Chapter: The Solar System Table of Contents Section 3: The Outer PlanetsThe Outer Planets Section 1:...

106

Transcript of Chapter: The Solar System Table of Contents Section 3: The Outer PlanetsThe Outer Planets Section 1:...

Page 1: Chapter: The Solar System Table of Contents Section 3: The Outer PlanetsThe Outer Planets Section 1: The Solar System Section 2: The Inner PlanetsThe.
Page 2: Chapter: The Solar System Table of Contents Section 3: The Outer PlanetsThe Outer Planets Section 1: The Solar System Section 2: The Inner PlanetsThe.

Chapter: The Solar System

Table of ContentsTable of Contents

Section 3: The Outer Planets

Section 1: The Solar System

Section 2: The Inner Planets

Section 4: Other Objects in the Solar System

Page 3: Chapter: The Solar System Table of Contents Section 3: The Outer PlanetsThe Outer Planets Section 1: The Solar System Section 2: The Inner PlanetsThe.

Ideas About the Solar System—Earth-Centered Model

• Many early Greek scientists thought the planets, the sun, and the moon were fixed in separate spheres that rotated around Earth.

11The Solar SystemThe Solar System

Page 4: Chapter: The Solar System Table of Contents Section 3: The Outer PlanetsThe Outer Planets Section 1: The Solar System Section 2: The Inner PlanetsThe.

• The stars were thought to be in another sphere that also rotated around Earth.

11The Solar SystemThe Solar System

• This is called the Earth-centered model of the solar system.

Ideas About the Solar SystemIdeas About the Solar System—Earth-Centered Model

Page 5: Chapter: The Solar System Table of Contents Section 3: The Outer PlanetsThe Outer Planets Section 1: The Solar System Section 2: The Inner PlanetsThe.

Sun-Centered Model

• In 1543, Nicholas Copernicus stated that the moon revolved around Earth and that Earth and the other planets revolved around the Sun.

11The Solar SystemThe Solar System

Page 6: Chapter: The Solar System Table of Contents Section 3: The Outer PlanetsThe Outer Planets Section 1: The Solar System Section 2: The Inner PlanetsThe.

Sun-Centered Model

• He also stated that the daily movement of the planets and the stars was caused by Earth's rotation.

11The Solar SystemThe Solar System

• This is the Sun-centered model of the solar system.

Page 7: Chapter: The Solar System Table of Contents Section 3: The Outer PlanetsThe Outer Planets Section 1: The Solar System Section 2: The Inner PlanetsThe.

Sun-Centered Model

• Using his telescope, Galileo Galilei observed that Venus went through a full cycle of phases like the Moon's.

11The Solar SystemThe Solar System

• He also observed that the apparent diameter of Venus was smallest when the phase was near full.

Page 8: Chapter: The Solar System Table of Contents Section 3: The Outer PlanetsThe Outer Planets Section 1: The Solar System Section 2: The Inner PlanetsThe.

Sun-Centered Model

• This only could be explained if Venus were orbiting the Sun.

11The Solar SystemThe Solar System

• Galileo concluded that the Sun is the center of the solar system.

Page 9: Chapter: The Solar System Table of Contents Section 3: The Outer PlanetsThe Outer Planets Section 1: The Solar System Section 2: The Inner PlanetsThe.

Modern View of the Solar System

• We now know that the solar system is made up of nine planets, including Earth, and many smaller objects that orbit the Sun.

11The Solar SystemThe Solar System

• The Sun's gravity holds the planets and other objects in the solar system in their orbits.

Page 10: Chapter: The Solar System Table of Contents Section 3: The Outer PlanetsThe Outer Planets Section 1: The Solar System Section 2: The Inner PlanetsThe.

Modern View of the Solar System11The Solar SystemThe Solar System

Page 11: Chapter: The Solar System Table of Contents Section 3: The Outer PlanetsThe Outer Planets Section 1: The Solar System Section 2: The Inner PlanetsThe.

How the Solar System Formed11The Solar SystemThe Solar System

• Scientists hypothesize that the solar system formed from part of a nebula of gas, ice, and dust.

• A nearby star might have exploded or nearby O- or B-type stars formed, and the shock waves produced by these events could have caused the cloud to start contracting.

Page 12: Chapter: The Solar System Table of Contents Section 3: The Outer PlanetsThe Outer Planets Section 1: The Solar System Section 2: The Inner PlanetsThe.

How the Solar System Formed11The Solar SystemThe Solar System

• The density in the cloud fragments became greater, and the attraction of gravity pulled more gas and dust toward several centers of contraction.

• As the cloud fragments continued to contract, they began to rotate faster and faster.

Page 13: Chapter: The Solar System Table of Contents Section 3: The Outer PlanetsThe Outer Planets Section 1: The Solar System Section 2: The Inner PlanetsThe.

How the Solar System Formed11The Solar SystemThe Solar System

• As each cloud fragment contracted, its temperature increased.

• A star was born—the beginning of the Sun.

• Eventually, the temperature in the core of one of these cloud fragments reached about 10 million degrees Celsius and nuclear fusion began.

Page 14: Chapter: The Solar System Table of Contents Section 3: The Outer PlanetsThe Outer Planets Section 1: The Solar System Section 2: The Inner PlanetsThe.

How the Solar System Formed11The Solar SystemThe Solar System

• A cluster of stars like the Sun, or smaller, likely formed from fragments of the original cloud.

