pith:FBSBVP3T
The Colors of Ices: Measuring ice column density through photometry
JWST photometry alone can quantify interstellar ices in the Galactic Center, showing over 25 percent of carbon frozen as CO and implying at least 2.5 times solar metallicity.
arxiv:2510.00292 v4 · 2025-09-30 · astro-ph.GA
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Claims
Accounting for all likely ices, we infer that >25% of the total carbon is frozen into CO ice in the GC, which exceeds the entire solar-neighborhood carbon budget. By assuming the freezeout fraction is the same in GC and disk clouds, we obtain a metallicity measurement indicating that Z_GC ≳2.5 Z_⊙.
The assumption that the ice freezeout fraction is identical between Galactic Center and Galactic disk clouds, which is required to convert the fitted ice column densities into the claimed metallicity value.
JWST photometry detects CO, H2O, and CO2 ices in Galactic Center clouds, with >25% of carbon frozen in CO ice implying Z_GC ≳2.5 Z_⊙ under equal freezeout assumption.
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| First computed | 2026-06-09T01:05:09.718568Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
28641abf738fdf987e8a8ecd88e1b5dd60f1c91731b243e582fc8c842c50fb89
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curl -sH 'Accept: application/ld+json' https://pith.science/pith/FBSBVP3TR7PZQ7UKR3GYRYNV3V \
| 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())"
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Canonical record JSON
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