Physics Homework Set 3 Fall 2015

Size: px
Start display at page:

Download "Physics Homework Set 3 Fall 2015"

Transcription

1 1) Mercury presents the same side to the Sun 1) A) every third orbit. B) every 12 hours. C) all the time, just like our Moon. D) every other orbit. E) Twice every orbit. 2) Both the Moon and Mercury are geologically inactive and have been that way for most of the history of the solar system. However, about 4 billion years ago, it is thought that 2) A) both bodies were covered in ice. B) the Moon differentiated. C) Mercury had more common volcanic activity than the Moon. D) the Moon had more frequent and violent volcanic activity than Mercury. E) the Moon's atmosphere dissipated. 3) Evidence of liquid water in Mars' distant past suggests that it had a substantial atmosphere compared to what it has presently. What happened to its water vapor? 3) A) The carbon dioxide in its atmosphere dissolved in the water and combined with surface rocks. B) Its atmosphere was mostly hydrogen and helium. Mars' gravity is too weak to hold them. C) Mars initially had such a large Greenhouse effect that the atmosphere became quite hot and slowly escaped. D) It has now all been lost in space, including the carbon dioxide and water vapor. E) The atmosphere has frozen out into the polar ice caps and permafrost as Mars has cooled. 4) Compare the atmospheres of Mars and Venus. 4) A) Both are made of hydrogen and helium, like the jovians. B) Both are chiefly carbon dioxide, but at Mars it can freeze as dry ice. C) Mars is rich in oxygen, like ours, accounting for its red surface. D) Both are too hot for water to now exist as a liquid at the surface. E) Like Earth, nitrogen is the chief atmospheric gas. 5) What is true of the lunar highlands? 5) A) They are less heavily cratered than the mare. B) They are the darker regions of the Moon seen with the naked eye. C) They are found on the Moon's northern hemisphere. D) They are younger than the darker mare. E) They are the oldest part of the lunar surface.. 6) The youngest features visible with telescopes on the Moon are:6) A) the darkest regions of the mare. B) the craters sitting atop the mare. C) the bright polar caps of new ice. D) the scarps recently created by tectonic activity. E) the volcanoes seen erupting in the highlands. 7) What is the result of the Greenhouse effect on the surface environment of Venus? 7) A) It has raised the surface temperature by hundreds of degrees Celsius B) It causes the surface temperature of Venus to become hotter than the Sun. C) Its effect is about the same as on Earth

2 D) It has little or no effect. E) It has reduced the surface temperature by about 30 degrees Celsius. 8) The NASA missions that landed on Mars in 1976 were the 8) A) the Galileo probe. B) Venera 14. C) Vikings I and II. D) Magellan lander. E) Voyagers. 9) The synodic period of Venus is about how many Earth years? 9) A) about 2 years B) about 5 years C) about 1.25 years D) about 0.7 years E) about 3.5 years 10) Astronomers believe that the Moon did not differentiate to the same degree as Earth because: 10) A) the Moon was formed after the Earth was, so its radioactivity was less. B) the Moon was made of very different materials than our mantle and crust. C) the less dense and smaller moon did not have as much radioactivity as the larger Earth in its core. D) the meteors that hit the moon were lighter than those that hit us, so did not generate as much heat on the surface. E) the Moon was made of solid debris, not liquids like our hydrosphere. 11) The highest peak on Venus is called: 11) A) Cleopatra. B) Lakshmi. C) Shif. D) Gula. E) Maxwell. 12) Our most detailed maps of Venus come from: 12) A) Earth based radio telescopes. B) manned landings. C) direct observation from Earth based optical telescopes. D) the Magellan spaceprobe. E) the Hubble Space Telescope. 13) What physical feature of Mars are atypical compared with the other terrestrial planets? 13) A) its surface composition B) its atmospheric content C) its density D) its rotation rate E) its size 14) Which of these would support the capture theory of the Moon's origin? 14) A) the four large moons of Jupiter orbit its equator B) the Caloris basin on Mercury C) the retrograde orbit and large orbital inclination of Neptune's moon Triton D) the rings of all the jovians lying around their equators E) the Pluto-Charon system 15) Olympus Mons and Maxwell Mons are both 15) A) sheild volcanoes. B) features visible from Earth

3 C) dormant volcanoes. D) large features on the surface of Mars. E) the two largest known volcanoes in the solar system. 16) Venus is only a little bit (5%) smaller than Earth, and its density is only slightly less than Earth's. Therefore, its mass is: 16) A) just a little bit less than Earth's. B) much less than Earth's (more than 20% different). C) much greater than Earth's (more than 20% different). D) the same as Earth's. E) just a little bit greater than Earth's. 17) The orbiter that gave us the most detailed maps of Venus to date was:17) A) Pioneer 11. B) Cassini. C) Magellan. D) Venera 14. E) Galileo. 18) The main constituent of the martian atmosphere is 18) A) carbon dioxide. B) hydrogen. C) helium. D) nitrogen. E) methane. 19) The scarps on Mercury were probably caused by 19) A) meteorite bombardment. B) tectonic activity. C) volcanism. D) the interior cooling and shrinking. E) a tidal bulge. 20) Why was the summer of 2003 a fine time for Mars observers? 20) A) The Mars Rovers returned live images from the surface. B) The skies were unusually clear and calm. C) Mars was even brighter than Venus for several weeks. D) Mars' north pole was tilted to face the Earth head-on. E) Mars was closer to us than it has been in over 50,000 years. 21) Which statement about the rotations of the Moon and Mercury is FALSE? 21) A) Like our Moon, Mercury does not rotate at all, keeping the same side facing the Sun. B) Our Moon is in a 1:1 synch with the Earth, keeping the same side toward us. C) Mercury is in the 3:2 synch with the Sun, with the same side Sunward at perihelion. D) On Mercury, three days exactly equal two years. E) On the Moon, each "day" lasts about 15 earth days of constant sunlight. 22) Volcanic activity on Venus is thought to be: 22) A) the same as volcanic activity on Earth. B) more frequent and more violent than volcanic activity on Earth

