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Lesson 6: Moons & Natural Satellites

12 Jan 2026 The Solar System
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Lesson Overview

This lesson explores moons, also known as natural satellites, which orbit planets and dwarf planets throughout the Solar System. Learners will discover the diversity of moons, how they form, and why some moons are among the most promising places to search for life beyond Earth.


Lesson Content

What Are Moons (Natural Satellites)?

Moons are natural objects that orbit planets or dwarf planets due to gravity. Unlike artificial satellites built by humans, natural satellites formed naturally during the early history of the Solar System.

The Solar System contains hundreds of known moons, ranging from small, irregularly shaped rocks to large worlds bigger than the planet Mercury. Each moon’s characteristics depend on how and where it formed.


How Moons Form

Scientists believe moons form in several different ways:

  • Co-formation – forming from the same disk of material as the planet

  • Capture – a planet’s gravity captures a passing object

  • Impact formation – debris from a collision forms a moon

Earth’s Moon is thought to have formed after a massive impact early in Earth’s history, while many small moons of outer planets were likely captured objects.


Diversity of Moons in the Solar System

Moons vary widely in size, composition, and activity:

  • Rocky moons – such as Earth’s Moon

  • Icy moons – such as Europa and Enceladus

  • Volcanically active moons – such as Io

  • Atmosphere-bearing moons – such as Titan

Some moons have smooth icy surfaces, while others are heavily cratered or geologically active.


Earth’s Moon

Earth has a single, large moon that plays a crucial role in stabilising Earth’s axial tilt. This stability helps maintain relatively consistent seasons over long periods.

The Moon also causes tides on Earth through gravitational interaction and has strongly influenced Earth’s geological and biological history.


Moons of the Outer Planets

The outer planets possess extensive moon systems:

  • Jupiter has dozens of moons, including the four large Galilean moons

  • Saturn hosts many icy moons, including Enceladus

  • Uranus and Neptune have moons with unusual orbits and compositions

Many of these moons are worlds in their own right, with complex geology and internal structures.


Moons and the Search for Life

Some moons are considered prime candidates in the search for extraterrestrial life:

  • Europa (Jupiter) – likely has a global subsurface ocean

  • Enceladus (Saturn) – ejects water-rich plumes into space

  • Titan (Saturn) – has lakes of liquid hydrocarbons and complex chemistry

These moons contain water, energy sources, and chemical building blocks, making them scientifically significant.


Why Moons Matter

Studying moons helps scientists:

  • Understand planetary formation

  • Learn how gravity shapes systems

  • Identify environments where life might exist

  • Compare Earth’s Moon with other natural satellites

Moons also help scientists understand the long-term evolution of planetary systems, including those around other stars.


Key Terms Introduced

  • Natural satellite

  • Gravity

  • Tides

  • Subsurface ocean

  • Capture

  • Impact formation

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