How to Assemble the Saturn System Diagram
|
|
- Gervase Johnston
- 5 years ago
- Views:
Transcription
1 How to Assemble the Saturn System Diagram (from the NASA Saturn Educator s Guide). Be sure you have all 4 sections (A, B, C, and D) of the Saturn System Diagram. Place Section B to the right of Section A so they are lined up along the center line, as illustrated below. 2. Place the meterstick over the two sections so that the end 0 mark of the meterstick lines up with the center of Saturn located near the left edge of Section A. Now align your meter stick with the black line running from left to right across the center of each section of the diagram. Adjust the position of Section B to the left or right as needed so that the G ring crosses the center line at 34 cm on the meter stick. When you are certain that it is in position, tape the two sections together. (When the pages are correctly positioned, the horizontal edges may or may not overlap.) Tape them together so that the center lines are continuous, aligned, and straight. Don t tape the meter stick to the sections! 3. Place Section C to the right of Section B; then place D next to C. Adjust Section D to the left or right so that the moon Dione is located at 75.5 cm on the meter stick. When
2 you have Dione in position, tape Sections B, C, and D together. As before, the edges may or may not align. You have now assembled your Saturn System Diagram and you are ready to begin your scavenger hunt!
3 Voyager Image of Saturn Figure It appears that three moons are scattered about Saturn, but in reality, all of Saturn s known moons except the two outermost ones orbit in the same plane as do Saturn s rings. In images, a moon may appear outside Saturn s ring plane because of the moon s position in its orbit and the angle from which the Saturn system is being viewed. The small dark shadow on the surface of Saturn is that of a fourth moon, which does not appear in the image. A similar image of Saturn may be found at < cassini/ Images/ astro/ html>. TOP Saturn Educator Guide Cassini Program website EG JPL
4 Saturn Ring System (shown to scale) G RING F RING E RING Figure 2 A RING B RING C RING D RING Colored markers can enchance the visual distinction between rings. CASSINI DIVISION ENCKE GAP EARTH MOON APPROXIMATE DISTANCE BETWEEN EARTH AND ITS MOON Saturn s rings are not located in alphabetical order outward from the planet because they were named in order of their discovery. From inner to outer, the rings are D, C, B, A, F, G, E. Saturn Educator Guide Cassini Program website EG JPL 3
5 Saturn System Diagram (A) ( of 4) Figure 4 B RING Scale: cm = 5,000 km. The radius of Saturn corresponds to the radius of a basketball in this scale diagram. C RING D RING Scale: cm = 5,000 km CENTER OF SATURN (BEGIN MEASUREMENTS FROM THIS POINT) CLOUD TOPS RADIUS OF SATURN DIAMETER OF EARTH SCALED SIZE OF EARTH Cut first, then tape sheets. Do not tape the meter stick to the diagram. Saturn Educator Guide Cassini Program website EG JPL 7
6 Saturn System Diagram (B) (2 of 4) Figure 4 G RING F RING VOYAGER IMAGE OF MIMAS, THE DEATH STAR MOON ENCKE GAP MIMAS CASSINI DIVISION A RING PAN EPIMETHEUS JANUS PANDORA NOTE: TO PRESERVE ACCURATE DISTANCE SCALE, PLACE THIS SECTION SO THAT THE G RING IS LOCATED 34 cm FROM SATURN'S CENTER. SCALE: cm = 5,000 km PROMETHEUS ATLAS Cut first, then tape sheets. Do not tape the meter stick to the diagram. Saturn Educator Guide Cassini Program website EG JPL 8
7 Figure 4 Saturn System Diagram (C) (3 of 4) APPROXIMATE OUTER "EDGE" OF E RING (ESTIMATES VARY FROM 300,000 km to OVER 480,000 km FROM SATURN'S CENTER.) SCALE: cm = 5,000 km TELESTO E RING TETHYS ENCELADUS CALYPSO ICE GEYSER ON ENCELADUS Cut first, then tape sheets. Do not tape the meter stick to the diagram. Saturn Educator Guide Cassini Program website EG JPL 9