• The Sun probably escaped from this cluster and has since revolved around the galaxy about 20 times.

Page 15: Chapter: The Solar System Table of Contents Section 3: The Outer PlanetsThe Outer Planets Section 1: The Solar System Section 2: The Inner PlanetsThe.

Planet Formation11The Solar SystemThe Solar System

• The matter that did not get pulled into the center collided and stuck together to form the planets and asteroids.

• The inner planets of the solar system— Mercury, Venus, Earth, and Mars—are small, rocky planets with iron cores.

Page 16: Chapter: The Solar System Table of Contents Section 3: The Outer PlanetsThe Outer Planets Section 1: The Solar System Section 2: The Inner PlanetsThe.

Planet Formation11The Solar SystemThe Solar System

• The outer planets are Jupiter, Saturn, Uranus, Neptune, and Pluto.

• Pluto, a small planet, is the only outer planet made mostly of rock and ice.

Page 17: Chapter: The Solar System Table of Contents Section 3: The Outer PlanetsThe Outer Planets Section 1: The Solar System Section 2: The Inner PlanetsThe.

Planet Formation11The Solar SystemThe Solar System

• The other outer planets are much larger and are made mostly of lighter substances such as hydrogen, helium, methane, and ammonia.

Page 18: Chapter: The Solar System Table of Contents Section 3: The Outer PlanetsThe Outer Planets Section 1: The Solar System Section 2: The Inner PlanetsThe.

Motions of the Planets11The Solar SystemThe Solar System

• In the early 1600s, German mathematician Johannes Kepler began studying the orbits of the planets.

• He discovered that the shapes of the orbits are not circular.

• They are oval shaped, or elliptical.

Page 19: Chapter: The Solar System Table of Contents Section 3: The Outer PlanetsThe Outer Planets Section 1: The Solar System Section 2: The Inner PlanetsThe.

Motions of the Planets11The Solar SystemThe Solar System

• Kepler also discovered that the planets travel at different speeds in their orbits around the Sun.

• Planets closer to the Sun travel faster than planets farther away from the Sun.

Page 20: Chapter: The Solar System Table of Contents Section 3: The Outer PlanetsThe Outer Planets Section 1: The Solar System Section 2: The Inner PlanetsThe.

11Section CheckSection Check

Question 1

__________ gravity holds the solar system together.

A. Earth’s B. Jupiter’s C. The Moon’sD. The Sun’s

NC: 5.01, 5.03

Page 21: Chapter: The Solar System Table of Contents Section 3: The Outer PlanetsThe Outer Planets Section 1: The Solar System Section 2: The Inner PlanetsThe.

11Section CheckSection Check

Answer

The answer is D. Earth’s gravity holds the Moon in its orbit; the Sun’s gravity holds the solar system together.

NC: 5.01, 5.03

Page 22: Chapter: The Solar System Table of Contents Section 3: The Outer PlanetsThe Outer Planets Section 1: The Solar System Section 2: The Inner PlanetsThe.

11Section CheckSection Check

Question 2

The Sun, nine planets, and many smaller objects that orbit the Sun make up the _________.

A. galaxyB. solar systemC. inner planetsD. outer planets

NC: 5.01

Page 23: Chapter: The Solar System Table of Contents Section 3: The Outer PlanetsThe Outer Planets Section 1: The Solar System Section 2: The Inner PlanetsThe.

11Section CheckSection Check

Answer

The answer is B. The solar system also includes a huge volume of space.

NC: 5.01

Page 24: Chapter: The Solar System Table of Contents Section 3: The Outer PlanetsThe Outer Planets Section 1: The Solar System Section 2: The Inner PlanetsThe.

11Section CheckSection Check

Question 3

__________ developed the first Sun-centered model of the solar system.

A. EuripidesB. CopernicusC. GalileoD. Kepler

NC: 5.04

Page 25: Chapter: The Solar System Table of Contents Section 3: The Outer PlanetsThe Outer Planets Section 1: The Solar System Section 2: The Inner PlanetsThe.

11Section CheckSection Check

Answer

The answer is B. Nicholas Copernicus published his Sun-centered model in 1543.

NC: 5.04

Page 26: Chapter: The Solar System Table of Contents Section 3: The Outer PlanetsThe Outer Planets Section 1: The Solar System Section 2: The Inner PlanetsThe.

Inner Planets—Mercury

• The closest planet to the Sun is Mercury.

• The first American spacecraft mission to Mercury was in 1974-1975 by Mariner 10.

22The Inner PlanetsThe Inner Planets

Page 27: Chapter: The Solar System Table of Contents Section 3: The Outer PlanetsThe Outer Planets Section 1: The Solar System Section 2: The Inner PlanetsThe.

• The surface of Mercury has many craters and looks much like Earth's Moon.

• It also has cliffs as high as 3 km on its surface.

22The Inner PlanetsThe Inner Planets

• These cliffs might have formed at a time when Mercury shrank in diameter.

Inner PlanetsInner Planets—Mercury

Page 28: Chapter: The Solar System Table of Contents Section 3: The Outer PlanetsThe Outer Planets Section 1: The Solar System Section 2: The Inner PlanetsThe.

• Why would Mercury have shrunk?

• Mariner 10 detected a weak magnetic field around Mercury.

22The Inner PlanetsThe Inner Planets

• This indicates that the planet has an iron core.

