Scott Foresman Science - Plain Local Schools

Scott Foresman ScienceNonfi ction Predict • Captions
Scott Foresman Science 4.18
Nonfi ction Predict • Captions
ì<(sk$m)=bdjbbi< +^-Ä-U-Ä-U 13911_01-04_CVR_FSD.indd Cover113911_01-04_CVR_FSD.indd Cover1 5/12/05 8:42:13 PM5/12/05 8:42:13 PM
1. How are the orbits of the inner planets different from the orbits of the outer planets?
2. Why is it diffi cult to study Venus?
3. What makes Pluto’s orbit different from all the other planets?
4. Gravity is the force that holds the solar system together. Write to explain what effect gravity has between the Sun and the planets, and between the planets and their moons. Use details from the book to support your answer.
5. Predict Do you think scientists will fi nd other planets in the solar system? Explain your prediction.
What did you learn?Vocabulary
astronomy craters galaxy satellite solar system space probe universe
Picture Credits Every effort has been made to secure permission and provide appropriate credit for photographic material. The publisher deeply regrets any omission and pledges to correct errors called to its attention in subsequent editions.
Photo locators denoted as follows: Top (T), Center (C), Bottom (B), Left (L), Right (R), Background (Bkgd).
Opener Brand X Pictures; 2 (T) ©Myron Jay Dorf/Corbis; 3 Getty Images; 7 (T) Brand X Pictures; 10 (TL, BR) Brand X Pictures; 11 (BR) Getty Images; 13 (TR) Getty Images, (BR) ©JPL/NASA; 14 (TR) Getty Images; 16 (TR) Getty Images; 17 (TR) Getty Images, (CR, BR) Calvin J Hamilton/©Galaxy Picture Library; 23 (CR) NASA/JPL-Caltech/©Galaxy Picture Library.
Scott Foresman/Dorling Kindersley would also like to thank: 1, 2 (B) NASA/JPL/DK Images; 6 (TL) NASA/DK Images, (TR) NASA/Finley Holiday Films/DK Images; 9 (TR) NASA/DK Images; 11 (T) NASA/DK Images; 12 NASA/DK Images; 15 (CL, BL) Jet Propulsion Lab/DK Images; 19 (TR, CL) Jet Propulsion Lab/DK Images; 21 (BR) NASA/JPL/DK Images.
Unless otherwise acknowledged, all photographs are the copyright © of Dorling Kindersley, a division of Pearson.
ISBN: 0-328-13911-4
Copyright © Pearson Education, Inc. All Rights Reserved. Printed in the United States of America. This publication is protected by Copyright, and permission should be obtained from the publisher prior to any prohibited reproduction, storage in a retrieval system, or transmission in any form by any means, electronic, mechanical, photocopying, recording, or likewise. For information regarding permission(s), write to Permissions Department, Scott Foresman, 1900 East Lake Avenue, Glenview, Illinois 60025.
3 4 5 6 7 8 9 10 V010 13 12 11 10 09 08 07 06 05
13911_01-04_CVR_FSD.indd Cover213911_01-04_CVR_FSD.indd Cover2 5/12/05 8:42:20 PM5/12/05 8:42:20 PM
by Maria Estes
2005
Other
3.1869376
The universe is all of space and everything in it. The universe has millions of galaxies. A galaxy is a system of billions of stars, gases, and dust. The galaxy that we live in is called the Milky Way. When you look at the night sky, most of the stars you see are part of the Milky Way. From Earth, it looks like a glowing band of light that stretches across the sky.
If you could look down on the Milky Way, it would look similar to a spinning pinwheel. It is thicker at the center than at the edges.
The Universe
3
This is how the Milky Way would look if you could look down on it. Our solar system is just one tiny part of this galaxy.
The study of the Sun, Moon, stars, and other objects in space is called astronomy. Early astronomers noticed that most of the lights in the sky remained in the same place. A few of them, however, moved across the sky. We call these moving objects “planets.” The word planet comes from the Greek word planetes, meaning “wanderer.”
