R
R. G. Sandness
Publications - 2
Citations - 265
R. G. Sandness is an academic researcher. The author has contributed to research in topics: Planetary system & Planet. The author has an hindex of 1, co-authored 1 publications receiving 246 citations.
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A ring system detected around the centaur (10199) chariklo
Felipe Braga-Ribas,Bruno Sicardy,Jose Luis Ortiz,Colin Snodgrass,F. Roques,R. Vieira-Martins,R. Vieira-Martins,R. Vieira-Martins,Julio Camargo,Marcelo Assafin,Rene Duffard,Emmanuel Jehin,Joe Pollock,Rodrigo Leiva,Marcelo Emilio,D. I. Machado,C. Colazo,E. Lellouch,Jesper Skottfelt,Jesper Skottfelt,Michaël Gillon,N. Ligier,L. Maquet,G. Benedetti-Rossi,A. Ramos Gomes,Pierre Kervella,Hektor Monteiro,Rafael Sfair,M. El Moutamid,M. El Moutamid,Gonzalo Tancredi,J. Spagnotto,Alain Maury,Nicolás Morales,Ricardo Gil-Hutton,S. Roland,A. Ceretta,Shenghong Gu,Xuefeng Wang,Kasper Harpsøe,Kasper Harpsøe,Markus Rabus,Markus Rabus,Jean Manfroid,Cyrielle Opitom,L. Vanzi,L. Mehret,L. Lorenzini,E. M. Schneiter,R. Melia,J. Lecacheux,François Colas,Frédéric Vachier,Thomas Widemann,L. Almenares,R. G. Sandness,F. Char,V. Perez,P. Lemos,Nicolás Marín Martínez,U. G. Jørgensen,U. G. Jørgensen,Martin Dominik,Fernando Roig,Daniel E. Reichart,Aaron P. LaCluyze,J. B. Haislip,K. M. Ivarsen,J. P. Moore,N. R. Frank,D. G. Lambas,D. G. Lambas +71 more
TL;DR: Observations of a multichord stellar occultation revealed the presence of a ring system around (10199) Chariklo, which is a Centaur—that is, one of a class of small objects orbiting primarily between Jupiter and Neptune—with an equivalent radius of 124 9 kilometres.
Characterization of the ejecta from NASA/DART impact on Dimorphos: observations and Monte Carlo models
Fernando Moreno,A. Campo Bagatin,Gonzalo Tancredi,Jian-Yang Li,Alessandro Rossi,Fabio Ferrari,Masatoshi Hirabayashi,Eugene G. Fahnestock,A. Maury,R. G. Sandness,Andrew S. Rivkin,Andrew F. Cheng,Tony L. Farnham,Stefania Soldini,C. Giordano,G. Merisio,Paolo Panicucci,M. Pugliatti,A. J. Castro-Tirado,Emilio Fernandez-Garcia,I. Perez-Garcia,Stavro Ivanovski,A. Penttila,Ludmilla Kolokolova,Javier Licandro,O. Munoz,Zuri Gray,Jose Luis Ortiz,Zhong Lin +28 more
TL;DR: In this paper , the authors provide a characterization of the ejecta dust properties, i.e., particle size distribution and ejection speeds, ejection geometric parameters, and mass, by combining both observational data sets, and by using Monte Carlo models of the observed dust tail.