4 C) less frequent and less violent than volcanic activity on Earth. D) less frequent, but more violent than volcanic activity on Earth. E) more frequent, but less violent than volcanic activity on Earth. 23) Mars is best viewed from Earth when it is at 23) A) aphelion. B) opposition. C) perihelion. D) conjunction. E) none of the above 24) Which type of feature is the best evidence of lunar volcanism? 24) A) vents seen erupting in the mountainous highlands B) craters all over the Moon C) rilles associated with lava flows accompanying the mare formation D) the Orientale Basin E) rays around the latest eruptions 25) Venus' full phase occurs when Venus is at: 25) A) the deferent. B) opposition. C) conjunction. D) inferior conjunction. E) superior conjunction. 26) In size, Mercury is intermediate between: 26) A) Pluto and the Moon. B) the Moon and Mars. C) Mars and Earth. D) Earth and Venus. E) Ceres and Pluto. 27) Why is Mars red? 27) A) Dust storms on the planet have blasted the planet so fiercely that the rocks have reddened. B) The ancient volcanoes poured out vast plains of molten sulfur, much as on Io, which has now solidified and preserved the reddish color. C) Mercuric oxide is abundant and has a red tint. D) The iron in the surface rocks have been oxidized over time. E) Sulfuric acid rain etched a reddish color into iron-rich surface rocks. 28) Because the atmosphere of Venus is so dense, 28) A) clouds cannot form. B) clouds form at an altitude much lower than on Earth. C) clouds form at the same altitude as on Earth. D) clouds form at an altitude much higher than on Earth. E) clouds are made of frozen carbon dioxide ice crystals. 29) The surface of Venus can be observed with: 29) A) the Mt. Wilson 100" telescope. B) the Hubble Space Telescope. C) most amateur telescopes

5 D) radar observations from Arecibo. E) All of these have provided detailed observations about the surface of our sister planet. 30) Which statement about Mars' two moons is FALSE? 30) A) Both are probably captured asteroids. B) Both are very dark, heavily cratered bodies. C) Both are in retrograde orbits. D) Phobos revolves around Mars in less than a Martian day. E) Phobos is larger than Deimos. 31) The atmospheric pressure on Venus: 31) A) is about the same as on Mercury. B) causes variations in surface temperature. C) is much higher than on Earth. D) shows an extreme change with the seasons. E) is much lower than on Earth. 32) The lunar mare are radioactively dated at: 32) A) billion years old, forming after most of the bombardment was over. B) 4.6 billion years old, forming first among the lunar features. C) billion years old, comparable to the adjacent highlands. D) less than a billion years old, the most recent additions to the Moon. E) billion years old, similar to the formation of our own oceans. 33) What property of Mars is responsible for producing the great heights of its volcanos? 33) A) Its cold temperatures allows the magma to freeze faster. B) Mars has more radioactive material than the Earth. C) Its higher surface gravity allows higher peaks to form. D) Its volcanoes are made of sulfur, like Io's. E) Its thick crust can support larger peaks, and lower surface gravity does not pull them down as much as on Earth. 34) What resonance exists between Venus' rotational period and its synodic period? 34) A) 5:1, with the Earth always closest to the same side of Venus when they pass B) 1:2, like the Cassini Division and the Saturnian Moon Mimas C) 1:1, like the Moon D) 3:2, like the planet Mercury E) There is no apparent match. 35) What is the reason that it is so difficult to view Mercury from Earth? 35) A) Mercury is very dim. B) Mercury is very small. C) Mercury is always very close to the Sun. D) Mercury can't be seen at night. E) Mercury is often hidden by the Moon. 36) What do moonquakes reveal about the Moon? 36) A) It has a differentiated core, displaced away from us by the Moon's rotation. B) It has a strong magnetic field generated by a large molten core. C) Its small, partially molten core has been pulled toward us by tidal forces. D) The Moon has been geologically dead throughout its entire history. E) The Moon is quite active, almost as much so as Jupiter's moon Io

6 37) The absence of a magnetic field on Venus probably stems from its: 37) A) high surface temperatures. B) slow rotation. C) extremely thick atmosphere. D) lower density than Earth, suggesting an absence of an iron core. E) nearness to the Sun. 38) The largest volcanic structures on Venus are called: 38) A) shield volcanoes. B) calderas. C) crater cones. D) coronae. E) cinder cones. 39) Which of these features is attributed to the shrinking of Mercury's core? 39) A) rilles B) mare C) rays D) craters E) scarps 40) The deepest depression found on the surface of Mars is the 40) A) Mariannas Trench. B) Caloris basin. C) Mare Crisium. D) Valles Marineris rift, E) Hellas Basin of Mars

Astronomy Ch. 10 Mars Review. MULTIPLE CHOICE. Choose the one alternative that best completes the statement or answers the question.

Astronomy Ch. 10 Mars Review. MULTIPLE CHOICE. Choose the one alternative that best completes the statement or answers the question. Name: Period: Date: Astronomy Ch. 10 Mars Review MULTIPLE CHOICE. Choose the one alternative that best completes the statement or answers the question. 1) Why was the summer of 2003 a fine time for Mars

More information

Astronomy Ch. 8 The Moon and Mercury. MULTIPLE CHOICE. Choose the one alternative that best completes the statement or answers the question.

Astronomy Ch. 8 The Moon and Mercury. MULTIPLE CHOICE. Choose the one alternative that best completes the statement or answers the question. Name: Period: Date: Astronomy Ch. 8 The Moon and Mercury MULTIPLE CHOICE. Choose the one alternative that best completes the statement or answers the question. 1) The best way to find the exact distance

More information

Lecture Outlines. Chapter 10. Astronomy Today 8th Edition Chaisson/McMillan Pearson Education, Inc.

