Astronomy:NGC 5056

From HandWiki
NGC 5056
NGC 5056 imaged by SDSS
Observation data (J2000 epoch)
ConstellationComa Berenices
Right ascension 13h 16m 12.3527s[1]
Declination+30° 57′ 01.239″[1]
Redshift0.018653±0.000005[1]
Helio radial velocity5,592±1 km/s[1]
Distance208.31 ± 10.46 Mly (63.867 ± 3.207 Mpc)[1]
Group or cluster[M98j] 192
Apparent magnitude (V)13.7[1]
Characteristics
TypeScd[1]
Size~135,800 ly (41.65 kpc) (estimated)[1]
Apparent size (V)1.7′ × 1.0′[1]
Other designations
IRAS 13138+3112, UGC 8337, MCG+05-31-166, PGC 46180[1]

NGC 5056 is a spiral galaxy in the constellation of Coma Berenices. Its velocity with respect to the cosmic microwave background is 5,839±17 km/s, which corresponds to a Hubble distance of 280.9 ± 19.7 Mly (86.13 ± 6.03 Mpc).[1] However, 39 non-redshift measurements give a closer mean distance of 208.31 ± 10.46 Mly (63.867 ± 3.207 Mpc).[2] It was discovered by German-British astronomer William Herschel on 13 March 1785.[3][4]

NGC 5056 is listed as having an active galactic nucleus.[5]

According to Abraham Mahtessian, NGC 5056 and NGC 5065 form a pair of galaxies, known as [M98j] 192.[6]

Supernova

One supernova has been observed in NGC 5056:

  • SN 2005au (Type II, mag. 15.8) was discovered by British amateur astronomer Ron Arbour on 19 March 2005.[7][8]

See also

References

Coordinates: Sky map 13h 16m 12.3527s, +30° 57′ 01.239″