About the Weight on Other Planets Calculator
Your weight changes depending on which world you are standing on, even though your mass stays exactly the same. Weight is a force — how hard gravity pulls on your mass — and it is calculated as W = m × g, where m is your mass and g is the local surface gravity. This calculator takes the weight you enter for Earth, works out your unchanging mass, and then multiplies that mass by the real surface gravity of the world you choose to find out what you would weigh there.
Understanding the formula
Surface gravity itself comes from Newton's law of universal gravitation: g = GM / R², where G is the gravitational constant (6.674 × 10⁻¹¹ N·m²/kg²), M is the planet's mass, and R is its radius. A more massive planet pulls harder, but a larger radius spreads that pull over a bigger sphere and weakens it at the surface — which is why Jupiter, despite being about 318 times more massive than Earth, has only around 2.53 times Earth's surface gravity. Instead of recomputing g = GM/R² from raw mass and radius, this calculator uses each planet's published surface gravity (in m/s²), forms the ratio g_other ÷ g_earth, and applies it to your mass: W_other = m × g_other = W_earth × (g_other ÷ g_earth).
Working with units
- Enter your Earth weight in pounds (lbf), kilograms (used colloquially as a weight unit), or newtons (the SI unit of force) — the result is returned in the same unit.
- Behind the scenes, the calculator converts your entry to a force in newtons using standard gravity (g = 9.80665 m/s²) and 1 lbf = 4.4482216153 N, then recovers your invariant mass in kilograms.
- That mass is multiplied by the destination world's surface gravity to get your weight there, then converted back to whichever unit you entered.
Knowing the limits
The gas giants — Jupiter, Saturn, Uranus, and Neptune — have no solid surface, so their listed "surface gravity" is a standard reference value taken at the level where atmospheric pressure equals 1 bar, not a place you could actually stand. Published surface gravity figures are also equatorial averages; a fast-spinning, oblate planet like Jupiter or Saturn has measurably lower gravity at its equator than at its poles because of centrifugal effects, so treat results here as solar-system-scale estimates rather than a precise value for one exact location.