Inner PlanetsInner Planets—Mercury

Page 29: Chapter: The Solar System Table of Contents Section 3: The Outer PlanetsThe Outer Planets Section 1: The Solar System Section 2: The Inner PlanetsThe.

• Scientists hypothesize that Mercury's crust solidified while the iron core was still hot and molten.

22The Inner PlanetsThe Inner Planets

• As the core started to solidify, it contracted.

Inner PlanetsInner Planets—Mercury

Page 30: Chapter: The Solar System Table of Contents Section 3: The Outer PlanetsThe Outer Planets Section 1: The Solar System Section 2: The Inner PlanetsThe.

Does Mercury have an atmosphere?

• Because of Mercury's low gravitational pull and high daytime temperatures, most gases that could form an atmosphere escape into space.

22The Inner PlanetsThe Inner Planets

• Hydrogen and helium gas that were first thought to be an atmosphere are now known to be temporarily taken from the solar wind.

Page 31: Chapter: The Solar System Table of Contents Section 3: The Outer PlanetsThe Outer Planets Section 1: The Solar System Section 2: The Inner PlanetsThe.

• Earth-based observations have found traces of sodium and potassium around Mercury.

22The Inner PlanetsThe Inner Planets

• These atoms probably come from rocks in the planet’s crust.

• Therefore, Mercury has no true atmosphere. • Mercury's temperature can reach 425C

during the day, and it can drop to –170C at night.

Does Mercury have an atmosphere?

Page 32: Chapter: The Solar System Table of Contents Section 3: The Outer PlanetsThe Outer Planets Section 1: The Solar System Section 2: The Inner PlanetsThe.

Venus• The second

planet from the Sun is Venus.

22The Inner PlanetsThe Inner Planets

• In 1962, Mariner 2 flew past Venus and sent back information about Venus's atmosphere and rotation.

Page 33: Chapter: The Solar System Table of Contents Section 3: The Outer PlanetsThe Outer Planets Section 1: The Solar System Section 2: The Inner PlanetsThe.

Venus

• Between 1990 and 1994, the U.S. Magellan probe used its radar to make the most detailed maps yet of Venus's surface.

22The Inner PlanetsThe Inner Planets

• Clouds on Venus are so dense that only a small percentage of the sunlight that strikes the top of the clouds reaches the planet’s surface.

Page 34: Chapter: The Solar System Table of Contents Section 3: The Outer PlanetsThe Outer Planets Section 1: The Solar System Section 2: The Inner PlanetsThe.

Venus

• The sunlight that does get through warms Venus's surface, which then gives off heat to the atmosphere.

22The Inner PlanetsThe Inner Planets

• Much of this heat is absorbed by carbon dioxide gas in Venus’s atmosphere.

Page 35: Chapter: The Solar System Table of Contents Section 3: The Outer PlanetsThe Outer Planets Section 1: The Solar System Section 2: The Inner PlanetsThe.

Venus

• This causes a greenhouse effect.

22The Inner PlanetsThe Inner Planets

• Due to this intense greenhouse effect, the temperature on the surface of Venus is between 450°C and 475°C.

Page 36: Chapter: The Solar System Table of Contents Section 3: The Outer PlanetsThe Outer Planets Section 1: The Solar System Section 2: The Inner PlanetsThe.

Earth • Earth is the third planet from the sun.

22The Inner PlanetsThe Inner Planets

• Unlike other planets, Earth has abundant liquid water and supports life.

Page 37: Chapter: The Solar System Table of Contents Section 3: The Outer PlanetsThe Outer Planets Section 1: The Solar System Section 2: The Inner PlanetsThe.

Earth • Earth's atmosphere causes most meteors to burn up before they reach the surface, and it protects life-forms from the effects of the Sun's intense radiation.

22The Inner PlanetsThe Inner Planets

Page 38: Chapter: The Solar System Table of Contents Section 3: The Outer PlanetsThe Outer Planets Section 1: The Solar System Section 2: The Inner PlanetsThe.

Mars • Can you guess

why Mars, the fourth planet from the Sun, is called the red planet?

22The Inner PlanetsThe Inner Planets

• Iron oxide in soil on its surface gives it a reddish color.

Page 39: Chapter: The Solar System Table of Contents Section 3: The Outer PlanetsThe Outer Planets Section 1: The Solar System Section 2: The Inner PlanetsThe.

Mars

• Other features visible from Earth are Mars's polar ice caps and changes in the coloring of the planet’s surface.

22The Inner PlanetsThe Inner Planets

• The ice caps are made of frozen water covered by a layer of frozen carbon dioxide.

Page 40: Chapter: The Solar System Table of Contents Section 3: The Outer PlanetsThe Outer Planets Section 1: The Solar System Section 2: The Inner PlanetsThe.

Mars • Most of the information scientists have

about Mars came from Mariner 9, the Viking probes, Mars Pathfinder, Mars Global Surveyor, and Mars Odyssey.

22The Inner PlanetsThe Inner Planets

• Mariner 9 revealed long channels on the planet that might have been carved by flowing water.

• Mariner 9 also discovered the largest volcano in the solar system, Olympus Mons.

Page 41: Chapter: The Solar System Table of Contents Section 3: The Outer PlanetsThe Outer Planets Section 1: The Solar System Section 2: The Inner PlanetsThe.

Mars

• Olympus Mons is probably extinct.

22The Inner PlanetsThe Inner Planets

• Large rift valleys that formed in the Martian crust also were discovered.

