{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2020:FIEVQ5YJSFIZMMZJXJPS2KIZ3R","short_pith_number":"pith:FIEVQ5YJ","schema_version":"1.0","canonical_sha256":"2a095877099151963329ba5f2d2919dc6fdbc73b1e9be008f9a0b8a9aedae703","source":{"kind":"arxiv","id":"2010.00146","version":2},"attestation_state":"computed","paper":{"title":"Beyond Equilibrium Temperature: How the Atmosphere/Interior Connection Affects the Onset of Methane, Ammonia, and Clouds in Warm Transiting Giant Planets","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"Callie E. Hood, Channon Visscher, Daniel P. Thorngren, Jonathan J. Fortney, Mark S. Marley, Michael R. Line, Richard S. Freedman, Roxana Lupu","submitted_at":"2020-09-30T23:27:22Z","abstract_excerpt":"The atmospheric pressure-temperature profiles for transiting giant planets cross a range of chemical transitions. Here we show that the particular shape of these irradiated profiles for warm giant planets below 1300 K lead to striking differences in the behavior of non-equilibrium chemistry compared to brown dwarfs of similar temperatures. Our particular focus is H$_2$O, CO, CH$_4$, CO$_2$, and NH$_3$ in Jupiter- and Neptune-class planets. We show the cooling history of a planet, which depends most significantly on planetary mass and age, can have a dominant effect on abundances in the visible"},"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":"2010.00146","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.EP","submitted_at":"2020-09-30T23:27:22Z","cross_cats_sorted":[],"title_canon_sha256":"2a79643d77f00500b7b4137eb874c058878631b1afd6adbfcf46089d0a87601f","abstract_canon_sha256":"b8c0e5a4c7a6c0aeb080faf4b7d2c1cc51410c5ee25015a236217fbb7efc04ee"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T01:56:10.532987Z","signature_b64":"6GFRcP3BpRTiFrvwid8GpyFmJdiHhVOPl9wZlmGD2fi9t+GUWGQ1kq7yTJljUY0YX09qIz2S3TOaBFgk0BUiCg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"2a095877099151963329ba5f2d2919dc6fdbc73b1e9be008f9a0b8a9aedae703","last_reissued_at":"2026-07-05T01:56:10.532617Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T01:56:10.532617Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Beyond Equilibrium Temperature: How the Atmosphere/Interior Connection Affects the Onset of Methane, Ammonia, and Clouds in Warm Transiting Giant Planets","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"Callie E. Hood, Channon Visscher, Daniel P. Thorngren, Jonathan J. Fortney, Mark S. Marley, Michael R. Line, Richard S. Freedman, Roxana Lupu","submitted_at":"2020-09-30T23:27:22Z","abstract_excerpt":"The atmospheric pressure-temperature profiles for transiting giant planets cross a range of chemical transitions. Here we show that the particular shape of these irradiated profiles for warm giant planets below 1300 K lead to striking differences in the behavior of non-equilibrium chemistry compared to brown dwarfs of similar temperatures. Our particular focus is H$_2$O, CO, CH$_4$, CO$_2$, and NH$_3$ in Jupiter- and Neptune-class planets. We show the cooling history of a planet, which depends most significantly on planetary mass and age, can have a dominant effect on abundances in the visible"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2010.00146","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2010.00146/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":"2010.00146","created_at":"2026-07-05T01:56:10.532665+00:00"},{"alias_kind":"arxiv_version","alias_value":"2010.00146v2","created_at":"2026-07-05T01:56:10.532665+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2010.00146","created_at":"2026-07-05T01:56:10.532665+00:00"},{"alias_kind":"pith_short_12","alias_value":"FIEVQ5YJSFIZ","created_at":"2026-07-05T01:56:10.532665+00:00"},{"alias_kind":"pith_short_16","alias_value":"FIEVQ5YJSFIZMMZJ","created_at":"2026-07-05T01:56:10.532665+00:00"},{"alias_kind":"pith_short_8","alias_value":"FIEVQ5YJ","created_at":"2026-07-05T01:56:10.532665+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/FIEVQ5YJSFIZMMZJXJPS2KIZ3R","json":"https://pith.science/pith/FIEVQ5YJSFIZMMZJXJPS2KIZ3R.json","graph_json":"https://pith.science/api/pith-number/FIEVQ5YJSFIZMMZJXJPS2KIZ3R/graph.json","events_json":"https://pith.science/api/pith-number/FIEVQ5YJSFIZMMZJXJPS2KIZ3R/events.json","paper":"https://pith.science/paper/FIEVQ5YJ"},"agent_actions":{"view_html":"https://pith.science/pith/FIEVQ5YJSFIZMMZJXJPS2KIZ3R","download_json":"https://pith.science/pith/FIEVQ5YJSFIZMMZJXJPS2KIZ3R.json","view_paper":"https://pith.science/paper/FIEVQ5YJ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2010.00146&json=true","fetch_graph":"https://pith.science/api/pith-number/FIEVQ5YJSFIZMMZJXJPS2KIZ3R/graph.json","fetch_events":"https://pith.science/api/pith-number/FIEVQ5YJSFIZMMZJXJPS2KIZ3R/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/FIEVQ5YJSFIZMMZJXJPS2KIZ3R/action/timestamp_anchor","attest_storage":"https://pith.science/pith/FIEVQ5YJSFIZMMZJXJPS2KIZ3R/action/storage_attestation","attest_author":"https://pith.science/pith/FIEVQ5YJSFIZMMZJXJPS2KIZ3R/action/author_attestation","sign_citation":"https://pith.science/pith/FIEVQ5YJSFIZMMZJXJPS2KIZ3R/action/citation_signature","submit_replication":"https://pith.science/pith/FIEVQ5YJSFIZMMZJXJPS2KIZ3R/action/replication_record"}},"created_at":"2026-07-05T01:56:10.532665+00:00","updated_at":"2026-07-05T01:56:10.532665+00:00"}