{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2011:VGYKMLUBVMS4DETEBXFZHITERS","short_pith_number":"pith:VGYKMLUB","schema_version":"1.0","canonical_sha256":"a9b0a62e81ab25c192640dcb93a2648ca1041ac9e0957b09347ca3d11dbd9753","source":{"kind":"arxiv","id":"1107.2051","version":1},"attestation_state":"computed","paper":{"title":"Constraining Ceres' interior from its Rotational Motion","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.EP"],"primary_cat":"astro-ph.SR","authors_text":"JPL), Julie Castillo-Rogez (JPL), Nicolas Rambaux (IMCCE), Petr Kuchynka (IMCCE, V\\'eronique Dehant (ROB)","submitted_at":"2011-07-11T15:11:06Z","abstract_excerpt":"Context. Ceres is the most massive body of the asteroid belt and contains about 25 wt.% (weight percent) of water. Understanding its thermal evolution and assessing its current state are major goals of the Dawn Mission. Constraints on internal structure can be inferred from various observations. Especially, detailed knowledge of the rotational motion can help constrain the mass distribution inside the body, which in turn can lead to information on its geophysical history. Aims. We investigate the signature of the interior on the rotational motion of Ceres and discuss possible future measuremen"},"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":"1107.2051","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2011-07-11T15:11:06Z","cross_cats_sorted":["astro-ph.EP"],"title_canon_sha256":"c9249cbaa9a9c34acd9bc284e201359881eace35c1ea9ad5ccf21b941ba67df9","abstract_canon_sha256":"6676b5fd6066c6e64b56c3e677e422cf2b9a857a423fdbf4880619cb570a82cc"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:01:20.348613Z","signature_b64":"4QtVdhlef6LNtHYfgRqRItN+31VIqF/s/KGo1U2sQUMsGPJkyHu+jpUFkjOzMSuQxotqwpyGlsDfkbg1/dopDA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"a9b0a62e81ab25c192640dcb93a2648ca1041ac9e0957b09347ca3d11dbd9753","last_reissued_at":"2026-05-18T02:01:20.347675Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:01:20.347675Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Constraining Ceres' interior from its Rotational Motion","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.EP"],"primary_cat":"astro-ph.SR","authors_text":"JPL), Julie Castillo-Rogez (JPL), Nicolas Rambaux (IMCCE), Petr Kuchynka (IMCCE, V\\'eronique Dehant (ROB)","submitted_at":"2011-07-11T15:11:06Z","abstract_excerpt":"Context. Ceres is the most massive body of the asteroid belt and contains about 25 wt.% (weight percent) of water. Understanding its thermal evolution and assessing its current state are major goals of the Dawn Mission. Constraints on internal structure can be inferred from various observations. Especially, detailed knowledge of the rotational motion can help constrain the mass distribution inside the body, which in turn can lead to information on its geophysical history. Aims. We investigate the signature of the interior on the rotational motion of Ceres and discuss possible future measuremen"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1107.2051","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":"1107.2051","created_at":"2026-05-18T02:01:20.347842+00:00"},{"alias_kind":"arxiv_version","alias_value":"1107.2051v1","created_at":"2026-05-18T02:01:20.347842+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1107.2051","created_at":"2026-05-18T02:01:20.347842+00:00"},{"alias_kind":"pith_short_12","alias_value":"VGYKMLUBVMS4","created_at":"2026-05-18T12:26:44.992195+00:00"},{"alias_kind":"pith_short_16","alias_value":"VGYKMLUBVMS4DETE","created_at":"2026-05-18T12:26:44.992195+00:00"},{"alias_kind":"pith_short_8","alias_value":"VGYKMLUB","created_at":"2026-05-18T12:26:44.992195+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/VGYKMLUBVMS4DETEBXFZHITERS","json":"https://pith.science/pith/VGYKMLUBVMS4DETEBXFZHITERS.json","graph_json":"https://pith.science/api/pith-number/VGYKMLUBVMS4DETEBXFZHITERS/graph.json","events_json":"https://pith.science/api/pith-number/VGYKMLUBVMS4DETEBXFZHITERS/events.json","paper":"https://pith.science/paper/VGYKMLUB"},"agent_actions":{"view_html":"https://pith.science/pith/VGYKMLUBVMS4DETEBXFZHITERS","download_json":"https://pith.science/pith/VGYKMLUBVMS4DETEBXFZHITERS.json","view_paper":"https://pith.science/paper/VGYKMLUB","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1107.2051&json=true","fetch_graph":"https://pith.science/api/pith-number/VGYKMLUBVMS4DETEBXFZHITERS/graph.json","fetch_events":"https://pith.science/api/pith-number/VGYKMLUBVMS4DETEBXFZHITERS/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/VGYKMLUBVMS4DETEBXFZHITERS/action/timestamp_anchor","attest_storage":"https://pith.science/pith/VGYKMLUBVMS4DETEBXFZHITERS/action/storage_attestation","attest_author":"https://pith.science/pith/VGYKMLUBVMS4DETEBXFZHITERS/action/author_attestation","sign_citation":"https://pith.science/pith/VGYKMLUBVMS4DETEBXFZHITERS/action/citation_signature","submit_replication":"https://pith.science/pith/VGYKMLUBVMS4DETEBXFZHITERS/action/replication_record"}},"created_at":"2026-05-18T02:01:20.347842+00:00","updated_at":"2026-05-18T02:01:20.347842+00:00"}