Page 42: Chapter: The Solar System Table of Contents Section 3: The Outer PlanetsThe Outer Planets Section 1: The Solar System Section 2: The Inner PlanetsThe.

The Viking Probes• The Viking 1 and 2 probes arrived at Mars

in 1976.

22The Inner PlanetsThe Inner Planets

• Each spacecraft consisted of an orbiter and a lander.

• The Viking 1 and 2 orbiters photographed the entire surface of Mars, while the Viking 1 and 2 landers touched down on the planet’s surface.

Page 43: Chapter: The Solar System Table of Contents Section 3: The Outer PlanetsThe Outer Planets Section 1: The Solar System Section 2: The Inner PlanetsThe.

The Viking Probes

• The landers carried equipment to detect possible life on Mars.

22The Inner PlanetsThe Inner Planets

• These experiments found no conclusive evidence of life on Mars.

Page 44: Chapter: The Solar System Table of Contents Section 3: The Outer PlanetsThe Outer Planets Section 1: The Solar System Section 2: The Inner PlanetsThe.

Pathfinder, Global Surveyor, and Odyssey

• The Mars Pathfinder carried a robot rover named Sojourner with equipment that allowed it to analyze samples of Martian rock and soil.

22The Inner PlanetsThe Inner Planets

Page 45: Chapter: The Solar System Table of Contents Section 3: The Outer PlanetsThe Outer Planets Section 1: The Solar System Section 2: The Inner PlanetsThe.

Pathfinder, Global Surveyor, and Odyssey

22The Inner PlanetsThe Inner Planets

• Cameras onboard Global Surveyor showed features that look like gullies formed by flowing water and deposits of sediment carried by the water flows.

Page 46: Chapter: The Solar System Table of Contents Section 3: The Outer PlanetsThe Outer Planets Section 1: The Solar System Section 2: The Inner PlanetsThe.

Pathfinder, Global Surveyor, and Odyssey

• The features are young enough that scientists are considering the idea that liquid groundwater might exist on Mars and that it sometimes reaches the surface.

22The Inner PlanetsThe Inner Planets

Page 47: Chapter: The Solar System Table of Contents Section 3: The Outer PlanetsThe Outer Planets Section 1: The Solar System Section 2: The Inner PlanetsThe.

Pathfinder, Global Surveyor, and Odyssey

• Instruments on another probe called Mars Odyssey detected frozen water on Mars.

22The Inner PlanetsThe Inner Planets

• The water occurs as frost beneath a thin layer of soil.

Page 48: Chapter: The Solar System Table of Contents Section 3: The Outer PlanetsThe Outer Planets Section 1: The Solar System Section 2: The Inner PlanetsThe.

Mars's Atmosphere

• Mars's atmosphere is much thinner than Earth's. It is composed mostly of carbon dioxide, with some nitrogen and argon. Surface temperatures range from –125C to 35C.

22The Inner PlanetsThe Inner Planets

Page 49: Chapter: The Solar System Table of Contents Section 3: The Outer PlanetsThe Outer Planets Section 1: The Solar System Section 2: The Inner PlanetsThe.

Martian Seasons

• Mars goes through seasons as it orbits the Sun, just like Earth does.

22The Inner PlanetsThe Inner Planets

• The polar ice caps on Mars change with the season.

• During winter, carbon dioxide ice accumulates and makes the ice cap larger.

Page 50: Chapter: The Solar System Table of Contents Section 3: The Outer PlanetsThe Outer Planets Section 1: The Solar System Section 2: The Inner PlanetsThe.

Martian Seasons

• During summer, carbon dioxide ice changes to carbon dioxide gas and the ice cap shrinks.

22The Inner PlanetsThe Inner Planets

• The color of the ice caps and other areas on Mars also changes with the season.

• The movement of dust and sand during dust storms causes the changing colors.

Page 51: Chapter: The Solar System Table of Contents Section 3: The Outer PlanetsThe Outer Planets Section 1: The Solar System Section 2: The Inner PlanetsThe.

Martian Moons

• Mars has two small, irregularly shaped moons that are heavily cratered.

22The Inner PlanetsThe Inner Planets

• Phobos is about 25 km in length, and Deimos is about 13 km in length.

Page 52: Chapter: The Solar System Table of Contents Section 3: The Outer PlanetsThe Outer Planets Section 1: The Solar System Section 2: The Inner PlanetsThe.

Martian Moons

• Phobos has many interesting surface features.

22The Inner PlanetsThe Inner Planets

• Grooves and chains of smaller craters seem to radiate out from the large Stickney Crater.

• These features probably are the result of the large impact that formed the Stickney Crater.

Page 53: Chapter: The Solar System Table of Contents Section 3: The Outer PlanetsThe Outer Planets Section 1: The Solar System Section 2: The Inner PlanetsThe.

Martian Moons

• Deimos is among the smallest known moons in the solar system.

22The Inner PlanetsThe Inner Planets

• Its surface is smoother in appearance than that of Phobos because some of its craters have partially filled with soil and rock.

Page 54: Chapter: The Solar System Table of Contents Section 3: The Outer PlanetsThe Outer Planets Section 1: The Solar System Section 2: The Inner PlanetsThe.

22Section CheckSection Check

Question 1

Which planet is closest to the Sun?

