| NGC 5970 | |
|---|---|
NGC 5970 imaged by Hubble Space Telescope
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| Observation data (J2000 epoch) | |
| Constellation | Serpens Caput |
| Right ascension | 15h38m 29.96s[1] |
| Declination | +12° 11′ 11.9″[1] |
| Redshift | 0.00661[2] |
| Heliocentric radial velocity | 1974 km/s[2] |
| Distance | 91.91 ± 0.65 Mly (28.18 ± 0.20 Mpc)[3] |
| Apparent magnitude (V) | 11.61[1] |
| Apparent magnitude (B) | 12.00[1] |
| Characteristics | |
| Type | SB(r)c[4] |
| Other designations | |
| UGC 9943, MCG +02-40-006, PGC 55665[2] | |
NGC 5970 is a large barred-spiral galaxy located about 90 million light years away in the constellation Serpens Caput. It appears to have two satellite or companion galaxies. It is a member of the Virgo Cluster of galaxies.[2] It was discovered on March 15, 1784, by the astronomer William Herschel.[5]
LINER-type emission has been detected from the disk of NGC 5970.[6]
NGC 5970 can be seen 1° southwest of the star Chi Serpentis. A faint halo of dust can be seen around the galaxy's outer spiral arms.
Media related to NGC 5970 at Wikimedia Commons|
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