NGC 665 | |
---|---|
Observation data (J2000 epoch) | |
Constellation | Pisces |
Right ascension | 01h 44m 56.10s[1] |
Declination | 10° 25′ 23″[1] |
Redshift | 0.018079±0.000103[1] |
Distance | 236 Mly (72.3 Mpc)[2] |
Apparent magnitude (V) | 12.2[2] |
Characteristics | |
Type | (R)S0^0[2] |
Size | 100,000 ly |
Apparent size (V) | 1.8 x 1.0[1] |
Notable features | Small halo of gas visible at galactic center |
Other designations | |
UGC 1223,[2] PGC 6415,[2] MCG+02-05-019[2] |
NGC 665 is a Lenticular galaxy 236 million light-years away in the constellation Pisces.[2] NGC 665 was discovered in 1786 by William Herschel, and is 100,000 light-years across. In the center of NGC 665, a small halo of dust and gas can be seen, indicating some small star-forming regions.[2] NGC 665 is not known to have an active galactic nuclei, as seen in the SDSS image.[1]
Nearby and satellite galaxies
Like other galaxies, NGC 665 has a satellite galaxy (MCG 02-05-022),[3] a dwarf elliptical galaxy, as seen in the SDSS image of NGC 665.[2] Its nearby cluster of stars is NGC 663.
References
External links
- Media related to NGC 665 at Wikimedia Commons
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