How can one detect the rotation of the Earth "around the Moon"? Part 2: Ultra-slow fall
Bertrand M. Roehner

TL;DR
This paper proposes a novel method using buoyancy in superfluid helium to detect Earth's rotation around the Moon by amplifying eastward deflections during ultra-slow falls, offering greater flexibility than Foucault's pendulum.
Contribution
It introduces an alternative approach to measure Earth's rotation using buoyancy-driven ultra-slow falls in superfluid helium, with adjustable parameters for enhanced detection sensitivity.
Findings
Preliminary water experiments showed promising results despite noise.
The method can amplify deflections by over 1,000 times compared to traditional Foucault pendulum.
Future experiments aim to reduce noise and optimize parameters for better detection.
Abstract
The paper proposes an alternative to the Foucault pendulum for detecting various movements of rotation of the Earth. Calculations suggest that if the duration of a "free" fall becomes longer the eastward deflection will be amplified in proportion with the increased duration. Instead of 20 micrometers for a one-meter fall, one can expect deflections more than 1,000 times larger when the fall lasts a few minutes. The method proposed in this paper consists in using the buoyancy of a (non viscous) liquid in order to work in reduced gravity. Not surprisingly, as in many astronomical observations, the main challenge is to minimize the level of "noise". Possible sources of noise are discussed and remedies are proposed. In principle, the experiment should be done in superfluid helium. However, a preliminary experiment done in water gave encouraging results in spite of a fairly high level of…
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Taxonomy
TopicsSolar and Space Plasma Dynamics · Geophysics and Gravity Measurements · Astro and Planetary Science
