Fayl:M27 - Dumbbell Nebula.jpg — Vikipediya

Fayl:M27 - Dumbbell Nebula.jpg

Faylın orijinalı (2.044 × 2.042 piksel, fayl həcmi: 1,74 MB, MIME növü: image/jpeg)

İzah
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
.
Tarix
Mənbə http://www.eso.org/public/images/eso9846a/
Müəllif ESO
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təsvir edir

copyrighted ingilis

7 oktyabr 1998

media type ingilis

image/jpeg

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Tarix/VaxtMiniatürÖlçülərİstifadəçiŞərh
hal-hazırkı18:14, 25 avqust 202218:14, 25 avqust 2022 tarixindəki versiyanın miniatür görüntüsü2.044 × 2.042 (1,74 MB)Fabian RRRRfrom the actual source
08:34, 2 mart 201008:34, 2 mart 2010 tarixindəki versiyanın miniatür görüntüsü4.961 × 5.004 (3,04 MB)TryphonHigher resolution, from http://www.eso.org/public/archives/images/large/eso9846a.jpg.
09:02, 18 sentyabr 200809:02, 18 sentyabr 2008 tarixindəki versiyanın miniatür görüntüsü3.966 × 4.000 (849 KB)Lars Lindberg Christensen{{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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