Rationale for BepiColombo Studies of Mercury’s Surface and Composition

Autor: Rothery, David A., Massironi, Matteo, Alemanno, Giulia, Barraud, Océane, 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, Jörn, 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, Väisänen, Timo, Varatharajan, Indhu, Weber, Iris, Wright, Jack, Wurz, Peter, Zambon, Francesca

BepiColombo has a larger and in many ways more capable suite of instrumentsrelevant for determination of the topographic, physical, chemical and mineralogical proper-ties of Mercury’s surface than the suite carried by NASA’s MESSENGER spacecraft.

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_________::33830da389a9a46d5038adf0bb48fb0c