NGC 6822
| NGC 6822 | |
|---|---|
 |
|
| Observation data (J2000 epoch) | |
| Constellation | Sagittarius |
| Right ascension | 19h 44m 56.6s[1] |
| Declination | −14° 47′ 21″[1] |
| Redshift | -57 ± 2 km/s[1] |
| Distance | 1.63 ± 0.03 Mly (500 ± 10 kpc)[2][3][4] |
| Type | IB(s)m[1] |
| Apparent dimensions (V) | 15′.5 × 13′.5[1] |
| Apparent magnitude (V) | 9.3[1] |
| Other designations | |
| Barnard's Galaxy,[1] IC 4895,[1] DDO 209,[1] PGC 63616,[1] Caldwell 57 |
|
NGC 6822 (also known as Barnard's Galaxy, IC 4895, or Caldwell 57) is a barred irregular galaxy approximately 1.6 million light-years away in the constellation Sagittarius. Part of the Local Group of galaxies, it was discovered by E. E. Barnard in 1884 (hence its name), with a six-inch refractor telescope. It is one of the closer galaxies to the Milky Way. It is similar in structure and composition to the Small Magellanic Cloud. It is about 7,000 light-years in diameter.[5]
Observational history
Edwin Hubble wrote the seminal paper N.G.C. 6822, A Remote Stellar System (Hubble 1925) wherein he identified 15 variable stars (11 of which were Cepheids). He also surveyed the galaxy's stars distribution down to magnitude 19.4. He provided spectral characteristics, luminosities and dimensions for the five brightest "diffuse nebulae" (giant H II regions) that included the Bubble Nebula and the Ring Nebula. He also computed the absolute magnitude of the entire galaxy.
Hubble's detection of eleven Cepheid variable stars was a milestone in astronomy. Utilizing the Cepheid Period-Luminosity relationship, Hubble determined a distance of more than 700,000 light-years. This was the first system beyond the Magellanic Clouds to have its distance accurately determined. (Hubble continued this process with the Andromeda Galaxy and the Triangulum Galaxy). His distance to the galaxy was way beyond Harlow Shapley's value of 300,000 light-years for the size of universe. In this paper, Hubble concluded the "Great Debate" of 1920 between Heber Curtis and Shapley over the scale of the universe and the nature of the "spiral nebula". It soon became evident that all spiral nebulae were in fact spiral galaxies far outside our own Milky Way.
In 1977, Paul W. Hodge extended the list of known H II regions in Barnard to 16. Today, there are over 150 of these regions cataloged in Barnard's Galaxy.
Gallery
-
NGC 6822 GALEX WikiSky.jpg
NGC 6822 in ultraviolet by GALEX.
-
0101a.jpg
"Star-Forming Region" in NGC 6822.
-
Region of NGC 6822.jpg
"A Giant Star Factory" in NGC 6822.
-
Barnard's Galaxy.jpg
NGC 6822 from ESO's Wide Field Imager.
See also
 |
Wikimedia Commons has media related to NGC 6822. |
- Bubble Nebula (NGC 6822)
- Ring Nebula (NGC 6822)
- Large Magellanic Cloud - another irregular galaxy within the Local Group
- Small Magellanic Cloud - another irregular galaxy within the Local Group
Notes
- ↑ 1.0 1.1 1.2 1.3 1.4 1.5 1.6 1.7 1.8 1.9 Lua error in package.lua at line 80: module 'strict' not found.
- ↑ Karachentsev et al. 2004
- ↑ Karachentsev & Kashibadze 2006
- ↑ Cannon et al. 2006
- ↑ NGC 6822: Barnard's Galaxy APOD , NASA , 8 February 2013
References
- Lua error in package.lua at line 80: module 'strict' not found.
- Lua error in package.lua at line 80: module 'strict' not found.
- Lua error in package.lua at line 80: module 'strict' not found.
- Lua error in package.lua at line 80: module 'strict' not found.
External links
- The Milky Way's Tiny but Tough Galactic Neighbour — ESO Press Release
- NGC 6822: Barnard's Galaxy
- NGC 6822 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images
Coordinates: 
19h 44m 56.6s, −14° 47′ 21″
| List |
|
|---|---|
| See also | |
