Rationale for BepiColombo Studies of Mercury's Surface and Composition

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http://hdl.handle.net/10138/317028

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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

Julkaisun nimi: Rationale for BepiColombo Studies of Mercury's Surface and Composition
Tekijä: Rothery, David A.; Massironi, Matteo; Alemanno, Giulia; Barraud, Oceane; Besse, Sebastien; Bott, Nicolas; Brunetto, Rosario; Bunce, Emma; Byrne, Paul; Capaccioni, Fabrizio; Capria, Maria Teresa; Carli, Cristian; Charlier, Bernard; Cornet, Thomas; Cremonese, Gabriele; D'Amore, Mario; De Sanctis, M. Cristina; Doressoundiram, Alain; Ferranti, Luigi; Filacchione, Gianrico; Galluzzi, Valentina; Giacomini, Lorenza; Grande, Manuel; Guzzetta, Laura G.; Helbert, Joern; Heyner, Daniel; Hiesinger, Harald; Hussmann, Hauke; Hyodo, Ryuku; Kohout, Tomas; Kozyrev, Alexander; Litvak, Maxim; Lucchetti, Alice; Malakhov, Alexey; Malliband, Christopher; Mancinelli, Paolo; Martikainen, Julia; Martindale, Adrian; Maturilli, Alessandro; Milillo, Anna; Mitrofanov, Igor; Mokrousov, Maxim; Morlok, Andreas; Muinonen, Karri; Namur, Olivier; Owens, Alan; Nittler, Larry R.; Oliveira, Joana S.; Palumbo, Pasquale; Pajola, Maurizio; Pegg, David L.; Penttilä, Antti; Politi, Romolo; Quarati, Francesco; Re, Cristina; Sanin, Anton; Schulz, Rita; Stangarone, Claudia; Stojic, Aleksandra; Tretiyakov, Vladislav; Vaisanen, Timo; Varatharajan, Indhu; Weber, Iris; Wright, Jack; Wurz, Peter; Zambon, Francesca
Tekijän organisaatio: Geology and Geophysics
Department of Geosciences and Geography
Planetary-system research
Department of Physics
Particle Physics and Astrophysics
Päiväys: 2020-06-02
Kieli: eng
Sivumäärä: 46
Kuuluu julkaisusarjaan: Space Science Reviews
ISSN: 0038-6308
DOI-tunniste: https://doi.org/10.1007/s11214-020-00694-7
URI: http://hdl.handle.net/10138/317028
Tiivistelmä: 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.
Avainsanat: BepiColombo
Mercury
Volatiles
Crust
Tectonism
Volcanism
X-RAY-FLUORESCENCE
NORTH POLAR-REGION
EXPLOSIVE VOLCANISM
CALORIS BASIN
WATER ICE
SPECTROSCOPIC PROPERTIES
SILICATE FRACTIONATION
REFLECTANCE SPECTRA
GLOBAL DISTRIBUTION
METEOROID STREAM
115 Astronomy, Space science
114 Physical sciences
Vertaisarvioitu: Kyllä
Tekijänoikeustiedot: cc_by
Pääsyrajoitteet: openAccess
Rinnakkaistallennettu versio: publishedVersion


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