Subject |
has right ascension |
has declination |
has spectral type |
is part of |
has surface temperature |
is an instance of |
has V magnitude |
has been observ |
has color |
has symbol |
has B-V magnitude |
has distance |
has abundance |
has period |
is usually part of |
has proper motion |
is a kind of |
has apparent magnitude |
has synonym |
has definition |
has luminosity class |
has number of star |
binary star | | | | | greater than 1000 Kelvin | | | | | | | | half the stars in the solar neighborhood are members of star systems | | | | star system | | | A system of two stars orbiting around a common center of gravity. Visual binaries are those whose components can be resolved telescopically (i.e., angular separation > 0'.5) and which have detectable orbital motion. Astrometric binaries are those whose dual nature can be deduced from their variable proper motion; spectroscopic binaries, those whose dual nature can be deduced from their variable radial velocity. At least half of the stars in the solar neighborhood are members of binary (or multiple) systems. (See photometric binaries; optical pairs.) | | 2 |
dwarf | | | | | greater than 1000 Kelvin | | | | | d | | | | | | | star | | main sequence star | Star with mass equal to or less than that of the sun. More generally, any star on or below the main sequence in the Hertzprung-Russell diagram. | V | |
G star | | | cooler than G2 | | 5000 to 6000 K | | | | yellowish | | | | | | | | late star | | | Yellowish star in which the H and K lines of Ca II have become dominant and in which a tremendous profusion of spectral lines of both neutral and ionized metals, particularly iron, begins to show. The Balmer lines of hydrogen are still recognizable. Examples are the Sun and Capella. | | |
naked eye star | | | | Milky Way | greater than 1000 Kelvin | | | for many centuries | | | | | | | asterism | | naked eye object | brighter than 5 | | A star visible without visual aids | | |
alpha Centauri | 14 39 36.2 | -60 50 07 | G2V | Milky Way | 5000 to 6000 K | naked eye star | -0.01 | for many centuries | yellowish | d | 0.71 | 4.35 light-years | half the stars in the solar neighborhood are members of star systems | 80 years | asterism | 3'.68 per year | | brighter than 5 | HR 5459 | A binary star whose components have G2 V and K5 V spectral types. The nearest star system to the Sun and the third brightest star in the night sky. | V | 2 |