Chapter 8 MOONS, RINGS, AND PLUTO Small Worlds Among Giants
|
|
|
- Blaze Summers
- 5 years ago
- Views:
Transcription
1 Chapter 8 MOONS, RINGS, AND PLUTO Small Worlds Among Giants 8.1 THE RINGS AND MOONS OF SATURN Figure 65 shows the rings and moons when Titan is sufficiently close to Saturn to be included in the field. To obtain a better idea of the extremely large orbit for Titan, set a trail for Titan and follow its motion for a month or so. Placing the cursor on each moon and clicking the mouse will reveal the names of the moons. If it is desired to locate Titan, an easy way to find it is to decrease the magnitude setting with key F4 until only one moon remains. Figure 65. The rings and moons of Saturn. 62
2 8.2 WHAT GALILEO SAW OF SATURN S RINGS Saturn was visible only early evening in January If Galileo used a 1 diameter telescope with a magnification of 30, he could resolve about 2 arc seconds. See below. Following this for three years shows Saturn mostly edge on. Figure 66. Galileo s view of Saturn s rings. 8.3 HUYGENS VIEW In the four years leading up to 1659, Saturn moves from edge on to slightly tilted one way, back to edge on, to tilted substantially one way. Relying on better telescopes, Huygens surmised the explanation for Saturn s children. 8.4 A CLOCK IN THE SKY VIEW/Center Planet/Jupiter. VIEW/Coordinates/Ecliptic. COMPUTATION/Date & Time, Local Date & Time = 2005/1/1 00:00:00, Time Zone = 0.0. COMPUTATION/Precision, under Planet Position Computations select Correct for Light Time. ANIMATION/1 Minute. 63
3 Sample Data: Start Time span 2005/01/01 02:43: /01/02 21:12:00 42:29: /01/04 15:41:00 42:29: /01/06 10:09:00 42:28:00 Figure 67. Io will begin eclipsing at 2005/01/01 02:38:00. Note that Io is in the shadow of Jupiter at this time. The time span between eclipses is 42:29:00. 64
4 8.5 ECLIPSE CHARTS Chart showing data from Project 8.4 and a six-month prediction (some rows hidden). Start Time span 2005/01/01 02:43: /01/02 21:12:00 42:29: /01/04 15:41:00 42:29: /01/06 10:09:00 42:28:00 Predicted Start Time span 5/1/ :29 42:28:00 5/3/2005 4:57 42:28:00 5/4/ :25 42:28:00 5/6/ :53 42:28:00 5/8/ :21 42:28:00 5/10/2005 6:49 42:28:00 5/12/2005 1:17 42:28:00 *Hidden Rows 5/13/ :45 42:28:00 *Hidden Rows 5/15/ :13 42:28:00 5/17/2005 8:41 42:28:00 5/19/2005 3:09 42:28:00 5/20/ :37 42:28:00 5/22/ :05 42:28:00 5/24/ :33 42:28:00 5/26/2005 5:01 42:28:00 5/27/ :29 42:28:00 6 mo. Prediction 5/29/ :57 42:28:00 5/31/ :25 42:28: ACCURACY OF THE PREDICTIONS VIEW/Center Planet/Jupiter. VIEW/Coordinates/Ecliptic. COMPUTATION/Date & Time. Local Date & Time = 2000/05/25 2:48:00, Time Zone = 0.0 COMPUTATION/Precision, under Planet Position Computations select Correct for Light Time 65
5 Figure 68. The predicted eclipse on 5/31/ :25. Io will actually eclipse at 2005/05/31 11:44:00, a difference of 1 hour and 19 minutes. 8.7 CONJUNCTIONS COMPUTATION/Date & Time, Local Date & Time = 1962/02/05 00:00:00. View/Center Planet/Sun. Deselect Stars, Constellations, and Deep Sky Objects DRAW/Symbols & Grids. Under Draw Planets select Draw As = Stars Conjunction on February 5, 1962 at 06:00:00 (angular span of ~15 ). Note: the conjunctions are ambiguous and the exact positioning and times are location specific. From San Francisco on February 4, 1962 at 18:00:00 the conjunction can be seen along with a partial solar eclipse! 66