Lecture Outlines. Chapter 10. Astronomy Today 8th Edition Chaisson/McMillan Pearson Education, Inc. Lecture Outlines Chapter 10 Astronomy Today 8th Edition Chaisson/McMillan Chapter 10 Mars Units of Chapter 10 10.1 Orbital Properties 10.2 Physical Properties 10.3 Long-Distance Observations of Mars 10.4

More information

Chapter 17: Mercury, Venus and Mars

Chapter 17: Mercury, Venus and Mars Chapter 17: Mercury, Venus and Mars Mercury Very similar to Earth s moon in several ways: Small; no atmosphere lowlands flooded by ancient lava flows heavily cratered surfaces Most of our knowledge based

More information

Lecture #11: Plan. Terrestrial Planets (cont d) Jovian Planets

Lecture #11: Plan. Terrestrial Planets (cont d) Jovian Planets Lecture #11: Plan Terrestrial Planets (cont d) Jovian Planets Mercury (review) Density = 5.4 kg / liter.. ~ Earth s Rocky mantle + iron/nickel core Slow spin: 59 days (orbital period = 88 days) No satellites

More information

Mercury and Venus 3/20/07

Mercury and Venus 3/20/07 Announcements Reading Assignment Chapter 13 4 th Homework due today Quiz on Thursday (3/22) Will cover all material since the last exam. This is Chapters 9-12 and the part of 13 covered in the lecture

More information

The Solar System 6/23

The Solar System 6/23 6/23 The Solar System I. Earth A. Earth is the prototype terrestrial planet 1. Only planet in the solar system (we know of so far) with life 2. Temperature 290 K B. Physical Characteristics 1. Mass: 6

More information

Overview of Solar System

Overview of Solar System Overview of Solar System The solar system is a disk Rotation of sun, orbits of planets all in same direction. Most planets rotate in this same sense. (Venus, Uranus, Pluto are exceptions). Angular momentum

More information

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

UNIT 3: Chapter 8: The Solar System (pages ) CORNELL NOTES Directions: You must create a minimum of 5 questions in this column per page (average). Use these to study your notes and prepare for tests and quizzes. Notes will be turned in to your teacher

More information

Our Planetary System. Chapter 7

Our Planetary System. Chapter 7 Our Planetary System Chapter 7 Key Concepts for Chapter 7 and 8 Inventory of the Solar System Origin of the Solar System What does the Solar System consist of? The Sun: It has 99.85% of the mass of the

More information

Mars: The Red Planet. Roman God of war Blood Reflects 30% of its incident sunlight 2 small moons : Phobos and Deimos

Mars: The Red Planet. Roman God of war Blood Reflects 30% of its incident sunlight 2 small moons : Phobos and Deimos Mars: The Red Planet Roman God of war Blood Reflects 30% of its incident sunlight 2 small moons : Phobos and Deimos Property Earth Mars Radius 6378km 3394km ~ 0.51R E Mass 5.97x10 24 kg 6.42x10 23 kg =

More information

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

Edmonds Community College ASTRONOMY 100 Sample Test #2 Fall Quarter 2006 Edmonds Community College ASTRONOMY 100 Sample Test #2 Fall Quarter 2006 Instructor: L. M. Khandro 10/19/06 Please Note: the following test derives from a course and text that covers the entire topic of

More information

9. Moon, Mercury, Venus

9. Moon, Mercury, Venus 9. Moon, Mercury, Venus All the heavier elements were manufactured by stars later, either by thermonuclear fusion reactions deep in their interiors or by the violent explosions that mark the end of massive

More information

The Solar System. Tour of the Solar System

The Solar System. Tour of the Solar System The Solar System Tour of the Solar System The Sun more later 8 planets Mercury Venus Earth more later Mars Jupiter Saturn Uranus Neptune Various other objects Asteroids Comets Pluto The Terrestrial Planets

More information

3. The name of a particularly large member of the asteroid belt is A) Halley B) Charon C) Eris D) Ceres E) Triton

3. The name of a particularly large member of the asteroid belt is A) Halley B) Charon C) Eris D) Ceres E) Triton Summer 2013 Astronomy - Test 2 Test form A Name Do not forget to write your name and fill in the bubbles with your student number, and fill in test form A on the answer sheet. Write your name above as

More information

Jupiter. Jupiter is the third-brightest object in the night sky (after the Moon and Venus). Exploration by Spacecrafts

Jupiter. Jupiter is the third-brightest object in the night sky (after the Moon and Venus). Exploration by Spacecrafts Jupiter Orbit, Rotation Physical Properties Atmosphere, surface Interior Magnetosphere Moons (Voyager 1) Jupiter is the third-brightest object in the night sky (after the Moon and Venus). Exploration by

More information

MULTIPLE CHOICE. Choose the one alternative that best completes the statement or answers the question.

MULTIPLE CHOICE. Choose the one alternative that best completes the statement or answers the question. ASTRO 102/104 Prelim 2 Name Section MULTIPLE CHOICE. Choose the one alternative that best completes the statement or answers the question. 1) This is version E of the exam. Please fill in (E). A) This

More information

page - Lab 13 - Introduction to the Geology of the Terrestrial Planets

page - Lab 13 - Introduction to the Geology of the Terrestrial Planets page - Lab 13 - Introduction to the Geology of the Terrestrial Planets Introduction There are two main families of planets in our solar system: the inner Terrestrial planets (Earth, Mercury, Venus, and

More information

MULTIPLE CHOICE. Choose the one alternative that best completes the statement or answers the question.

