UGC 9405 explained
UGC 9405 |
Credit: | ESA/Hubble & NASA |
Epoch: | J2000 |
Constellation Name: | Ursa Major |
Ra: | [1] |
Z: | 0.000741[2] |
H Radial V: | 222 ± 7 km/s |
Dist Ly: | [3] |
Type: | I |
Appmag V: | 14.08[4] |
Appmag B: | 15.39 |
UGC 9405 (also known as PGC 52142) is a faint dwarf irregular galaxy situated in the constellation of Ursa Major. It is about 20.5 million light-years, or 6.3 megaparsecs, away from the Earth.[3] It is listed as a member of the M101 Group, a group containing the several galaxies orbiting the largest, Pinwheel Galaxy (M101).[5] However, due to its far distance from the Pinwheel Galaxy, its membership of the group is uncertain.[3]
Notes and References
- VizieR Online Data Catalog: The SDSS Photometric Catalog, Release 7. Adelman-McCarthy, J. K.. etal. VizieR On-line Data Catalog. 2009. 2009yCat.2294....0A.
- UGC 9405. 2021-03-19.
- 10.3847/2041-8213/ab24d2. 1901.07578. 2019ApJ...878L..16C. Using Surface Brightness Fluctuations to Study nearby Satellite Galaxy Systems: The Complete Satellite System of M101. 2019. Carlsten. Scott G.. Beaton. Rachael L.. Greco. Johnny P.. Greene. Jenny E.. The Astrophysical Journal. 878. 1. L16. 119089770 . free .
- Web site: Search specification: UGC 9405. HyperLeda. Université Claude Bernard Lyon 1. 2021-03-19.
- Web site: The M101 group of galaxies. www.messier.seds.org. 2020-04-26.