File:The radial velocity method (artist’s impression).jpg
Appearance
Size of this preview: 800 × 597 pixels. Other resolutions: 320 × 239 pixels | 640 × 478 pixels | 1,024 × 765 pixels | 1,280 × 956 pixels | 2,374 × 1,773 pixels.
Original file (2,374 × 1,773 pixels, file size: 339 KB, MIME type: image/jpeg)
File history
Click on a date/time to view the file as it appeared at that time.
Date/Time | Thumbnail | Dimensions | User | Comment | |
---|---|---|---|---|---|
current | 02:35, 13 May 2020 | 2,374 × 1,773 (339 KB) | Acagastya | essentially croppping | |
19:32, 9 November 2008 | 2,374 × 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 |
File usage
The following page uses this file:
Global file usage
The following other wikis use this file:
- Usage on af.wikipedia.org
- Usage on arz.wikipedia.org
- Usage on ast.wikipedia.org
- Usage on bg.wikipedia.org
- Usage on bs.wikipedia.org
- Usage on ca.wikipedia.org
- Usage on de.wikipedia.org
- Usage on el.wikipedia.org
- Usage on en.wikipedia.org
- Usage on es.wikipedia.org
- Usage on fa.wikipedia.org
- Usage on fi.wikipedia.org
- Usage on hi.wikipedia.org
- Usage on ja.wikipedia.org
- Usage on kk.wikipedia.org
- Usage on mk.wikipedia.org
- Usage on ms.wikipedia.org
- Usage on nl.wikipedia.org
- Usage on or.wikipedia.org
- Usage on pt.wikipedia.org
- Usage on sr.wikipedia.org
- Usage on tr.wikipedia.org
- Usage on uk.wikipedia.org