Which of the following correctly describes the meaning of albedo?

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

What is it like? When did it form? How did it form. The Solar System. Fall, 2005 Astronomy 110 1

Cosmology Vocabulary

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

Chapter 15: The Origin of the Solar System

Astronomy 1001/1005 Midterm (200 points) Name:

9.2 - Our Solar System

Astronomy 103: First Exam

9. Formation of the Solar System

1star 1 star 9 8 planets 63 (major) moons asteroids, comets, meteoroids

Which of the following planets are all made up of gas? When a planets orbit around the Sun looks like an oval, it s called a(n)

Edmonds Community College Astronomy 100 Winter Quarter 2007 Sample Exam # 2

23.1 The Solar System. Orbits of the Planets. Planetary Data The Solar System. Scale of the Planets The Solar System

Ag Earth Science Chapter 23

Lesson 3 THE SOLAR SYSTEM

Universe Celestial Object Galaxy Solar System

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

Making a Solar System

Prentice Hall EARTH SCIENCE

What s in Our Solar System?

9/22/ A Brief Tour of the Solar System. Chapter 6: Formation of the Solar System. What does the solar system look like?

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

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

Prentice Hall EARTH SCIENCE

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

1. Cosmology is the study of. a. The sun is the center of the Universe. b. The Earth is the center of the Universe

Lecture Outlines. Chapter 6. Astronomy Today 7th Edition Chaisson/McMillan Pearson Education, Inc.

Patterns in the Solar System (Chapter 18)

Comparative Planetology I: Our Solar System

The Big Bang Theory (page 854)

( ) a3 (Newton s version of Kepler s 3rd Law) Units: sec, m, kg

Origin of the Solar System

The History of the Solar System. From cloud to Sun, planets, and smaller bodies

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

Clicker Question: Clicker Question: Clicker Question:

Moon Obs #1 Due! Moon visible: early morning through afternoon. 6 more due June 13 th. 15 total due June 25 th. Final Report Due June 28th

STUDENT RESOURCE 1.1 INFORMATION SHEET. Vocabulary

Astronomy 1140 Quiz 4 Review

Chapter 23: Touring Our Solar System

Uranus & Neptune: The Ice Giants. Discovery of Uranus. Bode s Law. Discovery of Neptune

Earth Science 11 Learning Guide Unit Complete the following table with information about the sun:

The Solar System. Chapter Test A. Multiple Choice. Write the letter of the correct answer on the line at the left.

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

Chapter 23. Our Solar System

Joy of Science Experience the evolution of the Universe, Earth and Life

LESSON topic: formation of the solar system Solar system formation Star formation Models of the solar system Planets in our solar system

OUR SOLAR SYSTEM. James Martin. Facebook.com/groups/AstroLSSC Twitter.com/AstroLSSC

WHAT WE KNOW. Scientists observe that every object in the universe is moving away from each other. Objects furthest away are moving the fastest. So..

Solar System Formation

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

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

Patterns in the Solar System (Chapter 18)

Currently, the largest optical telescope mirrors have a diameter of A) 1 m. B) 2 m. C) 5 m. D) 10 m. E) 100 m.

Intro to Earth Science Chapter 23 Study Guide

Jovian Planet Properties

Chapter Outline. Earth and Other Planets. The Formation of the Solar System. Clue #1: Planetary Orbits. Clues to the Origin of the Solar System

Lecture 23: Jupiter. Solar System. Jupiter s Orbit. The semi-major axis of Jupiter s orbit is a = 5.2 AU

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

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

Coriolis Effect - the apparent curved paths of projectiles, winds, and ocean currents

Radioactive Dating. U238>Pb206. Halflife: Oldest earth rocks. Meteors and Moon rocks. 4.5 billion years billion years

TABLE OF CONTENTS. click one to go to that page, or just go on. What is the Solar System? Neptune (Pluto) The Sun. Asteroids. Mercury.

Phys 214. Planets and Life

Where did the solar system come from?

