NGC 1077
| Galaxy NGC 1077 |
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|---|---|
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| NGC 1077 & PGC 10465 | |
| AladinLite | |
| Constellation | Perseus |
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Position equinox : J2000.0 , epoch : J2000.0 |
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| Right ascension | 02 h 46 m 01.7 s |
| declination | + 40 ° 05 ′ 30 ″ |
| Appearance | |
| Morphological type | Sb |
| Brightness (visual) | 13.7 mag |
| Brightness (B-band) | 14.5 mag |
| Angular expansion | 1.1 ′ × 0.8 ′ |
| Position angle | 165 ° |
| Surface brightness | 13.4 mag / arcmin² |
| Physical data | |
| Redshift | 0.029900 |
| Radial velocity | 8964 km / s |
|
Stroke distance v rad / H 0 |
(406 ± 28) x 10 6 ly (124.4 ± 8.7) Mpc |
| history | |
| discovery | Lewis Swift |
| Discovery date | August 16, 1885 |
| Catalog names | |
| NGC 1077 • 1077A • UGC 2230 • PGC 10468 • CGCG 539-095 • MCG + 07-06-069 • IRAS 02428 + 3952 • 2MASX J02460057 + 4005248 • | |
NGC 1077 is a spiral galaxy of Hubble type Sb in the constellation Perseus in the northern sky . It is an estimated 406 million light years from the Milky Way and about 130,000 light years in diameter. Together with PGC 10465 , it forms an interacting pair of galaxies.
The object was discovered by Lewis Swift on August 16, 1885 .