ASTR 1110H Fall 2004 Exam 1 Solutions - September 24, 2004
|
|
- Brendan Hopkins
- 5 years ago
- Views:
Transcription
1 ASTR 1110H Fall 2004 Exam 1 Solutions - September 24, 2004 Short answer questions (2 points each): 1. What is the definition of an Astronomical Unit? It is the average distance between the Earth and the Sun. 2. What is the cause of the seasons on Earth? The tilt of the Earth s rotation axis. 3. The Full Moon phase occurs every month; why isn t there a lunar eclipse every month? Because the Moon s orbit is slightly inclined relative to the orbit of the Earth around the Sun. 4. What information/observation did the ancient Greeks use to measure the ratio of the Earth-Moon distance to the Earth-Sun distance? Don t explain how they did it, just state what they used. The first- and third-quarter phases of the Moon. 5. What information/observation did the ancient Greeks use to measure the relative sizes of the Earth and the Moon? Again, don t explain how they did it, just state what they used. The size of the Moon compared to the Earth s shadow during a lunar eclipse. 6. How does the Geocentric model explain retrograde motion? With the help of epicycles and deferrents. 7. How does the Copernican model explain retrograde motion? By placing the Sun at the center, the Earth laps more distance planets. 8. What revolutionary ideas were introduced by Copernicus and by Kepler? Copernicus introduced the idea of a heliocentric universe and Kepler introduced the idea of elliptical orbits. 1
2 9. Consider the following three atoms: Atom-1 has 7 protons and 8 neutrons; Atom-2 has 8 protons and 7 neutrons; Atom-3 has 8 protons and 8 neutrons. Which two are isotopes of the same element? Atoms 2 and 3, because they have the same number of protons. 10. What are the two requirements for thermonuclear fusion to occur in the center of the Sun? High temperature and high density. 11. Which object radiates more energy per area: a large, cool object or a small, hot object? What is the basis for your answer? The small, hot object because the Stefan-Boltzmann law depends only on temperature and is independent of size. 12. What is the significance of the number in the thermonuclear fusion process? It represents the fraction of hydrogen mass that is converted into energy. 13. Is the presence of ozone in the Earth s atmosphere good or bad? Why? Good, because the ozone absorbs the Sun s harmful UV radiation. 14. Give an example of the difference between the resolution of a telescope and its magnification. A sketch might be the most useful way of answering. Better magnification makes objects appear larger, while better resolution makes objects appear sharper. 15. Give at least one reason why telescopes using mirrors can be built to a larger size than telescopes using lenses. Mirrors can be supported from behind, making them easier to support. Also, mirrors don t have to be made as perfectly as lenses. 16. What is the difference between the way planetesimals grow and the way protoplanets grow? Planetesimals grow via collisions and sticking together, protoplanets grow via the gravitational accretion process. 2
3 17. Can the iron meteorites come from differentiated parent bodies? Why or why not? Yes, because the irons are metals and it s the metals of high density that sink to the center of a differentiated body. 18. In a sentence or two, explain the scientific significance of meteorites. They represent the elemental composition of the primordial solar system. 19. What role did Bode s Law play in the discovery of asteroids? Because the law indicated there was a gap between Mars and Jupiter, it led to a search for the missing planet, which resulted in the accidental discovery of Ceres. 20. Other than taking photos, name two methods by which we can determine the shapes of asteroids. Radar imaging and occultations. Slightly longer answer questions (4 points each): 21. Make a sketch of the celestial sphere showing the locations of the equinoxes and the solstices. I ll show you in class again, if you wish. 22. How did the ancient Greeks measure the size of the Earth? By noticing that the Sun at noon on the summer solstice was directly overhead (i.e., at the zenith) when standing in Syene. Meanwhile, in Alexandria, the Sun was 7º away from the zenith. This difference of 7º divided by 360º corresponded to the distance between the two cities divided by the circumference of the Earth, 2πR. Thus, they could solve for R, the radius of the Earth. 23. Suppose you lived on the Earth-facing side of the Moon and your best friend lived on the Earth. When your friend was seeing a full moon, what phase would you see for Earth? Would it be daylight or dark where you live? You d see a new Earth phase. It d be daylight. 3
4 24. Again, suppose you lived on the Earth-facing side of the Moon and your best friend lived on the Earth. What would you see when people on Earth were experiencing an eclipse? Answer for both solar and lunar eclipses. When your friend was seeing a solar eclipse, you d be seeing a full Earth at what you considered to be nighttime. You wouldn t see an eclipse of the Earth because the Moon s shadow is not large enough to engulf the Earth. When your friend was seeing a lunar eclipse, you d be seeing an eclipse of the Sun because the Moon is entirely within the shadow cast by the Earth. 25. What were Galileo s two most important observational discoveries and what was their significance? The moons of Jupiter, indicating that not everything orbited the Earth, and the complete cycle of phases of Venus, demonstrating that Venus had to orbit the Sun (not the Earth). 26. You get X-rays of your teeth at the dentist s office. You see visible light with your eyes. Which of these two types of electromagnetic radiation has the greater wavelength? Which has the higher frequency? Which has the greater energy? Which travels faster? Visible light has greater wavelengths than X-rays, while X-rays have higher frequencies. Since they have higher frequencies, they also have greater energies. Both travel at the same speed, the speed of light. 27. The electron in a hydrogen atom jumps from the ground state to the first excited state. Has the atom absorbed or emitted energy? Is it more energy than if it had jumped from the first excited state to the second? The atom has absorbed energy. And, yes, it is more energy than if it had jumped from the first excited state to the second, because the spacing between adjacent levels, which corresponds to energy, decreases as the levels increase. 28. Describe how magnetic fields cause sunspots. The magnetic fields interact strongly with the charged particles in the convection zone of the Sun, thus diminishing their ability to undergo convection. This lessening of convection in the strong magnetic field regions reduces the amount of energy transported to the surface, thus making those regions appear relatively dark compared to the normal photosphere. Those dark regions are the sunspots. 4
5 29. Which group of meteorites is more common, falls or finds? Which group (falls or finds) are the Antarctic meteorites most like? Which group of meteorites is more common, primitive stones or irons? Finds are much more common. The distribution of Antarctic meteorites is more like the falls, with the large majority of them being the primitive stones. But, of course, most of them are finds. The last question is poorly worded: the true distribution of meteorites is probably more like the falls, thus primitive stones are more common in that sense, but since finds far outnumber falls and there are more irons among the finds than there are primitive stones, then answering irons would be acceptable, too. 30. Why, despite the fact that the Kirkwood gaps are clearly demonstrable, does the asteroid belt seem to have no physical gaps in it? There are no physical gaps in the asteroid belt because the asteroids have very eccentric elliptical orbits which carry them through the gaps one might expect from the Kirkwood gaps in the orbital periods. Problems (10 points each): 31. Although the asteroid Ida is not a sphere, suppose it were shaped that way and had a radius of 20 km and a density of 2.6 g/cm 3. (a) What is the volume of Ida (in cubic centimeters)? The volume is 4/3 π R 3 = cm 3. (b) What is its mass (in grams and in kilograms)? The mass is density volume = g = kg. (c) The escape speed is given by V esc = (2GM/R), where G = m 3 /(kg s 2 ). If Roger Clemens (famous baseball pitcher) were standing on Ida, could he throw a baseball off of Ida, never to return? He can throw the ball approximately 44 m/sec. Be sure to keep all of your units straight, i.e., for this part of the problem use meters, kilograms and seconds. V esc = (2GM/R) = ( m 3 /(kg s 2 ) kg /20,000 m) = 24 m/s, which is less than the speed that Clemens can throw. So, yes, he could throw a baseball off of Ida. 5
6 32. Consider a rock that contains some U-238 (which decays into Pb-206 with a half-life of 4.47 billion years). Pb-204 is non-radiogenic (not produced by radioactive decay). (a) If we had been present when this rock first solidified and we had taken samples from different parts of the rock, would the ratios of Pb-206 to Pb-204 have been the same in all of the samples? What about the ratios of U-238 to Pb-204? Yes, the Pb-206 to Pb-204 ratios would have been the same in all of the samples, since the two are isotopes of the same element. The ratios of U-238 to Pb-204 would not have to be the same. (b) How much of the original amount of U-238 is left today if the rock formed years ago? The half-life of U-238 is 4.47 billion years, so, using N f /N i = 1/2 (age/half-life), we get N f /N i = _ (2.235/4.47) = _ (1/2) = 0.71 = 71%. 6
Exam# 1 Review Gator 1 Keep the first page of the exam. Scores will be published using the exam number Chapter 0 Charting the Heavens
Exam# 1 Review Exam is Wednesday October 11 h at 10:40AM, room FLG 280 Bring Gator 1 ID card Bring pencil #2 (HB) with eraser. We provide the scantrons No use of calculator or any electronic device during
More informationAstronomy I Exam I Sample Name: Read each question carefully, and choose the best answer.
Name: Read each question carefully, and choose the best answer. 1. During a night in Schuylkill Haven, most of the stars in the sky (A) are stationary through the night. (B) the actual motion depends upon
More informationAstronomy 101 Test 1 Review FOUNDATIONS
Astronomy 101 Test 1 Review FOUNDATIONS Scientists use the metric system to measure things. It is based on powers ten, and is thus more logical than our everyday Imperial system. The kilogram (or gram),
More informationChapter 26 Section 1 pages Directed Reading Section: Viewing the Universe
Name: Period: Chapter 26 Section 1 pages 659-666 Directed Reading Section: Viewing the Universe 1. How did observations of the sky help sailors in the past? 2. What is the main reason people study the
More informationExam #1 Covers material from first day of class, all the way through Tides and Nature of Light Supporting reading chapters 1-5 Some questions are
Exam #1 Covers material from first day of class, all the way through Tides and Nature of Light Supporting reading chapters 1-5 Some questions are concept questions, some involve working with equations,
More informationa. 0.1 AU b. 10 AU c light years d light years
1 AST104 Sp2006: EXAM 1 Multiple Choice Questions: Mark the best answer choice on the bubble form. Read all answer choices before making selection. (No credit given when multiple answers are marked.) 1.
More informationASTRONOMY. S6E1 a, b, c, d, e, f S6E2 a, b, c,
ASTRONOMY S6E1 a, b, c, d, e, f S6E2 a, b, c, UNIVERSE Age 13.7 billion years old The Big Bang Theory Protons and Neutrons formed hydrogen and helium. This created heat that formed the stars. Other elements
More informationAST Section 2: Test 1
AST1002 - Section 2: Test 1 Date: 10/06/2009 Name: Equations: c = λ f, λ peak = Question 1: A star with a declination of +40.0 degrees will be 1. east of the vernal equinox. 2. west of the vernal equinox.
More informationASTR : Stars & Galaxies (Spring 2019)... Study Guide for Midterm 1
ASTR-1200-01: Stars & Galaxies (Spring 2019)........................ Study Guide for Midterm 1 The first midterm exam for ASTR-1200 takes place in class on Wednesday, February 13, 2019. The exam covers
More informationMidterm 1. - Covers Ch. 1, 2, 3, 4, & 5 (HW 1, 2, 3, & 4) ** bring long green SCANTRON 882 E short answer questions (show work)
Midterm 1 - Covers Ch. 1, 2, 3, 4, & 5 (HW 1, 2, 3, & 4) - 20 multiple choice/fill-in the blank ** bring long green SCANTRON 882 E - 10 short answer questions (show work) - formula sheet will be included
More informationExam #1 Study Guide (Note this is not all the information you need to know for the test, these are just SOME of the main points)
Exam #1 Study Guide (Note this is not all the information you need to know for the test, these are just SOME of the main points) Moon Phases Moon is always ½ illuminated by the Sun, and the sunlit side
More informationAstronomy. Study of objects in space such as the Sun, stars, planets, comets, gas, & galaxies. *Also, the Earth s place in the universe.
Astronomy Study of objects in space such as the Sun, stars, planets, comets, gas, & galaxies. *Also, the Earth s place in the universe. Universe = everything that exists Disclaimer: Astrology is NOT science!!!
More informationD. A system of assumptions and principles applicable to a wide range of phenomena that has been repeatedly verified
ASTRONOMY 1 EXAM 1 Name Identify Terms - Matching (20 @ 1 point each = 20 pts.) 1 Solar System G 7. aphelion N 14. eccentricity M 2. Planet E 8. apparent visual magnitude R 15. empirical Q 3. Star P 9.
More informationEarly Theories. Early astronomers believed that the sun, planets and stars orbited Earth (geocentric model) Developed by Aristotle
Planetary Motion Early Theories Early astronomers believed that the sun, planets and stars orbited Earth (geocentric model) Developed by Aristotle Stars appear to move around Earth Observations showed
More informationLecture #4: Plan. Early Ideas of the Heavens (cont d): Geocentric Universe Heliocentric Universe
Lecture #4: Plan Early Ideas of the Heavens (cont d): Shape & size of the Earth Size & distance of Moon & Sun Geocentric Universe Heliocentric Universe Shape of the Earth Aristotle (Greece, 384 322 B.C.)
More informationName: Exam 1, 9/30/05
Multiple Choice: Select the choice that best answers each question. Write your choice in the blank next to each number. (2 points each) 1. At the North Pole in mid-november, the sun rises at a. North of
More informationAstronomy 1001/1005 Midterm (200 points) Name:
Astronomy 1001/1005 Midterm (00 points) Name: Instructions: Mark your answers on this test AND your bubble sheet You will NOT get your bubble sheet back One page of notes and calculators are allowed Use
More informationAst ch 4-5 practice Test Multiple Choice
Ast ch 4-5 practice Test Multiple Choice 1. The distance from Alexandria to Syene is about 500 miles. On the summer solstice the sun is directly overhead at noon in Syene. At Alexandria on the summer solstice,
More informationPHYS 160 Astronomy Test #1 Fall 2017 Version B
PHYS 160 Astronomy Test #1 Fall 2017 Version B 1 I. True/False (1 point each) Circle the T if the statement is true, or F if the statement is false on your answer sheet. 1. An object has the same weight,
More informationPosition 3. None - it is always above the horizon. Agree with student 2; star B never crosses horizon plane, so it can t rise or set.
