{"corpus_id":18658829,"paper_sha":"01302f0d12a8998c8e4dbe10381eedb18af8d071","doi":"10.1051/0004-6361:20053355","arxiv_id":"astro-ph/0506656","pmid":null,"pmcid":null,"mag_id":1971209491,"dblp_id":null,"acl_id":null,"title":"On the V-type asteroids outside the Vesta family. I. Interplay of nonlinear secular resonances and the Yarkovsky effect: the cases of 956 Elisa and 809 Lundia","year":2005,"publication_date":"2005-06-27","venue":"","journal":{"name":"Astronomy and Astrophysics","pages":"819-829","volume":"441"},"journal_issn":null,"journal_title":null,"publication_types":[],"pubmed_pub_types":null,"s2_fields_of_study":["Physics"],"reference_count":32,"citation_count":84,"influential_citation_count":10,"is_open_access":true,"arxiv_categories":["astro-ph"],"arxiv_license":null,"arxiv_journal_ref":null,"mesh_headings":null,"chemicals":null,"comments_corrections":null,"source_flags":1,"s2_open_access_pdf_url":"https://www.aanda.org/articles/aa/pdf/2005/38/aa3355-05.pdf","s2_open_access_landing_url":"https://www.semanticscholar.org/paper/01302f0d12a8998c8e4dbe10381eedb18af8d071","s2_open_access_license":null,"s2_open_access_status":"BRONZE","pmc_open_access_pdf_url":null,"pmc_open_access_landing_url":null,"pmc_open_access_license":null,"pmc_open_access_status":null,"unpaywall_open_access_pdf_url":null,"unpaywall_open_access_landing_url":null,"unpaywall_open_access_license":null,"unpaywall_open_access_status":null,"abstract":"Among the largest objects in the main belt, asteroid 4 Vesta is unique in showing a basaltic crust. It is also the biggest member of the Vesta family, which is supposed to originate from a large cratering event about 1 Gyr ago (Marzari et al. 1996, AA ii) why their size is significantly larger than that of the typical member of the Vesta family; and iii) provide a lower limit on the Vesta family age. We believe that other V-type asteroids could have followed the same path, and could currently be inside the z 2 resonance. 
In an forthcoming article of this series we will investigate the role that other mechanisms of dynamical mobility, such as close encounters with massive asteroids, may have played in causing the current orbital distribution of the remaining 20 other V-type asteroids.","claims":[{"public_id":"cl_b3bb77cf89786512a331137d558f282e","status":"active","text":"Asteroids 956 Elisa and 809 Lundia are V-type asteroids outside the Vesta family that have been captured in the z2 secular resonance, likely due to the Yarkovsky effect.","confidence":0.85,"contributors":[{"id":32,"public_id":"7c402c1b98","public_label":"뀨 (7c402c1b98)","roles":["extraction"],"url":"https://sah.borca.ai/u/7c402c1b98"},{"id":35,"public_id":"b2adb6bfad","public_label":"Anonymous (b2adb6bfad)","roles":["review"],"url":"https://sah.borca.ai/u/b2adb6bfad"},{"id":1,"public_id":"12632b8b5f","public_label":"Anonymous 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(12632b8b5f)","roles":["review"],"url":"https://sah.borca.ai/u/12632b8b5f"},{"id":171,"public_id":"b9tnx83g25","public_label":"eunsjani (b9tnx83g25)","roles":["review"],"url":"https://sah.borca.ai/u/b9tnx83g25"}],"url":"https://sah.borca.ai/claims/cl_e7f8cfcc86b483183c8fc6768673c3cd"},{"public_id":"cl_7db87eaad25704a72f76b4c8f91c390c","status":"active","text":"The capture of 956 Elisa and 809 Lundia into the z2 resonance explains their larger size compared to typical Vesta family members and provides a lower limit on the Vesta family age.","confidence":0.8,"contributors":[{"id":32,"public_id":"7c402c1b98","public_label":"뀨 (7c402c1b98)","roles":["extraction"],"url":"https://sah.borca.ai/u/7c402c1b98"},{"id":35,"public_id":"b2adb6bfad","public_label":"Anonymous (b2adb6bfad)","roles":["review"],"url":"https://sah.borca.ai/u/b2adb6bfad"},{"id":1,"public_id":"12632b8b5f","public_label":"Anonymous 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