Origin of the Solar System
|
|
- Trevor Ward
- 5 years ago
- Views:
Transcription
1 Origin of the Solar System and Solar System Debris 1
2 Debris comets meteoroids asteroids gas dust 2
3 Asteroids irregular, rocky hunks small in mass and size Ceres - largest, 1000 km in diameter (1/3 Moon) 3
4 Asteroid Belt 2.8 AU from the Sun, between Mars and Jupiter some with highly eccentric orbits, e.g. Icarus, goes inside the orbit of Mercury 5500 asteroids discovered so far 4
5 A Typical Asteroid fluctuates in brightness => tumbling, irregular in shape cratered surfaces, often rough and pitted lose chunks in collisions Toutatis - two orbiting each other 5
6 Categories of Asteroids S type (stony) relatively bright stony silicate materials C type (carbon) darker contains carbon compounds M type (metallic) brighter than C, darker than S metallic substances 6
7 Comets - Heralds of Disaster first seen as a bright blob later grows brighter and sprouts a tail as it nears the Sun 7
8 Comets coma: bright head of the comet may reach a million km diameter nucleus: small central core, about 10 km tail: material in the comet is heated by the Sun and vaporizes, can be millions of km s long 8
9 Two Tails! gas tail: ion tail emission lines ionized gas plasma carbon monoxide (CO) carbon dioxide (CO 2 ) molecular nitrogen (N 2 ) magnetic fields interact with plasma giving the comet a glow 9
10 dust tail: spectrum of sunlight reflected by the dust radiation pressure pushes dust out of the coma points downward from the ion tail 10
11 Dirty Snowball Model Nucleus: solid, compact body frozen ices (water, methane, ammonia) embedded in rocky material Coma: nears the Sun, icy material vaporizes, forming the coma Tail: continual vaporizing enlarges the coma and forms the tail 11
12 Periodic Comets make regular passes near the Sun follow Kepler s Laws have elliptical orbits short period: long period: orbit in same directions as the planets, less eccentric highly eccentric orbits, cut through plane of Solar System 12
13 Oort Cloud a reservoir of comets out beyond Pluto, beyond the Kuiper Belt (belt of icy objects) average semi-major axis is 50,000 AU, period of 10 million years, eccentricity close to 1 travel very slowly, spend a lot of time far out in their orbits 13
14 Wonder of It All How did they get out there in the first place? 14
15 Meteors and Meteoroids meteoroid: meteor: meteorite: name for particles and such before entering Earth s atmosphere solid particle that vaporizes in Earth s atmosphere particles large enough to survive and land on Earth 15
16 Origins of Meteoroids dust and ice flaked from comets 99% comes from comets follow orbits of original comets meteor showers: many meteors in a short period of time 16
17 irons stones Types of Meteoroids 90% iron, 9% nickel high density, melted appearance low density silicates similar to Earth s crust chondrules - silicate spheres carbonaceous chondrites: chondrules embedded in material containing a lot of carbon 17
18 stony iron: crossbreed between stones and irons meteorites - come from asteroids rather than from comets have enough density to make it through our atmosphere Identify a meteorite: etch a polished surface with acid and look for Widmanstatten figures They were originally inside a larger body and could cool slowly. 18
19 C type asteroid S type asteroid M type asteroid carbonaceous chondrite stony meteorite iron meteorites probable that the parent bodies were first things to form in the Solar System - ages will directly indicate the age of Solar System 19
20 Solar System Chemically: Sun mostly gaseous with some icy/rocky material as gases Terrestrial planets & asteroids rocky, metallic Jupiter, Saturn mostly gaseous Uranus, Neptune, Pluto, Charon, comets mostly icy 20
21 Dynamically planets revolve counterclockwise Sun rotates counterclockwise major planets have orbits only slightly inclined with plane of Sun exceptions: Pluto and Mercury planets move in orbits that are nearly circular (low eccentricity) exceptions: Pluto, Mercury 21
22 planets rotate counterclockwise (same direction as orbital motion exception: Venus, Uranus, Pluto planets orbital distances follow a regular spacing (sort of) - about twice as one before most satellites revolve in same direction as parent planet rotates and lie close to equatorial plane some satellites orbital distance follows a regular spacing rule 22
