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Pith Number

pith:VFWYKYW2

pith:2026:VFWYKYW2XFEDSMUH4OOFUYHU7C
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Modeling Volcanic Plume Heights Across Exoplanet Atmospheres: Insights from TRAPPIST-1

Prabal Saxena, Thomas Fauchez

A 1D model adapted for exoplanets predicts that volcanic plumes frequently reach low-pressure levels suitable for detection in transmission observations.

arxiv:2605.04423 v2 · 2026-05-06 · astro-ph.EP

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\usepackage{pith}
\pithnumber{VFWYKYW2XFEDSMUH4OOFUYHU7C}

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Record completeness

1 Bitcoin timestamp
2 Internet Archive
3 Author claim open · sign in to claim
4 Citations open
5 Replications open
Portable graph bundle live · download bundle · merged state
The bundle contains the canonical record plus signed events. A mirror can host it anywhere and recompute the same current state with the deterministic merge algorithm.

Claims

C1strongest claim

These results provide a physically grounded framework for predicting whether and how volcanic emissions might be detected on rocky exoplanets, including-but not limited to-those experiencing strong tidal heating.

C2weakest assumption

The 1D plume model assumptions (vent thermodynamics, buoyant entrainment, and vertically varying static stability) originally developed for Venus and Mars transfer without major revision to the diverse exoplanet background states explored.

C3one line summary

A Python port of a classic volcanic plume model is applied to exoplanet conditions, identifying parameter regions where plumes reach low-pressure altitudes and become potentially detectable.

Receipt and verification
First computed 2026-06-04T01:08:13.313762Z
Builder pith-number-builder-2026-05-17-v1
Signature Pith Ed25519 (pith-v1-2026-05) · public key
Schema pith-number/v1.0

Canonical hash

a96d8562dab948393287e39c5a60f4f8bdcc805bc89939e9e7efeb1068a9da7f

Aliases

arxiv: 2605.04423 · arxiv_version: 2605.04423v2 · doi: 10.48550/arxiv.2605.04423 · pith_short_12: VFWYKYW2XFED · pith_short_16: VFWYKYW2XFEDSMUH · pith_short_8: VFWYKYW2
Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/VFWYKYW2XFEDSMUH4OOFUYHU7C \
  | jq -c '.canonical_record' \
  | python3 -c "import sys,json,hashlib; b=json.dumps(json.loads(sys.stdin.read()), sort_keys=True, separators=(',',':'), ensure_ascii=False).encode(); print(hashlib.sha256(b).hexdigest())"
# expect: a96d8562dab948393287e39c5a60f4f8bdcc805bc89939e9e7efeb1068a9da7f
Canonical record JSON
{
  "metadata": {
    "abstract_canon_sha256": "cc3c6a0c088c23f6aa406bf610d64c5692e2112eacf7f005741b61b054ca9671",
    "cross_cats_sorted": [],
    "license": "http://creativecommons.org/licenses/by/4.0/",
    "primary_cat": "astro-ph.EP",
    "submitted_at": "2026-05-06T02:29:21Z",
    "title_canon_sha256": "fa9c2d65d4c506020a49852155a966770996c8f2f8da2593ca5a50299209d90d"
  },
  "schema_version": "1.0",
  "source": {
    "id": "2605.04423",
    "kind": "arxiv",
    "version": 2
  }
}