MULTIPLE CHOICE. Choose the one alternative that best completes the statement or answers the question. ASTRO 102/104 Prelim 2 Name Section MULTIPLE CHOICE. Choose the one alternative that best completes the statement or answers the question. 1) This is version B of the exam. Please fill in (B). A) This

More information

Planets. Chapter 5 5-1

Planets. Chapter 5 5-1 Planets Chapter 5 5-1 The Solar System Terrestrial Planets: Earth-Like Jovian Planets: Gaseous Sun Mercury Venus Earth Mars Jupiter Saturn Uranus Neptune Pluto Inferior Planets Superior Planets Inferior

More information

Terrestrial Atmospheres

Terrestrial Atmospheres Terrestrial Atmospheres Why Is There Air? An atmosphere is a layer of gas trapped by the gravity of a planet or moon. Here s Earth s atmosphere viewed from orbit: Why Is There Air? If atoms move faster

More information

Ag Earth Science Chapter 23

Ag Earth Science Chapter 23 Ag Earth Science Chapter 23 Chapter 23.1 Vocabulary Any of the Earth- like planets, including Mercury, Venus, and Earth terrestrial planet Jovian planet The Jupiter- like planets: Jupiter, Saturn, Uranus,

More information

Terrestrial Bodies of the Solar System. Valerie Rapson

Terrestrial Bodies of the Solar System. Valerie Rapson Terrestrial Bodies of the Solar System Valerie Rapson March 22, 2012 Terrestrial Bodies Many different bodies in the Solar System Gaspra Terrestrial bodies are those with solid surfaces on which one could

More information

11/4/2015. Venus and Mars. Chapter 13. Venus and Mars. The Rotation of Venus. The Atmosphere of Venus. The Surface of Venus

11/4/2015. Venus and Mars. Chapter 13. Venus and Mars. The Rotation of Venus. The Atmosphere of Venus. The Surface of Venus Venus and Mars Two most similar planets to Earth: Chapter 13 Venus and Mars Similar in size and mass Same part of the solar system Atmosphere Similar interior structure The Rotation of Venus Almost all

More information

Inner and Outer Planets

Inner and Outer Planets Inner and Outer Planets Inner Planets Terrestrial planets are those that are closest to the Sun. Terrestrial planets are made mostly of rock and have similar characteristics to Earth. There are four terrestrial

More information

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

After you read this section, you should be able to answer these questions: CHAPTER 16 4 Moons SECTION Our Solar System California Science Standards 8.2.g, 8.4.d, 8.4.e BEFORE YOU READ After you read this section, you should be able to answer these questions: How did Earth s moon

More information

SOLAR SYSTEM NOTES. Scientists believe its at least 4.6 billion years old!!! 10/26/2017 ENERGY TRANSFERS RADIATION FROM THE SUN

SOLAR SYSTEM NOTES. Scientists believe its at least 4.6 billion years old!!! 10/26/2017 ENERGY TRANSFERS RADIATION FROM THE SUN SOLAR SYSTEM NOTES Our Solar System is composed of: 1. The Sun 2. The Planets 3. Asteroids 4. Comets 5. Meteors 6. Natural & Artificial satellites Remember: How old is our Solar System? Scientists believe

More information

TopHat quizzes for astro How would you represent in scientific notation? A 2.7 x 10 2 B 2.7 x 10 3 C 2.7 x 10 4 D 2.

TopHat quizzes for astro How would you represent in scientific notation? A 2.7 x 10 2 B 2.7 x 10 3 C 2.7 x 10 4 D 2. TopHat quizzes for astro 111 Lecture week 1 1. If you multiply 2 x 10 4 by itself, what do you get? A. 4 x 10 4 B. 4 x 10 8 C. 2 x 10 4 D. 4 x 10 16 2. Jupiter's maximum distance from the sun is approximately

More information

Class Announcements. Solar System. Objectives for today. Will you read Chap 32 before Wed. class? Chap 32 Beyond the Earth

Class Announcements. Solar System. Objectives for today. Will you read Chap 32 before Wed. class? Chap 32 Beyond the Earth Class Announcements Please fill out an evaluation for this class. If you release your name I ll I give you quiz credit. Will you read Chap 32 before Wed. class? a) Yes b) No Chap 32 Beyond the Earth Objectives

More information

Motion of the planets

Motion of the planets Our Solar system Motion of the planets Our solar system is made up of the sun and the 9 planets that revolve around the sun Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, Neptune & Pluto (maybe?)

More information

ASTRO 120 Sample Exam

ASTRO 120 Sample Exam ASTRO 120 Sample Exam 1) If a planet has a reasonably strong magnetic field, we know that a. It is made entirely of iron b. There is liquid nitrogen below the surface c. It can harbor life d. It has a

More information

Jovian Planets Jupiter, Saturn, Uranus and Neptune

Jovian Planets Jupiter, Saturn, Uranus and Neptune The Inner Planets The Inner Planets Terrestrial Planets Mercury, Venus, Earth and Mars Rocky Surfaces No rings No or Few Moons Jovian Planets Jupiter, Saturn, Uranus and Neptune Gas Surfaces rings Many

More information

Learning Objectives. they differ in density (composition, core), atmosphere, surface age, size, geological activity, magnetic field?

Learning Objectives. they differ in density (composition, core), atmosphere, surface age, size, geological activity, magnetic field? Mercury and Venus Learning Objectives! Contrast the Earth, the Moon, Venus and Mercury. Do they differ in density (composition, core), atmosphere, surface age, size, geological activity, magnetic field?!

