Contents. Section 1: The Sun s Energy. Section 2: The Solar System. Section 3: The Moon

Similar documents
Planet Power. Of all the objects in our solar system, eight match these requirements: Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, & Neptune

The Outer Planets (pages )

Unit 2 Lesson 1 What Objects Are Part of the Solar System? Copyright Houghton Mifflin Harcourt Publishing Company

Voyage to the Planets

known since prehistoric times almost 10 times larger than Jupiter

Exploring The Planets: Jupiter

The Outer Planets. Video Script: The Outer Planets. Visual Learning Company

After you read this section, you should be able to answer these questions:

Motion of the planets

Directed Reading B. Section: The Outer Planets

Chapter 29. The Solar System. The Solar System. Section 29.1 Models of the Solar System notes Models of the Solar System

Inner and Outer Planets

Inner and Outer Planets

STUDENT RESOURCE 1.1 INFORMATION SHEET. Vocabulary

Uranus, Neptune, and Pluto. Outer Worlds 4/19/07

Our Solar System. Lesson 5. Distances Between the Sun and the Planets

The Sun s center is much hotter than the surface. The Sun looks large and bright in the sky. Other stars look much smaller.

Starting from closest to the Sun, name the orbiting planets in order.

What Objects Are Part of the Solar System?

The Solar System. Name Test Date Hour

Name Date Class. Earth in Space

Greeks watched the stars move across the sky and noticed five stars that wandered around and did not follow the paths of the normal stars.

Earth & Space Science ~ The Solar System

Chapter 3 The Solar System

Traveler s Guide to the Planets Uranus & Neptune

The Inner Planets. Chapter 3 Lesson 1. Pages Workbook pages 51-52

When you have completed this workbook, you should know and understand the following:

Earth, Uranus, Neptune & Pluto

The Solar System LEARNING TARGETS. Scientific Language. Name Test Date Hour

Sun Mercury Venus. Earth Mars Jupiter

A medium-sized star. The hottest object found in our solar system.

Unit 12 Lesson 1 What Objects Are Part of the Solar System?

The Planet Pluto. & Kuiper Belt. The Search for PLANET X Pluto Discovered. Note how Pluto Moved in 6 days. Pluto (Hades): King of the Underworld

Unit 3 Lesson 5 The Gas Giant Planets. Copyright Houghton Mifflin Harcourt Publishing Company

Astronomy. Uranus Neptune & Remote Worlds

Our Solar System and Its Place in the Universe

Physical Science 1 Chapter 16 INTRODUCTION. Astronomy is the study of the universe, which includes all matter, energy, space and time.

The Outermost Planets. The 7 Wanderers known since Antiquity. Uranus and Neptune distinctly Blue-ish!

What is the Solar System?

Unusual Moon Information

Chapter 23. Our Solar System

Object Type Moons Rings Planet Terrestrial none none. Max Distance from Sun. Min Distance from Sun. Avg. Distance from Sun 57,910,000 km 0.

Lesson 1 The Structure of the Solar System

Unit 6 Lesson 4 What Are the Planets in Our Solar System? Copyright Houghton Mifflin Harcourt Publishing Company

1. The Sun is the largest and brightest object in the universe. 2. The period that the Earth takes to revolve once around the Sun is approximately a

Lecture 25: The Outer Planets

Unit 1: The Earth in the Universe

What s in Our Solar System?

1781: Uranus Discovered. The Outer Worlds. 1846: Neptune Discovered. Distance Comparison. Uranus Rotates Sideways. Exaggerated Seasons On Uranus

UNIT 1: THE UNIVERSE VOCABULARY

Our Planetary System. Chapter 7

SPI Use data to draw conclusions about the major components of the universe.

Chapter 23: Touring Our Solar System

Chapter 7 Our Planetary System

Read each slide then use the red or some underlined words to complete the organizer.

Chapter 15 & 16 Science Review (PATTERNS IN THE SKY, OUR SOLAR SYSTEM)

1. thought the earth was at the center of the solar system and the planets move on small circles that move on bigger circles

Classifying the Solar System

CHAPTER 2 Strand 1: Structure and Motion within the Solar System

It Might Be a Planet If...

