Today, NGC 2959 is a topic of great relevance and interest in today's society. More and more people are getting involved and concerned about NGC 2959, looking for information, opinions and advice about it. In this article, we will explore the topic of NGC 2959 in depth, analyzing its different facets and offering a comprehensive approach that allows readers to better understand its importance and implications. From its origin to its impact today, NGC 2959 is a topic that leaves no one indifferent, and through this article we hope to provide a broad and detailed vision that helps enrich the knowledge and understanding of this topic.
NGC 2959 | |
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![]() The intermediate spiral galaxy NGC 2959 | |
Observation data (J2000 epoch) | |
Constellation | Ursa Major |
Right ascension | 09h 45m 08.9714s[1] |
Declination | +68° 35′ 40.507″[1] |
Redshift | 0.01482[1] |
Heliocentric radial velocity | 4442 ± 3 km/s[1] |
Distance | 217.7 ± 15.2 Mly (66.74 ± 4.67 Mpc)[1] |
Apparent magnitude (V) | 12.8[1] |
Characteristics | |
Type | (R')SAB(rs)ab pec?[1] |
Size | ~131,400 ly (40.28 kpc) (estimated)[1] |
Apparent size (V) | 1.4′ × 1.4′[1] |
Other designations | |
IRAS 09409+6849, UGC 5202, MCG +12-09-062, PGC 27939, CGCG 332-061[1] |
NGC 2959 is an intermediate spiral galaxy in the constellation Ursa Major. Its velocity relative to the cosmic microwave background is 4,525 ± 6 km/s, which corresponds to a Hubble distance of 66.7 ± 4.7 Mpc (~218 million light years.).[1] NGC 2959 was discovered by British astronomer John Herschel on 28 October 1831.
NGC 2959 has a luminosity class of I-II and a broad H I line.[1]
According to the Simbad database, NGC 2959 is a LINER galaxy, i.e. a galaxy whose nucleus has an emission spectrum characterized by broad lines of weakly ionized atoms.[2]
Two supernovae have been observed in NGC 2959: