If Earth had no tilt, what else would happen?
|
|
- Eugenia Parrish
- 6 years ago
- Views:
Transcription
1 A more in depth explanation from last week: If Earth had no tilt, what else would happen? The equator would be much hotter due to the direct sunlight which would lead to a lower survival rate and little life. The poles would receive less direct light and thus be colder making the survival rate there lower as well. The species would have evolved differently (micro-evolution), thus different life would be on Earth. But we would have a habitable zone between the poles and the equator, but unfortunately it would be a smaller habitable region than we have now.
2 Solar & Sidereal Motion and Models of the Solar System (Week 7)
3 Why does Sidereal Motion (Time) matter? It is a system of timekeeping used by astronomers, useful because a star rises and sets at the same sidereal time every day, but not at the same solar (synodic) time which is our typical time system. Because local sidereal time is the right ascension (RA) of a star on the observers meridian, it is a direct indication of whether a celestial object of known right ascension is observable at that instant. Our clocks are based upon Solar time and we measure stars rising about 4 minutes earlier each day. Why does this happen? The short version because of Earth s motion around the Sun. What types of motion can be measured with the Sidereal system? Sidereal Day, Sidereal Periods of Celestial Bodies to include the Sidereal Month of the Moon
4 Sidereal Time vs. Solar (Synodic) Time A time-keeping system astronomers use to keep track of the direction to point their telescopes to view a given star in the night sky. One sidereal day corresponds to the time taken for the Earth to rotate once with respect to a distant star. A time keeping system based upon when the Sun is highest in the sky (~12 pm). One solar day corresponds to the time taken for the Earth to rotate once with respect to the Sun.
5 Prior to Tutorial completion, the Instructor will: a) define parallel lines b) define period c) define high noon (in the diagram below) d) in the diagram below illustrate a 360 degree rotation of person/earth with a ruler (students use toothpick) while Earth is still orbiting the Sun & sketch the Earth/person in a later snapshot e) help students visualize distant stars (see top of page) and have them draw similar stars on their Tutorial f) provide every student with a toothpick
6 Solar vs. Sidereal Day - Lecture Tutorial (pg 11-12; minutes) STOP the Tutorial just after the Note: on page 12, put name on it and turn it in to Instructor next Tuesday. Be ready to struggle a little bit, this is a discovery! Work with a partner! Read the instructions and questions carefully. Discuss the concepts and your answers with one another. Come to a consensus answer you both agree on. If you get stuck or are not sure of your answer, ask another group. If you get really stuck or don t understand what the Lecture Tutorial is asking, ask one of us for help.
7 Follow up to Tutorial Using the angle that the Earth sweeps out as it goes once around the Sun and the number of days in a year, the number of degrees per day that Earth moves in orbit about the Sun is: A) 365 days/180 degrees = 2 days/degree B) 365 days/180 degrees = 0.5 degrees/day C) 360 degrees/365 days = 1 degree/day D) 360 degrees/24 hours = 15 degrees/hour E) none of the above ANSWER: C or 1 degree/day for Earth revolving about the Sun [Realize that choice D or 15 degrees/hour is the rotation rate of the Earth about its axis, which is also the rate the celestial sphere appears to rotate.]
8 Follow up to Tutorial During what type of a day does the Earth rotate through slightly more than 360 degrees? A) Synodic day which is 24 hrs B) Solar day which is less than 24 hrs C) Sidereal day which is less than 24 hrs D) Sidereal day which is more than 24 hrs E) Both A) & B) above ANSWER: A One solar/synodic day corresponds to the time taken for the Earth to rotate once with respect to the Sun which is more than 360 degrees and takes 24 hours.
9 Follow up to Tutorial During what type of a day does the Earth rotate through 360 degrees? A) Synodic day in 24 hrs B) Solar day in less than 24 hrs C) Sidereal day in less than 24 hrs D) Sidereal day in 24 hrs E) Both A) & B) above ANSWER: C One sidereal day corresponds to the time taken for the Earth to rotate once with respect to a distant star.
10 One sidereal day lasts approximately 23 hours and 56 minutes during which time the Earth rotates 360 degrees (~4 minutes shorter than a solar day). One solar (synodic) day lasts 24 hours during which time the Earth rotates more than 360 degrees.