6 Aquarius Capricornus Mercury Moon Sun Jupiter Venus Saturn Mars Viewed from: Mt Wilson ' 36.0" W 34 13' 00.0" N Local time: 06:00: /02/05 JD Figure 69. The planets in conjunction. Field of view: 45 00' 00.0" Ecliptic Lon: Ecliptic Lat: Magnitudes: Single star Multiple star Variable star Deep sky objects: Open Glob Diff Plan Ga 8.8 A CONJUNCTION VIEWED FROM ABOVE COMPUTATION/Date & Time. Local Date & Time = 1962/02/05 00:00:00. COMPUTATION/Location. Select View from Object, Select, enter Sun, Find, Select, Offset. Distance = 60, select AU, Offset R.A. = , Offset Dec. = View/Center Planet/Sun. DRAW/Stars, Constellations, Deep Sky Objects and Symbols & Grids Off. Mars Venus Sun Mercury Earth Uranus Viewed from: AU from Sun Local time: Field of view: 06:00: ' 00.0" 1962/02/06 Ecliptic Lon: JD Ecliptic Lat: Magnitudes: Single star Multiple star Variable star Figure 70. Notice Uranus in this alignment. (As opposed to this top-down view, an edge-on view would yield different results.) 67
A. The moon B. The sun C. Jupiter D. Earth A. 1 B. 2 C. 3 D. 4. Sky Science Unit Review Konrad. Here is a selection of PAT style questions.
Sky Science Unit Review Konrad Here is a selection of PAT style questions. Use the following information to answer the next question 1. 2. The source of light that allows astronimors to see Jupitor through
The Outer Planets (pages )
The Outer Planets (pages 720 727) Gas Giants and Pluto (page 721) Key Concept: The first four outer planets Jupiter, Saturn, Uranus, and Neptune are much larger and more massive than Earth, and they do
Yes, inner planets tend to be and outer planets tend to be.
1. Planet Density Make some general comments about inner and outer planets density Inner Planets Density Outer Planets Density Is there a pattern or a trend in planet density? Yes, inner planets tend to
LEARNING ABOUT THE OUTER PLANETS. NASA's Cassini spacecraft. Io Above Jupiter s Clouds on New Year's Day, Credit: NASA/JPL/University of Arizona
LEARNING ABOUT THE OUTER PLANETS Can see basic features through Earth-based telescopes. Hubble Space Telescope especially useful because of sharp imaging. Distances from Kepler s 3 rd law, diameters from
Astronomy Club of Asheville January 2016 Sky Events
January 2016 Sky Events The Planets this Month - page 2 Planet Highlights - page 7 All 5 Naked-Eye Planets in the Dawn Sky - page 10 Moon Phases - page 11 Earth Reaches Perihelion on Jan. 4 - page 12 Quadrantid
Chapter 15 & 16 Science Review (PATTERNS IN THE SKY, OUR SOLAR SYSTEM)
Chapter 15 & 16 Science Review (PATTERNS IN THE SKY, OUR SOLAR SYSTEM) The Milky Way the galaxy that contains our solar system Our solar system is a speck in the Milky Way galaxy Pluto is now considered
Exercise 4.0 PLANETARY ORBITS AND CONFIGURATIONS
Exercise 4.0 PLANETARY ORBITS AND CONFIGURATIONS I. Introduction The planets revolve around the Sun in orbits that lie nearly in the same plane. Therefore, the planets, with the exception of Pluto, are
Across the Universe. By Gabrielle Sierra
Across the Universe By Gabrielle Sierra Our universe is an amazing place. Since prehistoric days, inquisitive minds have been wondering about the celestial objects that surround our planet, and today scientists
ASTR 2310: Chapter 2