23 planets together contain more angular momentum than the Sun (99.5% vs 0.5%) long period comets - come in from all angles and directions short period comets, planets, satellites, asteroids - coplanar orbits all Jovian planets have rings 23
24 Nebular Model Sun and planets form from a cloud of interstellar material Sun forms in the center of flattened cloud Planets grow from the disk of the cloud Solar System is basically flat with the Sun in the middle. 24
25 Conservation of Angular Momentum once something starts spinning, it will continue unless acted on by an external influence angular momentum: tendency to keep spinning angular momentum depends on the mass and on how that mass is spread out Any time a body contracts (gets smaller), it spins faster in order to conserve angular momentum. 25
26 Imagine, a large cloud of gas and dust, slowly spinning. It starts to shrink, pulling in on itself with its own gravity. What happens? It spins even faster!! And eventually it collapses along the rotation axis. a flat disk with a fat center! 26
27 Nice model.. one problem... Angular momentum is not as expected. Sun 99% mass 1% ang. momentum Planets 1% mass 99% ang. momentum Sun should be spinning very rapidly! 27
28 gravitational contraction: a mass pulling itself together gets hotter gravitational potential energy kinetic energy (heat energy) As the cloud contracts, it gets hotter. 28
29 Stages of Evolution formation of nebula out of which the planets and Sun originate formation of original planetary debris evolution of planets dissipation of leftover gas and dust 29
30 Planetary Formation grains collide & accrete to form larger, pebble-sized objects pebbles accumulate into planetesimals by gravitational contraction composed of whatever is handy planetesimals gather into larger bodies takes tens of thousands of years clear out a space in the nebula protoplants - process takes 100 million years 30
31 Condensation Sequence temperature determines what materials condense below 2000 K, grains of terrestrial material condense below 273 K, grains of terrestrial and icy materials condense 31
32 Different distances from the Sun, different temperatures allow different materials to condense and form into grains. How LOW the temperature gets determines what materials. Leftover planetesimals bombard the new planets surfaces causing craters. 32
33 Planets become differentiated. Some rocky, metallic planetesimals end up as asteroids. Icy ones become comet nuclei. 33
1star 1 star 9 8 planets 63 (major) moons asteroids, comets, meteoroids
The Solar System 1star 1 star 9 8 planets 63 (major) moons asteroids, comets, meteoroids The distances to planets are known from Kepler s Laws (once calibrated with radar ranging to Venus) How are planet
More informationAt this point of its orbit, any solar satellite such as a comet or a planet is farthest away from the sun. What is the aphelion?
At this point of its orbit, any solar satellite such as a comet or a planet is farthest away from the sun. What is the aphelion? These small, rocky worlds orbit the sun generally between the orbits of
More informationEarth Science 11 Learning Guide Unit Complete the following table with information about the sun:
Earth Science 11 Learning Guide Unit 2 Name: 2-1 The sun 1. Complete the following table with information about the sun: a. Mass compare to the Earth: b. Temperature of the gases: c. The light and heat
More information23.1 The Solar System. Orbits of the Planets. Planetary Data The Solar System. Scale of the Planets The Solar System
23.1 The Solar System Orbits of the Planets The Planets: An Overview The terrestrial planets are planets that are small and rocky Mercury, Venus, Earth, and Mars. The Jovian planets are the huge gas giants
More informationThe Solar Nebula Theory. This lecture will help you understand: Conceptual Integrated Science. Chapter 28 THE SOLAR SYSTEM
This lecture will help you understand: Hewitt/Lyons/Suchocki/Yeh Conceptual Integrated Science Chapter 28 THE SOLAR SYSTEM Overview of the Solar System The Nebular Theory The Sun Asteroids, Comets, and
More informationMULTIPLE CHOICE. Choose the one alternative that best completes the statement or answers the question.
Chapter 4 - Group Homework Name MULTIPLE CHOICE. Choose the one alternative that best completes the statement or answers the question. 1) Density is defined as A) mass times weight. B) mass per unit volume.