Position 3 None - it is always above the horizon. N E W S Agree with student 2; star B never crosses horizon plane, so it can t rise or set. Imaginary plane No; the Earth blocks the view. Star A at position
More informationName and Student ID Section Day/Time:
AY2 - Overview of the Universe - Midterm #1 - Instructor: Maria F. Duran Name and Student ID Section Day/Time: 1) Imagine we ve discovered a planet orbiting another star at 1 AU every 6 months. The planet
More informationLecture 3: History of Astronomy. Astronomy 111 Monday September 4, 2017
Lecture 3: History of Astronomy Astronomy 111 Monday September 4, 2017 Reminders Labs start this week Homework #2 assigned today Astronomy of the ancients Many ancient cultures took note of celestial objects
More informationa. 1/3 AU b. 3 AU 5. Meteor showers occur
1 AST104 Sp. 2006: WELCOME TO EXAM 3 Multiple Choice Questions: Mark the best answer choice on the answer form. Read all answer choices before making selection. CHECK YOUR WORK CAREFULLY BEFORE HANDING
More informationExam 1 Astronomy 114. Part 1
Exam 1 Astronomy 114 Part 1 [1-40] Select the most appropriate answer among the choices given. 1. If the Moon is setting at 6AM, the phase of the Moon must be (A) first quarter. (B) third quarter. (C)
More informationF = ma P 2 = a 3 (M + m) P 2 = a 3. max T = 2900 K m
Summer 2013 Astronomy - Test 1 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 informationPractice Test DeAnza College Astronomy 04 Test 1 Spring Quarter 2009
Practice Test DeAnza College Astronomy 04 Test 1 Spring Quarter 2009 Multiple Choice Identify the letter of the choice that best completes the statement or answers the question. Mark answer on Scantron.
More informationChapter 2. The Rise of Astronomy. Copyright (c) The McGraw-Hill Companies, Inc. Permission required for reproduction or display.
Chapter 2 The Rise of Astronomy Copyright (c) The McGraw-Hill Companies, Inc. Permission required for reproduction or display. Periods of Western Astronomy Western astronomy divides into 4 periods Prehistoric
More informationAST 101 INTRODUCTION TO ASTRONOMY SPRING MIDTERM EXAM 1 TEST VERSION 1 ANSWERS NOTE: Question 20 Fixed
AST 101 INTRODUCTION TO ASTRONOMY SPRING 2008 - MIDTERM EXAM 1 TEST VERSION 1 ANSWERS NOTE: Question 20 Fixed Multiple Choice. In the blanks provided before each question write the letter for the phrase
More information3) During retrograde motion a planet appears to be A) dimmer than usual. B) the same brightness as usual C) brighter than usual.
Descriptive Astronomy (ASTR 108) Exam 1 B February 17, 2010 Name: In each of the following multiple choice questions, select the best possible answer. In the line on the scan sheet corresponding to the
More information1) Kepler's third law allows us to find the average distance to a planet from observing its period of rotation on its axis.
Descriptive Astronomy (ASTR 108) Exam 1 A February 17, 2010 Name: In each of the following multiple choice questions, select the best possible answer. In the line on the scan sheet corresponding to the
More informationBenefit of astronomy to ancient cultures
Benefit of astronomy to ancient cultures Usefulness as a tool to predict the weather (seasons) Usefulness as a tool to tell time (sundials) Central Africa (6500 B.C.) Alignments Many ancient cultures built
More informationa. 0.5 AU b. 5 AU c. 50 AU d.* AU e AU
1 AST104 Sp04: WELCOME TO EXAM 1 Multiple Choice Questions: Mark the best answer choice. Read all answer choices before making selection. (No credit given when multiple answers are marked.) 1. A galaxy
More informationGravitation and the Motion of the Planets
Gravitation and the Motion of the Planets 1 Guiding Questions 1. How did ancient astronomers explain the motions of the planets? 2. Why did Copernicus think that the Earth and the other planets go around
More informationScience Period. Astronomy Unit PracticeTest 2014 Sci 7
Name: Date: Science Period Astronomy Unit PracticeTest 2014 Sci 7 Directions: Write the letter of the BEST answer on the appropriate space on the answer sheet. 2 points each 1.The model in which SUN is
More informationUnit 1: The Earth in the Universe
Unit 1: The Earth in the Universe 1. The Universe 1.1. First ideas about the Universe 1.2. Components and origin 1.3. Sizes and distances 2. The Solar System 3. The planet Earth 3.1. Movements of the Earth
More informationChapter. Origin of Modern Astronomy
Chapter Origin of Modern Astronomy 22.1 Early Astronomy Ancient Greeks Astronomy is the science that studies the universe. It includes the observation and interpretation of celestial bodies and phenomena.
