pith:NVCYLYP4
Kozai-driven mass loss of the circumbinary disk in D9 in orbit around the supermassive black hole Sgr A*
The circumbinary disk around D9 loses about 7 percent of its mass every von Zeipel-Lidov-Kozai cycle induced by Sgr A*.
arxiv:2604.09856 v2 · 2026-04-10 · astro-ph.GA · astro-ph.SR
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Claims
We find the disk loses ∼7% ± 2% of its mass every vZLK cycle. If we extrapolate this mass loss, the disk will have 1% of its current mass left after another ∼4 Myr. D9 will then be ∼6.7 Myr old, which is on the same order as the current average age of S cluster members. The vZLK-driven mass loss could, therefore, explain the absence of Brγ emission from other S cluster members.
The mass loss rate of ~7% per cycle remains constant over multiple Myr without significant changes from unmodeled physics such as stellar winds, radiation, or variations in initial disk conditions.
Numerical simulations find that vZLK oscillations induce periodic mass loss from D9's circumbinary disk at a rate of ~7% per 62.5 kyr cycle, leading to near-total depletion after ~4 Myr.
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| First computed | 2026-06-19T16:10:37.257854Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
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curl -sH 'Accept: application/ld+json' https://pith.science/pith/NVCYLYP4URVG6EOBOXWFKBIQTE \
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| 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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