When.com Web Search

Search results

  1. Results From The WOW.Com Content Network
  2. Binary star - Wikipedia

    en.wikipedia.org/wiki/Binary_star

    An eclipsing binary star is a binary star system in which the orbital plane of the two stars lies so nearly in the line of sight of the observer that the components undergo mutual eclipses. [20] In the case where the binary is also a spectroscopic binary and the parallax of the system is known, the binary is quite valuable for stellar analysis.

  3. LL Aquarii - Wikipedia

    en.wikipedia.org/wiki/LL_Aquarii

    LL Aquarii is an eclipsing binary star system in the equatorial constellation of Aquarius, abbreviated LL Aqr.At peak brightness it has a combined apparent visual magnitude of 9.23, [1] which is too dim to be visible to the naked eye.

  4. Algol variable - Wikipedia

    en.wikipedia.org/wiki/Algol_variable

    Algol variables or Algol-type binaries are a class of eclipsing binary stars that are similar to the prototype member of this class, β Persei (Beta Persei, Algol). An Algol binary is a system where both stars are near-spherical such that the timing of the start and end of the eclipses is well-defined.

  5. List of variable stars - Wikipedia

    en.wikipedia.org/wiki/List_of_variable_stars

    The following is a list of variable stars that are well-known, ... Eclipsing binary Algol type (EA/GS) R Aur: Auriga 6 m.7 13 m.9 7.2: 458 d Mira variable (M)

  6. Contact binary - Wikipedia

    en.wikipedia.org/wiki/Contact_binary

    In astronomy, a contact binary is a binary star system whose component stars are so close that they touch each other or have merged to share their gaseous envelopes. A binary system whose stars share an envelope may also be called an overcontact binary. [1] [2] The term "contact binary" was introduced by astronomer Gerard Kuiper in 1941. [3]

  7. Alpha Coronae Borealis - Wikipedia

    en.wikipedia.org/wiki/Alpha_Coronae_Borealis

    Alpha Coronae Borealis is a binary system, its stars orbiting each other in an eccentric orbit every 17.36 days. Because the plane of this orbit is inclined at an angle of 88.2° to the line of sight to the Earth, [8] the pair form a detached eclipsing binary system similar to Algol (β Per). The periodic eclipses result in a magnitude ...

  8. BX Trianguli - Wikipedia

    en.wikipedia.org/wiki/BX_Trianguli

    This is an eclipsing binary variable, first identified by the Northern Sky Variability Survey survey in 2004 [4] and given its variable-star designation BX Trianguli in 2010. Both stars in the system eclipse each other as seen from Earth, causing the brightness of the system to drop from a magnitude of 12.35 to 12.6/12.7 on the secondary ...

  9. Category:Eclipsing binaries - Wikipedia

    en.wikipedia.org/wiki/Category:Eclipsing_binaries

    Main page; Contents; Current events; Random article; About Wikipedia; Contact us