| NGC 5714 | |
|---|---|
 NGC 5714 taken by 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] |
| Heliocentric radial velocity | 2228km/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.
One supernova has been observed in NGC 5714: SN 2003dr (type Ib/c, mag. 17.9).[3]
- ^ a b c "The curious case of calcium-rich supernovae". www.spacetelescope.org. Retrieved 26 March 2018.
- ^ a b c d e f g h "SIMBAD Astronomical Database - CDS (Strasbourg)". Results for NGC 5714. Retrieved 2018-03-26.
- ^ Transient Name Server entry for SN 2003dr. Retrieved 3 April 2023.