Background: (write a few things that you already know pertaining to about the question above)

The Solar System consists of

What is Earth Science?

Chapter 19 Origin of the Solar System

HNRS 227 Fall 2006 Chapter 13. What is Pluto? What is a Planet? There are two broad categories of planets: Terrestrial and Jovian

Solar System Formation

Chapter 11 Jovian Planet Systems

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

The Jovian Planets. Why do we expect planets like this in the outer reaches of the solar system?(lc)

Solar System Formation

CHAPTER 11. We continue to Learn a lot about the Solar System by using Space Exploration

ASTRONOMY CURRICULUM Unit 1: Introduction to Astronomy

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

Earth in the Universe Unit Notes

The Solar Nebula Theory. This lecture will help you understand: Conceptual Integrated Science. Chapter 28 THE SOLAR SYSTEM

The History of the Earth

Chapter 19 The Origin of the Solar System

1/13/16. Solar System Formation

4. THE SOLAR SYSTEM 1.1. THE SUN. Exercises

Chapter 4 The Solar System

Lecture Outlines. Chapter 15. Astronomy Today 7th Edition Chaisson/McMillan Pearson Education, Inc.

1UNIT. The Universe. What do you remember? Key language. Content objectives

Section 25.1 Exploring the Solar System (pages )

Chapter 16 Astronomy Study Guide. VOCABULARY WORDS TO KNOW geocentric system meteorite meteoroid

Other Planetary Systems (Chapter 13) Extrasolar Planets. Is our solar system the only collection of planets in the universe?

Chapter 11 Lecture. The Cosmic Perspective Seventh Edition. Jovian Planet Systems Pearson Education, Inc.

Formation of the Solar System

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

TEACHER BACKGROUND INFORMATION

The Solar System 6/23

Astronomy Test Review. 3 rd Grade

A star is a massive sphere of gases with a core like a thermonuclear reactor. They are the most common celestial bodies in the universe are stars.

Human Understanding of both Earth and Space has Changed Over Time. Unit E: Topic One

Chapter 11 Jovian Planet Systems. Jovian Planet Composition. Are jovian planets all alike? Density Differences. Density Differences

The Coriolis effect. Why does the cloud spin? The Solar Nebula. Origin of the Solar System. Gravitational Collapse

Announcements. HW #3 is Due on Thursday (September 22) as usual. Chris will be in RH111 on that day.

Transcription:

Which of the following correctly describes the meaning of albedo? A) The lower the albedo, the more light the surface reflects, and the less it absorbs. B) The higher the albedo, the more light the surface reflects, and the less it absorbs. C) The higher the albedo, the more light the surface absorbs. D) The higher the albedo, the more light the surface emits. E) The higher the albedo, the more light the atmosphere absorbs. Which of the following worlds has the most substantial atmosphere? A) Mercury B) Venus C) the Moon D) Mars E) Earth Which of the following planets has the least substantial atmosphere? A) Venus B) Earth C) Mars D) Neptune E) Mercury Which of the following worlds has the greatest difference in temperature between its "no atmosphere" temperature and its actual temperature? A) Mercury B) Venus C) Earth D) the Moon E) Mars Why does Venus have such a great difference in temperature between its "no atmosphere" temperature and its actual temperature? A) It has a slow rotation. B) It is so close to the Sun. C) It has a large amount of greenhouse gases in its atmosphere. D) It has a high level of volcanic activity. E) It has no cooling effects from oceans.

