SOLID STATE PRESS
← Back to catalog
Free Fall: Motion Under Gravity Alone cover
Coming soon
Coming soon to Amazon
This title is in our publishing queue.
Browse available titles
Physics

Free Fall: Motion Under Gravity Alone

A High School and Early College Physics Primer

Free fall is one of the first places high school physics students hit a wall. The equations look simple, but sign errors, mixed-up reference frames, and the tricky case of objects thrown upward eat exam points fast. Whether you are staring down a test next week or trying to help your student get unstuck, this guide cuts straight to what matters.

**Free Fall: Motion Under Gravity Alone** covers everything in a single, focused primer: what free fall actually means (and why a bowling ball and a feather fall the same way in a vacuum), how to set up the four kinematic equations for vertical motion, and how to work through both the simple dropped-object problems and the harder upward-launch problems that trip up even prepared students. Every section includes worked examples with full solutions, and a dedicated chapter on common pitfalls gives you a clear checklist for avoiding the mistakes that cost points.

This is a TLDR study guide — short by design. There is no filler, no chapter-long review of material you already know. If you need to understand free fall physics problems in high school or early college, get oriented fast, and walk into class or an exam with confidence, this primer does exactly that.

If you are prepping for AP Physics 1 kinematics or just need a clean foundation before tackling projectile motion, pick this up and work through it in one sitting.

What you'll learn
  • Define free fall and explain why all objects fall at the same rate when air resistance is negligible
  • Apply the kinematic equations to objects dropped, thrown downward, and thrown upward
  • Choose and stick with a sign convention for displacement, velocity, and acceleration
  • Analyze the symmetry of an object thrown straight up and returning to its launch height
  • Solve standard exam problems involving time of flight, maximum height, and impact velocity
What's inside
  1. 1. What Free Fall Actually Means
    Defines free fall, introduces g, and addresses the common confusion about heavy versus light objects falling.
  2. 2. The Kinematic Equations for Free Fall
    Adapts the four standard kinematic equations to vertical motion under gravity and explains sign conventions.
  3. 3. Objects Dropped or Thrown Downward
    Walks through the simplest free-fall problems where motion is one-directional, with worked examples for time, distance, and impact speed.
  4. 4. Objects Thrown Straight Up
    Handles the harder case of upward launches, including peak height, time symmetry, and why velocity at the top is zero but acceleration is not.
  5. 5. Common Pitfalls and Problem-Solving Strategy
    A checklist-style guide to avoiding sign errors, mismatched reference frames, and other mistakes that cost exam points.
  6. 6. Where Free Fall Shows Up Next
    Connects free fall to projectile motion, terminal velocity, and orbital mechanics so students see what their next physics chapter builds on.
Published by Solid State Press
Free Fall: Motion Under Gravity Alone cover
TLDR STUDY GUIDES

Free Fall: Motion Under Gravity Alone

A High School and Early College Physics Primer
Solid State Press

Who This Book Is For

If you are working through free fall physics problems in a high school physics course, prepping for the AP Physics 1 kinematics exam, or sitting in an introductory college mechanics class wondering why your numbers keep coming out wrong, this book is for you. It also works for parents and tutors who need a fast, reliable reference.

This guide covers one-dimensional motion under gravity — the core ideas a student needs to handle any dropped or launched object near Earth's surface. That means the kinematics gravity equations, sign conventions, objects thrown upward, and a clear strategy for how to solve free fall problems step by step. Think of it as a focused physics study guide for beginners and returning students alike. About 15 pages, no padding.

Read it straight through once — each section builds on the last. Work every example yourself before reading the solution. Then tackle the practice problems at the end to confirm your understanding holds under pressure.

Contents

  1. 1 What Free Fall Actually Means
  2. 2 The Kinematic Equations for Free Fall
  3. 3 Objects Dropped or Thrown Downward
  4. 4 Objects Thrown Straight Up
  5. 5 Common Pitfalls and Problem-Solving Strategy
  6. 6 Where Free Fall Shows Up Next
Chapter 1

What Free Fall Actually Means

Drop a bowling ball and a tennis ball from the same height. Which hits the ground first? Most people say the bowling ball — and they are wrong. Both hit at the same time, and understanding exactly why is the foundation for everything in this book.

Free fall is the motion of an object when gravity is the only force acting on it. That "only" is doing real work in the definition. In true free fall there is no air resistance, no rope tension, no rocket thrust — nothing except gravity pulling the object downward. In practice, near Earth's surface and for dense, compact objects moving at everyday speeds, air resistance is small enough that we treat it as zero. That approximation is what makes the math clean and what makes free fall a tractable topic for a first physics course.

The gravitational acceleration near Earth's surface

Gravity does not merely pull objects downward — it accelerates them downward. Gravitational acceleration, symbolized $g$, is the rate at which a freely falling object's speed increases every second. Near Earth's surface, that value is

$g = 9.8 \ \text{m/s}^2$

What does that number mean concretely? If you drop an object from rest, after one second it is moving at $9.8 \ \text{m/s}$ downward. After two seconds, $19.6 \ \text{m/s}$. After three seconds, $29.4 \ \text{m/s}$. Every second of fall adds another $9.8 \ \text{m/s}$ of downward speed. The acceleration is constant — it does not depend on how fast the object is already going, and, crucially, it does not depend on the object's mass.

You will sometimes see $g$ rounded to $10 \ \text{m/s}^2$ for quick estimates or on certain exams. Use whichever value your instructor specifies; the physics is identical.

Why heavy and light objects fall together

Keep reading

You've read the first half of Chapter 1. The complete book covers 6 chapters in roughly fifteen pages — readable in one sitting.

Coming soon to Amazon