NGC 1569 | |
---|---|
Observation data (J2000 epoch) | |
Constellation | Camelopardalis |
Right ascension | 4h 30m 49.1s[1] |
Declination | +64° 50′ 53″[1] |
Redshift | -104 km/s[1] |
Distance | 10.96 ± 0.65 Mly (3.36 ± 0.20 Mpc[2]) |
Apparent magnitude (V) | 11.9[1] |
Characteristics | |
Type | IBm[1] |
Apparent size (V) | 3.6′ × 1.8′[1] |
Notable features | Contains two super star clusters |
Other designations | |
UGC 3056,[1] PGC 15345,[1] VII Zw 016,[1] Arp 210[1] |
NGC 1569 is a dwarf irregular galaxy in Camelopardalis. The galaxy is relatively nearby and consequently, the Hubble Space Telescope can easily resolve the stars within the galaxy.[3] The distance to the galaxy was previously believed to be only 2.4 Mpc (7.8 Mly).[4] However, in 2008 scientists studying images from Hubble calculated the galaxy's distance at nearly 11 million light-years away, about 4 million light-years farther than previously thought, meaning it is a member of the IC 342 group of galaxies.[2][5]
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