NGC 262 (also known as Markarian 348) is a huge spiral galaxy in the cluster LGG 14.[1] It is a Seyfert 2 spiral galaxy located 287 million light years away in the constellation Andromeda.[2] It was discovered on September 17, 1885 by Lewis A. Swift.

NGC 262
NGC 262 as imaged by the SDSS.
Observation data (J2000 epoch)
Constellation	Andromeda
Right ascension	00h 48m 47.14154s[1]
Declination	+31° 57′ 25.08″[1]
Distance	287 million light-years (88 Mpc)[2]
Apparent magnitude (V)	13.1
Characteristics
Type	S0a
Apparent size (V)	1,1' × 1,1'
Other designations
2MASX J00484711+3157249, UGC 499, Markarian 348 [1]

Size

This galaxy has an apparent diameter of 1.1' of the Earth's sky.[3] It holds approximately 15 trillion stars.^{[citation needed]} [NGC 262] was tidally disturbed by the gravitational forces of smaller galaxies, which resulted in its large size.[3]

NGC 262 is very unusual, since it is 10 times larger than a regular spiral galaxy of its type.[2] According to Morris and Wannier, NGC 262 is surrounded by a huge cloud of neutral hydrogen[2] that is probably caused by the tidal stripping of smaller galaxies. The cloud has an apparent mass of approximately 50 billion solar masses[2] at a distance of 88 kiloparsecs (287,000 light-years)[2] from the nucleus of NGC 262 and extending up to 300 kiloparsecs (1 million light-years) away.[2] The cloud is spiral shaped with at least one arm, and possibly another one extending throughout the galaxy.

References

External links

• Media related to NGC 262 at Wikimedia Commons

This lenticular galaxy article is a stub. You can help Wikipedia by expanding it.

• v
• t
• e

На других языках

[de] NGC 262

[ru] NGC 262