NGC 6946 | |
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Spiral galaxy NGC 6946
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Observation data (J2000 epoch) | |
Constellation | Cepheus & Cygnus |
Right ascension | 20h 34m 52.3s |
Declination | +60° 09′ 14″ |
Redshift | 0.000160 |
Helio radial velocity | 48 ± 2 km/s |
Distance | 22.5 ± 7.8 Mly (6.9 ± 2.4 Mpc) |
Apparent magnitude (V) | +9.6 |
Characteristics | |
Type | SAB(rs)cd |
Apparent size (V) | 11.5 x 9.8 arcmin |
Other designations | |
UGC 11597, PGC 65001, Arp 29,Caldwell 12 | |
NGC 6946 (also tentatively known as the Fireworks Galaxy) is an intermediate spiral galaxy about 22 million light-years away, in the constellations of Cepheus and Cygnus. It was discovered by William Herschel on 9 September 1798. NGC 6946 is highly obscured by interstellar matter of the Milky Way galaxy, as it is quite close to the galactic plane. The true diameter of the galaxy is approximately 40,000 light-years or just about one-third of the Milky Way's size. In the past century, ten supernovae have been observed to explode in the arms of this galaxy, which has been classified as a starburst galaxy. Chandra Space Telescope observations have revealed three of the oldest supernovae ever detected in X-rays. This composite image also includes optical data from the Gemini Observatory in red, yellow, and cyan.
Ten supernovae have been observed in NGC 6946 in the last 100 years: SN 1917A, SN 1939C, SN 1948B, SN 1968D, SN 1969P, SN 1980K, SN 2002hh, SN 2004et, SN 2008S, and SN 2017eaw. This makes it the most prolific known galaxy for this type of event over a period of 100 years. By comparison, the Milky Way galaxy, which has double the number of stars as NGC 6946, averages one supernova event per century. It also contains a failed supernova, potential black hole-forming star N6946-BH1.
Coordinates: 20h 34m 52.3s, +60° 09′ 14″