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Formation, Habitability, and Detection of Extrasolar Moons

hal.structure.identifierMcMaster University [Hamilton, Ontario]
dc.contributor.authorHELLER, René
hal.structure.identifierPenn State Behrend
dc.contributor.authorWILLIAMS, Darren
hal.structure.identifierHarvard-Smithsonian Center for Astrophysics [CfA]
dc.contributor.authorKIPPING, David
hal.structure.identifierDepartment of Astrophysical Sciences [Princeton]
dc.contributor.authorLIMBACH, Mary Anne
hal.structure.identifierDepartment of Astrophysical Sciences [Princeton]
dc.contributor.authorTURNER, Edwin
hal.structure.identifierUniversity of Arizona
dc.contributor.authorGREENBERG, Richard
dc.contributor.authorSASAKI, Takanori
hal.structure.identifierSSE 2014
dc.contributor.authorBOLMONT, Emeline
hal.structure.identifierLaboratoire de Planétologie et Géodynamique [UMR 6112] [LPG]
dc.contributor.authorGRASSET, Olivier
hal.structure.identifierTokyo Institute of Technology [Tokyo] [TITECH]
dc.contributor.authorLEWIS, Karen
hal.structure.identifierNASA Astrobiology Institute [NAI]
dc.contributor.authorBARNES, Rory
hal.structure.identifierUniversidad de Antioquia = University of Antioquia [Medellín, Colombia]
dc.contributor.authorZULUAGA, Jorge I.
dc.date.created2014-08-26
dc.date.issued2014
dc.identifier.issn1531-1074
dc.description.abstractEnThe diversity and quantity of moons in the Solar System suggest a manifold population of natural satellites exist around extrasolar planets. Of peculiar interest from an astrobiological perspective, the number of sizable moons in the stellar habitable zones may outnumber planets in these circumstellar regions. With technological and theoretical methods now allowing for the detection of sub-Earth-sized extrasolar planets, the first detection of an extrasolar moon appears feasible. In this review, we summarize formation channels of massive exomoons that are potentially detectable with current or near-future instruments. We discuss the orbital effects that govern exomoon evolution, we present a framework to characterize an exomoon's stellar plus planetary illumination as well as its tidal heating, and we address the techniques that have been proposed to search for exomoons. Most notably, we show that natural satellites in the range of 0.1 - 0.5 Earth mass (i) are potentially habitable, (ii) can form within the circumplanetary debris and gas disk or via capture from a binary, and (iii) are detectable with current technology.
dc.language.isoen
dc.publisherMary Ann Liebert
dc.subject.enAstrophysics
dc.subject.enEarth and Planetary Astrophysics
dc.title.enFormation, Habitability, and Detection of Extrasolar Moons
dc.typeArticle de revue
dc.identifier.doi10.1089/ast.2014.1147
dc.subject.halPlanète et Univers [physics]/Astrophysique [astro-ph]/Planétologie et astrophysique de la terre [astro-ph.EP]
dc.identifier.arxiv1408.6164
bordeaux.journalAstrobiology
bordeaux.page798-835
bordeaux.volume14
bordeaux.issue9
bordeaux.peerReviewedoui
hal.identifierhal-01059901
hal.version1
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-01059901v1
bordeaux.COinSctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.jtitle=Astrobiology&rft.date=2014&rft.volume=14&rft.issue=9&rft.spage=798-835&rft.epage=798-835&rft.eissn=1531-1074&rft.issn=1531-1074&rft.au=HELLER,%20Ren%C3%A9&WILLIAMS,%20Darren&KIPPING,%20David&LIMBACH,%20Mary%20Anne&TURNER,%20Edwin&rft.genre=article


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