Physical Science 8 mascot: a cartoon scientist heating a sample over a Bunsen burner Mr. LaMarr’s Physical Science ClassroomPlacerita Junior High - Grade 8

Table of Contents

Unit 1: Energy of Motion
Unit 2: Gravity & Energy Related to Position
Unit 3: Electricity & Magnetism
Unit 4: Waves Transmitting Energy & Information
Unit 5: Thermal Energy & Heat Flow
Unit 6: Chemical Energy & Reactions
Unit 2, Chapter 8 · Gravity & Energy Related to Position

Universal Law of Gravity

NGSS standards: MS-PS2-4MS-PS2-5MS-ESS1-2

Chapter infographic, Universal Law of Gravity. Every pair of masses in the universe attracts each other with a gravitational force. The poster works through the idea in labelled photo panels and ends with a list of key takeaways.
the poster to open it full size.

A Pull With No Strings Attached

Gravity is strange when you really think about it. It's a force, which means it can push or pull objects, yet it never needs to touch anything to do its job. The Moon orbits Earth without any rope connecting them, and you're pulled toward the ground without anything physically grabbing you. Scientists describe this by saying gravity acts at a distance, and it always pulls objects together. Gravity never pushes things apart; it only attracts.

Here's another key rule: gravity requires at least two objects. It doesn't make sense to talk about the gravity of a single object all by itself in empty space with nothing else around. Gravity is always a relationship between two masses pulling on each other, even if one of them, like Earth, is doing almost all of the noticeable pulling.

More Mass, More Force. More Distance, Less Force.

Even though gravity is a universal force acting between literally any two objects with mass, it doesn't pull on everything with equal strength. Two things change how strong the force of gravity is between objects. The first is mass: the more mass two objects have, the stronger the gravitational force pulling them together. That's why Earth's gravity noticeably affects you, but your gravity and your friend's gravity pulling on each other is far too tiny to ever feel.

The second factor is distance. The farther apart two objects are, the weaker the gravitational force between them becomes. Move two objects twice as far apart, and the force drops off fast. This means gravity has an inverse relationship with distance: as distance goes up, force goes down. Put mass and distance together, and you can explain why planets, stars, and moons produce gravity strong enough to notice, while two backpacks sitting next to each other on a desk don't visibly attract each other at all.

This distance effect is actually stronger than a simple inverse relationship: it's what scientists call an inverse-square relationship. That means if you double the distance between two objects, the gravitational force between them doesn't just cut in half, it drops all the way to one-fourth of its original strength. Triple the distance, and the force falls to just one-ninth. This is exactly why a satellite orbiting close to Earth feels a much stronger gravitational pull than a satellite far out near the Moon's orbit, even though Earth's mass hasn't changed at all, only the distance has.

Same Acceleration, Different Force

Here's a detail that confuses a lot of people: near Earth's surface, gravity accelerates every object at the same rate, about 9.8 meters per second every second, regardless of mass. Drop a bowling ball and a marble at the same instant in a vacuum, and they hit the ground at the same time. That seems to contradict the idea that mass matters, but it doesn't. The force of gravity pulling on the bowling ball actually is bigger than the force pulling on the marble, but the bowling ball also has more mass to move, and those two effects cancel out perfectly, leaving the same acceleration for both.

Three panels of a basketball dropping from a cliff: it starts to fall, a downward arrow labeled gravity pulls on it, and it streaks toward the ground moving faster.
Figure 8.1. Gravity pulls downward the whole way, so the ball keeps speeding up as it falls. Ignoring air resistance, it gains about 9.8 m/s of speed every second, and so would a marble dropped beside it.

Outside of a vacuum, though, things look different. Drop a feather and a bowling ball in a regular room, and the bowling ball wins easily. That's not because gravity treats them differently, it's because of air resistance and surface area. A feather has a large surface area for its tiny mass, so air pushes back against it much more, slowing its fall dramatically. A tightly balled-up piece of paper falls faster than a flat sheet of the same paper for exactly this reason.

