Planet Weight Calculator
Calculate your weight on all 8 planets, the Moon, and Pluto. Compare surface gravity and discover fun facts about weight across the solar system.
Planet Weight Calculator
Calculator
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Formula: Weight on Planet = Earth Weight × (Planet Surface Gravity ÷ Earth Surface Gravity)
Worked example — 26.55 kg on Mars (37.9% of Earth weight)
Formula
Weight on Planet = Earth Weight × (Planet Surface Gravity ÷ Earth Surface Gravity)
Your weight on any celestial body is proportional to its surface gravity compared to Earth's. Surface gravity (g) is determined by the body's mass and radius: g = GM/r². Earth's surface gravity is 9.81 m/s².
Worked Examples
Example 1: Weight on Mars
Problem:A 70 kg person wants to know their weight on Mars.
Solution:Mars gravity = 3.72 m/s², Earth gravity = 9.81 m/s² Ratio = 3.72 / 9.81 = 0.379 Weight on Mars = 70 × 0.379 = 26.55 kg-equivalent
Result:26.55 kg on Mars (37.9% of Earth weight)
Example 2: Weight on Jupiter
Problem:A 150 lb person wants to know their weight on Jupiter.
Solution:Jupiter gravity = 24.79 m/s², Earth gravity = 9.81 m/s² Ratio = 24.79 / 9.81 = 2.527 Weight on Jupiter = 150 × 2.527 = 379.1 lbs
Result:379.1 lbs on Jupiter (252.7% of Earth weight)
Frequently Asked Questions
Does your mass change on other planets?
No. Mass is the amount of matter in your body and stays constant everywhere in the universe. What changes is your weight, which is the force of gravity acting on your mass. Weight = mass × gravitational acceleration. Since each planet has a different surface gravity, your weight varies, but your mass (in kilograms) remains the same.
Why is Jupiter's gravity so strong?
Jupiter is the most massive planet in our solar system at 1.898 × 10²⁷ kg — about 318 times Earth's mass. Despite being a gas giant with lower density, its enormous mass produces surface gravity of 24.79 m/s², about 2.53 times Earth's. This means a 70 kg person would weigh about 177 kg-equivalent on Jupiter.
How is surface gravity calculated?
Surface gravity is calculated using 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 the planet's radius. A planet can be very massive but if it has a large radius, its surface gravity may be moderate (like Saturn).
Could humans walk on all planets?
Practically, no. Mercury, Venus, Jupiter, Saturn, Uranus, and Neptune have hostile environments (extreme temperatures, no solid surface for gas giants, crushing atmospheric pressure). Mars and the Moon are the most feasible. On Mars (0.38g), walking would feel light and bouncy. On the Moon (0.17g), astronauts developed a hopping gait because normal walking was inefficient.
Why do Mercury and Mars give almost the same weight when Mercury is much smaller?
Because surface gravity depends on density as well as size. Writing the mass as density times volume turns g = GM/r squared into g proportional to density times radius, so a small dense world can match a larger loose one. Mercury has a radius of about 2,440 km but a mean density near 5,427 kg per cubic metre, second only to Earth thanks to its oversized iron core. Mars is far bigger at 3,390 km yet much less dense at about 3,933. The two products land within one percent of each other, which is why the table shows 3.70 m/s squared for Mercury and 3.72 for Mars.
Why is Saturn's surface gravity so close to Earth's when it is 95 times more massive?
Because g = GM/r squared punishes radius twice over. Saturn holds about 95 Earth masses but its equatorial radius is roughly 9.4 times Earth's, so the mass advantage is divided by nearly 89, leaving about 10.4 m/s squared, only some 6 percent above Earth. Its mean density is under 0.7 g/cm cubed, less than water, which is the same fact seen from another angle. Rapid rotation trims the effective equatorial value further.
What does surface gravity mean for a gas giant with no solid surface?
By convention it is quoted at the 1 bar pressure level, the depth where atmospheric pressure matches sea level on Earth, since there is no crust to stand on. The figure is also usually the equatorial one, which is reduced by the centrifugal effect of very fast rotation: Jupiter turns once in under ten hours and is visibly oblate, so its polar gravity is noticeably higher than the 24.79 m/s squared normally listed. Any number for these planets is therefore a defined reference point, not a place you could stand.
Does your weight vary across Earth's own surface?
Slightly, and for two reasons. Earth is an oblate spheroid, so the poles sit closer to the centre than the equator does, and the equator additionally loses a little apparent weight to the centrifugal effect of rotation. The result runs from about 9.78 m/s squared at the equator to 9.83 at the poles, roughly half a percent. Altitude adds a smaller drop, near 0.3 percent at the summit of Everest. The agreed reference value, standard gravity, is 9.80665 m/s squared.
If kilograms measure mass, why does a bathroom scale change its reading on other worlds?
A spring or load-cell scale actually measures force, then quietly divides by Earth's g to display a mass. Take the same scale to the Moon and it would show about one sixth of your Earth reading, because the force pressing on it has fallen while your mass has not. A double-pan balance, which compares your weight against reference masses in the same gravity field, would read correctly anywhere. The unit trap is the kilogram-force, defined as 9.80665 newtons, which is what these readings really report.
How much higher could you jump on the Moon or Mars?
Jump height follows h = v squared divided by 2g, so with the same launch speed from your legs the height scales as the inverse of surface gravity. A standing jump that lifts your centre of mass 0.5 m on Earth would lift it about 3.0 m on the Moon at 1.62 m/s squared and about 1.3 m on Mars at 3.72. You would also hang in the air far longer, since fall time grows as the square root of height divided by g, which is why Apollo crews adopted a hopping gait.
References
Background & Theory
History
Reviewed for accuracy by Daniel Agrici, Founder & Lead Developer · Editorial policy
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