In this article, we will explore the fascinating world of NGC 4845, a topic that has captured the attention of millions of people around the world. From its origins to its impact on today's society, NGC 4845 has generated debates and reflections on its relevance in various fields. Along these lines, we will immerse ourselves in its history, analyze its most relevant aspects and examine its influence in different areas. With an in-depth approach, this reading invites you to discover and better understand the nuances and complexities that characterize NGC 4845, offering new perspectives and reflections on this exciting topic.
NGC 4845 | |
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![]() NGC 4845 as seen by HST | |
Observation data (J2000 epoch) | |
Constellation | Virgo |
Right ascension | 12h 58m 01.2s[1] |
Declination | 1° 34′ 33″ |
Redshift | z=0.004110 (1232 km/s)[1] |
Distance | 65 Mly |
Apparent magnitude (V) | 11.2[2] |
Characteristics | |
Type | Sab[2] |
Apparent size (V) | 4′.9 × 1′.3[2] |
Other designations | |
UGC 08087, 2MASX J12580124+0134320, NGC 4910, PGC 44392[3] |
NGC 4845 (also known as NGC 4910) is a spiral galaxy located in the constellation Virgo around 65 million light years away.[4] The galaxy was originally discovered by William Herschel in 1786.[5] It is a member of the NGC 4753 Group of galaxies, which is a member of the Virgo II Groups, a series of galaxies and galaxy clusters strung out from the southern edge of the Virgo Supercluster.[6]
The galaxy has a supermassive black hole, called IGR J12580+0134, at its center with a mass of 300,000. In 2013, the ESA observed the black hole absorbing matter from a nearby, low-mass object; possibly a brown dwarf star.[7][8] The observed X-ray flare was caught by the ESA's INTEGRAL telescope.[9]