NGC 997

NGC 997 is an interacting galaxy in the constellation of Cetus. The galaxy was discovered by Albert Marth on 10 November 1863.^[3] It has a regularly rotating central molecular gas disk, containing a black hole of between 4 x 10⁷ and 1.8 x 10⁹ solar masses.^[4] Its speed relative to the cosmological background is 6,270 ± 45 km/s, corresponding to a Hubble distance of 92.5 ± 6.5 Mpc (~302 million ly).^[2]

ConstellationCetus

Right ascension02^h 37^m 14.50^s

Declination±07° 18′ 28.0″

Redshift0.021695

Quick facts Observation data (J2000 epoch), Constellation ...

NGC 997
NGC 997 and its neighbouring galaxies captured by SDSS
Observation data (J2000 epoch)
Constellation	Cetus
Right ascension	02h 37m 14.50s
Declination	±07° 18′ 28.0″
Redshift	0.021695
Heliocentric radial velocity	6504 ± 42 km/s
Distance	301.6 ± 21.3 Mly (92.48 ± 6.54 Mpc)
Group or cluster	[CHM2007] HDC 157, [CHM2007] LDC 181, [T2015] nest 200334
Characteristics
Type	E[1]
Size	~105,800 ly (32.44 kpc) (estimated)
Other designations
IRAS F02345+0705, UGC 2102, MCG +01-07-016, CGCG 414-027
References: [2][1]

Close

NGC 997 is accompanied by PGC 200205, also designated as NGC 997 NED01,^[5] a compact galaxy. No data is available for the latter galaxy. So, this pair may be due to an optical alignment, or they may be two gravitationally interacting galaxies about to merge.

One supernova has been observed in NGC 997: SN 2020nej (type Ia, mag. 17).^[6]