Think of it this way: gravity pulls twice as hard on an object with twice the mass, but that object also takes twice as much force to speed it up at all, since more massive objects resist changes in motion more strongly. Those two doublings cancel each other out perfectly, which is why a bowling ball and a marble, dropped together with no air in the way, hit the ground at the exact same moment despite the very different forces gravity exerts on each of them.

Fields and Force Diagrams

So how does gravity reach across empty space without touching anything? Scientists explain this using the idea of a field, an invisible region of influence that surrounds any object with mass. Earth's gravitational field fills the space around our planet, and any object that enters that field feels a pull toward Earth's center, even though nothing is physically connecting them. Electric charges and magnets create their own kinds of fields too, which is why magnets can attract metal from across a table without touching it.

Scientists and engineers often draw force diagrams to show these invisible pulls visually. An arrow represents a force, pointing in the direction the force acts, with a longer arrow meaning a stronger force. If you drew a force diagram of Earth pulling on the Moon compared to Earth pulling on a satellite much closer by, the arrow toward the closer satellite would generally need to reflect the different distances and masses involved.

Mass vs. Weight: Why You'd Weigh Less on the Moon

Here's a mix-up almost everyone makes at some point: confusing mass and weight. Mass measures how much matter is packed into an object, and it never changes no matter where that object travels in the universe. Weight, on the other hand, is actually a measurement of the force of gravity pulling on that mass, and it absolutely can change depending on location. A 10-kilogram object always has 10 kilograms of mass, whether it's sitting in your living room or floating near Jupiter. But that same object would weigh about 98 Newtons on Earth (10 kilograms x 9.8 m/s2), while on the Moon, where gravity is only about one-sixth as strong, it would weigh only around 16 Newtons.

Bar graph of weight in newtons for the same object on four worlds: Moon 162 N, Earth 980 N, Mars 371 N, and Jupiter 2,350 N.
Figure 8.2. One object, four worlds. The bars are for a 100 kg object, ten times the example above: its mass never changes, but its weight rises and falls with the strength of each world's gravity.

This is exactly why astronauts can bound across the lunar surface in giant leaps despite wearing bulky spacesuits: their mass hasn't changed one bit, but the Moon's much smaller mass produces much weaker gravity, and therefore much less weight pulling them down. If you ever see a scale reading in kilograms, it's technically reporting mass, since a truly precise weight reading would be given in Newtons and would change dramatically depending on which planet, or moon, you happened to be standing on.

Why Astronauts Float (It Isn't Because Gravity Quit)

Almost everyone has seen astronauts drifting around inside a spacecraft, and almost everyone draws the same conclusion: there must be no gravity up there. It is probably the single most common misconception in this whole unit, and it is wrong. A space shuttle orbits only a few hundred kilometers up, and at that height Earth's gravitational pull on it is still nearly 90 percent as strong as it is at the surface. Gravity is very much on duty.

To see what is really happening, think about how a scale measures your weight. You stand on it, gravity pulls you down onto it, and by Newton's third law the scale pushes back up on you with an equal force. That upward push from the scale is what the pointer actually reports, and it is what your body feels as the sensation of weight.

Now picture standing on that same scale inside an elevator whose cable has snapped. The elevator, the scale, and you are all in free fall, meaning gravity is the only force acting on any of you. You are all accelerating downward together at exactly the same rate, so the scale is no longer pressing up into your feet, and you are no longer pressing down on it. The pointer reads zero. Gravity never stopped pulling on you for even an instant, but with nothing pushing back, you would feel completely weightless. That is what weightlessness really means: not the absence of gravity, but the absence of anything pushing back.

An orbiting spacecraft is in exactly that situation, just going sideways very fast at the same time. The shuttle, the astronauts, and every floating orange in the cabin are all in free fall together, falling around Earth on a curved path instead of straight down. Because they all fall at the same rate, nothing moves relative to anything else inside the cabin, and everything appears to hover. Astronauts are not escaping gravity. They are falling, endlessly, and missing the planet.

