{"title":"共振附近近轨小行星对的动力学演化","authors":"A. E. Potoskuev, E. Kuznetsov","doi":"10.15826/b978-5-7996-2935-9.66","DOIUrl":null,"url":null,"abstract":"Dynamical evolution of asteroid pairs in close orbits near Jovian mean motion resonances (3 : 1, 4 : 1, 5 : 2, 7 : 3) has been researched. We analyzed scenarios of pair’s dynamical evolution by integrating the equations of motion in the future and past. It’s shown, that the op-portunity of close encountering, as well as the possibility of scattering under passing through the resonances, is dependent on the asteroids’ semimajor axis drifts values and signs due to the Yarkovsky effect.","PeriodicalId":183711,"journal":{"name":"Proceedings of the 48-th International student's conferences \"Physics of Space\"","volume":"1 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"1900-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"DYNAMICAL EVOLUTION OF ASTEROID PAIRS IN CLOSE ORBITS NEAR RESONANCES\",\"authors\":\"A. E. Potoskuev, E. Kuznetsov\",\"doi\":\"10.15826/b978-5-7996-2935-9.66\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"Dynamical evolution of asteroid pairs in close orbits near Jovian mean motion resonances (3 : 1, 4 : 1, 5 : 2, 7 : 3) has been researched. We analyzed scenarios of pair’s dynamical evolution by integrating the equations of motion in the future and past. It’s shown, that the op-portunity of close encountering, as well as the possibility of scattering under passing through the resonances, is dependent on the asteroids’ semimajor axis drifts values and signs due to the Yarkovsky effect.\",\"PeriodicalId\":183711,\"journal\":{\"name\":\"Proceedings of the 48-th International student's conferences \\\"Physics of Space\\\"\",\"volume\":\"1 1\",\"pages\":\"0\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"1900-01-01\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Proceedings of the 48-th International student's conferences \\\"Physics of Space\\\"\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/10.15826/b978-5-7996-2935-9.66\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Proceedings of the 48-th International student's conferences \"Physics of Space\"","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.15826/b978-5-7996-2935-9.66","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
DYNAMICAL EVOLUTION OF ASTEROID PAIRS IN CLOSE ORBITS NEAR RESONANCES
Dynamical evolution of asteroid pairs in close orbits near Jovian mean motion resonances (3 : 1, 4 : 1, 5 : 2, 7 : 3) has been researched. We analyzed scenarios of pair’s dynamical evolution by integrating the equations of motion in the future and past. It’s shown, that the op-portunity of close encountering, as well as the possibility of scattering under passing through the resonances, is dependent on the asteroids’ semimajor axis drifts values and signs due to the Yarkovsky effect.