Astronomy 103: First Exam

Similar documents
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.

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

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

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

ASTR 1050: Survey of Astronomy Fall 2012 PRACTICE Exam #2 Instructor: Michael Brotherton Covers Solar System and Exoplanet Topics

Inner Planets (Part II)

ASTRONOMY 1010 Exam 2 October 19, 2007

Astronomy 1001/1005 Midterm (200 points) Name:

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..

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

a. 1/3 AU b. 3 AU 5. Meteor showers occur

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

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)

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

X Rays must be viewed from space used for detecting exotic objects such as neutron stars and black holes also observing the Sun.

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

Universe Celestial Object Galaxy Solar System

Which of the following correctly describes the meaning of albedo?

The History of the Earth

ASTRO 120 Sample Exam

Astro 1: Introductory Astronomy

Earth s Formation Unit [Astronomy] Student Success Sheets (SSS)

Chapter 15: The Origin of the Solar System

HW #2. Solar Nebular Theory. Predictions: Young stars have disks. Disks contain gas & dust. Solar System should contain disk remnants

Unit 1: The Earth in the Universe

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

Class 15 Formation of the Solar System

Chapter 23: Touring 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?

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

Comparative Planetology I: Our Solar System

Making a Solar System

Solution for Homework# 3. Chapter 5 : Review & Discussion

Solar System Formation

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

Overview of 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

Origin of the Solar System

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

Planetarium observing is over. Nighttime observing starts next week.

Chapter 19 The Origin of the Solar System

Astronomy Study Guide Answer Key

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

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

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

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

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

4. THE SOLAR SYSTEM 1.1. THE SUN. Exercises

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

Stellar Astronomy Sample Questions for Exam 3

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

Cosmic Microwave Background Radiation

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

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

Astronomy 1504 Section 10 Final Exam Version 1 May 6, 1999

FCAT Review Space Science

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

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

ASTRONOMY CURRICULUM Unit 1: Introduction to Astronomy

Chapter 8 Lecture. The Cosmic Perspective Seventh Edition. Formation of the Solar System

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

Solar System Formation

F = ma P 2 = a 3 (M + m) P 2 = a 3. max T = 2900 K m

Solar System Formation

Astronomy 210 Midterm #2

ASTRONOMY 1 FINAL EXAM 1 Name

Today. Solar System Formation. a few more bits and pieces. Homework due

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.

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

The Solar System. Name Test Date Hour

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

Inner and Outer Planets

Lunar Eclipse. Solar Eclipse

Exploring Our Solar System

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

The Cosmic Perspective Seventh Edition. Asteroids, Comets, and Dwarf Planets: Their Natures, Orbits, and Impacts. Chapter 12 Review Clickers

What does the solar system look like?

9. Formation of the Solar System

ES - Astronomy Part 2 Post-Test

Astro 1010 Planetary Astronomy Sample Questions for Exam 3

Answers. The Universe. Year 10 Science Chapter 6

CST Prep- 8 th Grade Astronomy

Our Planetary System & the Formation of the Solar System

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

Astronomy 104: Second Exam

Origin of the Solar System

~15 GA. (Giga Annum: Billion Years) today

AST Section 2: Test 2

-Melissa Greenberg, Arielle Hoffman, Zachary Feldmann, Ryan Pozin, Elizabeth Weeks, Christopher Pesota, & Sara Pilcher

Astronomy Final Exam Study Guide

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

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

Lecture: Planetology. Part II: Solar System Planetology. A. Components of Solar System. B. Formation of Solar System. C. Xtra Solar Planets

Opaque Atmosphere. Astronomy 210. Question. Why would it be useful to place telescopes in. Section 1 MWF Astronomy Building. space?

Astronomy (Geology 360, Physics 360) take-home test. There is no class on Monday March 16th

Astronomy Part 1 Regents Questions

ASTRONOMY SNAP GAME. with interesting facts

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

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

Which letter on the timeline best represents the time when scientists estimate that the Big Bang occurred? A) A B) B C) C D) D

Transcription:

Name: Astronomy 103: First Exam Stephen Lepp October 27, 2010 Each question is worth 2 points. Write your name on this exam and on the scantron. 1 Short Answer A. What is the largest of the terrestrial planets? Earth 2 Multiple Choice 1. When you come to the lectures, you see me lecturing because I (a) emit infrared radiation (b) scatter infrared radiation (c) emit visible radiation (d) scatter visible radiation (e) refract visible radiation 2. X-rays have shorter wavelengths then radio waves. 1

3. The largest optical telescopes are (a) 1 m (b) 2 m (c) 5 m (d) 10 m (e) 100 m 4. The diffraction limit of a telescope is (a) The largest a telescope of a particular wavelength can be (b) The smallest a telescope of a particular wavelength can be (c) the best angular resolution for a particular telescope (d) the furthest object that can be seen with a particular telescope (e) 73 5. Which of the following could be determined by the spectra of an object (a) the chemical composition (b) the rotation rate (c) the temperature (d) all of these (e) none of these 6. Where did the elements heavier then hydrogen and helium come from (a) the big bang. (b) the little bang (c) produced in planets (d) produced in interstellar gas (e) produced in stars 2

7. Why did the solar nebula heat as it collapsed? (a) it turned gravitational potential energy to thermal (b) to conserve angular momentum (c) to conserve linear momentum (d) radiation from nearby stars (e) converted hydrogen to helium 8. Which of the following lie just beyond Neptune in the plane of the ecliptic (a) Mars (b) Moon (c) Oort Cloud (d) Kuiper Belt (e) Asteroid Belt 9. According to nebular theory what are asteroids and comets? (a) remains of collisions among planets (b) remains of collisions among moons (c) left over from planet formation. (d) from volcano s. (e) from vocations on mars. 10. From low to high photon energy the bands of electromagnetic radiation are (a) UV, radio, visible, infrared, x-ray, gamma-ray (b) gamma-ray, UV, visible, infrared, x-ray, radio (c) UV, radio, x-ray, infrared, visible, gamma-ray (d) radio, infrared, visible, UV, x-ray, gamma-ray (e) radio, UV, visible, infrared, x-ray, gamma-ray 3

11. Which of the following is most likely to lead to an absorption line spectrum (a) a very fast moving bird (b) a fast moving star (c) gas between us and a star (d) a star in front of some gas (e) large telescopes 12. When an electron in an atom goes from a high energy state to a lower state (a) the atom absorbs a photon of the energy difference. (b) the atom emits a photon of the energy difference. (c) the atom emits a photon of thermal energy (d) the electron becomes a photon of the energy difference (e) the atom loses half its electric charge. 13. The terrestrial worlds from small to large are (a) Moon, Mars, Mercury, Earth, Venus (b) Mercury, Mars, Moon, Earth, Venus (c) Mercury, Moon, Mars, Earth, Venus (d) Moon, Mercury, Mars, Earth, Venus (e) Moon, Mercury, Mars, Venus, Earth 14. What is differentiation in planetary geology (a) The process by which gravity separates materials by density (b) the process by which different types of minerals form (c) any process by which a planets surfaces evolves (d) any process by which a planet evolves differently from other planets (e) any of these. 4

15. Smaller planets cool quicker then large planets because? (a) They form cooler (b) They are further from the sun (c) They have a larger surface to volume ratio (d) They have more volcano s (e) Actually they cool slower 16. Why does Venus have a weaker magnetic field then Earths? (a) The earth is directly overhead. (b) Venus doesn t have a metal core. (c) Venus rotates slower (d) Venus is hotter. (e) none of the above 17. Which of the following shows the greatest evidence of plate tectonics? (a) Mercury (b) Venus (c) Moon (d) Earth (e) Mars 18. Which of the following has the hottest surface? (a) Mercury (b) Venus (c) Moon (d) Earth (e) Mars 5

19. Which of the following has the densest atmosphere? (a) Mercury (b) Venus (c) Moon (d) Earth (e) Mars 20. Which of the following has the largest volcano in the solar system? (a) Mercury (b) Venus (c) Moon (d) Earth (e) Mars 21. Water arrived on Earth (a) from the initial accretion (b) it was accreted out of the gas (c) from comets during the heavy bombardment following the formation (d) from volcano s (e) none of the above 22. The age of the solar system is approximately (a) 4 hundred years (b) 4 thousand years (c) 4 million years (d) 4 billion years (e) 4 trillion years 6

