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| physical object > natural object > celestial body > collection of stars > galaxy > galaxy containing Cepheids |
| galaxy containing Cepheids | ||||
| subject | fact | |||
| galaxy containing Cepheids | is a kind of galaxy | ![]() |
| has distance determined from Cepheid period-luminosity relation | ![]() | |
| has number of Cepheids | ![]() | |
| galaxy | has number of stars 106 to 1012 | ![]() |
| has catalog galaxy catalog | ![]() | |
| 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 | ![]() |
Kinds of galaxy containing Cepheids :
(13 facts) (M 31) - Major spiral galaxy, 2.2 million light-years from Earth. Gravitationally bound to the Milky Way with which it shares membership in the Local Group, it is currently approaching us, rather than receding as is the case for most galaxies., A spiral galaxy (kS5 in Morgan's classification) in the Local Group, about 650-700 kpc distant (MV = -21), visible to the naked eye as a fuzzy patch in the constellation of Andromeda. Total mass about 3.1 × 1011 Msun ; i = 77°, heliocentric velocity - 180 km s-1. Its nucleus exhibits noncircular gas motions. It is similar to but slightly larger than our Galaxy., The largest galaxy in the Local Group. Also known as the Great Spiral and M31. It is about one and a half times the size of our own galaxy, and contains at least 300 globular clusters. Two smaller, elliptical galaxies (M32 and NGC 205) lie close to it., The largest member of the local group. It is a giant spiral galaxy that lies 2.4 million light-years away.