M8SCI-3.1

Gravity: Mass, Distance & Weight

Learn how gravity works: why it always attracts, how mass and distance affect gravitational force, and why your weight changes on the Moon but your mass never does.

What you'll do in this lesson

A voice-first session with the Crimsora tutor on Gravity: Mass, Distance & Weight, then targeted practice and FRQs — with the tutor adapting to where you get stuck.

What this lesson covers

Gravity is everywhere — it holds planets in orbit, keeps you on the ground, and shapes the entire universe. But what exactly is gravity? And why does a heavier object feel heavier on Earth than it would on the Moon, even though it contains the same amount of matter? In this lesson, you'll build a solid understanding of how gravity works by examining the relationship between mass, distance, and gravitational force. You'll learn to argue from evidence that gravity always pulls objects together, grows stronger when objects are more massive, and weakens as objects move farther apart. Most importantly, you'll discover why mass and weight are not the same thing — and why an astronaut would weigh far less on the Moon despite containing exactly the same amount of matter.

What Is Gravity?

Gravity is a fundamental force of nature that pulls all objects with mass toward each other. Unlike electric or magnetic forces, gravity is always attractive — it never pushes. Every object in the universe, from a grain of sand to a star, exerts a gravitational pull on every other object. In most everyday situations, this pull is incredibly weak. You don't notice the gravitational attraction between two apples sitting on a table, for instance. But when one object is enormous — like Earth — the gravitational pull becomes strong enough to noticeably affect other objects around it. Earth's gravity pulls you toward the ground and keeps the Moon orbiting around us. The strength of gravity depends on two main factors: how much mass the objects contain and how far apart they are. This predictable relationship allows scientists to calculate gravitational force and predict the motion of planets, moons, and satellites.

Mass, Distance, and Gravitational Force

Gravitational force follows a clear pattern. First, gravity grows stronger as the masses of the objects increase. If you double the mass of one object, the gravitational force between them doubles. If you double both masses, the force increases by a factor of four. This makes sense: more matter means a stronger pull. Second, gravity weakens as objects move farther apart. Specifically, if you double the distance between two objects, the gravitational force becomes one-quarter as strong. If you triple the distance, the force becomes one-ninth as strong. Scientists describe this as an inverse-square relationship: the force is inversely proportional to the square of the distance. The equation is Fg=Gm1m2d2F_g = G\frac{m_1 m_2}{d^2}, where FgF_g is gravitational force, m1m_1 and m2m_2 are the masses, dd is the distance between them, and GG is a constant. You don't need to memorize this equation, but understanding the pattern helps explain why distant planets have almost no effect on you, while Earth's gravity affects you constantly.

Mass versus Weight

A critical distinction exists between mass and weight — and many students confuse them. Mass is the amount of matter in an object. It is measured in kilograms or grams and is constant everywhere: your mass on Earth is identical to your mass on the Moon, on Mars, or floating in space. Your mass never changes (unless you add or remove matter from your body). Weight, by contrast, is the gravitational force acting on your mass. It is measured in newtons (a unit of force) and depends on the strength of gravity where you are located. On Earth, you weigh about 9.8 newtons for every kilogram of mass you have. On the Moon, where gravity is about one-sixth as strong as on Earth, you would weigh only about 1.6 newtons per kilogram. The equation is W=mgW = mg, where WW is weight (in newtons), mm is mass (in kilograms), and gg is the gravitational acceleration (which is different on different planets and moons). An astronaut with a mass of 80 kilograms weighs 784 newtons on Earth (80×9.8=78480 \times 9.8 = 784) but only about 131 newtons on the Moon (80×1.612880 \times 1.6 \approx 128). The astronaut's mass never changed — only the gravitational pull changed. This is why astronauts can jump much higher on the Moon: they weigh less, but their mass (and inertia) remains the same.

Gravity at Different Scales

Gravity operates at every scale, from everyday objects to cosmic systems. At human scales, gravity is typically very weak. Two bowling balls sitting side by side exert gravitational attraction on each other, but the force is so tiny — far less than a millionth of a newton — that we cannot measure it without specialized equipment. We only notice gravity when one object is extremely massive, like a planet. Earth is so massive that it exerts a significant gravitational pull on everything near it. At astronomical scales, gravity becomes the dominant force shaping the universe. The Sun's gravity holds planets in orbit. Each planet's gravity holds its moons. Gravity keeps galaxies bound together and, on the largest scales, influences the expansion and structure of the entire universe. Understanding how gravity depends on mass and distance explains all of these phenomena with a single principle: the gravitational force between any two objects follows the same relationship. It is always attractive, always grows with greater mass, and always weakens with greater distance — whether you're examining objects in a laboratory or galaxies billions of light-years apart.

Key terms

Gravity.
A fundamental force of nature that always attracts all objects with mass toward each other.
Mass.
The amount of matter in an object, measured in kilograms; stays the same everywhere (on Earth, the Moon, in space, etc.).
Weight.
The gravitational force exerted on an object's mass; measured in newtons and changes depending on the strength of local gravity.
Gravitational force.
The attractive force between two objects due to their masses; stronger with greater mass and weaker with greater distance.
Inverse-square relationship.
A relationship where a quantity decreases with the square of the distance (doubling distance reduces force to one-fourth).
Gravitational acceleration.
The rate at which gravity accelerates an object at a particular location; on Earth, approximately 9.8 meters per second squared.