Other early civilizations also studied the Sun and the stars. Stonehenge is a giant circle of stones in England. Scientists believe that the ancient people who built this had a good understanding of the movements and patterns of the Sun and the stars. Some of the stones point to where the Sun rises and sets on the longest day of the year.
Stonehenge
2005
49.267128
2005
Other
64.26176
4
The solar system includes the Sun, the planets and their moons, and other objects. The Sun is in the center of the solar system. All the other objects in the solar system travel around the Sun in a path called an orbit.
A planet is a very large, round object that moves around a star. Earth is a planet that moves around the Sun. The Sun is a star. Planets are cooler than stars. They are also smaller than stars. Planets don’t give off their own light, as stars do. They refl ect light from the star that they orbit.
The Solar System
5
Our solar system has inner and outer planets. Mercury, Venus, Earth, and Mars are the inner planets. They are solid and rocky. Jupiter, Saturn, Uranus, Neptune, and Pluto are the outer planets. With the exception of Pluto, these planets are made mostly of gas or ice.
Asteroids are rocky objects that are too small to be called planets. Asteroids travel around the Sun in a path between Mars and Jupiter. This area is called the asteroid belt.
Pluto
Uranus
2005
Other
54.126015
2005
Other
47.22953
6
Gravity is the force that holds the solar system together. Without gravity, the planets would move in a straight line off into space. The Sun’s gravity pulls the planets toward it. This pull from the Sun makes the planets move in orbits around it.
Look at the diagram of the solar system above. The orbits of the inner planets are almost in the shape of circles. The orbits of the outer planets are not quite as round. Their orbits are longer and narrower than those of the inner planets.
This is our solar system as viewed from above. Pluto has a much narrower orbit than the other planets have.
What is gravity?
Neptune
Uranus
Jupiter
Earth
Mercury
Saturn
Mars
Venus
Pluto
Sun
The sizes and distances in this diagram are not true to scale.
13911_05-28_FSD.indd 613911_05-28_FSD.indd 6 5/12/05 8:44:10 PM5/12/05 8:44:10 PM
7
The Sun
Our Sun is an average-sized star. But it is big enough that all the planets and their moons could fi t in a small corner of it! The Sun, like all other stars, is a huge ball of very hot gases. Energy from the Sun provides light and heat on Earth.
The inner parts of the Sun are much hotter than the outer parts. Scientists have not been able to actually record the temperature of the Sun. However, they believe that the outer part of the Sun is about 5,500°C (10,000°F). The inside of the Sun could be as hot as 15,000,000°C (27,000,000°F).
The Sun’s gravity holds its gases together in the shape of a ball.
2005
Other
45.87113
2005
Other
60.029823
8
The Inner Planets
Mercury is the planet closest to the Sun. It’s only a little bigger than Earth’s moon. The surface of Mercury is covered with huge, bowl-shaped dents called craters.
In late 1973, scientists sent the Mariner 10 space probe to Mercury to gather information. A space probe is a vehicle that carries cameras and other tools for studying objects in space.
It is very hot on Mercury during the day. The hottest temperature recorded on Mercury was 467°C (870°F). But it has almost no atmosphere to hold the Sun’s heat. This makes the nights very cold. The coldest temperature recorded on Mercury was –183°C (–297°F).
Facts about Mercury
Distance from the Sun: 57,900,000 km (35,983,000 mi) Diameter: 4,879 km (3,032 mi) Length of a day as measured in Earth time: 59 days Length of a year as measured in Earth time: 88 days Average surface temperature: 117°C (243°F) Number of moons: none Weight of a child who is 75 lb on Earth: 28.5 lb
Mercury
9
Venus
Venus is about the same size as Earth. Venus is diffi cult to study because it is always covered by thick, hot, poisonous clouds. The clouds on Venus refl ect the Sun’s light. This makes Venus one of the brightest objects in Earth’s night sky.
