Statistical-likelihood Exo-Planetary Habitability Index (SEPHI)
| Autor: | J. M. Rodríguez-Mozos, A. Moya |
|---|---|
| Rok vydání: | 2017 |
| Předmět: |
Earth and Planetary Astrophysics (astro-ph.EP)
Physics 010504 meteorology & atmospheric sciences Planetary habitability Habitability FOS: Physical sciences Astronomy Astronomy and Astrophysics Planetary system 01 natural sciences Exoplanet Habitability of orange dwarf systems Astrobiology Space and Planetary Science Planet 0103 physical sciences Astrophysics::Earth and Planetary Astrophysics 010303 astronomy & astrophysics Kepler-62e Planetary mass Astrophysics - Earth and Planetary Astrophysics 0105 earth and related environmental sciences |
| Zdroj: | Monthly Notices of the Royal Astronomical Society. 471:4628-4636 |
| ISSN: | 1365-2966 0035-8711 |
| DOI: | 10.1093/mnras/stx1910 |
| Popis: | A new Statistical-likelihood Exo-Planetary Habitability Index (SEPHI) is presented. It has been developed to cover the current and future features required for a classification scheme disentangling whether any discovered exoplanet is potentially habitable compared with life on Earth. The SEPHI uses likelihood functions to estimate the habitability potential. It is defined as the geometric mean of four sub-indexes related with four comparison criteria: Is the planet telluric?; Does it have an atmosphere dense enough and a gravity compatible with life?; Does it have liquid water on its surface?; Does it have a magnetic field shielding its surface from harmful radiation and stellar winds?. Only with seven physical characteristics, can the SEPHI be estimated: Planetary mass, radius, and orbital period; stellar mass, radius, and effective temperature; planetary system age. We have applied the SEPHI to all the planets in the Exoplanet Encyclopaedia using a Monte Carlo Method. Kepler-1229 b, Kepler-186 f, and Kepler-442 b have the largest SEPHI values assuming certain physical descriptions. Kepler-1229 b is the most unexpected planet in this privileged position since no previous study pointed to this planet as a potentially interesting and habitable one. In addition, most of the tidally locked Earth-like planets present a weak magnetic field, incompatible with habitability potential. We must stress that our results are linked to the physics used in this study. Any change in the physics used only implies an updating of the likelihood functions. We have developed a web application allowing the on-line estimation of the SEPHI: http://sephi.azurewebsites.net/ 10 pages, 4 figures, 6 tables. Accepted for publication in MNRAS |
| Databáze: | OpenAIRE |
| Externí odkaz: |
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