Free Fall
GeneralFree Fall (Physics)
Motion where gravity is the only force acting on an object, with no air resistance or other forces, governed by constant gravitational acceleration.
Definition
Free fall describes motion where gravity is the only force acting on an object — no air resistance, no other forces — making it the simplest and most idealized form of falling motion. It's governed entirely by gravitational acceleration (g = 9.8 m/s² on Earth), independent of the falling object's mass.
The Free Fall Calculator computes fall time, final velocity, and distance fallen from any single known value.
Formula
Velocity after time t: v = gt Distance fallen: d = ½gt² Velocity after falling distance d: v = √(2gd)
where g is 9.8 m/s² on Earth.
Worked Example
An object dropped from a 45-meter height (starting from rest) takes t = √(2 × 45 ÷ 9.8) ≈ 3.03 seconds to hit the ground, reaching a final velocity of v = 9.8 × 3.03 ≈ 29.7 m/s (about 107 km/h) just before impact.
Key Things to Know
- Mass doesn't affect free fall rate: all objects accelerate at the same rate under gravity alone, regardless of how heavy they are.
- Air resistance is what makes real-world falling different: a feather falls slower than a bowling ball on Earth due to air resistance, not because free fall physics differs for each.
- Free fall is the vertical component of projectile motion: projectile motion combines free-fall vertical motion with independent constant horizontal motion.
- Real falling objects eventually reach terminal velocity, once air resistance grows large enough to balance gravity — free fall describes the phase before that balance point.
- The direction of "falling" doesn't have to be downward: the same equations apply to any object accelerating uniformly under a constant force, though gravity-driven vertical fall is the classic case.
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