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    Gravitational Force Calculator

    The gravitational pull between Earth and the Moon is 1.98211 × 10²⁰ N: F = Gm₁m₂/r² with the two masses and the 384,400 km between their centres.

    Solve for:

    Earth: 5.972e24 kg; Sun: 1.989e30 kg.

    Moon: 7.348e22 kg.

    Earth–Moon: 384,400 km = 3.844e8 m.

    Gravitational force F =

    1.98211072907925 × 10²⁰ N

    In kN
    1.982110729 × 10¹⁷ kN
    In mN
    1.982110729 × 10²³ mN
    In lbf
    4.455962181 × 10¹⁹ lbf
    In kgf
    2.021190446 × 10¹⁹ kgf
    In dyn
    1.982110729 × 10²⁵ dyn
    Pull of m₁ on m₂ (field g = Gm₁/r²)
    0.0026974833 m/s²
    G (CODATA 2018)
    6.67430 × 10⁻¹¹ N·m²/kg²
    Step-by-step solution
    1. F = G × m₁ × m₂ ÷ r²
    2. F = G × (5.972 × 10²⁴) × (7.348 × 10²²) ÷ 384400000²
    3. F = 1.982110729 × 10²⁰ N

    Gravitational Force Formula

    F = G m₁ m₂ / r²

    G = 6.67430 × 10⁻¹¹ N·m²/kg², m₁ and m₂ the masses, r the distance between their centres

    Worked Example

    Earth (5.972 × 10²⁴ kg) and the Moon (7.348 × 10²² kg) 384,400 km apart:

    1. F = G × m₁ × m₂ ÷ r²
    2. F = G × (5.972 × 10²⁴) × (7.348 × 10²²) ÷ 384400000²
    3. F = 1.982110729 × 10²⁰ N

    In mN: 1.982110729 × 10²³ mN · In lbf: 4.455962181 × 10¹⁹ lbf · In kgf: 2.021190446 × 10¹⁹ kgf · In dyn: 1.982110729 × 10²⁵ dyn · Pull of m₁ on m₂ (field g = Gm₁/r²): 0.0026974833 m/s² · G (CODATA 2018): 6.67430 × 10⁻¹¹ N·m²/kg²

    Gravity on a planet’s surface

    Setting F = mg for an object on a planet gives g = GM/R². With Earth’s mass and mean radius of 6371 km this is about 9.82 m/s², close to standard gravity 9.80665 m/s²; the small difference comes from Earth’s rotation and its flattened shape.

    More Forces and Newton’s Laws Calculators

    Frequently asked questions

    What is the universal gravitational constant G?

    G = 6.67430 × 10⁻¹¹ N·m²/kg² (CODATA 2018). It is one of the least precisely known constants, uncertain in the fifth digit, so answers beyond five significant figures reflect the inputs rather than nature.

    Why is r measured between centres?

    A uniform sphere attracts as if all its mass sat at its centre, so for planets and balls r is the centre-to-centre distance, not the gap between surfaces.

    How does force change with distance?

    It falls with the square of the distance: doubling r cuts the force to a quarter; ten times further gives one hundredth.

    Sources

    Last reviewed: . Factors are stored exactly and computed with 50-digit decimal arithmetic. See how we verify conversion factors.

    Cite this page

    APA

    Scientific Converters. (2026, October 15). Gravitational Force Calculator. Retrieved October 25, 2026, from https://scientificconverters.com/calculators/gravitational-force-calculator/

    IEEE

    Scientific Converters, "Gravitational Force Calculator," scientificconverters.com. Accessed: Oct. 25, 2026. [Online]. Available: https://scientificconverters.com/calculators/gravitational-force-calculator/

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