{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2012:7YBKX7F4MFCHWGKB7OJ2MQBZSH","short_pith_number":"pith:7YBKX7F4","schema_version":"1.0","canonical_sha256":"fe02abfcbc61447b1941fb93a6403991d97780a17419d5b5394a4156ad7b9de7","source":{"kind":"arxiv","id":"1207.3171","version":2},"attestation_state":"computed","paper":{"title":"Dissipation in planar resonant planetary systems","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"A. C. M. Correia, G. Bou\\'e, J.-B. Delisle, J. Laskar","submitted_at":"2012-07-13T08:45:47Z","abstract_excerpt":"Close-in planetary systems detected by the Kepler mission present an excess of periods ratio that are just slightly larger than some low order resonant values. This feature occurs naturally when resonant couples undergo dissipation that damps the eccentricities. However, the resonant angles appear to librate at the end of the migration process, which is often believed to be an evidence that the systems remain in resonance.\n  Here we provide an analytical model for the dissipation in resonant planetary systems valid for low eccentricities. We confirm that dissipation accounts for an excess of p"},"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":"1207.3171","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.EP","submitted_at":"2012-07-13T08:45:47Z","cross_cats_sorted":[],"title_canon_sha256":"a6f6f030798fb20faa6ae5dddb53ee8773c20ddca7bf67c5947a953474f5e087","abstract_canon_sha256":"831271adce6003e58eba7c0e38585afd0fe40852ec7ef82ff09dbb6cc226b6ca"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:56:24.076593Z","signature_b64":"+n5Prlaq0X9ijV5rFQUzmul4uQSB2ZkZILWNGQpynPUjLKZdK+WbSeJZt7IeVlV9rbIAH443VLjakcNPgr/oCQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"fe02abfcbc61447b1941fb93a6403991d97780a17419d5b5394a4156ad7b9de7","last_reissued_at":"2026-05-18T01:56:24.076074Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:56:24.076074Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Dissipation in planar resonant planetary systems","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"A. C. M. Correia, G. Bou\\'e, J.-B. Delisle, J. Laskar","submitted_at":"2012-07-13T08:45:47Z","abstract_excerpt":"Close-in planetary systems detected by the Kepler mission present an excess of periods ratio that are just slightly larger than some low order resonant values. This feature occurs naturally when resonant couples undergo dissipation that damps the eccentricities. However, the resonant angles appear to librate at the end of the migration process, which is often believed to be an evidence that the systems remain in resonance.\n  Here we provide an analytical model for the dissipation in resonant planetary systems valid for low eccentricities. We confirm that dissipation accounts for an excess of p"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1207.3171","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":"1207.3171","created_at":"2026-05-18T01:56:24.076158+00:00"},{"alias_kind":"arxiv_version","alias_value":"1207.3171v2","created_at":"2026-05-18T01:56:24.076158+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1207.3171","created_at":"2026-05-18T01:56:24.076158+00:00"},{"alias_kind":"pith_short_12","alias_value":"7YBKX7F4MFCH","created_at":"2026-05-18T12:26:58.693483+00:00"},{"alias_kind":"pith_short_16","alias_value":"7YBKX7F4MFCHWGKB","created_at":"2026-05-18T12:26:58.693483+00:00"},{"alias_kind":"pith_short_8","alias_value":"7YBKX7F4","created_at":"2026-05-18T12:26:58.693483+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2607.01559","citing_title":"CHEOPS observations of V1298 Tau: updated planetary densities and implications on the early evolution of the young system","ref_index":65,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/7YBKX7F4MFCHWGKB7OJ2MQBZSH","json":"https://pith.science/pith/7YBKX7F4MFCHWGKB7OJ2MQBZSH.json","graph_json":"https://pith.science/api/pith-number/7YBKX7F4MFCHWGKB7OJ2MQBZSH/graph.json","events_json":"https://pith.science/api/pith-number/7YBKX7F4MFCHWGKB7OJ2MQBZSH/events.json","paper":"https://pith.science/paper/7YBKX7F4"},"agent_actions":{"view_html":"https://pith.science/pith/7YBKX7F4MFCHWGKB7OJ2MQBZSH","download_json":"https://pith.science/pith/7YBKX7F4MFCHWGKB7OJ2MQBZSH.json","view_paper":"https://pith.science/paper/7YBKX7F4","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1207.3171&json=true","fetch_graph":"https://pith.science/api/pith-number/7YBKX7F4MFCHWGKB7OJ2MQBZSH/graph.json","fetch_events":"https://pith.science/api/pith-number/7YBKX7F4MFCHWGKB7OJ2MQBZSH/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/7YBKX7F4MFCHWGKB7OJ2MQBZSH/action/timestamp_anchor","attest_storage":"https://pith.science/pith/7YBKX7F4MFCHWGKB7OJ2MQBZSH/action/storage_attestation","attest_author":"https://pith.science/pith/7YBKX7F4MFCHWGKB7OJ2MQBZSH/action/author_attestation","sign_citation":"https://pith.science/pith/7YBKX7F4MFCHWGKB7OJ2MQBZSH/action/citation_signature","submit_replication":"https://pith.science/pith/7YBKX7F4MFCHWGKB7OJ2MQBZSH/action/replication_record"}},"created_at":"2026-05-18T01:56:24.076158+00:00","updated_at":"2026-05-18T01:56:24.076158+00:00"}