More informationPrentice Hall EARTH SCIENCE
Prentice Hall EARTH SCIENCE Tarbuck Lutgens Chapter 23 Touring Our Solar System 23.1 The Solar System The Planets: An Overview The terrestrial planets are planets that are small and rocky Mercury, Venus,
More informationAstronomy A BEGINNER S GUIDE TO THE UNIVERSE EIGHTH EDITION
Astronomy A BEGINNER S GUIDE TO THE UNIVERSE EIGHTH EDITION CHAPTER 4 The Solar System Lecture Presentation 4.0 What can be seen with the naked eye? Early astronomers knew about the Sun, Moon, stars, Mercury,
More informationVagabonds of the Solar System
Vagabonds of the Solar System Guiding Questions 1. How and why were the asteroids first discovered? 2. Why didn t the asteroids coalesce to form a single planet? 3. What do asteroids look like? 4. How
More information12/3/14. Guiding Questions. Vagabonds of the Solar System. A search for a planet between Mars and Jupiter led to the discovery of asteroids
Guiding Questions Vagabonds of the Solar System 1. How and why were the asteroids first discovered? 2. Why didn t the asteroids coalesce to form a single planet? 3. What do asteroids look like? 4. How
More informationChapter 4 The Solar System
Chapter 4 The Solar System Comet Tempel Chapter overview Solar system inhabitants Solar system formation Extrasolar planets Solar system inhabitants Sun Planets Moons Asteroids Comets Meteoroids Kuiper
More informationStarting from closest to the Sun, name the orbiting planets in order.
Chapter 9 Section 1: Our Solar System Solar System: The solar system includes the sun, planets and many smaller structures. A planet and its moon(s) make up smaller systems in the solar system. Scientist
More informationCh 23 Touring Our Solar System 23.1 The Solar System 23.2 The Terrestrial Planet 23.3 The Outer Planets 23.4 Minor Members of the Solar System
Ch 23 Touring Our Solar System 23.1 The Solar System 23.2 The Terrestrial Planet 23.3 The Outer Planets 23.4 Minor Members of the Solar System Ch 23.1 The Solar System Terrestrial planets- Small Rocky
More informationUnit 3 Lesson 6 Small Bodies in the Solar System. Copyright Houghton Mifflin Harcourt Publishing Company
Florida Benchmarks SC.8.N.1.1 Define a problem from the eighth grade curriculum using appropriate reference materials to support scientific understanding, plan and carry out scientific investigations of
More informationPrentice Hall EARTH SCIENCE
Prentice Hall EARTH SCIENCE Tarbuck Lutgens 23.1 The Solar System The Planets: An Overview The terrestrial planets are planets that are small and rocky Mercury, Venus, Earth, and Mars. The Jovian planets
More informationAg Earth Science Chapter 23
Ag Earth Science Chapter 23 Chapter 23.1 Vocabulary Any of the Earth- like planets, including Mercury, Venus, and Earth terrestrial planet Jovian planet The Jupiter- like planets: Jupiter, Saturn, Uranus,
More informationChapter 23 Earth Science 11
Chapter 23 Earth Science 11 Inner planets: Closest planets to the sun A.k.a. terrestrial planets All have a rocky crust, dense mantle layer, and a very dense core Mercury, Venus, Earth, and Mars Outer
More informationComparative Planetology I: Our Solar System
Comparative Planetology I: Our Solar System Guiding Questions 1. Are all the other planets similar to Earth, or are they very different? 2. Do other planets have moons like Earth s Moon? 3. How do astronomers
More informationCHAPTER 11. We continue to Learn a lot about the Solar System by using Space Exploration
CHAPTER 11 We continue to Learn a lot about the Solar System by using Space Exploration Section 11.1 The Sun page 390 -Average sized star -Millions of km away -300,000 more massive then Earth, 99% of all
More information9.2 - Our Solar System
9.2 - Our Solar System Scientists describe our solar system as the Sun and all the planets and other celestial objects, such as moons, comets, and asteroids, that are held by the Sun s gravity and orbit
More informationWhich of the following statements best describes the general pattern of composition among the four jovian
Part A Which of the following statements best describes the general pattern of composition among the four jovian planets? Hint A.1 Major categories of ingredients in planetary composition The following
More informationVagabonds of the Solar System. Chapter 15
