File:The radial velocity method (artist’s impression).jpg
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DescriptionThe radial velocity method (artist’s impression).jpg | 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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Source | European Southern Observatory | ||||
Author | European Southern Observatory | ||||
Permission (Reusing this file) |
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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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current | 02:35, 13 May 2020 | 2,374 × 1,773 (339 KB) | Acagastya (talk | contribs) | essentially croppping | |
19:32, 9 November 2008 | 2,374 × 2,094 (1.04 MB) | ComputerHotline (talk | contribs) | {{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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- File:ESO - The Radial Velocity Method (by).jpg (file redirect)
- File:ESO wobble.png
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Image title |
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Credit/Provider | ESO |
Source | European Southern Observatory |
Short title |
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Usage terms |
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Date and time of data generation | 00:00, 25 April 2007 |
Keywords | Radial velocity |
Contact information |
Karl-Schwarzschild-Strasse 2 Garching bei München, , D-85748 Germany |
IIM version | 4 |