Calculate free fall velocity (v = √(2gh)), fall duration (t = √(2h/g)), drop height (h = 1/2·g·t²), and kinetic energy under Earth, Moon, Mars, and custom gravities with the free Free Fall Calculator.
99.1 mph • 159.5 km/h • Fall Duration: 4.52 s • Drop Height: 100.0 m
Time to impact
328.1 ft
159.5 km/h
Impact energy
Conserved energy
\(v_{\text{avg}} = h / t\)
In classical Newtonian mechanics, free fall is the unconstrained vertical motion of a body acted upon solely by the fundamental force of gravity (\(F_g = m g\)), with zero opposing aerodynamic drag. In an ideal vacuum, all objects—regardless of their mass, shape, or density—accelerate downward at the exact same constant gravitational acceleration (\(g = 9.80665\text{ m/s}^2\) on Earth).
| Free Fall Variable | Formula (from Rest \(v_0 = 0\)) | Formula with Initial Velocity (\(v_0\)) |
|---|---|---|
| Impact Velocity (\(v\)) | $$v = \sqrt{2 g h} = g t$$ | $$v = \sqrt{v_0^2 + 2 g h} = v_0 + g t$$ |
| Time of Flight (\(t\)) | $$t = \sqrt{\frac{2 h}{g}} = \frac{v}{g}$$ | $$t = \frac{-v_0 + \sqrt{v_0^2 + 2 g h}}{g}$$ |
| Drop Distance (\(h\)) | $$h = \frac{1}{2} g t^2 = \frac{v^2}{2 g}$$ | $$h = v_0 t + \frac{1}{2} g t^2 = \frac{v^2 - v_0^2}{2 g}$$ |
| Kinetic Energy (\(E_k\)) | $$E_k = \frac{1}{2} m v^2 = m g h$$ | $$E_k = \frac{1}{2} m (v_0^2 + 2 g h)$$ |
How drop times from a 100-meter height vary across the solar system:
Fall Time: 4.52 s
Impact Speed: 44.3 m/s (99.1 mph)
Fall Time: 11.11 s (\(2.46\times\) slower)
Impact Speed: 18.0 m/s (40.3 mph)
Fall Time: 7.34 s (\(1.63\times\) slower)
Impact Speed: 27.2 m/s (60.9 mph)
Fall Time: 2.84 s (\(37\%\) faster)
Impact Speed: 70.4 m/s (157.5 mph)
Choose whether you are solving from Drop Height (\(h\)), Fall Time (\(t\)), Final Velocity (\(v\)), or Initial Launch Speed (\(v_0\)).
Input drop height in meters/feet, time in seconds, or speed in \(\text{m/s}\) or \(\text{mph}\).
Choose Earth (\(9.807\text{ m/s}^2\)), Moon, Mars, Venus, or Jupiter.
Inspect calculated impact velocity, fall duration, mechanical kinetic energy, and live step-by-step mathematical proofs.
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Instantly verifies homework and laboratory free fall experiments with step-by-step mathematical substitutions.
Solves for any variable: Drop Height (\(h\)), Fall Time (\(t\)), Impact Velocity (\(v\)), or Initial Velocity (\(v_0\)).
Includes precise gravitational fields for Earth, Moon, Mars, Venus, Jupiter, and the Sun.
Tracks the complete conversion of gravitational potential energy (\(U_g = mgh\)) into kinetic energy (\(E_k = \frac{1}{2}mv^2\)).
Albert Einstein's "happiest thought" and the foundation of General Relativity:
When an object is in free fall, every atom accelerates downward at the exact same rate (\(a = g\)). Because there is no upward normal contact force from a floor or scale (\(F_N = m(g - a) = 0\)), an observer inside a freely falling enclosure feels completely weightless. This fundamental equivalence between gravitational acceleration and inertial acceleration led Einstein to formulate General Relativity: gravity is not a traditional mechanical contact force, but the curvature of spacetime. The International Space Station (ISS) is not outside Earth's gravity (\(g \approx 8.7\text{ m/s}^2\) in orbit); astronauts float because the station is in perpetual free fall around Earth.
Comprehensive answers to common questions about free fall equations, gravity drop formulas, flight durations, and Apollo lunar tests.