Chapter 8 MOONS, RINGS, AND PLUTO Small Worlds Among Giants

Similar documents
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.

The Outer Planets (pages )

Yes, inner planets tend to be and outer planets tend to be.

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

Astronomy Club of Asheville January 2016 Sky Events

Chapter 15 & 16 Science Review (PATTERNS IN THE SKY, OUR SOLAR SYSTEM)

Exercise 4.0 PLANETARY ORBITS AND CONFIGURATIONS

Across the Universe. By Gabrielle Sierra

ASTR 2310: Chapter 2

Planets. Chapter 5 5-1

Planetary Motion from an Earthly Perspective

Developing/Secure Pathway. End of Topic Assessment. Space

Astronomy Club of Asheville February 2018 Sky Events

After you read this section, you should be able to answer these questions:

ASTR 310 Tutorial 3: A Human Orrery

Astron 104 Laboratory #4 Orbital Motion of a Planet

Selected Topics Starry, Starry Night. Exploring the Universe of Science 1

STANDARD. S6E1 d. Explain the motion of objects in the day/night sky in terms of relative position.

Planets in the Sky ASTR 101 2/16/2018

Lecture 5. Motions of the Planets

ASTRONOMY Merit Badge Requirements

TEKS Cluster: Space. identify and compare the physical characteristics of the Sun, Earth, and Moon

Solar Noon The point at which the Sun is highest in the sky (and when shadows are shortest).

Homework Assignment #9: Apparent Motions of the Heavens Due to Actual Motions of Earth

Astronomy Club of Asheville April 2017 Sky Events

UNIT 6 CELESTIAL SPHERE AND EQUINOCTIAL SYSTEM OF COORDINATES

Eclipses September 12th, 2013

Paper Reference. Monday 9 June 2008 Morning Time: 2 hours

A medium-sized star. The hottest object found 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.

Solar System Test Review

Investigating the Solar System

Motions in the Sky. Stars Planets Sun Moon. Photos - APOD. Motions in the Sky - I. Intro to Solar System

Key Concepts Solar System, Movements, Shadows Recall that Earth is one of many planets in the solar system that orbit the Sun.

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

Name: (This only happens every four years or does it?)

OCCULTATIONS OF PLANETS AND BRIGHT STARS BY THE MOON January 27, 2018

Science Revision Paper- Final Exam May-June Write the scientific terms for the following statements/definitions: Part A

Griffith Observatory Field Trip Guide

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)

Class VIII Chapter 17 Stars and the Solar System Science

Paper Reference. Paper Reference(s) 1627/01 Edexcel GCSE Astronomy Paper 01. Friday 15 May 2009 Morning Time: 2 hours

SPI Use data to draw conclusions about the major components of the universe.

RETROGRADE MOTION AND PLANETARY ORBITS Computer Simulations

Astronomy Test Review. 3 rd Grade

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.

Dive into Saturn.

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

PHSC 1053: Astronomy Time and Coordinates

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

(All times listed are UT); Singapore Standard (Local) Time = UT + 8 h

PHYS 160 Astronomy Test #1 Fall 2017 Version B

Science Assessment Year 5: Earth and Space. The Solar System. Movements, Shape and Size. Saturn. Mars. Mercury. Earth. Neptune.

Topic 1: Celestial Objects, phenomena, and interactions are important to people in many different ways.

Sky views October 2007 revised 10/8/07 (excerpted from Astronomy magazine, 10/2007 issue) by Barbara Wiese

Astronomy Club of Asheville June 2018 Sky Events

Chapter 3 The Solar System

Chapters 7&8. ASTRONOMY 202 Spring 2007: Solar System Exploration. Class 21: Solar System [3/12/07] Announcements.

Chapter 06 Let s Make a Solar System

Astronomy Club of Asheville December 2017 Sky Events

Astronomy Club of Asheville November 2017 Sky Events

How did it come to be this way? Will I stop sounding like the

The ecliptic and the sidereal motion of the sun Moon and the planets on it.