8 Figure 4 Saturn System Diagram (D) (4 of 4) SIZE OF EARTH'S MOON TITAN SATURN'S LARGEST MOON DIAMETER OF 5,50 km IS SHOWN TO SCALE HERE. DISTANCE FROM CENTER OF SATURN =,22,900 km. SCALED DISTANCE = 244 cm (2.44 meters). OTHER MOONS: RHEA: 527,000 km (ABOUT meter FROM SATURN s CENTER) HYPERION:,480,000 km (ABOUT 3 meters FROM SATURN s CENTER) IAPETUS: 3,560,000 km (ABOUT 7 meters FROM SATURN s CENTER) PHOEBE: 3,000,000 km (26 meters FROM SATURN s CENTER) NOTE: TO PRESERVE ACCURATE DISTANCE SCALE, PLACE THIS SECTION SO THAT DIONE IS LOCATED 75.5 cm FROM SATURN'S CENTER SCALE: cm = 5,000 km DIONE HELENE NOTE THE BREAK IN THE SCALE HERE Cut first, then tape sheets. Do not tape the meter stick to the diagram. Saturn Educator Guide Cassini Program website EG JPL 20
9 Saturn System Table Moon/Ring Distance from Saturn s Center (cm) Scale Factor (km/cm) Approximate Distance from Saturn s Center (km) Figure 7 D Ring (inner edge) 3.4 5,000 67,000 C Ring (inner edge) 4.9 5,000 74,500 D Ring (outer edge) B Ring (inner edge) 8.4 5,000 92,000 C Ring (outer edge) B Ring (outer edge) ,000 7,500 Cassini Division (inner edge) A Ring (inner edge) ,000 22,000 Cassini Division (outer edge) Encke Gap and Pan ,000 33,500 A Ring (outer edge) ,000 37,000 Atlas ,000 37,500 Prometheus ,000 39,500 F Ring ,000 40,000 Pandora ,000 4,500 Epimetheus and Janus ,000 5,500 G Ring ,000 70,000 E Ring (approx. inner edge) ,000 8,000 Mimas 37. 5,000 85,500 Enceladus , ,000 Tethys, Telesto, and Calypso , ,500 Dione and Helene , ,500 E Ring (approx. outer edge) , ,000 Rhea , ,000 Titan ,000,220,000 Optional: Students can measure the shaded items using the Saturn System Diagram. Saturn Educator Guide Cassini Program website EG JPL 27
Moons, Rings, and Relationships
Names Moons, Rings, and Relationships Materials Rubber ball Paper, markers, pencils Procedure Part I: What Do We Know about Objects in Orbit? 1. In your group, discuss, predict, and draw what they think
More informationAmazing Saturn. Saturn from the ground
1 Amazing Saturn Saturn from the ground 2 Saturn Information Overload The Cassini Mission started orbiting Saturn in 2004. 3 Getting There Planetary pinball with passes by Venus, Venus, Earth, and Jupiter
More informationKey Ideas: A Warm Up Exercise. A Warm Up Exercise. The Moons of Saturn. Saturn s Moons
Saturn s Moons Key Ideas: Saturn is the second largest Jovian Planet Gas planet much like Jupiter 62 moons (13 larger than 50 km in diameter) Titan only giant moon Largest of Saturn s moons Thick Nitrogen
More informationCircular Motion and Gravitation Auxilliary Items
Circular Motion and Gravitation Auxilliary Items For The Loop-the-Loop Lab (Tape the following into your Data section and complete using the simulation program.) Post-Lab Questions: 1. Construct a free-body
More informationMimas, moon of Saturn and Death Star impersonator responsible for several gaps in Saturn s ring system
Last time: Gravitational signs of large outer moons in the rings Ring shepherding/gap maintenance Longer lived structures due to mean motion resonances with large satellites Example: 2:1 resonance with
More informationPhysics 112 Star Systems
Physics 112 Star Systems Lecture 16 Saturn Kevin H Knuth University at Albany Fall 2015 Saturn Mankind will not remain on Earth forever, but in its quest for light and space will at first timidly penetrate
More informationPlanetary Rings (cont.) Rings / Galilean Satellites 4/10/07
Planetary Rings (cont.) + Galilean Satellites Announcements Reading Assignment Finish Chapter 15 5 th homework due Thursday. Reminder about term paper due April 17. A sample planet fact sheet has been
