NGC 1295
| Galaxy NGC 1295 |
|
|---|---|
|
|
| AladinLite | |
| Constellation | Eridanus |
|
Position equinox : J2000.0 , epoch : J2000.0 |
|
| Right ascension | 03 h 20 m 03.3 s |
| declination | -13 ° 59 ′ 54 ″ |
| Appearance | |
| Morphological type | (R ') SB? (S?) 0+: |
| Brightness (visual) | 14.3 mag |
| Brightness (B-band) | 15.3 mag |
| Angular expansion | 0.9 ′ × 0.5 ′ |
| Position angle | 175 ° |
| Surface brightness | 13.3 mag / arcmin² |
| Physical data | |
| Redshift | 0.016521 ± 0.000117 |
| Radial velocity | 4953 ± 35 km / s |
|
Stroke distance v rad / H 0 |
(219 ± 15) x 10 6 ly (67.1 ± 4.7) Mpc |
| history | |
| discovery | Ormond Stone |
| Discovery date | 1886 |
| Catalog names | |
| NGC 1295 • PGC 12465 • MCG -02-09-030 • IRAS 03177-1410 • 2MASX J03200331-1359537 • GALEX ASC J032003.22-135953.8 | |
NGC 1295 is a lenticular galaxy of the Hubble type S0 in the constellation Eridanus in the southern sky . It is estimated to be 219 million light-years away from the Milky Way and has a diameter of about 60,000 ly
. a. the galaxies NGC 1290 , NGC 1296 , IC 318 .
The object was discovered in 1886 by the astronomer Ormond Stone .