11 Local Sidereal Time Clock Apparent Movement of a Star
12 Synodic (Solar) vs. Sidereal Period of the Moon ( & brief intro. to Moon phases)
13 In this video, be sure to: a) notice how the Earth s orbit around the Sun makes the Moon s sidereal period different from its synodic period b) try to identify several Moon phases at various points in the animation c) read the blue writing, see next slide for a snapshot of it
14
15 Sidereal vs. Synodic Period of the Moon (zooming in) Sidereal Period is days, Moon rotates to the purple line (which should be parallel to the leftmost red dotted line), 360 degrees; not back to New Moon - same phase as leftmost image Synodic Period is days, Moon rotates to the orange line, more than 360 degrees; back to the same phase (new moon) as leftmost image.
16 Models of the Solar System Retrograde Motion of the Planets Geocentric vs. Heliocentric Kepler s Laws
17 Planets were often called wandering stars because they seem to slowly move from one constellation to the next. East South Mars prograde & retrograde motion is in red between May 1 and Dec. 31 West
18 Retrograde Motion Models of the universe MUST adequately describe this retrograde motion!
19 What did the Greeks have to say about the motion of the Solar System? The astronomer must try his utmost to explain celestial motions by the simplest possible hypothesis; but if he fails to do so, he must choose whatever other hypotheses meet the case. -Ptolemy of Alexandria (140 A.D.)
20 Ptolemy He tried to create a model that would account for retrograde motion. He placed the planets in orbits (deferments) using epicycles. What is this Earth-centered theory called? Geocentric theory: (in Greek, geo means earth) which maintained that Earth was the center of the universe
21 For most of human history, we have thought the universe was geocentric. Copernicus devised the first comprehensive heliocentric cosmogony to successfully explain retrograde motion. Copernicus ( AD) Heliocentric theory: with the Sun at the center of the universe or solar system
22 Retrograde motion is an apparent motion caused when one planet moves from being behind another planet to being in front of the other planet.
23 Let s watch a movie(s) of this motion.
24 Tycho Brahe ( )
25 Tycho Brahe ( ) is known for - 1. First telescope observations of the sun 2. First sun centered scientific model of the solar system or universe 3. Being the world s best nakedeye astronomer 4. Creating first a theoretical model to explain planetary motions 5. Creating first a theoretical model for explaining gravity
26 Tycho Brahe ( ) is known for - 1. First telescope observations of the sun 2. First sun centered scientific model of the solar system or universe 3. Being the world s best naked-eye astronomer 4. Creating first a theoretical model to explain planetary motions 5. Creating first a theoretical model for explaining gravity
27 What do we mean by Greatest Naked-eye Astronomer? No telescope!
28 Scientists use parallax to measure distances.
29
30 Tycho Brahe measured distances using parallax that disproved ancient ideas about the heavens He observed a supernova in 1572 and with this showed that the heavens were both changing and had a dimension of distance; this troubled scholars who previously thought the heavens were unchanging. He showed that comets were objects that occurred in the region of the planets, not in Earth s atmosphere.
31 Johannes Kepler He was rumored to have hated Tycho Brahe and was in the relationship for the data. With that data he changed the understanding of motion of heavenly bodies forever.
32 Johannes Kepler is Known for - 1. First telescope observations of the sun 2. First sun centered scientific model of the solar system or universe 3. Being the world s best naked-eye astronomer 4. Creating the first theoretical model to explain planetary motions 5. Creating the first theoretical model for explaining gravity
33 Johannes Kepler is Known for - 1. First telescope observations of the sun 2. First sun centered scientific model of the solar system or universe 3. Being the world s best naked-eye astronomer 4. Creating first a theoretical model to explain planetary motions 5. Creating first a theoretical model for explaining gravity
34 Johannes Kepler Kepler s Three Laws of Planetary Motion
35 Eccentricity, e how squashed or out of round the ellipse is a number ranging from 0 for a circle to 1 for a straight line e = 0.02 e = 0.7 e = 0.9