More informationIcy Satellites: Geological Evolution and Surface Processes
Icy Satellites: Geological Evolution and Surface Processes Ralf Jaumann, Roger Clark, Francis Nimmo, Tilmann Denk, Amanda Hendrix, Bonnie Borutti, Jeff Moore, Paul Schenk, Ralf Srama ISSI WS January 2010
More informationSaturn. Slightly smaller 1/3 the mass density 700 kg/m 3. Interior - light elements, lack of rocky materials. Voyager 2, NASA
Saturn Slightly smaller 1/3 the mass density 700 kg/m 3 Interior - light elements, lack of rocky materials Voyager 2, NASA 1 Saturn - Atmosphere belts - driven by rapid rotation period - 10 hrs 14 min
More informationTidal Forces. Effects of Tidal Forces. The Roche Distance: Tidal Breakup
Reading:, Chap. 4, Sect. 4.6 (Tides); Chap. 12 (all) Homework #8: On website, due in recitation on Friday/Monday, Oct. 27/30 Exam 2 - Two weeks from Today (November 6) Last time: The Gas and Ice Giant
More informationThe Main Point. Planetary Ring Systems
Lecture #31: Satellites and Rings II Ring Systems Overview of rings: Jupiter, Saturn, Uranus, Neptune. What are rings made of? How do they form? Reading: Chapter 11.3. The Main Point All of the giant planets
More informationPhysics 1305 Notes: The Outer Solar System
Physics 1305 Notes: The Outer Solar System Victor Andersen University of Houston vandersen@uh.edu April 5, 2004 Copyright c Victor Andersen 2004 1 The Gas Giant Planets The predominant feature of Jupiter,
More informationHonors Math 2 Exam Review Packet 1. Mastery Review from 2 nd Quarter
Honors Math 2 Exam Review Packet 1 Mastery Review from 2 nd Quarter 1. A card is drawn from a 52-card deck. What is the probability of NOT drawing a face card or a spade? 2. A bag of marbles contains 6
More informationThe moons of Saturn 14 September 2015, by Matt Williams
The moons of Saturn 14 September 2015, by Matt Williams simple telescopes. The first to be discovered was Titan, Saturn's largest moon, which was observed by Christiaan Huygens in 1655 using a telescope
More informationToday in Astronomy 111: rings, gaps and orbits
Today in Astronomy 111: rings, gaps and orbits Gap sizes: the Hill radius Perturbations and resonances The variety of structures in planetary rings Spiral density waves Titan Bending waves Horseshoe and
More informationThe Jovian Planets and Their Moons
The Jovian Planets and Their Moons Jupiter 1 Physical Properties of Earth and Jupiter Jupiter Earth Equatorial lradius 11.2 R Earth 6378 km Mass 318 M Earth 5.976 10 24 kg Average Density 1.34 g/cm 3 5.497
More informationA Peek At Cassini After 7 Years In Saturn Orbit
After becoming humankind's first artificial satellite of Saturn on 1 July 2004, the Cassini orbiter shared headlines with its companion spacecraft Huygens until the latter reached the surface of Saturn's
More informationPlanetary science with adaptive optics: results from the UH AO systems
Planetary science with adaptive optics: results from the UH AO systems F. Roddier 1, C. Roddier 1, L. Close 1, C. Dumas 1, J. E. Graves 1, O. Guyon 1, B. Han 1, M. J. Northcott 1, T. Owen 1, D. Tholen
More informationRings PHYS Week 6, Part 2
Rings PHYS 178 2008 Week 6, Part 2 PIA00335: Voyager 1 image of Saturn and its ring four days after closest approach to Saturn. The Saturnian rings, are visible because they reflect sunlight. The translucent
More informationJupiter and Saturn s Satellites of Fire and Ice. Chapter Fifteen
Jupiter and Saturn s Satellites of Fire and Ice Chapter Fifteen ASTR 111 003 Fall 2006 Lecture 12 Nov. 20, 2006 Introduction To Modern Astronomy I Introducing Astronomy (chap. 1-6) Planets and Moons (chap.
