NGC 4965
| Galaxy NGC 4965 |
|
|---|---|
|
|
|
| AladinLite | |
| Constellation | Water snake |
|
Position equinox : J2000.0 , epoch : J2000.0 |
|
| Right ascension | 13 h 07 m 09.4 s |
| declination | -28 ° 13 ′ 41 ″ |
| Appearance | |
| Morphological type | SAB (s) d / HII |
| Brightness (visual) | 12.1 mag |
| Brightness (B-band) | 12.8 mag |
| Angular expansion | 2.4 ′ × 2.0 ′ |
| Position angle | 136 ° |
| Surface brightness | 13.7 mag / arcmin² |
| Physical data | |
| Affiliation | LGG 331 |
| Redshift | 0.007542 ± 0.000017 |
| Radial velocity | 2261 ± 5 km / s |
|
Stroke distance v rad / H 0 |
(95 ± 7) x 10 6 ly (29.0 ± 2.0) Mpc |
| history | |
| discovery | John Herschel |
| Discovery date | May 5, 1834 |
| Catalog names | |
| NGC 4965 • UGCA 326 • PGC 45437 • ESO 443-070 • MCG -05-31-036 • IRAS 13044-2757 • 2MASX J13070938-2813414 • SGC 130426-2757.6 • GC 3404 • h 3466 • HIPASS J1307-28 | |
NGC 4965 is a 12.1 likes bright barred spiral galaxy with extensive star formation from Hubble type SBCD in the constellation of Hydra south of the ecliptic . It is estimated to be 95 million light years away from the Milky Way and has a diameter of around 70,000 ly.
In the same area of the sky is the galaxy NGC 4980 .
The Type II n supernova SN 2000P was observed here.
The object was discovered on May 5, 1834 by John Herschel with an 18-inch reflector telescope, which it marked with “vF, vL, oval; cf.bM, 3 ′ long, 2 ′ broad “. On a second observation he noted “eF, vL, oval; vlbM, 3 ′ “.