NGC 5970
| Galaxy NGC 5970 |
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| NGC 5970 SDSS image | |
| AladinLite | |
| Constellation | Snake |
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Position equinox : J2000.0 , epoch : J2000.0 |
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| Right ascension | 15 h 38 m 29.97 s |
| declination | + 12 ° 11 ′ 11.8 ″ |
| Appearance | |
| Morphological type | SB (r) c / HII / LINER |
| Brightness (visual) | 11.5 likes |
| Brightness (B-band) | 12.2 mag |
| Angular expansion | 3 ′ × 2 ′ |
| Position angle | 88 ° |
| Surface brightness | 13.3 mag / arcmin² |
| Physical data | |
| Affiliation | NGC 5970 group LGG 401 |
| Redshift | 0.006527 ± 0.000017 |
| Radial velocity | (1957 ± 5) km / s |
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Stroke distance v rad / H 0 |
(90 ± 6) x 10 6 ly (27.7 ± 1.9) Mpc |
| history | |
| discovery | William Herschel |
| Discovery date | March 15, 1784 |
| Catalog names | |
| NGC 5970 • UGC 9943 • PGC 55665 • CGCG 078-034 • MCG + 02-40-006 • IRAS 15361 + 1220 • 2MASX J15382998 + 1211117 • GC 4122 • H II 76 • HIPASS J1538 + 12b • LDCE 1138 NED003 | |
NGC 5970 is an active bar-spiral galaxy of the Hubble-type SBc with extensive star formation areas in the constellation Snake north of the celestial equator . It is estimated to be 90 million light years from the Milky Way and about 80,000 light years in diameter. Presumably it forms a gravitationally bound galaxy pair together with IC 1131 . She is the brightest member of the NGC 5970 group ( LGG 401 ).
In the same area of the sky are u. a. the galaxies NGC 5956 and NGC 5957 .
The object was discovered on March 15, 1784 by the astronomer William Herschel with the help of his 18.7-inch mirror telescope and was later included in his New General Catalog by Johan Dreyer .
NGC 5970 group ( LGG 401 )
| Galaxy | Alternative name | Distance / million ly |
|---|---|---|
| NGC 5956 | PGC 55501 | 87 |
| NGC 5957 | PGC 55520 | 84 |
| NGC 5970 | PGC 55665 | 90 |
| PGC 55660 | UGC 9941 | 86 |