Mercury & Mars weigh alike
Both worlds tug at ~0.38 g, so your Mars “moonwalk” weight also works for Mercury—even though one bakes near the Sun and the other orbits farther out.
mass × g. Changes from world to world.
Weight is a force (Newtons) caused by gravity. Your mass stays the same everywhere,
but weight changes with the local surface gravity g.
Earth mass (kg) from your input: - If you enter Earth weight in kg (a scale reading): mass ≈ kg_value - If you enter Earth weight in lb: mass ≈ lb × 0.45359237 - If you enter Earth weight in N: mass ≈ N ÷ g_earth - If you enter mass (kg): mass = kg Weight on a world = mass × g_world (in Newtons) Earth-relative weight factor = g_world ÷ g_earth
We use standard surface gravity values based on mean radii and mass. Real bodies vary slightly with latitude and altitude.
On Earth, most bathroom scales show kilograms, but they’re really reporting how much
force your body exerts on the scale under Earth’s gravity. That’s why this tool lets you
enter either Earth weight (kg, lb, or N) or your mass in kilograms. Your mass is an
amount of “stuff” and it doesn’t change when you travel; what changes is the local
g, the strength of gravity at the surface of another world.
Surface gravity depends on two things: the world’s mass and its radius. A heavier world pulls harder, but a larger radius spreads that pull over a bigger distance. This is why Saturn (huge but puffy) has surface gravity only a bit stronger than Earth’s, while Jupiter (even denser) produces a much bigger pull. Small rocky bodies like the Moon or Ceres can only tug a little, so you’d feel almost “bouncy” there.
Quick example with a 40 kg person:
Fun takeaway: if you can jump 0.4 m on Earth, you might jump a couple of meters on the
Moon—same legs, smaller g!
Not always. Radius matters. If a planet is very large and not very dense, the surface can be
far from the center, reducing g. That’s why Saturn’s surface gravity is close to Earth’s
even though Saturn could fit many Earths inside by volume.
Your scale measures force but labels it in kilograms for convenience—think “kilogram-force.” This tool converts that reading into true mass, then recomputes weight in Newtons for other worlds.
They don’t have solid surfaces. “Surface gravity” is a standard reference value, useful for learning and comparisons—not an invitation to land there.
Tip: switch the calculator to Mass mode if you know your exact kilograms. The results list shows Newtons plus an Earth multiplier (e.g., “0.38× Earth” for Mars), which is perfect for classrooms and quick demos.
Both worlds tug at ~0.38 g, so your Mars “moonwalk” weight also works for Mercury—even though one bakes near the Sun and the other orbits farther out.
Venus clocks in at 0.904 g. A 70 kg person would appear as ~63 kg there—a barely noticeable difference until the pressure and heat remind you you’re not home.
Neptune’s surface gravity (1.14 g) beats Saturn’s (1.07 g) despite Saturn being larger. Density matters more than size—sort the results table to see this surprise.
Enter 180 lb and the Jupiter row shows ~425 lb. That’s why our chart’s dashed Earth line helps you see the more-than-2× jump at a glance.
On dwarf planet Ceres you’d weigh about 3% of your Earth value—50 kg becomes 1.5 kg. The calculator’s bars nearly vanish for these tiny worlds.