UGC 6697 | |
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![]() Hubble Space Telescope Image of UGC 6697 | |
Observation data (J2000 epoch) | |
Constellation | Leo |
Right ascension | 11h 43m 49.07s |
Declination | +19d 58m 06.40s |
Redshift | 0.022432 |
Heliocentric radial velocity | 6,717 km/s |
Distance | 378 Mly (115.8 Mpc) |
Group or cluster | Leo Cluster |
Apparent magnitude (V) | 13.59 |
Characteristics | |
Type | Im, HII, Sbrst |
Size | 205,000 y |
Apparent size (V) | 1.9' x 0.3' |
Other designations | |
PGC 36466, CGCG 097-087, MCG +03-30-066, 2MFGC 09207, WBL 353-022, SDSS J114349.07+195806.4, IRAS F11412+2014, 2CXO J114349.1-195807, 2XMM J114349.2+195804, ABELL 1367:[BFG83] 08, 2MASX J11434911+1958063, ECO 02995, NSA 140139, UITBOC 1673, LEDA 36466 |
UGC 6697 is a large irregular[1] spiral galaxy with a bar[2] located in the Leo constellation.[3] It is located 378 million light-years from the Solar System and has an estimated diameter of 205,000 light-years.[4] UGC 6697 is considered a starburst galaxy which produces high rates of star formation.[4][5] The first known reference to this galaxy comes from volume II of the Catalogue of Galaxies and of Clusters of Galaxies compiled by Fritz Zwicky in 1968, where it was listed as CGCG 097-087, and its coordinates listed as 1141.2 + 2015 (epoch B1950).[6]