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  2. Star system - Wikipedia

    en.wikipedia.org/wiki/Star_system

    A multiple star system consists of two or more stars that appear from Earth to be close to one another in the sky. [dubious – discuss] This may result from the stars actually being physically close and gravitationally bound to each other, in which case it is a physical multiple star, or this closeness may be merely apparent, in which case it is an optical multiple star [a] Physical multiple ...

  3. Circumtriple planet - Wikipedia

    en.wikipedia.org/wiki/Circumtriple_planet

    A circumtriple planet is a celestial mass that is hypothesized to be orbiting not only a single star but three stars at the same time. [1] Scientists observing the star system GW Ori , which is a huge disk of dust and gases about 1,300 light years away from Earth, suspect that there may be a circumtriple planet orbiting the three stars. [ 2 ]

  4. Kepler-444 - Wikipedia

    en.wikipedia.org/wiki/Kepler-444

    The Kepler-444 system consists of the planet hosting primary and a pair of M-dwarf stars. The M-dwarfs orbit each other at a distance of less than 0.3 AU while the pair orbits the primary in a highly eccentric 324-year orbit. The pair comes within 23.55 AU of the primary potentially truncating the protoplanetary disk from which the planets ...

  5. HD 134439 and HD 134440 - Wikipedia

    en.wikipedia.org/wiki/HD_134439_and_HD_134440

    Further adding to this, using Gaia data, HD 134440 appears to be 0.54 ± 0.26 light years further than HD 134439, [3] resulting in a true separation of 0.56 ± 0.25 light years from each other. If they are orbiting each other, they would have an orbital period on the scale of 5.3 ± 3 million years, making them one of the longest period binary ...

  6. Syzygy (astronomy) - Wikipedia

    en.wikipedia.org/wiki/Syzygy_(astronomy)

    Because the orbits of all the planets in the Solar System (as well as the Moon) are inclined by only a few degrees, they always appear very near the ecliptic in our sky. Therefore, although an apparent planetary alignment may appear as a line (actually, a great arc ), the planets are not necessarily aligned in space.

  7. List of multiplanetary systems - Wikipedia

    en.wikipedia.org/wiki/List_of_multiplanetary_systems

    4.09: 44: F8V: 1.27: 6107: 3.781: 3: Nearest F-type main sequence star with a multiplanetary system. Second-brightest star in the night sky with a multiplanetary system after 7 Canis Majoris. All exoplanets orbit around star A in the binary system. 47 Ursae Majoris: Ursa Major: 10 h 59 m 27.97 s +40° 25′ 48.9″ 5.10: 46: G0V: 1.029: 5892: 7 ...

  8. Category:Triple star systems - Wikipedia

    en.wikipedia.org/wiki/Category:Triple_star_systems

    This category is for physical triple stars, sometimes called trinary stars or ternary star systems in the case of a hierarchical star system. For optical triple stars, see Category:Triple stars v

  9. Binary star - Wikipedia

    en.wikipedia.org/wiki/Binary_star

    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 as a single object to the naked eye are often resolved as separate stars using a telescope, in which case they are called visual binaries. Many visual binaries have long ...

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