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Opis 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 star. When the star moves towards us, its spectrum is blueshifted, while it is redshifted when it moves away from us. By regularly looking at the spectrum of a star - and so, measure its velocity - one can see if it moves periodically due to the influence of a companion.
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This file, which was originally posted to European Southern Observatory, was reviewed on 13 May 2020 by reviewer Acagastya, who confirmed that it was available there under the stated license on that date.

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Datum/vrijemeSmanjeni pregledDimenzijeKorisnikKomentar
trenutno04:35, 13 maj 2020Smanjeni pregled verzije na dan 04:35, 13 maj 20202.374 × 1.773 (339 KB)Acagastyaessentially croppping
21:32, 9 novembar 2008Smanjeni pregled verzije na dan 21:32, 9 novembar 20082.374 × 2.094 (1,04 MB)ComputerHotline{{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 star

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