{"refrec":{"BRefID":339455,"RR":"<b>Rovira-Navarro, M.; van der Wal, W.; Steinke, T.; Dirkx, D.</b> (2021). Tidally heated exomoons around gas giants. <i>PSJ 2(3)</i>: 119. <a href=\"https://dx.doi.org/10.3847/psj/abf6cb\" target=\"_blank\">https://dx.doi.org/10.3847/psj/abf6cb</a>","BEntID":336090,"PublicFlag":1,"CheckedFlag":0,"wosflag":0,"vabbflag":0,"RefStringPartII":". <i>PSJ 2(3)</i>: 119. <a href=\"https://dx.doi.org/10.3847/psj/abf6cb\" target=\"_blank\">https://dx.doi.org/10.3847/psj/abf6cb</a>","DocTypID":8,"DocType":"Journal article","MarineFlag":0,"FreshFlag":0,"BrackishFlag":0,"TerrestrialFlag":0,"Authorstring":"Rovira-Navarro, M.; van der Wal, W.; Steinke, T.; Dirkx, D.","OrigTitleTranslFlag":0,"Authorstringtrunc":"Rovira-Navarro, M. <i>et al.</i>","Englishabstract":"<p>    Thousands of exoplanets have been discovered; however, the detection of    exomoons remains elusive. Tidally heated exomoons have been proposed as    candidate targets for observation; vigorous tidal dissipation can raise the    moon's surface temperature, making direct imaging possible, and cause    widespread volcanism that can have a signature in transits. We assess    whether the required amounts of tidal dissipation can be attained and how    long it can be sustained. In a first step, we look at the thermal state of    a super-Io for different orbital configurations. We show that close-in    exomoons with moderate    <img        width=\"44\"        height=\"14\"        src=\"file:///C:/Users/LVDWEE~1/AppData/Local/Temp/msohtmlclip1/01/clip_image001.gif\"        alt=\"$(e\\sim {e}_{\\mathrm{Io}}$\"    />    ) to high (    <img        width=\"42\"        height=\"12\"        src=\"file:///C:/Users/LVDWEE~1/AppData/Local/Temp/msohtmlclip1/01/clip_image002.gif\"        alt=\"$e\\sim 0.1$\"    />    ) orbital eccentricities can feature surface heat fluxes 1–3 orders of    magnitude higher than that of Io if heat transfer is dominated by heat    piping or the moon has a magma ocean. In a second step, we investigate the    longevity of a super-Io. The free eccentricity of an isolated close-in    exomoon is quickly dampened due to tides; high orbital eccentricities can    be maintained if the moon is in a mean-motion resonance with another moon    and the planet is highly dissipative. However, this scenario leads to fast    orbital migration. For a Mars-sized exomoon, we find that tides alone can    raise the surface temperatures to more than 400 K for 10 million yr, and    surface heat fluxes higher than that of Io can be maintained for billions    of years. Such tidally active bodies are expected to feature more vigorous    volcanic activity than Io. The material outgassed via volcanism might be    detected in transits.</p>","AbstractOtherLang":null,"BibLvlCode":"AS","StandardTitle":"Tidally heated exomoons around gas giants","OrigTitleLangCode":"en","OrigTitleLangCodeExtended":"eng","OrigTitleLangID":15,"DateLastModified":{"date":"2026-04-20 01:32:45.218995","timezone_type":1,"timezone":"+02:00"},"UserAccessRight":null,"UserAccID":null,"AuthorKeywords":null,"OtherDescriptors":null,"Notes":null,"AnaPub":2021,"MonPub":null,"DateUpdate":"2021-07-12","DateCreate":"2021-06-30","SecASFANote":null,"ConfID":null,"PeerRev":1,"VlizCoreFlag":1,"WoScode":"WOS:000917988300001","VABBcode":null,"OpenAcc":1,"DOI":"10.3847/psj/abf6cb"},"refs":null,"anarec":{"AnaID":339455,"PubliDate":2021,"Pagination":"119","XtraPublOfAnaID":null,"ISBN":null,"Volume":"2","Issue":"3","BRefMon":null,"BRefMonRR":null,"BRefXtra":null,"BRefXtraRR":null,"SerBRefID":339466,"SerRR":"The Planetary Science Journal. IOP Publishing: Bristol.  