More information

Unit 3 Lesson 4 The Terrestrial Planets. Copyright Houghton Mifflin Harcourt Publishing Company

Unit 3 Lesson 4 The Terrestrial Planets. Copyright Houghton Mifflin Harcourt Publishing Company Florida Benchmarks SC.8.N.1.5 Analyze the methods used to develop a scientific explanation as seen in different fields of science. SC.8.E.5.3 Distinguish the hierarchical relationships between planets

More information

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

Physical Science 1 Chapter 16 INTRODUCTION. Astronomy is the study of the universe, which includes all matter, energy, space and time. INTRODUCTION Astronomy is the study of the universe, which includes all matter, energy, space and time. Although the universe is vast and almost beyond imagination, much is known about its make-up and

More information

Lecture #10: Plan. The Moon Terrestrial Planets

Lecture #10: Plan. The Moon Terrestrial Planets Lecture #10: Plan The Moon Terrestrial Planets Both Sides of the Moon Moon: Direct Exploration Moon: Direct Exploration Moon: Direct Exploration Apollo Landing Sites Moon: Apollo Program Magnificent desolation

More information

Name. Physical Science Astronomy Exam II. Questions 1-18 have to do with the terrestrial planets, choose your answer from the list below:

Name. Physical Science Astronomy Exam II. Questions 1-18 have to do with the terrestrial planets, choose your answer from the list below: Name Physical Science 113 - Astronomy Exam II Questions 1-18 have to do with the terrestrial planets, choose your answer from the list below: 1. The smallest terrestrial planet. A) Mercury B) Venus C)

More information

Inner and Outer Planets

Inner and Outer Planets Inner and Outer Planets SPI 0607.6.2 Explain how the relative distance of objects from the earth affects how they appear. Inner Planets Terrestrial planets are those that are closest to the Sun. Terrestrial

More information

2. Terrestrial Planet G 9. Coulomb Force C 16. Babcock model Q. 3. Continuous Spectrum K 10. Large-impact hypothesis I 17.

2. Terrestrial Planet G 9. Coulomb Force C 16. Babcock model Q. 3. Continuous Spectrum K 10. Large-impact hypothesis I 17. Astronomy 1 S 16 Exam 1 Name Identify terms Label each term with the appropriate letter of a definition listed 1. Spectral line R 8. Albedo H 15. helioseismology E 2. Terrestrial Planet G 9. Coulomb Force

More information

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

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 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 Ch 23.1 The Solar System Terrestrial planets- Small Rocky

More information

Astronomy 1140 Quiz 3 Review

Astronomy 1140 Quiz 3 Review Astronomy 1140 Quiz 3 Review Anil Pradhan October 26, 2016 I The Inner Planets 1. What are the terrestrial planets? What do they have in common? Terrestrial planets: Mercury, Venus, Earth, Mars. Theses

More information

The Moon. Tides. Tides. Mass = 7.4 x 1025 g = MEarth. = 0.27 REarth. (Earth 5.5 g/cm3) Gravity = 1/6 that of Earth

The Moon. Tides. Tides. Mass = 7.4 x 1025 g = MEarth. = 0.27 REarth. (Earth 5.5 g/cm3) Gravity = 1/6 that of Earth The Moon Mass = 7.4 x 1025 g = 0.012 MEarth Radius = 1738 km = 0.27 REarth Density = 3.3 g/cm3 (Earth 5.5 g/cm3) Gravity = 1/6 that of Earth Dark side of the moon We always see the same face of the Moon.

More information

Astronomy Ch. 11 Jupiter. MULTIPLE CHOICE. Choose the one alternative that best completes the statement or answers the question.

Astronomy Ch. 11 Jupiter. MULTIPLE CHOICE. Choose the one alternative that best completes the statement or answers the question. Name: Period: Date: Astronomy Ch. 11 Jupiter MULTIPLE CHOICE. Choose the one alternative that best completes the statement or answers the question. 1) Jupiter is noticeably oblate because: A) it has a

More information

A Look at Our Solar System: The Sun, the planets and more. by Firdevs Duru

A Look at Our Solar System: The Sun, the planets and more. by Firdevs Duru A Look at Our Solar System: The Sun, the planets and more by Firdevs Duru Week 1 An overview of our place in the universe An overview of our solar system History of the astronomy Physics of motion of the

More information

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

The Inner Planets. Chapter 3 Lesson 1. Pages Workbook pages 51-52 The Inner Planets Chapter 3 Lesson 1 Pages 152-159 Workbook pages 51-52 Create the Foldable on pg 159 The solar The planets system The four inner planets Compare and Contrast Question What are planets?

More information

Jovian Planet Systems

Jovian Planet Systems Jovian Planet Systems Reading: Chapter 14.1-14.5 Jovian Planet Systems Voyager 1 and 2 explored the outer planets in the 1970s and 1980s. The Galileo spacecraft circled Jupiter dozens of times in the late

More information

Red Planet Mars. Chapter Thirteen

Red Planet Mars. Chapter Thirteen Red Planet Mars Chapter Thirteen ASTR 111 003 Fall 2006 Lecture 11 Nov. 13, 2006 Introduction To Modern Astronomy I Introducing Astronomy (chap. 1-6) Planets and Moons (chap. 7-17) Ch7: Comparative Planetology

More information

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.

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. Mercury Mercury is the closest planet to the sun. It is extremely hot on the side of the planet facing the sun and very cold on the other. There is no water on the surface. There is practically no atmosphere.

More information

Today. Events. Terrestrial Planet Atmospheres (continued) Homework DUE. Review next time? Exam next week

Today. Events. Terrestrial Planet Atmospheres (continued) Homework DUE. Review next time? Exam next week Today Terrestrial Planet Atmospheres (continued) Events Homework DUE Review next time? Exam next week Planetary Temperature A planet's surface temperature is determined by the balance between energy from

More information

Jupiter & Saturn. Moons of the Planets. Jupiter s Galilean satellites are easily seen with Earth-based telescopes. The Moons

Jupiter & Saturn. Moons of the Planets. Jupiter s Galilean satellites are easily seen with Earth-based telescopes. The Moons The Moons Jupiter & Saturn Earth 1 Mars 2 Jupiter 63 Saturn 47 Uranus 27 Neptune 13 Pluto 3 Moons of the Planets Galileo (1610) found the first four moons of Jupiter. Total 156 (as of Nov. 8, 2005) Shortened

