NGC 1592

NGC 1592
NGC 1592 with legacy surveys
Observation data (J2000.0 epoch)
Constellation	Eridanus
Right ascension	04h 29m 40.1s[1]
Declination	−27° 24′ 31″[1]
Redshift	0.003149[1]
Heliocentric radial velocity	944 km/s[1]
Distance	45 mly (redshift) 30 (TF relation)
Apparent magnitude (V)	15.5
Characteristics
Type	Irr[2]
Apparent size (V)	1.6 x 0.55
Other designations
ESO 421-IG 002 ESO 042739-2731.0 VV 647 AM 0427-273 MCG -05-11-011 LCSB L0237O IRAS F 04276-2731 SGC 042739-2731.0 GSC 6467 01772 HIPASS J0429-27 PGC 015292 11HUGS 079

NGC 1592 is an irregular galaxy in the constellation Eridanus. It is about 20,000 light-years across. It has not been studied in detail, as it is at 27 degrees south, making it not visible below 63 degrees north in a flat area, and about 50 degrees north in a hilly area. It was discovered in 1835 by John Herschel.^[2]

Until 2014, not much was known about the galaxy, other than the fact it was irregular. In early 2014, the galaxy was observed with a 2-foot telescope at the SARA remote observatory in Chile, revealing the galaxy in higher resolution. It appears the galaxy is in the process of forming stars at a high rate - primarily in the red areas in the image. Additionally, the galaxy has several small clumps of stars, implying an ongoing merger.^[3]

NGC 1592 appears to have a companion, 2MFGC (2MASS Flat Galaxy Catalog) 3572, at 40 million light years away, assuming similar velocity with NGC 1592. they are separated by about 750,000 ±200,000 light years.^[1]

• Media related to NGC 1592 at Wikimedia Commons