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Using this simplified model, we obtain a criterion showing that depending on the balance of the tidal dissipation in both planets, their final period ratio may stay at the resonant value, increase above, or decrease below the resonant value.\n  Applying this criterion to the two inner planets orbiting GJ163, we deduce that the current period ratio (2.9"},"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":"1404.4861","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.EP","submitted_at":"2014-04-18T19:22:32Z","cross_cats_sorted":[],"title_canon_sha256":"24f54df1caab1326598cffdee2c3f8066c32b11f1f9993bfbeb96901bdc0ab10","abstract_canon_sha256":"c3dd154dddace863b7d85ebcb6bfc1666a2339633a0b39a92def30cba4ab2b22"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:48:36.244107Z","signature_b64":"6BfuUizX5iUwJGHaUH+VzV6hsqnt1e5Dnh0n8DAhUpygsThVjNLC7FWkYfVvvWO7ETLCPrmJvje06de5EX5tBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"6bfec7f4629a3fa5e89ab2f11f15f8134a1e3577b4fe4253fbd2a3d064bebeb2","last_reissued_at":"2026-05-18T02:48:36.243601Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:48:36.243601Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Resonance breaking due to dissipation in planar planetary systems","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"A.C.M. 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