File:ESO wobble.png

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	Date/Time	Thumbnail	Dimensions	User	Comment
current	20:41, 8 September 2015		2,367 × 1,584 (704 KB)	commons>Rfassbind	{{Information \|Description=The radial velocity method to detect exoplanet is based on the detection of variations in the velocity of the central star, due to the changing direction of the gravitational pull from an (unseen) exoplanet as it orbits the s...

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