Why do jovian planets bulge around the equator, that is, have a "squashed" appearance? A) They are much more massive than the terrestrial planets. B) Their large systems of moons and rings gravitationally attract the mass around the equator more. C) Their rapid rotation flings the mass near the equator outward. D) Their internal heat sources exert a pressure against the sides of the planets. E) all of the above How much energy does Jupiter emit compared with how much it receives from the Sun? A) It emits 10 times as much. B) It emits twice as much. C) It emits half as much. D) It emits 10 percent as much. E) It emits 1 percent as much. How many more times is the atmospheric pressure in Jupiter's core greater than the atmospheric pressure at Earth's surface? A) 10 thousand B) 100 thousand C) 1 million D) 10 million E) 100 million How do astronomers think Jupiter generates its internal heat? A) radioactive decay B) internal friction due to its high rotation rate C) chemical processes D) nuclear fusion in the core E) by contracting, changing gravitational potential energy into thermal energy How does Jupiter's core compare to Earth's? A) It is the same size and mass. B) It is about 10 times larger both in size and mass. C) It is about 10 times larger in size and the same mass. D) It is about the same size but is 10 times more massive. E) Jupiter doesn't have a core!it is made entirely from hydrogen and helium.

Which of the following statements about comets and asteroids is true? A) Only asteroids collide with Earth. B) Comets are balls of ice and dust. C) Most of the trillions of comets in our solar system have tails. D) All asteroids lie in the asteroid belt between Mars and Jupiter. E) There are about 1 million known asteroids in the solar system. What do asteroids and comets have in common? A) Most are unchanged since their formation in the solar nebula. B) They have similar densities. C) They have similar orbital radii. D) They have a similar range of orbital inclinations. E) They have nothing in common with each other. A rocky leftover planetesimal orbiting the Sun is A) a comet. B) a meteor. C) an asteroid. D) a meteorite. E) possibly any of the above An icy leftover planetesimal orbiting the Sun is A) a comet. B) a meteor. C) an asteroid. D) a meteorite. E) possibly any of the above Why do asteroids and comets differ in composition? A) Asteroids formed inside the frost line, while comets formed outside. B) Asteroids and comets formed at different times. C) Comets formed from the jovian nebula, while asteroids did not. D) Comets are much larger than asteroids. E) Asteroids are much larger than comets. What is astrometry? A) measuring distances to stars B) searching for planets around stars C) measuring the positions of stars on the sky D) measuring the velocities of stars via the Doppler effect E) using metric units for distance (e.g. meters rather than light years) By itself, the Doppler technique provides a measure of a planet's A) minimum mass. B) orbital radius. C) orbital eccentricity. D) all of the above

Planets detected via the Doppler technique have been mostly A) Earth-mass, in Earth-like orbits. B) Jupiter-mass, in Jupiter-like orbits. C) Jupiter-mass, in very close orbits. D) Earth-mass, in very close orbits. E) a wide range of masses, in edge-on orbits. Current techniques can measure stellar motion to less than A) walking speed. B) running speed. C) freeway speed. D) cruising speed of an airplane. E) orbital speed of Jupiter. A planet's density can be measured by combining A) Doppler and astrometric observations. B) Doppler and transit observations. C) spectral observations of the planet's atmosphere. D) any method that measures the gravitational tug of the planet on the star. E) direct imaging from the new generation of space telescopes. The composition of a planet can be determined by A) the Doppler technique. B) astrometric measurements. C) transit observations. D) spectra. E) all of the above The size and shape of a planet's orbit can be determined by A) the Doppler technique. B) transit observations. C) spectral measurements. D) knowing the planet's mass by any technique and applying Newton's version of Kepler's third law. The astrometric technique of planet detection works best for A) large planets around nearby stars. B) massive planets around nearby stars. C) large planets around distant stars. D) massive planets around distant stars. E) planets in edge-on orbits.

Test 3 covers Ch 10-13 Chapter 10 Planetary Atmospheres What are the atmospheres around the various planets Greeenhouse Effect Earth's is unique Mars, Venus and Earth probably started the same, What happend? weather Chapter 11 Jovian Planets Jupiter and Saturn Uranus and Neptune What causes excess heat weather and storms Jovian planets moons Chapter 12 Astroids, Comets Astroids Comets Where were they formed, where are they now Meteor, Meteorite,... CHapter 13 Other Planets. How do we find them? (Doppler, Astronometry, Transit, Grav. Lens,...) What are the strengths of each method? What kind of systems have we found? How do we need to modify our Nebular Theory?