{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:RK3MV2DRHZIOSVBHFJGIHGULAT","short_pith_number":"pith:RK3MV2DR","schema_version":"1.0","canonical_sha256":"8ab6cae8713e50e954272a4c839a8b04d71bee789dacf36c141182eaa8c966c7","source":{"kind":"arxiv","id":"1703.02670","version":1},"attestation_state":"computed","paper":{"title":"The Spherical Bolometric Albedo of Planet Mercury","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"Anthony Mallama","submitted_at":"2017-03-08T02:03:35Z","abstract_excerpt":"Published reflectance data covering several different wavelength intervals has been combined and analyzed in order to determine the spherical bolometric albedo of Mercury. The resulting value of 0.088 +/- 0.003 spans wavelengths from 0 to 4 {\\mu}m which includes over 99% of the solar flux. This bolometric result is greater than the value determined between 0.43 and 1.01 {\\mu}m by Domingue et al. (2011, Planet. Space Sci., 59, 1853-1872). The difference is due to higher reflectivity at wavelengths beyond 1.01 {\\mu}m. The average effective blackbody temperature of Mercury corresponding to the ne"},"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":"1703.02670","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.EP","submitted_at":"2017-03-08T02:03:35Z","cross_cats_sorted":[],"title_canon_sha256":"410fce27f82c8037a1c943872a9cbfe99614955a430faadc7ab6846ae3316b3e","abstract_canon_sha256":"60d1e62bf2ce480e0c7ed301e3db849cd6402432cf25ea43c23801f14bac82f5"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:49:05.913380Z","signature_b64":"R6S+ca8KwtdxzwzIukmAwLWYV1uSoyI5MY6W6IZ+dC8v73qYzvZE5NBCVqG1r89ZorRUWOMcYRZHaajvAb2oCQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"8ab6cae8713e50e954272a4c839a8b04d71bee789dacf36c141182eaa8c966c7","last_reissued_at":"2026-05-18T00:49:05.912709Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:49:05.912709Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The Spherical Bolometric Albedo of Planet Mercury","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"Anthony Mallama","submitted_at":"2017-03-08T02:03:35Z","abstract_excerpt":"Published reflectance data covering several different wavelength intervals has been combined and analyzed in order to determine the spherical bolometric albedo of Mercury. The resulting value of 0.088 +/- 0.003 spans wavelengths from 0 to 4 {\\mu}m which includes over 99% of the solar flux. This bolometric result is greater than the value determined between 0.43 and 1.01 {\\mu}m by Domingue et al. (2011, Planet. Space Sci., 59, 1853-1872). The difference is due to higher reflectivity at wavelengths beyond 1.01 {\\mu}m. The average effective blackbody temperature of Mercury corresponding to the ne"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1703.02670","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":"1703.02670","created_at":"2026-05-18T00:49:05.912801+00:00"},{"alias_kind":"arxiv_version","alias_value":"1703.02670v1","created_at":"2026-05-18T00:49:05.912801+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1703.02670","created_at":"2026-05-18T00:49:05.912801+00:00"},{"alias_kind":"pith_short_12","alias_value":"RK3MV2DRHZIO","created_at":"2026-05-18T12:31:39.905425+00:00"},{"alias_kind":"pith_short_16","alias_value":"RK3MV2DRHZIOSVBH","created_at":"2026-05-18T12:31:39.905425+00:00"},{"alias_kind":"pith_short_8","alias_value":"RK3MV2DR","created_at":"2026-05-18T12:31:39.905425+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2605.00100","citing_title":"The dark and featureless surface of rocky exoplanet LHS 3844 b from JWST mid-infrared spectroscopy","ref_index":102,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/RK3MV2DRHZIOSVBHFJGIHGULAT","json":"https://pith.science/pith/RK3MV2DRHZIOSVBHFJGIHGULAT.json","graph_json":"https://pith.science/api/pith-number/RK3MV2DRHZIOSVBHFJGIHGULAT/graph.json","events_json":"https://pith.science/api/pith-number/RK3MV2DRHZIOSVBHFJGIHGULAT/events.json","paper":"https://pith.science/paper/RK3MV2DR"},"agent_actions":{"view_html":"https://pith.science/pith/RK3MV2DRHZIOSVBHFJGIHGULAT","download_json":"https://pith.science/pith/RK3MV2DRHZIOSVBHFJGIHGULAT.json","view_paper":"https://pith.science/paper/RK3MV2DR","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1703.02670&json=true","fetch_graph":"https://pith.science/api/pith-number/RK3MV2DRHZIOSVBHFJGIHGULAT/graph.json","fetch_events":"https://pith.science/api/pith-number/RK3MV2DRHZIOSVBHFJGIHGULAT/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/RK3MV2DRHZIOSVBHFJGIHGULAT/action/timestamp_anchor","attest_storage":"https://pith.science/pith/RK3MV2DRHZIOSVBHFJGIHGULAT/action/storage_attestation","attest_author":"https://pith.science/pith/RK3MV2DRHZIOSVBHFJGIHGULAT/action/author_attestation","sign_citation":"https://pith.science/pith/RK3MV2DRHZIOSVBHFJGIHGULAT/action/citation_signature","submit_replication":"https://pith.science/pith/RK3MV2DRHZIOSVBHFJGIHGULAT/action/replication_record"}},"created_at":"2026-05-18T00:49:05.912801+00:00","updated_at":"2026-05-18T00:49:05.912801+00:00"}