23. What kind of features may result from tectonics (a) mountains (b) valleys (c) volcano s (d) all of the above (e) none of the above. 24. Surface features on Venus are known primarily from (a) observations by large telescopes. (b) rovers on the surface. (c) manned space missions. (d) UV telescopes. (e) radar measurements. 25. Which of the following appear to have ancient river beds? (a) Moon. (b) Mars. (c) Venus. (d) Mercury. (e) all of the above. 26. Why do we believe the surface of the moon and mercury are mostly unchanged in the last billion years. (a) because of the smooth polished surface (b) because of the heavy cratering (c) because of the dust on these surfaces (d) because of the large amounts of water (e) all of these 7

27. Which of the following are not characteristic of the inner planets (a) a substantial atmosphere (b) small compared to outer planets (c) solid rocky surfaces (d) few satellites (e) metallic cores 28. Which of the following is not characteristic of the outer planets (a) primarily made of gas (b) very few satellites (c) primarily hydrogen and helium (d) rings (e) large compared to inner planets 29. Rather then being a planet, Pluto is considered a member of (a) Kuiper Belt (b) Asteroid Belt (c) Oort Cloud (d) Moons of Neptune (e) Extrasolar Planets 30. Which of the following planets have rings (a) Jupiter (b) Saturn (c) Uranus (d) Neptune (e) all of the above 8

31. If we say a material is opaque to ultraviolet light, we mean that it (a) emits ultraviolet light (b) transmits ultraviolet light (c) refracts ultraviolet light (d) absorbs ultraviolet light (e) all of these 32. If we observe the same spectral lines in two stars with one of the stars rotating faster the lines in the faster rotating star will be (a) redshifted (b) blueshifted (c) greenshifted (d) narrower (e) broader 33. You are currently emitting electromagnetic waves of what type (a) mostly radio (b) mostly infrared (c) mostly visible (d) mostly UV (e) not emitting any radiation. 34. The moon is emitting in what band (a) mostly radio (b) mostly infrared (c) mostly visible (d) mostly UV (e) not emitting any radiation. 9

35. Which of the following planets doesn t rotate in the same direction as it orbits the sun (a) Mercury (b) Mars (c) Jupiter (d) Uranus (e) Neptune 36. Potassium-40 has a half-life of 1.3 billion years, if we start with 100 atoms, how much is left after 2.6 billion years? (a) 100 atoms (b) 50 atoms (c) 25 atoms (d) 1/16 of 100 atoms (e) none. 37. Erosion is more effective on Earth then Mars or Venus because of (a) Earth is bigger. (b) Earth is smaller (c) Earth is hotter (d) Earth is colder (e) Earth has water 38. The core and the mantle on earth are kept hot primarily by (a) accretion (b) differentiation (c) chemical energy (d) radioactive decay (e) atoms and molecules. 10

39. Subduction is where (a) The densest material sinks to the center (b) One plate slides under another (c) the plates pull apart (d) the gasses get added to the gas giants (e) none of these 40. Which planet has the most extreme seasons? (a) Venus (b) Earth (c) Jupiter (d) Uranus (e) Pluto 41. In what way is Pluto more like a comet then a planet (a) It is made of rock and ice. (b) It sometimes enters the inner solar system. (c) It has a long tail. (d) It is further then average. (e) It has a moon. 42. One big advantage to flyby missions is they cost less then orbiting missions, mostly because (a) of the extra weight of the instruments to keep in orbit (b) of the extra fuel needed to land on the planet. (c) because the fuel needed for getting into orbit means a larger takeoff weight (d) of the manpower needed to fly the satellite in orbit. (e) of the manpower needed for extra design problems. 11

43. The age of the Solar System is found by (a) radioactive dating of ancient artifacts (b) studies of the historical record (c) radioactive dating of meteorites (d) the solar nebular model (e) none of these 44. The Moon is believed to have formed as a result of a collision of a massive object with earth 45. In the solar nebula the frost line determines where rocky material forms 46. Jupiter is the largest planet 47. Grass is green because it absorbs colors other than green. 48. The shorter the wavelength of a photon the lower its frequency. 49. The terrestrial planets are all closer to the sun than the gas giants. 12