In this article, we are going to delve into the fascinating world of NGC 2927. From its impact on society to its applications in daily life, NGC 2927 represents a topic of universal interest that has captured the attention of people of all ages and backgrounds. Along these lines, we will explore its origins, evolution and relevance in today's world, as well as the opinions and perspectives of experts in the field. Prepare to immerse yourself in an in-depth and diverse analysis of NGC 2927, which will undoubtedly leave you with new understanding and inspiration about this exciting topic.
NGC 2927 | |
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![]() The barred spiral galaxy NGC 2927 | |
Observation data (J2000 epoch) | |
Constellation | Leo |
Right ascension | 09h 37m 15.21s[1] |
Declination | +23° 35′ 26.209″[1] |
Redshift | 0.025147[1] |
Heliocentric radial velocity | 7539 ± 2 km/s[1] |
Distance | 376.7 ± 26.4 Mly (115.49 ± 8.09 Mpc)[1] |
Apparent magnitude (V) | 12.9[1] |
Characteristics | |
Type | SAB(rs)b[1] |
Size | ~229,000 ly (70.20 kpc) (estimated)[1] |
Apparent size (V) | 1.3′ × 1.0′[1] |
Other designations | |
IRAS F09343+2349, 2MASX J09371521+2335261, UGC 5122, MCG +04-23-016, PGC 27385, CGCG 122-032[1] |
NGC 2927 is a large barred spiral galaxy in the constellation of Leo. Its velocity with respect to the cosmic microwave background is 7830 ± 20 km/s, which corresponds to a Hubble distance of 115.49 ± 8.09 Mpc (~377 million light-years).[1] In addition, three non-redshift measurements give a distance of 120.667 ± 0.882 (~394 million light-years).[2] The galaxy was discovered by German astronomer Heinrich d'Arrest on 21 February 1863.[3]
The SIMBAD database lists NGC 2927 as a radio galaxy, i.e. it has giant regions of radio emission extending well beyond its visible structure.[4]
One supernova has been observed in NGC 2927: SN 2023uvg (type Ic, mag. 18.7389) was discovered by the Automatic Learning for the Rapid Classification of Events (ALeRCE) on 13 October 2023.[5]
NGC 2927 forms a pair of galaxies with NGC 2929.[6]