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Remote life-detection criteria, habitable zone boundaries, and the frequency of Earth-like planets around M and late K stars
The habitable zone (HZ) around a star is typically defined as the region where a rocky planet can maintain liquid water on its surface. That definition is appropriate, because this allows for the possibility that carbon-based, photosynthetic life exists on the planet in sufficient abundance to modif...
Αποθηκεύτηκε σε:
| Κύριοι συγγραφείς: | , , , |
|---|---|
| Μορφή: | Artigo |
| Γλώσσα: | Inglês |
| Έκδοση: |
National Academy of Sciences
2014
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| Θέματα: | |
| Διαθέσιμο Online: | https://ncbi.nlm.nih.gov/pmc/articles/PMC4156685/ https://ncbi.nlm.nih.gov/pubmed/24277805 https://ncbi.nlm.nih.govhttp://dx.doi.org/10.1073/pnas.1309107110 |
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