Tidal Force on a Test Body from a Distant Mass Calculator
F_tidal ≈ 2 · G · M · m · R / d³.
Compute the differential gravitational pull (tidal force) exerted by a distant mass M on a small body of mass m and characteristic radius R, separated by centre-to-centre distance d: F_tidal ≈ 2 · G · M · m · R / d³. The 1/d³ falloff is faster than the 1/d² of Newtonian gravity itself.
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Formula
F_tidal ≈ 2 · G · M · m · R / d³; G = 6.674·10⁻¹¹ N·m²/kg².
In depth
Compute the differential gravitational pull (tidal force) exerted by a distant mass M on a small body of mass m and characteristic radius R, separated by centre-to-centre distance d: F_tidal ≈ 2 · G · M · m · R / d³. The 1/d³ falloff is faster than the 1/d² of Newtonian gravity itself.
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