Top Banner
The Inner Planets Ch 11.2 (p382-387)
21

Chapter 11.2: The Inner Planets

May 10, 2015

Download

Education

Grade 8 Integrated Science Chapter 11 Lesson 2 on the inner planets. Discusses the four inner planets, their atmosphere, interior, surface, weather, and other defining features. Includes individual slides on Mercury, Venus, Earth and Mars.
Welcome message from author
This document is posted to help you gain knowledge. Please leave a comment to let me know what you think about it! Share it to your friends and learn new things together.
Transcript
Page 1: Chapter 11.2: The Inner Planets

The Inner Planets

Ch 11.2 (p382-387)

Page 2: Chapter 11.2: The Inner Planets

Planets Made of Rock

• The inner planets – Mercury, Venus, Earth, Mars – are also called terrestrial planets.

• Terrestrial planets are the planets closet to the Sun, are made of rock and metal, and have solid outer layers.

Page 3: Chapter 11.2: The Inner Planets
Page 4: Chapter 11.2: The Inner Planets

Mercury

• The smallest planet• Closest to the Sun• No atmosphere

– The strength of a planet’s gravity depends on the planet’s mass. Because Mercury’s mass is so small, its gravity is not strong enough to hold onto an atmosphere

• No atmosphere = no wind– Temperatures:

• -170C on the side facing away from the Sun

• 450 C on the side facing the Sun

Page 5: Chapter 11.2: The Inner Planets

Mercury’s Surface

• Impact craters, depressions formed by collisions with objects from space, cover the surface of Mercury.

• There are smooth plains of solidified lava from long-ago eruptions.

• There are also high cliffs that might have formed when the planet cooled quickly

• Without an atmosphere, almost no erosion occurs on Mercury’s surface– As a result, features that formed billions of years ago have

changed very little.

Page 6: Chapter 11.2: The Inner Planets

Mercury’s Surface

• Like all inner planets, Mercury has a core made of iron and nickel.

• Surrounding the core is a layer called the mantle.

• The mantle is mainly made of silicon and oxygen.

• The crust is a thin, rocky layer above the mantle.• Mercury’s large core might have been formed by

a collision with a large object during Mercury’s formation.

Page 7: Chapter 11.2: The Inner Planets
Page 8: Chapter 11.2: The Inner Planets

Venus

• 2nd planet from the Sun

• About the same size as Earth

• It rotates so slowly that its period of rotation is longer than its period of revolution.– One day is longer than one year

• Venus rotates east to west, unlike most planets

Page 9: Chapter 11.2: The Inner Planets

Venus’s Atmosphere

• The atmosphere of Venus is about 97% carbon dioxide

• It is so dense that the atmospheric pressure on Venus is about 90 times greater than on Earth

• Venus has no water on its surface.

• It is covered by a thick layer of clouds made of acid

Page 10: Chapter 11.2: The Inner Planets

The Greenhouse Effect on Venus

• With an average temperature of about 460C, Venus is the hottest planet in our solar system.

• The high temperature are caused by the greenhouse effect– The greenhouse effect occurs when a planet’s

atmosphere traps solar energy and causes the surface temperature to increase.

• Without the greenhouse effect Venus would be about 450C cooler.

Page 11: Chapter 11.2: The Inner Planets

Venus’s Structure and Surface

• Venus’s internal structure is similar to Earth’s.

• Radar images show that more than 80% of Venus’s surface is covered by solidified lava

Page 12: Chapter 11.2: The Inner Planets
Page 13: Chapter 11.2: The Inner Planets

Concept Check

• How are the inner planets similar?

• Why is Venus hotter than Mercury?

Page 14: Chapter 11.2: The Inner Planets

Earth

• The third planet from the Sun

• Unlike Mercury and Venus, Earth has a moon.

Page 15: Chapter 11.2: The Inner Planets

Earth’s Atmosphere

• A mixture of gases and a small amount of water vapor make up most of Earth’s atmosphere

• They produce a greenhouse effect that increases Earth’s average surface temperature

• This effect and Earth’s distance from the Sun warm Earth enough for large bodies of water to exist.

• Earth’s protective atmosphere, the presence of liquid water, and the planet’s moderate temperature range support a variety of life

Page 16: Chapter 11.2: The Inner Planets

Earth’s Structure

• Earth has a solid inner core surrounded by a liquid outer core

• The mantle surrounds the liquid outer core.

• Above the mantle is Earth’s crust.

• It’s broken into large pieces, called plates, that constantly slide past, away from, or into each other

Page 17: Chapter 11.2: The Inner Planets
Page 18: Chapter 11.2: The Inner Planets

Mars

• 4th planet from the Sun• Half the size of Earth• Two very small and irregularly shaped

moons• Water on Mars is mainly trapped in the

polar ice caps and a small amount in found as liquid vapor

• However, little evidence of liquid water or life has been found

Page 19: Chapter 11.2: The Inner Planets

Mar’s Atmosphere

• 95% carbon dioxide

• Temperatures: -125C – 20C

• Dust storms that last for months

Page 20: Chapter 11.2: The Inner Planets

Mar’s Surface

• Reddish due to iron oxide in the soil (rust)

• Enormous canyons

• Largest mountain in the solar system

• Polar ice caps made of frozen carbon dioxide and ice

Page 21: Chapter 11.2: The Inner Planets