Vagabonds of the Solar System Chapter 15 ASTR 111 003 Fall 2007 Lecture 13 Nov. 26, 2007 Introduction To Modern Astronomy I: Solar System Introducing Astronomy (chap. 1-6) Planets and Moons (chap. 7-15)
More informationThe Formation of the Solar System
The Formation of the Solar System Basic Facts to be explained : 1. Each planet is relatively isolated in space. 2. Orbits nearly circular. 3. All roughly orbit in the same plane. 4. Planets are all orbiting
More informationGalaxies: enormous collections of gases, dust and stars held together by gravity Our galaxy is called the milky way
Celestial bodies are all of the natural objects in space ex. stars moons, planets, comets etc. Star: celestial body of hot gas that gives off light and heat the closest star to earth is the sun Planet:
More informationToday. Solar System Formation. a few more bits and pieces. Homework due
Today Solar System Formation a few more bits and pieces Homework due Pluto Charon 3000 km Asteroids small irregular rocky bodies Comets icy bodies Formation of the Solar System How did these things come
More informationAstronomy 3. Earth Movements Seasons The Moon Eclipses Tides Planets Asteroids, Meteors, Comets
Astronomy 3 Earth Movements Seasons The Moon Eclipses Tides Planets Asteroids, Meteors, Comets Earth s Movements Orbit- the path in which an object travels around another object in space Revolution the
More informationClicker Question: Clicker Question: Clicker Question:
Test results Last day to drop without a grade is Feb 29 Grades posted in cabinet and online F D C B A In which direction would the Earth move if the Sun s gravitational force were suddenly removed from
More informationComparative Planetology I: Our Solar System. Chapter Seven
Comparative Planetology I: Our Solar System Chapter Seven ASTR 111 003 Fall 2006 Lecture 07 Oct. 16, 2006 Introduction To Modern Astronomy I Introducing Astronomy (chap. 1-6) Planets and Moons (chap. 7-17)
More informationExploring Our Solar System
Exploring Our Solar System Our Solar System What do you think? Read the two statements below and decide whether you agree or disagree with them. Place an A in the Before column if you agree with the statement
More informationComparative Planetology I: Our Solar System. Chapter Seven
Comparative Planetology I: Our Solar System Chapter Seven ASTR 111 003 Fall 2006 Lecture 07 Oct. 16, 2006 Introduction To Modern Astronomy I Introducing Astronomy (chap. 1-6) Planets and Moons (chap. 7-17)
More informationThe Cosmic Perspective Seventh Edition. Asteroids, Comets, and Dwarf Planets: Their Natures, Orbits, and Impacts. Chapter 12 Review Clickers
Review Clickers The Cosmic Perspective Seventh Edition Asteroids, Comets, and Dwarf Planets: Their Natures, Orbits, and Impacts Asteroids a) are rocky and small typically the size of a grain of rice or
More informationAstronomy Wed. Oct. 6
Astronomy 301 - Wed. Oct. 6 Guest lectures, Monday and today: Prof. Harriet Dinerstein Monday: The outer planets & their moons Today: asteroids, comets, & the Kuiper Belt; formation of the Solar System
More informationUNIT 3: Chapter 8: The Solar System (pages )
CORNELL NOTES Directions: You must create a minimum of 5 questions in this column per page (average). Use these to study your notes and prepare for tests and quizzes. Notes will be turned in to your teacher
More informationOUR SOLAR SYSTEM. James Martin. Facebook.com/groups/AstroLSSC Twitter.com/AstroLSSC
OUR SOLAR SYSTEM James Martin Facebook.com/groups/AstroLSSC Twitter.com/AstroLSSC It s time for the human race to enter the solar system. -Dan Quayle Structure of the Solar System Our Solar System contains
More informationNotes: The Solar System
Notes: The Solar System The Formation of the Solar System 1. A gas cloud collapses under the influence of gravity. 2. Solids condense at the center, forming a protostar. 3. A falttened disk of matter surrounds
More information9/22/ A Brief Tour of the Solar System. Chapter 6: Formation of the Solar System. What does the solar system look like?
9/22/17 Lecture Outline 6.1 A Brief Tour of the Solar System Chapter 6: Formation of the Solar System What does the solar system look like? Our goals for learning: What does the solar system look like?
