NGC 262

NGC 262
NGC 262 imaged by Legacy Surveys.
Observation data (J2000 epoch)
ConstellationAndromeda
Right ascension00h 48m 47.141479s
Declination+31° 57′ 25.0845702″
Redshift0.01466916±0.0005
Heliocentric radial velocity4,365±150 km/s
Galactocentric velocity4,397.7±150 km/s
Distance213.3 ± 15.00 Mly (65.4 ± 4.6 Mpc)h−1
0.6774

(Comoving)
200 Mly (61.32 Mpc)h−1
0.6774

(Light-travel)
Group or clusterNGC 315 Group
Apparent magnitude (V)13.06±0.19
Apparent magnitude (B)13.90±0.19
magnitude (J)11.240±0.033
magnitude (H)10.554±0.044
magnitude (K)10.097±0.047
Characteristics
TypeSA0/a?(s): Sy2
Size99,249 ly × 93,313 ly
(30.43 kpc × 28.61 kpc)
(diameter; 25.0 B-mag arcsec−2)
101,110 ly × 78,865 ly
(31.00 kpc × 24.18 kpc)
(diameter; "total" magnitude)
Apparent size (V)2.1′ × 1.9′
H I scale length (physical)400 kpc (1,300,000 ly)
Notable featuresSurrounded by a large H I disk
Other designations
IRAS 00461+3141, 2MASX J00484711+3157249, UGC 499, MCG +05-03-008, Mrk 348, PGC 2855, CGCG 501-020

NGC 262 (also known as Markarian 348) is a Seyfert 2 spiral galaxy located 65.4 megaparsecs (213 million light-years) away in the constellation Andromeda. It was discovered on 17 September 1885 by Lewis A. Swift.

NGC 262 was tidally disturbed by the gravitational forces of smaller galaxies, which resulted in a surrounding large cloud over 10 times larger than the Milky Way. It is also a member of the NGC 315 Group (also known as LGG 14), which contains 42 galaxies, including NGC 226, NGC 243, NGC 266, NGC 311, NGC 315, NGC 338, IC 43, IC 66, and IC 69, among others.