More informationThe moons of Saturn 7 August 2015, by Matt Williams
The moons of Saturn 7 August 2015, by Matt Williams the irregular moons in the outermost regions have orbital radii of millions of kilometers, orbital periods lasting several years, and move in retrograde
More informationThe Jovian Planets. Why do we expect planets like this in the outer reaches of the solar system?(lc)
The Jovian Planets Beyond Mars and the Asteroid belt are the Jovian or Gas Giant Planets that are totally different than the terrestrial planets: They are composed almost entirely of gas They do not have
More informationPlanets. By Christian Bennett
Planets By Christian Bennett Mercury The smallest planet Closest to the sun It takes 116 days to orbit around the sun At night its -208 degrees, and at day time it is 800 degrees Its axis has the smallest
More informationJovian planets, their moons & rings
Jovian planets, their moons & rings The Moons of the Jovian Planets The terrestrial planets have a total of 3 moons. The jovian planets have a total of 166 moons. Each collection of moons orbiting the
More informationPlanets. 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
More informationChapter 11 Jovian Planet Systems. Comparing the Jovian Planets. Jovian Planet Composition 4/10/16. Spacecraft Missions
Chapter 11 Jovian Planet Systems Jovian Planet Interiors and Atmospheres How are jovian planets alike? What are jovian planets like on the inside? What is the weather like on jovian planets? Do jovian
More informationASTR-1010: Astronomy I Course Notes Section X
ASTR-1010: Astronomy I Course Notes Section X Dr. Donald G. Luttermoser Department of Physics and Astronomy East Tennessee State University Edition 2.0 Abstract These class notes are designed for use of
More informationJupiter and Saturn s Satellites of Fire and Ice. Chapter Fifteen. Guiding Questions
Jupiter and Saturn s Satellites of Fire and Ice Chapter Fifteen Guiding Questions 1. What is special about the orbits of Jupiter s Galilean satellites? 2. Are all the Galilean satellites made of rocky
More informationAST 248, Lecture 21. James Lattimer. Department of Physics & Astronomy 449 ESS Bldg. Stony Brook University. November 15, 2018
vi AST 248, Lecture 21 James Lattimer Department of Physics & Astronomy 449 ESS Bldg. Stony Brook University November 15, 2018 The Search for Intelligent Life in the Universe james.lattimer@stonybrook.edu
More informationGiant Planets Or Why the Solar System Is the Way It Is. Dr. Josh Colwell University of Central Florida
Giant Planets Or Why the Solar System Is the Way It Is Dr. Josh Colwell University of Central Florida Almost everything you see in this image is a galaxy containing tens of billions of stars each. Figure
More informationSpacecraft to the Outer Solar System
Spacecraft to the Outer Solar System Flybys: Pioneer 10, 11 Voyager 1, 2 Orbiters/ : Galileo, Cassini Landers (Jupiter) (Saturn) Voyager 2 is the only spacecraft to visit all four outer planets. Gas Giant
More informationLecture 24: Saturn. The Solar System. Saturn s Rings. First we focus on solar distance, average density, and mass: (where we have used Earth units)
Lecture 24: Saturn The Solar System First we focus on solar distance, average density, and mass: Planet Distance Density Mass Mercury 0.4 1.0 0.06 Venus 0.7 0.9 0.8 Earth 1.0 1.0 1.0 Mars 1.5 0.7 0.1 (asteroid)
More informationUnit 1 Astronomy: Kepler s Laws Of Planetary Motion Assessed Activity (66 marks total)
Name: Solutions & Marking Scheme 2009 TG: PF Unit 1 Astronomy: Kepler s Laws Of Planetary Motion Assessed Activity (66 marks total) Aim: To investigate Kepler s three laws planetary motion. Apparatus:
More informationSaturn: Diameter, 120,000 km; Mass, 95.2 Earth masses; Density, 0.7 (density of water is 1.0); Rotation Period, 10 hours, 14 minutes; Axis
Saturn: Diameter, 120,000 km; Mass, 95.2 Earth masses; Density, 0.7 (density of water is 1.0); Rotation Period, 10 hours, 14 minutes; Axis Inclination, 26 44 ; Oblateness, 0.1; Surface Gravity, 1.15 (Earth
More informationAs part of a solar system unit, this math lesson plan uses the diameters of the planets to teach place value, rounding and ordering numbers skills.
