{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2003:X54X26NTDQ33VMYLVSPFIDUVA4","short_pith_number":"pith:X54X26NT","schema_version":"1.0","canonical_sha256":"bf797d79b31c37bab30bac9e540e95072daf9922deb27f502a3e5e439e8f4c55","source":{"kind":"arxiv","id":"astro-ph/0301458","version":3},"attestation_state":"computed","paper":{"title":"Resonance Occupation in the Kuiper Belt: Case Examples of the 5:2 and Trojan Resonances","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"A. B. Jordan (UC Berkeley), D. E. Trilling (U Penn), E. I. Chiang, J. L. Elliot, K. J. Meech (IfA Hawaii), L. H. Wasserman (Lowell Observatory), M. W. Buie, R. L. Millis, & R. M. Wagner (U Arizona), S. D. Kern (MIT)","submitted_at":"2003-01-22T21:01:11Z","abstract_excerpt":"As part of our ongoing Deep Ecliptic Survey (DES) of the Kuiper belt, we report on the occupation of the 1:1 (Trojan), 4:3, 3:2, 7:4, 2:1, and 5:2 Neptunian mean-motion resonances (MMRs). The occupation of the 1:1 and 5:2 MMRs is not easily understood within the standard model of resonance sweeping by a migratory Neptune over an initially dynamically cold belt. Our dynamically hot, 5:2 resonant objects can librate with modest amplitudes of 90 deg within the resonance for at least 1 Gyr. Their trajectories cannot be explained by close encounters with Neptune alone, given the latter's current or"},"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":"astro-ph/0301458","kind":"arxiv","version":3},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2003-01-22T21:01:11Z","cross_cats_sorted":[],"title_canon_sha256":"dde1ab6bebf595df4bb5fe5f095930f99c88085f20649473ad9f1314a3f14e69","abstract_canon_sha256":"0bfaf327b9c1f5c68976ad206820d6b22398108796eea391463b6110ce269b0b"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T16:36:22.116540Z","signature_b64":"ZuE1yXdR41xbT0rDvAUtTIcXoULtQcaPkYggp6kY9XM23q1lcCv+6dDbsoH5JLjnu+DrrP5dzvVR2mdMILqkAQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"bf797d79b31c37bab30bac9e540e95072daf9922deb27f502a3e5e439e8f4c55","last_reissued_at":"2026-07-04T16:36:22.116171Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T16:36:22.116171Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Resonance Occupation in the Kuiper Belt: Case Examples of the 5:2 and Trojan Resonances","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"A. B. Jordan (UC Berkeley), D. E. Trilling (U Penn), E. I. Chiang, J. L. Elliot, K. J. Meech (IfA Hawaii), L. H. Wasserman (Lowell Observatory), M. W. Buie, R. L. Millis, & R. M. Wagner (U Arizona), S. D. Kern (MIT)","submitted_at":"2003-01-22T21:01:11Z","abstract_excerpt":"As part of our ongoing Deep Ecliptic Survey (DES) of the Kuiper belt, we report on the occupation of the 1:1 (Trojan), 4:3, 3:2, 7:4, 2:1, and 5:2 Neptunian mean-motion resonances (MMRs). The occupation of the 1:1 and 5:2 MMRs is not easily understood within the standard model of resonance sweeping by a migratory Neptune over an initially dynamically cold belt. Our dynamically hot, 5:2 resonant objects can librate with modest amplitudes of 90 deg within the resonance for at least 1 Gyr. Their trajectories cannot be explained by close encounters with Neptune alone, given the latter's current or"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0301458","kind":"arxiv","version":3},"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/astro-ph/0301458/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":"astro-ph/0301458","created_at":"2026-07-04T16:36:22.116240+00:00"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/0301458v3","created_at":"2026-07-04T16:36:22.116240+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/0301458","created_at":"2026-07-04T16:36:22.116240+00:00"},{"alias_kind":"pith_short_12","alias_value":"X54X26NTDQ33","created_at":"2026-07-04T16:36:22.116240+00:00"},{"alias_kind":"pith_short_16","alias_value":"X54X26NTDQ33VMYL","created_at":"2026-07-04T16:36:22.116240+00:00"},{"alias_kind":"pith_short_8","alias_value":"X54X26NT","created_at":"2026-07-04T16:36:22.116240+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/X54X26NTDQ33VMYLVSPFIDUVA4","json":"https://pith.science/pith/X54X26NTDQ33VMYLVSPFIDUVA4.json","graph_json":"https://pith.science/api/pith-number/X54X26NTDQ33VMYLVSPFIDUVA4/graph.json","events_json":"https://pith.science/api/pith-number/X54X26NTDQ33VMYLVSPFIDUVA4/events.json","paper":"https://pith.science/paper/X54X26NT"},"agent_actions":{"view_html":"https://pith.science/pith/X54X26NTDQ33VMYLVSPFIDUVA4","download_json":"https://pith.science/pith/X54X26NTDQ33VMYLVSPFIDUVA4.json","view_paper":"https://pith.science/paper/X54X26NT","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=astro-ph/0301458&json=true","fetch_graph":"https://pith.science/api/pith-number/X54X26NTDQ33VMYLVSPFIDUVA4/graph.json","fetch_events":"https://pith.science/api/pith-number/X54X26NTDQ33VMYLVSPFIDUVA4/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/X54X26NTDQ33VMYLVSPFIDUVA4/action/timestamp_anchor","attest_storage":"https://pith.science/pith/X54X26NTDQ33VMYLVSPFIDUVA4/action/storage_attestation","attest_author":"https://pith.science/pith/X54X26NTDQ33VMYLVSPFIDUVA4/action/author_attestation","sign_citation":"https://pith.science/pith/X54X26NTDQ33VMYLVSPFIDUVA4/action/citation_signature","submit_replication":"https://pith.science/pith/X54X26NTDQ33VMYLVSPFIDUVA4/action/replication_record"}},"created_at":"2026-07-04T16:36:22.116240+00:00","updated_at":"2026-07-04T16:36:22.116240+00:00"}