Similar to Mercury, Venus is hot and dry. It also is covered by craters, cracks, and ridges. Venus is the hottest planet in the solar system. Ten Russian space probes have been able to land on the surface of Venus. Several of them sent photographs back to Earth before they were destroyed by the heat.
The thick clouds that cover Venus are hot and poisonous.
Distance from the Sun: 108,200,000 km (67,200,000 mi) Diameter: 12,104 km (7,521 mi) Length of a day as measured in Earth time: 243 days; spins backward Length of a year as measured in Earth time: 225 days Average surface temperature: 464°C (867°F) Number of moons: none Weight of a child who is 75 lb on Earth: 68.25 lb
Facts about Venus
2005
70.26971
2005
Other
56.99955
2005
Other
50.782265
2005
Other
54.70072
10
Earth is the largest rocky planet in our solar system. It is colder at night and warmer during the day. No other planet in the solar system has any liquid water on its surface. Much of Earth’s surface is covered with water.
The atmosphere is a layer of gas. Earth has a different atmosphere than other planets have. The atmosphere is about 150 kilometers (93 miles) thick. The gases in the atmosphere block some of the Sun’s harmful rays. Some of these gases are nitrogen, oxygen, and carbon dioxide. Plants and animals need water and these gases to live. Earth is the only planet in the solar system that is known to support life.
Earth rotates around its axis every twenty-four hours. Half of Earth is always in darkness.
Distance from the Sun: 149,600,000 km (93,000,000 mi) Diameter: 12,756 km (7,926 mi) Length of a day as measured in Earth time: 24 hours Length of a year as measured in Earth time: 365 days Average surface temperature: 15°C (59°F) Number of moons: 1 Weight of a child who is 75 lb on Earth: 75 lb
Earth
11
The Moon An astronaut walks on the Moon.
A moon is a natural satellite of a planet. A satellite is an object that travels around another object in space. Moons orbit planets, just as planets orbit the Sun. Gravity keeps moons traveling in orbits around planets.
Earth’s moon is about one-fourth the size of Earth. The Moon has no air, water, or atmosphere.
The country that was known as the Soviet Union sent the fi rst man-made satellite, called Sputnik 1, into space in 1957. In 1961, a Soviet cosmonaut named Yuri Gagarin became the fi rst person in space. In 1969, Americans Neil Armstrong and Buzz Aldrin were the fi rst people to walk on the Moon.
Distance from Earth: 385,000 km (239,000 mi) Diameter: 3,475 km (2,159 mi) Time it takes to travel around Earth: 27.3 days Range of temperatures: –233°C to 123°C (–387°F to 253°F) Weight of a child who is 75 lb on Earth: 12 lb
Facts about Earth’s Moon
2005
Other
61.335976
2005
Other
57.887733
2005
Other
62.06742
2005
Other
46.654823
12
Astronomers have nicknamed Mars the “Red Planet.” The rocks and dirt that cover the surface of Mars contain a mineral called iron oxide. Iron oxide is rust. Mars and the dust that swirls around it are a rusty, red color.
Mars has two moons called Phobos and Deimos. Phobos is very close to Mars. It is only about 6,000 km (3,700 mi) away from Mars. That is much closer than the Moon is to Earth. Earth’s moon is 385,000 km (239,000 mi) from Earth.
The atmosphere on Mars has very little oxygen. No plants or animals that need oxygen to live could survive on Mars. Strong winds can cause huge dust storms. The red dust that covers the planet is blown around. Reddish-pink clouds often surround the entire planet.
Distance from the Sun: 227,900,000 km (141,600,000 mi) Diameter: 6,794 km (4,222 mi) Length of a day as measured in Earth time: 25 hours Length of a year as measured in Earth time: 687 days Average surface temperature: –63°C (–81°F) Number of moons: 2 Weight of a child who is 75 lb on Earth: 28.5 lb
Mars
13
Opportunity
Ice caps cover small areas on Mars. There are also many volcanoes and canyons on Mars. The Valles Marineris canyon is more than 4,000 km (1,864 mi) long. That’s about the same as the distance from New York City to Los Angeles.
