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Marseille Observatory use the GRAPE, a gravity simulation software to simulate planetary formation
Marseille Observatory use the GRAPE, a gravity simulation software to simulate planetary formation
Palais Longchamp
Palais Longchamp
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Clockwise from upper left: NGC 7320, NGC 7319, NGC 7318 (a and b), NGC 7317
Clockwise from upper left: NGC 7320, NGC 7319, NGC 7318 (a and b), NGC 7317
Stephan's Quintet. The blue arc across the top center is a shock caused by colliding intergalactic gas. Image Credits: X-ray (blue): NASA/CXC/CfA/E. O
Stephan's Quintet. The blue arc across the top center is a shock caused by colliding intergalactic gas. Image Credits: X-ray (blue): NASA/CXC/CfA/E. O'Sullivan Optical (brown): Canada-France-Hawaii-Telescope/Coelum
Earthbound monochrome (sdss-g filtered) image of Stephan's Quintet from the Liverpool Telescope
Earthbound monochrome (sdss-g filtered) image of Stephan's Quintet from the Liverpool Telescope
Detail of the quintet in a photo by Hubble Space Telescope, 1998–99. Credits: NASA/ESA
Detail of the quintet in a photo by Hubble Space Telescope, 1998–99. Credits: NASA/ESA