Emergence of Modern Astronomy Early Greek Astronomy Ptolemaic Astronomy Copernican Astronomy Galileo: The First Modern Scientist Kepler's Laws of Planetary Motion Proof of the Earth's Motion Early Greek
Planets. Chapter 5 5-1
Planets Chapter 5 5-1 The Solar System Terrestrial Planets: Earth-Like Jovian Planets: Gaseous Sun Mercury Venus Earth Mars Jupiter Saturn Uranus Neptune Pluto Inferior Planets Superior Planets Inferior
Planetary Motion from an Earthly Perspective
1 Planetary Motion from an Earthly Perspective Stars appear fixed from night-to-night providing the familiar background of the constellations and asterisms. We see the same star patterns that were visible
Developing/Secure Pathway. End of Topic Assessment. Space
Name: Group: Year 8 Developing/Secure Pathway End of Topic Assessment Space Analysis and Targets No. Score Below/On/Above Target for next Assessment. How will you achieve it? 1 /6 2 /4 3 /6 4 /6 5 /4 6
Astronomy Club of Asheville February 2018 Sky Events
February 2018 Sky Events The Planets this Month page 2 The Gibbous Moon Joins Jupiter, Mars and Antares page 7 A Crescent Moon Pairs with Venus page 8 Conjunction of Near Full Moon with Regulus page 9
After you read this section, you should be able to answer these questions:
CHAPTER 16 4 Moons SECTION Our Solar System California Science Standards 8.2.g, 8.4.d, 8.4.e BEFORE YOU READ After you read this section, you should be able to answer these questions: How did Earth s moon
ASTR 310 Tutorial 3: A Human Orrery
ASTR Tutorial : A Human Orrery An orrery is a mechanical model of the Solar System. When you turn a crank, the planets and moons orbit the Sun at correctly-scaled distances with correctly-scaled periods.
Astron 104 Laboratory #4 Orbital Motion of a Planet
Name: Date: Section: Astron 104 Laboratory #4 Orbital Motion of a Planet Introduction The nature of the Solar System was first derived from careful measurements of the positions of the planets in the night
Selected 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,
STANDARD. S6E1 d. Explain the motion of objects in the day/night sky in terms of relative position.
STANDARD S6E1 d. Explain the motion of objects in the day/night sky in terms of relative position. S6E2 b. Explain the alignment of the earth, moon, and sun during solar and lunar eclipses. c. Relate the
Planets in the Sky ASTR 101 2/16/2018
Planets in the Sky ASTR 101 2/16/2018 1 Planets in the Sky 2018 paths of Jupiter among stars (2017/2018) Unlike stars which have fixed positions in the sky (celestial sphere), planets seem to move with
Lecture 5. Motions of the Planets
Lecture 5 Motions of the Planets; Geometric models of the Solar System Motion of Planets Opposition, Conjunction Retrograde Motion Scientific Method and "Models" Size of the Earth Geocentric vs Heliocentric
ASTRONOMY Merit Badge Requirements
ASTRONOMY Merit Badge Requirements 1) Do the following: A) Sketch the face of the moon, indicating on it the locations of at least five seas and five craters. B) Within a single week, sketch the position
TEKS Cluster: Space. identify and compare the physical characteristics of the Sun, Earth, and Moon
5.8 Earth and space. The student knows that there are recognizable patterns in the natural world and among the Sun, Earth, and Moon system. 5.8(C) 5.8(D) demonstrate that Earth rotates on its axis once
Solar Noon The point at which the Sun is highest in the sky (and when shadows are shortest).