36 Kepler s First Law: The orbit of a planet about the Sun is an Ellipse with the Sun at one focus.
37 What is the shape of Earth s orbit around the Sun? Earth, e = 0.016
38 Kepler s Second Law: A line joining a planet and the Sun sweeps out equal Areas in equal intervals of time.
39 Kepler's Second Law Movie &ns= 0
40 Kepler s SECOND LAW A line drawn from the planet to the Sun sweeps out equal Areas in equal times orbital speed is not constant for an ellipse only for a circle planets move faster when near the Sun (perihelion) planets move slower when they are far from the Sun (aphelion)
41 SECOND LAW The speed a planet travels during its orbit is related to the distance from the star When the planet is near the sun the planet goes faster than when the planet is farther from the sun Planet travels slow here Planet travels fast here
42 Kepler s THIRD LAW The size of the orbit (a is the length of its orbit s semi-major axis) determines the orbital period, T a 3 AU= T 2 years Thus planets that orbit near the Sun orbit with shorter periods (T) than planets that are far from the Sun
43 THIRD LAW The size of the orbit determines the orbital period planets that orbit near the Sun orbit with shorter periods than planets that are far from the Sun
44 Kepler s Third Law: The square of a planet s sidereal (orbital) period is proportional to the cube of the length of its orbit s semimajor axis (T 2 a 3 ). =,T T 2
45 The Second and Third Laws The Second Law tells us what a particular planet does when it orbits a Star The planet will move faster when it is close to the Sun and slower when it is farther from the Sun The Third Law how the orbital periods are related to the orbital distances for all the planets in the Solar System planets that are in an orbit located near the Sun have short orbital periods planets that are in an orbit located far from the Sun have long orbital periods
46 THIRD LAW The size of the orbit determines the orbital period planets that orbit near the Sun orbit with shorter periods than planets that are far from the Sun T = ~ 12 years T = 1 year
47 THIRD LAW The size of the orbit determines the orbital period planets that orbit near the Sun orbit with shorter periods than planets that are far from the Sun MASS DOES NOT MATTER Both have T = 1 year
48 According to Kepler s second law, a planet with an orbit like Earth s would: A. move faster when further from the Sun. B. move slower when closer to the Sun. C. experience a dramatic change in orbital speed from month to month. D. experience very little change in orbital speed over the course of the year. E. none of the above.
49 Which of the following best describes what would happen to a planet s orbital speed if it s mass were doubled but it stayed at the same orbital distance? A. It would orbit half as fast. B. It would orbit less that half as fast. C. It would orbit twice as fast. D. It would orbit more than twice as fast. E. It would orbit with the same speed.
50 Kepler s second law says a line joining a planet and the Sun sweeps out equal areas in equal amounts of time. Which of the following statements means nearly the same thing? A. Planets move fastest when they are moving toward the Sun. B. Planets move equal distances throughout their orbit of the Sun. C. Planets move slowest when they are moving away from the Sun. D. Planets travel farther in a given time when they are closer to the Sun. E. Planets move the same speed at all points during their orbit of the Sun.
51 If a small weather satellite and the large International Space Station are orbiting Earth at the same altitude above Earth s surface, which of the following is true? A. The large space station has a longer orbital period. B. The small weather satellite has a longer orbital period. C. Each has the same orbital period
52 Kepler s 2 nd & 3 rd Laws - Lecture Tutorials: (pg 21-27) Work with a partner! Read the instructions and questions carefully. Discuss the concepts and your answers with one another. Come to a consensus answer you both agree on. If you get stuck or are not sure of your answer, ask another group. If you get really stuck or don t understand what the Lecture Tutorial is asking, ask one of us for help.
cosmogony geocentric heliocentric How the Greeks modeled the heavens
Cosmogony A cosmogony is theory about ones place in the universe. A geocentric cosmogony is a theory that proposes Earth to be at the center of the universe. A heliocentric cosmogony is a theory that proposes
More informationModels of the Solar System, Gravitation and the motion of the Planets A.K.A DEAD WHITE GUYS WEEK! 1/28/14
Models of the Solar System, Gravitation and the motion of the Planets A.K.A DEAD WHITE GUYS WEEK! 1/28/14 Cosmogony A cosmogony is theory about ones place in the universe. A geocentric cosmogony is a theory
More informationWhat was once so mysterious about planetary motion in our sky? We see apparent retrograde motion when we pass by a planet
What was once so mysterious about planetary motion in our sky? Planets usually move slightly eastward from night to night relative to the stars. You cannot see this motion on a single night. But sometimes
More informationLearning Objectives. one night? Over the course of several nights? How do true motion and retrograde motion differ?
