NGC 2997
From Wikipedia, the free encyclopedia
Image:NGC 2997.jpg
Spiral Galaxy NGC 2997 |
|
Observation data: J2000 epoch | |
---|---|
Constellation: | Antlia |
Right ascension: | 09h 45m 38.8s[1] |
Declination: | -31° 11′ 28″[1] |
Redshift: | 1088 ± 2 km/s[1] |
Distance: | 24.8 Mly[citation needed] |
Type: | SA(s)c[1] |
Apparent dimensions (V): | 8′.9 × 6′.8[1] |
Apparent magnitude (V): | 10.1[1] |
Notable features: | |
Other designations | |
ESO 434- G 35,[1] PGC 27978[1] | |
See also: Galaxy, List of galaxies |
NGC 2997 (also known as ESO 434- G 35) is an unbarred spiral galaxy about 24.8 million light-years away in the constellation Antlia. From our perspective its plane is inclined about 45 degrees, giving it an elliptical appearance. It is the brightest galaxy of the NGC 2997 group of galaxies.
NGC 2997 is particularly notable for a nucleus surrounded by a chain of hot giant clouds of ionized hydrogen.
Contents |