Astronomy:NGC 5714
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| NGC 5714 | |
|---|---|
| File:NGC 5714 - HST - Potw1813a.tif NGC 5714 imaged by the Hubble Space Telescope[1] | |
| Observation data (J2000[2] epoch) | |
| Constellation | Boötes[1] |
| Right ascension | 14h 38m 11.543s[2] |
| Declination | +46° 38′ 18.09″[2] |
| Redshift | 0.00746[2] |
| Helio radial velocity | 2228 km/s[2] |
| Apparent magnitude (B) | 14.2[2] |
| Characteristics | |
| Type | Sc [2] |
| Other designations | |
| FGC 1785, IRAS 14363+4651, IRAS F14363+4651, LEDA 52307, 2MASX J14381154+4638180, MCG+08-27-011, 2MFGC 11872, PSCz Q14363+4651, RFGC 2826, SDSS J143811.51+463817.6, TC 547, UGC 9431, UZC J143811.7+463817, Z 248-14, Z 1436.4+4651, [CHM2007] LDC 1062 J143811.54+4638180[2] | |
NGC 5714 is a spiral galaxy located 130 million light-years away in the constellation of Boötes (the Herdsman).[1] It was discovered by William Herschel in 1787. This galaxy is about 130 million light-years away.
Supernova
One supernova has been observed in NGC 5714:
- SN 2003dr (Type Ib/c, mag. 17.9) was discovered by Tim Puckett and D. Toth, and independently by LOTOSS (Lick Observatory and Tenagra Observatory Supernova Searches), on 13 April 2003.[3][4]
References
- ↑ 1.0 1.1 1.2 "The curious case of calcium-rich supernovae". https://www.spacetelescope.org/images/potw1813a/.
- ↑ 2.0 2.1 2.2 2.3 2.4 2.5 2.6 2.7 "SIMBAD Astronomical Database - CDS (Strasbourg)". Results for NGC 5714. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=NGC+5714&submit=SIMBAD+search.
- ↑ Puckett, T.; Toth, D.; Schwartz, M.; Holvorcem, P. R.; Wood-Vasey, W. M.; Aldering, G.; Nugent, P.; Kulkarni, A. (2003). "Supernovae 2003dm, 2003dn, 2003do, 2003dp, 2003dq, 2003dr". International Astronomical Union Circular (8117): 1. Bibcode: 2003IAUC.8117....1P. http://www.cbat.eps.harvard.edu/iauc/08100/08117.html#Item1.
- ↑ "SN 2003dr". IAU. https://www.wis-tns.org/object/2003dr.
External links
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