SOLAR SYSTEM As part of a solar system unit, this math lesson plan uses the diameters of the planets to teach place value, rounding and ordering numbers skills. Background for Solar System Math Lesson
More informationUranus System: 27 Satellites, Rings
Uranus System: 27 Satellites, Rings 1 27 Uranian Satellites Distance Radius Mass Satellite (000 km) (km) (kg) Discoverer Date --------- -------- ------ ------- ---------- ----- Cordelia 50 13? Voyager
More informationì<(sk$m)=bdjbab< +^-Ä-U-Ä-U
Space and Technology Genre Comprehension Skill Text Features Science Content Nonfiction Predict Captions Call Outs Text Boxes Glossary Solar System Scott Foresman Science 4.18 ì
More informationIcy Moons of Jupiter, Saturn, and Beyond Rosaly Lopes, JPL
Icy Moons of Jupiter, Saturn, and Beyond Rosaly Lopes, JPL Galilean satellites: Io, Europa, Ganymede, and Callisto Io: hot volcanoes, colorful surface, lots of sulfur, no impact craters Europa: icy crust,
More informationCASSINI HALF TIME REPORT
Jean Dominique Cassini CASSINI HALF TIME REPORT Christiaan Huygens Cassini-Huygens Second Anniversary Cassini Spacecraft Spacecraft Specs Height: 6.8 m (22 ft) Diameter: 4 m (13 ft) Mass: 2500 kg (2.8
More informationGalilean Moons of Jupiter
Astronomy A. Dayle Hancock adhancock@wm.edu Small 239 Office hours: MTWR 10-11am Satellites of Jupiter & Saturn Galilean satellites Similarities and differences among the Galilean satellites How the Galilean
More informationAntarctic Infrared Astronomy
Antarctic Astronomy Antarctic Infrared Astronomy AIR-T-40 40 cm Antarctic Infra-Red Telescope Overview AIR-C Predicted Performance Science Potential for AIR-T-40 Space Debris Planets Pre-Antarctic observations:
More informationHi-resolution Solar System textures for SpaceEngine 0.98
Hi-resolution Solar System textures for SpaceEngine 0.98 These addons Solar System HD and Solar System Ultra contains hi-resolution maps of some planets, moons and asteroids of the Solar System. The maps
More informationNANOSATELLITE PROBES IN INTERPLANETARY SPACE: AN AUGMENTED CASSINI MISSION. A Thesis. presented to
NANOSATELLITE PROBES IN INTERPLANETARY SPACE: AN AUGMENTED CASSINI MISSION A Thesis presented to the Faculty of California Polytechnic State University, San Luis Obispo In Partial Fulfillment of the Requirements
More informationTHE SEARCH FOR NITROGEN IN SATURN S MAGNETOSPHERE. Author: H. Todd Smith, University of Virginia Advisor: Robert E. Johnson University of Virginia
THE SEARCH FOR NITROGEN IN SATURN S MAGNETOSPHERE Author: H. Todd Smith, University of Virginia Advisor: Robert E. Johnson University of Virginia Abstract We have discovered N + in Saturn s inner magnetosphere
More informationSaturn. AST 101 chapter 12. Spectacular Rings and Mysterious Moons Orbital and Physical Properties Orbital and Physical Properties
Saturn Spectacular Rings and Mysterious Moons 12.1 Orbital and Physical Properties This figure shows the solar system from a vantage point that emphasizes the relationship of the jovian planets to the
More informationPA04/2 (JUN09PA04201) General CertiÞ cate of Education June 2009 Advanced Level Examination
Surname Other Names For Examiner s Use Centre Number Candidate Number Candidate Signature General CertiÞ cate of Education June 2009 Advanced Level Examination PHYSICS (SPECIFICATION A) Unit 4 Waves, Fields
More informationSolar System Layered Curriculum Assignment Sheet
Name Solar System Layered Curriculum Assignment Sheet Introductory Assignment (Required of ALL students) Read Kids Discover Planets Magazine and complete one of the assignments on the assignment sheet.
More informationSaturn 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
More informationLesson 3 The Outer Planets
Lesson 3 Student Labs and Activities Page Launch Lab 44 Content Vocabulary 45 Lesson Outline 46 MiniLab 48 Content Practice A 49 Content Practice B 50 Language Arts Support 51 Math Skills 53 School to
More informationLecture Outlines. Chapter 13. Astronomy Today 7th Edition Chaisson/McMillan Pearson Education, Inc.
Lecture Outlines Chapter 13 Astronomy Today 7th Edition Chaisson/McMillan Chapter 13 Uranus and Neptune Units of Chapter 13 13.1 The Discoveries of Uranus and Neptune 13.2 Orbital and Physical Properties
More informationPhys 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 29. Search for life on jovian moons. Habitability.
More informationThe Icy Moons. and the. Extended Habitable Zone
The Icy Moons and the Extended Habitable Zone Europa Interior Models Other Types of Habitable Zones Water requires heat and pressure to remain stable as a liquid Extended Habitable Zones You do not need
More informationJupiter & Saturn. Moons of the Planets. Jupiter s Galilean satellites are easily seen with Earth-based telescopes. The Moons
The Moons Jupiter & Saturn Earth 1 Mars 2 Jupiter 63 Saturn 47 Uranus 27 Neptune 13 Pluto 3 Moons of the Planets Galileo (1610) found the first four moons of Jupiter. Total 156 (as of Nov. 8, 2005) Shortened
More informationSpace Physics THE MOONS OF THE PLANETS 1
Space Physics THE MOONS OF THE PLANETS 1 Neeke Katharina Rothe 2010/10/18 1 Kjell Rönnmark, Umeå Universitet, fysik Contents 1 Planets 2 2 Natural Satellite 2 3 The moons 3 3.1 Earth-Moon............................