More informationChapter 19 The Origin of the Solar System
Chapter 19 The Origin of the Solar System Early Hypotheses catastrophic hypotheses, e.g., passing star hypothesis: Star passing closely to the the sun tore material out of the sun, from which planets could
More informationExam# 2 Review. Exam #2 is Wednesday November 8th at 10:40 AM in room FLG-280
Exam# 2 Review Exam #2 is Wednesday November 8th at 10:40 AM in room FLG-280 Bring Gator 1 ID card Bring pencil #2 with eraser No use of calculator or any electronic device during the exam We provide the
More informationGravity: Motivation An initial theory describing the nature of the gravitational force by Newton is a product of the resolution of the
Gravity: Motivation An initial theory describing the nature of the gravitational force by Newton is a product of the resolution of the Geocentric-Heliocentric debate (Brahe s data and Kepler s analysis)
More informationThe History of the Solar System. From cloud to Sun, planets, and smaller bodies
The History of the Solar System From cloud to Sun, planets, and smaller bodies The Birth of a Star Twenty years ago, we knew of only one star with planets the Sun and our understanding of the birth of
More informationWhat is it like? When did it form? How did it form. The Solar System. Fall, 2005 Astronomy 110 1
What is it like? When did it form? How did it form The Solar System Fall, 2005 Astronomy 110 1 Fall, 2005 Astronomy 110 2 The planets all orbit the sun in the same direction. The Sun spins in the same
More informationThe Solar System LEARNING TARGETS. Scientific Language. Name Test Date Hour
Name Test Date Hour Astronomy#3 - Notebook The Solar System LEARNING TARGETS I can describe the objects that make up our solar system. I can identify the inner and outer planets. I can explain the difference
More informationLecture Outlines. Chapter 15. Astronomy Today 7th Edition Chaisson/McMillan Pearson Education, Inc.
Lecture Outlines Chapter 15 Astronomy Today 7th Edition Chaisson/McMillan Chapter 15 The Formation of Planetary Systems Units of Chapter 15 15.1 Modeling Planet Formation 15.2 Terrestrial and Jovian Planets
More informationUnit 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
More informationAstr 1050 Wed., March. 22, 2017
Astr 1050 Wed., March. 22, 2017 Today: Chapter 12, Pluto and Debris March 24: Exam #2, Ch. 5-12 (9:00-9:50) March 27: Mastering Astronomy HW Chapter 11 & 12 1 Chapter 12: Meteorites, Asteroids, Comets
More informationChapter 19: Meteorites, Asteroids, and Comets
Chapter 19: Meteorites, Asteroids, and Comets Comet Superstition Throughout history, comets have been considered as portants of doom, even until very recently: Appearances of comet Kohoutek (1973), Halley
More informationThe Solar System. Name Test Date Hour
Name Test Date Hour Astronomy#3 - Notebook The Solar System LEARNING TARGETS I can describe the objects that make up our solar system. I can identify the inner and outer planets. I can explain the difference
More informationRadioactive Dating. U238>Pb206. Halflife: Oldest earth rocks. Meteors and Moon rocks. 4.5 billion years billion years
U238>Pb206 Halflife: 4.5 billion years Oldest earth rocks 3.96 billion years Meteors and Moon rocks 4.6 billion years This is the time they solidified The solar system is older than this. Radioactive Dating
More informationMoon Obs #1 Due! Moon visible: early morning through afternoon. 6 more due June 13 th. 15 total due June 25 th. Final Report Due June 28th
Moon Obs #1 Due! Moon visible: early morning through afternoon 6 more due June 13 th 15 total due June 25 th Final Report Due June 28th Our Solar System Objectives Overview of what is in our solar system
More informationLecture Outlines. Chapter 6. Astronomy Today 7th Edition Chaisson/McMillan Pearson Education, Inc.
Lecture Outlines Chapter 6 Astronomy Today 7th Edition Chaisson/McMillan Chapter 6 The Solar System Units of Chapter 6 6.1 An Inventory of the Solar System 6.2 Measuring the Planets 6.3 The Overall Layout
More informationAnnouncements. HW #3 is Due on Thursday (September 22) as usual. Chris will be in RH111 on that day.
Announcements The Albuquerque Astronomical Society (TAAS) is hosting a public lecture SATURDAY, SEPTEMBER 17TH - 7:00pm SCIENCE AND MATH LEARNING CENTER, UNM CAMPUS Free and open to the public USA Total
More informationFormation of the Solar System. What We Know. What We Know
Formation of the Solar System Many of the characteristics of the planets we discussed last week are a direct result of how the Solar System formed Until recently, theories for solar system formation were
More informationSolar System revised.notebook October 12, 2016 Solar Nebula Theory
Solar System revised.notebook The Solar System Solar Nebula Theory Solar Nebula was a rotating disk of dust and gas w/ a dense center dense center eventually becomes the sun start to condense b/c of gravity
More informationJoy of Science Experience the evolution of the Universe, Earth and Life
Joy of Science Experience the evolution of the Universe, Earth and Life Review Introduction Main contents Quiz Unless otherwise noted, all pictures are taken from wikipedia.org Review 1 The presence of
More informationChapter 23: Touring Our Solar System
Chapter 23: Touring Our Solar System The Sun The is the center of our solar system. The Sun makes up of all the mass of our solar system. The Sun s force holds the planets in their orbits around the Sun.