Ch. 22 Origin of Modern Astronomy Pretest

Our Planetary System. Chapter 7

Locating the Planets (Chapter 20) and the Moon and Sun (Chapter 22)

Introduction To Modern Astronomy II

Phys 214. Planets and Life

Locating the Planets (Chapter 19) and the Moon and Sun (Chapter 21)

Voyage to the Planets

Chapter 23. Our Solar System

WHAT'S UP THIS MONTH MAY 2018

Saturn and Planetary Rings 4/5/07

Welcome to the Solar System

Chapter 7 Our Planetary System

ASTR 200 : Lecture 6 Introduction to the Solar System Pearson Education Inc., publishing as Addison-Wesley

STUDENT RESOURCE 1.1 INFORMATION SHEET. Vocabulary

Lecture 2 Motions in the Sky September 10, 2018

Planet Time to orbit the Sun (Earth years) Distance from the Sun (million km) Mercury Venus Earth Mars 2.

4. What is the main advantage of the celestial coordinate system over altitude-azimuth coordinates?

Observational Astronomy - Lecture 4 Orbits, Motions, Kepler s and Newton s Laws

Survey of the Solar System. The Sun Giant Planets Terrestrial Planets Minor Planets Satellite/Ring Systems

Stellar and Planetary aberration Working Model

Chapter 02 The Rise of Astronomy

The Sun s center is much hotter than the surface. The Sun looks large and bright in the sky. Other stars look much smaller.

Lecture #27: Saturn. The Main Point. The Jovian Planets. Basic Properties of Saturn. Saturn:

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.

WHAT'S UP THIS MONTH - OCTOBER 2015

DO NOT WRITE ON THIS TEST PACKET. Test Booklet NSCD Invitational 2010

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

Key #

Space Science Jeopardy!

7. Our Solar System. Planetary Orbits to Scale. The Eight Planetary Orbits

1. The Sun is a huge ball of very hot gas in space, which radiates heat and light in one direction.

What is the Solar System?

Lecture 25: The Outer Planets

Prairie State Park June 11, 2017

Observing the Universe for Yourself

Chapter 2 Discovering the Universe for Yourself. Copyright 2012 Pearson Education, Inc.

Explore the Universe Observing Certificate and Pin #3

Transcription:

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

8.2 WHAT GALILEO SAW OF SATURN S RINGS Saturn was visible only early evening in January 1612. 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

Sample Data: Start Time span 2005/01/01 02:43:00 2005/01/02 21:12:00 42:29:00 2005/01/04 15:41:00 42:29:00 2005/01/06 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

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 02:43:00 2005/01/02 21:12:00 42:29:00 2005/01/04 15:41:00 42:29:00 2005/01/06 10:09:00 42:28:00 Predicted Start Time span 5/1/2005 10:29 42:28:00 5/3/2005 4:57 42:28:00 5/4/2005 23:25 42:28:00 5/6/2005 17:53 42:28:00 5/8/2005 12:21 42:28:00 5/10/2005 6:49 42:28:00 5/12/2005 1:17 42:28:00 *Hidden Rows 5/13/2005 19:45 42:28:00 *Hidden Rows 5/15/2005 14:13 42:28:00 5/17/2005 8:41 42:28:00 5/19/2005 3:09 42:28:00 5/20/2005 21:37 42:28:00 5/22/2005 16:05 42:28:00 5/24/2005 10:33 42:28:00 5/26/2005 5:01 42:28:00 5/27/2005 23:29 42:28:00 6 mo. Prediction 5/29/2005 17:57 42:28:00 5/31/2005 12:25 42:28:00 8.6 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

Figure 68. The predicted eclipse on 5/31/2005 12:25. 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

Aquarius Capricornus Mercury Moon Sun Jupiter Venus Saturn Mars Viewed from: Mt Wilson 118 03' 36.0" W 34 13' 00.0" N Local time: 06:00:00 1962/02/05 JD 2437701.08 Figure 69. The planets in conjunction. Field of view: 45 00' 00.0" Ecliptic Lon: 315.2254 Ecliptic Lat: -00.0616 Magnitudes: Single star Multiple star Variable star 3.0 2.0 1.0 0.0-1.0-2.0 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. = 00 00 00.00, Offset Dec. = 90 00 00.0. View/Center Planet/Sun. DRAW/Stars, Constellations, Deep Sky Objects and Symbols & Grids Off. Mars Venus Sun Mercury Earth Uranus Viewed from: 60.00000 AU from Sun Local time: Field of view: 06:00:00 22 30' 00.0" 1962/02/06 Ecliptic Lon: 247.8982 JD 2437702.08 Ecliptic Lat: -69.1582 Magnitudes: Single star Multiple star Variable star 10.0 9.0 8.0 7.0 6.0 5.0 Figure 70. Notice Uranus in this alignment. (As opposed to this top-down view, an edge-on view would yield different results.) 67