More informationMercury from Messenger
Mercury from Messenger 2 Mercury Surface Details 3 Leaving Mercury 4 Venus Volcano 5 Mars Gully Channels 6 Mars Lava Channels 7 Mars Sand Dunes 8 Mars Streaks on Slopes 9 Mars Slope Streaks 10 Mars North
More informationTest #2 Results : A 80 89: B 70 79: C 60 69: D <60: F
Test #2 Results 90 100: A 80 89: B 70 79: C 60 69: D
More informationJupiter and Saturn: Lords of the Planets
11/5/14 Jupiter and Saturn: Lords of the Planets Guiding Questions 1. Why is the best month to see Jupiter different from one year to the next? 2. Why are there important differences between the atmospheres
More informationClassifying the Solar System
Name Classifying the Solar System Introduction Scientists classify planets in many different ways. Today you work for NASA and will use information you gather from the Solar System Data Sheet and other
More informationAstronomy November, 2016 Introduction to Astronomy: The Solar System. Mid-term Exam 3. Practice Version. Name (written legibly):
Astronomy 101 16 November, 2016 Introduction to Astronomy: The Solar System Mid-term Exam 3 Practice Version Name (written legibly): Honor Pledge: On my honor, I have neither given nor received unauthorized
More informationSatellites of giant planets. Satellites and rings of giant planets. Satellites of giant planets
Satellites of giant planets Satellites and rings of giant planets Regular and irregular satellites Regular satellites: The orbits around the planet have low eccentricity and are approximately coplanar
More informationSurvey 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
More informationCassini ISS. The Imaging Science Subsystem. (The Cameras)
Cassini ISS The Imaging Science Subsystem (The Cameras) "We are the eyes of Cassini, our cameras capture all the dramatic sights and vistas there are to see around Saturn. And through their imagery, they
More informationReport to Planetary Science Decadal Survey Primitive Bodies Panel. Perspectives from the Previous PBP Experience,
Report to Planetary Science Decadal Survey Primitive Bodies Panel Perspectives from the Previous PBP Experience, 2001-2002 Primitive Bodies Panel Meeting, Sept. 9, 2009, Washington, DC Dale Cruikshank
More informationWhen you have completed this workbook, you should know and understand the following:
Name When you have completed this workbook, you should know and understand the following: Standard Description Passed SciBer Text III.1.a III.1.b. Understand and correctly use unit vocabulary. List the
More informationChapter 8 Jovian Planet Systems
Chapter 8 Jovian Planet Systems How do jovian planets differ from terrestrials? They are much larger than terrestrial planets They do not have solid surfaces The things they are made of are quite different
More informationSolar System Physical Data
Solar System Physical Data Physical Properties of Solar System Members Equatorial Mass 1 Density 2 H 2 O=1 Gravity 3 Albedo 4 SUN 865,278 miles 1,392,530 km 332,946 1.41 27.9 n/a MERCURY 3,032 miles 4,879
More informationTheory of periodical bursts of the Sun and the planets
Theory of periodical bursts of the Sun and the planets G.-P. Zhang a, * ( a Independent researcher, Shanghai 201400, China ) *Corresponding author. E-mail address: 435918950@qq.com ABSTRACT: Raise the
More informationSaturn s icy satellites and rings investigated by Cassini - VIMS. III. Radial compositional variability
Saturn s icy satellites and rings investigated by Cassini - VIMS. III. Radial compositional variability G. Filacchione a,, F. Capaccioni a, M. Ciarniello a, R. N. Clark b, J. N. Cuzzi c, P. D. Nicholson
More informationCelestial Mechanics and Orbital Motions. Kepler s Laws Newton s Laws Tidal Forces
Celestial Mechanics and Orbital Motions Kepler s Laws Newton s Laws Tidal Forces Tycho Brahe (1546-1601) Foremost astronomer after the death of Copernicus. King Frederick II of Denmark set him up at Uraniborg,
More informationGrades 1-6. Exploring Astronomy. Learning Lapbook with Study Guide. Sample Page. A Journey Through Learning
A J T L Grades 1-6 Exploring Astronomy Learning Lapbook with Study Guide A Journey Through Learning www.ajourneythroughlearning.com Copyright 2013 A Journey Through Learning 1 Authors-Paula Winget and
