Berkas:M83 - Southern Pinwheel.jpg

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Deskripsi
English: Spiral galaxy Messier 83*

This dramatic image of the galaxy Messier 83 was captured by the Wide Field Imager at ESO's La Silla Observatory, located high in the dry desert mountains of the Chilean Atacama Desert. Messier 83 lies roughly 15 million light-years away towards the huge southern constellation of Hydra (the sea serpent). It stretches over 40 000 light-years, making it roughly 2.5 times smaller than our own Milky Way. However, in some respects, Messier 83 is quite similar to our own galaxy. Both the Milky Way and Messier 83 possess a bar across their galactic nucleus, the dense spherical conglomeration of stars seen at the centre of the galaxies.

Credit:

ESO

Coordinates
Position (RA):	13 37 0.91
Position (Dec):	-29° 51' 56.57"
Field of view:	17.59 x 17.59 arcminutes
Orientation:	North is 0.0° left of vertical
Colours & filters Band	Telescope
Optical B       	MPG/ESO 2.2-metre telescope WFI
Optical V       	MPG/ESO 2.2-metre telescope WFI
Optical R       	MPG/ESO 2.2-metre telescope WFI
.
Tanggal
Sumber https://www.eso.org/public/images/eso0825a/ https://cdn.eso.org/images/large/eso0825a.jpg
Pembuat (Credit) ESO
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Barred spiral galaxy, Messier 83

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2005

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Tanggal/WaktuMiniaturDimensiPenggunaKomentar
terkini24 November 2020 00.15Miniatur versi sejak 24 November 2020 00.154.432 × 4.432 (7 MB)Fabian RRRRSource: https://www.eso.org/public/images/eso0825a/ https://cdn.eso.org/images/large/eso0825a.jpg
18 September 2008 15.02Miniatur versi sejak 18 September 2008 15.023.750 × 3.746 (14,69 MB)Lars Lindberg Christensen{{Information |Description= |Source= |Date= |Author= |Permission= |other_versions= }}
18 September 2008 11.13Miniatur versi sejak 18 September 2008 11.131.381 × 1.380 (833 KB)Lars Lindberg Christensen{{Information |Description={{en|1=If our Milky Way were to resemble this one, we certainly would be proud of our home! The beautiful spiral galaxy Messier 83 [4] is located in the southern constellation Hydra (the Water Snake) and is also known as NGC 523

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