The Solar System. Sun. Rotates and revolves around the Milky Way galaxy at such a slow pace that we do not notice any effects.

SOLAR SYSTEM. planet feature cards

Chapter 06 Let s Make a Solar System

UNIT 1: EARTH AND THE SOLAR SYSTEM.

Solar System Research Teacher Notes The Sun

How did it come to be this way? Will I stop sounding like the

Sol o ar a r S yste t m e F o F r o m r at a i t on o The Ne N b e u b l u a a Hypothesis

The Solar System. Presented By; Rahul Chaturvedi

Announcement Test 2. is coming up on Mar 19. Start preparing! This test will cover the classes from Feb 27 - Mar points, scantron, 1 hr.

ALL ABOUT THE PLANETS

Dwarf Planets and Other Objects

9.2 - Our Solar System

A. The moon B. The sun C. Jupiter D. Earth A. 1 B. 2 C. 3 D. 4. Sky Science Unit Review Konrad. Here is a selection of PAT style questions.

Uranus and Neptune. Uranus and Neptune Properties. Discovery of Uranus

Earth Science. Unit 9: Our Place in the Universe

What is in outer space?

ASTR-1010: Astronomy I Course Notes Section X

The Moon s relationship with Earth The formation of the Moon The surface of the Moon Phases of the Moon Travelling to the Moon

Saturn and Planetary Rings 4/5/07

Earth, Uranus, Neptune & Pluto. 14a. Uranus & Neptune. The Discovery of Uranus. Uranus Data: Numbers. Uranus Data (Table 14-1)

Outline. Question of Scale. Planets Dance. Homework #2 was due today at 11:50am! It s too late now.

4 A(n) is a small, rocky object that orbits the sun; many of these objects are located in a band between the orbits of Mars and Jupiter.

UNIT 3: Chapter 8: The Solar System (pages )

Name: Date: Hour: 179 degrees celsius. 5% of Earth A 70 pound person would weigh 27 pounds on Mercury.

Lecture 16 Dwarf Planets and Comets January 8a, 2014

Planetarium observing is over. Nighttime observing starts next week.

CVtpf 2-1. Section 1 Review. 3. Describe How did the process of outgassing help shape Earth's atmosphere?

Investigating Astronomy Timothy F. Slater, Roger A. Freeman Chapter 7 Observing the Dynamic Giant Planets

Ch 23 Touring Our Solar System 23.1 The Solar System 23.2 The Terrestrial Planet 23.3 The Outer Planets 23.4 Minor Members of the Solar System

PLANETS OF OUR SOLAR SYSTEM

At this point of its orbit, any solar satellite such as a comet or a planet is farthest away from the sun. What is the aphelion?

Edmonds Community College ASTRONOMY 100 Sample Test #2 Fall Quarter 2006

of stars constellations. Perhaps you have seen The Big Dipper, Taurus the bull, Orion the hunter, or other well-known star groups.

Mercury Named after: Mercury, the fast-footed Roman messenger of the gods. Mean Distance from the Sun: 57,909,175 km (35,983,093.1 miles) or 0.

Chapter 23 Earth Science 11

Astronomy November, 2016 Introduction to Astronomy: The Solar System. Mid-term Exam 3. Practice Version. Name (written legibly):

Space Science Jeopardy!

Does it matter what you call an object? Does the public care so much? Were scientists made fun of, but not HP Computer Company?

Astronomy Test Review. 3 rd Grade

Activity 12: Solar System

Transcription:

Contents Section 1: The Sun s Energy 1. Earth s Powerhouse.... 3 2. Our Nuclear Furnace.... 7 3. Quiz 1.... 10 Section 2: The Solar System 4. Mercury, Venus, and Earth... 12 5. Mars and the Asteroid Belt.... 17 6. The Gas Giants: Jupiter and Saturn... 21 7. Uranus, Neptune, and... 25 8. Comets.... 30 9. Quiz 2.... 34 Section 3: The Moon 10. The Surface of the Moon and Its Phases.... 35 11. Rotation and Revolution.... 40 12. Tides.... 43 13. Eclipses.... 46 14. Build a Model of the Solar System.... 51 15. Self Check.... 54 16. LightUnit Test........................................ 57

