pith:XB7SR6GA
The Role of Formation Location in Shaping Sulfur-, Nitrogen-, and Carbon-Bearing Species in Super-Earth and Sub-Neptune Atmospheres
Formation location imprints on atmospheric C/O ratios and silicon species in super-Earths and sub-Neptunes even after magma ocean equilibration, with nitrogen depletion as a common result.
arxiv:2605.15170 v1 · 2026-05-14 · astro-ph.EP
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\pithnumber{XB7SR6GAGTXEI44JX7OHBYL7OO}
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Claims
We identify atmospheric C/O, SiH4, and H2O as potential indicators of formation location, while nitrogen depletion emerges as a generic outcome of magma ocean equilibration.
That the extended global chemical equilibrium framework and the Bern Generation III synthetic population accurately capture the dominant processes without significant kinetic barriers or missing reactions at ~40 Myr.
Magma ocean equilibration depletes atmospheric nitrogen and shifts C/O ratios in sub-Neptune atmospheres, making C/O, SiH4, and H2O potential tracers of formation location.
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| First computed | 2026-05-17T21:40:25.291595Z |
|---|---|
| Last reissued | 2026-05-17T21:57:18.627332Z |
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | unsigned_v0 |
| Schema | pith-number/v1.0 |
Canonical hash
b87f28f8c034ee447389bfdc70e17f738294ec72f8c4baec9d4b6dc0dc15e214
Aliases
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curl -sH 'Accept: application/ld+json' https://pith.science/pith/XB7SR6GAGTXEI44JX7OHBYL7OO \
| 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: b87f28f8c034ee447389bfdc70e17f738294ec72f8c4baec9d4b6dc0dc15e214
Canonical record JSON
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