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dc.contributor.authorDehant, V.
dc.contributor.authorBlanc, M.
dc.contributor.authorMackwell, S.
dc.contributor.authorSoderlund, K.M.
dc.contributor.authorBeck, P.
dc.contributor.authorBunce, E.
dc.contributor.authorCharnoz, S.
dc.contributor.authorFoing, B.
dc.contributor.authorFilice, V.
dc.contributor.authorFletcher, L.N.
dc.contributor.authorForget, F.
dc.contributor.authorGriton, L.
dc.contributor.authorHammel, H.
dc.contributor.authorHöning, D.
dc.contributor.authorImamura, T.
dc.contributor.authorJackman, C.
dc.contributor.authorKaspi, Y.
dc.contributor.authorKorablev, O.
dc.contributor.authorLeconte, J.
dc.contributor.authorLellouch, E.
dc.contributor.authorMarty, B.
dc.contributor.authorMangold, N.
dc.contributor.authorMichel, P.
dc.contributor.authorMorbidelli, A.
dc.contributor.authorMousis, O.
dc.contributor.authorPrieto-Ballesteros, O.
dc.contributor.authorSpohn, T.
dc.contributor.authorSchmidt, J.
dc.contributor.authorSterken, V.J.
dc.contributor.authorTosi, N.
dc.contributor.authorVandaele, A.C.
dc.contributor.authorVernazza, P.
dc.contributor.authorVazan, A.
dc.contributor.authorWestall, F.
dc.date2023
dc.date.accessioned2023-04-21T16:40:52Z
dc.date.available2023-04-21T16:40:52Z
dc.identifier.urihttps://orfeo.belnet.be/handle/internal/10949
dc.descriptionThis chapter reviews the way the six key questions about planetary systems, from their origins to the way they work and their habitability, identified in Chapter 1 (Blanc et al., 2021), can be addressed by means of solar system exploration, and how one can find partial answers to these six questions by flying to the different provinces to the solar system: terrestrial planets, giant planets, small bodies, and up to its interface with the local interstellar medium. It derives from this analysis a synthetic description of the most important space observations to be performed at the different solar system objects by future planetary exploration missions. These “observation requirements” illustrate the diversity of measurement techniques to be used as well as the diversity of destinations where these observations must be made. They constitute the base for the identification of the future planetary missions we need to fly by 2061, which are described in Chapter 4.
dc.languageeng
dc.publisherElsevier
dc.titleFrom science questions to Solar System exploration
dc.typeBook chapter
dc.subject.frascatiPhysical sciences
dc.audienceScientific
dc.subject.freeAsteroid
dc.subject.freeMedium
dc.subject.freePlanets
dc.subject.freeSmall bodies
dc.subject.freeSolar System
dc.source.titlePlanetary Exploration Horizon 2061
dc.source.page65-175
Orfeo.peerreviewedYes
dc.identifier.doi10.1016/B978-0-323-90226-7.00006-4
dc.identifier.scopus
dc.source.editorBlanc, M.
dc.source.editorBousquet, P.W.
dc.source.editorDehant, V.
dc.source.editorFoing, B.
dc.source.editorGrande, M.
dc.source.editorGuo, l.
dc.source.editorHutzler, A.
dc.source.editorLasue, J.
dc.source.editorLewis, J.
dc.source.editorPerino, M.-A.
dc.source.editorRauer, H.


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