{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2008:BTJJNHIIMSOVHDCMWJHAF4H6YL","short_pith_number":"pith:BTJJNHII","schema_version":"1.0","canonical_sha256":"0cd2969d08649d538c4cb24e02f0fec2de899ddac28698a555e725d161ddddf5","source":{"kind":"arxiv","id":"0806.1689","version":1},"attestation_state":"computed","paper":{"title":"Formation and accretion history of terrestrial planets from runaway growth through to late time: implications for orbital eccentricity","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"Ben Moore, Joachim Stadel, Max W. Schmidt, Ryuji Morishima","submitted_at":"2008-06-10T15:19:08Z","abstract_excerpt":"Remnant planetesimals might have played an important role in reducing the orbital eccentricities of the terrestrial planets after their formation via giant impacts. However, the population and the size distribution of remnant planetesimals during and after the giant impact stage are unknown, because simulations of planetary accretion in the runaway growth and giant impact stages have been conducted independently. Here we report results of direct N-body simulations of the formation of terrestrial planets beginning with a compact planetesimal disk. The initial planetesimal disk has a total mass "},"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":"0806.1689","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph","submitted_at":"2008-06-10T15:19:08Z","cross_cats_sorted":[],"title_canon_sha256":"653636a49fa84ca2baace133422c6d91460df5e0571a9a207c062db67fa9a33c","abstract_canon_sha256":"5e746f0b79ea70b75ab55bbcbd196825aecb9b4cea913b9e19047ad053faa9f0"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T17:11:13.334960Z","signature_b64":"vg1uvgf0yqifODn3CJrKM/qwzyurkQOiqTI9XUzOZjmZSkf0TB860cJ5ZbdRgLzgpK2/uYWzSZKGFbL4rNN2Bw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"0cd2969d08649d538c4cb24e02f0fec2de899ddac28698a555e725d161ddddf5","last_reissued_at":"2026-07-04T17:11:13.334562Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T17:11:13.334562Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Formation and accretion history of terrestrial planets from runaway growth through to late time: implications for orbital eccentricity","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"Ben Moore, Joachim Stadel, Max W. Schmidt, Ryuji Morishima","submitted_at":"2008-06-10T15:19:08Z","abstract_excerpt":"Remnant planetesimals might have played an important role in reducing the orbital eccentricities of the terrestrial planets after their formation via giant impacts. However, the population and the size distribution of remnant planetesimals during and after the giant impact stage are unknown, because simulations of planetary accretion in the runaway growth and giant impact stages have been conducted independently. Here we report results of direct N-body simulations of the formation of terrestrial planets beginning with a compact planetesimal disk. The initial planetesimal disk has a total mass "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"0806.1689","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/0806.1689/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":"0806.1689","created_at":"2026-07-04T17:11:13.334621+00:00"},{"alias_kind":"arxiv_version","alias_value":"0806.1689v1","created_at":"2026-07-04T17:11:13.334621+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.0806.1689","created_at":"2026-07-04T17:11:13.334621+00:00"},{"alias_kind":"pith_short_12","alias_value":"BTJJNHIIMSOV","created_at":"2026-07-04T17:11:13.334621+00:00"},{"alias_kind":"pith_short_16","alias_value":"BTJJNHIIMSOVHDCM","created_at":"2026-07-04T17:11:13.334621+00:00"},{"alias_kind":"pith_short_8","alias_value":"BTJJNHII","created_at":"2026-07-04T17:11:13.334621+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/BTJJNHIIMSOVHDCMWJHAF4H6YL","json":"https://pith.science/pith/BTJJNHIIMSOVHDCMWJHAF4H6YL.json","graph_json":"https://pith.science/api/pith-number/BTJJNHIIMSOVHDCMWJHAF4H6YL/graph.json","events_json":"https://pith.science/api/pith-number/BTJJNHIIMSOVHDCMWJHAF4H6YL/events.json","paper":"https://pith.science/paper/BTJJNHII"},"agent_actions":{"view_html":"https://pith.science/pith/BTJJNHIIMSOVHDCMWJHAF4H6YL","download_json":"https://pith.science/pith/BTJJNHIIMSOVHDCMWJHAF4H6YL.json","view_paper":"https://pith.science/paper/BTJJNHII","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=0806.1689&json=true","fetch_graph":"https://pith.science/api/pith-number/BTJJNHIIMSOVHDCMWJHAF4H6YL/graph.json","fetch_events":"https://pith.science/api/pith-number/BTJJNHIIMSOVHDCMWJHAF4H6YL/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/BTJJNHIIMSOVHDCMWJHAF4H6YL/action/timestamp_anchor","attest_storage":"https://pith.science/pith/BTJJNHIIMSOVHDCMWJHAF4H6YL/action/storage_attestation","attest_author":"https://pith.science/pith/BTJJNHIIMSOVHDCMWJHAF4H6YL/action/author_attestation","sign_citation":"https://pith.science/pith/BTJJNHIIMSOVHDCMWJHAF4H6YL/action/citation_signature","submit_replication":"https://pith.science/pith/BTJJNHIIMSOVHDCMWJHAF4H6YL/action/replication_record"}},"created_at":"2026-07-04T17:11:13.334621+00:00","updated_at":"2026-07-04T17:11:13.334621+00:00"}