NGC 6139
NGC 6139 is a globular cluster of the Milky Way in the constellation Scorpius. It is located 3.6 kiloparsecs (10 kilolight-years) from the Galactic Center[3] (less than half the distance of the Sun from the Galactic Center).
NGC 6139 | |
---|---|
![]() | |
Observation data (J2000 epoch) | |
Class | II[1] |
Constellation | Scorpius |
Right ascension | 16h 27m 41.6s[2] |
Declination | –38° 50′ 18″[2] |
Distance | 10.1 kiloparsecs (30 kilolight-years)[3] |
Apparent magnitude (V) | +9.68[4] |
Apparent dimensions (V) | 1′.6 x 1′.4[4] |
Physical characteristics | |
Visibility
The cluster appears visibly small and requires larger +12" aperture telescopes to view the core. Appearing around 1.5 arcmins having a radius of .75 arcmins, despite its rather bright magnitude.
Visibility
- Globular clusters are denser and more spherical than open star clusters.[5]
gollark: Great!
gollark: *Some* problems admit simple 100-line solutions, some really don't.
gollark: You can't just make programs arbitrarily small and so not require documentation.
gollark: As if I wrote a *manual*.
gollark: I agree. I simply remember how my code is structured, and everyone else can just reverse engineer it.
References
- "Results for NGC 6139". VizieR Catalogue Database. Retrieved 2013-09-06.
- "NED Results for NGC 6139". NASA/IPAC Extragalactic Database. Retrieved 2013-09-06.
- Harris, William E. (1996). "A Catalog of Parameters for Globular Clusters in the Milky Way (2010 edition)". Astronomical Journal. 112: 1487. doi:10.1086/118116.
- "NGC 6139". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2013-09-06.
- "An aging beauty". www.spacetelescope.org. Retrieved 25 June 2018.
This article is issued from Wikipedia. The text is licensed under Creative Commons - Attribution - Sharealike. Additional terms may apply for the media files.