Uranus, Neptune, and Vocabulary Words aphelion (a fēl yən): the point farthest from the sun in the orbit of a planet perihelion (per ə hēl yən): the point nearest the sun in the orbit of a planet Pronounce these words to someone. Uranus Uranus was discovered by Sir William Herschel in 1781 as he was looking through his large reflecting telescope. He named this planet George s Star in honor of his king. In our imaginary trip we just zipped up here from one planet to another in a short time. In August of 1977 the space probe Voyager 2 left Cape Canaveral, Florida, and reached Uranus in January of 1986. It took 8 ½ years to reach the planet! That should give you some idea of the immense distances between planets. On Uranus, we re 2.87 billion kilometers (1.78 billion miles) from the Sun. Though Uranus is smaller than Jupiter and Saturn, it is still a giant. Its diameter is four times larger than Earth s. Our day up here will be about 17 hours and 14 minutes, but I m sure you won t want to stay a year. A year on Uranus is equal to 84 earth-years. If you lived up here, you d have only one birthday during your entire life. Uranus is tilted so far that it actually lies on its side as it rotates. This tilt causes its poles to receive dim sunlight for 42 years and then darkness for 42 years. Surface gravity on Uranus is 0.89 g and its mass is 14.5 times that of Earth. By 1948 astronomers had discovered five large moons orbiting Uranus. When Voyager 2 flew past the planet in 1986, it found ten more moons. They are small 10 to 12 miles in diameter, sooty black moons in a black sky. The moons of Uranus are outstanding because of their great variety of surfaces. There are craters, high rocky mountains, icy canyons, and long valleys. Further investigation of Uranus moons since the flyby of Voyager 2 has brought the number of moons to twenty-seven. Uranus appears blue-green through its cloud cover. Clouds circle Uranus with winds of up to 900 km (560 miles) per hour. These clouds indicate there is some kind of weather on Uranus, but only God knows what kind! Uranus Orbital Distance: 2.87 billion km Length of Day: 17 hr 14 min Length of Year: 84 years Diameter: 50,700 km Surface Gravity: 0.89 g Avg. Temperature: 197.2 C Moons: 27 Uranus rotates on its side and has faint rings. Wikimedia Commons/NASA/JPL/STScl 25

Voyager 2 discovered Uranus has narrow rings. They are made up of small dark particles. Such marvelous exploration of a planet almost two billion miles away was possible because of God s perfect timing of the universe and His gift of knowledge to man. Neptune Neptune was discovered using mathematics and a telescope. An English astronomer, John Adams, and a French astronomer, Urbain Le Verrier, used mathematical calculations to predict where another planet should exist. In 1848 Galle, a German astronomer, used a telescope to locate this planet within one degree of where Le Verrier had predicted it would be! Neptune Orbital Distance: 4.5 billion km Length of Day: 16 hr 6 min Length of Year: 165 years Diameter: 49,200 km Surface Gravity: 1.14 g Avg. Temperature: 210 C Moons: 14 The Great Dark Spot can be seen in this picture of Neptune taken by Voyager 2. Wikimedia Commons/NASA/JPL Voyager 2 came near Neptune in August of 1989. It sent back thousands of pictures of the planet. Scientists were surprised to see rings around Neptune. The pictures also showed six previously unknown moons, and a large storm in Neptune s atmosphere called the Great Dark Spot. Neptune has the strongest winds in the solar system. Voyager 2 measured the winds in the Great Dark Spot at 2,400 kilometers (1,500 miles) per hour! Neptune makes one rotation in approximately 16 hours. It revolves around the sun once every 165 years. What a long year! You couldn t even live long enough to celebrate one birthday out here. We re a long way from the sun 4.5 billion kilometers (2.79 billion miles)! The temperature here is around 210 C ( 340 F). Burr! I m ready to leave this cold, lifeless place. How about you? This dwarf planet is farther away from the sun than any planet. It is an average distance of 5.90 billion kilometers (3.66 billion miles) from the sun. This is 39.5 times the distance from the sun to the earth! Its aphelion is 7.31 billion kilometers (4.53 billion miles) and its perihelion is 4.44 billion kilometers (2.75 billion miles). At its nearest point to the sun, actually comes inside Neptune s orbit. But most of the time s very elliptical path is beyond Neptune s orbit. The orbit of is different in another way. When compared to the orbits of the planets, the orbit of is tilted. Because it orbits so far from the sun, takes around 248 years to make one complete revolution. was discovered in 1930 by the young astronomer Clyde Tombaugh. As he looked through photographs of the night sky, he noticed that one of the bright dots on a series of photos seemed to move. After further measurements confirmed his finding, it was announced that Clyde had found the ninth planet! 26

