M 65
M65, together with its neighbors M66 and NGC 3628, forms a most conspicuous triplet of galaxies, the Leo Triplett or M66 group, located at a distance of about 35 million light years.
Although it is close to and thus under the gravitational influence of its neighbors, M65 looks like a very "normal" Sa type spiral and seems to have felt little influence. It has a prominent central lense and tightly wound spiral arms, plus a prominent dust lane marking the facing edge. This lane may hide regions of star formation usually associated with such features in spiral galaxies.
| Right ascension | 11 : 16.3 (hours : minutes) |
|---|---|
| Declination | +13 : 23 (degrees : minutes) |
| Distance | 35000.0 (light-years*10^3) |
| Visual magnitude | 9.3 |