Kepler s Laws Learning Objectives! Do the planets move east or west over the course of one night? Over the course of several nights? How do true motion and retrograde motion differ?! What are geocentric
More informationKepler s Laws of Orbital Motion. Lecture 5 January 30, 2014
Kepler s Laws of Orbital Motion Lecture 5 January 30, 2014 Parallax If distance is measured in parsecs then d = 1 PA Where PA is the parallax angle, in arcsec NOTE: The distance from the Sun to the Earth
More informationIntroduction To Modern Astronomy II
ASTR 111 003 Fall 2006 Lecture 03 Sep. 18, 2006 Introduction To Modern Astronomy II Introducing Astronomy (chap. 1-6) Planets and Moons (chap. 7-17) Ch1: Astronomy and the Universe Ch2: Knowing the Heavens
More informationKepler s Laws of Orbital Motion. Lecture 5 January 24, 2013
Kepler s Laws of Orbital Motion Lecture 5 January 24, 2013 Team Extra Credit Two teams: Io & Genius Every class (that is not an exam/exam review) will have a question asked to a random member of each team
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 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 informationPhases of the Moon. Two perspectives: On Earth, or outside the Moon s orbit. More Phases. What if we zoom out? Phases of the Moon Demo 2/3/17
Phases of the Moon The Moon goes through a set of phases about once every month Month comes from the word moon Time period of the phases (from Full Moon to Full Moon) is 29.5 days. The different phases
More informationLecture 13. Gravity in the Solar System
Lecture 13 Gravity in the Solar System Guiding Questions 1. How was the heliocentric model established? What are monumental steps in the history of the heliocentric model? 2. How do Kepler s three laws
More information18. Kepler as a young man became the assistant to A) Nicolaus Copernicus. B) Ptolemy. C) Tycho Brahe. D) Sir Isaac Newton.
Name: Date: 1. The word planet is derived from a Greek term meaning A) bright nighttime object. B) astrological sign. C) wanderer. D) nontwinkling star. 2. The planets that were known before the telescope
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 informationPHYS 155 Introductory Astronomy
PHYS 155 Introductory Astronomy - observing sessions: Sunday Thursday, 9pm, weather permitting http://www.phys.uconn.edu/observatory - Exam - Tuesday March 20, - Review Monday 6:30-9pm, PB 38 Marek Krasnansky
More informationIntroduction To Modern Astronomy I
ASTR 111 003 Fall 2006 Lecture 03 Sep. 18, 2006 Introduction To Modern Astronomy I Introducing Astronomy (chap. 1-6) Planets and Moons (chap. 7-17) Ch1: Astronomy and the Universe Ch2: Knowing the Heavens
More informationAnnouncements. Topics To Be Covered in this Lecture
Announcements! Tonight s observing session is cancelled (due to clouds)! the next one will be one week from now, weather permitting! The 2 nd LearningCurve activity was due earlier today! Assignment 2
More information1. The Moon appears larger when it rises than when it is high in the sky because
2-1 Copyright 2016 All rights reserved. No reproduction or distribution without the prior written consent of 1. The Moon appears larger when it rises than when it is high in the sky because A. you are
More informationAstronomy Notes Chapter 02.notebook April 11, 2014 Pythagoras Aristotle geocentric retrograde motion epicycles deferents Aristarchus, heliocentric
Around 2500 years ago, Pythagoras began to use math to describe the world around him. Around 200 years later, Aristotle stated that the Universe is understandable and is governed by regular laws. Most
More informationHow big is the Universe and where are we in it?
Announcements Results of clicker questions from Monday are on ICON. First homework is graded on ICON. Next homework due one minute before midnight on Tuesday, September 6. Labs start this week. All lab
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 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 informationEarth Science, 13e Tarbuck & Lutgens
Earth Science, 13e Tarbuck & Lutgens Origins of Modern Astronomy Earth Science, 13e Chapter 21 Stanley C. Hatfield Southwestern Illinois College Early history of astronomy Ancient Greeks Used philosophical
More informationMost of the time during full and new phases, the Moon lies above or below the Sun in the sky.
