Gravitomagnetic measurement of the angular momentum of celestial bodies
A. Tartaglia, M.L. Ruggiero

TL;DR
This paper proposes a practical method to measure the angular momentum of celestial bodies by analyzing light signal asymmetries caused by gravitomagnetic effects, including frequency shifts.
Contribution
It introduces a novel procedure to detect gravitomagnetic effects and measure the angular momentum of celestial bodies through light signal asymmetries.
Findings
Frequency shifts due to gravitomagnetism are identified.
A practical measurement procedure is proposed.
Order of magnitude estimates are discussed.
Abstract
The asymmetry in the time delay for light rays propagating on opposite sides of a spinning body is analyzed. A frequency shift in the perceived signals is found. A practical procedure is proposed for evidencing the asymmetry, allowing for a measurement of the specific angular momentum of the rotating mass. Orders of magnitude are considered and discussed.
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