pith:B3LJX7SA
A short-period binary OGLE-BLG-ELL-006503 showing slow variations in brightness
Eclipse timings in OGLE-BLG-ELL-006503 show an orbital period change on a two-million-year timescale.
arxiv:2604.26710 v2 · 2026-04-29 · astro-ph.SR
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Claims
The eclipse time O-C residuals reveal an orbital period change characterized by a timescale of approximately 2x10^6 years, suggesting a mild mass redistribution, potentially linked to global magnetic fields reconfiguration.
Seasonal light-curves suggest that this long-term variability is driven by large photospheric spots (approx 0.3 stellar radii) that exhibit a tendency to orient themselves relative to the tidal interaction line.
28-year OGLE observations of short-period binary OGLE-BLG-ELL-006503 show tidal variations plus long-term spot-driven brightness drifts and orbital period changes suggesting mild mass redistribution.
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| First computed | 2026-05-22T01:03:19.488611Z |
|---|---|
| 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/B3LJX7SAJ2KABQOPAISUVGXNFK \
| jq -c '.canonical_record' \
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Canonical record JSON
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