A. MarsB. MercuryC. Earth D. Venus

NC: 5.01

Page 55: Chapter: The Solar System Table of Contents Section 3: The Outer PlanetsThe Outer Planets Section 1: The Solar System Section 2: The Inner PlanetsThe.

22Section CheckSection Check

Answer

The answer is B. Mercury is the closest planet to the Sun. Venus is the second planet from the Sun.

NC: 5.01

Page 56: Chapter: The Solar System Table of Contents Section 3: The Outer PlanetsThe Outer Planets Section 1: The Solar System Section 2: The Inner PlanetsThe.

22Section CheckSection Check

Question 2

Which planet has size and mass similar to Earth’s?

A. JupiterB. MercuryC. PlutoD. Venus

NC: 5.01, 5.02

Page 57: Chapter: The Solar System Table of Contents Section 3: The Outer PlanetsThe Outer Planets Section 1: The Solar System Section 2: The Inner PlanetsThe.

22Section CheckSection Check

Answer

The answer is D. Venus has similar size and mass but the temperatures on its surface are between 450º C and 475º C.

NC: 5.01, 5.02

Page 58: Chapter: The Solar System Table of Contents Section 3: The Outer PlanetsThe Outer Planets Section 1: The Solar System Section 2: The Inner PlanetsThe.

22Section CheckSection Check

Question 3

Earth is the __________ planet from the Sun.

A. secondB. thirdC. fourthD. fifth

NC: 5.01, 5.02, 5.05

Page 59: Chapter: The Solar System Table of Contents Section 3: The Outer PlanetsThe Outer Planets Section 1: The Solar System Section 2: The Inner PlanetsThe.

22Section CheckSection Check

Answer

The answer is B. Mercury and Venus are closer to the Sun than Earth.

NC: 5.01, 5.02, 5.05

Page 60: Chapter: The Solar System Table of Contents Section 3: The Outer PlanetsThe Outer Planets Section 1: The Solar System Section 2: The Inner PlanetsThe.

Outer Planets—Jupiter • In 1979, Voyager 1 and Voyager 2 flew past

Jupiter, the fifth planet from the Sun.

33The Outer PlanetsThe Outer Planets

• The Voyager probes revealed that Jupiter has faint dust rings around it and that one of its moons has active volcanoes on it.

Page 61: Chapter: The Solar System Table of Contents Section 3: The Outer PlanetsThe Outer Planets Section 1: The Solar System Section 2: The Inner PlanetsThe.

Jupiter's Atmosphere• Jupiter is composed mostly of hydrogen and

helium, with some ammonia, methane, and water vapor.

• Scientists hypothesize that the atmosphere of hydrogen and helium changes to an ocean of liquid hydrogen and helium toward the middle of the planet.

33The Outer PlanetsThe Outer Planets

Page 62: Chapter: The Solar System Table of Contents Section 3: The Outer PlanetsThe Outer Planets Section 1: The Solar System Section 2: The Inner PlanetsThe.

Jupiter's Atmosphere• Below this liquid layer might be a rocky core.

• Continuous storms of swirling, high-pressure gas have been observed on Jupiter.

33The Outer PlanetsThe Outer Planets

• The Great Red Spot is the most spectacular of these storms.

Page 63: Chapter: The Solar System Table of Contents Section 3: The Outer PlanetsThe Outer Planets Section 1: The Solar System Section 2: The Inner PlanetsThe.

Moons of Jupiter

• At least 61 moons orbit Jupiter.

• In 1610, the astronomer Galileo Galilei was the first person to see Jupiter's four largest moons described in the table.

33The Outer PlanetsThe Outer Planets

Page 64: Chapter: The Solar System Table of Contents Section 3: The Outer PlanetsThe Outer Planets Section 1: The Solar System Section 2: The Inner PlanetsThe.

Saturn

• The Voyager probes surveyed Saturn in 1980 and 1981.

• Saturn is the sixth planet from the Sun.

33The Outer PlanetsThe Outer Planets

• It is the second-largest planet in the solar system, but it has the lowest density.

Page 65: Chapter: The Solar System Table of Contents Section 3: The Outer PlanetsThe Outer Planets Section 1: The Solar System Section 2: The Inner PlanetsThe.

Saturn's Atmosphere• Saturn is a large, gaseous planet. It has a thick

outer atmosphere composed mostly of hydrogen and helium.

33The Outer PlanetsThe Outer Planets

• As you go deeper into Saturn’s atmosphere, the gases gradually change to liquid hydrogen and helium.

• Saturn might have a small, rocky core.

Page 66: Chapter: The Solar System Table of Contents Section 3: The Outer PlanetsThe Outer Planets Section 1: The Solar System Section 2: The Inner PlanetsThe.

Rings and Moons• Saturn has several broad rings. • Each large ring is

composed of thousands of thin ringlets.

33The Outer PlanetsThe Outer Planets

• Saturn's rings are composed of countless ice and rock particles.

Page 67: Chapter: The Solar System Table of Contents Section 3: The Outer PlanetsThe Outer Planets Section 1: The Solar System Section 2: The Inner PlanetsThe.

Rings and Moons

• At least 31 moons orbit Saturn.

• The largest of Saturn's moons, Titan, is larger than the planet Mercury.

33The Outer PlanetsThe Outer Planets

• It has an atmosphere of nitrogen, argon, and methane.

Page 68: Chapter: The Solar System Table of Contents Section 3: The Outer PlanetsThe Outer Planets Section 1: The Solar System Section 2: The Inner PlanetsThe.

