Jupiter: Giant of the Solar System

Size: px
Start display at page:

Download "Jupiter: Giant of the Solar System"

Transcription

1 Jupiter: Giant of the Solar System Jupiter s Red spot : A huge storm that has raged for over 300 years that is ~2x size of the Earth. Gas Giant is really a Liquid Giant! Pictures over ~7 years from Hubble

2 Jupiter Third brightest object in the sky (Moon and Venus) Largest size is: ~50 arc-seconds. Has 63 moons; 16 have size >10 km, 4 largest are Galilean Moons.

3 Property Earth Jupiter Radius 6378km 71492km (11.21 R E ) Mass 5.97x10 24 kg 1.90x10 27 kg = M E Average Density 5520kg/m kg/m 3 (0.241) Gravity Earth s Escape Speed 11.2km/s 59.5km/s Average Temperature = 1 M E 290K / 17C 124K / -149C (at Cloud tops) Eccentricity

4 More Properties of Jupiter Mass is ~1/1000 Mass of the Sun Sidereal orbital period years. Synodic orbital period days. Surface magnetic field 13.89x that of Earth Sidereal rotation period ~0.41 days, ~9h 55m Axial Tilt 3.08 Orbital inclination to the ecliptic 1.31

5 Differential Rotation Jupiter has no Solid Surface! Internal structure is mainly H 2 and He. Rotation rate varies with latitude. Faster at Equator by ~5mins. Rotation Bulge ~6.5% R Eq = 71,500km R Po = 66,900km

6 Jupiter s Atmosphere Ever-changing, multicoloured bands, parallel to the equator. Reds Yellows White Greens Tans Blues Browns

7 Atmospheric Composition Spectroscopic studies in UV, IR H 2 : 86.1% Helium: 13.8% Smaller amounts of: methane, ammonia, water vapour. Galileo Probe found traces of ethane and phosphine: PH 3, Xe, Ar, Kr, and elements C, N, S Note: Escape speed so high that light gases cannot escape Jupiter s gravity.

8 Atmospheric Bands Divided into Bright Zones and Dark Belts. Vary in both latitude and intensity. Left: Infra- Red image. Bright = Hot, Dark = Cold

9 Atmospheric Bands II No Seasons Dynamic patterns Light Zones warm rising gas will then cool. Dark belts Cool sinking gas will warm up. Convection Cycles

10 Zone / Belt Differences Different Pressures (Zones higher) Different Temperatures Different Colours due to different rates ons chemical reactions in clouds. Different Speeds (Faster near Equator) Different flow Directions (bit simplistic)

11 Zonal Flow Very stable underlying eastward and westward wind flow. Near Poles both zonal flow and bands disappear. Wind speed and direction relative to the Planet s internal rotation rate

12 Atmospheric Structure Colour due to complex chemical and photochemical reactions not fully understood (but involving Sulphur compounds). Different colours implies we are viewing different depths in atmosphere. Clouds in 3 main layers.

13 Layered Atmosphere Top of Troposphere is 0 km, as no solid surface. Ammonia ice: K (~ -140C) Ammonia + H 2 S ~200K (~ - 73C) Water ice/vapour

14 Galileo: Atmospheric Probe, 1995 Survived ~1hr before crushed at 150km! High Winds very deep in atmosphere Heated from surface? - rather than sunlight No pre-biotic compounds found! Galileo s entry point

15 Weather Systems: Jupiter s Great Red Spot White oval is ~ size of Earth and seen since Eye of a Hurricane Persistence due to no solid surface like Hurricanes

16 Red Spot s Stability Red Spot s size varies: in 1979 ~20,000km x 10,000km In 1976/7 ~40,000km x 14,000km

17 Smaller storms quite common. White Ovals Brown Oval hole in upper cloud layer. Only appear >20 N Last ~1-10 years Reasons for different colours not known. Jovial Storms

18 Shoemaker- Levy 9 comet July 1994 Jupiter s tidal forces broke up passing comet into 23 pieces. Hit on far side Biggest hit 600Megatons same as all Earth s Nuclear Weapons. Spectral analysis of explosions is hard

19 Views of Shoemaker-Levy 9 remnants from Hubble Over a period of weeks the high winds gradually erased the impact scars.

20 Jupiter s Emits Heat Based on distance from the Sun, expected cloud top temperature was 105K (-168C) Actually 125K (-148C) Small difference but it implies Jupiter emits 2x what it receives! Not due to radioactivity or fusion. Gravitational Energy converted to Heat

21 Jupiter s Internal Structure Mainly from theoretical modelling not direct evidence. No real surface Just gets denser, gradually becomes liquid. Super high densities and temperature. Interior has hydrogen in liquid metallic state Center is small rocky core Chemically like rocks not physically

22 Jupiter s Internal Structure II

23 Jupiter s Magnetic Field Very powerful magnetic Field due to rapid rotation of metallic hydrogen interior. Intrinsic strength ~ 20,000x Earth s Magnetosphere larger that the Sun s size and ~1million x bigger that that of Earth. Tail extends beyond Saturn s orbit. Magnetic Axis is offset by ~10 and poles are opposite to that of Earth. High-speed ions hostile to passing spacecraft!