Solar Noon The point at which the Sun is highest in the sky (and when shadows are shortest). Rotation The movement of one object as it turns or spins around a central point or axis. Revolution The movement
Homework Assignment #9: Apparent Motions of the Heavens Due to Actual Motions of Earth
Name Homework Assignment #9: Apparent Motions of the Heavens Due to Actual Motions of Earth 2002 Ann Bykerk-Kauffman, Dept. of Geological and Environmental Sciences, California State University, Chico
Astronomy Club of Asheville April 2017 Sky Events
April 2017 Sky Events The Planets this Month page 2 April 6 th - Regulus and the Gibbous Moon page 5 April 10 th -The Full Moon Joins Jupiter and Spica page 6 Planet Highlights page 7 Moon Phases page
UNIT 6 CELESTIAL SPHERE AND EQUINOCTIAL SYSTEM OF COORDINATES
UNIT 6 CELESTIAL SPHERE AND EQUINOCTIAL SYSTEM OF COORDINATES Structure 6.1 Introduction Objectives 6.2 References 6.3 Apparent Annual Motion of the Sun and the Concept of the Ecliptic and the Obliquity
Eclipses September 12th, 2013
Eclipses September 12th, 2013 Who was the favorite Star Wars character of the class? A) Obi-Wan B) Jar Jar C) Luke Skywalker D) Yoda News! Dark matter http://mcdonaldobservatory.org/news/releases/2013/09/10
Paper Reference. Monday 9 June 2008 Morning Time: 2 hours
Centre No. Candidate No. Paper Reference(s) 1627/01 Edexcel GCSE Astronomy Paper 01 Monday 9 June 2008 Morning Time: 2 hours Materials required for examination Calculator Items included with question papers
A medium-sized star. The hottest object found in our solar system.
A medium-sized star. The hottest object found in our solar system. It gives off heat, light, and energy. It affects the seasons, climate, and weather on Earth. The second smallest planet in our solar system.
The 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.
Solar System Test Review
Solar System Test Review There are several planets in the solar system. What do all of these planets have in common? A.They all orbit the Sun. B. They are all close to the Moon. C.They are all called Earth.
Investigating the Solar System
Investigating the Solar System This Workbook belongs to: Our Local Star: The Sun Location in The Solar System Interesting Facts 1. 2. 3. 4. Name of Star: THE SUN 5. Draw and Color your own Sun in the blank
Motions in the Sky. Stars Planets Sun Moon. Photos - APOD. Motions in the Sky - I. Intro to Solar System
Motions in the Sky Stars Planets Sun Moon Photos - APOD 1 STARS: background for motion of other objects patterns - constellations zodiac: special set of constellations trace the apparent path of the Sun
Key Concepts Solar System, Movements, Shadows Recall that Earth is one of many planets in the solar system that orbit the Sun.
Key Concepts Solar System, Movements, Shadows 4-3.1 Recall that Earth is one of many planets in the solar system that orbit the Sun. It is essential for students to know that Earth is a planet that orbits
Unit 2 Lesson 1 What Objects Are Part of the Solar System? Copyright Houghton Mifflin Harcourt Publishing Company
Unit 2 Lesson 1 What Objects Are Part of the Solar System? Florida Benchmarks SC.5.E.5.2 Recognize the major common characteristics of all planets and compare/contrast the properties of inner and outer
Name: (This only happens every four years or does it?)
Name: (This only happens every four years or does it?) Calendars: Then and Now Name: 1. What is a leap year? What do you already know about leap years? 2. List at least three questions about leap years
OCCULTATIONS OF PLANETS AND BRIGHT STARS BY THE MOON January 27, 2018
OCCULTATIONS OF PLANETS AND BRIGHT STARS BY THE MOON January 27, 2018 The moon, as our nearest neighbor, sometimes blocks the light coming from a planet, a star, or the sun. Occultations are listed below
Science Revision Paper- Final Exam May-June Write the scientific terms for the following statements/definitions: Part A
Name Grade 4 Date : Science Revision Paper- Final Exam May-June 2018 Write the scientific terms for the following statements/definitions: Part A 1. An imaginary line that goes through an object s center:
Griffith Observatory Field Trip Guide
To enter the Griffith Observatory you must make a reservation for a seat on a shuttle. There is a cost associated with each shuttle ticket and it is $8.00. There is no other way to enter Griffith Observatory!