More informationPutting Earth In Its Place
Teacher Instructions Overview: During this activity, students build a model of our Solar System to gain insight into the relative sizes and distances involved. ives: The student will: create a scale model
More informationTraveler s Guide to the Planets Uranus & Neptune
Traveler s Guide to the Planets Uranus & Neptune 1. These worlds are the ice giants. (There are two or more answers to this a. Jupiter c. Saturn b. Neptune d. Uranus 2. Uranus is the th planet in the Solar
More informationLab #8. The Moons of the Outer Planets
Lab #8 The Moons of the Outer Planets Introduction In this lab, we will explore the outer planets and their fascinating moons using the latest information on the Web. There are several processes at work
More information3. The name of a particularly large member of the asteroid belt is A) Halley B) Charon C) Eris D) Ceres E) Triton
Summer 2013 Astronomy - Test 2 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 informationPLATO - 6. The outer solar system. Tethis eclipsed by Titan; Cassini (NASA)
PLATO - 6 The outer solar system Tethis eclipsed by Titan; Cassini (NASA) 1 The Jovian Planets Cassini image of Jupiter, Io, and Io s shadow (NASA/JPL) 2 The Jovian Planets Gas giants in the outer solar
More information1/13/16. Solar System Formation
Solar System Formation 1 Your Parents Solar System 21 st Century Solar System 2 The 21 st Century Solar System Sun Terrestrial Planets Asteroid Belt Jovian Planets Kuiper Belt Oort Cloud The Solar System:
More informationC A S S I N I MISSION PLAN. REVISION O, Change 1 August Jet Propulsion Laboratory California Institute of Technology
C A S S I N I MISSION PLAN REVISION O, Change 1 August 2005 J Jet Propulsion Laboratory California Institute of Technology PD 699-100, Rev O, chg 1 JPL D-5564, Rev O, chg 1 1.0 MISSION OVERVIEW... 1-1
More informationDr. Linda Spilker Cassini Project Scientist, JPL/Caltech Outer Planets Assessment Group 8 February 2016
Dr. Linda Spilker Cassini Project Scientist, JPL/Caltech Outer Planets Assessment Group 8 February 2016 Solstice Mission Inclination Profile Saturn s Breathing Atmosphere Saturn s atmosphere has been found
More informationSimilarities & Differences to Inner Planets
Similarities & Differences to Inner Planets Jupiter Jupiter: Basic Characteristics Mass = 1.898 10 27 kg (318 x Earth) Radius = 71,492 km (11x Earth) Albedo (reflectivity) = 0.34 (Earth = 0.39) Average
More informationSolar System. The Solar System. Nebular animation. Planets drawn to scale. Mercury. Mariner 10. Chapter 22 Pages
The Solar System Chapter 22 Pages 612-633 Solar System Planets drawn to scale Nebular animation Distances not to scale Earth approximately 12,800 km diameter Earth is about 150,000,000 km from Sun Mercury
More informationions in the Saturnian Magnetosphere
Main Rings Rhea Titan Enceladus torus Neutral H 2 and H 2 + ions in the Saturnian Magnetosphere Wendy Tseng 1, R. Johnson 1, M. Thomsen 2, T. Cassidy 3 and M. Elrod 1 1 University of Virginia, USA 2 Los
More informationThe Giant Planets [10]
The Giant Planets [10] Distance Period Diameter Mass Rotation Tilt (au) (yrs) (hrs) (deg) Earth 1 1 1 1 24.0 23 Jupiter 5.2 11.9 11.2 318 9.9 3 Saturn 9.5 29.5 9.4 95 10.7 27 Uranus 19.2 84.1 4.0 14 17.2
More informationActivity 3: Modeling the Sun/Earth System
Activity 3: Modeling the Sun/Earth System Time: 2 class periods (1 class period = 45 min) Materials: Solar system model Sun poster (optional) Rolling measuring wheel or 100-meter measuring tape Modeling
More informationDate: Wednesday, 2 November :00PM. Location: Museum of London
A voyage round Saturn, its rings and moons Transcript Date: Wednesday, 2 November 2011-1:00PM Location: Museum of London 2 November 2011 A Voyage Round Saturn, its Moons and Rings Professor Carolin Crawford
More informationThe observations. The deductions. Determine the density of the Galilean satellites. Two classes of Galilean satellites
The Galilean satellites are easily seen Spacecraft reveal unique properties The Galilean satellites mimic a planetary system Io is covered with volcanic sulfur compounds Io s interior is affected by Jupiter
More informationSolar System B Division Mesa Robles Invitational February 1, 2014
