Gravity, Geodesy and Fundamental Physics with BepiColombo’s MORE Investigation

dc.contributor.authorIess, L.
dc.contributor.authorAsmar, S. W.
dc.contributor.authorCappuccio, P.
dc.contributor.authorCascioli,  Gael
dc.contributor.authoret al
dc.date.accessioned2023-01-19T20:45:53Z
dc.date.available2023-01-19T20:45:53Z
dc.date.issued2021-02-08
dc.descriptionAuthors:- L. Iess , S.W. Asmar , P. Cappuccio , Gael Cascioli , F. De Marchi , I. di Stefano , A. Genova , N. Ashby , J.P. Barriot , P. Bender , C. Benedetto , J.S. Border , F. Budnik , S. Ciarcia , T. Damour , V. Dehant , G. Di Achille , A. Di Ruscio , A. Fienga , R. Formaro , S. Klioner , A. Konopliv , A. Lemaître , F. Longo , M. Mercolino , G. Mitri , V. Notaro , A. Olivieri , M. Paik , A. Palli , G. Schettino , D. Serra , L. Simone , G. Tommei , P. Tortora , T. Van Hoolst , D. Vokrouhlický , M. Watkins , X. Wu , M. Zannonien_US
dc.description.abstractThe Mercury Orbiter Radio Science Experiment (MORE) of the ESA mission BepiColombo will provide an accurate estimation of Mercury’s gravity field and rotational state, improved tests of general relativity, and a novel deep space navigation system. The key experimental setup entails a highly stable, multi-frequency radio link in X and Ka band, enabling two-way range rate measurements of 3 micron/s at nearly all solar elongation angles. In addition, a high chip rate, pseudo-noise ranging system has already been tested at 1-2 cm accuracy. The tracking data will be used together with the measurements of the Italian Spring Accelerometer to provide a pseudo drag free environment for the data analysis. We summarize the existing literature published over the past years and report on the overall configuration of the experiment, its operations in cruise and at Mercury, and the expected scientific results.en_US
dc.description.sponsorshipThe authors would like to thank the ESA BepiColombo Project for its continuous support. The MORE team acknowledges the crucial and inspiring contribution of the late Andrea Milani, who died prematurely on Nov. 28, 2018. LI, PC, GC, GDA, FDM, IDS, AG, ADR, VN, GM, AP, GS, DS, GT, PT, MZ acknowledge support from the Italian Space Agency (grant 2017-40-H.1-2020). This work was carried out, in part, at the Jet Propulsion Laboratory, California Institute of Technology, under contract for the National Aeronautics and Space Administration.en_US
dc.description.urihttps://link.springer.com/article/10.1007/s11214-021-00800-3en_US
dc.format.extent39 pagesen_US
dc.genrejournal articlesen_US
dc.identifierdoi:10.13016/m2k33j-j05q
dc.identifier.citationIess, L., Asmar, S.W., Cappuccio, P. et al. Gravity, Geodesy and Fundamental Physics with BepiColombo’s MORE Investigation. Space Sci Rev 217, 21 (2021). https://doi.org/10.1007/s11214-021-00800-3en_US
dc.identifier.urihttps://doi.org/10.1007/s11214-021-00800-3
dc.identifier.urihttp://hdl.handle.net/11603/26690
dc.language.isoen_USen_US
dc.publisherSpringer Natureen_US
dc.relation.isAvailableAtThe University of Maryland, Baltimore County (UMBC)
dc.relation.ispartofUMBC Center for Space Sciences and Technology
dc.relation.ispartofUMBC Faculty Collection
dc.rightsThis work was written as part of one of the author's official duties as an Employee of the United States Government and is therefore a work of the United States Government. In accordance with 17 U.S.C. 105, no copyright protection is available for such works under U.S. Law.en_US
dc.rightsPublic Domain Mark 1.0*
dc.rights.urihttp://creativecommons.org/publicdomain/mark/1.0/*
dc.titleGravity, Geodesy and Fundamental Physics with BepiColombo’s MORE Investigationen_US
dc.typeTexten_US
dcterms.creatorhttps://orcid.org/0000-0001-9070-7947en_US

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