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)
When a planets orbit around the Sun looks like an oval, it s called a(n) - ellipse - circle - axis - rotation Which of the following planets are all made up of gas? - Venus, Mars, Saturn and Pluto - Jupiter,
Class VIII Chapter 17 Stars and the Solar System Science
Question 1: Which of the following is NOT a member of the solar system? (a) An asteroid (b) A satellite (c) A constellation (d) A comet (c) Constellation A constellation is not a member of the solar system.
Paper Reference. Paper Reference(s) 1627/01 Edexcel GCSE Astronomy Paper 01. Friday 15 May 2009 Morning Time: 2 hours
Centre No. Candidate No. Paper Reference(s) 1627/01 Edexcel GCSE Astronomy Paper 01 Friday 15 May 2009 Morning Time: 2 hours Materials required for examination Calculator Items included with question papers
SPI Use data to draw conclusions about the major components of the universe.
SPI 0607.6.1 - Use data to draw conclusions about the major components of the universe. o Stars are huge, hot, brilliant balls of gas trillions of kilometers away. A Galaxy is a collection of billions
RETROGRADE MOTION AND PLANETARY ORBITS Computer Simulations
RETROGRADE MOTION AND PLANETARY ORBITS Computer Simulations OBJECTIVE: To see planetary orbits simulated on a computer and to see how this suncentered model explains retrograde motion. Initial Procedure:
Astronomy Test Review. 3 rd Grade
Astronomy Test Review 3 rd Grade Match the vocabulary word to its definition. Outer Planets The path a planet takes around the sun. Inner Planets Orbit Sun The center of our solar system. Small, rocky
Position 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
Dive into Saturn.
Dive into Saturn http://www.pbs.org/wgbh/nova/space/death-dive-to-saturn.html Read Ch. 3 By next class time Do practice online quiz 01 Axis tilt changes directness of sunlight during the year. Why Does
Unit 12 Lesson 1 What Objects Are Part of the Solar System?
Unit 12 Lesson 1 What Objects Are Part of the Solar System? The Solar System Earth, other planets, and the moon are part of a solar system. A solar system is made up of a star and the planets and other
PHSC 1053: Astronomy Time and Coordinates
PHSC 1053: Astronomy Time and Coordinates Astronomical Clocks Earth s Rotation on its Axis Time between two successive meridian transits of the sun 1 solar day (our adopted clock time) 24 hours (86,400
Solar wind is the name for the radiation that is emitted from the sun - even though it is just energy, it is strong enough to 'push' objects
I can explain and demonstrate that the Sun and stars are the sources of light in our universe and that the Moon, planets, their moons, comets and asteroids are seen by reflecting that light. Emit vs. Reflect
(All times listed are UT); Singapore Standard (Local) Time = UT + 8 h
SKYTRACK Diary of Astronomical Events 2011 (All times listed are UT); Singapore Standard (Local) Time = UT + 8 h January 02 15 Mercury 4º N of Moon 04 09 NEW MOOM (Partial Solar Eclipse not visible from
PHYS 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,
Science Assessment Year 5: Earth and Space. The Solar System. Movements, Shape and Size. Saturn. Mars. Mercury. Earth. Neptune.
Name: Science Assessment Year 5: Earth and Space Date: 7 total marks The Solar System. Join up these labels to the correct planet, star or satellite: Mars Earth Saturn Mercury Neptune Sun Uranus Venus
Topic 1: Celestial Objects, phenomena, and interactions are important to people in many different ways.
