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Three regimes of extrasolar planet radius inferred from host star metallicities
Approximately half of the extrasolar planets (exoplanets) with radii less than four Earth radii are in orbits with short periods(1). Despite their sheer abundance, the compositions of such planets are largely unknown. The available evidence suggests that they range in composition from small, high-de...
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| Hlavní autoři: | , , , , , , , , |
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| Médium: | Artigo |
| Jazyk: | Inglês |
| Vydáno: |
2014
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| Témata: | |
| On-line přístup: | https://ncbi.nlm.nih.gov/pmc/articles/PMC4048851/ https://ncbi.nlm.nih.gov/pubmed/24870544 https://ncbi.nlm.nih.govhttp://dx.doi.org/10.1038/nature13254 |
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