Rationale for BepiColombo Studies of Mercury's Surface and Composition

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dc.contributor.author Rothery, David A.
dc.contributor.author Massironi, Matteo
dc.contributor.author Alemanno, Giulia
dc.contributor.author Barraud, Oceane
dc.contributor.author Besse, Sebastien
dc.contributor.author Bott, Nicolas
dc.contributor.author Brunetto, Rosario
dc.contributor.author Bunce, Emma
dc.contributor.author Byrne, Paul
dc.contributor.author Capaccioni, Fabrizio
dc.contributor.author Capria, Maria Teresa
dc.contributor.author Carli, Cristian
dc.contributor.author Charlier, Bernard
dc.contributor.author Cornet, Thomas
dc.contributor.author Cremonese, Gabriele
dc.contributor.author D'Amore, Mario
dc.contributor.author De Sanctis, M. Cristina
dc.contributor.author Doressoundiram, Alain
dc.contributor.author Ferranti, Luigi
dc.contributor.author Filacchione, Gianrico
dc.contributor.author Galluzzi, Valentina
dc.contributor.author Giacomini, Lorenza
dc.contributor.author Grande, Manuel
dc.contributor.author Guzzetta, Laura G.
dc.contributor.author Helbert, Joern
dc.contributor.author Heyner, Daniel
dc.contributor.author Hiesinger, Harald
dc.contributor.author Hussmann, Hauke
dc.contributor.author Hyodo, Ryuku
dc.contributor.author Kohout, Tomas
dc.contributor.author Kozyrev, Alexander
dc.contributor.author Litvak, Maxim
dc.contributor.author Lucchetti, Alice
dc.contributor.author Malakhov, Alexey
dc.contributor.author Malliband, Christopher
dc.contributor.author Mancinelli, Paolo
dc.contributor.author Martikainen, Julia
dc.contributor.author Martindale, Adrian
dc.contributor.author Maturilli, Alessandro
dc.contributor.author Milillo, Anna
dc.contributor.author Mitrofanov, Igor
dc.contributor.author Mokrousov, Maxim
dc.contributor.author Morlok, Andreas
dc.contributor.author Muinonen, Karri
dc.contributor.author Namur, Olivier
dc.contributor.author Owens, Alan
dc.contributor.author Nittler, Larry R.
dc.contributor.author Oliveira, Joana S.
dc.contributor.author Palumbo, Pasquale
dc.contributor.author Pajola, Maurizio
dc.contributor.author Pegg, David L.
dc.contributor.author Penttilä, Antti
dc.contributor.author Politi, Romolo
dc.contributor.author Quarati, Francesco
dc.contributor.author Re, Cristina
dc.contributor.author Sanin, Anton
dc.contributor.author Schulz, Rita
dc.contributor.author Stangarone, Claudia
dc.contributor.author Stojic, Aleksandra
dc.contributor.author Tretiyakov, Vladislav
dc.contributor.author Vaisanen, Timo
dc.contributor.author Varatharajan, Indhu
dc.contributor.author Weber, Iris
dc.contributor.author Wright, Jack
dc.contributor.author Wurz, Peter
dc.contributor.author Zambon, Francesca
dc.date.accessioned 2020-06-29T11:36:02Z
dc.date.available 2020-06-29T11:36:02Z
dc.date.issued 2020-06-02
dc.identifier.citation Rothery , D A , Massironi , M , Alemanno , G , Barraud , O , Besse , S , Bott , N , Brunetto , R , Bunce , E , Byrne , P , Capaccioni , F , Capria , M T , Carli , C , Charlier , B , Cornet , T , Cremonese , G , D'Amore , M , De Sanctis , M C , Doressoundiram , A , Ferranti , L , Filacchione , G , Galluzzi , V , Giacomini , L , Grande , M , Guzzetta , L G , Helbert , J , Heyner , D , Hiesinger , H , Hussmann , H , Hyodo , R , Kohout , T , Kozyrev , A , Litvak , M , Lucchetti , A , Malakhov , A , Malliband , C , Mancinelli , P , Martikainen , J , Martindale , A , Maturilli , A , Milillo , A , Mitrofanov , I , Mokrousov , M , Morlok , A , Muinonen , K , Namur , O , Owens , A , Nittler , L R , Oliveira , J S , Palumbo , P , Pajola , M , Pegg , D L , Penttilä , A , Politi , R , Quarati , F , Re , C , Sanin , A , Schulz , R , Stangarone , C , Stojic , A , Tretiyakov , V , Vaisanen , T , Varatharajan , I , Weber , I , Wright , J , Wurz , P & Zambon , F 2020 , ' Rationale for BepiColombo Studies of Mercury's Surface and Composition ' , Space Science Reviews , vol. 216 , no. 4 , 66 . https://doi.org/10.1007/s11214-020-00694-7