Topic 1: Celestial Objects, phenomena, and interactions are important to people in many different ways. To complete this booklet you must do the following: Define each term within this booklet Answer Each
Sky views October 2007 revised 10/8/07 (excerpted from Astronomy magazine, 10/2007 issue) by Barbara Wiese
Sky views October 2007 revised 10/8/07 (excerpted from Astronomy magazine, 10/2007 issue) by Barbara Wiese Monthly Overview - Views by Date Definitions Overview Viewing Notes Jupiter in Ophiuchus Neptune
Astronomy Club of Asheville June 2018 Sky Events
June 2018 Sky Events The Planets this Month - page 2 June 14 th Dusk s Venus, Mercury and a Sliver of Moon page 5 June 27 th Conjunction of the Full Moon with Saturn page 6 Planet Highlights - page 7 Moon
Chapter 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
Chapters 7&8. ASTRONOMY 202 Spring 2007: Solar System Exploration. Class 21: Solar System [3/12/07] Announcements.
![Chapters 7&8. ASTRONOMY 202 Spring 2007: Solar System Exploration. Class 21: Solar System [3/12/07] Announcements.](/thumbs/81/83429897.jpg "Chapters 7&8. ASTRONOMY 202 Spring 2007: Solar System Exploration. Class 21: Solar System [3/12/07] Announcements.")
ASTRONOMY 202 Spring 2007: Solar System Exploration Instructor: Dr. David Alexander Web-site: www.ruf.rice.edu/~dalex/astr202_s07 Class 21: Solar System [3/12/07] Announcements The Solar System Comparative
Chapter 06 Let s Make a Solar System
like? Big picture. Chapter 06 Let s Make a Solar System How did it come to be this way? Where did it come from? Will I stop sounding like the Talking Heads? The solar system exhibits clear patterns of
Astronomy Club of Asheville December 2017 Sky Events
December 2017 Sky Events The Planets this Month - page 2 December 13-16 Crescent Moon with Jupiter and Mars page 8 Planet Highlights - page 9 Moon Phases - page 12 December 13 th Geminid Meteor Shower
Astronomy Club of Asheville November 2017 Sky Events
November 2017 Sky Events The Planets this Month page 2 Close Conjunction of Venus and Jupiter page 7 Conjunction of Crescent Moon, Saturn & Mercury page 8 Planet Highlights page 9 Moon Phases page 12 November
How did it come to be this way? Will I stop sounding like the
Chapter 06 Let s Make a Solar System How did it come to be this way? Where did it come from? Will I stop sounding like the Talking Heads? What does the solar system look like? Big picture. The solar system
The ecliptic and the sidereal motion of the sun Moon and the planets on it.
The ecliptic and the sidereal motion of the sun Moon and the planets on it. The following picture is a picture of the sky as it looks about noon on May 18 2012. The light of the Sun has been erased artificially
Ch. 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
Our Planetary System. Chapter 7
Our Planetary System Chapter 7 Key Concepts for Chapter 7 and 8 Inventory of the Solar System Origin of the Solar System What does the Solar System consist of? The Sun: It has 99.85% of the mass of the
Locating the Planets (Chapter 20) and the Moon and Sun (Chapter 22)
GEOLOGY 306 Laboratory Instructor: TERRY J. BOROUGHS NAME: Locating the Planets (Chapter 20) and the Moon and Sun (Chapter 22) For this assignment, you will require: a calculator, colored pencils, a metric
Introduction 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
Phys 214. Planets and Life
Phys 214. Planets and Life Dr. Cristina Buzea Department of Physics Room 259 E-mail: cristi@physics.queensu.ca (Please use PHYS214 in e-mail subject) Lecture 8. The scale of time and nature of worlds (Page
Locating the Planets (Chapter 19) and the Moon and Sun (Chapter 21)
GEOLOGY 306 Laboratory Instructor: TERRY J. BOROUGHS NAME: Locating the Planets (Chapter 19) and the Moon and Sun (Chapter 21) For this assignment, you will require: a calculator, colored pencils, a metric
Voyage to the Planets
UNIT 5 WEEK 4 Read the article Voyage to the Planets before answering Numbers 1 through 5. Voyage to the Planets A voyage to Jupiter, the largest planet in our solar system, takes years. Saturn and Uranus
