| NGC 3245 | |
|---|---|
Hubble Space Telescope image of NGC 3245 | |
| Observation data (J2000 epoch) | |
| Constellation | Leo Minor |
| Right ascension | 10h 27m 18s |
| Declination | +28° 30′ 26″ |
| Redshift | 0.004423 |
| Heliocentric radial velocity | 1,326±5 km/s |
| Apparent magnitude (V) | 10.7 |
| Apparent magnitude (B) | 11.6 |
| Characteristics | |
| Type | SA(r)0^0^ |
| Apparent size (V) | 3.2′ × 1.8′ |
| Other designations | |
| NGC 3245,MCG+05-25-013, LEDA 30744 | |
NGC 3245 is a lenticular galaxy in the constellation Leo Minor. It was discovered by German-British astronomer William Herschel on April 11, 1785. The galaxy has an apparent visual magnitude of 10.7 and spans an angular size of 3.2′ × 1.8′. It is located at a distance of 68 million light-years (20.9 Mpc). The morphological classification of NGC 3245 is SA(r)0^0^, which is consistent with a lenticular galaxy (SA0) possessing a ring-like structure (r).
There is a circumnuclear dust with a radius of 1.1″, which corresponds to a radius of 360 ly (110 pc). The rotational motion of this disk is consistent with a supermassive black hole at the core with a mass of (2.1±0.5)×108 M☉, or 210 million times the mass of the Sun.
This is a member of the NGC 3254 Group of galaxies, which is a member of the Leo II Groups, a series of galaxies and galaxy clusters strung out from the right edge of the Virgo Supercluster.
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