{"record":{"author":{"account_ref":null,"orcid":null},"builds_on":[],"content_schema":"pubphys.content.topic/1","content_sha256":"cdab3d6c47567dd05753b06b28f1faa2c0ef7679daae78e6a1bb356607ed27e7","created":"2026-10-03T07:17:50Z","files":[],"origin":{"assisted_by":[],"kind":"seed"},"parents":[],"salt":"6cae02c13e741e21bdf0eb2f4c20edd8fc2229c950469cc91136c4706711aaa2","schema":"pubphys.record/2","site":"pubphys.com","target":null,"type":"topic"},"content":{"external_id":"astro.hot-jupiters","field":"astro","n":"1","review_cite":"R. I. Dawson, J. A. Johnson, Origins of Hot Jupiters, Annual Review of Astronomy and Astrophysics, 2018","review_link":"https://arxiv.org/abs/1801.06117","review_verified":"true","summary":"Hot Jupiters are gas giants that orbit their stars in a few days, far inside the region where giant planets are thought to form. Whether they moved inward through the gas disk, were thrown inward onto stretched orbits that tides then made circular, or formed in place is still argued.","title":"Origin of hot Jupiters","topic_ref":null,"why":"They were the first planets found around Sun-like stars and test theories of planet migration and tides."},"attested":{"attestation":{"batch":null,"client_id":null,"id_token_sha256":null,"kind":"platform"},"record_hash":"1e0254cb819018d5ed8997a7e251ef6a68c90da1082e1990c43ed16b01153ec7","schema":"pubphys.attested/1"},"envelope":{"attested_hash":"261f659921f0f6213962deaeb48d93ec410fdad4b331f87fcf8c36c714266d74","platform_signature":{"key_id":"c6afc19b31429869751f06879c75cd64ea92654423d15b44be775bf1310a60da","sig":"BgjZMqkZh4BYL64gFUY2qGGa5GaGg7ARj6WqVk3SZxKwUOZ5rZ4XPNSA38ajF3ec58JdfFQjNfNxgSGUmmbVCw"},"schema":"pubphys.envelope/1"},"record_hash":"1e0254cb819018d5ed8997a7e251ef6a68c90da1082e1990c43ed16b01153ec7","leaf_index":42}