Solar System B Division Mesa Robles Invitational February 1, 2014 Team Name: Team #: Student Names: IMAGE SHEET A A B C D E F G H I J K L M N O P Q R S T U IMAGE SHEET B V W I X II Y Z A B C D E PLEASE
More informationDiscovering Planet X
Discovering Planet X Overview: An activity exploring parallax and then simulating the discovery of Pluto with a Blink Comparator via an online interactive. Target Grade Level: 3-5 Estimated Duration: 1
More informationChapter 8 Jovian Planet Systems
Chapter 8 Jovian Planet Systems How do jovian planets differ from terrestrials? They are much larger than terrestrial planets They do not have solid surfaces The things they are made of are quite different
More informationClass: 6 Science Date: 1/30/13 Solar System Simulator + Guide
Class: 6 Science Date: 1/30/13 Solar System Simulator + Guide Objectives Today we will learn information about each planet and continue to familiarize ourselves with the solar system. We will learn this
More informationPLANETARY TEMPERATURES
APS 1010 Astronomy Lab 97 Planetary Temperatures PLANETARY TEMPERATURES Mars is essentially in the same orbit. Mars is somewhat the same distance from the Sun, which is very important. We have seen pictures
More informationChapter 11 Lecture. The Cosmic Perspective Seventh Edition. Jovian Planet Systems
Chapter 11 Lecture The Cosmic Perspective Seventh Edition Jovian Planet Systems Jovian Planet Systems 2014 Pearson Education, Inc. Belts and Zones Rapid rotation of these planets stretch weather systems
More informationSOLAR SYSTEM B Division
SOLAR SYSTEM B Division Team Name: Team #: Student Names: IMAGE SHEET A E B C D F G H Spectrum I Spectrum II SS2014 Spectrum III Spectrum IV Spectrum V Spectrum VI 1. A. What satellite is pictured in Image
More informationMercury Named after: Mercury, the fast-footed Roman messenger of the gods. Mean Distance from the Sun: 57,909,175 km (35,983,093.1 miles) or 0.
Mercury Named after: Mercury, the fast-footed Roman messenger of the gods. Mean Distance from the Sun: 57,909,175 km (35,983,093.1 miles) or 0.387 astronomical units Diameter: 4,879.4 km (3,031.92 miles)
More informationThe Gas Giants Astronomy Lesson 13
The Gas Giants Astronomy Lesson 13 The four outer planets: Jupiter, Saturn, Uranus, and Neptune, are much larger and more massive than Earth, and they do not have solid surfaces. Because these planets
More informationUranus and Neptune. Uranus and Neptune Properties. Discovery of Uranus
Uranus and Neptune Uranus and Neptune are much smaller than Jupiter and Saturn, but still giants compared to Earth Both are worlds we know relatively little about Voyager 2 is the only spacecraft to visit
More informationJupiter and Saturn. Guiding Questions. Long orbital periods of Jupiter and Saturn cause favorable viewing times to shift
Jupiter and Saturn 1 2 Guiding Questions 1. Why is the best month to see Jupiter different from one year to the next? 2. Why are there important differences between the atmospheres of Jupiter and Saturn?
More informationTHE ORBITS OF SATURN S SMALL SATELLITES DERIVED FROM COMBINED HISTORIC AND CASSINI IMAGING OBSERVATIONS
The Astronomical Journal, 132:692 710, 2006 August # 2006. The American Astronomical Society. All rights reserved. Printed in U.S.A. A THE ORBITS OF SATURN S SMALL SATELLITES DERIVED FROM COMBINED HISTORIC
More informationEarth 110 Exploration of the Solar System Assignment 4: Jovian Planets Due in class Tuesday, Feb. 23, 2016
Name: Section: Earth 110 Exploration of the Solar System Assignment 4: Jovian Planets Due in class Tuesday, Feb. 23, 2016 The jovian planets have distinct characteristics that set them apart from the terrestrial
More informationChapter Introduction Lesson 1 Lesson 2 Lesson 3 Lesson 4 Chapter Wrap-Up
Chapter Introduction Lesson 1 The Structure of the Solar System Lesson 2 The Inner Planets Lesson 3 The Outer Planets Lesson 4 Dwarf Planets and Other Objects Chapter Wrap-Up NASA/JPL/USGS What kinds of
More informationUnusual Moon Information
Saturn s Numbers Saturn is 1.35 billion km from the Sun minimum. Saturn is 1.5 billion km from the Sun maximum. One day on Saturn takes about 10.67 hours. One full rotation around the sun takes about 29.5
More information