Triangulum Galaxy | |
---|---|
Observation data (J2000 epoch) | |
Pronunciation | /traɪˈæŋɡjʊləm/ |
Constellation | Triangulum |
Right ascension | 01h 33m 50.02s[1] |
Declination | +30° 39′ 36.7″[1] |
Redshift | -0.000607 ± 0.000010[1] |
Heliocentric radial velocity | -179 ± 3 km/s[2] |
Galactocentric velocity | -44 ± 6 km/s[2] |
Distance | 970 kpc (3.2 Mly)[3] |
Apparent magnitude (V) | 5.72[1] |
Characteristics | |
Type | SA(s)cd[2] |
Mass | 5×1010[4] M☉ |
Number of stars | 40 billion (4×1010)[6] |
Size | 18.74 kpc (61,120 ly) (diameter; 25.0 mag/arcsec2 B-band isophote)[5][6] |
Apparent size (V) | 70.8 × 41.7 arcminutes[1] |
Other designations | |
NGC 0598, MCG+05-04-069, UGC 1117, PGC 5818[2] |
The Triangulum Galaxy is a spiral galaxy 2.73 million light-years (ly) from Earth in the constellation Triangulum. It is catalogued as Messier 33 or NGC (New General Catalogue) 598. With the D25 isophotal diameter of 18.74 kiloparsecs (61,100 light-years), the Triangulum Galaxy is the third-largest member of the Local Group of galaxies, behind the Andromeda Galaxy and the Milky Way.
The galaxy is the second-smallest spiral galaxy in the Local Group after the Large Magellanic Cloud, which is a Magellanic-type spiral galaxy.[7] It is believed to be a satellite of the Andromeda Galaxy or on its rebound into the latter due to their interactions, velocities,[8] and proximity to one another in the night sky. It also has an H II nucleus.[9]
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