Subtract common acceleration before interpreting a tidal effect
Gravity accelerates the whole body toward a source, but it also varies across the body. A tidal effect concerns that spatial difference rather than the common acceleration. In a freely falling center frame, the near side is pulled toward the source more strongly than the center, while the far side falls behind it. Both inertial accelerations still point toward the source; the opposite relative signs do not require a repulsive gravitational force.
Learning outcome: Compare exact endpoint differences with the small-body approximation at different D and R. Retain common and relative accelerations separately, and identify the missing material information needed to predict deformation.
Starting recap
Retain relative versus barycentric geometry, time versus angle, fitted versus instantaneous velocity and complete energy/angular-momentum boundaries.
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At D=10 and R=0.2, near-minus-center is≈0.000412328 and far-minus-center≈−0.000388312. Full stretching is≈0.000800640, close to the leading 4R/D³=0.0008. The slight asymmetry reflects finite R/D, not opposite gravitational force directions.
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Why can the near and far center-relative accelerations have opposite signs when both are attracted toward the source?
Experiment
Compare exact endpoint differences with the small-body approximation at different D and R. Retain common and relative accelerations separately, and identify the missing material information needed to predict deformation.
Subtract center acceleration before interpreting tidal stretching
Worked teaching model · synthetic values · Original source μ=1 and three collinear test points at D−R, D and D+R. Accelerations toward source are inverse-square; near-minus-far stretch compared with leading small-body approximation 4R/D³. No deformation, ocean dynamics, self-gravity or tide-height prediction.
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Common free fall and differential stretching are different gravitational effects.
All three inertial accelerations point toward the source, yet center-relative accelerations have opposite signs. The leading differential term scales as distance cubed in the denominator, unlike the inverse-square center acceleration. Actual tides require material response and dynamics.
| Quantity | Value | Unit |
|---|---|---|
| Near-point acceleration toward source | 0.01041233 | length/time² |
| Center acceleration toward source | 0.01000000 | length/time² |
| Far-point acceleration toward source | 0.009611688 | length/time² |
| Near relative to center | 0.0004123282 | length/time² |
| Far relative to center | -0.0003883122 | length/time² |
| Exact near-minus-far stretching | 0.0008006404 | length/time² |
| Leading small-body approximation | 0.0008000000 | length/time² |
| Approximation relative error | -0.0007998400 | fraction |
These original models are not measured orbit records or operational mission instructions. Retain the frame, assumptions and missing evidence before interpreting a real system.
Common free fall and differential stretching are different gravitational effects.
All three inertial accelerations point toward the source, yet center-relative accelerations have opposite signs. The leading differential term scales as distance cubed in the denominator, unlike the inverse-square center acceleration. Actual tides require material response and dynamics.
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Keep R=0.2 and reduce D from 10 to 5. Compare leading full stretching and center acceleration factors.
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