More informationThe Solar System. Chapter Test A. Multiple Choice. Write the letter of the correct answer on the line at the left.
The Solar System Chapter Test A Multiple Choice Write the letter of the correct answer on the line at the left. 1. 2. 3. 4. 5. The fact that each planet s orbit is an ellipse was discovered by a. Copernicus.
More informationChapter: The Earth-Moon-Sun System
Chapter 7 Table of Contents Chapter: The Earth-Moon-Sun System Section 1: Earth in Space Section 2: Time and Seasons Section 3: Earth s Moon 1 Earth in Space Earth s Size and Shape Ancient Measurements
More information1/3/12. Chapter: The Earth-Moon-Sun System. Ancient Measurements. Earth s Size and Shape. Ancient Measurements. Ancient Measurements
// Table of Contents Chapter: The Earth-Moon-Sun System Section : Chapter 7 Section : Section : Earth s Size and Shape Ancient Measurements First, no matter where you are on Earth, objects fall straight
More informationBrock University. Test 1, May 2014 Number of pages: 9 Course: ASTR 1P01 Number of Students: 500 Date of Examination: May 21, 2014
Brock University Test 1, May 2014 Number of pages: 9 Course: ASTR 1P01 Number of Students: 500 Date of Examination: May 21, 2014 Number of hours: 50 min Time of Examination: 14:00 14:50 Instructor: B.Mitrović
More informationName: 12/20/05 Phys 010 Astronomy Final Exam Prof. Finn
Matching 1. 2. 3. 4. 5. 6. 7. 8. 9. 10. 11. 12. 13. 14. 15. 16. 17. 18. 19. 20. 21. 22. 23. 24. 25. 26. Multiple Choice 1. 2. 3. 4. 5. 6. 7. 8. 9. 10. 11. 12. 13. 14. 15. 16. 17. 18. 19. 20. 21. 22. 23.
More information12.1 Earth, Moon and Sun Interactions
12.1 Earth, Moon and Sun Interactions Humans have been aware of the relationships between the Earth, Sun and Moon for thousands of years, but only recently have we began to better understand the true nature
More informationGravitation and the Waltz of the Planets
Gravitation and the Waltz of the Planets Chapter Four Guiding Questions 1. How did ancient astronomers explain the motions of the planets? 2. Why did Copernicus think that the Earth and the other planets
More informationGravitation and the Waltz of the Planets. Chapter Four
Gravitation and the Waltz of the Planets Chapter Four Guiding Questions 1. How did ancient astronomers explain the motions of the planets? 2. Why did Copernicus think that the Earth and the other planets
More informationFCAT 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 informationThe point in an orbit around the Sun at which an object is at its greatest distance from the Sun (Opposite of perihelion).
ASTRONOMY TERMS Albedo Aphelion Apogee A measure of the reflectivity of an object and is expressed as the ratio of the amount of light reflected by an object to that of the amount of light incident upon
More informationThe Sun. How are these quantities measured? Properties of the Sun. Chapter 14
The Sun Chapter 14 The Role of the Sun in the Solar System > 99.9% of the mass Its mass is responsible for the orderly orbits of the planets Its heat is responsible for warming the planets It is the source
More information2) The number one million can be expressed in scientific notation as: (c) a) b) 10 3 c) 10 6 d)
Astronomy Phys 181 Midterm Examination Choose the best answer from the choices provided. 1) What is the range of values that the coordinate Declination can have? (a) a) -90 to +90 degrees b) 0 to 360 degrees
More informationSection 25.1 Exploring the Solar System (pages )
Name Class Date Chapter 25 The Solar System Section 25.1 Exploring the Solar System (pages 790 794) This section explores early models of our solar system. It describes the components of the solar system
More informationEXAM #2. ANSWERS ASTR , Spring 2008
EXAM #2. ANSWERS ASTR 1101-001, Spring 2008 1. In Copernicus s heliocentric model of the universe, which of the following astronomical objects was placed in an orbit around the Earth? The Moon 2. In his
More informationThe Universe and Galaxies
The Universe and Galaxies 16.1 http://dingo.care-mail.com/cards/flash/5409/galaxy.swf Universe The sum of all matter and energy that exists, that has ever existed, and that will ever exist. We will focus
More informationAstronomy Practice Test
Name: ate: 1. In laska, there are fewer hours of daylight in the winter than in the summer. Which statement best explains why this difference occurs?. The Sun burns hotter in the summer.. The Sun moves
More informationAST 103 Midterm 1 Review Exam is 3/3/08 in class
AST 103 Midterm 1 Review Exam is 3/3/08 in class Exam is closed book/closed notes. Formulas will be provided. Bring a No. 2 pencil for the exam and a photo ID. Calculators are OK, but will not be needed.