More information

Solar System revised.notebook October 12, 2016 Solar Nebula Theory

Solar System revised.notebook October 12, 2016 Solar Nebula Theory Solar System revised.notebook The Solar System Solar Nebula Theory Solar Nebula was a rotating disk of dust and gas w/ a dense center dense center eventually becomes the sun start to condense b/c of gravity

More information

Inner Planets (Part II)

Inner Planets (Part II) Inner Planets (Part II) Sept. 18, 2002 1) Atmospheres 2) Greenhouse Effect 3) Mercury 4) Venus 5) Mars 6) Moon Announcements Due to technical difficulties, Monday s quiz doesn t count An extra credit problem

More information

Image of the Moon from the Galileo Space Craft

Image of the Moon from the Galileo Space Craft Image of the Moon from the Galileo Space Craft Moon: Overview Due to its size (diameter 3476 km, Mercury s diameter is 4880 km) and composition, the moon is sometimes considered as a terrestrial planet

More information

The Sun and Planets Lecture Notes 6.

The Sun and Planets Lecture Notes 6. The Sun and Planets Lecture Notes 6. Lecture 6 Venus 1 Spring Semester 2017 Prof Dr Ravit Helled Cover photo: Venus in true color (Courtesy of NASA) Venus Properties Venus is the second brightest natural

More information

The Planets, Asteroids, Moons, etc.

The Planets, Asteroids, Moons, etc. DATE DUE: Ms. Terry J. Boroughs Geology 305 Name: Section: The Planets, Asteroids, Moons, etc. Instructions: Read each question carefully before selecting the BEST answer or option. Use GEOLOGIC vocabulary

More information

What are terrestrial planets like on the inside? Chapter 9 Planetary Geology: Earth and the Other Terrestrial Worlds. Seismic Waves.

What are terrestrial planets like on the inside? Chapter 9 Planetary Geology: Earth and the Other Terrestrial Worlds. Seismic Waves. Chapter 9 Planetary Geology: Earth and the Other Terrestrial Worlds What are terrestrial planets like on the inside? Seismic Waves Vibrations that travel through Earth s interior tell us what Earth is

More information

The Jovian Planets (Gas Giants)

The Jovian Planets (Gas Giants) The Jovian Planets (Gas Giants) Discoveries and known to ancient astronomers. discovered in 1781 by Sir William Herschel (England). discovered in 1845 by Johann Galle (Germany). Predicted to exist by John

More information

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.

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. Chapter 23 Our Solar System Our Solar System Historical Astronomy Wandering Stars Greeks watched the stars move across the sky and noticed five stars that wandered around and did not follow the paths of

More information

Earth & Space Science ~ The Solar System

Earth & Space Science ~ The Solar System Earth & Space Science ~ The Solar System In e r Sci Uni 11 I. Sun, Earth & Moon A. The Solar System 1. the sun & the objects orbiting it a. incl. 8 planets, other stars, asteroids, meteoroids, dwarf planets,

More information

1 Describe the structure of the moon 2. Describe its surface features 3. Summarize the hypothesis of moon formation

1 Describe the structure of the moon 2. Describe its surface features 3. Summarize the hypothesis of moon formation Loulousis 1 Describe the structure of the moon 2. Describe its surface features 3. Summarize the hypothesis of moon formation moon -a body that revolves around a planet and that has less mass than the

More information

Moons of Sol Lecture 13 3/5/2018

Moons of Sol Lecture 13 3/5/2018 Moons of Sol Lecture 13 3/5/2018 Tidal locking We always see the same face of the Moon. This means: period of orbit = period of spin Top view of Moon orbiting Earth Earth Why? The tidal bulge in the solid

More information

Astronomy 1140 Quiz 3 Review

Astronomy 1140 Quiz 3 Review Astronomy 1140 Quiz 3 Review Anil Pradhan October 27, 2017 I The Inner Planets 1. What are the terrestrial planets? What do they have in common? Terrestrial planets: Mercury, Venus, Earth, Mars. Theses

More information

3. Titan is a moon that orbits A) Jupiter B) Mars C) Saturn D) Neptune E) Uranus

3. Titan is a moon that orbits A) Jupiter B) Mars C) Saturn D) Neptune E) Uranus Fall 2013 Astronomy - Test 2 Test form A Name Do not forget to write your name and fill in the bubbles with your student number, and fill in test form A on the answer sheet. Write your name above as well.

More information

37. Planetary Geology p

37. Planetary Geology p 37. Planetary Geology p. 656-679 The Solar System Revisited We will now apply all the information we have learned about the geology of the earth to other planetary bodies to see how similar, or different,

More information

FCAT Review Space Science

FCAT Review Space Science FCAT Review Space Science The Law of Universal Gravitation The law of universal gravitation states that ALL matter in the universe attracts each other. Gravity is greatly impacted by both mass and distance

More information

Jupiter and its Moons

Jupiter and its Moons Jupiter and its Moons Summary 1. At an average distance of over 5 AU, Jupiter takes nearly 12 years to orbit the Sun 2. Jupiter is by far the largest and most massive planet in the solar system being over

More information

Mars ( ) The Sun and Planets Lecture Notes 6. Spring Semester 2018 Prof Dr Ravit Helled

Mars ( ) The Sun and Planets Lecture Notes 6. Spring Semester 2018 Prof Dr Ravit Helled The Sun and Planets Lecture Notes 6. Spring Semester 2018 Prof Dr Ravit Helled Mars ( ) Mars is the fourth planet from the Sun and the outermost terrestrial planet. It has a density of 3.93 g/cm3, which

More information

- newmanlib.ibri.org - The Solar System. Robert C. Newman. Abstracts of Powerpoint Talks

- newmanlib.ibri.org - The Solar System. Robert C. Newman. Abstracts of Powerpoint Talks The Solar System Robert C. Newman The Solar System This is the name we give to the sun (Latin, sol) and its planets, plus the other objects that are gravitationally bound to the sun. In this talk, we will