The fi rst space probe to land on Mars was called Viking I. In 2004, two vehicles called Spirit and Opportunity landed on Mars. These robotlike machines gathered samples, such as dirt and rocks, and sent information about them back to Earth.
2005
Other
78.99415
2005
Other
52.506386
2005
Other
47.12504
Jupiter, Saturn, And Uranus
Jupiter is the largest planet in the solar system. It is a gas giant. This means that it is made mostly of gas, not rock. Space probes have fl own by Jupiter to get information. However, they are not able to land on Jupiter. It does not have any solid surface.
The gases in Jupiter’s atmosphere are mostly hydrogen and helium. Jupiter’s atmosphere has a weather system called the Great Red Spot. This huge storm has been going on for more than three hundred years! Jupiter has rings around it, but they are too thin and dark to be seen from Earth.
Great Red Spot
Distance from the Sun: 778,400,000 km (484,000,000 mi) Diameter: 142,984 km (88,846 mi) Length of a day as measured in Earth time: 10 hours Length of a year as measured in Earth time: 12 years Average surface temperature: –148°C (–234°F) Number of moons: at least 63 Rings: yes Weight of a child who is 75 lb on Earth: 160.5 lb
Jupiter
Jupiter’s largest moons are Io, Europa, Ganymede, and Callisto.
They are about the same size as Earth’s moon.
Io has many active volcanoes. They give off a gas that appears as different shades of yellow, orange, and green.
The surface of Europa is a frozen crust that is several miles thick. Scientists believe that an ocean of saltwater might lie under this crust.
Ganymede is the largest moon in the solar system. It is even bigger than Mercury and Pluto.
Callisto is covered with craters. Scientists think that there might be a frozen ocean far below its rocky crust.
Colorful yellow, orange, red, and white clouds swirl around Jupiter.
Io
Europa
Ganymede
Callisto
15
2005
Other
56.633827
2005
Other
55.588905
2005
Other
52.506386
16
Saturn is a gas giant made of mostly hydrogen and helium. Saturn is a very large planet—only Jupiter is larger. It is a gigantic ball of gases that contains very little solid matter.
Saturn is surrounded by rings. In 1981, the Voyager space probe collected information about the particles that make up the rings. These particles can be as small as grains of sand or as large as boulders. They are probably made of ice, dust, and chunks of rock.
Saturn
Galileo thought Saturn had handles when he fi rst saw it through his telescope. The handles were the colorful rings that surround Saturn.
Galileo’s Handles
Facts about Saturn Distance from the Sun: 1,426,700,000 km (885,900,000 mi) Diameter: 120,536 km (74,897 mi) Length of a day as measured in Earth time: 11 hours Length of a year as measured in Earth time: 29 years Average surface temperature: –178°C (–288°F) Number of moons: at least 33 Rings: yes Weight of a child who is 75 lb on Earth: 55.5 lb
17
Rhea
Astronomers have discovered that Saturn has at least thirty-three moons. Some are small chunks of ice with odd shapes, such as Pan and Atlas. Others are medium-sized round balls, such as Dione and Rhea. Titan, Saturn’s largest moon, is even larger than Mercury and Pluto. Titan is the only moon in the solar system that has an atmosphere.
Saturn’s rings are made of billions of particles
that travel in orbits around the planet.
Titan
Atlas
2005
Other
59.507362
2005
Other
58.514687
2005
Other
34.63822
18
Uranus was the fi rst planet discovered using a telescope. This planet is a gas giant. Its atmosphere is made of mostly hydrogen, helium, and methane. Uranus is so cold that the methane in the atmosphere is a liquid. Tiny drops of methane form clouds that surround the planet. These clouds make Uranus a fuzzy blue-green color.
The rings of Uranus are dark and diffi cult to see from Earth even with powerful telescopes. In fact, astronomers didn’t know that Uranus had rings until they were discovered by a space probe in 1977.