6/16 Eclipses: We don t have eclipses every month because the plane of the Moon s orbit about the Earth is different from the plane the ecliptic, the Earth s orbital plane about the Sun. The planes of
More informationChapter 02 The Rise of Astronomy
Chapter 02 The Rise of Astronomy Multiple Choice Questions 1. The moon appears larger when it rises than when it is high in the sky because A. You are closer to it when it rises (angular-size relation).
More informationDays of the week: - named after 7 Power (moving) objects in the sky (Sun, Moon, 5 planets) Models of the Universe:
Motions of the Planets ( Wanderers ) Planets move on celestial sphere - change RA, Dec each night - five are visible to naked eye Mercury, Venus, Mars, Jupiter, Saturn Days of the week: - named after 7
More informationTHE SUN AND THE SOLAR SYSTEM
Chapter 26 THE SUN AND THE SOLAR SYSTEM CHAPTER 26 SECTION 26.1: THE SUN S SIZE, HEAT, AND STRUCTURE Objectives: What is the Sun s structure and source of energy? Key Vocabulary: Fusion Photosphere Corona
More informationLecture #5: Plan. The Beginnings of Modern Astronomy Kepler s Laws Galileo
Lecture #5: Plan The Beginnings of Modern Astronomy Kepler s Laws Galileo Geocentric ( Ptolemaic ) Model Retrograde Motion: Apparent backward (= East-to-West) motion of a planet with respect to stars Ptolemy
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 informationYou should have finished reading Chapter 3, and started on chapter 4 for next week.
Announcements Homework due on Sunday at 11:45pm. Thank your classmate! You should have finished reading Chapter 3, and started on chapter 4 for next week. Don t forget your out of class planetarium show
More informationTest Bank for Life in the Universe, Third Edition Chapter 2: The Science of Life in the Universe
1. The possibility of extraterrestrial life was first considered A) after the invention of the telescope B) only during the past few decades C) many thousands of years ago during ancient times D) at the
More informationGravitation Part I. Ptolemy, Copernicus, Galileo, and Kepler
Gravitation Part I. Ptolemy, Copernicus, Galileo, and Kepler Celestial motions The stars: Uniform daily motion about the celestial poles (rising and setting). The Sun: Daily motion around the celestial
More informationAstronomy 1143 Quiz 1 Review
Astronomy 1143 Quiz 1 Review Prof. Pradhan September 7, 2017 I What is Science? 1. Explain the difference between astronomy and astrology. Astrology: nonscience using zodiac sign to predict the future/personality
More informationEarth Science, 11e. Origin of Modern Astronomy Chapter 21. Early history of astronomy. Early history of astronomy. Early history of astronomy
2006 Pearson Prentice Hall Lecture Outlines PowerPoint Chapter 21 Earth Science 11e Tarbuck/Lutgens This work is protected by United States copyright laws and is provided solely for the use of instructors
More informationHistory of Astronomy. PHYS 1411 Introduction to Astronomy. Tycho Brahe and Exploding Stars. Tycho Brahe ( ) Chapter 4. Renaissance Period
PHYS 1411 Introduction to Astronomy History of Astronomy Chapter 4 Renaissance Period Copernicus new (and correct) explanation for retrograde motion of the planets Copernicus new (and correct) explanation
More informationAstronomy 1010 Planetary Astronomy Sample Questions for Exam 1
Astronomy 1010 Planetary Astronomy Sample Questions for Exam 1 Chapter 1 1. A scientific hypothesis is a) a wild, baseless guess about how something works. b) a collection of ideas that seems to explain
More informationClaudius Ptolemaeus Second Century AD. Jan 5 7:37 AM
Claudius Ptolemaeus Second Century AD Jan 5 7:37 AM Copernicus: The Foundation Nicholas Copernicus (Polish, 1473 1543): Proposed the first modern heliocentric model, motivated by inaccuracies of the Ptolemaic
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 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 informationToday. Planetary Motion. Tycho Brahe s Observations. Kepler s Laws Laws of Motion. Laws of Motion
Today Planetary Motion Tycho Brahe s Observations Kepler s Laws Laws of Motion Laws of Motion In 1633 the Catholic Church ordered Galileo to recant his claim that Earth orbits the Sun. His book on the
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 informationName: Earth 110 Exploration of the Solar System Assignment 1: Celestial Motions and Forces Due on Tuesday, Jan. 19, 2016
Name: Earth 110 Exploration of the Solar System Assignment 1: Celestial Motions and Forces Due on Tuesday, Jan. 19, 2016 Why are celestial motions and forces important? They explain the world around us.