More informationBrooks Observatory telescope observing
Brooks Observatory telescope observing Mon. - Thurs., March 22 55, 8:30 to about 9:45 PM See the class web page for weather updates. This evening s session has been cancelled. Present your blue ticket
More information1 Solar System Debris and Formation
1 Solar System Debris and Formation Chapters 14 and 15 of your textbook Exercises: Do all Review and Discussion and all Conceptual Self-Test 1.1 Solar System Debris Asteroids small rocky bodies Most under
More informationHNRS 227 Fall 2006 Chapter 13. What is Pluto? What is a Planet? There are two broad categories of planets: Terrestrial and Jovian
Key Points of Chapter 13 HNRS 227 Fall 2006 Chapter 13 The Solar System presented by Prof. Geller 24 October 2006 Planets Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, Neptune Dwarf Planets Pluto,
More informationThe Solar System 6/23
6/23 The Solar System I. Earth A. Earth is the prototype terrestrial planet 1. Only planet in the solar system (we know of so far) with life 2. Temperature 290 K B. Physical Characteristics 1. Mass: 6
More informationJovian Planet Properties
The Outer Planets Jovian Planet Properties Jovian Planet Properties Compared to the terrestrial planets, the Jovians: are much larger & more massive are composed mostly of Hydrogen, Helium, & Hydrogen
More informationMaking a Solar System
Making a Solar System Learning Objectives! What are our Solar System s broad features? Where are asteroids, comets and each type of planet? Where is most of the mass? In what direction do planets orbit
More informationChapter 15: The Origin of the Solar System
Chapter 15: The Origin of the Solar System The Solar Nebula Hypothesis Basis of modern theory of planet formation: Planets form at the same time from the same cloud as the star. Planet formation sites
More informationWhat does the solar system look like?
What does the solar system look like? The solar system exhibits clear patterns of composition and motion. These patterns are far more important and interesting than numbers, names, and other trivia. Relative
More information9. Formation of the Solar System
9. Formation of the Solar System The evolution of the world may be compared to a display of fireworks that has just ended: some few red wisps, ashes, and smoke. Standing on a cool cinder, we see the slow
More informationThe Solar System. Tour of the Solar System
The Solar System Tour of the Solar System The Sun more later 8 planets Mercury Venus Earth more later Mars Jupiter Saturn Uranus Neptune Various other objects Asteroids Comets Pluto The Terrestrial Planets
More information1 of 5 5/2/2015 5:50 PM
1 of 5 5/2/2015 5:50 PM 1. A comet that has a semi-major axis of 100 AU must have a period of about 10 years. 20 years. 100 years. 1000 years. 2. Astronomers believe chondrite meteorites are about 4.6
More information-Melissa Greenberg, Arielle Hoffman, Zachary Feldmann, Ryan Pozin, Elizabeth Weeks, Christopher Pesota, & Sara Pilcher
-Melissa Greenberg, Arielle Hoffman, Zachary Feldmann, Ryan Pozin, Elizabeth Weeks, Christopher Pesota, & Sara Pilcher Formation Overview All explanations as to how the solar system was formed are only
More informationAstro 1: Introductory Astronomy
Astro 1: Introductory Astronomy David Cohen Class 16: Thursday, March 20 Spring 2014 large cloud of interstellar gas and dust - giving birth to millions of stars Hubble Space Telescope: Carina Nebula
More informationWhich 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,
More informationUnit 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
More informationEdmonds Community College ASTRONOMY 100 Sample Test #2 Fall Quarter 2006
Edmonds Community College ASTRONOMY 100 Sample Test #2 Fall Quarter 2006 Instructor: L. M. Khandro 10/19/06 Please Note: the following test derives from a course and text that covers the entire topic of
More informationFormation of the Solar System Chapter 8
Formation of the Solar System Chapter 8 To understand the formation of the solar system one has to apply concepts such as: Conservation of angular momentum Conservation of energy The theory of the formation