Uranus travels around the Sun on its side. Scientists think that an object as large as Earth might have crashed into the planet when the solar system was still forming. This might have knocked Uranus onto its side.
Uranus is nearly 2 billion miles away from the Sun. The cameras on Voyager 2 had to be adjusted to take photographs in such dim light.
Uranus
19
The Moons of Uranus Scientists know that Uranus
has at least twenty-seven moons. More may be discovered in the future. Voyager 2 is the only space probe to fl y near Uranus. When it fl ew past the planet in 1986, it discovered ten small moons that astronomers had not known about. The moons are all small to medium-sized. The larger moons have deep valleys and craters.
Facts about Uranus Distance from the Sun: 2,871,000,000 km (1,784,000,000 mi) Diameter: 51,118 km (31,763 mi) Length of a day as measured in Earth time: 17 hours; spins backward Length of a year as measured in Earth time: 84 years Average surface temperature: –216°C (–357°F) Number of moons: at least 27 Rings: yes Weight of a child who is 75 lb on Earth: 64.5 lb
Miranda
Arial
Oberon
2005
70.94885
2005
Other
11.807377
2005
34.324745
2005
59.193886
20
Neptune, Pluto, And Beyond
Neptune is the smallest of the gas giants, but it’s still enormous. If it were hollow, sixty objects the size of Earth could fi t inside! Neptune can’t be seen without a telescope.
The force of gravity between the Sun and the outer planets is weaker than the force of gravity among the Sun and the inner planets. Since Neptune is so far away from the Sun, its orbit is very long. It takes more than one hundred Earth years for Neptune to circle the Sun one time.
Neptune is very windy. Neptune’s winds blew a huge storm called the Great Dark Spot across the planet.
Distance from the Sun: 4,498,300,000 km (2,795,000,000 mi) Diameter: 49,528 km (30,775 mi) Length of a day as measured in Earth time: 16 hours Length of a year as measured in Earth time: 165 years Average surface temperature: –214°C (–353°F) Number of moons: at least 13 Rings: yes Weight of a child who is 75 lb on Earth: 82.5 lb
Neptune
21
The Moons of Neptune Triton
In the 1800s, British astronomer John Couch Adams noticed that Uranus’s orbit was not following the path he thought it should. He thought that the force of gravity between Uranus and another, undiscovered planet might be the cause.
At the same time, a man named Urbain Leverrier calculated the location and size of the other planet. In 1846, an astronomer named Johann Galle pointed his telescope where Leverrier predicted the planet would be. There was Neptune!
Neptune has at least thirteen moons. The largest is called Triton. Astronomers think that Triton may have formed farther away from the Sun and was grabbed by Neptune’s gravity.
On Neptune, the methane gas in the atmosphere makes the planet look very blue.
Great Dark Spot
2005
Other
55.53666
2005
58.72367
2005
Other
42.579628
2005
Other
23.771372
22
Pluto is the planet farthest from the Sun. It is the only outer planet that is not a gas giant. Its surface is icy and solid. Pluto is the smallest planet in the solar system. It’s even smaller than our own moon.
Pluto has one moon. It is called Charon. Charon is very close to Pluto and is only slightly smaller. This makes many astronomers think of them as a double planet system. Astronomers also believe that Pluto and Charon may share the same atmosphere when their orbits bring them closest to the Sun.
Distance from the Sun: 5,906,300,000 km (3,670,000,000 mi) Diameter: 2,302 km (1,430 mi) Length of a day as measured in Earth time: 6 days; spins backward Length of a year as measured in Earth time: 248 years Average surface temperature: –233°C (–387°F) Number of moons: 1 Weight of a child who is 75 lb on Earth: 6 lb
Facts about Pluto
23
Sedna
Look at the diagram above. The other planets all travel around the Sun at the same angle. Pluto’s orbit is tilted. It takes 248 years for Pluto to travel around the Sun. For twenty of those years, Pluto is closer to the Sun than Neptune. This won’t happen again until the year 2237.