More informationWhat is a Satellite? A satellite is an object that orbits another object. Ex. Radio satellite, moons, planets
Planetary Orbit Planetary Orbits What shape do planets APPEAR to orbit the sun? Planets APPEAR to orbit in a circle. What shape do the planets orbit the sun??? Each planet Orbits the Sun in an ellipse
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 informationChapter 16 The Solar System
Chapter 16 The Solar System Finding the Standard Time and Date at Another Location Example When it is 12 noon in London, what is the standard time in Denver, Colorado (40 N, 105 W)? Section 15.3 Finding
More informationSpace Notes Covers Objectives 1 & 2
Space Notes Covers Objectives 1 & 2 Space Introduction Space Introduction Video Celestial Bodies Refers to a natural object out in space 1) Stars 2) Comets 3) Moons 4) Planets 5) Asteroids Constellations
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 informationAt Home Phases Demo. Astronomy 210. Section 1 MWF Astronomy Building. Geocentric vs. Heliocentric system. The Motion of the Planets
Astronomy 210 Section 1 MWF 1500-1550 134 Astronomy Building This Class (Lecture 4): Early Cosmology HW #1 Due on Friday! Next Class: You missed the first planetarium show. Cosmic Revolution Music: Twilight
More informationToday. Planetary Motion. Tycho Brahe s Observations. Kepler s Laws of Planetary Motion. Laws of Motion. in physics
Planetary Motion Today Tycho Brahe s Observations Kepler s Laws of Planetary Motion Laws of Motion in physics Page from 1640 text in the KSL rare book collection That the Earth may be a Planet the seeming
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 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 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 informationUnit 2: Celestial Mechanics
Unit 2: Celestial Mechanics The position of the Earth Ptolemy (90 168 AD) Made tables that allowed a user to locate the position of a planet at any past, present, or future date. In order to maintain circular
More informationIn so many and such important. ways, then, do the planets bear witness to the earth's mobility. Nicholas Copernicus
In so many and such important ways, then, do the planets bear witness to the earth's mobility Nicholas Copernicus What We Will Learn Today What did it take to revise an age old belief? What is the Copernican
More informationPlanetary Mechanics:
Planetary Mechanics: Satellites A satellite is an object or a body that revolves around another body due to the gravitational attraction to the greater mass. Ex: The planets are natural satellites of the
More informationlightyears observable universe astronomical unit po- laris perihelion Milky Way
1 Chapter 1 Astronomical distances are so large we typically measure distances in lightyears: the distance light can travel in one year, or 9.46 10 12 km or 9, 600, 000, 000, 000 km. Looking into the sky
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 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 informationAstro 210 Lecture 6 Jan 29, 2018
Astro 210 Lecture 6 Jan 29, 2018 Announcements HW2 due online in PDF, Friday 5:00 pm HW1 extended until 11:59pm today register your iclicker; link on course webpage first Planetarium shows Mon Feb 5 and
More informationName Period Date Earth and Space Science. Solar System Review
Name Period Date Earth and Space Science Solar System Review 1. is the spinning a planetary object on its axis. 2. is the backward motion of planets. 3. The is a unit less number between 0 and 1 that describes
More informationTopic 10: Earth in Space Workbook Chapters 10 and 11
Topic 10: Earth in Space Workbook Chapters 10 and 11 We can imagine all the celestial objects seen from Earth the sun, stars, the Milky way, and planets as being positioned on a celestial sphere. Earth
More informationPlanetary Orbits: Kepler s Laws 1/18/07
Planetary Orbits: Kepler s Laws Announcements The correct link for the course webpage http://www.lpl.arizona.edu/undergrad/classes/spring2007/giacalone_206-2 The first homework due Jan 25 (available for
More informationJanuary 19, notes.notebook. Claudius Ptolemaeus Second Century AD. Jan 5 7:37 AM
8.1 notes.notebook Claudius Ptolemaeus Second Century AD Jan 5 7:7 AM Copernicus: The Foundation Nicholas Copernicus (Polish, 147 154): Proposed the first modern heliocentric model, motivated by inaccuracies
More informationObservational Astronomy - Lecture 4 Orbits, Motions, Kepler s and Newton s Laws
Observational Astronomy - Lecture 4 Orbits, Motions, Kepler s and Newton s Laws Craig Lage New York University - Department of Physics craig.lage@nyu.edu February 24, 2014 1 / 21 Tycho Brahe s Equatorial
More information9/12/2010. The Four Fundamental Forces of Nature. 1. Gravity 2. Electromagnetism 3. The Strong Nuclear Force 4. The Weak Nuclear Force
The Four Fundamental Forces of Nature 1. Gravity 2. Electromagnetism 3. The Strong Nuclear Force 4. The Weak Nuclear Force The Universe is made of matter Gravity the force of attraction between matter
More informationChapter 2 The Science of Life in the Universe
In ancient times phenomena in the sky were not understood! Chapter 2 The Science of Life in the Universe The Ancient Greeks The Scientific Method Our ideas must always be consistent with our observations!
