{"id":628,"date":"2026-07-19T17:09:21","date_gmt":"2026-07-19T17:09:21","guid":{"rendered":"https:\/\/physicsfundamentalsinfo.com\/blog\/?p=628"},"modified":"2026-07-19T17:09:23","modified_gmt":"2026-07-19T17:09:23","slug":"weight-on-other-planets","status":"publish","type":"post","link":"https:\/\/physicsfundamentalsinfo.com\/blog\/mechanics\/weight-on-other-planets\/","title":{"rendered":"Weight on Other Planets: Moon, Mars &amp; More"},"content":{"rendered":"\n<div class=\"pf-citation\"><div class=\"eyebrow\">Definition<\/div><p>\nWeight on other planets is the gravitational pull on an object, calculated with the formula weight = mass \u00d7 gravity (W = m \u00d7 g). Your mass stays the same everywhere, but each world&#8217;s surface gravity g differs \u2014 1.62 m\/s\u00b2 on the Moon, 3.72 on Mars, 24.79 on Jupiter \u2014 so the same body weighs far more on some planets than others.\n<\/p><\/div>\n<p>Step onto a bathroom scale on the Moon and the number would drop to about a sixth of what you see at home \u2014 not because you&#8217;ve lost anything, but because the Moon pulls on you far more gently than Earth does. Fly to Jupiter&#8217;s cloud tops and the same scale would read roughly two and a half times higher. You, unchanged, would be crushingly heavy.<\/p>\n<p>That single idea \u2014 the <em>you<\/em> stays constant while the <em>pull<\/em> changes \u2014 is what makes weight on other planets one of the most intuitive ways into gravity. Below you&#8217;ll find the formula, a full solar-system comparison, worked examples, and the misconceptions that trip almost everyone up.<\/p>\n<h2>What Is Weight on Other Planets?<\/h2>\n<p>Weight on other planets is the force of gravity acting on a mass at that world&#8217;s surface, and it changes because each planet has its own gravitational strength. Weight is a <strong>force<\/strong>, measured in newtons (N), not a fixed property you carry around. It is the answer to &#8220;how hard is this world pulling me down right now?&#8221;<\/p>\n<p>Mass is the constant. A 70 kg astronaut is 70 kg of matter on Earth, in orbit, on Mars, and adrift between the stars.<\/p>\n<p>What shifts from place to place is how strongly gravity tugs on that matter \u2014 and that tug is what a scale actually reads. Keeping these two ideas apart is the whole game, which is exactly why the <a href=\"https:\/\/physicsfundamentalsinfo.com\/blog\/mechanics\/weight-vs-mass\/\">difference between weight and mass<\/a> is worth nailing down first.<\/p>\n<p>Think of it like this. Your mass is your bank balance; your weight is how heavy that balance feels when someone hands it to you in coins. On the Moon, an unseen cashier hands you the same money in a much lighter bag.<\/p>\n<h2>The Weight on Other Planets Formula<\/h2>\n<p>Weight on any planet is found by multiplying an object&#8217;s mass by that planet&#8217;s surface gravity. There is only one equation to learn, and it works for every world in the solar system.<\/p>\n<div class=\"pf-formula\">W = m \u00d7 g<\/div>\n<p>Every symbol, with its SI unit:<\/p>\n<div class=\"pf-table-scroll\" style=\"display:block;width:100%;max-width:100%;overflow-x:auto;-webkit-overflow-scrolling:touch;margin:1.5em 0;\">\n<table style=\"width:100%;border-collapse:collapse;word-break:break-word;\">\n<thead>\n<tr style=\"background:#142139;color:#FAF6EE;\">\n<th style=\"padding:10px;border:1px solid #D9CFB8;text-align:left;\">Symbol<\/th>\n<th style=\"padding:10px;border:1px solid #D9CFB8;text-align:left;\">Quantity<\/th>\n<th style=\"padding:10px;border:1px solid #D9CFB8;text-align:left;\">SI unit<\/th>\n<\/tr>\n<\/thead>\n<tbody>\n<tr>\n<td style=\"padding:10px;border:1px solid #D9CFB8;\"><strong>W<\/strong><\/td>\n<td style=\"padding:10px;border:1px solid #D9CFB8;\">Weight (the gravitational force)<\/td>\n<td style=\"padding:10px;border:1px solid #D9CFB8;\">newton (N)<\/td>\n<\/tr>\n<tr>\n<td style=\"padding:10px;border:1px solid #D9CFB8;\"><strong>m<\/strong><\/td>\n<td style=\"padding:10px;border:1px solid #D9CFB8;\">Mass of the object (never changes)<\/td>\n<td style=\"padding:10px;border:1px solid #D9CFB8;\">kilogram (kg)<\/td>\n<\/tr>\n<tr>\n<td style=\"padding:10px;border:1px solid #D9CFB8;\"><strong>g<\/strong><\/td>\n<td style=\"padding:10px;border:1px solid #D9CFB8;\">Surface gravity (gravitational field strength)<\/td>\n<td style=\"padding:10px;border:1px solid #D9CFB8;\">newton per kilogram (N\/kg), equal to m\/s\u00b2<\/td>\n<\/tr>\n<\/tbody>\n<\/table>\n<\/div>\n<p>Here is a detail worth pausing on: <strong>g<\/strong> can be read two ways that are numerically identical. It is the gravitational field strength in N\/kg, and it is also the acceleration due to gravity in m\/s\u00b2. On Earth that number is about 9.81 whichever way you read it.