18 Mar

File:A loose spiral galaxy.jpg

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Revision as of 03:09, 18 March 2013
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{{Information--[[Special:Contributions/98.206.114.127|98.206.114.127]] 01:34, 11 January 2013 (UTC)--[[Special:Contributions/98.206.114.127|98.206.114.127]] 01:34, 11 January 2013 (UTC)''
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[[File:Milky Way|500px|thumbnail|As you can see the Milky Way has actually nine planets that nineth is Pluto and it has A big ball of gases thatburning which is the sunand thousands of Astroids]]
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|description={{en|1=The NASA/ESA Hubble Space Telescope has spotted the spiral galaxy ESO 499-G37, seen here against a backdrop of distant galaxies, scattered with nearby stars.
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''|description={{en|1=The NASA/ESA Hubble Space Telescope has spotted the spiral galaxy ESO 499-G37, seen here against a backdrop of distant galaxies, scattered with nearby stars.

The galaxy is viewed from an angle, allowing Hubble to reveal its spiral nature clearly. The faint, loose spiral arms can be distinguished as bluish features swirling around the galaxy’s nucleus. This blue tinge emanates from the hot, young stars located in the spiral arms. The arms of a spiral galaxy have large amounts of gas and dust, and are often areas where new stars are constantly forming.

The galaxy is viewed from an angle, allowing Hubble to reveal its spiral nature clearly. The faint, loose spiral arms can be distinguished as bluish features swirling around the galaxy’s nucleus. This blue tinge emanates from the hot, young stars located in the spiral arms. The arms of a spiral galaxy have large amounts of gas and dust, and are often areas where new stars are constantly forming.
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{{cc-by-3.0}}
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{{cc-by-3.0|ESA/Hubble & NASA}}

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