More informationAlien Skies. Todd Timberlake
Alien Skies Todd Timberlake Have you ever wanted to send your students to another planet? What would they see while looking up at the skies from their new home? Would they be able to interpret what they
More informationKepler s laws. Astronomy 101 Syracuse University, Fall 2018 Walter Freeman. October 2, Astronomy 101 Kepler s laws October 2, / 23
Kepler s laws Astronomy 101 Syracuse University, Fall 2018 Walter Freeman October 2, 2018 Astronomy 101 Kepler s laws October 2, 2018 1 / 23 And yet it moves. Galileo (attributed), on the Earth Astronomy
More informationLast time we finished Ch. 2
Last time we finished Ch. 2 Everyday astronomy 1. Patterns in the Sky 2. The Cause of Seasons 3. The Phases of the Moon 4. The Ancient Mystery of the Planets Last time we finished Ch. 2 You re getting
More informationThe History of Astronomy
The History of Astronomy The History of Astronomy Earliest astronomical record: a lunar calendar etched on bone from 6500 B.C. Uganda. Also we find early groups noted the Sun, Moon, Mercury, Venus, Earth,
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 informationPlato ( BC) All natural motion is circular Reason is more important than observation
Plato (428-348 BC) All natural motion is circular Reason is more important than observation Aristotle (384-322 BC) Physics elements earth water air fire quintessence Eratosthenes (276-195 BC) He measured
More informationA100 Exploring the Universe: The Invention of Science. Martin D. Weinberg UMass Astronomy
A100 Exploring the Universe: The Invention of Science Martin D. Weinberg UMass Astronomy astron100-mdw@courses.umass.edu September 09, 2014 Read: Chap 3 09/09/14 slide 1 Problem Set #1: due this afternoon
More informationASTR-1010: Astronomy I Course Notes Section III
ASTR-1010: Astronomy I Course Notes Section III Dr. Donald G. Luttermoser Department of Physics and Astronomy East Tennessee State University Edition 2.0 Abstract These class notes are designed for use
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 informationChapter 3 The Science of Astronomy
Chapter 3 The Science of Astronomy 3.1 The Ancient Roots of Science Our goals for learning: In what ways do all humans employ scientific thinking? How did astronomical observations benefit ancient societies?
More informationThe Science of Astronomy - Copernicus, Tycho, and Kepler. Reminder to take out your clicker and turn it on!
The Science of Astronomy - Copernicus, Tycho, and Kepler Reminder to take out your clicker and turn it on! Attendance Quiz Are you here today? Here! (a) yes (b) no (c) here? hear? hear, hear! Clicker Registration
More informationAncient Cosmology: A Flat Earth. Alexandria
Today Competing Cosmologies Geocentric vs. Heliocentric Ptolemy vs. copernicus Retrograde Motion Phases of Venus Galileo FIRST HOMEWORK DUE How d it work? Ancient Cosmology: A Flat Earth Here there be
More informationHistory of Astronomy. Historical People and Theories
History of Astronomy Historical People and Theories Plato Believed he could solve everything through reasoning. Circles and Spheres are good because they are perfect (never ending) and pleasing to the
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 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 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 information[05] Historical Perspectives (9/12/17)
1 [05] Historical Perspectives (9/12/17) Upcoming Items 1. Homework #2 due now. 2. Read Ch. 4.1 4.2 and do self-study quizzes. 3. Homework #3 due in one week. Ptolemaic system http://static.newworldencyclopedia.org/thumb/3/3a/
More informationAstronomy 100 Section 2 MWF Greg Hall. Outline. Total Lunar Eclipse Time Lapse. Homework #1 is due Friday, 11:50 a.m.!!!!!
