NGC 207 explained
NGC 207 |
Epoch: | J2000 |
Ra: | [1] |
Constellation Name: | Cetus |
Z: | 0.013276 |
Dist Ly: | 178 Mly[2] |
Type: | Sc |
Appmag V: | 14.59 |
Size V: | 0.6' × 0.3' |
Names: | MCG -03-02-035, 2MASX J00394071-1414134, IRAS 00371+1430, F00371+1430, 6dF J0039407-141414, PGC 2395. |
Upright: | 1.35 |
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]
See also
External links
Notes and References
- Web site: NASA/IPAC Extragalactic Database . Results for NGC 0207 . 2016-09-02.
- An object's distance from Earth can be determined using Hubble's law: v=Ho 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=Ho
- Web site: New General Catalog Objects: NGC 200 - 249. Cseligman. September 11, 2016.