Today, NGC 3613 is a topic that arouses interest in a wide variety of people around the world. Whether because of its influence on society, its relevance in history, or its impact on daily life, this topic has captured the attention of academics, experts, and enthusiasts alike. From its origins to its implications in the present, NGC 3613 continues to be the subject of constant debate and analysis. In this article, we will explore in depth the different aspects of NGC 3613, from its origins to its evolution over time, in order to provide a comprehensive look at this fascinating topic.
| NGC 3613 | |
|---|---|
Pan-STARRS image of NGC 3613 | |
| Observation data (J2000 epoch) | |
| Constellation | Ursa Major |
| Right ascension | 11h 18m 36.130s[1] |
| Declination | +57° 59′ 59.73″[1] |
| Redshift | 0.006738[2] |
| Heliocentric radial velocity | 2013 ± 47 km/s[2] |
| Distance | 98 Mly (30.1 Mpc)[3] |
| Absolute magnitude (V) | −21.5[3] |
| Characteristics | |
| Type | E6[3] |
| Apparent size (V) | 1.347′ × 0.997′[2] |
| Other designations | |
| UGC 6323, MCG +10-16-109, PGC 34583[2] | |
NGC 3613 is an elliptical galaxy in the constellation Ursa Major. It was discovered by the astronomer William Herschel on April 8, 1793.[4] NGC 3613 is the center of a cluster of galaxies, and has an estimated globular cluster population of over 2,000.[3]
In 2011, SN 2011eh, a type Ia supernova with a peculiar spectrum, was detected within NGC 3613.[5]