<\/p>\n<p>W = m \u00d7 g is really <a href=\"https:\/\/physicsfundamentalsinfo.com\/blog\/mechanics\/newtons-second-law\/\">Newton&#8217;s second law (F = m \u00d7 a)<\/a> with gravity supplying the acceleration \u2014 which is why weight is measured in newtons, and why <a href=\"https:\/\/physicsfundamentalsinfo.com\/blog\/mechanics\/types-of-forces\/\">weight is a force<\/a>, not a mass. To skip the arithmetic and compare worlds instantly, drop your mass into our <a href=\"https:\/\/physicsfundamentalsinfo.com\/calculators\/weight-on-other-planets\">Weight on Other Planets calculator<\/a> and switch between planet presets.<\/p>\n<div class=\"pf-sim-slot\"><div class=\"pf-sim-slot-header\"><span class=\"icon-dot\"><\/span><span class=\"label\">Weight on Other Planets Lab<\/span><\/div><div class=\"pf-sim-slot-body\">\n<style>\n.pf-sim-frame{width:100%;border:none;height:600px}\n@media(max-width:760px){.pf-sim-frame{height:1000px}}\n<\/style>\n<iframe src=\"\/labs\/weight-on-other-planets.html?embed=1\" class=\"pf-sim-frame\" loading=\"lazy\"><\/iframe>\n<\/div><\/div>\n<h2>Why Does Weight Change from Planet to Planet?<\/h2>\n<p>Your weight changes because a planet&#8217;s surface gravity depends on both its mass and its radius, and those two things vary enormously across the solar system. The surface gravity comes straight from Newton&#8217;s law of universal gravitation:<\/p>\n<div class=\"pf-formula\">g = G \u00d7 M \/ r\u00b2<\/div>\n<ul>\n<li><strong>G<\/strong> \u2014 the gravitational constant, 6.674 \u00d7 10<sup>-11<\/sup> N\u00b7m\u00b2\/kg\u00b2 (the same everywhere in the universe).<\/li>\n<li><strong>M<\/strong> \u2014 the mass of the planet, in kilograms (kg).<\/li>\n<li><strong>r<\/strong> \u2014 the distance from the planet&#8217;s centre to its surface, i.e. its radius, in metres (m).<\/li>\n<li><strong>g<\/strong> \u2014 the resulting surface gravity, in m\/s\u00b2.<\/li>\n<\/ul>\n<p>Notice what the equation is telling you. Pile on more mass and g climbs \u2014 but push the surface further from the centre, a bigger radius, and g falls off with the <em>square<\/em> of that distance.<\/p>\n<p>Gravity is a tug-of-war between how much stuff a planet has and how spread out that stuff is.<\/p>\n<svg viewBox=\"0 0 560 300\" role=\"img\" aria-label=\"Diagram of the equation g equals big G times planet mass divided by radius squared, showing that more mass strengthens gravity while a larger radius weakens it\" xmlns=\"http:\/\/www.w3.org\/2000\/svg\" style=\"width:100%;height:auto;max-width:640px;display:block;margin:1.5em auto;\">\n<rect x=\"0\" y=\"0\" width=\"560\" height=\"300\" fill=\"#0A1628\" rx=\"6\"><\/rect>\n<circle cx=\"150\" cy=\"170\" r=\"95\" fill=\"#142139\" stroke=\"#C8932A\" stroke-width=\"2\"><\/circle>\n<circle cx=\"150\" cy=\"170\" r=\"4\" fill=\"#FAF6EE\"><\/circle>\n<text x=\"160\" y=\"188\" font-family=\"Arial, sans-serif\" font-size=\"15\" fill=\"#FAF6EE\">M<\/text>\n<line x1=\"150\" y1=\"170\" x2=\"150\" y2=\"78\" stroke=\"#C5D0DC\" stroke-width=\"1.5\" stroke-dasharray=\"4 3\"><\/line>\n<text x=\"158\" y=\"128\" font-family=\"Arial, sans-serif\" font-size=\"15\" fill=\"#C5D0DC\">r<\/text>\n<circle cx=\"150\" cy=\"42\" r=\"7\" fill=\"#FAF6EE\"><\/circle>\n<line x1=\"150\" y1=\"49\" x2=\"150\" y2=\"66\" stroke=\"#FAF6EE\" stroke-width=\"3\"><\/line>\n<line x1=\"150\" y1=\"55\" x2=\"139\" y2=\"63\" stroke=\"#FAF6EE\" stroke-width=\"3\"><\/line>\n<line x1=\"150\" y1=\"55\" x2=\"161\" y2=\"63\" stroke=\"#FAF6EE\" stroke-width=\"3\"><\/line>\n<line x1=\"150\" y1=\"66\" x2=\"143\" y2=\"75\" stroke=\"#FAF6EE\" stroke-width=\"3\"><\/line>\n<line