More information

Chapter 11 Jovian Planet Systems. Comparing the Jovian Planets. Jovian Planet Composition 4/10/16. Spacecraft Missions

Chapter 11 Jovian Planet Systems. Comparing the Jovian Planets. Jovian Planet Composition 4/10/16. Spacecraft Missions Chapter 11 Jovian Planet Systems Jovian Planet Interiors and Atmospheres How are jovian planets alike? What are jovian planets like on the inside? What is the weather like on jovian planets? Do jovian

More information

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

When you have completed this workbook, you should know and understand the following: Name When you have completed this workbook, you should know and understand the following: Standard Description Passed SciBer Text III.1.a III.1.b. Understand and correctly use unit vocabulary. List the

More information

Outline 9: Origin of the Earth: solids, liquids, and gases. The Early Archean Earth

Outline 9: Origin of the Earth: solids, liquids, and gases. The Early Archean Earth Outline 9: Origin of the Earth: solids, liquids, and gases The Early Archean Earth Origin of Earth s Matter The earth is made of recycled elements formed in stars that existed prior to our Sun. Supernova

More information

Exam# 2 Review. Exam #2 is Wednesday November 8th at 10:40 AM in room FLG-280

Exam# 2 Review. Exam #2 is Wednesday November 8th at 10:40 AM in room FLG-280 Exam# 2 Review Exam #2 is Wednesday November 8th at 10:40 AM in room FLG-280 Bring Gator 1 ID card Bring pencil #2 with eraser No use of calculator or any electronic device during the exam We provide the

More information

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.

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. 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 0.387 astronomical units Diameter: 4,879.4 km (3,031.92 miles)

More information

Outline 9: Origin of the Earth: solids, liquids, and gases

Outline 9: Origin of the Earth: solids, liquids, and gases Outline 9: Origin of the Earth: solids, liquids, and gases The Early Archean Earth Origin of Earth s Matter The earth is made of recycled elements formed in stars that existed prior to our Sun. Supernova

More information

Astronomy I Exam 2 Sample

Astronomy I Exam 2 Sample NAME: Part I: Multiple Choice (2 points. ea.) Read carefully, choose the best answer 1. Which of the following occurs because of the orbital motion of the Earth about the Sun and cannot be accounted for

More information

A Survey of the Planets Earth Mercury Moon Venus

A Survey of the Planets Earth Mercury Moon Venus A Survey of the Planets [Slides] Mercury Difficult to observe - never more than 28 degree angle from the Sun. Mariner 10 flyby (1974) Found cratered terrain. Messenger Orbiter (Launch 2004; Orbit 2009)

More information

Chapter: The Solar System

Chapter: The Solar System Table of Contents Chapter: The Solar System Section 1: Planet Motion Section 2: The Inner Planets Section 3: The Outer Planets Section 4: Life in the Solar System 1 Planet Motion Models of the Solar System

More information

Radiation - a process in which energy travels through vacuum (without a medium) Conduction a process in which energy travels through a medium

Radiation - a process in which energy travels through vacuum (without a medium) Conduction a process in which energy travels through a medium SOLAR SYSTEM NOTES ENERGY TRANSFERS Radiation - a process in which energy travels through vacuum (without a medium) Conduction a process in which energy travels through a medium Convection - The transfer

More information

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

Starting from closest to the Sun, name the orbiting planets in order. Chapter 9 Section 1: Our Solar System Solar System: The solar system includes the sun, planets and many smaller structures. A planet and its moon(s) make up smaller systems in the solar system. Scientist

More information

The Planets. The Terrestrial Planets. Admin. 9/19/17. Key Concepts: Lecture 13. Formulae (will be displayed for you in Midterm 1):

The Planets. The Terrestrial Planets. Admin. 9/19/17. Key Concepts: Lecture 13. Formulae (will be displayed for you in Midterm 1): Admin. 9/19/17 1. Class website http://www.astro.ufl.edu/~jt/teaching/ast1002/ 2. Optional Discussion sections: Tue. ~11.30am (period 5), Bryant 3; Thur. ~12.35pm (end of period 5 and period 6), start

More information

Mars Opposition Friday 27 th July 2018

Mars Opposition Friday 27 th July 2018 Mars Opposition Friday 27 th July 2018 Mars is about 6,780 kilometres in diameter or roughly half the size of the Earth whose diameter is 12,742km. As they orbit the Sun, the minimum distance between the

More information

Which of the following statements best describes the general pattern of composition among the four jovian

Which of the following statements best describes the general pattern of composition among the four jovian Part A Which of the following statements best describes the general pattern of composition among the four jovian planets? Hint A.1 Major categories of ingredients in planetary composition The following

More information

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

Name: Date: Hour: 179 degrees celsius. 5% of Earth A 70 pound person would weigh 27 pounds on Mercury. Planet Exploration- http://www.kidsastronomy.com/solar_.htm Mercury 1 87.9 days 58.6 days 57 million Km 465 degrees celsius Minimum -184 degrees celsius 179 degrees celsius Moons Terrestrial or Gaseous?

