{"database":"biostudies-literature","file_versions":[],"scores":null,"additional":{"submitter":["Barnouin O"],"funding":["National Aeronautics and Space Administration (NASA)","Swiss National Science Foundation","European Commission (EC)","Agenzia Spaziale Italiana","National Aeronautics and Space Administration","European Commission","Agenzia Spaziale Italiana (Italian Space Agency)"],"pagination":["6202"],"full_dataset_link":["https://www.ebi.ac.uk/biostudies/studies/S-EPMC11289119"],"repository":["biostudies-literature"],"omics_type":["Unknown"],"volume":["15(1)"],"pubmed_abstract":["Images collected during NASA's Double Asteroid Redirection Test (DART) mission provide the first resolved views of the Didymos binary asteroid system. These images reveal that the primary asteroid, Didymos, is flattened and has plausible undulations along its equatorial perimeter. At high elevations, its surface is rough and contains large boulders and craters; at low elevations its surface is smooth and possesses fewer large boulders and craters. Didymos' moon, Dimorphos, possesses an intimate mixture of boulders, several asteroid-wide lineaments, and a handful of craters. The surfaces of both asteroids include boulders that are large relative to their host body, suggesting that both asteroids are rubble piles. Based on these observations, our models indicate that Didymos has a surface co"],"journal":["Nature communications"],"pubmed_title":["The geology and evolution of the Near-Earth binary asteroid system (65803) Didymos."],"pmcid":["PMC11289119"],"funding_grant_id":["200021","No 870377","80MSFC20D0004","n. 2019-31-HH.0","207359"],"pubmed_authors":["Agrusa H","Ieva S","Karatekin O","Barnouin O","Gai I","Mazzotta Epifani E","Impresario G","Walsh KJ","Ernst CM","CampoBagatin A","Rossi A","Chabot NL","Dotto E","Capannolo A","Bertini I","Trigo-Rodriguez JM","Farnham TL","Lavagn M","Stickle AM","Richardson DC","Deshapriya JDP","Pajola M","Cremonese G","Rivkin AS","Michel P","Beccarelli J","Palumbo P","Brucato JR","Tusberti F","Amoroso M","Asphaug E","Ivanovski SL","Jutzi M","Hasselmann PHA","Pirrotta S","Perna D","Rizos JL","Ferrari F","Zanotti G","Nolan MC","Della Corte V","Raducan SD","Cheng AF","Modenini D","Zannoni M","Ballouz RL","Dall'Ora M","Zinzi A","Poggiali G","Robin CQ","Li JY","Hirabayashi M","Daly RT","Kahout T","Vincent JB","Palmer E","Tortora P","Sunshine JM","Zhang Y","Marchi S","Murdoch N","Lucchetti A","Parro LM"],"additional_accession":[]},"is_claimable":false,"name":"The geology and evolution of the Near-Earth binary asteroid system (65803) Didymos.","description":"Images collected during NASA's Double Asteroid Redirection Test (DART) mission provide the first resolved views of the Didymos binary asteroid system. These images reveal that the primary asteroid, Didymos, is flattened and has plausible undulations along its equatorial perimeter. At high elevations, its surface is rough and contains large boulders and craters; at low elevations its surface is smooth and possesses fewer large boulders and craters. Didymos' moon, Dimorphos, possesses an intimate mixture of boulders, several asteroid-wide lineaments, and a handful of craters. The surfaces of both asteroids include boulders that are large relative to their host body, suggesting that both asteroids are rubble piles. Based on these observations, our models indicate that Didymos has a surface co","dates":{"release":"2024-01-01T00:00:00Z","publication":"2024 Jul","modification":"2025-04-04T00:21:53.898Z","creation":"2025-04-04T00:21:53.898Z"},"accession":"S-EPMC11289119","cross_references":{"pubmed":["39080262"],"doi":["10.1038/s41467-024-50146-x"]}}