More informationASTRONOMY CURRICULUM Unit 1: Introduction to Astronomy
Chariho Regional School District - Science Curriculum September, 2016 ASTRONOMY CURRICULUM Unit 1: Introduction to Astronomy OVERVIEW Summary Students will be introduced to the overarching concept of astronomy.
More informationUseful Formulas and Values
Name Test 1 Planetary and Stellar Astronomy 2017 (Last, First) The exam has 20 multiple choice questions (3 points each) and 8 short answer questions (5 points each). This is a closed-book, closed-notes
More informationAstro 102 Spring 2008 Sample Prelim 1 Exam. Instructions. Name: Section Number: Name of TA:
A Astro 102 Spring 2008 Sample Prelim 1 Exam Name: Section Number: Name of TA: Instructions Read the instructions carefully before you begin, your grade may be penalized for failing to follow instructions.
More informationSunlight and its Properties Part I. EE 446/646 Y. Baghzouz
Sunlight and its Properties Part I EE 446/646 Y. Baghzouz The Sun a Thermonuclear Furnace The sun is a hot sphere of gas whose internal temperatures reach over 20 million deg. K. Nuclear fusion reaction
More informationCh. 22 Origin of Modern Astronomy Pretest
Ch. 22 Origin of Modern Astronomy Pretest Ch. 22 Origin of Modern Astronomy Pretest 1. True or False: Early Greek astronomers (600 B.C. A.D. 150) used telescopes to observe the stars. Ch. 22 Origin of
More informationASTR 138 Fall 2017 Exam 2 10/19/2017
ASTR 138 Fall 2017 Exam 2 10/19/2017 Wien's Law: λ max = C / T, where C = 2,900 in units of (micrometers*kelvins degrees) Newton's Universal Law of Gravitation: Force of Gravity = G M 1 M 2 / R 2 1) An
More information3. The diagram below shows the Moon at four positions in its orbit around Earth as viewed from above the North Pole.
1. Which object orbits Earth in both the Earth-centered (geocentric) and Sun-centered (heliocentric) models of our solar system? (1) Polaris (3) the Sun (2) Venus (4) the Moon 2. A cycle of Moon phases
More informationClass Notes: Astronomy
Name: Date: Period: Astronomy The Physical Setting: Earth Science Class Notes: Astronomy I. Apparent Motion Geocentric Universe -! Starts all rotate around the Earth on a single sphere at º/hour Planets
More informationPHYS 160 Astronomy Test #1 Name Answer Key Test Version A
PHYS 160 Astronomy Test #1 Name Answer Key Test Version A True False Multiple Choice 1. T 1. C 2. F 2. B 3. T 3. A 4. T 4. E 5. T 5. B 6. F 6. A 7. F 7. A 8. T 8. D 9. F 9. D 10. F 10. B 11. B 12. D Definitions
More informationES - Astronomy Part 2 Post-Test
ES - Astronomy Part 2 Post-Test True/False Indicate whether the statement is true or false. 1. Compared to the human eye, telescopes can collect light over longer periods of time. 2. The inner planets
More informationBROCK UNIVERSITY. 1. The observation that the intervals of time between two successive quarter phases of the Moon are very nearly equal implies that
BROCK UNIVERSITY Page 1 of 10 Test 1: November 2014 Number of pages: 10 Course: ASTR 1P01, Section 2 Number of students: 30 Examination date: 10 November 2014 Time limit: 50 min Time of Examination: 9:00
More informationReturn both exam and scantron sheet when you leave the gym
BROCK UNIVERSITY Page 1 of 17 Final Exam December 2017 Number of pages: 17 Course: ASTR 1P01, Section 1 Number of Students: 465 Date of Examination: December 13, 2017 Number of hours: 2 Time of Examination:
More informationOrigin of the Solar System
Solar nebula Formation of planetismals Formation of terrestrial planets Origin of the Solar System Announcements There will be another preceptor-led study group Wednesday at 10:30AM in room 330 of Kuiper
More informationTest 1 Review Chapter 1 Our place in the universe
Test 1 Review Bring Gator 1 ID card Bring pencil #2 with eraser No use of calculator or any electronic device during the exam We provide the scantrons Formulas will be projected on the screen You can use
More informationApparent Motion. How do celestial objects appear to move across the sky?
