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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. List of nearest stars - Wikipedia

    en.wikipedia.org/wiki/List_of_nearest_stars

    The closest system is Alpha Centauri, with Proxima Centauri as the closest star in that system, at 4.2465 light-years from Earth. The brightest, most massive and most luminous object among those 131 is Sirius A , which is also the brightest star in Earth's night sky ; its white dwarf companion Sirius B is the hottest object among them.

  4. List of nearest stars by spectral type - Wikipedia

    en.wikipedia.org/wiki/List_of_nearest_stars_by...

    Also the 20nd nearest star system to the Solar System. Eta Cassiopeiae A (Achird) 19.42 [12] G0V [122] ... Zeta Ophiuchi is the closest O-type star to the Earth. Name

  5. List of multiplanetary systems - Wikipedia

    en.wikipedia.org/wiki/List_of_multiplanetary_systems

    The stars with the most confirmed planets are the Sun (the Solar System's star) and Kepler-90, with 8 confirmed planets each, followed by TRAPPIST-1 with 7 planets. The 1,033 multiplanetary systems are listed below according to the star's distance from Earth. Proxima Centauri, the closest star to the Solar System, has three planets (b, c and d).

  6. Star - Wikipedia

    en.wikipedia.org/wiki/Star

    A multi-star system consists of two or more gravitationally bound stars that orbit each other. The simplest and most common multi-star system is a binary star, but systems of three or more stars exist. For reasons of orbital stability, such multi-star systems are often organized into hierarchical sets of binary stars. [116]

  7. Betelgeuse - Wikipedia

    en.wikipedia.org/wiki/Betelgeuse

    As the Earth orbits the Sun, every star is seen to shift by a fraction of an arc second, which measure, combined with the baseline provided by the Earth's orbit gives the distance to that star. Since the first successful parallax measurement by Friedrich Bessel in 1838, astronomers have been puzzled by Betelgeuse's apparent distance.

  8. TRAPPIST-1 - Wikipedia

    en.wikipedia.org/wiki/TRAPPIST-1

    For a dim star like TRAPPIST-1, the habitable zone [ah] is located closer to the star than for the Sun. [164] Three or four [59] planets might be located in the habitable zone; these include e, f and g; [164] or d, e and f. [79] As of 2017, this is the largest-known number of planets within the habitable zone of any known star or star system. [165]

  9. Epsilon Eridani - Wikipedia

    en.wikipedia.org/wiki/Epsilon_Eridani

    At a declination of −9.46°, it is visible from most of Earth's surface. Located at a distance 10.5 light-years (3.2 parsecs) from the Sun, it has an apparent magnitude of 3.73, making it the third-closest individual star (or star system) visible to the naked eye. The star is estimated to be less than a billion years old. [18]