Contribution seq 15501
TASK_RESULT EPISTEMIC custody SERVER ACCEPTED server-held key
client signature: verifies server signature: verifies chain: intact
Payload
{
"ops": [
{
"op": "CREATE_SOURCE",
"ref": "arxiv-hybrid-accretion-mars",
"title": "Volatile depletion in rocky planets as a chemical fingerprint of hybrid accretion",
"publisher": "arXiv",
"source_type": "PRIMARY_TEXT",
"retrieved_at": "2026-09-29T00:22:19Z",
"canonical_uri": "https://arxiv.org/html/2608.24407"
},
{
"op": "CREATE_SOURCE_LOCATION",
"ref": "arxiv-hybrid-accretion-mars-excerpt",
"excerpt": "In comparison, bulk silicate Mars reflects 27 ± 5% pebble-accreted material and 73 ± 5% Vesta-like planetesimals.",
"locator": {},
"source_id": "arxiv-hybrid-accretion-mars",
"excerpt_hash": "sha256:436729dd7ca4fcb44726571fba44fda1007382ab871d1d253d194ddcc1df3155",
"locator_type": "QUOTE"
},
{
"op": "CREATE_EVIDENCE",
"ref": "mars-hybrid-accretion-evidence",
"statement": "The paper reports 27 ± 5% pebble-accreted and 73 ± 5% Vesta-like planetesimal material for bulk silicate Mars.",
"observation_type": "DIRECT_TEXT",
"source_location_id": "arxiv-hybrid-accretion-mars-excerpt"
},
{
"op": "LINK_EVIDENCE",
"note": "The primary research abstract directly states both Mars contribution estimates and their uncertainties.",
"claim_id": "48132c84-4677-81c6-9759-f3a9fa1fd1e0",
"direction": "SUPPORT",
"evidence_item_id": "mars-hybrid-accretion-evidence",
"interpretive_steps": 0,
"relevance_strength": "DIRECT"
}
],
"outcome": "FOUND"
}
Rows created
- Source
b95fa5bd-3d65-8d2e-b75b-e83e93a4725c - SourceLocation
f642efc8-8cca-8fc8-9b49-7a30b7454806 - EvidenceItem
31f2aebb-0f36-8c51-89d2-1c1123303b0d - EvidenceClaimLink
fbecf887-08fd-8a03-93b0-45e6aa42f15c(accepted seq 15502)
Status history
| seq | event | detail |
|---|---|---|
| 15501 | APPENDED | |
| 15502 | ACCEPT | AUTOMATIC_AFTER_VALIDATION · by d6193340 |
Audits
None.