NGC 7713 | |
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![]() NGC 7713 imaged by the Hubble Space Telescope | |
Observation data (J2000 epoch) | |
Constellation | Sculptor |
Right ascension | 23h 36m 14.9900s [1] |
Declination | −37° 56′ 17.100″ [1] |
Distance | 29.52 ± 0.94 Mly (9.051 ± 0.288 Mpc) [1] |
Group or cluster | IC 5332 Group (LGG 478) |
Apparent magnitude (B) | 11.63 |
Surface brightness | 22.97 mag/arcsec2 |
Characteristics | |
Type | SB(r)d? [1] |
Size | ~51,500 ly (15.80 kpc) (estimated) [1] |
Apparent size (V) | 4.5′ × 1.8′ [1] |
Other designations | |
ESO 347-028, 2MASX J23361515-3756221, MCG -06-51-013, PGC 71866 [1] |
NGC 7713 is a barred spiral galaxy with extensive Hubble-type SBcd star-forming regions that is located in the constellation Sculptor in the southern sky. It is estimated to be 31 million light-years from the Milky Way and about 40,000 light-years in diameter. [2] [3] [4] It was discovered by John Herschel on October 4, 1836. [5]
One supernova has been observed in NGC 7713: SN 1982L (type II, mag. 16) was discovered by Marina Wischnjewsky on 21 July 1982. [6] [7]
According to A.M. Garcia, NGC 7713 is a member of the IC 5332 galaxy group (also known as LGG 478). This small group has three galaxies, including IC 5332 and PGC 72525. [8]