File:Radial Velocity Method.gif
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Captions
Captions
Animation showing the Doppler shifting of stellar line as a planet orbits its host star.
Summary
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| Description |
English: This shows the radial velocity method of detecting extra-Solar planets. As a planet orbits its host star, they both orbit the common center of mass (top left). The "wobble" of the star can be detected through the Doppler shifting of stellar absorption features (bottom). The radial velocity curve is made of measurements of the stellar Doppler shift through the planet's orbital period (top right). |
| Date | |
| Source | Own work |
| Author | Aspolanski |
Licensing
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I, the copyright holder of this work, hereby publish it under the following license:
 
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This file is made available under the Creative Commons CC0 1.0 Universal Public Domain Dedication. |
| The person who associated a work with this deed has dedicated the work to the public domain by waiving all of their rights to the work worldwide under copyright law, including all related and neighboring rights, to the extent allowed by law. You can copy, modify, distribute and perform the work, even for commercial purposes, all without asking permission.
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| Date/Time | Thumbnail | Dimensions | User | Comment | |
|---|---|---|---|---|---|
| current | 17:19, 16 June 2024 | | 1,100 × 800 (11.71 MB) | Aspolanski (talk | contribs) | Uploaded own work with UploadWizard |
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