Calculate and convert gravitational force between objects using Newton's Law of Universal Gravitation
Newton's Law of Universal Gravitation states that every particle attracts every other particle in the universe with a force that is directly proportional to the product of their masses and inversely proportional to the square of the distance between their centers.
F = G × (m₁ × m₂) / r²
Where:
• F = gravitational force
• G = gravitational constant (6.67430 × 10⁻¹¹ N•m²/kg²)
• m₁, m₂ = masses of two bodies
• r = distance between centers of mass
Try changing units or values to see how gravity changes!
The gravitational force between Earth (5.972 × 10²⁴ kg) and Moon (7.347 × 10²² kg) at average distance of 384,400 km:
F ≈ 1.98 × 10²⁰ N (or about 2.0 × 10²⁰ dynes, 4.45 × 10¹⁹ lbf)
The gravitational force between two 1000 kg objects separated by 10 meters:
F ≈ 6.674 × 10⁻⁷ N (very weak force)
The gravitational force between Sun (1.989 × 10³⁰ kg) and Earth (5.972 × 10²⁴ kg) at average distance of 1 AU (149.6 million km):
F ≈ 3.54 × 10²² N (extremely strong force that keeps Earth in orbit)
Try doubling the distance between two masses and observe how the force becomes 1/4 of the original value. This demonstrates the inverse square law of gravitation.
Try doubling one mass while keeping other parameters constant. The force should exactly double, showing the direct proportionality to mass.
This tool helps you understand the invisible gravitational pull between objects. While we feel Earth's gravity daily, this calculator reveals how gravity works between any two masses, from planets to everyday objects. For related calculations, you might also find our online force converter helpful for exploring other types of forces.
You might need this converter when:
The standard force unit. 1 N is the force needed to accelerate 1 kg by 1 m/s². An apple weighs about 1 N on Earth.
A tiny force unit. 1 dyne = 0.00001 N. Used in physics for very small forces.
The force of Earth's gravity on one pound of mass. Familiar for weight measurements.
To understand your results:
A: The force is incredibly weak - about 0.000000001 N for two people standing close. Earth's gravity (about 700 N on you) completely overwhelms it.
A: Newton's law works for most situations, but near black holes, Einstein's relativity is needed. For basic comparisons at safe distances, this works fine.
A: G is the proportionality constant that makes the math work with our chosen units. It's one of the most precisely measured constants in physics.
A: Yes! Use the planet's mass and radius as distance. Your mass stays the same, but the gravitational force (your weight) changes. This is essentially calculating a gravitational force between you and the planet.
Educational Tool Notice: This calculator uses Newton's Law of Universal Gravitation with the standard gravitational constant (G = 6.67430 × 10⁻¹¹ N·m²/kg²).
Last Updated: November 2025
This gravitational force converter has been enhanced with practical guidance, real-life examples, and user-friendly explanations while maintaining precise calculation accuracy.
Calculation integrity: All physics formulas and constants remain unchanged from original implementation.
Explore the invisible force that shapes our universe. Start with the examples above, then create your own scenarios!
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