{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:6WV4ZU4WVUQVYLY34PN5HDEXMD","short_pith_number":"pith:6WV4ZU4W","schema_version":"1.0","canonical_sha256":"f5abccd396ad215c2f1be3dbd38c9760ead497c52b749ff33f49bab5c4faf3a2","source":{"kind":"arxiv","id":"1707.01234","version":2},"attestation_state":"computed","paper":{"title":"Origin of water in the inner Solar System: Planetesimals scattered inward during Jupiter and Saturn's rapid gas accretion","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.SR"],"primary_cat":"astro-ph.EP","authors_text":"Andre Izidoro, Sean N. Raymond","submitted_at":"2017-07-05T07:07:06Z","abstract_excerpt":"There is a long-standing debate regarding the origin of the terrestrial planets' water as well as the hydrated C-type asteroids. Here we show that the inner Solar System's water is a simple byproduct of the giant planets' formation. Giant planet cores accrete gas slowly until the conditions are met for a rapid phase of runaway growth. As a gas giant's mass rapidly increases, the orbits of nearby planetesimals are destabilized and gravitationally scattered in all directions. Under the action of aerodynamic gas drag, a fraction of scattered planetesimals are deposited onto stable orbits interior"},"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":"1707.01234","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.EP","submitted_at":"2017-07-05T07:07:06Z","cross_cats_sorted":["astro-ph.SR"],"title_canon_sha256":"e0280536e6e2a6c3040ac64bf872a515825b4e31c1691c33cd9c28b03aa6be5d","abstract_canon_sha256":"bef60440b1ae5925667048e498c5f38c04f496fc61abbc6155ae543fabc4ca90"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:36:08.564959Z","signature_b64":"najfmCY1a+TGv7SP49dwLX5mnee+nQfzyOg5J2ljWZRPXTsUdRZcQqy6ngFm4IfWFp/S5bZW/SruWCiAyChNDQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"f5abccd396ad215c2f1be3dbd38c9760ead497c52b749ff33f49bab5c4faf3a2","last_reissued_at":"2026-05-18T00:36:08.564289Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:36:08.564289Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Origin of water in the inner Solar System: Planetesimals scattered inward during Jupiter and Saturn's rapid gas accretion","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.SR"],"primary_cat":"astro-ph.EP","authors_text":"Andre Izidoro, Sean N. Raymond","submitted_at":"2017-07-05T07:07:06Z","abstract_excerpt":"There is a long-standing debate regarding the origin of the terrestrial planets' water as well as the hydrated C-type asteroids. Here we show that the inner Solar System's water is a simple byproduct of the giant planets' formation. Giant planet cores accrete gas slowly until the conditions are met for a rapid phase of runaway growth. As a gas giant's mass rapidly increases, the orbits of nearby planetesimals are destabilized and gravitationally scattered in all directions. Under the action of aerodynamic gas drag, a fraction of scattered planetesimals are deposited onto stable orbits interior"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1707.01234","kind":"arxiv","version":2},"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":"1707.01234","created_at":"2026-05-18T00:36:08.564413+00:00"},{"alias_kind":"arxiv_version","alias_value":"1707.01234v2","created_at":"2026-05-18T00:36:08.564413+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1707.01234","created_at":"2026-05-18T00:36:08.564413+00:00"},{"alias_kind":"pith_short_12","alias_value":"6WV4ZU4WVUQV","created_at":"2026-05-18T12:31:03.183658+00:00"},{"alias_kind":"pith_short_16","alias_value":"6WV4ZU4WVUQVYLY3","created_at":"2026-05-18T12:31:03.183658+00:00"},{"alias_kind":"pith_short_8","alias_value":"6WV4ZU4W","created_at":"2026-05-18T12:31:03.183658+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2605.31081","citing_title":"Oxidation Constraints on Terrestrial Planet Formation from a Ring","ref_index":34,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/6WV4ZU4WVUQVYLY34PN5HDEXMD","json":"https://pith.science/pith/6WV4ZU4WVUQVYLY34PN5HDEXMD.json","graph_json":"https://pith.science/api/pith-number/6WV4ZU4WVUQVYLY34PN5HDEXMD/graph.json","events_json":"https://pith.science/api/pith-number/6WV4ZU4WVUQVYLY34PN5HDEXMD/events.json","paper":"https://pith.science/paper/6WV4ZU4W"},"agent_actions":{"view_html":"https://pith.science/pith/6WV4ZU4WVUQVYLY34PN5HDEXMD","download_json":"https://pith.science/pith/6WV4ZU4WVUQVYLY34PN5HDEXMD.json","view_paper":"https://pith.science/paper/6WV4ZU4W","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1707.01234&json=true","fetch_graph":"https://pith.science/api/pith-number/6WV4ZU4WVUQVYLY34PN5HDEXMD/graph.json","fetch_events":"https://pith.science/api/pith-number/6WV4ZU4WVUQVYLY34PN5HDEXMD/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/6WV4ZU4WVUQVYLY34PN5HDEXMD/action/timestamp_anchor","attest_storage":"https://pith.science/pith/6WV4ZU4WVUQVYLY34PN5HDEXMD/action/storage_attestation","attest_author":"https://pith.science/pith/6WV4ZU4WVUQVYLY34PN5HDEXMD/action/author_attestation","sign_citation":"https://pith.science/pith/6WV4ZU4WVUQVYLY34PN5HDEXMD/action/citation_signature","submit_replication":"https://pith.science/pith/6WV4ZU4WVUQVYLY34PN5HDEXMD/action/replication_record"}},"created_at":"2026-05-18T00:36:08.564413+00:00","updated_at":"2026-05-18T00:36:08.564413+00:00"}