Apparent Motion How do celestial objects appear to move across the sky? 1 Apparent Motions Geocentric Universe - idea that Earth was at the center of the solar system Stars all rotate around the Earth
More informationAstronomy Unit Notes Name:
Astronomy Unit Notes Name: (DO NOT LOSE!) To help with the planets order 1 My = M 2 V = Venus 3 Eager = E 4 M = Mars 5 Just = J 6 Served = Saturn 7 Us = Uranus 8 N = N 1 Orbit: The path (usually elliptical)
More informationUnit 1 Discovering the Heavens I. Introduction to Astronomy A. Celestial Sphere
Unit 1 Discovering the Heavens I. Introduction to Astronomy A. Celestial Sphere celestial sphere - a model that represents the real sky with the Earth at the center - used to help visualize positions of
More informationRemember that for one of your observing projects you can go to a star party (stargazing). This is available at the Lawrence Hall of Science every 1st
Observing Project Remember that for one of your observing projects you can go to a star party (stargazing). This is available at the Lawrence Hall of Science every 1st and 3rd Saturday of the month. For
More informationPhysics Unit 7: Circular Motion, Universal Gravitation, and Satellite Orbits. Planetary Motion
Physics Unit 7: Circular Motion, Universal Gravitation, and Satellite Orbits Planetary Motion Geocentric Models --Many people prior to the 1500 s viewed the! Earth and the solar system using a! geocentric
More informationMar 22, INSTRUCTIONS: First ll in your name and social security number (both by printing
ASTRONOMY 0089: EXAM 2 Class Meets M,W,F, 1:00 PM Mar 22, 1996 INSTRUCTIONS: First ll in your name and social security number (both by printing and by darkening the correct circles). Sign your answer sheet
More informationObserving the Universe for Yourself
Observing the Universe for Yourself Figure 6-20 Solar-System Formation What does the universe look like from Earth? With the naked eye, we can see more than 2,000 stars as well as the Milky Way. A constellation
More informationDirected Reading. Section: Viewing the Universe THE VALUE OF ASTRONOMY. Skills Worksheet. 1. How did observations of the sky help farmers in the past?
Skills Worksheet Directed Reading Section: Viewing the Universe 1. How did observations of the sky help farmers in the past? 2. How did observations of the sky help sailors in the past? 3. What is the
More informationASTRONOMY 1010 Exam 1 September 21, 2007
ASTRONOMY 1010 Exam 1 September 21, 2007 Name Please write and mark your name and student number in the Scantron answer sheet. FILL THE BUBBLE IN THE "TEST FORM" BOX CORRESPONDING TO YOUR TEST VERSION
More informationChapter 3 The Solar System
Name: Date: Period: Chapter 3 The Solar System Section 1 Observing the Solar System (pp. 72-77) Key Concepts What are the geocentric and heliocentric systems? How did Copernicus, Galileo, and Kepler contribute
More informationAstronomy 201 Review 1 Answers
Astronomy 201 Review 1 Answers What is temperature? What happens to the temperature of a box of gas if you compress it? What happens to the temperature of the gas if you open the box and let the gas expand?
More informationTHE UNIVERSE AND THE EARTH
ESO1 THE UNIVERSE AND THE EARTH Unit 1 What is the Universe like? Universe theories Ideas about the Universe: Geocentric theory Aristotle (B.C) and Ptolomy (A.D) Heliocentric theory Copernicus in 1542
More information1 of 5 5/2/2015 5:50 PM
1 of 5 5/2/2015 5:50 PM 1. A comet that has a semi-major axis of 100 AU must have a period of about 10 years. 20 years. 100 years. 1000 years. 2. Astronomers believe chondrite meteorites are about 4.6
More informationMeteorites. A Variety of Meteorite Types. Ages and Compositions of Meteorites. Meteorite Classification
Meteorites A meteor that survives its fall through the atmosphere is called a meteorite Hundreds fall on the Earth every year Meteorites do not come from comets First documented case in modern times was
More information( ) a3 (Newton s version of Kepler s 3rd Law) Units: sec, m, kg
Astronomy 18, UCSC Planets and Planetary Systems Generic Mid-Term Exam (A combination of exams from the past several times this class was taught) This exam consists of two parts: Part 1: Multiple Choice
More informationThings to do today. Terminal, Astronomy is Fun. Lecture 24 The Science of Astronomy. Scientific Thinking. After this lecture, please pick up:
Things to do today After this lecture, please pick up: Review questions for the final exam Homework#6 (due next Tuesday) No class on Thursday (Thanksgiving) Final exam on December 2 (next Thursday) Terminal,
More informationTopic 1: Earth s Motion Topic 2: The Moon Earth s Satellite Topic 3: Solar System Topic 4: The Planets Topic 5: Stars & Galaxies
Topic 1: Earth s Motion Topic 2: The Moon Earth s Satellite Topic 3: Solar System Topic 4: The Planets Topic 5: Stars & Galaxies Topic 1: Earth s Motion Essential Question: What causes the cycle of seasons
More informationSolar System Formation/The Sun
Solar System Formation/The Sun Objective 4 Examine the orbital paths of planets and other astronomical bodies (comets and asteroids). Examine the theories of geocentric and heliocentric models and Kepler
More informationSelected Topics Starry, Starry Night. Exploring the Universe of Science 1
Selected Topics Starry, Starry Night 2015 Exploring the Universe of Science 1 Revolution & Rotation Key concepts: What is the difference between revolution vs. rotation? Describe the basis for day, month,
More informationWhat is in outer space?
