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  2. White dwarf - Wikipedia

    en.wikipedia.org/wiki/White_dwarf

    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: in an Earth sized volume, it packs a mass that is comparable to the Sun.

  3. Alvan Graham Clark - Wikipedia

    en.wikipedia.org/wiki/Alvan_Graham_Clark

    Alvan Graham Clark was born in Fall River, Massachusetts, the son of Alvan Clark, founder of Alvan Clark & Sons. [1]On January 31, 1862, while testing a new 18.5-inch (470 mm) aperture great refractor telescope in Cambridgeport, Massachusetts, Clark made the first ever observation of a white dwarf star.

  4. List of white dwarfs - Wikipedia

    en.wikipedia.org/wiki/List_of_white_dwarfs

    Sirius B: 1852 Sirius system Sirius B is also the nearest white dwarf (as of 2005) [2] [3] First found in a binary star system 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− ...

  5. Sirius - Wikipedia

    en.wikipedia.org/wiki/Sirius

    Sirius is a binary star consisting of a main-sequence star of spectral type A0 or A1, termed Sirius A, and a faint white dwarf companion of spectral type DA2, termed Sirius B. The distance between the two varies between 8.2 and 31.5 astronomical units as they orbit every 50 years.

  6. List of exoplanets and planetary debris around white dwarfs

    en.wikipedia.org/wiki/List_of_exoplanets_and...

    About 6% of white dwarfs show infrared excess due to a disk around a white dwarf. [66] In the past only a relative small sample of white dwarf disks was known. [ 67 ] Due to advances in white dwarf detection (e.g. with Gaia or LAMOST ) and improvement of WISE infrared catalogs with unWISE/CatWISE, the number has increased to hundreds of candidates.

  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. 1914 – Walter Sydney Adams determines an incredibly high density for Sirius B. 1926 – Ralph Fowler uses Fermi–Dirac statistics to explain white dwarf stars. 1930 – Subrahmanyan Chandrasekhar discovers the white dwarf maximum mass limit.

  8. Category:White dwarfs - Wikipedia

    en.wikipedia.org/wiki/Category:White_dwarfs

    Download as PDF; Printable version; ... White dwarf star stubs (24 P) Pages in category "White dwarfs" ... Sirius; Stein 2051; SU Ursae Majoris;

  9. Canis Major - Wikipedia

    en.wikipedia.org/wiki/Canis_Major

    Sirius was the basis for the ancient Egyptian calendar. [6] The star marked the Great Dog's mouth on Bayer's star atlas. [33] Flanking Sirius are Beta and Gamma Canis Majoris. Also called Mirzam or Murzim, Beta is a blue-white Beta Cephei variable star of magnitude 2.0, which varies by a few hundredths of a magnitude over a period of six hours ...