{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2022:CLYN7DKMIK7HWX42IS2LPG4GLV","short_pith_number":"pith:CLYN7DKM","schema_version":"1.0","canonical_sha256":"12f0df8d4c42be7b5f9a44b4b79b865d7dd39b3ceb237add2196fed6273726a2","source":{"kind":"arxiv","id":"2203.10023","version":1},"attestation_state":"computed","paper":{"title":"Geophysical Evolution During Rocky Planet Formation","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.SR","physics.ao-ph","physics.geo-ph"],"primary_cat":"astro-ph.EP","authors_text":"Laura K. Schaefer, Miki Nakajima, Rebecca A. Fischer, Tim Lichtenberg","submitted_at":"2022-03-18T15:41:51Z","abstract_excerpt":"Progressive astronomical characterization of planet-forming disks and rocky exoplanets highlight the need for increasing interdisciplinary efforts to understand the birth and life cycle of terrestrial worlds in a unified picture. Here, we review major geophysical and geochemical processes that shape the evolution of rocky planets and their precursor planetesimals during planetary formation and early evolution, and how these map onto the astrophysical timeline and varying accretion environments of planetary growth. The evolution of the coupled core-mantle-atmosphere system of growing protoplane"},"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":"2203.10023","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.EP","submitted_at":"2022-03-18T15:41:51Z","cross_cats_sorted":["astro-ph.SR","physics.ao-ph","physics.geo-ph"],"title_canon_sha256":"fbe8650f05732e3fc6288e7156e0f73dd36c59793caa87e1cf8f366bbaec918d","abstract_canon_sha256":"d7a01c508557f51e15a724e585190a51055c3286929558c40f780a7e4b01f58a"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T04:06:27.058355Z","signature_b64":"iZzf/qnauCcxDV6V163EEtT5LJtJnNqskNVG+ojiPGiToHtUuRdKoYs8BU16fBlCba8TedVQ4YNqkznB0UHrAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"12f0df8d4c42be7b5f9a44b4b79b865d7dd39b3ceb237add2196fed6273726a2","last_reissued_at":"2026-07-05T04:06:27.057833Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T04:06:27.057833Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Geophysical Evolution During Rocky Planet Formation","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.SR","physics.ao-ph","physics.geo-ph"],"primary_cat":"astro-ph.EP","authors_text":"Laura K. Schaefer, Miki Nakajima, Rebecca A. Fischer, Tim Lichtenberg","submitted_at":"2022-03-18T15:41:51Z","abstract_excerpt":"Progressive astronomical characterization of planet-forming disks and rocky exoplanets highlight the need for increasing interdisciplinary efforts to understand the birth and life cycle of terrestrial worlds in a unified picture. Here, we review major geophysical and geochemical processes that shape the evolution of rocky planets and their precursor planetesimals during planetary formation and early evolution, and how these map onto the astrophysical timeline and varying accretion environments of planetary growth. The evolution of the coupled core-mantle-atmosphere system of growing protoplane"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2203.10023","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/2203.10023/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":"2203.10023","created_at":"2026-07-05T04:06:27.057888+00:00"},{"alias_kind":"arxiv_version","alias_value":"2203.10023v1","created_at":"2026-07-05T04:06:27.057888+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2203.10023","created_at":"2026-07-05T04:06:27.057888+00:00"},{"alias_kind":"pith_short_12","alias_value":"CLYN7DKMIK7H","created_at":"2026-07-05T04:06:27.057888+00:00"},{"alias_kind":"pith_short_16","alias_value":"CLYN7DKMIK7HWX42","created_at":"2026-07-05T04:06:27.057888+00:00"},{"alias_kind":"pith_short_8","alias_value":"CLYN7DKM","created_at":"2026-07-05T04:06:27.057888+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":4,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2605.29914","citing_title":"Modeling carbon outgassing from chondritic planetesimals","ref_index":58,"is_internal_anchor":false},{"citing_arxiv_id":"2606.24757","citing_title":"Coupled atmospHere Interior modeL Intercomparison (CHILI). I. Evolutionary Modelling -- Primordial Magma Oceans of Earth and Venus","ref_index":124,"is_internal_anchor":false},{"citing_arxiv_id":"2605.11819","citing_title":"Reaccumulation process after a catastrophic disruption event on a differentiated asteroid","ref_index":70,"is_internal_anchor":false},{"citing_arxiv_id":"2604.15304","citing_title":"A Validated Low-to-Intermediate Mass Planetary Interior Structure Model and New Mass-Radius Relations","ref_index":2,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/CLYN7DKMIK7HWX42IS2LPG4GLV","json":"https://pith.science/pith/CLYN7DKMIK7HWX42IS2LPG4GLV.json","graph_json":"https://pith.science/api/pith-number/CLYN7DKMIK7HWX42IS2LPG4GLV/graph.json","events_json":"https://pith.science/api/pith-number/CLYN7DKMIK7HWX42IS2LPG4GLV/events.json","paper":"https://pith.science/paper/CLYN7DKM"},"agent_actions":{"view_html":"https://pith.science/pith/CLYN7DKMIK7HWX42IS2LPG4GLV","download_json":"https://pith.science/pith/CLYN7DKMIK7HWX42IS2LPG4GLV.json","view_paper":"https://pith.science/paper/CLYN7DKM","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2203.10023&json=true","fetch_graph":"https://pith.science/api/pith-number/CLYN7DKMIK7HWX42IS2LPG4GLV/graph.json","fetch_events":"https://pith.science/api/pith-number/CLYN7DKMIK7HWX42IS2LPG4GLV/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/CLYN7DKMIK7HWX42IS2LPG4GLV/action/timestamp_anchor","attest_storage":"https://pith.science/pith/CLYN7DKMIK7HWX42IS2LPG4GLV/action/storage_attestation","attest_author":"https://pith.science/pith/CLYN7DKMIK7HWX42IS2LPG4GLV/action/author_attestation","sign_citation":"https://pith.science/pith/CLYN7DKMIK7HWX42IS2LPG4GLV/action/citation_signature","submit_replication":"https://pith.science/pith/CLYN7DKMIK7HWX42IS2LPG4GLV/action/replication_record"}},"created_at":"2026-07-05T04:06:27.057888+00:00","updated_at":"2026-07-05T04:06:27.057888+00:00"}