Uranus• Uranus (YOOR uh

nus) is the seventh planet from the Sun and was discovered in 1781.

• It is a large, gaseous planet with at least 21 moons and a system of thin, dark rings.

33The Outer PlanetsThe Outer Planets

Page 69: Chapter: The Solar System Table of Contents Section 3: The Outer PlanetsThe Outer Planets Section 1: The Solar System Section 2: The Inner PlanetsThe.

Uranus• Uranus's largest

moon, Titania, has many craters and deep valleys.

• The valleys on this moon indicate that some process reshaped its surface after it formed.

33The Outer PlanetsThe Outer Planets

Page 70: Chapter: The Solar System Table of Contents Section 3: The Outer PlanetsThe Outer Planets Section 1: The Solar System Section 2: The Inner PlanetsThe.

Uranus's Characteristics

• The atmosphere of Uranus is composed of hydrogen, helium, and some methane.

• Methane gives the planet bluish green color.

33The Outer PlanetsThe Outer Planets

• Evidence suggests that under its atmosphere, Uranus has a mantle of liquid water, methane, and ammonia surrounding a rocky core.

Page 71: Chapter: The Solar System Table of Contents Section 3: The Outer PlanetsThe Outer Planets Section 1: The Solar System Section 2: The Inner PlanetsThe.

Uranus's Characteristics• Uranus's axis of rotation is tilted on its side

compared with the other planets. • The axis of rotation of

the other planets, except Pluto, are nearly perpendicular to the planes of their orbits.

33The Outer PlanetsThe Outer Planets

• Uranus's axis of rotation is nearly parallel to the plane of its orbit.

Page 72: Chapter: The Solar System Table of Contents Section 3: The Outer PlanetsThe Outer Planets Section 1: The Solar System Section 2: The Inner PlanetsThe.

Neptune

• Discovered in 1846, Neptune is usually the eighth planet from the Sun. However, Pluto's orbit crosses inside Neptune's during part of its voyage around the Sun.

• Between 1979 and 1999, Pluto was closer to the Sun than was Neptune.

33The Outer PlanetsThe Outer Planets

Page 73: Chapter: The Solar System Table of Contents Section 3: The Outer PlanetsThe Outer Planets Section 1: The Solar System Section 2: The Inner PlanetsThe.

Neptune's Characteristics• Neptune's atmosphere is similar to Uranus's

atmosphere. • The methane content gives

Neptune, its distinctive bluish-green color.

33The Outer PlanetsThe Outer Planets

• Neptune has dark-colored storms in its atmosphere that are similar to the Great Red Spot on Jupiter.

Page 74: Chapter: The Solar System Table of Contents Section 3: The Outer PlanetsThe Outer Planets Section 1: The Solar System Section 2: The Inner PlanetsThe.

Neptune's Characteristics• Bright clouds form and then disappear. • This shows that Neptune's atmosphere is

active and changes rapidly.

33The Outer PlanetsThe Outer Planets

• Under its atmosphere, Neptune is thought to have a layer of liquid water, methane, and ammonia that might change to solid ice. • Neptune probably has a rocky core.

Page 75: Chapter: The Solar System Table of Contents Section 3: The Outer PlanetsThe Outer Planets Section 1: The Solar System Section 2: The Inner PlanetsThe.

Neptune's Characteristics

• Neptune has at least 11 moons and several rings.

• Triton, is Neptune's largest moon.

33The Outer PlanetsThe Outer Planets

• Neptune's rings are young and probably won't last very long.

Page 76: Chapter: The Solar System Table of Contents Section 3: The Outer PlanetsThe Outer Planets Section 1: The Solar System Section 2: The Inner PlanetsThe.

Pluto• The smallest planet in the solar system, and the

one scientists know the least about, is Pluto.

33The Outer PlanetsThe Outer Planets

• Because Pluto is farther from the Sun than Neptune during most of its orbit, it is considered to be the ninth planet from the Sun.

Page 77: Chapter: The Solar System Table of Contents Section 3: The Outer PlanetsThe Outer Planets Section 1: The Solar System Section 2: The Inner PlanetsThe.

Pluto

• Pluto is vastly different from the other outer planets.

33The Outer PlanetsThe Outer Planets

• It's surrounded by only a thin atmosphere, and it's the only outer planet with a solid, icy-rock surface.

Page 78: Chapter: The Solar System Table of Contents Section 3: The Outer PlanetsThe Outer Planets Section 1: The Solar System Section 2: The Inner PlanetsThe.

Pluto's Moon

• Pluto's single moon, Charon, has a diameter about half the size of Pluto's.

33The Outer PlanetsThe Outer Planets

• Because of their close size and orbit, some scientists consider them to be a double planet.

Page 79: Chapter: The Solar System Table of Contents Section 3: The Outer PlanetsThe Outer Planets Section 1: The Solar System Section 2: The Inner PlanetsThe.

Pluto's Moon

• Data from the Hubble Space Telescope indicate the presence of a vast disk of icy objects called the Kuiper Belt beyond Neptune's orbits.

33The Outer PlanetsThe Outer Planets

• Many astronomers think that Pluto and Charon are members of the Kuiper Belt.

Page 80: Chapter: The Solar System Table of Contents Section 3: The Outer PlanetsThe Outer Planets Section 1: The Solar System Section 2: The Inner PlanetsThe.

33Section CheckSection Check

Question 1

The fifth planet from the Sun is __________.