Orbital Distance: 5.90 billion km Length of Day: 6.4 days Length of Year: 248 years Diameter: 2,370 km Surface Gravity: 0.063 g Avg. Temperature: 229 C Moons: 5 Later investigations with more powerful telescopes, including the Hubble Space Telescope, showed that has a total of five moons. The largest, Charon (ker ən), is just over half the size of. For many years was considered a planet. However, in 2006, an international group of astronomers decided to downgrade from a planet to a dwarf planet. This decision was reached because was too small and did not meet all the conditions required to be a planet. s diameter is only two-thirds that of our Moon. In 2015 the New Horizons space probe flew by. It took pictures and measurements as it sped past the dwarf planet at 49,600 kilometers (30,800 miles) per hour. Scientists were finally able to clearly see the object that had once been only a blur in their best telescopes. They found that had a relatively smooth surface with few craters, and 11,000 foot-high mountains of ice. s average temperature is estimated to be 229 C ( 373 F). It s no place for us! Let s head back to Earth! Mercury Venus Earth Mars Jupiter A picture of taken by New Horizons. Saturn s orbit is tilted compared to the planets. Neptune Uranus Wikimedia Commons/NASA/JHUAPL/SwRI Study Exercises Answer the questions. 1. Who discovered Uranus? 2. What is unusual about the tilt of Uranus? 3. How was discovered? 27

Circle the letters of the answers. 4. What were the two reasons was downgraded to a dwarf planet? a. It was too small. b. Its orbit was different than the rest of the planets. c. It did not meet the required conditions for planets. d. It was hard to study because it is so far from earth. Use the words and numbers to complete the statements. One answer will be used twice. Charon Galle Adams Le Verrier Voyager 2 8 27 165 5. It took Voyager 2 over years to reach Uranus. 6. Uranus has moons. 7. Neptune s location was predicted by and using mathematical calculations. 8. The astronomer discovered Neptune very close to its predicted location. 9. The spacecraft visited Neptune in 1989. 10. Neptune circles the sun once every years. 11. The orbit of is tilted. 12. s moon is just over half the size of. 13. The diameter of is about two-thirds the size of our Moon. Write true if the statement is true and false if it is false. Correct any false statements. 14. The unusual tilt of Uranus causes its poles to have 52 years of light. 15. Uranus has faint, narrow rings. 16. Uranus has the strongest winds in the solar system. 17. The Great Dark Spot is a storm on Neptune. 18. The New Horizons space probe flew past. 28

Looking Back Underline the correct choice. 19. It takes Jupiter 12, 24 years to orbit the sun. Lesson 7 20. The Great Red Spot is a large storm, crater on Jupiter. 21. The largest planet in the solar system is Mars, Jupiter. 22. Jupiter s moon Ganymede, Ceres is larger than Mercury. 23. Saturn has large, beautiful moons, rings made of ice and rock. 24. Jupiter appears slightly flattened because of how fast it revolves, rotates. 25. Jupiter s surface gravity is 2.53 g, which means its gravity is greater, less than Earth s gravity. 26. Saturn and Jupiter are known as the gas giants, giant storms because they are large and covered in gas. Complete the activity. 27. Record the moon phase on page 39. Did You Know? s moon Charon has a canyon that is about as deep as Mount Everest is high. There are estimated to be at least ten more dwarf planets out beyond the orbit of. Neptune s moon Triton orbits clockwise around Neptune. This is the opposite direction of every other large moon in the solar system. 29