x1=\"150\" y1=\"66\" x2=\"157\" y2=\"75\" stroke=\"#FAF6EE\" stroke-width=\"3\"><\/line>\n<line x1=\"190\" y1=\"48\" x2=\"190\" y2=\"86\" stroke=\"#C8932A\" stroke-width=\"3\"><\/line>\n<polygon points=\"190,96 184,82 196,82\" fill=\"#C8932A\"><\/polygon>\n<text x=\"200\" y=\"74\" font-family=\"Arial, sans-serif\" font-size=\"14\" fill=\"#C8932A\">W = m \u00d7 g<\/text>\n<text x=\"300\" y=\"72\" font-family=\"Arial, sans-serif\" font-size=\"25\" font-weight=\"bold\" fill=\"#C8932A\">g = G \u00b7 M \/ r\u00b2<\/text>\n<text x=\"300\" y=\"120\" font-family=\"Arial, sans-serif\" font-size=\"15\" fill=\"#FAF6EE\">Surface gravity g sets your weight.<\/text>\n<text x=\"300\" y=\"156\" font-family=\"Arial, sans-serif\" font-size=\"15\" fill=\"#C5D0DC\">More planet mass (M): stronger gravity<\/text>\n<text x=\"300\" y=\"186\" font-family=\"Arial, sans-serif\" font-size=\"15\" fill=\"#C5D0DC\">Bigger radius (r): weaker gravity<\/text>\n<text x=\"300\" y=\"230\" font-family=\"Arial, sans-serif\" font-size=\"14\" fill=\"#FAF6EE\">So puffy, giant Uranus pulls less<\/text>\n<text x=\"300\" y=\"250\" font-family=\"Arial, sans-serif\" font-size=\"14\" fill=\"#FAF6EE\">on you than small, rocky Earth.<\/text>\n<\/svg>\n<p style=\"text-align:center;font-size:13px;color:#1F2E47;font-style:italic;\">Surface gravity is a balance of a planet&#8217;s mass and its radius \u2014 which is why bigger isn&#8217;t always heavier.<\/p>\n<h3>The counter-intuitive part<\/h3>\n<p>Uranus has about 14.5 times Earth&#8217;s mass, yet you would weigh <em>less<\/em> standing at its cloud tops than at home. Its radius is roughly four times Earth&#8217;s, and squaring that (16\u00d7) more than cancels the extra mass.<\/p>\n<p>Mercury and Mars land at nearly the same surface gravity too, despite Mars being the larger planet \u2014 Mercury is simply far denser. Size alone tells you almost nothing; what matters is how mass and radius combine.<\/p>\n<h2>Your Weight Across the Solar System<\/h2>\n<p>Here is what a 70 kg person would weigh on every major world in the solar system, using each body&#8217;s surface gravity. The final column shows what an ordinary bathroom scale \u2014 calibrated for Earth \u2014 would display, which is the figure most people are really asking about.<\/p>\n<div class=\"pf-table-scroll\" style=\"display:block;width:100%;max-width:100%;overflow-x:auto;-webkit-overflow-scrolling:touch;margin:1.5em 0;\">\n<table style=\"width:100%;border-collapse:collapse;word-break:break-word;\">\n<thead>\n<tr style=\"background:#142139;color:#FAF6EE;\">\n<th style=\"padding:10px;border:1px solid #D9CFB8;text-align:left;\">World<\/th>\n<th style=\"padding:10px;border:1px solid #D9CFB8;text-align:left;\">Surface gravity g (m\/s\u00b2)<\/th>\n<th style=\"padding:10px;border:1px solid #D9CFB8;text-align:left;\">Compared to Earth<\/th>\n<th style=\"padding:10px;border:1px solid #D9CFB8;text-align:left;\">Weight of a 70 kg person (N)<\/th>\n<th style=\"padding:10px;border:1px solid #D9CFB8;text-align:left;\">Earth scale would read<\/th>\n<\/tr>\n<\/thead>\n<tbody>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">The Moon<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">1.62<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">0.17\u00d7 (about 1\/6)<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">113 N<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">~11.6 kg<\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">Mercury<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">3.70<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">0.38\u00d7<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">259 N<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">~26.4 kg<\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">Venus<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">8.87<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">0.90\u00d7<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">621 N<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">~63.3 kg<\/td><\/tr>\n<tr style=\"background:#F5F2EA;\"><td style=\"padding:10px;border:1px solid #D9CFB8;\"><strong>Earth<\/strong><\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\"><strong>9.81<\/strong><\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\"><strong>1.00\u00d7<\/strong><\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\"><strong>687 N<\/strong><\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\"><strong>70 kg<\/strong><\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">Mars<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">3.72<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">0.38\u00d7<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">260 N<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">~26.5 kg<\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">Jupiter*<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">24.79<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">2.53\u00d7<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">1,735 N<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">~177 kg<\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">Saturn*<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">10.44<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">1.06\u00d7<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">731 N<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">~74.5 kg<\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">Uranus*<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">8.69<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">0.89\u00d7<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">608 N<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">~62.0 kg<\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">Neptune*<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">11.15<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">1.14\u00d7<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">781 N<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">~79.6 kg<\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">Pluto<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">0.62<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">0.06\u00d7<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">43 N<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">~4.4 kg<\/td><\/tr>\n<tr><td style=\"padding:10px;border:1px solid #D9CFB8;\">The Sun*<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">274<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">27.9\u00d7<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">19,180 N<\/td><td style=\"padding:10px;border:1px solid #D9CFB8;\">~1,955 kg<\/td><\/tr>\n<\/tbody>\n<\/table>\n<\/div>\n<p><strong>*A note on the gas giants and the Sun:<\/strong> Jupiter, Saturn, Uranus, Neptune and the Sun have no solid surface to stand on, so &#8220;surface gravity&#8221; is measured at the 1-bar cloud level. The values above are mean surface gravities (matching this site&#8217;s calculator). NASA&#8217;s summary Planetary Fact Sheet lists slightly lower <em>equatorial<\/em> figures for the fast-spinning giants \u2014 about 23.1 for Jupiter and 9.0 for Saturn \u2014 because rapid rotation flings a little of your effective weight away at the equator.<\/p>\n<svg viewBox=\"0 0 560 340\" role=\"img\" aria-label=\"Bar chart comparing surface gravity in metres per second squared for the Moon at 1.62, Mars at 3.72, Earth at 9.81 and Jupiter at 24.79\" xmlns=\"http:\/\/www.w3.org\/2000\/svg\" style=\"width:100%;height:auto;max-width:640px;display:block;margin:1.5em auto;\">\n<rect x=\"0\" y=\"0\" width=\"560\" height=\"340\" fill=\"#0A1628\" rx=\"6\"><\/rect>\n<text x=\"280\" y=\"30\" text-anchor=\"middle\" font-family=\"Arial, sans-serif\" font-size=\"16\" font-weight=\"bold\" fill=\"#FAF6EE\">Surface gravity across four worlds (m\/s\u00b2)<\/text>\n<line x1=\"55\" y1=\"280\" x2=\"525\" y2=\"280\" stroke=\"#D9CFB8\" stroke-width=\"1.5\"><\/line>\n<rect x=\"70\" y=\"266\" width=\"70\" height=\"14\" fill=\"#C8932A\"><\/rect>\n<rect x=\"190\" y=\"247\" width=\"70\" height=\"33\" fill=\"#C8932A\"><\/rect>\n<rect x=\"310\" y=\"193\" width=\"70\" height=\"87\" fill=\"#C8932A\"><\/rect>\n<rect x=\"430\" y=\"60\" width=\"70\" height=\"220\" fill=\"#C8932A\"><\/rect>\n<text x=\"105\" y=\"260\" text-anchor=\"middle\" font-family=\"Arial, sans-serif\" font-size=\"14\" fill=\"#FAF6EE\">1.62<\/text>\n<text