{"refrec":{"BRefID":337577,"RR":"<b>Beuthe, M.</b> (2020). Comment on 'Heating of Enceladus due to the dissipation of ocean tides' by R. Tyler. <i>Icarus 350</i>: 113934. <a href=\"https://hdl.handle.net/10.1016/j.icarus.2020.113934\" target=\"_blank\">https://hdl.handle.net/10.1016/j.icarus.2020.113934</a>","BEntID":334200,"PublicFlag":1,"CheckedFlag":1,"wosflag":1,"vabbflag":0,"RefStringPartII":". <i>Icarus 350</i>: 113934. <a href=\"https://hdl.handle.net/10.1016/j.icarus.2020.113934\" target=\"_blank\">https://hdl.handle.net/10.1016/j.icarus.2020.113934</a>","DocTypID":8,"DocType":"Journal article","MarineFlag":0,"FreshFlag":0,"BrackishFlag":0,"TerrestrialFlag":0,"Authorstring":"Beuthe, M.","OrigTitleTranslFlag":0,"Authorstringtrunc":"Beuthe, M.","Englishabstract":"Dissipation of ocean potential energy is proposed by Tyler (2020) as a new mechanism leading to possible high-power states for Enceladus. 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