Formation of the Moon

Scientists hypothesize that the moon formed after an enormous collision early in Earth's history. At that time, about 4.6 billion years ago, the solar system was full of pieces of rocky debris, some of which were the size of small planets. This debris frequently collided with the planets, creating many large craters. While Earth was still forming, a Mars-sized object probably collided with it off-center, as shown in Figure 7. This collision ejected a large amount of material into space. This material orbited Earth until it eventually came together to form the moon.

Phases of the Moon

The moon doesn't produce its own light. You can see the moon because it reflects light from the sun. When you look at the moon, it sometimes appears full and bright, and sometimes appears as only a sliver. The different shapes of the moon visible from Earth are called phases.

The moon's phases are caused by changes in the relative positions of the moon, sun, and Earth as the moon revolves around Earth. Sunlight illuminates half of the moon. The phase of the moon depends on how much of the sunlit portion of the moon is facing Earth.

If you were to track the appearance of the moon from day to day, you would notice that the moon's phases change according to a regular cycle. Figure 8 shows the positions of the moon during its phases. A full moon occurs when the moon is on the opposite side of Earth from the sun, and the whole side of the moon facing Earth is lit by the sun. A new moon occurs when the moon is directly between the sun and Earth. A new moon cannot be seen from Earth because the sunlit side of the moon is facing away from us.

It takes about 29.5 days for the moon to complete a full cycle of phases from full moon to new moon and back again. This period of time is known as a lunar month.

Figure 7 The moon is thought to have formed in a spectacular collision between the early Earth and a Mars-sized object. A The collision knocked part of Earth's mantle into space. B Much of the ejected material began to revolve around Earth. It soon began to clump together to form the moon. C Earth and the moon today.

A diagram illustrating how the moon was formed as hypothesized by scientist. Diagram depicting the possible formation of the Moon by (A) a collision of a Mars-sized object with Earth knocking part of its mantle into space, (B) ejected material revolving around Earth and clumping together to form moon and (C) the Earth and Moon today.

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Table of Contents

Physical Science CHAPTER 1 Science Skills CHAPTER 2 Properties of Matter CHAPTER 3 States of Matter CHAPTER 4 Atomic Structure CHAPTER 5 The Periodic Table CHAPTER 6 Chemical Bonds CHAPTER 7 Chemical Reactions CHAPTER 8 Solutions, Acids, and Bases CHAPTER 9 Carbon Chemistry CHAPTER 10 Nuclear Chemistry CHAPTER 11 Motion CHAPTER 12 Forces and Motion CHAPTER 13 Forces in Fluids CHAPTER 14 Work, Power, and Machines CHAPTER 15 Energy CHAPTER 16 Thermal Energy and Heat CHAPTER 17 Mechanical Waves and Sound CHAPTER 18 The Electromagnetic Spectrum and Light CHAPTER 19 Optics CHAPTER 20 Electricity CHAPTER 21 Magnetism CHAPTER 22 Earth's Interior CHAPTER 23 Earth's Surface CHAPTER 24 Weather and Climate CHAPTER 25 The Solar System CHAPTER 26 Exploring the Universe Skills and Reference Handbook