At a distance of 2.5 million ly away in the constellation of Andromeda, the barred spiral galaxy Messier 31 has a diameter of about 152000 ly in space or 3.2º x 1º apparent in the sky. It resembles our Milky Way in various respects and both galaxies are expected to merge in 4-5 billion years. Shining at magnitude 3.4 with an estimated total of 1 trillion stars, M31 is visible to the naked eye. It has two major satellite galaxies, M32 and M110 (in total 20 known) plus 460 globular clusters associated with it. M31 is surrounded by a massive halo of hot gas which stretches about a million ly into space halfway to our Milky Way Galaxy.
M32
Galaxy
Magnitude
9.1
Size
8.5'
Distance
249000000
Constellation
Andromeda
Sky Atlas
page 4
R.A.
0.7116 hrs
Decl.
40.8653°
Catalogs
NGC 221
Popular
M32 is an elliptical dwarf galaxy which contains about 3 billion solar masses and stretches across space some 8,000 light-years. Its nucleus is almost as bright as M31's. Both contain about 100 million solar masses in rapid motion around a central supermassive object. M32 is the prototype for the relatively rare class of galaxies referred to as compact ellipticals.
M110
Galaxy
Magnitude
8.9
Size
19.5'
Distance
26900000
Constellation
Andromeda
Sky Atlas
page 4
R.A.
0.6728 hrs
Decl.
41.6847°
Catalogs
NGC 205
Popular
Classified as a dwarf spheroidal galaxy, M110 is some 2.9 million light-years away on the outskirts of the Andromeda Galaxy. Despite its diminuative size, its an active little galaxy with a system of 8 globular clusters in a halo around it.
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