Tidal force is the difference in gravitational pull across an object's size, caused by one side being closer to a massive body than the other — it's what raises ocean tides on Earth and can stretch or even tear apart moons that stray too close to their planet..
Tidal force is the difference in gravitational pull across an object's size, caused by one side being closer to a massive body than the other — it's what raises ocean tides on Earth and can stretch or even tear apart moons that stray too close to their planet.
A 1000 kg, 5 m-radius satellite orbits a planet of mass 5.97×10²⁴ kg at a distance of 1×10⁷ m. Tidal Force = 2×6.674×10⁻¹¹×5.97×10²⁴×1000×5 / (1×10⁷)³ ≈ 0.399 N — small here, but grows sharply as distance shrinks.
The differential gravitational pull an object experiences because one side is closer to a massive body.
Proportional to mass and the object's diameter, inversely proportional to distance cubed.
The Moon pulls more strongly on the nearest ocean water, creating stretching that produces tidal bulges.