pith:FWUKLPX5
Evidence for a bloated massive protostar in IRAS20126+4104
The 12 solar-mass protostar in IRAS20126+4104 is bloated to a radius of about 200 solar radii.
arxiv:2604.12552 v1 · 2026-04-14 · astro-ph.SR · astro-ph.GA
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Claims
The long rotation period implies that the 12 M_⊙ protostar is bloated, with a radius of ∼200 R_⊙.
That the observed 6.8 yr periodicity is produced by stellar rotation with a surface spot rather than any of the other three clocks considered, and that the 12 M_⊙ mass and spot geometry allow a direct conversion from period to radius.
Mid-IR light curves of IRAS20126+4104 confirm a 6.8 yr periodic variation interpreted as evidence that the 12 solar-mass protostar is bloated to a radius of roughly 200 solar radii due to rotation with an obscuring spot.
References
Receipt and verification
| First computed | 2026-05-20T14:03:26.822348Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
2da8a5befd6e8cc9273c3bcbdcb7e459727ba6d125cece4a07f4393b37d2da5d
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/FWUKLPX5N2GMSJZ4HPF5ZN7ELF \
| 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: 2da8a5befd6e8cc9273c3bcbdcb7e459727ba6d125cece4a07f4393b37d2da5d
Canonical record JSON
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