e-ISSN 2632-3338. <a href=\"https://dx.doi.org/10.3847/issn.2632-3338\" target=\"_blank\">https://dx.doi.org/10.3847/issn.2632-3338</a>","StandardTitleSer":"The Planetary Science Journal","ISSN":null,"AbbrevSer":"PSJ","StandardTitleMon":null,"StartPage":119,"Pages":null,"ToPubliDate":null,"BRefBibLvlCode":"S","SerNotes":null},"monrec":null,"serrec":null,"relations":null,"relationsRev":null,"addrec":null,"othpubs":null,"ownerships":null,"authors":[{"AutName":"Rovira-Navarro","Firstname":"Marc","Initials":"M.","Affiliation":null,"Discriminator":null,"CorporateFlag":0,"BEntID":336090,"AutID":371630,"OrderNr":1,"DegrID":null,"EditorFlag":0,"CorrespFlag":0,"IllustratorFlag":0,"ReviserFlag":0,"TranslatorFlag":0,"InsAcronym":"OCS","InsFSN":"Koninklijk Nederlands Instituut voor Onderzoek der Zee; Ocean Sciences","ORCID":"0000-0002-9980-5065","PersID":37487,"InsID":13654},{"AutName":"van der Wal","Firstname":"Wouter","Initials":"W.","Affiliation":null,"Discriminator":null,"CorporateFlag":0,"BEntID":336090,"AutID":371632,"OrderNr":2,"DegrID":null,"EditorFlag":0,"CorrespFlag":0,"IllustratorFlag":0,"ReviserFlag":0,"TranslatorFlag":0,"InsAcronym":null,"InsFSN":null,"ORCID":null,"PersID":null,"InsID":null},{"AutName":"Steinke","Firstname":null,"Initials":"T.","Affiliation":null,"Discriminator":null,"CorporateFlag":0,"BEntID":336090,"AutID":34938,"OrderNr":3,"DegrID":null,"EditorFlag":0,"CorrespFlag":0,"IllustratorFlag":0,"ReviserFlag":0,"TranslatorFlag":0,"InsAcronym":null,"InsFSN":null,"ORCID":null,"PersID":null,"InsID":null},{"AutName":"Dirkx","Firstname":"Dominic","Initials":"D.","Affiliation":null,"Discriminator":null,"CorporateFlag":0,"BEntID":336090,"AutID":448151,"OrderNr":4,"DegrID":null,"EditorFlag":0,"CorrespFlag":0,"IllustratorFlag":0,"ReviserFlag":0,"TranslatorFlag":0,"InsAcronym":null,"InsFSN":null,"ORCID":null,"PersID":null,"InsID":null}],"mapdetails":null,"datasets":null,"monographs":null,"monparts":null,"serparts":null,"BEntOpen":336090,"BEntPrivate":null,"availability":[{"BInstID":362789,"LibID":2779,"BRefID":339455,"EmbargoDate":null,"FullEmbargoDate":null,"PhysMedID":16,"hasOCRd":1,"ShelfLocCode":"362789","RFID":null,"PaidValue":null,"Medium":"Server","Description":null,"Acronym":null,"Library":"NIOZ","DutchTerm":null,"URL":null,"ClassifID":260,"Classification":"NIOZ Open Repository","ReqLink":null,"ClassifTypID":1,"URLLocation":"https://www.vliz.be/imisdocs/publications/","SubDir":1,"InternalReq":null,"LoggedInReq":null,"Disclaimer":"Disclaimer_NIOZ","DutchDisclaimer":null,"FileFormat":".pdf","FileDescr":"pdf","InsPub":1,"InsID":397,"FileFormID":6,"LendableFlag":null,"PublicFlag":1,"orderLib":"NIOZ","Notes":null,"AccConID":null,"AccessConstraint":null,"LicURL":null}],"litstyles":null,"thespers":null,"arch2discl":805,"SERpubls":[{"PublName":"IOP Publishing","City":"Bristol"}],"MONpubls":null,"pictures":[],"thestermsPath":null,"thestermsASFA":null,"taxtermsASFA":null,"geotermsASFA":null,"collections":null,"conf":null,"proj":null,"Physdatasets":null,"spcols":{"805":{"SpName":"Koninklijk Nederlands Instituut voor Onderzoek der Zee","SpColID":805,"ParSpColID":null,"TopParID":null,"ShortName":"NIOZ","URLLocation":"https://www.vliz.be/imis/nioz/imis.php?refid=","LibID":2779,"OpenRepoFlag":1,"SpTypID":1,"TopParIDNotWebsite":null,"SpColPath":"NIOZ"}},"doi":null,"publs":null,"serparttypes":null,"monauthors":null,"MParts":null,"SParts":null,"hLibs":null,"langs":[{"BEntID":336090,"AbstractFlag":0,"LangID":15,"LangCode":"en","Lang":"English","DutchTerm":"Engels","LangCodeExtended":"eng"},{"BEntID":336090,"AbstractFlag":1,"LangID":15,"LangCode":"en","Lang":"English","DutchTerm":"Engels","LangCodeExtended":"eng"}],"urls":[{"URL":"https://dx.doi.org/10.3847/psj/abf6cb","externalID":"10.3847/psj/abf6cb","URLTypeCode":"DOI","URLID":94615,"URLTypID":13,"URLType":"DOI","URLPrefix":"http://dx.doi.org/"}],"thesterms":null,"taxterms":null,"geoterms":null,"othterms":null,"asfacodes":null,"asfa2codes":null,"thestermsFRIS":null,"taxtermsFRIS":null,"geotermsFRIS":null,"othtermsFRIS":null,"resmessage":"","complete":1,"sessions":{"newSesName":"Leonne.van.der.Weegen@nioz.nl","newSesDate":{"date":"2021-06-30 08:36:14.650000","timezone_type":3,"timezone":"Europe/Brussels"},"updSesName":"Leonne.van.der.Weegen@nioz.nl","updSesDate":{"date":"2021-07-12 10:34:44.147000","timezone_type":3,"timezone":"Europe/Brussels"}}}