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dc.contributor.authorLuspay-Kuti, A.
dc.contributor.authorMousis, O.
dc.contributor.authorLunine, J.I.
dc.contributor.authorEllinger, Y.
dc.contributor.authorPauzat, F.
dc.contributor.authorRaut, U.
dc.contributor.authorBouquet, A.
dc.contributor.authorMandt, K.E.
dc.contributor.authorMaggiolo, R.
dc.contributor.authorRonnet, T.
dc.contributor.authorBrugger, B.
dc.contributor.authorOzgurel, O.
dc.contributor.authorFuselier, S.A.
dc.date2018
dc.date.accessioned2018-11-02T11:19:42Z
dc.date.available2018-11-02T11:19:42Z
dc.identifier.urihttps://orfeo.belnet.be/handle/internal/7097
dc.descriptionThe Rosetta Orbiter Spectrometer for Ion and Neutral Analysis (ROSINA) instrument onboard the Rosetta spacecraft has measured molecular oxygen (O2) in the coma of comet 67P/Churyumov-Gerasimenko (67P/C-G) in surprisingly high abundances. These measurements mark the first unequivocal detection of O2 in a cometary environment. The large relative abundance of O2 in 67P/C-G despite its high reactivity and low interstellar abundance poses a puzzle for its origin in comet 67P/C-G, and potentially other comets. Since its detection, there have been a number of hypotheses put forward to explain the production and origin of O2 in the comet. These hypotheses cover a wide range of possibilities from various in situ production mechanisms to protosolar nebula and primordial origins. Here, we review the O2 formation mechanisms from the literature, and provide a comprehensive summary of the current state of knowledge of the sources and origin of cometary O2.
dc.languageeng
dc.titleOrigin of Molecular Oxygen in Comets: Current Knowledge and Perspectives
dc.typeArticle
dc.subject.frascatiPhysical sciences
dc.audienceScientific
dc.subject.freeMolecular oxygen
dc.subject.freeComets
dc.subject.freeRadiolysis
dc.subject.freeIce
dc.subject.freeAstrobiology
dc.source.titleSpace Science Reviews
dc.source.volume214
dc.source.issue8
dc.source.pageA115
Orfeo.peerreviewedYes
dc.identifier.doi10.1007/s11214-018-0541-2


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