| Dawn arrives at Ceres: Exploration of a small, volatile-rich world CT Russell, CA Raymond, E Ammannito, DL Buczkowski, MC De Sanctis, ... Science 353 (6303), 1008-1010, 2016 | 199 | 2016 |
| A partially differentiated interior for (1) Ceres deduced from its gravity field and shape RS Park, AS Konopliv, BG Bills, N Rambaux, JC Castillo-Rogez, ... Nature 537 (7621), 515-517, 2016 | 192 | 2016 |
| Cratering on Ceres: Implications for its crust and evolution H Hiesinger, S Marchi, N Schmedemann, P Schenk, JH Pasckert, ... Science 353 (6303), aaf4759, 2016 | 158 | 2016 |
| Constraints on Ceres' internal structure and evolution from its shape and gravity measured by the Dawn spacecraft AI Ermakov, RR Fu, JC Castillo‐Rogez, CA Raymond, RS Park, ... Journal of Geophysical Research: Planets 122 (11), 2267-2293, 2017 | 136 | 2017 |
| The geomorphology of Ceres DL Buczkowski, BE Schmidt, DA Williams, SC Mest, JEC Scully, ... Science 353 (6303), aaf4332, 2016 | 129 | 2016 |
| The Vesta gravity field, spin pole and rotation period, landmark positions, and ephemeris from the Dawn tracking and optical data AS Konopliv, SW Asmar, RS Park, BG Bills, F Centinello, AB Chamberlin, ... Icarus 240, 103-117, 2014 | 128 | 2014 |
| The interior structure of Ceres as revealed by surface topography RR Fu, AI Ermakov, S Marchi, JC Castillo-Rogez, CA Raymond, ... Earth and Planetary Science Letters 476, 153-164, 2017 | 123 | 2017 |
| The missing large impact craters on Ceres S Marchi, AI Ermakov, CA Raymond, RR Fu, DP O’Brien, MT Bland, ... Nature Communications 7 (1), 12257, 2016 | 99 | 2016 |
| The Ceres gravity field, spin pole, rotation period and orbit from the Dawn radiometric tracking and optical data AS Konopliv, RS Park, AT Vaughan, BG Bills, SW Asmar, AI Ermakov, ... Icarus 299, 411-429, 2018 | 84 | 2018 |
| The vanishing cryovolcanoes of Ceres MM Sori, S Byrne, MT Bland, AM Bramson, AI Ermakov, CW Hamilton, ... Geophysical Research Letters 44 (3), 1243-1250, 2017 | 64 | 2017 |
| Constraints on Vesta’s interior structure using gravity and shape models from the Dawn mission AI Ermakov, MT Zuber, DE Smith, CA Raymond, G Balmino, RR Fu, ... Icarus 240, 146-160, 2014 | 58 | 2014 |
| High-resolution shape model of Ceres from stereophotoclinometry using Dawn imaging data RS Park, AT Vaughan, AS Konopliv, AI Ermakov, N Mastrodemos, ... Icarus 319, 812-827, 2019 | 54 | 2019 |
| Impact-driven mobilization of deep crustal brines on dwarf planet Ceres CA Raymond, AI Ermakov, JC Castillo-Rogez, S Marchi, BC Johnson, ... Nature Astronomy 4 (8), 741-747, 2020 | 53 | 2020 |
| Ceres: Astrobiological target and possible ocean world JC Castillo-Rogez, M Neveu, JEC Scully, CH House, LC Quick, ... Astrobiology 20 (2), 269-291, 2020 | 46 | 2020 |
| Conditions for the long‐term preservation of a deep brine reservoir in Ceres JC Castillo‐Rogez, MA Hesse, M Formisano, H Sizemore, M Bland, ... Geophysical Research Letters 46 (4), 1963-1972, 2019 | 45 | 2019 |
| Conditions for sublimating water ice to supply Ceres' exosphere ME Landis, S Byrne, N Schörghofer, BE Schmidt, PO Hayne, ... Journal of Geophysical Research: Planets 122 (10), 1984-1995, 2017 | 45 | 2017 |
| The Mercury gravity field, orientation, love number, and ephemeris from the MESSENGER radiometric tracking data AS Konopliv, RS Park, AI Ermakov Icarus 335, 113386, 2020 | 39 | 2020 |
| Ceres's obliquity history and its implications for the permanently shadowed regions AI Ermakov, E Mazarico, SE Schröder, U Carsenty, N Schorghofer, ... Geophysical Research Letters 44 (6), 2652-2661, 2017 | 38 | 2017 |
| The geology of the Kerwan quadrangle of dwarf planet Ceres: Investigating Ceres’ oldest, largest impact basin DA Williams, T Kneissl, A Neesemann, SC Mest, E Palomba, T Platz, ... Icarus 316, 99-113, 2018 | 37 | 2018 |
| Evidence for the interior evolution of Ceres from geologic analysis of fractures JEC Scully, DL Buczkowski, N Schmedemann, CA Raymond, ... Geophysical Research Letters 44 (19), 9564-9572, 2017 | 34 | 2017 |
Carol A. RaymondPrincipal Scientist, Jet Propulsion LaboratoryE-mail megerősítve itt: jpl.nasa.gov