Is Sedna the tenth planet? Sedna was fi rst seen in 2003. It is the largest object discovered in the solar system since Pluto was spotted in 1930. Sedna is about 84 billion miles away from the Sun. Because of that great distance, it has a temperature of –240°C. Sedna is red, just as Mars is. Sedna is not the only object that astronomers have seen beyond Pluto. However, all the others seem to be too small to be planets.
Spacecraft have landed on or passed by every planet up to Pluto. Space probes might land on Pluto one day. Will that be the end of our exploration? Probably not. With perhaps 50 billion solar systems in the Milky Way alone, it seems that space exploration has only just begun!
Pluto’s orbit
2005
Other
48.065468
2005
Other
54.85746
2005
Other
102.45089
24
and other objects in space
craters bowl-shaped dents on the surface of planets and their moons
galaxy a system of billions of stars, gases, and dust
satellite an object that travels around another object in space
solar system a system that includes the Sun, the planets, their moons, and other objects
space probe a vehicle that carries cameras and other tools for studying objects in space
universe all of space and everything in it
1. How are the orbits of the inner planets different from the orbits of the outer planets?
2. Why is it diffi cult to study Venus?
3. What makes Pluto’s orbit different from all the other planets?
4. Gravity is the force that holds the solar system together. Write to explain what effect gravity has between the Sun and the planets, and between the planets and their moons. Use details from the book to support your answer.
5. Predict Do you think scientists will fi nd other planets in the solar system? Explain your prediction.
What did you learn?Vocabulary
astronomy craters galaxy satellite solar system space probe universe
Picture Credits Every effort has been made to secure permission and provide appropriate credit for photographic material. The publisher deeply regrets any omission and pledges to correct errors called to its attention in subsequent editions.
Photo locators denoted as follows: Top (T), Center (C), Bottom (B), Left (L), Right (R), Background (Bkgd).
Opener Brand X Pictures; 2 (T) ©Myron Jay Dorf/Corbis; 3 Getty Images; 7 (T) Brand X Pictures; 10 (TL, BR) Brand X Pictures; 11 (BR) Getty Images; 13 (TR) Getty Images, (BR) ©JPL/NASA; 14 (TR) Getty Images; 16 (TR) Getty Images; 17 (TR) Getty Images, (CR, BR) Calvin J Hamilton/©Galaxy Picture Library; 23 (CR) NASA/JPL-Caltech/©Galaxy Picture Library.
Scott Foresman/Dorling Kindersley would also like to thank: 1, 2 (B) NASA/JPL/DK Images; 6 (TL) NASA/DK Images, (TR) NASA/Finley Holiday Films/DK Images; 9 (TR) NASA/DK Images; 11 (T) NASA/DK Images; 12 NASA/DK Images; 15 (CL, BL) Jet Propulsion Lab/DK Images; 19 (TR, CL) Jet Propulsion Lab/DK Images; 21 (BR) NASA/JPL/DK Images.
Unless otherwise acknowledged, all photographs are the copyright © of Dorling Kindersley, a division of Pearson.
ISBN: 0-328-13911-4
Copyright © Pearson Education, Inc. All Rights Reserved. Printed in the United States of America. This publication is protected by Copyright, and permission should be obtained from the publisher prior to any prohibited reproduction, storage in a retrieval system, or transmission in any form by any means, electronic, mechanical, photocopying, recording, or likewise. For information regarding permission(s), write to Permissions Department, Scott Foresman, 1900 East Lake Avenue, Glenview, Illinois 60025.
3 4 5 6 7 8 9 10 V010 13 12 11 10 09 08 07 06 05
13911_01-04_CVR_FSD.indd Cover213911_01-04_CVR_FSD.indd Cover2 5/12/05 8:42:20 PM5/12/05 8:42:20 PM
previous:
next:

Scott Foresman Science - Plain Local Schools

Documents

Transcript of Scott Foresman Science - Plain Local Schools