Chapter 23. Our Solar System
Chapter 23 Our Solar System Our Solar System 1 Historical Astronomy Wandering Stars Greeks watched the stars move across the sky and noticed five stars that wandered around and did not follow the paths
WHAT'S UP THIS MONTH MAY 2018
WHAT'S UP THIS MONTH MAY 2018 THESE PAGES ARE INTENDED TO HELP YOU FIND YOUR WAY AROUND THE SKY The chart on the last page is included for printing off and use outside The chart above shows the whole night
Saturn and Planetary Rings 4/5/07
Saturn and Planetary Rings Announcements Reading Assignment Chapter 15 5 th homework due next Thursday, April 12 (currently posted on the website). Reminder about term paper due April 17. There will be
Welcome to the Solar System
Welcome to the Solar System How vast those Orbs must be, and how inconsiderable this Earth, the Theater upon which all our mighty Designs, all our Navigations, and all our Wars are transacted, is when
Chapter 7 Our Planetary System
Chapter 7 Our Planetary System What does the solar system look like? Earth, as viewed by the Voyager spacecraft Eight major planets with nearly circular orbits Pluto is smaller than the major planets and
ASTR 200 : Lecture 6 Introduction to the Solar System Pearson Education Inc., publishing as Addison-Wesley
ASTR 200 : Lecture 6 Introduction to the Solar System 1 2004 Pearson Education Inc., publishing as Addison-Wesley Comparative Planetology Studying the similarities among and differences between the planets
STUDENT RESOURCE 1.1 INFORMATION SHEET. Vocabulary
Vocabulary STUDENT RESOURCE 1.1 INFORMATION SHEET asteroids thousands of rocky objects that orbit the Sun Most asteroids orbit in a belt between the orbits of Mars and Jupiter. More than 9, asteroids have
Lecture 2 Motions in the Sky September 10, 2018
1 Lecture 2 Motions in the Sky September 10, 2018 2 What is your year in school? A. New freshman B. Returning freshman C. Sophomore D. Junior E. Senior F. I ve been here, like, forever 3 What is your major?
Planet Time to orbit the Sun (Earth years) Distance from the Sun (million km) Mercury Venus Earth Mars 2.
The inner planets Burt and Duncan investigated the inner planets of our solar system. Burt compiled some information about the four inner planets. Planet Time to orbit the Sun (Earth years) Distance from
4. What is the main advantage of the celestial coordinate system over altitude-azimuth coordinates?
SUMMARY Looking at the night sky is not only fun, it will help you understand some of the phenomena described in chapters 1 and 2. Star maps will help you identify constellations and bright stars, and
Observational 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
Survey of the Solar System. The Sun Giant Planets Terrestrial Planets Minor Planets Satellite/Ring Systems
Survey of the Solar System The Sun Giant Planets Terrestrial Planets Minor Planets Satellite/Ring Systems Definition of a dwarf planet 1. Orbits the sun 2. Is large enough to have become round due to the
Stellar and Planetary aberration Working Model
Stellar and Planetary aberration Working Model Bart Leplae Updated on 2-Dec-2011 (Org. 7-Apr-2011) bartleplae@hotmail.com This paper describes why we can observe stars that are actually behind the moon
Chapter 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).
The Sun s center is much hotter than the surface. The Sun looks large and bright in the sky. Other stars look much smaller.
The Sun A star is a huge ball of hot, glowing gases. The Sun is a star. The width of the Sun is equal to the width of 100 Earths placed side by side. The Sun is extremely hot. The surface of the Sun has
Lecture #27: Saturn. The Main Point. The Jovian Planets. Basic Properties of Saturn. Saturn:
Lecture #27: Saturn Saturn: General properties. Atmosphere. Interior. Origin and evolution. Reading: Chapters 7.1 (Saturn) and 11.1. The Main Point Saturn is a large Jovian-class planet with a composition
a. exactly 360 b. less than 360 c. more than 360 On Figure 1, draw the Earth the next day and justify your answer above.