dc.identifier.other PURE: 139768004
dc.identifier.other PURE UUID: 5f9d9b7e-dd00-4d41-8527-7d2220061b68
dc.identifier.other WOS: 000538121700001
dc.identifier.other ORCID: /0000-0003-4458-3650/work/76723464
dc.identifier.other ORCID: /0000-0001-7403-1721/work/76723622
dc.identifier.other ORCID: /0000-0001-8058-2642/work/76724343
dc.identifier.other ORCID: /0000-0003-2211-4001/work/76725737
dc.identifier.uri http://hdl.handle.net/10138/317028
dc.description.abstract BepiColombo has a larger and in many ways more capable suite of instruments relevant for determination of the topographic, physical, chemical and mineralogical properties of Mercury's surface than the suite carried by NASA's MESSENGER spacecraft. Moreover, BepiColombo's data rate is substantially higher. This equips it to confirm, elaborate upon, and go beyond many of MESSENGER's remarkable achievements. Furthermore, the geometry of BepiColombo's orbital science campaign, beginning in 2026, will enable it to make uniformly resolved observations of both northern and southern hemispheres. This will offer more detailed and complete imaging and topographic mapping, element mapping with better sensitivity and improved spatial resolution, and totally new mineralogical mapping. We discuss MESSENGER data in the context of preparing for BepiColombo, and describe the contributions that we expect BepiColombo to make towards increased knowledge and understanding of Mercury's surface and its composition. Much current work, including analysis of analogue materials, is directed towards better preparing ourselves to understand what BepiColombo might reveal. Some of MESSENGER's more remarkable observations were obtained under unique or extreme conditions. BepiColombo should be able to confirm the validity of these observations and reveal the extent to which they are representative of the planet as a whole. It will also make new observations to clarify geological processes governing and reflecting crustal origin and evolution. We anticipate that the insights gained into Mercury's geological history and its current space weathering environment will enable us to better understand the relationships of surface chemistry, morphologies and structures with the composition of crustal types, including the nature and mobility of volatile species. This will enable estimation of the composition of the mantle from which the crust was derived, and lead to tighter constraints on models for Mercury's origin including the nature and original heliocentric distance of the material from which it formed. en
dc.format.extent 46
dc.language.iso eng
dc.relation.ispartof Space Science Reviews
dc.rights cc_by
dc.rights.uri info:eu-repo/semantics/openAccess
dc.subject BepiColombo
dc.subject Mercury
dc.subject Volatiles
dc.subject Crust
dc.subject Tectonism
dc.subject Volcanism
dc.subject X-RAY-FLUORESCENCE
dc.subject NORTH POLAR-REGION
dc.subject EXPLOSIVE VOLCANISM
dc.subject CALORIS BASIN
dc.subject WATER ICE
dc.subject SPECTROSCOPIC PROPERTIES
dc.subject SILICATE FRACTIONATION
dc.subject REFLECTANCE SPECTRA
dc.subject GLOBAL DISTRIBUTION
dc.subject METEOROID STREAM
dc.subject 115 Astronomy, Space science
dc.subject 114 Physical sciences
dc.title Rationale for BepiColombo Studies of Mercury's Surface and Composition en
dc.type Review Article
dc.contributor.organization Geology and Geophysics
dc.contributor.organization Department of Geosciences and Geography
dc.contributor.organization Planetary-system research
dc.contributor.organization Department of Physics
dc.contributor.organization Particle Physics and Astrophysics
dc.description.reviewstatus Peer reviewed
dc.relation.doi https://doi.org/10.1007/s11214-020-00694-7
dc.relation.issn 0038-6308
dc.rights.accesslevel openAccess
dc.type.version publishedVersion

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