Difference between revisions of "Omega nebula"
m (Wikify) |
(Expand infobox) |
||
| Line 1: | Line 1: | ||
{{Night Sky | {{Night Sky | ||
| image = | | image = | ||
| − | | designation =[[Messier catalogue|Messier 17]] | + | | designation =[[Messier catalogue|Messier 17]]<br/>[[NGC]] 6618 |
| − | [[NGC]] 6618 | + | | rightascension =18<sup>h</sup> 20<sup>m</sup> 26<sup>s</sup><ref name=messier-objects>[http://www.messier-objects.com/messier-17-omega-nebula/ Omega nebula] from messier-objects.com</ref> |
| − | | rightascension =18<sup>h</sup> 20<sup>m</sup> 26<sup>s</sup> | + | | declination =-16° 10′ 36″<ref name=messier-objects/> |
| − | | declination =-16° 10′ 36″ | + | | distance =5,000-6,000 ly<ref name=messier-objects/> |
| − | | distance =5,000-6,000 ly | ||
| constellation =[[Sagittarius]] | | constellation =[[Sagittarius]] | ||
| type =[[Emission nebula]] | | type =[[Emission nebula]] | ||
| − | | dimensions = | + | | dimensions = 20x15'<ref>[http://www.constellation-guide.com/omega-nebula-messier-17/ Omega nebula - M17] from constellation-guide.com</ref> |
| − | | magnitude = 6.0 | + | | magnitude =Apparent Mag: +6.0<ref name=messier-objects/><br/>Absolute Mag: -5.1<ref>From definition of absolute magnitude, using apparent magnitude given here and midway distance value, 5,500 ly.</ref> |
| − | | redshift = | + | | redshift =-0.000149±0.000002<ref name=simbad>[http://simbad.u-strasbg.fr/simbad/sim-id?Ident=m17&NbIdent=1&Radius=2&Radius.unit=arcmin&submit=submit+id NGC 6618] from simbad.u-strasbg.fr</ref> |
| − | | radvelocity = | + | | radvelocity =-44.577±0.682 km/s<ref name=simbad/> |
| − | | propmotion = | + | | propmotion =RA: 1.79 mas/yr<ref name=simbad/><br/>Dec.: -1.96 mas/yr<ref name=simbad/> |
| parallax = | | parallax = | ||
}} | }} | ||
| Line 18: | Line 17: | ||
==History== | ==History== | ||
| − | The first observation of the Omega nebula was made in 1745 by Jean-Philippe Loys de Chéseaux.<ref name=seds/> It was independently discovered by [[Charles Messier]] on 3<sup>rd</sup> June 1764.<ref name=messier-objects | + | The first observation of the Omega nebula was made in 1745 by Jean-Philippe Loys de Chéseaux.<ref name=seds/> It was independently discovered by [[Charles Messier]] on 3<sup>rd</sup> June 1764.<ref name=messier-objects/> [[William Herschel]]'s son, John, first noticed its resemblence to the letter omega. Admiral William Henry Smyth decided it appeared like a horseshoe and named it so in 1836.<ref name=messier-objects/> |
==Properties and Structure== | ==Properties and Structure== | ||
Revision as of 13:29, January 3, 2018
| Omega nebula | |
|---|---|
| Observational Data | |
| Designation | Messier 17 NGC 6618 |
| Right ascension | 18h 20m 26s[1] |
| Declination | -16° 10′ 36″[1] |
| Constellation | [[Sagittarius]] |
| Type of object | [[Emission nebula]] |
| Dimensions | 20x15'[2] |
| Magnitude | Apparent Mag: +6.0[1] Absolute Mag: -5.1[3] |
| Redshift | -0.000149±0.000002[4] |
| Astrometry | |
| Distance from Earth | 5,000-6,000 ly[1] |
| Radial velocity | -44.577±0.682 km/s[4] |
| Proper motion | RA: 1.79 mas/yr[4] Dec.: -1.96 mas/yr[4] |
The Omega nebula (M17, NGC 6618) is famous an emission nebula in the constellation of Sagittarius.[5] Sometimes called the Swan nebula, the Horseshoe nebula or the Lobster nebula, it is named for its resemblance to the Greek letter omega, Ω. Like many emission nebulae, it is illuminated by a star cluster within the nebula but unlike most nebulae, the nebulae obscures these stars in the visible. It is found not far from the Trifid nebula, the lagoon nebula and the Eagle nebula.
History
The first observation of the Omega nebula was made in 1745 by Jean-Philippe Loys de Chéseaux.[5] It was independently discovered by Charles Messier on 3rd June 1764.[1] William Herschel's son, John, first noticed its resemblence to the letter omega. Admiral William Henry Smyth decided it appeared like a horseshoe and named it so in 1836.[1]
Properties and Structure
The nebula has a diameter of 15 light years and is part of a larger cloud that is at least 40 light years across.[1] One of the larger H II (cloud of ionized hydrogen) in the galaxy, it is believed to have a mass of 800 solar masses. The open cluster housed within the nebula of 35 stars which illuminate the cloud. The nebula itself contains at least 800 stars. The gas an dust present in the the nebula prevent event the brightest of these stars being visible.
References
- ↑ 1.0 1.1 1.2 1.3 1.4 1.5 1.6 Omega nebula from messier-objects.com
- ↑ Omega nebula - M17 from constellation-guide.com
- ↑ From definition of absolute magnitude, using apparent magnitude given here and midway distance value, 5,500 ly.
- ↑ 4.0 4.1 4.2 4.3 NGC 6618 from simbad.u-strasbg.fr
- ↑ 5.0 5.1 M17 from messier.seds.org