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Optical stellar intensity interferometry of Sirius

Contribution grade

Astronomical instrumentation and stellar measurements · Source-reported experimental result or reusable measurement method

Reference score225,000Provisional editorial estimate of this exact contribution; its grade is assessed separately.

What changed

At Jodrell Bank Hanbury Brown and Twiss tested optical intensity interferometry on Sirius, observing a decrease in correlated intensity with projected baseline. A later participant account reproduces four observational signal-to-noise values and reports a best-fit angular diameter of 7.1 ± 0.55 milliarcseconds after a theoretical limb-darkening correction.

Scientific scope

At Jodrell Bank Hanbury Brown and Twiss tested optical intensity interferometry on Sirius, observing a decrease in correlated intensity with projected baseline. A later participant account reproduces four observational signal-to-noise values and reports a best-fit angular diameter of 7.1 ± 0.55 milliarcseconds after a theoretical limb-darkening correction. Hanbury Brown and Twiss’s 1956 paper gives the original two-author attribution. The quoted 7.1 ± 0.55 milliarcsecond diameter and four signal-to-noise values come from Hanbury Brown’s later participant account and subsequent analysis; they should not be presented as a direct reanalysis of the original observations. Atmospheric scintillation, optical bandwidth, normalization and limb-darkening assumptions affect the result.

Evidence

The linked original works support the scoped statement and contribution attribution. WRS has not independently replayed experiments or reconstructed a full mathematical proof. Hanbury Brown and Twiss’s 1956 paper gives the original two-author attribution. The quoted 7.1 ± 0.55 milliarcsecond diameter and four signal-to-noise values come from Hanbury Brown’s later participant account and subsequent analysis; they should not be presented as a direct reanalysis of the original observations. Atmospheric scintillation, optical bandwidth, normalization and limb-darkening assumptions affect the result.

Contributors

Provisional WRS assessment, edition 2026-10-28.1. Independent expert calibration is pending. This grade does not certify correctness or assign ownership.

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