| Messier 99 | |
|---|---|
A near-infrared image of M99. Credit: 2MASS/NASA. |
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| Observation data (J2000 epoch) | |
| Constellation | Coma Berenices[1] |
| Right ascension | 12h 18m 49.6s[2] |
| Declination | +14° 24′ 59″[2] |
| Redshift | 0.008029[2] |
| Helio radial velocity | 2407 ± 3 km/s[2] |
| Distance | 50.2 ± 5.5 Mly (15.4 ± 1.7 Mpc)[3] |
| Type | SA(s)c[2] |
| Apparent dimensions (V) | 5′.4 × 4′.7 |
| Apparent magnitude (V) | 10.4[2] |
| Other designations | |
| NGC 4254,[2] UGC 7345,[2] PGC 39578,[2] Coma Pinwheel Galaxy,[4] Virgo Cluster Pinwheel[4] | |
| See also: Galaxy, List of galaxies | |
Messier 99 (also known as M99 or NGC 4254) is an unbarred spiral galaxy approximately 50 million light-years away[3] in the constellation Coma Berenices.
The galaxy has a normal looking arm and an extended arm that is less tightly wound. A bridge of neutral hydrogen gas links NGC 4254 with VIRGOHI21. The gravity from the possible dark galaxy VIRGOHI21 may have distorted M99 and drawn out the gas bridge, as the two galaxy-sized objects have a close encounter, before they go their separate ways. It is expected that the drawn out arm will relax to match the normal arm once the encounter is over. Three supernovae have been observed in this galaxy.
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Messier 99 was discovered by Pierre Méchain on March 17, 1781 along . The discovery was then reported to Charles Messier, who included the object in the Messier Catalogue, which was the first astronomical catalogue of star clusters, nebulae, and galaxies.[5]
Messier 99 was one of the first galaxies in which a spiral pattern was first seen. The spiral pattern was first identified by Lord Rosse in the spring of 1846.[5]
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