The equatorial shape and gravity field of Mercury from MESSENGER flybys 1 and 2
David E. Smith(Nikon (United States)), Jürgen Oberst(Deutsches Zentrum für Luft- und Raumfahrt e. V. (DLR)), F. G. Lemoine(Goddard Space Flight Center), M. T. Zuber(Massachusetts Institute of Technology), O. S. Barnouin(Johns Hopkins University Applied Physics Laboratory), S. J. Peale(University of California, Santa Barbara), Sean C. Solomon(Lamont-Doherty Earth Observatory), J. W. Head(Planetary Science Institute), R. J. Phillips(Washington University in St. Louis), R. L. McNutt(Johns Hopkins University), G. A. Neumann(Goddard Space Flight Center), Jean‐Luc Margot(University of California, Los Angeles), M. E. Perry(Johns Hopkins University Applied Physics Laboratory), C. L. Johnson(Carnegie Institution for Science), Matthieu Talpe(Massachusetts Institute of Technology), M. H. Torrence(Jensen Hughes (United States)), S. A. Hauck(Washington University in St. Louis)
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