File:N103B from the Hubble.jpg

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DescriptionN103B from the Hubble.jpg	English: This image, taken with the NASA/ESA Hubble Space Telescope, shows the supernova remnant SNR 0509-68.7, also known as N103B (top of the image). N103B was a Type Ia supernova, located in the Large Magellanic Cloud— a neighbouring galaxy of the Milky Way. Owing to its relative proximity to Earth, astronomers observe the remnant to search for a potential stellar survivor of the explosion. The orange-red filaments visible in the image show the shock fronts of the supernova explosion. These filaments allow astronomers to calculate the original centre of the explosion. The filaments also show that the explosion is no longer expanding as a sphere, but is elliptical in shape. Astronomers assume that part of material ejected by the explosion hit a denser cloud of interstellar material, which slowed its speed. The shell of expanding material being open to one side supports this idea. The gas in the lower half of the image and the dense concentration of stars in the lower left are the outskirts of the star cluster NGC 1850, which has been observed by Hubble in the past [heic0108].
Date	30 March 2017, 16:00:00
Source	NASA/ESA Hubble
Author	NASA/Hubble

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current	14:47, 24 April 2024		1,280 × 1,246 (679 KB)	MemeGod27	Uploaded a work by NASA/Hubble from NASA/ESA Hubble with UploadWizard

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N103B

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Date and time of data generation	16:00, 30 March 2017
Credit/Provider	ESA/Hubble, NASA
Source	ESA/Hubble
Short title	Supernova remnant N103B
Image title	This image, taken with the NASA/ESA Hubble Space Telescope, shows the supernova remnant SNR 0509-68.7, also known as N103B (top of the image). N103B was a Type Ia supernova, located in the Large Magellanic Cloud— a neighbouring galaxy of the Milky Way. Owing to its relative proximity to Earth, astronomers observe the remnant to search for a potential stellar survivor of the explosion. The orange-red filaments visible in the image show the shock fronts of the supernova explosion. These filaments allow astronomers to calculate the original centre of the explosion. The filaments also show that the explosion is no longer expanding as a sphere, but is elliptical in shape. Astronomers assume that part of material ejected by the explosion hit a denser cloud of interstellar material, which slowed its speed. The shell of expanding material being open to one side supports this idea. The gas in the lower half of the image and the dense concentration of stars in the lower left are the outskirts of the star cluster NGC 1850, which has been observed by Hubble in the past [heic0108].
Usage terms	Creative Commons Attribution 4.0 International License
Horizontal resolution	72 dpi
Vertical resolution	72 dpi
Y and C positioning	Centered
Exif version	2.21
Meaning of each component	Y Cb Cr does not exist
Supported Flashpix version	1
Color space	sRGB
Scene capture type	Standard
Keywords	SNR 0509-68.7
Contact information	http://www.spacetelescope.org Karl-Schwarzschild-Strasse 2 Garching bei München, , D-85748 Germany
IIM version	4

File:N103B from the Hubble.jpg

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