Astronomy 100, Fall 2006 Name(s): Exercise 3: Geocentrism and heliocentrism In the previous exercise, you saw how the passage of time is intimately related to the motion of celestial objects. This, of
WHAT'S UP THIS MONTH - OCTOBER 2015
WHAT'S UP THIS MONTH - OCTOBER 2015 THESE PAGES ARE INTENDED TO HELP YOU FIND YOUR WAY AROUND THE SKY The chart above shows the night sky as it appears on 15 th October at 10 o clock in the evening British
DO NOT WRITE ON THIS TEST PACKET. Test Booklet NSCD Invitational 2010
Solar System Science Olympiad Test Booklet NSCD Invitational 2010 Multiple Choice: On the answer sheet, write the letter of the choice that best answers each question. No credit will be given for answers
Earth s Formation Unit [Astronomy] Student Success Sheets (SSS)
![Earth s Formation Unit [Astronomy] Student Success Sheets (SSS)](/thumbs/77/76655554.jpg "Earth s Formation Unit [Astronomy] Student Success Sheets (SSS)")
Page1 Earth s Formation Unit [Astronomy] Student Success Sheets (SSS) HS-ESSI-1; HS-ESS1-2; HS-ESS1-3; HS-ESSI-4 NGSS Civic Memorial High School - Earth Science A Concept # What we will be learning Mandatory
Key #
4-3.8. 1. Which of the following instruments is used to directly observe objects in the sky? 4-3.1. 2. Earth is a rocky planet that resides close to the Sun. Recognize the list of planets below that has
Space Science Jeopardy!
Space Science Jeopardy! Structure of the Universe Stars & HR Diagram Seasons, Tides, Phases, Eclipses Astronomical Bodies The Sun & Gravity 10 10 10 10 10 20 20 20 20 20 30 30 30 30 30 40 40 40 40 40 50
7. Our Solar System. Planetary Orbits to Scale. The Eight Planetary Orbits
7. Our Solar System Terrestrial & Jovian planets Seven large satellites [moons] Chemical composition of the planets Asteroids & comets The Terrestrial & Jovian Planets Four small terrestrial planets Like
1. The Sun is a huge ball of very hot gas in space, which radiates heat and light in one direction.
PLEASE ANSWER YOUR QUESTIONS ON THIS PROVIDED QUESTION PAPER. EACH QUESTION IS FOLLOWED BY ANSWERS MARKED A AND B, OR A, B, C AND D. ONLY ONE ANSWER IS CORRECT. CHOOSE THE MOST CORRECT ANSWER AND CIRCLE
What is the Solar System?
What is the Solar System? Our Solar System is one of many planetary systems. It consists of: The Sun Eight planets with their natural satellites Five dwarf planets Billions of asteroids, comets and meteors
Lecture 25: The Outer Planets
Lecture 25: The Outer Planets Neptune Uranus Pluto/Charon Uranus and three moons Neptune and two moons 1 The Outer Planets Uranus Discovered by William Herschel in 1781, who realized that this extended
Prairie State Park June 11, 2017
Prairie State Park June 11, 2017 References: https://skysafariastronomy.com/ http://astropixels.com/ephemeris/astrocal/astrocal2017cst.html http://www.seasky.org/astronomy/astronomy-calendar- 2017.html
Observing 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
Chapter 2 Discovering the Universe for Yourself. Copyright 2012 Pearson Education, Inc.
Chapter 2 Discovering the Universe for Yourself 1 2.1 Patterns in the Night Sky Our goals for learning: What does the universe look like from Earth? Why do stars rise and set? Why do the constellations
Explore the Universe Observing Certificate and Pin #3
Explore the Universe Observing Certificate and Pin #3 Lunar Phases (4 of 8) Waxing Crescent Day 3 seen within 3h of sunset First Quarter within +- 18 hours Waxing Gibbous 3-4 days after First Quarter Full