Messier 98 | |
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Messier 98 |
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Observation data (J2000 epoch) | |
Constellation | Coma Berenices |
Right ascension | 12h 13m 48.3s[1] |
Declination | +14° 54′ 01″[1] |
Redshift | -0.000474[1] |
Helio radial velocity | -142 ± 4 km/s[1] |
Distance | 54.1 ± 7.8 Mly (16.6 ± 2.4 Mpc)[2] |
Type | SAB(s)ab[1] |
Apparent dimensions (V) | 9′.8 × 2′.8[1] |
Apparent magnitude (V) | 11.0[1] |
Other designations | |
NGC 4192, UGC 7231, PGC 39028[1] | |
See also: Galaxy, List of galaxies |
Messier 98 (also known as M98 or NGC 4192) is an intermediate spiral galaxy about 60 million light-years away in the constellation Coma Berenices. It was discovered by Pierre Méchain on March 15, 1781 along with M99 and M100 and was cataloged as a Messier object on April 13, 1781. Messier 98 has a blue shift and is approaching us at about 140 km per second.[1]
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Messier 98 is a member of the Virgo Cluster, which is a large, relatively nearby cluster of galaxies.[3]
Coordinates: 12h 13m 48.3s, +14° 54′ 01″
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