File:WASP-8 b v2.tif
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![File:WASP-8 b v2.tif](https://upload.wikimedia.org/wikipedia/commons/thumb/e/e7/WASP-8_b_v2.tif/lossy-page1-800px-WASP-8_b_v2.tif.jpg?20230505234720)
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[edit]DescriptionWASP-8 b v2.tif | Up to now it was expected that exoplanets would all orbit in more or less the same plane, and that they would move along their orbits in the same direction as the star’s rotation — as they do in our Solar System. However, new results unexpectedly show that many exoplanets actually orbit at a large angle to their star’s spin axis. In the case shown here (WASP 8b) the orbit is completely reversed, or retrograde. | ||||
Date | 13 April 2010 | ||||
Source | https://www.eso.org/public/images/eso1016a/ | ||||
Author | ESO/L. Calçada | ||||
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Date/Time | Thumbnail | Dimensions | User | Comment | |
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current | 23:47, 5 May 2023 | ![]() | 3,000 × 2,120 (8.22 MB) | Юрий Д.К. (talk | contribs) | {{Information |Description=Up to now it was expected that exoplanets would all orbit in more or less the same plane, and that they would move along their orbits in the same direction as the star’s rotation — as they do in our Solar System. However, new results unexpectedly show that many exoplanets actually orbit at a large angle to their star’s spin axis. In the case shown here (WASP 8b) the orbit is completely reversed, or retrograde. |Source=https://www.eso.org/public/images/eso1016a/ |Dat... |
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Width | 3,000 px |
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Height | 2,120 px |
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Compression scheme | LZW |
Pixel composition | RGB |
Orientation | Normal |
Number of components | 3 |
Number of rows per strip | 29 |
Horizontal resolution | 72 dpi |
Vertical resolution | 72 dpi |
Data arrangement | chunky format |
Software used | CINEMA 4D |
File change date and time | 14:02, 12 April 2010 |
Color space | Uncalibrated |
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13 April 2010
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