Surface Gravity Calculator
Find the surface gravity of any planet relative to Earth.
Result
How it is calculated
Instead of using the gravitational constant directly, the tool scales everything against Earth: g = (M ÷ R²) × 9.80665. Here M is the body's mass in Earth masses and R is its radius in Earth radii, both unitless multiples of Earth. Gravity falls with the square of the radius, so a body twice as wide with the same mass has a quarter of the pull. The tool shows g in m/s² with two decimals and also as a multiple of Earth's surface gravity with three decimals. Mass and radius must both be above zero. The result is the gravity at the surface of a non-rotating sphere and ignores spin, which lowers the effective pull near the equator.
Worked example
Mars has about 0.107 Earth masses and 0.532 Earth radii. Radius squared: 0.532² = 0.283. Mass divided by that: 0.107 ÷ 0.283 = 0.378 of Earth's pull. Times 9.80665 gives about 3.71 m/s², shown as 3.71 m/s², and the tool also shows 0.378 g. A 70 kg person would weigh like about 26 kg on Earth.
Common mistakes
- Entering mass in kilograms or radius in kilometres. The fields use Earth units, so Earth itself is 1 and 1, and Mars is about 0.107 and 0.532.
- Entering the diameter instead of the radius. Doubling the radius cuts gravity to a quarter, so a diameter gives a result four times too low.
- Confusing mass and weight. The tool gives the acceleration at the surface; your mass stays the same on every body, only your weight changes.
- Applying it to gas giants as if it were solid ground. For a planet such as Jupiter the result is the pull at the cloud tops, not at a surface you can stand on.
- Treating the result as the pull inside the body or at some height above it. It holds only at the stated radius.
Sources
- 13.2 Gravitation near Earth's Surface - University Physics Volume 1 — OpenStax, University Physics Volume 1
- CODATA Value: standard acceleration of gravity — NIST Fundamental Physical Constants
About this calculator
This calculator computes a planet or body's surface gravity from g = GM/r², then expresses it relative to Earth's 9.8 m/s² so the result reads as a simple multiplier like 0.38g for Mars or 2.5g for Jupiter.
Astronomy students, sci-fi writers, and space enthusiasts use it to compare how heavy an object — or a person — would feel on another planet, moon, or exoplanet given its mass and radius. Surface gravity is reported both in m/s² and in Earth-relative units.
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Comments (1)
For gas giants there is no solid surface, so the radius you enter decides what the answer means. Astronomers usually quote the radius at the 1 bar pressure level. With about 317.8 Earth masses and 11.2 Earth radii for Jupiter, the tool gives roughly 2.5 g, but a different reference radius would shift it. The result also ignores rotation. Which planet, moon or exoplanet are you checking, and where did you get its mass and radius?