Space & Astronomy

Why You'd Weigh Less on Mars: Gravity Across the Solar System

October 9, 2026
5 min read

The short version

  • Mass stays the same everywhere; weight changes with local gravity.
  • Surface gravity depends on a world's mass and radius — more mass pulls harder, bigger radius weakens it.
  • Mars ≈ 0.38× Earth, the Moon ≈ 0.17×, Jupiter ≈ 2.5×.
  • Astronauts "float" because they're falling, not because gravity is absent.
  • To see your weight across the Solar System, use the Weight on Other Planets Calculator.

The same you, a different number on the scale

Step onto another world and the bathroom scale would tell a very different story — not because you'd changed, but because gravity would. On the Moon you could bound in great floating leaps; on Jupiter you'd struggle to stand. Yet in every case you'd be made of exactly the same stuff. That paradox dissolves the moment you separate two ideas people usually blur together: mass and weight.

Mass vs weight: the distinction that explains everything

  • Mass is the amount of matter in you, measured in kilograms. It's an intrinsic property — the same everywhere in the universe. A 70 kg person is 70 kg of mass on Earth, on Mars, in deep space.
  • Weight is the force that gravity exerts on that mass, measured in newtons. It depends entirely on the local gravity, so it changes from world to world.

Everyday scales read in kilograms, which quietly hides the difference — they're really measuring the force of Earth's gravity on you and converting it, assuming you're on Earth. Take that scale to the Moon and it would read far less, because the Moon pulls on your unchanged mass far more gently. The Weight on Other Planets Calculator shows this directly: your mass stays fixed while the weight figure swings across the Solar System.

What sets a world's gravity

Why does gravity differ between worlds? Two factors:

  • Mass — more massive bodies pull harder. A heavier world has stronger gravity.
  • Radius — a larger radius puts the surface farther from the centre of mass, which weakens surface gravity.

These can pull in opposite directions, which produces some surprises. Jupiter is enormous in size, which alone would weaken its surface gravity — but it's so massive that its gravity still comes out about 2.5 times Earth's at the cloud tops. Saturn, despite being a giant, has surface gravity only slightly above Earth's, because it's relatively low in density and spread over a huge radius. Surface gravity is the tug-of-war between how much a world weighs and how big it is.

A tour of the scale readings

For a 70 kg person on Earth, here's roughly what the scale would say elsewhere (as the equivalent Earth-kg the scale is calibrated for):

  • The Moon (0.17× Earth) → ~12 kg. Hence the Apollo astronauts' bounding gait.
  • Mars (0.38×) → ~27 kg. Light enough to feel spring-heeled, strong enough to walk normally.
  • Jupiter (2.5×) → ~177 kg. Standing would be a struggle.
  • The Sun (28×) → ~1,955 kg — crushing, if standing on it were remotely possible.
  • Pluto (0.06×) → ~4 kg. Almost floating.

Through all of it, the person's mass is unchanged at 70 kg. Only the gravitational force on it — their weight — differs. That's the whole point, and it's weirdly delightful to see laid out.

So why do astronauts float?

If gravity is always acting, why do astronauts on the Space Station drift around weightless? Not because they've escaped gravity — at that altitude Earth's gravity is still almost as strong as on the ground. They float because they're in continuous free fall.

An orbiting spacecraft is essentially falling toward Earth forever, moving sideways fast enough that it keeps missing. Everything inside falls at the same rate as the craft, so nothing presses the astronauts against a floor — there's no support force, and without that upward push, there's no sensation of weight. "Weightlessness" is really perpetual falling, which is why it's more accurately called microgravity. It's the same reason you feel momentarily lighter at the top of a roller-coaster drop. Gravity is still there; it's just no longer being resisted.

Seeing your weight out there

Enter your weight into the Weight on Other Planets Calculator to see it transformed across every world in the Solar System. For the related idea of how fast you'd need to go to leave a world entirely, see the Escape Velocity Calculator.

Sources

  1. NASA. Planetary Fact Sheets — surface gravity of Solar System bodies.
  2. Newton, Isaac. Philosophiæ Naturalis Principia Mathematica (1687) — law of universal gravitation.
  3. NASA. What Is Microgravity? — educational resources on free fall and orbit.

This article is for general educational purposes.

TA

Written by

Tufail Ahmed

Computer Scientist

Tufail builds CalcPool's calculators and writes the research behind them, turning documented formulas and primary sources into tools and explainers you can actually use.

Reviewed by Khizar Nadim · Technical Reviewer