{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2025:24IZQXUXAEVAX53VNCSC36YVV6","short_pith_number":"pith:24IZQXUX","schema_version":"1.0","canonical_sha256":"d711985e97012a0bf77568a42dfb15af926f706b3cf414651d6c3bc23f781965","source":{"kind":"arxiv","id":"2507.13072","version":1},"attestation_state":"computed","paper":{"title":"A dynamical dichotomy in large binary asteroids","license":"http://creativecommons.org/licenses/by-nc-nd/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"A. Conrad, A. Martin, B. Carry, C. Dumas, D. Gorshanov, E. Jehin, E. Sokov, F. Vachier, I. Sokova, J. Berthier, J. Hanu\\v{s}, J. L. Margot, J. \\v{D}urech, K. B. Alton, K. Minker, L. Liberato, L. M. Close, M. Ferrais, M. Marsset, R. Behrend, R. Roy, W. J. Merline, W. M. Grundy","submitted_at":"2025-07-17T12:40:33Z","abstract_excerpt":"No less than 15% of large (diameter greater than 140 km) asteroids have satellites. The commonly accepted mechanism for their formation is post-impact reaccumulation. However, the detailed physical and dynamical properties of these systems are not well understood, and many of them have not been studied in detail. We aim to study the population of large binary asteroid systems. To do so, we compare the gravitational fields predicted from the shape of the primary body with the non-Keplerian gravitational components identified in orbital models of the satellites of each system. We also aim to con"},"verification_status":{"content_addressed":true,"pith_receipt":true,"author_attested":false,"weak_author_claims":0,"strong_author_claims":0,"externally_anchored":false,"storage_verified":false,"citation_signatures":0,"replication_records":0,"graph_snapshot":true,"references_resolved":false,"formal_links_present":false},"canonical_record":{"source":{"id":"2507.13072","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by-nc-nd/4.0/","primary_cat":"astro-ph.EP","submitted_at":"2025-07-17T12:40:33Z","cross_cats_sorted":[],"title_canon_sha256":"40c050164897845389fc768a8ddf55b974d44d3dca4c0c5cd899cc25b0d20623","abstract_canon_sha256":"b1d754ba1edd5f1bdfb031db97b9e1aaab888c42be2e68365a3adff709280d50"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T12:03:29.616643Z","signature_b64":"UotYSC1Zt3WhykoHhfEIWEy3Axzmuhx9X2fWADhqLE57ukg7EVz5a+uydS3RUJGdajycK1lJ8w9CPo8FdNnsCQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"d711985e97012a0bf77568a42dfb15af926f706b3cf414651d6c3bc23f781965","last_reissued_at":"2026-07-05T12:03:29.616137Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T12:03:29.616137Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A dynamical dichotomy in large binary asteroids","license":"http://creativecommons.org/licenses/by-nc-nd/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"A. Conrad, A. Martin, B. Carry, C. Dumas, D. Gorshanov, E. Jehin, E. Sokov, F. Vachier, I. Sokova, J. Berthier, J. Hanu\\v{s}, J. L. Margot, J. \\v{D}urech, K. B. Alton, K. Minker, L. Liberato, L. M. Close, M. Ferrais, M. Marsset, R. Behrend, R. Roy, W. J. Merline, W. M. Grundy","submitted_at":"2025-07-17T12:40:33Z","abstract_excerpt":"No less than 15% of large (diameter greater than 140 km) asteroids have satellites. The commonly accepted mechanism for their formation is post-impact reaccumulation. However, the detailed physical and dynamical properties of these systems are not well understood, and many of them have not been studied in detail. We aim to study the population of large binary asteroid systems. To do so, we compare the gravitational fields predicted from the shape of the primary body with the non-Keplerian gravitational components identified in orbital models of the satellites of each system. We also aim to con"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2507.13072","kind":"arxiv","version":1},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2507.13072/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"},"aliases":[{"alias_kind":"arxiv","alias_value":"2507.13072","created_at":"2026-07-05T12:03:29.616208+00:00"},{"alias_kind":"arxiv_version","alias_value":"2507.13072v1","created_at":"2026-07-05T12:03:29.616208+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2507.13072","created_at":"2026-07-05T12:03:29.616208+00:00"},{"alias_kind":"pith_short_12","alias_value":"24IZQXUXAEVA","created_at":"2026-07-05T12:03:29.616208+00:00"},{"alias_kind":"pith_short_16","alias_value":"24IZQXUXAEVAX53V","created_at":"2026-07-05T12:03:29.616208+00:00"},{"alias_kind":"pith_short_8","alias_value":"24IZQXUX","created_at":"2026-07-05T12:03:29.616208+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/24IZQXUXAEVAX53VNCSC36YVV6","json":"https://pith.science/pith/24IZQXUXAEVAX53VNCSC36YVV6.json","graph_json":"https://pith.science/api/pith-number/24IZQXUXAEVAX53VNCSC36YVV6/graph.json","events_json":"https://pith.science/api/pith-number/24IZQXUXAEVAX53VNCSC36YVV6/events.json","paper":"https://pith.science/paper/24IZQXUX"},"agent_actions":{"view_html":"https://pith.science/pith/24IZQXUXAEVAX53VNCSC36YVV6","download_json":"https://pith.science/pith/24IZQXUXAEVAX53VNCSC36YVV6.json","view_paper":"https://pith.science/paper/24IZQXUX","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2507.13072&json=true","fetch_graph":"https://pith.science/api/pith-number/24IZQXUXAEVAX53VNCSC36YVV6/graph.json","fetch_events":"https://pith.science/api/pith-number/24IZQXUXAEVAX53VNCSC36YVV6/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/24IZQXUXAEVAX53VNCSC36YVV6/action/timestamp_anchor","attest_storage":"https://pith.science/pith/24IZQXUXAEVAX53VNCSC36YVV6/action/storage_attestation","attest_author":"https://pith.science/pith/24IZQXUXAEVAX53VNCSC36YVV6/action/author_attestation","sign_citation":"https://pith.science/pith/24IZQXUXAEVAX53VNCSC36YVV6/action/citation_signature","submit_replication":"https://pith.science/pith/24IZQXUXAEVAX53VNCSC36YVV6/action/replication_record"}},"created_at":"2026-07-05T12:03:29.616208+00:00","updated_at":"2026-07-05T12:03:29.616208+00:00"}