Reference : Water and related chemistry in the solar system. A guaranteed time key programme for ...
Scientific journals : Article
Physical, chemical, mathematical & earth Sciences : Space science, astronomy & astrophysics
http://hdl.handle.net/2268/24747
Water and related chemistry in the solar system. A guaranteed time key programme for Herschel
English
Hartogh, P. [Max Planck Institute for Solar System Research, 37191 Katlenburg-Lindau, Germany]
Lellouch, E. [LESIA, Observatoire de Paris, France]
Crovisier, J. [LESIA, Observatoire de Paris, France]
Banaszkiewicz, M. [Space Research Centre, Polish Academy of Sciences, Warsaw, Poland]
Bensch, F. [Argelander Institute für Astronomie, Universität Bonn, Germany; DLR, German Aerospace Centre, Bonn-Oberkassel, Germany]
Bergin, E. A. [Astronomy Department, University of Michigan, USA]
Billebaud, Françoise [Université de Bordeaux, Laboratoire dâ Astrophysique de Bordeaux, France; CNRS/INSU, UMR 5804, Floirac, France]
Biver, N. [LESIA, Observatoire de Paris, France]
Blake, G. A. [California Institute of Technology, Pasadena, USA]
Blecka, M. I. [Space Research Centre, Polish Academy of Sciences, Warsaw, Poland]
Blommaert, J. [Instituut voor Sterrenkunde, Katholieke Universiteit Leuven, Belgium]
Bockelée-Morvan, Dominique [LESIA, Observatoire de Paris, France]
Cavalié, T. [Max Planck Institute for Solar System Research, 37191 Katlenburg-Lindau, Germany]
Cernicharo, J. [Laboratory of Molecular Astrophysics, CAB-CSIC. INTA, Madrid, Spain]
Courtin, R. [LESIA, Observatoire de Paris, France]
Davis, G. [Joint Astronomy Centre, Hilo, USA]
Decin, L. [Instituut voor Sterrenkunde, Katholieke Universiteit Leuven, Belgium]
Encrenaz, P. [LERMA, Observatoire de Paris, France]
Encrenaz, T. [LESIA, Observatoire de Paris, France]
Gonzalez, A. [Max Planck Institute for Solar System Research, 37191 Katlenburg-Lindau, Germany; Instituto de Astrofísica de Andalucía-CSIC, Granada, Spain]
de Graauw, T. [SRON, Netherlands Institute for Space Research, Netherlands; Leiden University, Netherlands]
Hutsemekers, Damien mailto [Université de Liège - ULiège > Département d'astrophys., géophysique et océanographie (AGO) > Astroph. extragalactique et observations spatiales (AEOS) >]
Jarchow, C. [Max Planck Institute for Solar System Research, 37191 Katlenburg-Lindau, Germany]
Jehin, Emmanuel mailto [Université de Liège - ULiège > Département d'astrophys., géophysique et océanographie (AGO) > Astrophysique et traitement de l'image >]
Kidger, M. [Herschel Science Centre, European Space Astronomy Centre, European Space Agency, Madrid, Spain]
Küppers, M. [Rosetta Science Operations Centre, European Space Astronomy Centre, European Space Agency, Madrid, Spain]
de Lange, A. [SRON, Netherlands Institute for Space Research, Netherlands]
Lara, L*-M [Instituto de Astrofísica de Andalucía-CSIC, Granada, Spain]
Lis, D. C. [California Institute of Technology, Pasadena, USA]
Lorente, R. [Herschel Science Centre, European Space Astronomy Centre, European Space Agency, Madrid, Spain]
Manfroid, Jean mailto [Université de Liège - ULiège > Département d'astrophys., géophysique et océanographie (AGO) > Département d'astrophys., géophysique et océanographie (AGO) >]
Medvedev, A. S. [Max Planck Institute for Solar System Research, 37191 Katlenburg-Lindau, Germany]
Moreno, R. [LESIA, Observatoire de Paris, France]
Naylor, D. A. [Department of Physics and Astronomy, University of Lethbridge, Canada]
Orton, G. [Jet Propulsion Laboratory, California Institute of Technology, Pasadena, USA]
Portyankina, G. [Physikalisches Institut, University of Bern, Switzerland]
Rengel, M. [Max Planck Institute for Solar System Research, 37191 Katlenburg-Lindau, Germany]
Sagawa, H. [Max Planck Institute for Solar System Research, 37191 Katlenburg-Lindau, Germany]
Sanchez-Portal, M. [Herschel Science Centre, European Space Astronomy Centre, European Space Agency, Madrid, Spain]
Schieder, R. [1st Physics Institute, University of Cologne, Germany]
Sidher, S. [Space Science and Technology Department, Rutherford Appleton Laboratory, UK]
Stam, D. [SRON, Netherlands Institute for Space Research, Netherlands]
Swinyard, B. [Space Science and Technology Department, Rutherford Appleton Laboratory, UK]
Szutowicz, S. [Space Research Centre, Polish Academy of Sciences, Warsaw, Poland]
Thomas, N. [Physikalisches Institut, University of Bern, Switzerland]
Thornhill, G. [Herschel Science Centre, European Space Astronomy Centre, European Space Agency, Madrid, Spain]
Vandenbussche, B. [Instituut voor Sterrenkunde, Katholieke Universiteit Leuven, Belgium]
Verdugo, E. [Herschel Science Centre, European Space Astronomy Centre, European Space Agency, Madrid, Spain]
Waelkens, C. [Instituut voor Sterrenkunde, Katholieke Universiteit Leuven, Belgium]
Walker, H. [Space Science and Technology Department, Rutherford Appleton Laboratory, UK]
1-Nov-2009
Planetary and Space Science
Pergamon Press - An Imprint of Elsevier Science
57
1596-1606
Yes (verified by ORBi)
International
0032-0633
Oxford
United Kingdom
[en] â Water and related chemistry in the Solar Systemâ 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 Marsâ atmosphere evolution, will be accurately measured in H[SUB]2[/SUB]O and CO. The role of water vapor in Marsâ atmospheric chemistry will be studied by monitoring vertical profiles of H[SUB]2[/SUB]O and HDO and by searching for several other species (and CO and H[SUB]2[/SUB]O 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.
Researchers ; Students
http://hdl.handle.net/2268/24747
10.1016/j.pss.2009.07.009
http://cdsads.u-strasbg.fr/abs/2009P%26SS...57.1596H

File(s) associated to this reference

Fulltext file(s):

FileCommentaryVersionSizeAccess
Restricted access
sdarticle.pdfNo commentaryPublisher postprint330.68 kBRequest copy

Bookmark and Share SFX Query

All documents in ORBi are protected by a user license.