NGC 1573 | |
---|---|
Observation data (J2000 epoch) | |
Constellation | Camelopardalis |
Right ascension | 04h 35m 03.975s[1] |
Declination | +73° 15′ 44.66″[1] |
Redshift | 0.014080[2] |
Heliocentric radial velocity | 4221 km/s[2] |
Distance | 188.84 ± 15.59 Mly (57.900 ± 4.781 Mpc)[2] |
Apparent magnitude (V) | 11.50[2] |
Apparent magnitude (B) | 13.3[3] |
Absolute magnitude (V) | −22.31[2] |
Characteristics | |
Type | E[2] |
Size | 112,200 ly (34,390 pc)[2][note 1] |
Apparent size (V) | 2.042′[2][note 1] |
Other designations | |
UGC 3077, MGC+12-05-008, PGC 15570[3] |
NGC 1573 is an elliptical galaxy in the constellation of Camelopardalis.[2] It was discovered on 1 August 1883 by Wilhelm Tempel.[4] It was described as "very faint, small" by John Louis Emil Dreyer, the compiler of the New General Catalogue.[4] It is located about 190 million light-years (58 megaparsecs) away.[2]
The galaxy PGC 16052 is not a NGC object, nor is it physically associated with NGC 1573, but is often called NGC 1573A. It is an intermediate spiral galaxy with an apparent magnitude of about 14.0.[4] In 2010, a supernova was discovered in PGC 16052 and was designated as SN 2010X.[5]
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