NGC 4359 | |
---|---|
![]()
SDSS image of NGC 4359. | |
Observation data ( J2000 epoch) | |
Constellation | Coma Berenices |
Right ascension | 12h 24m 11.2s [1] |
Declination | 31° 31′ 19″ [1] |
Redshift | 0.004179 [1] |
Heliocentric radial velocity | 1253 km/s [1] |
Distance | 56.21 Mly (17.233 Mpc) [1] |
Group or cluster | Coma I (NGC 4274 subgroup) |
Apparent magnitude (V) | 13.6 [1] |
Characteristics | |
Type | SB(rs)c?+ [1] |
Size | ~27,100 ly (8.32 kpc) (estimated) [1] |
Apparent size (V) | 2.57 x 0.80 [1] |
Other designations | |
UGC 07483, PGC 040330, MCG +05-29-079 [1] |
NGC 4359 is a dwarf barred spiral galaxy [2] [3] seen edge-on that is about 56 million light-years away [4] in the constellation Coma Berenices. It was discovered by astronomer William Herschel on March 20, 1787. [5] It is a member of the NGC 4274 Group, [6] [7] which is part of the Coma I Group [6] [7] or Cloud. [8]
On the sky, NGC 4359 appears to lie closest to the flocculent spiral NGC 4414 [9] which is also a member of the NGC 4274 Group [7] and the Coma I cloud. [8] However, their radial velocities differ by around 500 km/s suggesting an interaction between the two is unlikely. [9]
NGC 4359 | |
---|---|
![]()
SDSS image of NGC 4359. | |
Observation data ( J2000 epoch) | |
Constellation | Coma Berenices |
Right ascension | 12h 24m 11.2s [1] |
Declination | 31° 31′ 19″ [1] |
Redshift | 0.004179 [1] |
Heliocentric radial velocity | 1253 km/s [1] |
Distance | 56.21 Mly (17.233 Mpc) [1] |
Group or cluster | Coma I (NGC 4274 subgroup) |
Apparent magnitude (V) | 13.6 [1] |
Characteristics | |
Type | SB(rs)c?+ [1] |
Size | ~27,100 ly (8.32 kpc) (estimated) [1] |
Apparent size (V) | 2.57 x 0.80 [1] |
Other designations | |
UGC 07483, PGC 040330, MCG +05-29-079 [1] |
NGC 4359 is a dwarf barred spiral galaxy [2] [3] seen edge-on that is about 56 million light-years away [4] in the constellation Coma Berenices. It was discovered by astronomer William Herschel on March 20, 1787. [5] It is a member of the NGC 4274 Group, [6] [7] which is part of the Coma I Group [6] [7] or Cloud. [8]
On the sky, NGC 4359 appears to lie closest to the flocculent spiral NGC 4414 [9] which is also a member of the NGC 4274 Group [7] and the Coma I cloud. [8] However, their radial velocities differ by around 500 km/s suggesting an interaction between the two is unlikely. [9]