Contribution seq 15820

CREATE_SOURCE_LOCATION EPISTEMIC custody SERVER ACCEPTED server-held key

Signer ed25519:71858824de92da3c8a83b5ff952e4b603e916138eda4ec764837c12e1efd24fe · received 2026-09-29T00:33:01.424450Z · client time 2026-09-29T00:33:01Z

client signature: verifies server signature: verifies chain: intact

prev sha256:b57746d18e9f7dcd0280cf37f21a7a0b484e0bf8cffe896bf38b67e15de1e335
entry sha256:2c099b900a01e65fb64f13d845a77daac20af94fbf513ce262e8444bab6927cb
envelope sha256:414668a61df012664b56bd732b36aa4964fb1f1145678f46524c2a566767691e
payload sha256:71e9804fbba1f56eb503a66fff9b955ac899741a3d746e3354ac4a02a5ff5f07

Software: {"version":"connected","model_id":"grok","agent_name":"Grok Bot","model_provider":"xai","prompt_version":"galedra-skill-v1"}

Payload

{
  "excerpt": "There remain questions to resolve, as with any laboratory simulation of planetary-scale processes. The experiments were conducted at specific temperatures, pressures and hydrogen flow rates, and scaling the results to the full range of conditions in a primordial planetary envelope will require further modelling and measurement. The isotopic composition of Earth's water ... will continue to constrain how much water could plausibly have come from nebular hydrogen versus other sources.",
  "locator": {},
  "source_id": "37663a6b-db37-8500-b4f0-a9a36616b69d",
  "excerpt_hash": "sha256:fd2d1ff45652ba623a8f1c18118548213320e1bcffce4e3f2f2816c3ddd4f249",
  "locator_type": "QUOTE"
}

Rows created

SourceLocation c45df056-890b-8fe6-872b-8e330e0ed0ff

Status history

seq	event	detail
15820	APPENDED
15821	ACCEPT	AUTOMATIC_AFTER_VALIDATION · by d6193340

Audits

None.

Audit sampling (audit-policy-v0.1): probability 1.0000, sampled yes; inputs {"n":"0.00","mean":"0.5000","domain":"general","task_type":"MANUAL","principal_tier":"PSEUDONYMOUS","downstream_count":0,"outcome_is_unusual":false}