Mr Calcu | Quickly calculate the gravitational pull between two masses—perfect for students, educators, and science enthusiasts.

Discover and compute gravitational force instantly. Empower your curiosity and simplify complex physics with this intuitive, science-backed calculator.

Gravitational Force Calculator

Gravitational Force Calculator Guidelines

Getting started is easy—follow these steps to calculate gravitational force in seconds:

Usage Guidelines

  • Input the mass of Object 1 and Object 2.
  • Specify the distance between their centers.
  • Choose your unit system (Metric or Imperial).
  • Units are auto-converted internally to SI (kg, m).
  • The output force is shown in Newtons (N).

Tips for Accurate Results

  • Use scientific notation for very large or small values.
  • Ensure distance is not zero — this leads to undefined values.
  • Set mass to 0 only if simulating absence of gravitational interaction.

Gravitational Force Calculator Description

Understanding Gravitational Force

Gravitational force is one of the four fundamental forces in physics. It governs the attraction between any two bodies with mass. This calculator helps quantify that attraction based on Newton’s Law of Universal Gravitation.

Formula

F = G * (m₁ * m₂) / r²
  • F: Gravitational force (Newtons)
  • G: Gravitational constant (6.67430 × 10⁻¹¹ m³/kg⋅s²)
  • m₁, m₂: Masses of the objects (kg)
  • r: Distance between object centers (m)

Key Principles

  • Force increases with greater mass.
  • Force decreases rapidly with distance.
  • Gravity is always attractive.

Case Study: Earth & Moon

Mass of Earth: 5.972 × 10²⁴ kg
Mass of Moon: 7.348 × 10²² kg
Distance: 384,400 km

F = G * (5.972e24 * 7.348e22) / (3.844e8)² ≈ 1.982 × 10²⁰ N

This is the force responsible for the Moon's orbit.

Case Study: Two People

Two 70 kg individuals standing 1 m apart experience:

F = G * (70 * 70) / (1)² ≈ 3.27 × 10⁻⁷ N

This force exists but is negligible in daily life.

Derivation Overview

Combining proportionalities:

F ∝ m₁ * m₂
F ∝ 1 / r²
⇒ F = G * (m₁ * m₂) / r²

G is measured experimentally and is constant across the universe.

Try it now to explore the invisible forces shaping our universe!

Example Calculation

Mass 1Mass 2DistanceForce
5.972e24 kg7.348e22 kg3.844e8 m1.982e20 N
70 kg70 kg1 m3.27e-7 N
1e30 kg1e30 kg1e9 m6.674e31 N
1 kg1 kg1e-10 m6.674e-1 N
0 kg1000 kg10 m0 N

Frequently Asked Questions

A fundamental force attracting two masses according to Newton's law of universal gravitation.

Using the formula F = G * (m₁ * m₂) / r², where G is the gravitational constant.

The gravitational force becomes zero, since the product of masses includes a zero factor.

No, classical gravity is always attractive. Repulsive effects exist only in speculative physics theories.

Because gravitational force is inversely proportional to the square of distance. As distance approaches zero, force tends toward infinity.

It is accurate for basic estimates. However, relativistic effects are not considered and become significant near massive bodies like black holes.

No, it assumes point masses or spherical symmetry. Real objects may have non-uniform mass distributions.

Use the satellite's mass, Earth's mass (5.972e24 kg), and the distance from Earth's center to the satellite in meters for accurate results.

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