Real-World Connections

Gravity-Assist Space Missions

NASA has sent spacecraft like Voyager 1 on flybys of massive planets like Jupiter specifically to use the planet's gravity to slingshot the spacecraft to higher speeds, saving enormous amounts of fuel.

Why the Moon Doesn't Fall on Us

The Moon is constantly falling toward Earth due to gravity, but it's also moving sideways fast enough that it keeps missing, resulting in the orbit we see every night.

How they tie togetherBoth examples depend on the same rule: every object with mass pulls on every other object with mass, and that pull gets weaker with distance: mission planners and the Moon's orbit both follow this one universal law.

Meet the Scientist

Illustration of an orbital mechanics engineer at a desk sketching orbits while studying a spacecraft's path from Earth to the Moon on a monitor, with a satellite model nearby.

Orbital Mechanics Engineers (Astrodynamicists)

These specialists calculate the exact paths spacecraft need to follow by accounting for the gravitational pull of the Sun, Earth, Moon, and other planets. A tiny miscalculation in these gravity equations could send a multi-million-dollar spacecraft missing its target by thousands of miles.

Average salary in Southern California
About $158,000 a yearBased on pay for aerospace engineers in the L.A., Orange County, Inland Empire, San Diego, and Ventura areas (U.S. Bureau of Labor Statistics, May 2025).

Key Vocabulary

Bold, underlined words in the reading above are clickable too: tap one to see its definition pop out. Or click or tap a card below to reveal the definition.

Universal Law of Gravitationtap to flip
The rule that any two objects with mass attract each other, with the force depending on their masses and the distance between them.
Fieldtap to flip
An invisible region of space around an object where its force, like gravity, magnetism, or electric charge, can affect other objects without touching them.
Inverse Relationshiptap to flip
A pattern where one quantity goes down as another goes up, such as gravitational force decreasing as distance increases.
Acceleration Due to Gravitytap to flip
The rate at which gravity speeds up a falling object, about 9.8 meters per second squared near Earth's surface, the same for all masses in a vacuum.
Air Resistancetap to flip
A force caused by air pushing back against a moving object, which can slow falling objects depending on their shape and surface area.
Force Diagramtap to flip
A drawing that uses arrows to show the direction and relative strength of forces acting on an object.
Attractive Forcetap to flip
A force that pulls objects toward each other rather than pushing them apart; gravity is always attractive.
Free Falltap to flip
Motion in which gravity is the only force acting on an object.
Weightlessnesstap to flip
The condition in free fall where an object's weight seems to be zero, even though gravity is still acting on it.
Masstap to flip
The amount of matter in an object, one of the two factors that determines the strength of gravitational force between two objects.

Explore More

Read

Newton's Theory of Universal Gravitation

NASA
Open article →
Try the simulation

Gravity Force Lab

PhET Interactive Simulations
Launch simulation →

Defining Gravity: Crash Course Kids #4.1

Crash Course Kids on YouTube
Watch on YouTube →

Introduction to Newton's Law of Gravitation

Khan Academy on YouTube
Watch on YouTube →

Mass and Weight Clarification

Khan Academy on YouTube
Watch on YouTube →

Chapter Review

1. Which statement correctly describes gravity between any two objects in the universe?

2. Planet X and Planet Y have identical masses, but Planet Y is twice as far from a nearby star as Planet X. How does the star's gravitational pull on each planet compare?

3. A hammer and a feather are dropped at the same time on the surface of the Moon, where there is no air. What happens?

4. Why don't two students sitting next to each other in class notice any gravitational pull between them?

5. A crumpled piece of paper and a flat sheet of the exact same paper are dropped from the same height in a normal room. What is the best explanation for why the crumpled paper lands first?

Design the Experiment

California Science Test (CAST) Practice

CAST-Style Practice Item

A science team measures the relative strength of gravitational attraction between a space probe and a planet at several different distances from the planet's center. Their measurements are shown in the table below, using a relative force scale where the closest distance is set to 100.

Distance (relative units)Relative Gravitational Force
1100
225
311
46

Which claim is best supported by the data in the table?

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