NGC 23 | |
---|---|
![]() NGC 23 by HST | |
Observation data (J 2000.0 epoch) | |
Constellation | Pegasus |
Right ascension | 00h 09m 53.411s[1] |
Declination | +25° 55′ 25.46″[1] |
Redshift | 0.015231[2] |
Heliocentric radial velocity | 4,568 km/s[3] |
Distance | 173.5 Mly (53.21 Mpc)[3] |
Apparent magnitude (V) | 11.9 mag |
Absolute magnitude (V) | -21.85 |
Characteristics | |
Type | SBb[4] |
Apparent size (V) | 1.9′ × 1.4′ |
Other designations | |
LEDA 698, UGC 89, Mrk 545, PGC 698, GC 9.[2][5] |
NGC 23 is a spiral galaxy located in the northern constellation of Pegasus, around 173.5 megalight-years distant from the Milky Way.[3] It was discovered by William Herschel on 10 September 1784. In the Webb Society Deep-Sky Observer's Handbook,[6] the visual appearance of NGC 23 is described as follows:
Bright, extended ellipse; a bright nuclear structure is noticeably elongated; two weak spiral enhancements emerge from opposite sides of the nucleus, one curving towards a bright star attached on the south end. The galaxy is likely interacting with NGC 9.
The shape of this galaxy is described by its morphological classification of SBb, which indicates it is a barred spiral (SB) with spiral arms that are moderately tightly wound (b).[4] It is a luminous infrared galaxy with star-forming clumps.[7]
Skrutskie2006
was invoked but never defined (see the help page).ned
was invoked but never defined (see the help page).tully2016
was invoked but never defined (see the help page).GarcíaLorenzo2015
was invoked but never defined (see the help page).SIMBAD
was invoked but never defined (see the help page).Webb
was invoked but never defined (see the help page).Larson2020
was invoked but never defined (see the help page).