ロード中...
EFFECT OF SURFACE-MANTLE WATER EXCHANGE PARAMETERIZATIONS ON EXOPLANET OCEAN DEPTHS
Terrestrial exoplanets in the canonical habitable zone may have a variety of initial water fractions due to random volatile delivery by planetesimals. If the total planetary water complement is high, the entire surface may be covered in water, forming a “waterworld.” On a planet with active tectonic...
保存先:
| 出版年: | Astrophys J |
|---|---|
| 主要な著者: | , |
| フォーマット: | Artigo |
| 言語: | Inglês |
| 出版事項: |
2016
|
| 主題: | |
| オンライン･アクセス: | https://ncbi.nlm.nih.gov/pmc/articles/PMC6350802/ https://ncbi.nlm.nih.gov/pubmed/30705445 https://ncbi.nlm.nih.govhttp://dx.doi.org/10.3847/0004-637X/832/1/54 |
| タグ: |
タグ追加
タグなし, このレコードへの初めてのタグを付けませんか!
|