x=\"225\" y=\"241\" text-anchor=\"middle\" font-family=\"Arial, sans-serif\" font-size=\"14\" fill=\"#FAF6EE\">3.72<\/text>\n<text x=\"345\" y=\"187\" text-anchor=\"middle\" font-family=\"Arial, sans-serif\" font-size=\"14\" fill=\"#FAF6EE\">9.81<\/text>\n<text x=\"465\" y=\"54\" text-anchor=\"middle\" font-family=\"Arial, sans-serif\" font-size=\"14\" fill=\"#FAF6EE\">24.79<\/text>\n<text x=\"105\" y=\"300\" text-anchor=\"middle\" font-family=\"Arial, sans-serif\" font-size=\"14\" fill=\"#C5D0DC\">Moon<\/text>\n<text x=\"225\" y=\"300\" text-anchor=\"middle\" font-family=\"Arial, sans-serif\" font-size=\"14\" fill=\"#C5D0DC\">Mars<\/text>\n<text x=\"345\" y=\"300\" text-anchor=\"middle\" font-family=\"Arial, sans-serif\" font-size=\"14\" fill=\"#C5D0DC\">Earth<\/text>\n<text x=\"465\" y=\"300\" text-anchor=\"middle\" font-family=\"Arial, sans-serif\" font-size=\"14\" fill=\"#C5D0DC\">Jupiter<\/text>\n<\/svg>\n<p style=\"text-align:center;font-size:13px;color:#1F2E47;font-style:italic;\">The Moon barely registers next to Jupiter \u2014 the same reason your Moon weight is tiny and your Jupiter weight is enormous.<\/p>\n<h2>Real-World Examples of Weight on Other Planets<\/h2>\n<p>The clearest example is an Apollo astronaut on the Moon, who weighed about a sixth of their Earth weight. A suited astronaut and life-support pack topping 90 kg pressed on the lunar surface as though they weighed only about 15 kg \u2014 light enough to bound across the regolith in those famous kangaroo hops. NASA&#8217;s <a href=\"https:\/\/science.nasa.gov\/moon\/\" target=\"_blank\" rel=\"noopener\">lunar science pages<\/a> document just how differently the Moon behaves as a world.<\/p>\n<p>Mars is the next frontier, and its 0.38 g reshapes the engineering. A 900 kg rover that would press down with almost 8,800 N on Earth weighs only about 3,350 N on Mars, which changes everything from parachute design to wheel loading. A future 70 kg astronaut would feel like a 26 kg version of themselves \u2014 easier on the joints, though bones and muscles quietly weaken without Earth&#8217;s full pull.<\/p>\n<p>Jupiter is the cautionary tale. You can&#8217;t stand on it \u2014 there&#8217;s no surface, just deepening gas \u2014 but at the cloud tops its 2.53 g would make a 70 kg person feel like 177 kg, a suffocating heaviness. Saturn, oddly, is gentler: despite being 95 times Earth&#8217;s mass, its surface gravity is only about 6% stronger than ours, because it&#8217;s vast and so low-density it would float in a big enough bath.<\/p>\n<figure style=\"margin:32px auto;max-width:640px;text-align:center;\">\n  <img decoding=\"async\" src=\"https:\/\/physicsfundamentalsinfo.com\/blog\/wp-content\/uploads\/2026\/07\/3CorBj4FSCunixkTsDZy5L.jpg\"\n       alt=\"Apollo astronaut on the Moon, where weight is about one sixth of Earth weight\"\n       loading=\"lazy\"\n       style=\"width:100%;height:auto;border-radius:4px;\" \/ width=\"1152\" height=\"1152\">\n  <figcaption style=\"font-size:13px;color:#1F2E47;font-style:italic;margin-top:8px;\">On the Moon&#8217;s 1.62 m\/s\u00b2 gravity, a suited astronaut weighs about a sixth of their Earth weight.<\/figcaption>\n<\/figure>\n<h2>Common Misconceptions About Weight on Other Planets<\/h2>\n<p>Most confusion around weight on other planets comes from mixing up weight with mass, or from misreading what &#8220;no gravity&#8221; actually means. Here are the four that cause the most trouble.<\/p>\n<h3>1. &#8220;My mass changes on the Moon&#8221;<\/h3>\n<p>It doesn&#8217;t. Your mass \u2014 the amount of matter in you \u2014 is identical on the Moon, on Mars, and in deep space. Only your <em>weight<\/em> changes, because weight is the local gravitational force on that mass. This is the single most common slip, and it&#8217;s why the mass\u2013weight distinction matters so much.<\/p>\n<h3>2. &#8220;A bigger, heavier planet always means I weigh more&#8221;<\/h3>\n<p>Not necessarily. Surface gravity depends on mass <em>and<\/em> radius through g = G \u00d7 M \/ r\u00b2, so a huge but spread-out planet can pull weakly. Uranus has over 14 times Earth&#8217;s mass, yet you&#8217;d weigh slightly less there because its radius is so large.