File:Neptunian Desert Visualization.png
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Summary
| Description |
English: Distribution of mass versus orbital period for planets with a measured mass. Planets discovered by the transit method are shown in blue, with those having masses measured to better than 30 per cent represented as filled circles. Planets found by radial velocity are shown as green circles and those detected by other methods are shown by grey circles. Black lines represent the Neptunian desert as defined in Mazeh et al.[1] NGTS-4b is shown as a red cross. Taken from the NASA Exoplanet Archive on 2018 August 14. |
| Date | |
| Source | https://doi.org/10.1093/mnras/stz1084 |
| Author | Watson, Christopher A.; Walker, Simon R.; Udry, Stéphane; Thompson, Samantha J.; Sohy, Sandrine; Rauer, Heike; Queloz, Didier; Pollacco, Don; Murray, Catriona |
Notes
- ↑ Faigler, S. (2016-05-01). "Dearth of short-period Neptunian exoplanets: A desert in period-mass and period-radius planes". Astronomy & Astrophysics 589: A75. DOI:10.1051/0004-6361/201528065. ISSN 0004-6361.
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| current | 18:31, 29 May 2019 | | 975 × 722 (383 KB) | Triesault | User created page with UploadWizard |
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