NGC 1003 | |
---|---|
Observation data (J2000[1] epoch) | |
Constellation | Perseus |
Right ascension | 02h 39m 16.893s[2] |
Declination | +40° 52′ 20.25″[2] |
Redshift | 0.002090[3] |
Heliocentric radial velocity | 624 km/s[4] |
Distance | 35.9 kly (11.02 kpc)[4] |
Group or cluster | NGC 1023 group[5] |
Apparent magnitude (B) | 12.1[3] |
Characteristics | |
Type | SAcd[6] |
Mass | 299+28 −26×1010[7] M☉ |
Mass/Light ratio | 0.70+0.16 −0.15[7] M☉/L☉ |
Notable features | Warped disk[6] |
Other designations | |
NGC 1003, UGC 2137, MCG +07-06-051, PGC 10052[3] |
NGC 1003 is a spiral galaxy at the western edge of the Perseus constellation.[8] It is located at a distance of about 36 million light years from the Milky Way and is receding with a heliocentric radial velocity of 624 km/s.[4] This galaxy was discovered by the Anglo-German astronomer William Herschel on October 6, 1784, who described it as "pretty faint, large, extended 90°±, much brighter middle, mottled but not resolved".[9] It is a member of the NGC 1023 group of galaxies.[5]
The morphological class of NGC 1003 is SAcd, which means it is an unbarred spiral galaxy (SA) with somewhat loosely-wound spiral arms (cd). It is inclined by an angle of 70° to the line of sight from the Earth, with the major axis aligned along a position angle of 276°. The visual disk of the galaxy shows a substantial warping in the eastern side, turning it almost face on. The estimated star formation rate is 0.40 M☉·yr−1.[6] It has a virial mass of 3×1012 M☉ and a mass-to-light ratio of 0.7.[7]
A type Ia supernova[10] was discovered in the galaxy by F. Zwicky in 1937,[11] and subsequently designated SN 1937D.
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