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Physics

Gravity Calculator | Free Fall, Force & Escape

Calculate free fall height, time, and velocity. Compute gravitational force with Newton's law. Find surface gravity and escape velocity for any planet. NASA planet data included.

Instant Results100% FreeAny DeviceNo Sign-up

QUICK PRESETS

Enter any one value to solve for the other two.

SURFACE GRAVITY, ALL PLANETS (NASA DATA)
Bodyg (m/s²)vs Earth
Mercury3.700.377 g
Venus8.870.904 g
Earth9.811.000 g
Moon1.620.165 g
Mars3.720.379 g
Jupiter24.792.528 g
Saturn10.441.065 g
Uranus8.870.904 g
Neptune11.151.137 g
Pluto0.620.063 g
Sun274.0027.940 g

What Is the Gravity Calculator | Free Fall, Force & Escape?

This gravity calculator covers four modes: free-fall kinematics (solve for height, time, or velocity), Newton's gravitational force between two masses, surface gravity of any spherical body, and escape velocity. Uses the NIST CODATA 2018 value G = 6.674×10⁻¹¹ N·m²/kg² and standard gravity g = 9.80665 m/s².

  • Free Fall: Enter any one of height, time, or velocity, the calculator solves for the other two. Select surface gravity from any planet or enter a custom g.
  • Gravitational Force: Computes F = Gm₁m₂/r² for any two masses at any distance. Presets for Earth-Moon, Earth-Sun, and Earth-person.
  • Surface Gravity: Given a body's mass and radius, finds its surface g. Includes Earth, Moon, Mars, and Jupiter presets.
  • Escape Velocity: Computes vₑ = √(2GM/R), the speed needed to escape a planet's gravity from its surface.
  • Planet table: Shows NASA surface gravity for all 8 planets, Moon, Pluto, and Sun.

Formula

Core Gravity Formulas
Free fall: h = ½gt²   v = gt   t = √(2h/g)
Newton's law: F = Gm₁m₂ / r²
Surface g: g = GM / R²
Escape velocity: vₑ = √(2GM/R)

Free Fall

h = ½gt² v = gt t = √(2h/g)

g = 9.80665 m/s² on Earth (standard). Select any planet for its surface g.

Newton's Law of Gravitation

F = G × m₁ × m₂ / r²

G = 6.674×10⁻¹¹ N·m²/kg² (NIST CODATA 2018)

Surface Gravity

g = G × M / R²

Derives surface gravitational acceleration from mass M and radius R of a body.

Escape Velocity

vₑ = √(2GM/R)

Minimum speed to escape gravitational field from surface, ignores atmospheric drag.

How to Use

  1. 1

    Select a mode

    Choose Free Fall, Gravitational Force, Surface Gravity, or Escape Velocity.

  2. 2

    Try a preset

    Click presets like Drop 10 m, Empire State, Moon landing, or Mars mission to auto-fill values.

  3. 3

    Select a planet (Free Fall)

    Click any planet button to set that body's surface gravity, or enter a custom g value.

  4. 4

    Choose your units

    Select m, ft, or km for distances; kg or lb for masses using the inline dropdowns.

  5. 5

    Enter your known value

    In Free Fall, enter any one of height, time, or velocity. In force/gravity modes, enter mass and distance.

  6. 6

    Press Calculate

    Results appear instantly with all derived values including equivalent units.

  7. 7

    Check the planet table

    In Free Fall mode, the planet gravity reference table shows NASA g values for all solar system bodies.

  8. 8

    Expand step-by-step

    Click Step-by-step working to see every formula substitution with your values.

Example Calculation

Example 1 | Free fall from Empire State Building (443 m)

Height443 m
g (Earth)9.80665 m/s²
Fall time: t = √(2h/g)√(886 / 9.807) = 9.51 s
Impact velocity: v = gt9.807 × 9.51 = 93.3 m/s = 335 km/h

No air resistance assumed. Actual terminal velocity is ~53 m/s for a human.

Example 2 | Gravitational force, Earth on a 70 kg person

m₁ (Earth)5.972×10²⁴ kg
m₂ (person)70 kg
r (Earth radius)6.371×10⁶ m
F = Gm₁m₂/r²686 N (weight of 70 kg at sea level)

This equals 70 kg × 9.80 m/s² = 686 N, confirming the formula.

