Figure 10 The seasons are caused by the tilt of Earth's axis as it revolves around the sun. Interpreting Visuals When is the south end of Earth's axis tilted most toward the sun?

A diagram illustrating how the seasons depend on the tilt of the Earth's axis as it revolves around the sun. dd

The seasons are not affected by Earth's changing distance from the sun. In fact, in the Northern Hemisphere, Earth is closer to the sun during winter than it is during summer.

Equinoxes

Look at Figure 10. Notice that halfway between the solstices are two days, called equinoxes. The equinoxes mark the beginning of spring and autumn. At an equinox, neither hemisphere is tilted toward the sun, and the lengths of daylight and of darkness are approximately equal. The vernal equinox, which occurs about March 21 in the Northern Hemisphere, marks the start of spring. The autumnal equinox, which occurs about September 22 in the Northern Hemisphere, marks the start of autumn. On these two days, the noon sun is directly overhead at the equator. Sunlight reaches the Northern Hemisphere and Southern Hemisphere in equal amounts on the equinoxes.


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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