Rosette Nebula
From Wikipedia, the free encyclopedia
| Rosette Nebula | |
 The Rosette Nebula (H-Alpha) |
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| Observation data: J2000.0 epoch | |
|---|---|
| Type | Emission |
| Right ascension | 06h 33m 45s[1] |
| Declination | +04° 59′ 54″[1] |
| Distance | 5,200 ly (1,600 pc)[2] |
| Apparent magnitude (V) | 9.0 |
| Apparent dimensions (V) | 1.3 ° |
| Constellation | Monoceros |
| Physical characteristics | |
| Radius | 65 ly |
| Absolute magnitude (V) | - |
| Notable features | Multipart nebula |
| Other designations | SH 2-275[1], CTB 21[1] |
| See also: Diffuse nebula, Lists of nebulae | |
The Rosette Nebula 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 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 (Usually 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 5,200 light years from Earth (although estimates of the distance vary considerably) and measure roughly 130 light years in diameter. The radiation from the young stars excite 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.
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[edit] 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.
[edit] Other images
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 A close up view of the Rosette Nebula |
[edit] External links
- 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
[edit] References
- ^ a b c d SIMBAD Astronomical Database. Results for NGC 2237. Retrieved on 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. doi:.
