|H II region|
The Rosette Nebula (H-Alpha + RGB)
|Observation data: J2000.0 epoch|
|Right ascension||06h 33m 45s|
|Declination||+04° 59′ 54″|
|Distance||5,200 ly (1,600 pc)|
|Apparent magnitude (V)||9.0|
|Apparent dimensions (V)||1.3 °|
|Notable features||Multipart nebula|
|Designations||SH 2-275, CTB 21, Caldwell 49|
The Rosette Nebula (also known as Caldwell 49) is a large, circular H II region located near one end of a giant molecular cloud in the Monoceros region of the Milky Way Galaxy. The open cluster NGC 2244 (Caldwell 50) is closely associated with the nebulosity, the stars of the cluster having been formed from the nebula's matter.
The complex has the following NGC designations:
- NGC 2237 – Part of the nebulous region (Also used to denote whole nebula)
- NGC 2238 – Part of the nebulous region
- NGC 2239 – Part of the nebulous region (Discovered by John Herschel)
- NGC 2244 – The open cluster within the nebula (Discovered by John Flamsteed in 1690)
- NGC 2246 – Part of the nebulous region
The cluster and nebula lie at a distance of some 5,000 light-years from Earth ) and measure roughly 50 light years in diameter. The radiation from the young stars excites the atoms in the nebula, causing them to emit radiation themselves producing the emission nebula we see. The mass of the nebula is estimated to be around 10,000 solar masses.
It is believed that stellar winds from a group of O and B stars are exerting pressure on interstellar clouds to cause compression, followed by star formation in the nebula. This star formation is currently still ongoing.
A survey of the nebula with the Chandra X-ray Observatory in 2001 has revealed the presence of very hot, young stars at the core of the Rosette Nebula. These stars have heated the surrounding gas to a temperature in the order of 6 million kelvins causing them to emit copious amounts of X-rays.
Observing the Rosette Nebula
The cluster of stars is visible in binoculars and quite well seen in small telescopes while the nebula itself is more difficult to spot visually and requires a telescope with a low magnification. A dark site is a must to see it. Photographically the Rosette Nebula is easier to record and it is the only way to record the red color which is not seen visually.
It is believed by Islamic Scholars that this star points to a verse in Holy Qur'an which is " Then when the heaven is rent asunder, and it becomes rosy or red like red-oil, or red hide " (Ar Rahman, 37).
- "SIMBAD Astronomical Database". Results for NGC 2237. Retrieved 2006-10-23.
- Phelps, Randy L.; Ybarra, Jason E. (2005). "A Parsec-Scale Outflow in the Rosette Molecular Cloud?". The Astrophysical Journal 627 (2): 845–849. Bibcode:2005ApJ...627..845P. doi:10.1086/430431.
- 'Cambridge Deep Sky Companions - The Caldwell Objects' , S.J. O'Meara & P. Moore, Cambridge University Press, ISBN 0-521-82796-5 (2002)
|Wikimedia Commons has media related to Rosette Nebula.|
- Rosette Nebula (SEDS)
- Chandra Observatory study of the Rosette Nebula
- NOAO; "Fitful Young Star Sputters to Maturity in the Rosette Nebula"
- NightSkyInfo.com – Rosette Nebula
- Astronomy Picture of the Day
- Slooh Videocast on Rosette Nebula
- Rosette Nebula from the Netherlands
- Deep image of the Rosette Nebula
- The Scale of the Universe (Astronomy Picture of the Day 2012 March 12)
- Rosette Nebula on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images
- Rosette Nebula at Constellation Guide