Gravity

Forces
definition

Also known as: gravitational force, g

Grade 6-8

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The universal attractive force between any two objects with mass, decreasing with the square of distance. Governs planetary motion, ocean tides, and keeps us on Earth's surface.

Definition

The universal attractive force between any two objects with mass, decreasing with the square of distance.

💡 Intuition

Everything pulls on everything else—but only huge things (like Earth) pull noticeably.

🎯 Core Idea

Gravity acts between all masses everywhere — it never turns off, only weakens with distance.

Example

Earth pulls you down; you also pull Earth up (but it doesn't move noticeably).

Formula

F = \frac{Gm_1 m_2}{r^2} (universal gravitation)

Notation

G is the universal gravitational constant (6.674 \times 10^{-11} N m^2 kg^{-2}), m_1 and m_2 are the two masses in kilograms, and r is the centre-to-centre distance in metres.

🌟 Why It Matters

Governs planetary motion, ocean tides, and keeps us on Earth's surface.

💭 Hint When Stuck

When you see a gravity problem, identify the two masses and the distance between their centres. First, substitute m_1, m_2, and r into F = Gm_1 m_2 / r^2. Then compute the numerator and denominator separately before dividing. Finally, check your answer's units are in newtons.

Formal View

Newton's law of universal gravitation states that every point mass attracts every other point mass with a force F = \frac{Gm_1 m_2}{r^2}, directed along the line joining their centres.

Compare With Similar Concepts

🚧 Common Stuck Point

Gravity never 'turns off' in space—astronauts float because they're falling around Earth.

⚠️ Common Mistakes

  • Using the distance between surfaces instead of the distance between the centres of mass of the two objects.
  • Forgetting to square the distance r in the denominator, which drastically changes the result.
  • Confusing g (gravitational field strength, ~9.8 m/s²) with G (the universal gravitational constant, 6.67 × 10⁻¹¹ N m²/kg²).

Common Mistakes Guides

Frequently Asked Questions

What is Gravity in Physics?

The universal attractive force between any two objects with mass, decreasing with the square of distance.

What is the Gravity formula?

F = \frac{Gm_1 m_2}{r^2} (universal gravitation)

When do you use Gravity?

When you see a gravity problem, identify the two masses and the distance between their centres. First, substitute m_1, m_2, and r into F = Gm_1 m_2 / r^2. Then compute the numerator and denominator separately before dividing. Finally, check your answer's units are in newtons.

How Gravity Connects to Other Ideas

To understand gravity, you should first be comfortable with force and mass. Once you have a solid grasp of gravity, you can move on to weight, orbital motion and gravitational field.

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