pith:4SDAISHT
Resizing the giants: How modelling adiabatic interiors impacts predicted planetary radii
Numerical methods for adiabatic temperature profiles can change giant planet radii by up to 3.4 percent.
arxiv:2603.24779 v2 · 2026-03-25 · astro-ph.EP · astro-ph.IM
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Claims
The choice of numerical method significantly impacts the inferred interior structure and radius. Using the logarithmic temperature equation, central temperatures deviate by several thousand Kelvin and surface radii differ by up to 3.4%.
That the planet is strictly one-dimensional, fully convective, and perfectly adiabatic with no composition gradients or non-adiabatic heat transport that would alter the temperature profile independently of the numerical method.
Numerical treatment of the adiabatic gradient changes predicted giant-planet radii by up to 3.4 percent depending on the temperature-equation form and derivative method used.
Receipt and verification
| First computed | 2026-05-27T14:06:41.937757Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
e4860448f3bc79b0f7f488741399efb290f06f8d2c7cff629aa80238448ef9eb
Aliases
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Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/4SDAISHTXR43B57URB2BHGPPWK \
| 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: e4860448f3bc79b0f7f488741399efb290f06f8d2c7cff629aa80238448ef9eb
Canonical record JSON
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