<\/p>\n<h3>3. &#8220;Astronauts float because there&#8217;s no gravity in space&#8221;<\/h3>\n<p>There&#8217;s plenty of gravity where the Space Station orbits \u2014 roughly 90% of the surface value. Astronauts feel weightless because they, and their station, are in continuous <a href=\"https:\/\/physicsfundamentalsinfo.com\/blog\/kinematics\/free-fall-physics\/\">free fall<\/a> around Earth, forever falling and forever missing. Weightlessness is falling, not the absence of gravity.<\/p>\n<h3>4. &#8220;The kilograms on a bathroom scale are my weight&#8221;<\/h3>\n<p>True weight is a force in newtons; a scale measures the push against it and then <em>assumes<\/em> Earth&#8217;s gravity to display a mass in kilograms. Carry that same scale to Mars and it would still assume Earth&#8217;s g, so it would under-read your &#8220;kg&#8221; by more than half \u2014 reading a fiction, not your real mass.<\/p>\n<h2>How Weight on Other Planets Connects to Mass, Gravity and Free Fall<\/h2>\n<p>Weight on other planets sits at the crossroads of several core ideas, and seeing the links makes each one click. Because weight is a force, it obeys the same F = m \u00d7 a logic as everything else in dynamics \u2014 gravity just plays the role of the acceleration.<\/p>\n<p>Mass invariance is the foundation: your mass is fixed, your weight is local. That same g controls how fast things accelerate in free fall, which is why a hammer and a feather hit the lunar ground together \u2014 lower g slows the fall for both equally.<\/p>\n<p>And because lifting a mass through a height depends on g, your <a href=\"https:\/\/physicsfundamentalsinfo.com\/blog\/mechanics\/gravitational-potential-energy\/\">gravitational potential energy<\/a> (PE = m \u00d7 g \u00d7 h) shrinks on low-gravity worlds too. Change one planet&#8217;s g and a whole chain of physics quietly rescales.<\/p>\n<h2>Worked Problems<\/h2>\n<div class=\"pf-problem\"><div class=\"pf-problem-num\">Problem 1<\/div><div class=\"pf-problem-question\">A 50 kg student stands on the Moon, where g = 1.62 m\/s\u00b2. What is their weight?<\/div><details><summary>Show Solution<\/summary><div class=\"pf-problem-solution\">\n<strong>Solution:<\/strong>\nStep 1: Use W = m \u00d7 g.\nStep 2: Substitute \u2014 W = 50 kg \u00d7 1.62 m\/s\u00b2.\nStep 3: W = 81 N.\n<strong>Answer: 81 N (compared with 491 N on Earth).<\/strong>\n<\/div><\/details><\/div>\n<div class=\"pf-problem\"><div class=\"pf-problem-num\">Problem 2<\/div><div class=\"pf-problem-question\">The same 50 kg student travels to Mars, where g = 3.72 m\/s\u00b2. What do they weigh now?<\/div><details><summary>Show Solution<\/summary><div class=\"pf-problem-solution\">\n<strong>Solution:<\/strong>\nStep 1: Apply W = m \u00d7 g with Mars gravity.\nStep 2: W = 50 kg \u00d7 3.72 m\/s\u00b2.\nStep 3: W = 186 N.\n<strong>Answer: 186 N \u2014 a little over twice their Moon weight, because Mars pulls more than twice as hard.<\/strong>\n<\/div><\/details><\/div>\n<div class=\"pf-problem\"><div class=\"pf-problem-num\">Problem 3<\/div><div class=\"pf-problem-question\">A rock weighs 120 N on Earth (g = 9.81 m\/s\u00b2). What would it weigh on Jupiter (g = 24.79 m\/s\u00b2)?<\/div><details><summary>Show Solution<\/summary><div class=\"pf-problem-solution\">\n<strong>Solution:<\/strong>\nStep 1: Find the mass first \u2014 rearrange W = m \u00d7 g to m = W \/ g.\nStep 2: m = 120 N \/ 9.81 m\/s\u00b2 = 12.23 kg.\nStep 3: Now weigh it on Jupiter \u2014 W = 12.23 kg \u00d7 24.79 m\/s\u00b2 = 303 N.\n<strong>Answer: about 303 N. Always convert to mass before switching worlds.<\/strong>\n<\/div><\/details><\/div>\n<div class=\"pf-problem\"><div class=\"pf-problem-num\">Problem 4<\/div><div class=\"pf-problem-question\">An astronaut reads 78 kg on an Earth bathroom scale. What would that Earth-calibrated scale read on the Moon (g = 1.62 m\/s\u00b2)?<\/div><details><summary>Show Solution<\/summary><div class=\"pf-problem-solution\">\n<strong>Solution:<\/strong>\nStep 1: The scale reading scales with gravity \u2014 multiply the Earth reading by g(Moon)\/g(Earth).\nStep 2: Ratio = 1.62 \/ 9.81 = 0.165.\nStep 3: Reading = 78 kg \u00d7 0.165 = 12.9 kg.