{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:FJSNNTQMHO7PIBP7PYMP36OR46","short_pith_number":"pith:FJSNNTQM","schema_version":"1.0","canonical_sha256":"2a64d6ce0c3bbef405ff7e18fdf9d1e78afede3facafaa079387207ab4b256f0","source":{"kind":"arxiv","id":"1411.1378","version":1},"attestation_state":"computed","paper":{"title":"Planetary chaotic zone clearing: destinations and timescales","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"Renu Malhotra, Sarah Morrison","submitted_at":"2014-11-05T19:50:33Z","abstract_excerpt":"We investigate the orbital evolution of particles in a planet's chaotic zone to determine their final destinations and their timescales of clearing. There are four possible final states of chaotic particles: collision with the planet, collision with the star, escape, or bounded but non-collision orbits. In our investigations, within the framework of the planar circular restricted three body problem for planet-star mass ratio $\\mu$ in the range $10^{-9}$ to $10^{-1.5}$, we find no particles hitting the star. The relative frequencies of escape and collision with the planet are not scale-free, as"},"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":"1411.1378","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.EP","submitted_at":"2014-11-05T19:50:33Z","cross_cats_sorted":[],"title_canon_sha256":"0bb6f233e726436500f59e329ce257605a0a35779886352b2e5fac0b09be6461","abstract_canon_sha256":"ae5905fcbc6f785415386468a60a0d0060d467d04e6b1d3ec1c8f7d293b592ee"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:41:34.754453Z","signature_b64":"gBawdUBzQ85bSq5ljBP9N9HLq4hA03L+2nJaP5a4tKE/nW2siSjoWtbl1G7GqjquszedhARw/UoUahCI/8dlBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"2a64d6ce0c3bbef405ff7e18fdf9d1e78afede3facafaa079387207ab4b256f0","last_reissued_at":"2026-05-18T01:41:34.753789Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:41:34.753789Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Planetary chaotic zone clearing: destinations and timescales","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"Renu Malhotra, Sarah Morrison","submitted_at":"2014-11-05T19:50:33Z","abstract_excerpt":"We investigate the orbital evolution of particles in a planet's chaotic zone to determine their final destinations and their timescales of clearing. There are four possible final states of chaotic particles: collision with the planet, collision with the star, escape, or bounded but non-collision orbits. In our investigations, within the framework of the planar circular restricted three body problem for planet-star mass ratio $\\mu$ in the range $10^{-9}$ to $10^{-1.5}$, we find no particles hitting the star. The relative frequencies of escape and collision with the planet are not scale-free, as"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1411.1378","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":""},"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":"1411.1378","created_at":"2026-05-18T01:41:34.753882+00:00"},{"alias_kind":"arxiv_version","alias_value":"1411.1378v1","created_at":"2026-05-18T01:41:34.753882+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1411.1378","created_at":"2026-05-18T01:41:34.753882+00:00"},{"alias_kind":"pith_short_12","alias_value":"FJSNNTQMHO7P","created_at":"2026-05-18T12:28:28.263976+00:00"},{"alias_kind":"pith_short_16","alias_value":"FJSNNTQMHO7PIBP7","created_at":"2026-05-18T12:28:28.263976+00:00"},{"alias_kind":"pith_short_8","alias_value":"FJSNNTQM","created_at":"2026-05-18T12:28:28.263976+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/FJSNNTQMHO7PIBP7PYMP36OR46","json":"https://pith.science/pith/FJSNNTQMHO7PIBP7PYMP36OR46.json","graph_json":"https://pith.science/api/pith-number/FJSNNTQMHO7PIBP7PYMP36OR46/graph.json","events_json":"https://pith.science/api/pith-number/FJSNNTQMHO7PIBP7PYMP36OR46/events.json","paper":"https://pith.science/paper/FJSNNTQM"},"agent_actions":{"view_html":"https://pith.science/pith/FJSNNTQMHO7PIBP7PYMP36OR46","download_json":"https://pith.science/pith/FJSNNTQMHO7PIBP7PYMP36OR46.json","view_paper":"https://pith.science/paper/FJSNNTQM","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1411.1378&json=true","fetch_graph":"https://pith.science/api/pith-number/FJSNNTQMHO7PIBP7PYMP36OR46/graph.json","fetch_events":"https://pith.science/api/pith-number/FJSNNTQMHO7PIBP7PYMP36OR46/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/FJSNNTQMHO7PIBP7PYMP36OR46/action/timestamp_anchor","attest_storage":"https://pith.science/pith/FJSNNTQMHO7PIBP7PYMP36OR46/action/storage_attestation","attest_author":"https://pith.science/pith/FJSNNTQMHO7PIBP7PYMP36OR46/action/author_attestation","sign_citation":"https://pith.science/pith/FJSNNTQMHO7PIBP7PYMP36OR46/action/citation_signature","submit_replication":"https://pith.science/pith/FJSNNTQMHO7PIBP7PYMP36OR46/action/replication_record"}},"created_at":"2026-05-18T01:41:34.753882+00:00","updated_at":"2026-05-18T01:41:34.753882+00:00"}