File:M27 - Dumbbell Nebula.jpg

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English: The Dumbbell Nebula

The Dumbbell Nebula ­— also known as Messier 27 or NGC 6853 — is a typical planetary nebula and is located in the constellation Vulpecula (The Fox). The distance is rather uncertain, but is believed to be around 1,200 light-years. It was first described by the French astronomer and comet hunter Charles Messier who found it in 1764 and included it as no. 27 in his famous list of extended sky objects [2] .Despite its class, the Dumbbell Nebula has nothing to do with planets. It consists of very rarified gas that has been ejected from the hot central star (well visible on this photo), now in one of the last evolutionary stages. The gas atoms in the nebula are excited (heated) by the intense ultraviolet radiation from this star and emit strongly at specific wavelengths.

This image is the beautiful by-product of a technical test of some FORS1 narrow-band optical interference filtres. They only allow light in a small wavelength range to pass and are used to isolate emissions from particular atoms and ions. In this three-colour composite, a short exposure was first made through a wide-band filtre registering blue light from the nebula. It was then combined with exposures through two interference filtres in the light of double-ionized oxygen atoms and atomic hydrogen. They were colour-coded as “blue”, “green” and “red”, respectively, and then combined to produce this picture that shows the structure of the nebula in “approximately true” colours.

They are three-colour composite based on two interference ([OIII] at 501 nm and 6 nm FWHM — 5 min exposure time; H-alpha at 656 nm and 6 nm FWHM — 5 min) and one broadband (Bessell B at 429 nm and 88 nm FWHM; 30 sec) filtre images, obtained on September 28, 1998, during mediocre seeing conditions (0.8 arcsec). The CCD camera has 2048 x 2048 pixels, each covering 24 x 24 µm and the sky fields shown measure 6.8 x 6.8 arcminutes and 3.5 x 3.9 arcminutes, respectively. North is up; East is left.

Credit:

ESO/I. Appenzeller, W. Seifert, O. Stahl, M. Zamani

Coordinates
Position (RA):  	19 59 36.41
Position (Dec): 	22° 43' 16.00"
Field of view:  	6.76 x 6.82 arcminutes
Orientation:    	North is 0.0° left of vertical
Colours & filters
Band            	Wavelength	Telescope
Optical u       	361 nm   	Very Large Telescope FORS1
Optical B       	429 nm   	Very Large Telescope FORS1
Optical Oiii    	501 nm   	Very Large Telescope FORS1
Optical HeII    	472 nm   	Very Large Telescope FORS1
Optical R       	655 nm   	Very Large Telescope FORS1
Optical H-alpha 	656 nm   g	Very Large Telescope FORS1
.
日期
来源 http://www.eso.org/public/images/eso9846a/
作者 ESO
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当前2022年8月25日 (四) 18:142022年8月25日 (四) 18:14版本的缩略图2,044 × 2,042(1.74 MB)Fabian RRRR留言 | 贡献from the actual source
2010年3月2日 (二) 08:342010年3月2日 (二) 08:34版本的缩略图4,961 × 5,004(3.04 MB)Tryphon留言 | 贡献Higher resolution, from http://www.eso.org/public/archives/images/large/eso9846a.jpg.
2008年9月18日 (四) 09:022008年9月18日 (四) 09:02版本的缩略图3,966 × 4,000(849 KB)Lars Lindberg Christensen留言 | 贡献{{Information |Description={{en|1=The Dumbbell Nebula - also known as Messier 27 or NGC 6853 - is a typical planetary nebula and is located in the constellation Vulpecula (The Fox). The distance is rather uncertain, but is believed to be around 1200 light

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