Worked example

An astronaut has a mass of 60 kilograms. On Earth, gravitational acceleration is about 9.8 meters per second squared. On Mars, gravitational acceleration is about 3.7 meters per second squared. (a) Calculate the astronaut's weight on Earth. (b) Calculate the astronaut's weight on Mars. (c) Explain why the astronaut's mass does not change between Earth and Mars.
(a) To find weight, use the equation W=mgW = mg. On Earth: W=60 kg×9.8 m/s2=588 newtonsW = 60 \text{ kg} \times 9.8 \text{ m/s}^2 = 588 \text{ newtons}. (b) On Mars, use the same equation with Mars's gravitational acceleration: W=60 kg×3.7 m/s2=222 newtonsW = 60 \text{ kg} \times 3.7 \text{ m/s}^2 = 222 \text{ newtons}. (c) Mass is the amount of matter in an object, and the amount of matter does not depend on location. No matter where the astronaut travels, their body contains the same number of atoms and molecules. The gravitational acceleration is weaker on Mars than on Earth, so the gravitational force (weight) is less, but the astronaut's mass stays exactly 60 kilograms on both planets. This illustrates the key distinction: mass is intrinsic to the object, while weight is the result of gravity acting on that mass.

Practice questions

A student places two magnets on a table and measures the force between them. She then separates the magnets to twice the original distance. How does the force between the magnets change?
  1. It becomes one-quarter as strong (inverse-square relationship).
  2. It becomes one-half as strong.
  3. It stays the same.
  4. It becomes twice as strong.

Answer: It becomes one-quarter as strong (inverse-square relationship).

This question tests understanding of the inverse-square relationship, a pattern that applies to both gravity and electric forces. When distance doubles, the force is divided by the square of 2 (which is 4), so the force becomes one-quarter as strong. Note: this question uses magnets as an example to show that the inverse-square relationship applies broadly to forces that act without contact — a preview of the neighboring lessons on electric and magnetic forces.
A planet has twice the mass of Earth. Based on the relationship between mass and gravitational force, how would the gravitational force between this planet and the Sun compare to Earth's gravitational force with the Sun?

Answer: The gravitational force would be twice as strong.

Gravitational force is directly proportional to the product of the two masses. If one mass doubles while the other stays the same, the force doubles. Since Fg=Gm1m2d2F_g = G\frac{m_1 m_2}{d^2}, and the Sun's mass (m1m_1) and distance (dd) remain constant, doubling the planet's mass (m2m_2) doubles the entire force. This shows why more massive objects exert stronger gravitational attraction.
An astronaut on the Moon picks up a rock with a mass of 2 kilograms. She notes that the rock is hard to move quickly, even though it weighs very little. Explain why the rock is hard to move quickly despite its small weight.

Answer: The rock's mass is 2 kilograms everywhere, including on the Moon. Mass determines inertia — resistance to a change in motion. Even though gravity on the Moon is weak (so weight is small), the rock still has 2 kilograms of matter that must be accelerated. A large force is still needed to change the rock's motion quickly. Weight affects how hard it is to lift something against gravity, but mass affects how hard it is to accelerate something in any direction.

This question probes a common misconception: that low weight means an object is easy to move. Students often confuse weight with inertia. Weight is only the gravitational force, which matters when lifting. Inertia, determined by mass, matters for any acceleration — whether lifting, pushing sideways, or throwing. On the Moon, the rock weighs less because gravity is weaker, but its mass never changed, so the effort to change its motion is just as great.

FAQ

If gravity is always between all objects, why don't I feel attracted to my desk?
You and your desk do attract each other gravitationally, but the force is incredibly tiny — far too small to feel or measure without specialized equipment. Gravity is only strong when at least one object is extremely massive, like Earth itself. Earth's gravity on you is strong enough to feel because Earth is enormous. Your desk's gravity on you is trillions of times weaker and is completely overpowered by Earth's pull and other forces around you.
Why do objects fall straight down instead of moving sideways toward the Sun?
Objects do experience gravitational attraction toward the Sun, but Earth's gravity is much, much stronger because Earth is so much closer. The gravitational force decreases with the square of distance: the Sun is about 150 million kilometers away, while Earth's surface is only about 6,400 kilometers from Earth's center. At that distance difference, Earth's gravitational effect dominates completely, even though the Sun is much more massive. Objects fall toward Earth because Earth's gravity overpowers the Sun's.
Does gravity get weaker in the upper atmosphere or on tall mountains?
Yes, gravity does get slightly weaker at higher altitudes. Since gravitational force depends on distance, objects farther from Earth's center experience a weaker pull. However, the change is small over the heights we normally experience. At the top of a very tall mountain (about 9 kilometers up), gravity is only about 0.3 percent weaker than at sea level. Astronauts orbiting Earth at hundreds of kilometers altitude experience significantly less gravity, which is why they float in spacecraft.
If weight changes on different planets, why do scientists measure things in mass instead of weight?
Mass is constant everywhere, so it's a reliable, universal measure of how much matter something contains. Weight changes depending on local gravity, making it location-dependent and harder to compare. Scientists use mass because it tells you something fundamental about the object itself — the amount of matter — regardless of where you are. For practical purposes (like finding how much food to buy), mass works everywhere the same way.

Learn this with a teacher, not a page

The Crimsora tutor teaches Gravity: Mass, Distance & Weight live — explaining on a whiteboard, asking you questions, and adapting to where you get stuck.