\n<strong>Answer: about 12.9 kg. Their true mass is still 78 kg \u2014 the scale is fooled because it assumes Earth&#8217;s gravity.<\/strong>\n<\/div><\/details><\/div>\n<div class=\"pf-problem\"><div class=\"pf-problem-num\">Problem 5<\/div><div class=\"pf-problem-question\">A rocky planet has mass M = 6.42 \u00d7 10^23 kg and radius r = 3.39 \u00d7 10^6 m. Find its surface gravity (G = 6.674 \u00d7 10^-11 N\u00b7m\u00b2\/kg\u00b2).<\/div><details><summary>Show Solution<\/summary><div class=\"pf-problem-solution\">\n<strong>Solution:<\/strong>\nStep 1: Use g = G \u00d7 M \/ r\u00b2.\nStep 2: Numerator = 6.674 \u00d7 10<sup>-11<\/sup> \u00d7 6.42 \u00d7 10<sup>23<\/sup> = 4.285 \u00d7 10<sup>13<\/sup>.\nStep 3: Denominator = (3.39 \u00d7 10<sup>6<\/sup>)\u00b2 = 1.149 \u00d7 10<sup>13<\/sup>; so g = 4.285 \u00d7 10<sup>13<\/sup> \/ 1.149 \u00d7 10<sup>13<\/sup> = 3.73 m\/s\u00b2.\n<strong>Answer: g \u2248 3.73 m\/s\u00b2 \u2014 these are Mars&#8217;s numbers, so this matches the accepted value of 3.72.<\/strong>\n<\/div><\/details><\/div>\n<div class=\"pf-problem\"><div class=\"pf-problem-num\">Problem 6<\/div><div class=\"pf-problem-question\">A person weighs 700 N on Earth. What would they weigh on Uranus (g = 8.69 m\/s\u00b2), and why is the result surprising?<\/div><details><summary>Show Solution<\/summary><div class=\"pf-problem-solution\">\n<strong>Solution:<\/strong>\nStep 1: Find mass \u2014 m = 700 N \/ 9.81 m\/s\u00b2 = 71.4 kg.\nStep 2: Weight on Uranus \u2014 W = 71.4 kg \u00d7 8.69 m\/s\u00b2.\nStep 3: W = 620 N.\n<strong>Answer: about 620 N \u2014 less than on Earth, even though Uranus has over 14 times Earth&#8217;s mass, because its large radius weakens its surface gravity.<\/strong>\n<\/div><\/details><\/div>\n<div class=\"pf-problem\"><div class=\"pf-problem-num\">Problem 7<\/div><div class=\"pf-problem-question\">What would a 70 kg person weigh at the Sun&#039;s surface, where g = 274 m\/s\u00b2?<\/div><details><summary>Show Solution<\/summary><div class=\"pf-problem-solution\">\n<strong>Solution:<\/strong>\nStep 1: Use W = m \u00d7 g.\nStep 2: W = 70 kg \u00d7 274 m\/s\u00b2.\nStep 3: W = 19,180 N, or about 19.2 kN.\n<strong>Answer: roughly 19,200 N \u2014 nearly 28 times their Earth weight, the equivalent of a small car pressing down on them.<\/strong>\n<\/div><\/details><\/div>\n<div class=\"pf-problem\"><div class=\"pf-problem-num\">Problem 8<\/div><div class=\"pf-problem-question\">Your weight on planet X is 0.38 of your Earth weight. If you weigh 640 N on Earth, what do you weigh on X \u2014 and which real bodies could X be?<\/div><details><summary>Show Solution<\/summary><div class=\"pf-problem-solution\">\n<strong>Solution:<\/strong>\nStep 1: Multiply Earth weight by the ratio \u2014 W = 0.38 \u00d7 640 N.\nStep 2: W = 243 N.\nStep 3: Identify worlds with g \u2248 0.38 of Earth \u2014 Mercury (0.38\u00d7) and Mars (0.38\u00d7) both fit.\n<strong>Answer: 243 N; planet X could be Mercury or Mars, which share almost the same surface gravity.<\/strong>\n<\/div><\/details><\/div>\n<h2>Frequently Asked Questions<\/h2>\n<details class=\"pf-faq-item\"><summary>How much would I weigh on the Moon?<\/summary><div class=\"pf-faq-item-answer\">\nOn the Moon you would weigh about one sixth of your Earth weight, because lunar surface gravity is 1.62 m\/s\u00b2 versus Earth&#8217;s 9.81. A 60 kg person&#8217;s Earth-calibrated scale would read roughly 10 kg there, and their true weight would be about 97 N. Their actual mass, though, stays exactly 60 kg.\n<\/div><\/details>\n<details class=\"pf-faq-item\"><summary>What is the formula for weight on another planet?<\/summary><div class=\"pf-faq-item-answer\">\nThe formula is W = m \u00d7 g, where W is weight in newtons, m is mass in kilograms, and g is that planet&#8217;s surface gravity in m\/s\u00b2 (equal to N\/kg). You keep your mass the same and simply swap in the new planet&#8217;s g. For example, on Mars g = 3.72, so a 70 kg person weighs 70 \u00d7 3.72 = 260 N.\n<\/div><\/details>\n<details class=\"pf-faq-item\"><summary>Does my mass change on other planets?