NGC 101 explained
NGC 101 |
Epoch: | J2000 |
Constellation Name: | Sculptor |
Dec: | [1] |
Z: | 0.011284 |
H Radial V: | 3383 |
Dist Ly: | [2] |
Type: | SAB(rs)cd: |
Size: | [3] |
Appmag V: | 12.84 |
Appmag B: | 13.36[4] |
Size V: | 2.2 × 2.0 |
Names: | MGC-05-02-003, PGC 1518 |
NGC 101 is a spiral galaxy estimated to be about 150 million light-years away in the constellation of Sculptor. It was discovered by John Herschel in 1834 and its magnitude is 12.8.[5] It is a member of the Southern Supercluster (also called the Laniakea Supercluster) the closest galaxy supercluster to the Local Supercluster.[6]
Notes and References
- Web site: NED results for object NGC 0101. National Aeronautics and Space Administration / Infrared Processing and Analysis Center. 11 March 2017.
- Star Formation in the Nearby Universe: The Ultraviolet and Infrared Points of View. Iglesias-Páramo, J.. etal. The Astrophysical Journal Supplement Series. 164. 1. 38–51. 2006. 2006ApJS..164...38I. 10.1086/502628. astro-ph/0601235. 17135800.
- [2MASS]
- NGC 101. 11 March 2017.
- Web site: NGC Objects: NGC 100 - 149.
- Shyamal . The Southern Supercluster . Astronomical Journal . October 1989 . 98 . 1175–1187 . 10.1086/115205 . 1989AJ.....98.1175M . 19 November 2020. free .