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Water and related chemistry in the solar system. A guaranteed time key programme for Herschel

hal.structure.identifierMax-Planck-Institut für Sonnensystemforschung = Max Planck Institute for Solar System Research [MPS]
dc.contributor.authorHARTOGH, P.
hal.structure.identifierLaboratoire d'études spatiales et d'instrumentation en astrophysique [LESIA]
dc.contributor.authorLELLOUCH, E.
hal.structure.identifierLaboratoire d'études spatiales et d'instrumentation en astrophysique [LESIA]
dc.contributor.authorCROVISIER, J.
hal.structure.identifierSpace Research Centre of Polish Academy of Sciences [CBK]
dc.contributor.authorBANASZKIEWICZ, M.
dc.contributor.authorBENSCH, F.
hal.structure.identifierHarvard-Smithsonian Center for Astrophysics [CfA]
dc.contributor.authorBERGIN, E. A.
hal.structure.identifierLaboratoire d'astrodynamique, d'astrophysique et d'aéronomie de bordeaux [L3AB]
hal.structure.identifierObservatoire aquitain des sciences de l'univers [OASU]
hal.structure.identifierLaboratoire d'Astrophysique de Bordeaux [Pessac] [LAB]
dc.contributor.authorBILLEBAUD, F.
hal.structure.identifierLaboratoire d'études spatiales et d'instrumentation en astrophysique [LESIA]
dc.contributor.authorBIVER, N.
hal.structure.identifierLabOratoire proCédés énergIe bâtimEnt [LOCIE]
dc.contributor.authorBLAKE, G. A.
hal.structure.identifierPolska Akademia Nauk = Polish Academy of Sciences = Académie polonaise des sciences [PAN]
dc.contributor.authorBLECKA, M. I.
dc.contributor.authorBLOMMAERT, J.
hal.structure.identifierLaboratoire d'études spatiales et d'instrumentation en astrophysique [LESIA]
dc.contributor.authorBOCKELÉE-MORVAN, D.
hal.structure.identifierLaboratoire d'astrodynamique, d'astrophysique et d'aéronomie de bordeaux [L3AB]
hal.structure.identifierObservatoire aquitain des sciences de l'univers [OASU]
hal.structure.identifierLaboratoire d'Astrophysique de Bordeaux [Pessac] [LAB]
dc.contributor.authorCAVALIÉ, T.
hal.structure.identifierCentro de Investigaciones Biológicas [CSIC]
dc.contributor.authorCERNICHARO, J.
hal.structure.identifierObservatoire de Paris - Site de Paris [OP]
dc.contributor.authorCOURTIN, R.
hal.structure.identifierDepartment of Ecology and Evolutionary Biology [Princeton]
dc.contributor.authorDAVIS, G.
dc.contributor.authorDECIN, L.
hal.structure.identifierLaboratoire d'Etude du Rayonnement et de la Matière en Astrophysique [LERMA]
dc.contributor.authorENCRENAZ, P.
hal.structure.identifierLaboratoire d'études spatiales et d'instrumentation en astrophysique [LESIA]
dc.contributor.authorENCRENAZ, T.
hal.structure.identifierDepartamento de Biologia Celular, Facultad de Biologia
dc.contributor.authorGONZÁLEZ, A.
dc.contributor.authorDE GRAAUW, T.
dc.contributor.authorHUTSEMÉKERS, D.
dc.contributor.authorJARCHOW, C.
hal.structure.identifierEuropean Southern Observatory [ESO]
dc.contributor.authorJEHIN, E.
dc.contributor.authorKIDGER, M.
hal.structure.identifierMax-Planck-Institut für Sonnensystemforschung = Max Planck Institute for Solar System Research [MPS]
dc.contributor.authorKÜPPERS, M.
dc.contributor.authorDE LANGE, A.
hal.structure.identifierLaboratorio de Ecologia Isotopica
dc.contributor.authorLARA, L.-M.
hal.structure.identifierCalifornia Institute of Technology [CALTECH]
dc.contributor.authorLIS, D. C.
