NGC 360
NGC 360 is a spiral galaxy located approximately 103 million light-years from the Solar System in the constellation Tucana. It was discovered on 2 November 1834 by John Herschel. Dreyer, creator of the New General Catalogue described the object as "extremely faint, very much extended 145°, very little brighter middle."
NGC 360 (2MASS)
See also
References
- ^ "NASA/IPAC Extragalactic Database". Results for NGC 0360. Retrieved September 2, 2016.
- ^ 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
- ^ "Revised NGC Data for NGC 360". spider.seds.org. Retrieved December 9, 2017.
- ^ "New General Catalog Objects: NGC 350 - 399". Cseligman. Retrieved November 19, 2016.
External links
Media related to NGC 360 at Wikimedia Commons- NGC 360 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images
- SEDS
| Stars |
| ||||||||||
|---|---|---|---|---|---|---|---|---|---|---|---|
| |||||||||||
| Star clusters |
| ||||||||||
| |||||||||||
| Galaxies |
| ||||||||||
 | This spiral galaxy article is a stub. You can help Wikipedia by expanding it. |