Submitted:
25 February 2026
Posted:
27 February 2026
Read the latest preprint version here
Abstract
Keywords:
1. Introduction
2. Present-Day Angular-Momentum Change from Direct Measurements
2.1. Loss Rate of Earth’s Rotational Angular Momentum
2.2. Gain Rate of the Moon’s Orbital Angular Momentum
2.3. Present-Day Comparison
3. Deep-Time Angular-Momentum Change from Fossil and Tidal-Rhythmite Histories
3.1. Earth’s Rotational Angular-Momentum Loss over the Past 3.2 Billion Years
3.2. Moon’s Orbital Angular-Momentum Gain over the Past 3.2 Ga
3.3. Angular-Momentum Dynamics over Earth–Moon History
- The arms and torso are rigidly connected.
- They rotate with exactly the same angular velocity.
- The system is closed and behaves as a rigid body.
- Angular momentum is conserved internally within the system.
- Earth and Moon are not rigidly connected.
- They rotate at vastly different angular velocities.
- They are separated by approximately 384,000 km.
- The tidal bulge on Earth is very small.
- The coupling between Earth and Moon is weak and dissipative.
4. A DMFF-Based Explanation for the Discrepancy
- Earth loses rotational angular momentum to the DMFF medium.
- The Moon experiences DMFF drag and an anti-gravitational push, increasing its orbital angular momentum.
- Earth’s loss and the Moon’s gain arise from different mechanisms, not mutual exchange.
- Angular-momentum conservation applies to the combined Earth–Moon–DMFF system.
- fits modern atomic-clock and LLR measurements,
- reproduces fossil and tidal rhythmite-derived LOD, DOY, and DOM histories,
- is independently validated using data dated to 3.2 billion years ago, as analyzed by Eulenfeld et al.
- requires no assumptions about ocean-basin geometry or resonances,
- naturally resolves the angular-momentum discrepancy.
5. Conclusion
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