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  2. Binary star - Wikipedia

    en.wikipedia.org/wiki/Binary_star

    Binary star. The well-known binary star Sirius, seen here in a Hubble photograph from 2005, with Sirius A in the center, and white dwarf, Sirius B, to the left bottom from it. A binary star or binary star system is a system of two stars that are gravitationally bound to and in orbit around each other. Binary stars in the night sky that are seen ...

  3. Gliese 65 - Wikipedia

    en.wikipedia.org/wiki/Gliese_65

    Gliese 65, also known as Luyten 726-8, is a binary star system that is one of Earth's nearest neighbors, at 8.8 light-years (2.7 parsecs) from Earth in the constellation Cetus. The two component stars are both flare stars with the variable star designations BL Ceti and UV Ceti .

  4. Category:Binary stars - Wikipedia

    en.wikipedia.org/wiki/Category:Binary_stars

    0–9. 1 Arietis. 1 Camelopardalis. 1 Serpentis. 2 Andromedae. 2 Aurigae. 2MASS J11011926−7732383. 2MASS J09393548−2448279. 2MASS J18352154–3123385.

  5. Star polygon - Wikipedia

    en.wikipedia.org/wiki/Star_polygon

    A regular star polygon is a self-intersecting, equilateral, and equiangular polygon. A regular star polygon is denoted by its Schläfli symbol {p / q}, where p (the number of vertices) and q (the density) are relatively prime (they share no factors) and where q ≥ 2. The density of a polygon can also be called its turning number: the sum of ...

  6. Binary system - Wikipedia

    en.wikipedia.org/wiki/Binary_system

    A binary system is a system of two astronomical bodies of the same kind that are comparable in size. Definitions vary, but typically require the center of mass to be located outside of either object. (See animated examples.) The most common kinds of binary system are binary stars and binary asteroids, but brown dwarfs, planets, neutron stars ...

  7. Beta Lyrae - Wikipedia

    en.wikipedia.org/wiki/Beta_Lyrae

    Beta Lyrae Aa is a semidetached binary system made up of a stellar class B6-8 primary star and a secondary that is probably also a B-type star. The fainter, less massive star in the system was once the more massive member of the pair, which caused it to evolve away from the main sequence first and become a giant star.

  8. Stellar designations and names - Wikipedia

    en.wikipedia.org/wiki/Stellar_designations_and_names

    The Bright Star Catalogue, which is a star catalogue listing all stars of apparent magnitude 6.5 or brighter, or roughly every star visible to the naked eye from Earth, contains 9,096 stars. [1] The most voluminous modern catalogues list on the order of a billion stars, out of an estimated total of 200 to 400 billion in the Milky Way .

  9. Visual binary - Wikipedia

    en.wikipedia.org/wiki/Visual_binary

    A visual binary is a gravitationally bound binary star system [1] that can be resolved into two stars. These stars are estimated, via Kepler 's third law, to have periods ranging from a few years to thousands of years. A visual binary consists of two stars, usually of a different brightness. Because of this, the brighter star is called the ...

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