NGC 226 explained

NGC 226
Caption:	SDSS image of NGC 226
Epoch:	J2000
Ra:	^[1]
Constellation Name:	Andromeda
Group Cluster:	NGC 315 Group
Z:	0.016094
Dist Ly:	216 Mly^[2]
Type:	S
Appmag V:	14.31
Size V:	0.9' × 0.9'
Names:	UGC 00459, CGCG 500-076, 2MASX J00425403+3234516, 2MASXi J0042540+323451, IRAS 00402+3218, F00401+3218, PGC 2572.

NGC 226 is a spiral galaxy located approximately 216 million light-years from the Sun^[2] in the constellation Andromeda. It was discovered on December 21, 1786, by William Herschel.^[3]

According to A.M. Garcia, NGC 226 is a member of the NGC 315 Group (also known as LGG 14). This group contains 42 galaxies, including NGC 243, NGC 262, NGC 266, NGC 311, NGC 315, NGC 338, IC 43, IC 66, AND IC 69, among others.^[4]

See also

• • Spiral galaxy List of NGC objects (1–1000)
• Andromeda (constellation)

External links

• • • SEDS

Notes and References

1. Web site: NASA/IPAC Extragalactic Database . Results for NGC 0226 . 2016-09-02.
2. An object's distance from Earth can be determined using Hubble's law: v=H_o is Hubble's constant (70±5 (km/s)/Mpc). The relative uncertainty Δd/d divided by the distance is equal to the sum of the relative uncertainties of the velocity and v=H_o
3. Web site: New General Catalog Objects: NGC 200 - 249. Cseligman. September 10, 2016.
4. 1993A&AS..100...47G . General study of group membership. II. Determination of nearby groups . Garcia . A. M. . Astronomy and Astrophysics Supplement Series . 1993 . 100 . 47.