<\/summary><div class=\"pf-faq-item-answer\">\nNo \u2014 your mass never changes, no matter which planet you visit. Mass is the amount of matter in you, and it is the same on Earth, on the Moon, on Jupiter, and in deep space. Only your weight changes, because weight is the gravitational force acting on that fixed mass, and gravity differs from world to world.\n<\/div><\/details>\n<details class=\"pf-faq-item\"><summary>Which planet would I weigh the most on?<\/summary><div class=\"pf-faq-item-answer\">\nOf the eight planets, you would weigh the most on Jupiter, where surface gravity is about 2.53 times Earth&#8217;s. A 70 kg person would feel like roughly 177 kg at Jupiter&#8217;s cloud tops. Only the Sun beats it, at about 28 times Earth&#8217;s gravity \u2014 but neither has a solid surface you could actually stand on.\n<\/div><\/details>\n<details class=\"pf-faq-item\"><summary>Why is gravity different on each planet?<\/summary><div class=\"pf-faq-item-answer\">\nGravity differs because surface gravity depends on a planet&#8217;s mass and radius through g = G \u00d7 M \/ r\u00b2. More mass strengthens gravity, but a larger radius weakens it, and the radius counts twice because it is squared. That balance is why dense little Mercury and much larger Mars end up with almost identical surface gravity.\n<\/div><\/details>\n<details class=\"pf-faq-item\"><summary>Can you actually stand on Jupiter or Saturn to be weighed?<\/summary><div class=\"pf-faq-item-answer\">\nNo \u2014 Jupiter and Saturn are gas giants with no solid surface, so there is nowhere to place a scale. Their quoted surface gravity is measured at the 1-bar cloud level, high in the atmosphere. Descend deeper and the gravity, pressure and temperature all rise sharply, long before you would reach anything solid.\n<\/div><\/details>\n<details class=\"pf-faq-item\"><summary>How much would I weigh on Mars?<\/summary><div class=\"pf-faq-item-answer\">\nOn Mars you would weigh about 38% of your Earth weight, since Martian surface gravity is 3.72 m\/s\u00b2. A 70 kg person&#8217;s Earth scale would read roughly 26.5 kg on Mars, and their true weight would be about 260 N. This lower gravity is one reason Mars is a realistic target for future crewed missions.\n<\/div><\/details>\n<p><em>Every gravity value above is a standard planetary figure; the gas-giant and Sun values are measured at the 1-bar cloud level, as explained in the table note. If you&#8217;re revising, try the interactive lab and calculator to test your own numbers.<\/em><\/p>\n","protected":false},"excerpt":{"rendered":"<p>Your weight changes from world to world even though your mass never does. Learn the W = mg formula and see what you&#8217;d weigh on the Moon, Mars, Jupiter and beyond.<\/p>\n","protected":false},"author":1,"featured_media":629,"comment_status":"open","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[2],"tags":[],"class_list":["post-628","post","type-post","status-publish","format-standard","has-post-thumbnail","hentry","category-mechanics"],"_links":{"self":[{"href":"https:\/\/physicsfundamentalsinfo.com\/blog\/wp-json\/wp\/v2\/posts\/628","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/physicsfundamentalsinfo.com\/blog\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/physicsfundamentalsinfo.com\/blog\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/physicsfundamentalsinfo.com\/blog\/wp-json\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/physicsfundamentalsinfo.com\/blog\/wp-json\/wp\/v2\/comments?post=628"}],"version-history":[{"count":2,"href":"https:\/\/physicsfundamentalsinfo.com\/blog\/wp-json\/wp\/v2\/posts\/628\/revisions"}],"predecessor-version":[{"id":632,"href":"https:\/\/physicsfundamentalsinfo.com\/blog\/wp-json\/wp\/v2\/posts\/628\/revisions\/632"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/physicsfundamentalsinfo.com\/blog\/wp-json\/wp\/v2\/media\/629"}],"wp:attachment":[{"href":"https:\/\/physicsfundamentalsinfo.com\/blog\/wp-json\/wp\/v2\/media?parent=628"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/physicsfundamentalsinfo.com\/blog\/wp-json\/wp\/v2\/categories?post=628"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/physicsfundamentalsinfo.com\/blog\/wp-json\/wp\/v2\/tags?post=628"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}