Astronomy 100 Section 2 MWF 1200-1300 100 Greg Hall Leslie Looney Phone: 217-244-3615 Email: lwl @ uiuc. edu Office: Astro Building #218 Office Hours: MTF 10:30-11:30 a.m. or by appointment Homework #1
More informationAstronomy. 1. (3 pts.) What is meant by the apparent magnitude of a star?
Astronomy Name NaSc 109 Summer 2018 Exam 2 Don't Panic! Take a big deep breath... hold it... holllld it now let it out. Use your available time on this exam very efficiently; if you don't know an answer
More informationVenus Project Book, the Galileo Project, GEAR
1 Venus Project Book, the Galileo Project, GEAR Jeffrey La Favre November, 2013 Updated March 31, 2016 You have already learned about Galileo and his telescope. Recall that he built his first telescopes
More informationHow Astronomers Learnt that The Heavens Are Not Perfect
1 How Astronomers Learnt that The Heavens Are Not Perfect Introduction In this packet, you will read about the discoveries and theories which changed the way astronomers understood the Universe. I have
More informationCopernican Revolution. ~1500 to ~1700
~1500 to ~1700 Copernicus (~1500) Brahe (~1570) Kepler (~1600) Galileo (~1600) Newton (~1670) The Issue: Geocentric or Heliocentric Which model explains observations the best? Copernicus (~1500) Resurrected
More informationThis Week... Week 3: Chapter 3 The Science of Astronomy. 3.1 The Ancient Roots of Science. How do humans employ scientific thinking?
Week 3: Chapter 3 The Science of Astronomy This Week... The Copernican Revolution The Birth of Modern Science Chapter 2 Walkthrough Discovering the solar system Creating a clockwork Universe 3.1 The Ancient
More information2. Modern: A constellation is a region in the sky. Every object in the sky, whether we can see it or not, is part of a constellation.
6/14 10. Star Cluster size about 10 14 to 10 17 m importance: where stars are born composed of stars. 11. Galaxy size about 10 21 m importance: provide a stable environment for stars. Composed of stars.
More information6/17. Universe from Smallest to Largest:
6/17 Universe from Smallest to Largest: 1. Quarks and Leptons fundamental building blocks of the universe size about 0 (?) importance: quarks combine together to form neutrons and protons. One of the leptons
More informationOrigins of the Universe
Cosmology Origins of the Universe The study of the universe, its current nature, its origin, and evolution 1 2 The Theory Theory Expansion indicates a denser, hotter past uniform, hot gas that cools as
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 informationChapter 3 The Science of Astronomy. Copyright 2012 Pearson Education, Inc.
Chapter 3 The Science of Astronomy 1 3.1 The Ancient Roots of Science Our goals for learning: In what ways do all humans employ scientific thinking? How did astronomical observations benefit ancient societies?
More informationWas Ptolemy Pstupid?
Was Ptolemy Pstupid? Why such a silly title for today s lecture? Sometimes we tend to think that ancient astronomical ideas were stupid because today we know that they were wrong. But, while their models
More informationHow can we describe the motion of the sun in the sky? Where is the Sun at noon today? What about the path of the Sun?
The changing position of the Sun during the year! How can we describe the motion of the sun in the sky? X Zenith or overhead How can we describe the motion of the sun in the sky? Where is the Sun at noon
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 information,.~ Readlng ~ What,~,~~ is a geocentric system? Chapter3 J 73
Earth at the Center When the ancient Greeks watched the stars move across the sky, they noticed that the patterns of the stars didn t change. Although the stars seemed to move, they stayed in the same
More informationA100 Exploring the Universe: The Rise of Science. Martin D. Weinberg UMass Astronomy
A100 Exploring the Universe: The Rise of Science Martin D. Weinberg UMass Astronomy weinberg@astro.umass.edu September 11, 2012 Read: Chap 3 09/11/12 slide 1 Problem Set #1 due this afternoon at 5pm! Read:
More information