Local Group | has members Milky Way, M31, M33, LMC, SMC, IC 1613, NGC 6822, NGC 147, NGC 185, NGC 205, M32, Sculptor galaxy, Fornax galaxy, Leo I, Leo II, UMi galaxy, Draco system and three companions to M31 | |
is a part of Local Supercluster | |
has number of galaxies 30 | |
has diameter 2 Mpc | |
has definition The gravitationally bound collection of nearby galaxies ruled by the Andromeda galaxy and the Milky Way, which are its largest members. The Local Group has about 30 known galaxies. | |
has definition The association of galaxies to which the Milky Way galaxy belongs. | |
has definition A conglomeration of about twenty galaxies including our own Milky Way. | |
has definition The cluster of galaxies to which our Galaxy belongs. It is a poor, irregular cluster with some 20 certain members: three spirals (the Galaxy, M31, and M33); four irregulars (LMC, SMC, IC 1613, and NGC 6822); and about 13 intermediate or dwarf ellipticals (NGC 147; NGC 185; NGC 205; M32; the Sculptor, Fornax, Leo I and II, UMi, and Draco systems; and three companions to M31 discovered by van den Bergh in 1972). It may also include several other dwarf galaxies as well as the giant elliptical Maffei 1. The total mass of the Local Group is less than 1.5 times the combined masses of the Galaxy and M31. | |
has definition The system of galaxies to which our Milky Way galaxy belongs is a small group, containing only two large spirals (our galaxy and the Andromeda galaxy, Messier 31) and twenty or more smaller systems. | |
has definition The cluster of galaxies of which our own, the Milky Way, is one. Its radius is estimated at 106 parsecs. Largest of the Group is the Andromeda galaxy. | |
is an instance of loose group | |
collection of stars | has number of stars | |
has catalog catalog about star systems | |
celestial body | has spectra | |
physical object | has location or center of gravity | |
has angular momentum | |
has mass | |
has velocity | |
has momentum | |
has temperature | |
has volume | |
has extent | |
has material | |