A More Comprehensive Habitable Zone for Finding Life on Other Planets

The habitable zone (HZ) is the circular region around a star(s) where standing bodies of water could exist on the surface of a rocky planet. Space missions employ the HZ to select promising targets for follow-up habitability assessment. The classical HZ definition assumes that the most important gre...

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Main Author: Ramses M. Ramirez
Format: Article
Language:English
Published: MDPI AG 2018-07-01
Series:Geosciences
Subjects:
Online Access:http://www.mdpi.com/2076-3263/8/8/280
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author Ramses M. Ramirez
author_facet Ramses M. Ramirez
author_sort Ramses M. Ramirez
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description The habitable zone (HZ) is the circular region around a star(s) where standing bodies of water could exist on the surface of a rocky planet. Space missions employ the HZ to select promising targets for follow-up habitability assessment. The classical HZ definition assumes that the most important greenhouse gases for habitable planets orbiting main-sequence stars are CO2 and H2O. Although the classical HZ is an effective navigational tool, recent HZ formulations demonstrate that it cannot thoroughly capture the diversity of habitable exoplanets. Here, I review the planetary and stellar processes considered in both classical and newer HZ formulations. Supplementing the classical HZ with additional considerations from these newer formulations improves our capability to filter out worlds that are unlikely to host life. Such improved HZ tools will be necessary for current and upcoming missions aiming to detect and characterize potentially habitable exoplanets.
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spelling doaj.art-e27ac1f2510e4ea1b9860bb6cbe268b92022-12-21T17:32:58ZengMDPI AGGeosciences2076-32632018-07-018828010.3390/geosciences8080280geosciences8080280A More Comprehensive Habitable Zone for Finding Life on Other PlanetsRamses M. Ramirez0Earth-Life Science Institute (ELSI), Tokyo Institute of Technology, Tokyo 152-8550, JapanThe habitable zone (HZ) is the circular region around a star(s) where standing bodies of water could exist on the surface of a rocky planet. Space missions employ the HZ to select promising targets for follow-up habitability assessment. The classical HZ definition assumes that the most important greenhouse gases for habitable planets orbiting main-sequence stars are CO2 and H2O. Although the classical HZ is an effective navigational tool, recent HZ formulations demonstrate that it cannot thoroughly capture the diversity of habitable exoplanets. Here, I review the planetary and stellar processes considered in both classical and newer HZ formulations. Supplementing the classical HZ with additional considerations from these newer formulations improves our capability to filter out worlds that are unlikely to host life. Such improved HZ tools will be necessary for current and upcoming missions aiming to detect and characterize potentially habitable exoplanets.http://www.mdpi.com/2076-3263/8/8/280astrobiologyplanetary atmosphereshabitable zonesextraterrestrial life
spellingShingle Ramses M. Ramirez
A More Comprehensive Habitable Zone for Finding Life on Other Planets
Geosciences
astrobiology
planetary atmospheres
habitable zones
extraterrestrial life
title A More Comprehensive Habitable Zone for Finding Life on Other Planets
title_full A More Comprehensive Habitable Zone for Finding Life on Other Planets
title_fullStr A More Comprehensive Habitable Zone for Finding Life on Other Planets
title_full_unstemmed A More Comprehensive Habitable Zone for Finding Life on Other Planets
title_short A More Comprehensive Habitable Zone for Finding Life on Other Planets
title_sort more comprehensive habitable zone for finding life on other planets
topic astrobiology
planetary atmospheres
habitable zones
extraterrestrial life
url http://www.mdpi.com/2076-3263/8/8/280
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