IC 1101 | |
---|---|
Observation data (J2000 epoch) | |
Constellation | Virgo |
Right ascension | 15h 10m 56.1s[1] |
Declination | +05° 44′ 41″[1] |
Redshift | 0.078054±0.000027[1][2] |
Heliocentric radial velocity | 22,419 km/s (13,931 mi/s)[1] |
Distance | 354.0 ± 24.8 Mpc (1,154.6 ± 80.9 million ly)h−1 0.67[1] |
Group or cluster | Abell 2029 |
Apparent magnitude (V) | 13.22[1] |
Characteristics | |
Type | cD; S0-[1] |
Size | 123.65 to 169.61 kpc (403,300 to 553,200 ly) (D25 B-band and total K-band isophotes)[3][4][a] |
Apparent size (V) | 1'.2 × 0'.6[1] |
Other designations | |
UGC 9752,[1] PGC 54167,[1] A2029-BCG[1] |
IC 1101 is a class S0 supergiant (cD) lenticular galaxy at the center of the Abell 2029 galaxy cluster. It has an isophotal diameter at about 123.65 to 169.61 kiloparsecs (400,000 to 550,000 light-years). It possesses a diffuse core which is the largest known core of any galaxy to date,[5] and contains a supermassive black hole, one of the largest discovered.[5] IC 1101 is located at 354.0 megaparsecs (1.15 billion light-years) from Earth. It was discovered on 19 June 1790, by the British astronomer William Herschel.[6]
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