More informationAstronomy. physics.wm.edu/~hancock/171/ A. Dayle Hancock. Small 239. Office hours: MTWR 10-11am. Page 1
Astronomy A. Dayle Hancock adhancock@wm.edu Small 239 Office hours: MTWR 10-11am Planetology I Terrestrial and Jovian planets Similarities/differences between planetary satellites Surface and atmosphere
More informationSpace Notes 2. Covers Objectives 3, 4, and 8
Space Notes 2 Covers Objectives 3, 4, and 8 Sun Average Size Star Sun 101 Sun s Mass almost 100 times the mass of all the planets combined. Most of the mass is hydrogen gas Thermonuclear Reaction Thermonuclear
More informationPlanetary Geology Earth 9th Edition Chapter 24 Mass wasting: summary in haiku form Overview of the solar system The solar system
1 2 3 4 5 6 7 8 9 Planetary Geology Earth 9 th Edition Chapter 24 Mass wasting: summary in haiku form Can it be geo-? When there's only one planet qualified as "Earth?" Solar system includes Sun Eight
More informationPhysics Homework 5 Fall 2015
1) Long period comets are thought to reside mainly in the 1) A) Interstellar Medium. B) asteroid belt. C) Oort Cloud. D) Kirkwood gaps. E) Kuiper Belt. 2) Pluto is most similar to 2) A) Mercury. B) Triton.
More informationPhysics Homework 5 Fall 2015
1) As the solar nebula contracts it 1) A) cools due to condensation. B) spins faster due to conservation of angular momentum. C) flattens out into the ecliptic plane around the Sun's poles. D) loses angular
More informationMotion of the planets
Our Solar system Motion of the planets Our solar system is made up of the sun and the 9 planets that revolve around the sun Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, Neptune & Pluto (maybe?)
More informationSolar System. Sun, 8 planets, hundred moons, thousand.dwarf.planets million asteroids, billion comets etc.
Solar System Sun, 8 planets, hundred moons, thousand.dwarf.planets million asteroids, billion comets etc. Comparative Planetology Compares planets and other solar system bodies to help understand how they
More informationChapter Outline. Earth and Other Planets. The Formation of the Solar System. Clue #1: Planetary Orbits. Clues to the Origin of the Solar System
Chapter Outline Earth and Other Planets The Formation of the Solar System Exploring the Solar System Chapter 16 Great Idea: Earth, one of the planets that orbit the Sun, formed 4.5 billion years ago from
More informationPlanets: Name Distance from Sun Satellites Year Day Mercury 0.4AU yr 60 days Venus yr 243 days* Earth 1 1 yr 1 day Mars 1.
The Solar System (Ch. 6 in text) We will skip from Ch. 6 to Ch. 15, only a survey of the solar system, the discovery of extrasolar planets (in more detail than the textbook), and the formation of planetary
More informationIX. Dwarf Planets A. A planet is defined to be an object that is large enough to coalesce into a sphere and to have cleared its orbit of other
7/1 VII. VIII. Uranus A. Gas Giant 1. Rings but not visible 2. HUGE axial tilt 97! 3. Mostly hydrogen and helium 4. Medium rotation rate 5. Cold 55 K at the cloud tops B. Physical characteristics 1. Mass:
More informationThe solar system pt 2 MR. BANKS 8 TH GRADE SCIENCE
The solar system pt 2 MR. BANKS 8 TH GRADE SCIENCE Dwarf planets Following the discovery of multiple objects similar to Pluto (and one that was even bigger than Pluto) a new classification for planets
More informationThe History of the Earth
The History of the Earth We have talked about how the universe and sun formed, but what about the planets and moons? Review: Origin of the Universe The universe began about 13.7 billion years ago The Big
More informationAstronomy. physics.wm.edu/~hancock/171/ A. Dayle Hancock. Small 239. Office hours: MTWR 10-11am
Astronomy A. Dayle Hancock adhancock@wm.edu Small 239 Office hours: MTWR 10-11am Planetology II Key characteristics Chemical elements and planet size Radioactive dating Solar system formation Solar nebula
More informationA s t e r o i d s, C o m e t s & N E O s ( B a c k g r o u n d I n f o r m a t i o n )
A s t e r o i d s, C o m e t s & N E O s ( B a c k g r o u n d I n f o r m a t i o n ) Author: Sarah Roberts Asteroids Asteroids, Comets and NEOs - Background Information Asteroids are rocky objects which
