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  2. 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− ...

  3. White dwarf - Wikipedia

    en.wikipedia.org/wiki/White_dwarf

    The metal-rich white dwarf WD 1145+017 is the first white dwarf observed with a disintegrating minor planet that transits the star. [ 176 ] [ 177 ] The disintegration of the planetesimal generates a debris cloud that passes in front of the star every 4.5 hours, causing a 5-minute-long fade in the star's optical brightness. [ 177 ]

  4. 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.

  5. A-type main-sequence star - Wikipedia

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

    The revised Yerkes Atlas system [7] listed a dense grid of A-type dwarf spectral standard stars, but not all of these have survived to this day as standards. The "anchor points" and "dagger standards" of the MK spectral classification system among the A-type main-sequence dwarf stars, i.e. those standard stars that have remained unchanged over years and can be considered to define the system ...

  6. 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.

  7. van Maanen 2 - Wikipedia

    en.wikipedia.org/wiki/Van_Maanen_2

    At a distance of 14.1 light-years it is the third closest of its type of star after Sirius B and Procyon B, in that order. [10] [11] Discovered in 1917 by Dutch–American astronomer Adriaan van Maanen, [12] Van Maanen 2 was the third white dwarf identified, after 40 Eridani B and Sirius B, and the first solitary example. [13]

  8. Alexandria Ocasio-Cortez announces bid to become top Democrat ...

    www.aol.com/news/aoc-run-top-democrat-oversight...

    Rep. Alexandria Ocasio-Cortez announced on Friday that she is jumping into the race to be the top Democrat on the influential House Oversight Committee.

  9. Canis Major - Wikipedia

    en.wikipedia.org/wiki/Canis_Major

    Its name comes from the Greek word for "scorching" or "searing". Sirius is also a binary star; its companion Sirius B is a white dwarf with a magnitude of 8.4–10,000 times fainter than Sirius A to observers on Earth. [32] The two orbit each other every 50 years. Their closest approach last occurred in 1993 and they will be at their greatest ...