IC 1101

IC 1101
June 1995 image of IC 1101 taken by the Hubble Space Telescope
Observation data (J2000 epoch)
ConstellationVirgo
Right ascension15h 10m 56.1s[1]
Declination+05° 44′ 41″[1]
Redshift0.078054±0.000027[1][2]
Heliocentric radial velocity22,419 km/s (13,931 mi/s)[1]
Distance354.0 ± 24.8 Mpc (1,154.6 ± 80.9 million ly)h−1
0.67
[1]
Group or clusterAbell 2029
Apparent magnitude (V)13.22[1]
Characteristics
TypecD; S0-[1]
Size123.65 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]
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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]

  1. ^ a b c d e f g h i j k "NED results for object IC 1101". NASA/IPAC Extragalactic Database. Retrieved 28 August 2022.
  2. ^ Cite error: The named reference Sohn was invoked but never defined (see the help page).
  3. ^ De Vaucouleurs, Gerard; De Vaucouleurs, Antoinette; Corwin, Herold G.; Buta, Ronald J.; Paturel, Georges; Fouque, Pascal (1991). Third Reference Catalogue of Bright Galaxies. Bibcode:1991rc3..book.....D.
  4. ^ "NASA/IPAC Extragalactic Database". Archived from the original on 15 August 2022. Retrieved 26 August 2022.
  5. ^ a b Cite error: The named reference Dullo2017 was invoked but never defined (see the help page).
  6. ^ "William Herschel's astronomical discoveries". MacTutor. University of St Andrews, Scotland. Retrieved 4 April 2020.


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