More informationComparative Planetology II: The Origin of Our Solar System. Chapter Eight
Comparative Planetology II: The Origin of Our Solar System Chapter Eight ASTR 111 003 Fall 2007 Lecture 07 Oct. 15, 2007 Introduction To Modern Astronomy I: Solar System Introducing Astronomy (chap. 1-6)
More informationCosmology Vocabulary
Cosmology Vocabulary Vocabulary Words Terrestrial Planets The Sun Gravity Galaxy Lightyear Axis Comets Kuiper Belt Oort Cloud Meteors AU Nebula Solar System Cosmology Universe Coalescence Jovian Planets
More informationThis asteroid was visited by the NEAR Shoemaker probe, which orbited it, taking extensive photographs of its
Chapter 9 Part 1 Asteroids and Comets Why is there an asteroid belt? This asteroid was visited by the NEAR Shoemaker probe, which orbited it, taking extensive photographs of its surface, and, on February
More informationASTRONOMY SNAP GAME. with interesting facts
ASTRONOMY SNAP GAME with interesting facts Sun Sun The Sun is the largest object in the solar system The Sun's life expectancy is approximately 5 billion more years At its core, the Sun s temperature is
More informationAstronomy 1504 Section 10 Final Exam Version 1 May 6, 1999
Astronomy 1504 Section 10 Final Exam Version 1 May 6, 1999 Reminder: When I write these questions, I believe that there is one one correct answer. The questions consist of all parts a e. Read the entire
More informationWhy are Saturn s rings confined to a thin plane? 1. Tidal forces 2. Newton s 1st law 3. Conservation of energy 4. Conservation of angular momentum
Announcements Astro 101, 12/2/08 Formation of the Solar System (text unit 33) Last OWL homework: late this week or early next week Final exam: Monday, Dec. 15, 10:30 AM, Hasbrouck 20 Saturn Moons Rings
More informationThe Coriolis effect. Why does the cloud spin? The Solar Nebula. Origin of the Solar System. Gravitational Collapse
Origin of the Solar System Our theory must explain the data 1. Large bodies in the Solar System have orderly motions. 2. There are two types of planets. small, rocky terrestrial planets large, hydrogen-rich
More informationFormation of the Solar System
Formation of the Solar System What theory best explains the features of our solar system? The nebular theory states that our solar system formed from the gravitational collapse of a giant interstellar
More information37. Planetary Geology p
37. Planetary Geology p. 656-679 The Solar System Revisited We will now apply all the information we have learned about the geology of the earth to other planetary bodies to see how similar, or different,
More informationNews. Exam 4/Final is Saturday December 9 at 2:00 p.m. here in Clark 107
News Exam 4/Final is Saturday December 9 at 2:00 p.m. here in Clark 107 A review session will be held on Friday December 8 at 5:15 p.m. (most likely here in this room) A sheet of review questions is available
More informationContents of the Solar System
The Solar System Contents of the Solar System Sun Planets 9 known (now: 8) Mercury, Venus, Earth, Mars ( Terrestrials ) Jupiter, Saturn, Uranus, Neptune ( Jovians ) Pluto (a Kuiper Belt object?) Natural
More informationOverview of the Solar System. Solar system contents one star, several planets, lots of debris.
Overview of the Solar System Solar system contents one star, several planets, lots of debris. Most of it is the Sun! 99.8% of the mass of the Solar System resides in the Sun. A hot ball of mostly hydrogen
More informationChapter 29. The Solar System. The Solar System. Section 29.1 Models of the Solar System notes Models of the Solar System
The Solar System Chapter 29 The Solar System Section 29.1 Models of the Solar System 29.1 notes Models of the Solar System Geocentric: : Earth-centered model of the solar system. (Everything revolves around
More informationSPACE NOTES 2. Covers Objectives 3, 4, and 8
SPACE NOTES 2 Covers Objectives 3, 4, and 8 THE SUN Average Size Star Sun 101 SUN S MASS o almost 100 times the mass of all the planets combined. o Most of the mass is hydrogen gas THERMONUCLEAR REACTION
More information