A. JupiterB. NeptuneC. SaturnD. Pluto

NC: 5.01

Page 81: Chapter: The Solar System Table of Contents Section 3: The Outer PlanetsThe Outer Planets Section 1: The Solar System Section 2: The Inner PlanetsThe.

33Section CheckSection Check

Answer

The answer is A. Jupiter is the largest planet in the solar system.

NC: 5.01

Page 82: Chapter: The Solar System Table of Contents Section 3: The Outer PlanetsThe Outer Planets Section 1: The Solar System Section 2: The Inner PlanetsThe.

33Section CheckSection Check

Question 2

Which of Jupiter’s large moons is closest to Jupiter and the most volcanically active object in the solar system?

A. CallistoB. EuropaC. GanymedeD. Io

NC: 5.01

Page 83: Chapter: The Solar System Table of Contents Section 3: The Outer PlanetsThe Outer Planets Section 1: The Solar System Section 2: The Inner PlanetsThe.

33Section CheckSection Check

Answer

The answer is D. Jupiter exerts tremendous gravitational pull on Io.

NC: 5.01

Page 84: Chapter: The Solar System Table of Contents Section 3: The Outer PlanetsThe Outer Planets Section 1: The Solar System Section 2: The Inner PlanetsThe.

33Section CheckSection Check

Question 3

It takes Pluto __________ to orbit the Sun one time.

A. 2 yearsB. 24 yearsC. 124 yearsD. 248 years

NC: 5.01

Page 85: Chapter: The Solar System Table of Contents Section 3: The Outer PlanetsThe Outer Planets Section 1: The Solar System Section 2: The Inner PlanetsThe.

33Section CheckSection Check

Answer

The answer is D. During part of its orbit, Pluto is closer to the Sun than Neptune, but is still considered to be the ninth planet from the Sun.

NC: 5.01

Page 86: Chapter: The Solar System Table of Contents Section 3: The Outer PlanetsThe Outer Planets Section 1: The Solar System Section 2: The Inner PlanetsThe.

Comets

• Comets, meteoroids and asteroids are other important objects in the solar system.

• A comet is composed of dust and rock particles mixed with frozen water, methane, and ammonia.

44Other Objects in the Solar SystemOther Objects in the Solar System

Page 87: Chapter: The Solar System Table of Contents Section 3: The Outer PlanetsThe Outer Planets Section 1: The Solar System Section 2: The Inner PlanetsThe.

Oort Cloud

• Astronomer Jan Oort proposed the idea that billions of comets surround the solar system.

• This cloud of comets, called the Oort Cloud, is located beyond the orbit of Pluto.

44Other Objects in the Solar SystemOther Objects in the Solar System

• Oort suggested that the gravities of the Sun and nearby stars interact with comets in the Oort Cloud.

Page 88: Chapter: The Solar System Table of Contents Section 3: The Outer PlanetsThe Outer Planets Section 1: The Solar System Section 2: The Inner PlanetsThe.

Comet Hale-Bopp • On July 23, 1995, two

amateur astronomers made an exciting discovery.

• A new comet, Comet Hale-Bopp, was headed toward the Sun.

44Other Objects in the Solar SystemOther Objects in the Solar System

• Larger than most that approach the Sun, it was the brightest comet visible from Earth in 20 years.

Page 89: Chapter: The Solar System Table of Contents Section 3: The Outer PlanetsThe Outer Planets Section 1: The Solar System Section 2: The Inner PlanetsThe.

Structure of Comets• As a comet approaches the Sun, it changes. • Ices of water, methane, and ammonia

vaporize because of the heat from the Sun, releasing dust and bits of rock.

44Other Objects in the Solar SystemOther Objects in the Solar System

Page 90: Chapter: The Solar System Table of Contents Section 3: The Outer PlanetsThe Outer Planets Section 1: The Solar System Section 2: The Inner PlanetsThe.

Structure of Comets44Other Objects in the Solar SystemOther Objects in the Solar System

• The gases and released dust form a bright cloud called a coma around the nucleus, or solid part, of the comet.

Page 91: Chapter: The Solar System Table of Contents Section 3: The Outer PlanetsThe Outer Planets Section 1: The Solar System Section 2: The Inner PlanetsThe.

Structure of Comets• The solar wind pushes on the gases and dust

in the coma, causing the particles to form separate tails that point away from the Sun.

• After many trips around the Sun, most of the ice in a comet's nucleus has vaporized.

44Other Objects in the Solar SystemOther Objects in the Solar System

• All that's left are dust and rock, which are spread throughout the orbit of the original comet.

Page 92: Chapter: The Solar System Table of Contents Section 3: The Outer PlanetsThe Outer Planets Section 1: The Solar System Section 2: The Inner PlanetsThe.

Meteoroids, Meteors, and Meteorites

• The small pieces from the comet's nucleus spread out into a loose group within the original orbit of the comet.

• These pieces of dust and rock, along with those derived from other sources, are called meteoroids.

44Other Objects in the Solar SystemOther Objects in the Solar System

Page 93: Chapter: The Solar System Table of Contents Section 3: The Outer PlanetsThe Outer Planets Section 1: The Solar System Section 2: The Inner PlanetsThe.

Meteoroids, Meteors, and Meteorites

• Most meteoroids are so small that they completely burn up in Earth's atmosphere.

• A meteoroid that burns up in Earth's atmosphere is called a meteor.

