NGC 2415
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| NGC 2415 | |
|---|---|
| File:NGC2415 - SDSS DR14.jpg NGC 2415 imaged by SDSS | |
| Observation data (J2000 epoch) | |
| Constellation | Gemini |
| Right ascension | 07h 36m 56.7796s[1] |
| Declination | +35° 14′ 30.789″[1] |
| Redshift | 0.012619±0.0000170[1] |
| Heliocentric radial velocity | 3,783±5 km/s[1] |
| Distance | 189.3 ± 13.3 Mly (58.04 ± 4.07 Mpc)[1] |
| Group or cluster | NGC 2415 group (LGG 148) |
| Apparent magnitude (V) | 12.3B[1] |
| Characteristics | |
| Type | Im?[1] |
| Size | ~63,800 ly (19.56 kpc) (estimated)[1] |
| Apparent size (V) | 0.9′ × 0.9′[1] |
| Other designations | |
| IRAS 07336+3521, 2MASS J07365677+3514307, UGC 3930, MCG +06-17-021, PGC 21399, CGCG 177-038[1] | |
NGC 2415 is an irregular galaxy in the constellation of Gemini. Its velocity with respect to the cosmic microwave background is 3,935±12 km/s, which corresponds to a Hubble distance of 189.3 ± 13.3 Mly (58.04 ± 4.07 Mpc).[1] It was discovered by German-British astronomer William Herschel on 10 March 1790.[2][3]
NGC 2415 group
[edit | edit source]NGC 2415 is the namesake of the NGC 2415 group (also known as LGG 148) which has at least 9 members. The other eight galaxies are NGC 2444, NGC 2445, NGC 2476, NGC 2493, NGC 2524, NGC 2528, UGC 3937, and UGC 3944.[4][5]
Supernovae
[edit | edit source]Two supernovae have been observed in NGC 2415:
- SN 1998Y (Type II, mag. 18.3) was discovered by the Lick Observatory Supernova Search (LOSS) 16 March 1998.[6][7]
- SN 2000C (Type Ic, mag. 15.5) was discovered by Steven Foulkes, and independently by Marco Migliardi, on 8 January 2000.[8][9]
See also
[edit | edit source]References
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External links
[edit | edit source]- Error creating thumbnail: File missing Media related to Lua error in Module:Commons_link at line 62: attempt to index field 'wikibase' (a nil value). at Wikimedia Commons
- NGC 2415 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images