dc.contributor.authorLORENTE, R.
dc.contributor.authorMANFROID, J.
dc.contributor.authorMEDVEDEV, A. S.
hal.structure.identifierLaboratoire d'études spatiales et d'instrumentation en astrophysique [LESIA]
dc.contributor.authorMORENO, R.
dc.contributor.authorNAYLOR, D. A.
hal.structure.identifierJet Propulsion Laboratory [JPL]
dc.contributor.authorORTON, G.
dc.contributor.authorPORTYANKINA, G.
dc.contributor.authorRENGEL, M.
hal.structure.identifierCenter for Mathematics and Physics
dc.contributor.authorSAGAWA, H.
dc.contributor.authorSÁNCHEZ-PORTAL, M.
dc.contributor.authorSCHIEDER, R.
dc.contributor.authorSIDHER, S.
hal.structure.identifierSRON Netherlands Institute for Space Research [SRON]
dc.contributor.authorSTAM, D.
dc.contributor.authorSWINYARD, B.
dc.contributor.authorSZUTOWICZ, S.
hal.structure.identifierUniversität Bern = University of Bern = Université de Berne [UNIBE]
dc.contributor.authorTHOMAS, N
dc.contributor.authorTHORNHILL, G.
dc.contributor.authorVANDENBUSSCHE, B.
dc.contributor.authorVERDUGO, E.
dc.contributor.authorWAELKENS, C.
dc.contributor.authorWALKER, H.
dc.date.issued2009-11
dc.identifier.issn0032-0633
dc.description.abstractEn"Water and related chemistry in the Solar System" is a Herschel Space Observatory Guaranteed-Time Key Programme. This project, approved by the European Space Agency, aims at determining the distribution, the evolution and the origin of water in Mars, the outer planets, Titan, Enceladus and the comets. It addresses the broad topic of water and its isotopologues in planetary and cometary atmospheres. The nature of cometary activity and the thermodynamics of cometary comae will be investigated by studying water excitation in a sample of comets. The D/H ratio, the key parameter for constraining the origin and evolution of Solar System species, will be measured for the first time in a Jupiter-family comet. A comparison with existing and new measurements of D/H in Oort-cloud comets will constrain the composition of pre-solar cometary grains and possibly the dynamics of the protosolar nebula. New measurements of D/H in giant planets, similarly constraining the composition of proto-planetary ices, will be obtained. The D/H and other isotopic ratios, diagnostic of Mars' atmosphere evolution, will be accurately measured in H2O and CO. The role of water vapor in Mars' atmospheric chemistry will be studied by monitoring vertical profiles of H2O and HDO and by searching for several other species (and CO and H2O isotopes). A detailed study of the source of water in the upper atmosphere of the Giant Planets and Titan will be performed. By monitoring the water abundance, vertical profile, and input fluxes in the various objects, and when possible with the help of mapping observations, we will discriminate between the possible sources of water in the outer planets (interplanetary dust particles, cometary impacts, and local sources). In addition to these inter-connected objectives, serendipitous searches will enhance our knowledge of the composition of planetary and cometary atmospheres.
dc.language.isoen
dc.publisherElsevier
dc.subject.enHerschel spaceobservatory Water Mars Giant planets Titan Comets
dc.title.enWater and related chemistry in the solar system. A guaranteed time key programme for Herschel
dc.typeArticle de revue
dc.identifier.doi10.1016/J.PSS.2009.07.009
dc.subject.halPlanète et Univers [physics]/Astrophysique [astro-ph]/Planétologie et astrophysique de la terre [astro-ph.EP]
dc.subject.halPhysique [physics]/Astrophysique [astro-ph]/Planétologie et astrophysique de la terre [astro-ph.EP]
bordeaux.journalPlanetary and Space Science
bordeaux.page1596-1606
bordeaux.volume57
bordeaux.peerReviewedoui
hal.identifierhal-00439338
hal.version1
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-00439338v1
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