44Other Objects in the Solar SystemOther Objects in the Solar System

Page 94: Chapter: The Solar System Table of Contents Section 3: The Outer PlanetsThe Outer Planets Section 1: The Solar System Section 2: The Inner PlanetsThe.

Meteor Showers

• Each time Earth passes through the loose group of particles within the old orbit of a comet, many small particles of rock and dust enter the atmosphere.

• Because more meteors than usual are seen, the event is called a meteor shower.

44Other Objects in the Solar SystemOther Objects in the Solar System

Page 95: Chapter: The Solar System Table of Contents Section 3: The Outer PlanetsThe Outer Planets Section 1: The Solar System Section 2: The Inner PlanetsThe.

Meteor Showers

• When a meteoroid is large enough, it might not burn up completely in the atmosphere.

• If it strikes Earth, it is called a meteorite.

44Other Objects in the Solar SystemOther Objects in the Solar System

• Most meteorites are probably debris from asteroid collisions or broken-up comets, but some originate from the Moon and Mars.

Page 96: Chapter: The Solar System Table of Contents Section 3: The Outer PlanetsThe Outer Planets Section 1: The Solar System Section 2: The Inner PlanetsThe.

Asteroids• An asteroid is a piece of rock similar to

the material that formed into the planets.

44Other Objects in the Solar SystemOther Objects in the Solar System

• Most asteroids are located in an area between the orbits of Mars and Jupiter called the asteroid belt.

Page 97: Chapter: The Solar System Table of Contents Section 3: The Outer PlanetsThe Outer Planets Section 1: The Solar System Section 2: The Inner PlanetsThe.

Asteroids

• Other asteroids are scattered throughout the solar system.

44Other Objects in the Solar SystemOther Objects in the Solar System

• They might have been thrown out of the belt by Jupiter's gravity.

• Scientists monitor the positions of these asteroids. However, it is unlikely that an asteroid will hit Earth in the near future.

Page 98: Chapter: The Solar System Table of Contents Section 3: The Outer PlanetsThe Outer Planets Section 1: The Solar System Section 2: The Inner PlanetsThe.

Exploring Asteroids

• The sizes of the asteroids in the asteroid belt range from tiny particles to objects 940 km in diameter.

44Other Objects in the Solar SystemOther Objects in the Solar System

• Ceres is the largest and the first one discovered.

• The next three in order of size are Vesta (530 km), Pallas (522 km), and 10 Hygiea (430 km).

Page 99: Chapter: The Solar System Table of Contents Section 3: The Outer PlanetsThe Outer Planets Section 1: The Solar System Section 2: The Inner PlanetsThe.

NEAR

• On February 14, 2000, the Near Earth Asteroid Rendezvous (NEAR) spacecraft went into orbit around the asteroid 433 Eros and successfully began its one-year mission of data gathering.

44Other Objects in the Solar SystemOther Objects in the Solar System

• On February 12, 2001, NEAR ended its mission by becoming the first spacecraft to land softly on an asteroid.

Page 100: Chapter: The Solar System Table of Contents Section 3: The Outer PlanetsThe Outer Planets Section 1: The Solar System Section 2: The Inner PlanetsThe.

44Section CheckSection Check

Question 1

A __________ is composed of dust and rock particles mixed with frozen water, methane and ammonia.

A. asteroidB. cometC. planetD. sun

NC: 5.01

Page 101: Chapter: The Solar System Table of Contents Section 3: The Outer PlanetsThe Outer Planets Section 1: The Solar System Section 2: The Inner PlanetsThe.

44Section CheckSection Check

Answer

The answer is B. Some comets, such as Hale-Bopp, are named after the astronomers who discover them.

NC: 5.01

Page 102: Chapter: The Solar System Table of Contents Section 3: The Outer PlanetsThe Outer Planets Section 1: The Solar System Section 2: The Inner PlanetsThe.

44Section CheckSection Check

Question 2

Small pieces from a comet’s nucleus that spread out into a loose group are called ____________.

A. asteroidsB. meteoritesC. meteoroidsD. meteors

NC: 5.01

Page 103: Chapter: The Solar System Table of Contents Section 3: The Outer PlanetsThe Outer Planets Section 1: The Solar System Section 2: The Inner PlanetsThe.

44Section CheckSection Check

Answer

The answer is C. A meteoroid that burns up in Earth’s atmosphere is called a meteor.

NC: 5.01

Page 104: Chapter: The Solar System Table of Contents Section 3: The Outer PlanetsThe Outer Planets Section 1: The Solar System Section 2: The Inner PlanetsThe.

44Section CheckSection Check

Question 3

What is a meteorite?

Meteorites are meteoroids that strike Earth.

Answer

NC: 5.01

Page 105: Chapter: The Solar System Table of Contents Section 3: The Outer PlanetsThe Outer Planets Section 1: The Solar System Section 2: The Inner PlanetsThe.

To advance to the next item or next page click on any of the following keys: mouse, space bar, enter, down or forward arrow.

Click on this icon to return to the table of contents

Click on this icon to return to the previous slide

Click on this icon to move to the next slide

Click on this icon to open the resources file.

HelpHelp

Click on this icon to go to the end of the presentation.

Page 106: Chapter: The Solar System Table of Contents Section 3: The Outer PlanetsThe Outer Planets Section 1: The Solar System Section 2: The Inner PlanetsThe.

End of Chapter Summary File