What is in outer space? Celestial Objects are any natural objects that move through space. Star:_a huge sphere of gas in space _Nuclear fusion within stars give off enormous amounts of energy such as light
More informationLunar Eclipse. Solar Eclipse
Lunar Eclipse SUN Moon Solar Eclipse SUN SUN Moon Total solar eclipse Partial solar eclipse Moon Phases What does the moon look like from at each position? G H F A E B D C SUNLIGHT Refracting Telescopes
More informationb. Remember, Sun is a second or third generation star the nebular cloud of dust and gases was created by a supernova of a preexisting
1. Evolution of the Solar System Nebular hypothesis, p 10 a. Cloud of atoms, mostly hydrogen and helium b. Gravitational collapse contracted it into rotating disc c. Heat of conversion of gravitational
More informationExercise 3: The history of astronomy
Astronomy 100 Name(s): Exercise 3: The history of astronomy In the previous exercise, you saw how the passage of time is intimately related to the motion of celestial objects. This, of course, led many
More informationAST101IN Final Exam. 1.) Arrange the objects below from smallest to largest. (3 points)
Name: Possibly useful formulae: AST101IN Final Exam F g = Gm 1 m 2 /r 2 p 2 =a 3 F=ma E=mc 2 1.) Arrange the objects below from smallest to largest. (3 points) The sun The Earth The universe The Milky
More informationrefractors satellite electromagnetic radiation
Chapter 19 Exploring Space space probe reflectors mirror refractors satellite electromagnetic radiation light lens thrust 1. All radiation is classified by wavelength in the. 2. Two types of telescopes
More informationAST 2010 Descriptive Astronomy Study Guide Exam I
AST 2010 Descriptive Astronomy Study Guide Exam I Wayne State University 1 Introduction and overview Identify the most significant structures in the universe: Earth, planets, Sun, solar system, stars,
More informationHNRS 227 Fall 2006 Chapter 13. What is Pluto? What is a Planet? There are two broad categories of planets: Terrestrial and Jovian
Key Points of Chapter 13 HNRS 227 Fall 2006 Chapter 13 The Solar System presented by Prof. Geller 24 October 2006 Planets Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, Neptune Dwarf Planets Pluto,
More informationStellar Astronomy Sample Questions for Exam 3
Stellar Astronomy Sample Questions for Exam 3 Chapter 7 1. A protostar is formed by a) the rapid expansion of gas from an exploding star. b) the gravitational collapse of a rotating interstellar cloud.
More informationToday FIRST HOMEWORK DUE. Ancient Astronomy. Competing Cosmologies. Geocentric vs. Heliocentric. Ptolemy vs. copernicus.
Today FIRST HOMEWORK DUE Ancient Astronomy Competing Cosmologies Geocentric vs. Heliocentric Ptolemy vs. copernicus Retrograde Motion Phases of Venus Galileo 1 3.1 The Ancient Roots of Science Our goals
More informationInvestigations in Earth and Space Science Semester Review: Unit 1 and Unit 2
IESS Unit 1: Solar Energy & Fluid Circulation Review Directions: Write the answer to each question in the box to the right of the question. Fold your paper along the line and use this as a review sheet!
More informationASTRONOMY LECTURE NOTES MIDTERM REVIEW. ASTRONOMY LECTURE NOTES Chapter 1 Charting the Heavens
ASTRONOMY LECTURE NOTES MIDTERM REVIEW ASTRONOMY LECTURE NOTES Chapter 1 Charting the Heavens How Do We Locate Objects in the Sky? Local-Sky Coordinates versus Celestial-Sphere Coordinates When the sky
More informationd. Galileo Galilei i. Heard about lenses being used to magnify objects 1. created his own telescopes to 30 power not the inventor! 2. looked
1. Age of Reason a. Nicolaus Copernicus 1473-1543 i. Commenteriolus manuscript circulated from 1512 1. unpublished 2. Heliocentric hypothesis ii. On the Revolutions of the Planets published year of his
More informationBROCK UNIVERSITY. 1. The observation that the intervals of time between two successive quarter phases of the Moon are very nearly equal implies that
BROCK UNIVERSITY Page 1 of 10 Test 1: November 2014 Number of pages: 10 Course: ASTR 1P01, Section 2 Number of students: 961 Examination date: 7 November 2014 Time limit: 50 min Time of Examination: 17:00
More information