Beginner

Surface Gravity Calculator

Find the gravitational acceleration at the surface of any celestial body from its mass and radius.
Mass of the body

Mass unit

Mean radius of the body

Radius unit

Surface gravity
9,820m/s²

Relative to Earth: 1,001 g

M = 5,972,000,000,000,000,000,000,000R = 6,371,000
Planetary body: g = G·M / R²
Surface gravity
9,8195 m/s²
Relative to Earth
1,0013 g
Massa
5 972 000 000 000 000 000 000 000 kg
Säde
6 371 000 m
Step by step
  1. 1

    Radius squared R²

    6 371 000 × 6 371 000 = 40 589 641 000 000
  2. 2

    G × M (numerator)

    6.674×10⁻¹¹ × 5 972 000 000 000 000 000 000 000 = 398 571 280 000 000
    G is the gravitational constant; M is the body mass in kg.
  3. 3

    Surface gravity g = G·M ÷ R²

    398 571 280 000 000 ÷ 40 589 641 000 000 = 9,820
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Miten tämä laskin toimii?

Surface gravity is g = G·M/R², where G = 6.674×10⁻¹¹, M is the body's mass, and R its radius. Enter mass and radius in your chosen units to get g in m/s² and as a multiple of Earth's 9.80665 m/s². Larger mass raises g; larger radius lowers it by the square.

Kaava
g = G·M / R² (G = 6.674e-11 N·m²/kg²)
How this is calculated

Surface gravity is the gravitational acceleration felt by an object resting at the surface of a body. It follows directly from Newton's law of universal gravitation: the force on a unit mass is G·M/R², where G is the gravitational constant (6.674×10⁻¹¹ N·m²/kg²), M is the body's mass, and R is the distance from its centre to the surface (its radius).

Enter the mass M (in kilograms or Earth masses, where 1 Earth mass = 5.972×10²⁴ kg) and the radius R (in metres, kilometres, or Earth radii, where 1 Earth radius = 6.371×10⁶ m). The calculator converts both to SI units, computes g in m/s², and divides by the standard Earth value g₀ = 9.80665 m/s² to express the result as a multiple of Earth gravity.

The model assumes a spherically symmetric, non-rotating body, so g depends only on total mass and radius — not on internal density distribution. Real bodies that rotate quickly or are oblate have a slightly lower effective gravity at the equator. Radius and mass must both be positive; a zero or negative radius is rejected to avoid division by zero.

Usein kysytyt kysymykset

Surface gravity scales with mass but falls off with the square of the radius. A large, low-density planet can have weaker surface gravity than a smaller, denser one because its surface sits farther from the centre of mass.

Using M = 5.972×10²⁴ kg and R = 6.371×10⁶ m gives about 9.82 m/s², very close to the standard reference value g₀ = 9.80665 m/s² used to define 1 g.

This calculator gives true gravitational acceleration. On a spinning body, centrifugal effects slightly reduce the measured weight at the equator, so the effective gravity there is a little less than G·M/R².

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APA

TG we-Calculate Editorial Team. (2026). Surface Gravity Calculator [Online calculator]. TG we-Calculate. https://we-calculate.com/fi/calculator/surface-gravity-calculator

Chicago

TG we-Calculate Editorial Team. "Surface Gravity Calculator." TG we-Calculate. 2026. https://we-calculate.com/fi/calculator/surface-gravity-calculator.

IEEE

TG we-Calculate Editorial Team, "Surface Gravity Calculator," TG we-Calculate, 2026. [Online]. Available: https://we-calculate.com/fi/calculator/surface-gravity-calculator

BibTeX

@misc{wecalculate_surface_gravity_calculator, title = {Surface Gravity Calculator}, author = {{TG we-Calculate Editorial Team}}, howpublished = {\url{https://we-calculate.com/fi/calculator/surface-gravity-calculator}}, year = {2026}, note = {TG we-Calculate} }

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