Example 3 | Escape velocity from Earth

M (Earth)5.972×10²⁴ kg
R (Earth)6.371×10⁶ m
vₑ = √(2GM/R)√(2 × 6.674×10⁻¹¹ × 5.972×10²⁴ / 6.371×10⁶)
Result11,186 m/s = 11.19 km/s ≈ 40,270 km/h

Rockets must exceed this speed to escape Earth's gravity well into space.

Understanding Gravity | Free Fall, Force & Escape

Gravity in Physics

Gravity is the fundamental force attracting any two masses. Newton's law of universal gravitation quantifies this: F = Gm₁m₂/r². At planetary scale, this force determines orbits, tides, and surface weight. All calculations in this calculator run live in your browser using the NIST CODATA 2018 gravitational constant G = 6.674×10⁻¹¹ N·m²/kg².

Free Fall Assumptions

  • No air resistance, actual fall times are longer due to drag.
  • Uniform gravitational field, valid for heights small compared to Earth's radius.
  • Object released from rest (initial velocity = 0).
  • Standard Earth g = 9.80665 m/s², varies slightly with latitude and altitude.

Planet Surface Gravities (NASA)

Surface gravity varies enormously across the solar system. Jupiter's surface gravity is 2.53 times Earth's; the Moon's is only 0.165 g. The Sun's is 27.9 g. These values are computed from g = GM/R² using NASA mass and radius data.

Escape Velocity Notes

  • Earth: 11.19 km/s, rockets need this minimum speed ignoring air drag.
  • Moon: 2.38 km/s, much easier to escape, which is why the Moon has no atmosphere.
  • Jupiter: 59.5 km/s, strong gravity makes escape very difficult.
  • Sun: 617.5 km/s, nothing in the solar system escapes the Sun without additional energy.

Frequently Asked Questions

What is the value of g and why 9.80665 m/s²?

The standard acceleration of free fall is defined as exactly 9.80665 m/s² by the International Bureau of Weights and Measures. The actual value varies by location:

  • • Equator: ≈9.78 m/s² (centrifugal effect reduces apparent gravity)
  • • Poles: ≈9.83 m/s² (closer to Earth's center)
  • Standard: 9.80665 m/s² (used in all calculations here)

What is the gravitational constant G?

G is the universal gravitational constant, measured experimentally. This calculator uses the NIST CODATA 2018 value:

  • G = 6.67430×10⁻¹¹ N·m²/kg²
  • • G is the least precisely known fundamental constant in physics
  • • First measured by Henry Cavendish in 1798 using a torsion balance

How do I calculate fall time from height?

From the kinematic equation h = ½gt² (starting from rest, no air resistance):

  • • Rearrange: t = √(2h / g)
  • • Example: h = 100 m, g = 9.807 m/s² → t = √(200/9.807) ≈ 4.52 s
  • • Enter height in the Free Fall tab and the calculator solves instantly.

Why does gravity vary on different planets?

Surface gravity depends on the planet's mass and radius: g = GM/R². A larger mass increases g, but a larger radius decreases it:

  • • Jupiter has 318× Earth's mass but only 11× the radius → g ≈ 24.8 m/s²
  • • Moon is 1/81 Earth's mass and 1/3.7 the radius → g ≈ 1.62 m/s²

What is escape velocity?

Escape velocity is the minimum speed needed to escape a body's gravitational field from its surface, ignoring air resistance:

  • vₑ = √(2GM/R)
  • • Earth: 11.19 km/s | Moon: 2.38 km/s | Mars: 5.03 km/s
  • • A body with vₑ > c (speed of light) is a black hole

Can I use pounds and feet in this calculator?

Yes. Each input has a unit selector:

  • • Distance: m, ft, or km
  • • Mass: kg or lb
  • • The calculator converts to SI internally before computing, then displays results in your chosen units.

Does free-fall calculation account for air resistance?

No, these are idealized vacuum calculations. In practice, air resistance limits terminal velocity:

  • • Human terminal velocity: ∼53 m/s (∼190 km/h)
  • • Skydiver with parachute: ∼5–7 m/s
  • • For precise engineering applications, use computational fluid dynamics models.

What is the difference between weight and gravitational force?

Weight is the gravitational force on a mass at a specific location:

  • • Weight (N) = mass (kg) × local g (m/s²)
  • • Your mass stays constant; your weight changes on different planets
  • F = G×M×m/R² = m×g (at surface)

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