More information

3. The moon with the most substantial atmosphere in the Solar System is A) Iapetus B) Io C) Titan D) Triton E) Europa

3. The moon with the most substantial atmosphere in the Solar System is A) Iapetus B) Io C) Titan D) Triton E) Europa Spring 2013 Astronomy - Test 2 Test form A Name Do not forget to write your name and fill in the bubbles with your student number, and fill in test form A on the answer sheet. Write your name above as

More information

Moon and Mercury 3/8/07

Moon and Mercury 3/8/07 The Reading Assignment Chapter 12 Announcements 4 th homework due March 20 (first class after spring break) Reminder about term paper due April 17. Next study-group session is Monday, March 19, from 10:30AM-12:00Noon

More information

Descriptive Astronomy (ASTR 108) Exam 2A March 29, 2010

Descriptive Astronomy (ASTR 108) Exam 2A March 29, 2010 Descriptive Astronomy (ASTR 108) Exam 2A March 29, 2010 Name: In each of the following multiple choice questions, select the best possible answer. First circle the answer on this exam, then in the line

More information

THE GAS GIANTS JUPITER VENUS MARS EARTH

THE GAS GIANTS JUPITER VENUS MARS EARTH THE GAS GIANTS JUPITER SATURN URANUS NEPTUNE VENUS The temperature at the cloud tops is 200 C while the interior temperatures reach tens of thousands of degrees. The churning of the atmosphere causes temperatures

More information

Astronomy. physics.wm.edu/~hancock/171/ A. Dayle Hancock. Small 239. Office hours: MTWR 10-11am. Page 1

Astronomy.  physics.wm.edu/~hancock/171/ A. Dayle Hancock. Small 239. Office hours: MTWR 10-11am. Page 1 Astronomy A. Dayle Hancock adhancock@wm.edu Small 239 Office hours: MTWR 10-11am Planetology I Terrestrial and Jovian planets Similarities/differences between planetary satellites Surface and atmosphere

More information

Lecture: Planetology. Part II: Solar System Planetology. Orbits of Planets. Rotational Oddities. A. Structure of Solar System. B.

Lecture: Planetology. Part II: Solar System Planetology. Orbits of Planets. Rotational Oddities. A. Structure of Solar System. B. Part II: Solar System Planetology 2 A. Structure of Solar System B. Planetology Lecture: Planetology C. The Planets and Moons Updated: 2012Feb10 A. Components of Solar System 3 Orbits of Planets 4 1. Planets

More information

Astro 1010 Planetary Astronomy Sample Questions for Exam 4

Astro 1010 Planetary Astronomy Sample Questions for Exam 4 Astro 1010 Planetary Astronomy Sample Questions for Exam 4 Chapter 8 1. Which of the following processes is not important in shaping the surface of terrestrial planets? a) Impact cratering b) Tectonism

More information

The Fathers of the Gods: Jupiter and Saturn

The Fathers of the Gods: Jupiter and Saturn The Fathers of the Gods: Jupiter and Saturn Learning Objectives! Order all the planets by size and distance from the Sun! How are clouds on Jupiter (and Saturn) different to the Earth? What 2 factors drive

More information

Directed Reading B. Section: The Outer Planets

Directed Reading B. Section: The Outer Planets Skills Worksheet Directed Reading B Section: The Outer Planets 1. What is one way that gas giants differ from the terrestrial planets? a. They are much smaller. b. They are rocky and icy. c. They are made

More information

Venus. Venus. (The most visited planet) Orbit, Rotation Atmosphere. Surface Features Interior. (Greenhouse effect) Mariner 10 image

Venus. Venus. (The most visited planet) Orbit, Rotation Atmosphere. Surface Features Interior. (Greenhouse effect) Mariner 10 image Venus Orbit, Rotation Atmosphere (Greenhouse effect) Surface Features Interior Mariner 10 image Venus (The most visited planet) Mariner 2 (1962) Mariner 5 (1967) Mariner 10 (1974) Poineer Venus (1978)

More information

Geology of the terrestrial planets Pearson Education, Inc.

Geology of the terrestrial planets Pearson Education, Inc. Geology of the terrestrial planets 2014 Pearson Education, Inc. Earth s Bulk Properties Earth s Bulk Properties albedo - A = 0.39 A = 0 planet absorbs all sunlight that hits it A =1 planet reflects all

More information

Lecture 19: The Moon & Mercury. The Moon & Mercury. The Moon & Mercury

Lecture 19: The Moon & Mercury. The Moon & Mercury. The Moon & Mercury Lecture 19: The Moon & Mercury The Moon & Mercury The Moon and Mercury are similar in some ways They both have: Heavily cratered Dark colored surfaces No atmosphere No water They also have some interesting

More information

Learning Objectives. they differ in density, composition, atmosphere, surface age, size, geological activity, magnetic field?

Learning Objectives. they differ in density, composition, atmosphere, surface age, size, geological activity, magnetic field? The Red Planet Learning Objectives! Contrast the Terrestrial Planets and the Moon. Do they differ in density, composition, atmosphere, surface age, size, geological activity, magnetic field?! Why is Mars

More information

Chapter 23 Earth Science 11

Chapter 23 Earth Science 11 Chapter 23 Earth Science 11 Inner planets: Closest planets to the sun A.k.a. terrestrial planets All have a rocky crust, dense mantle layer, and a very dense core Mercury, Venus, Earth, and Mars Outer

More information

The Galilean Moons. ENV235Y1 Yin Chen (Judy)

The Galilean Moons. ENV235Y1 Yin Chen (Judy) The Galilean Moons ENV235Y1 Yin Chen (Judy) Jupiter The Galilean Moons Discovered by Italian Astronomer Galileo Galilei in 1609 using a new invention called telescope. http://astronomyonline.org/solarsystem/galileanmoons.asp

More information

Solar System. The Solar System. Nebular animation. Planets drawn to scale. Mercury. Mariner 10. Chapter 22 Pages

Solar System. The Solar System. Nebular animation. Planets drawn to scale. Mercury. Mariner 10. Chapter 22 Pages The Solar System Chapter 22 Pages 612-633 Solar System Planets drawn to scale Nebular animation Distances not to scale Earth approximately 12,800 km diameter Earth is about 150,000,000 km from Sun Mercury

More information

The Moon & Mercury: Dead Worlds

The Moon & Mercury: Dead Worlds The Moon & Mercury: Dead Worlds There are many similarities between the Moon and Mercury, and some major differences we ll concentrate mostly on the Moon. Appearance of the Moon from the Earth We ve already

More information