NGC 207

NGC 207 is a spiral galaxy roughly 178 million light-years from the Solar System[2] in the constellation Cetus. It was discovered on December 7, 1857, by R. J. Mitchell.[3]

NGC 207
Observation data (J2000 epoch)
Constellation	Cetus
Right ascension	00^h 39^m 40.7^s[1]
Declination	−14° 14′ 13″[1]
Redshift	0.013276[1]
Distance	178 Mly[2]
Apparent magnitude (V)	14.59[1]
Characteristics
Apparent size (V)	0.6' × 0.3'[1]
Other designations
MCG -03-02-035, 2MASX J00394071-1414134, IRAS 00371+1430, F00371+1430, 6dF J0039407-141414, PGC 2395.[1]

See also

• List of NGC objects (1–1000)

References

1. "NASA/IPAC Extragalactic Database". Results for NGC 0207. Retrieved 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. "New General Catalog Objects: NGC 200 - 249". Cseligman. Retrieved September 11, 2016.

External links

• NGC 207 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images
• SEDS