagram of white dwarfs showing three branch-like groupings. In 2018, the second release of data from the Gaia astrometric space mission was made available to astronomers, providing precise location and photometric data for around 260,000 candidate white dwarfs. For the first time, this information provided data on the fundamental ...

  5. Hertzsprung–Russell diagram - Wikipedia

    en.wikipedia.org/wiki/Hertzsprung–Russell_diagram

    Two main concentrations appear in this diagram following the cooling sequence of white dwarfs that are explained with the atmospheric composition of white dwarfs, especially hydrogen versus helium dominated atmospheres of white dwarfs. [12] A third concentration is explained with core crystallization of the white dwarfs interior.

  6. van Maanen 2 - Wikipedia

    en.wikipedia.org/wiki/Van_Maanen_2

    Like other white dwarfs, it is a very dense star: its mass has been estimated to be about 67% of the Sun's, [28] yet it has only 1% of the Sun's radius (1.23 times the Earth's radius). [7] [a] The outer atmosphere has a temperature of approximately 6,110 K, [28] which is relatively cool for a white dwarf. As all white dwarfs steadily radiate ...

  7. 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.

  8. Dwarf planet - Wikipedia

    en.wikipedia.org/wiki/Dwarf_planet

    A dwarf planet is a small planetary-mass object ... Euler diagram showing the IAU Executive Committee ... Planetary discriminants of the planets ( white ...

  9. Compact object - Wikipedia

    en.wikipedia.org/wiki/Compact_object

    The Eskimo Nebula is illuminated by a white dwarf at its center. The stars called white or degenerate dwarfs are made up mainly of degenerate matter; typically carbon and oxygen nuclei in a sea of degenerate electrons. White dwarfs arise from the cores of main-sequence stars and are therefore very hot when