24 Jupiter s Magnetosphere Inner region has a flat current sheet, charged particles forced into equatorial plane by rapid rotation. Plasma Torus due to Moon: Io (Discussed later)

25 Aurora on Jupiter! Inserts are UV photos of ions colliding with atmospheric gases!

Lecture Outlines. Chapter 11. Astronomy Today 8th Edition Chaisson/McMillan Pearson Education, Inc.

Lecture Outlines. Chapter 11. Astronomy Today 8th Edition Chaisson/McMillan Pearson Education, Inc. Lecture Outlines Chapter 11 Astronomy Today 8th Edition Chaisson/McMillan Chapter 11 Jupiter Units of Chapter 11 11.1 Orbital and Physical Properties 11.2 Jupiter s Atmosphere Discovery 11.1 A Cometary

More information

Jupiter. Jupiter is the third-brightest object in the night sky (after the Moon and Venus). Exploration by Spacecrafts

Jupiter. Jupiter is the third-brightest object in the night sky (after the Moon and Venus). Exploration by Spacecrafts Jupiter Orbit, Rotation Physical Properties Atmosphere, surface Interior Magnetosphere Moons (Voyager 1) Jupiter is the third-brightest object in the night sky (after the Moon and Venus). Exploration by

More information

12a. Jupiter. Jupiter Data (Table 12-1) Jupiter Data: Numbers

12a. Jupiter. Jupiter Data (Table 12-1) Jupiter Data: Numbers 12a. Jupiter Jupiter & Saturn data Jupiter & Saturn seen from the Earth Jupiter & Saturn rotation & structure Jupiter & Saturn clouds Jupiter & Saturn atmospheric motions Jupiter & Saturn rocky cores Jupiter

More information

12. Jovian Planet Systems Pearson Education Inc., publishing as Addison Wesley

12. Jovian Planet Systems Pearson Education Inc., publishing as Addison Wesley 12. Jovian Planet Systems Jovian Planet Properties Compared to the terrestrial planets, the Jovians: are much larger & more massive 2. are composed mostly of Hydrogen, Helium, & Hydrogen compounds 3. have

More information

Lecture 11 The Structure and Atmospheres of the Outer Planets October 9, 2017

Lecture 11 The Structure and Atmospheres of the Outer Planets October 9, 2017 Lecture 11 The Structure and Atmospheres of the Outer Planets October 9, 2017 1 2 Jovian Planets 3 Jovian Planets -- Basic Information Jupiter Saturn Uranus Neptune Distance 5.2 AU 9.5 AU 19 AU 30 AU Spin

More information

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. 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

More information

A Look at Our Solar System: The Sun, the planets and more. by Firdevs Duru

A Look at Our Solar System: The Sun, the planets and more. by Firdevs Duru A Look at Our Solar System: The Sun, the planets and more by Firdevs Duru Week 1 An overview of our place in the universe An overview of our solar system History of the astronomy Physics of motion of the

More information

The Jovian Planets. The Jovian planets: Jupiter, Saturn, Uranus and Neptune

The Jovian Planets. The Jovian planets: Jupiter, Saturn, Uranus and Neptune The Jovian planets: Jupiter, Saturn, Uranus and Neptune Their masses are large compared with terrestrial planets, from 15 to 320 times the Earth s mass They are gaseous Low density All of them have rings

More information

Jupiter and its Moons

Jupiter and its Moons Jupiter and its Moons Summary 1. At an average distance of over 5 AU, Jupiter takes nearly 12 years to orbit the Sun 2. Jupiter is by far the largest and most massive planet in the solar system being over

More information

Astro 101 Lecture 12 The Jovian Planets

Astro 101 Lecture 12 The Jovian Planets Astro 101 Lecture 12 The Jovian Planets 2-28-2018 Jupiter, Saturn, Uranus and Neptune ASTR-101 Section 004 Bulk Properties of Terrestrial and Jovian Planets All Jovian planets have strong magnetic fields

More information

The Jovian Planets (Gas Giants)

The Jovian Planets (Gas Giants) The Jovian Planets (Gas Giants) Discoveries and known to ancient astronomers. discovered in 1781 by Sir William Herschel (England). discovered in 1845 by Johann Galle (Germany). Predicted to exist by John

More information

Jupiter and Saturn: Lords of the Planets

Jupiter 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 information

Test #2 Results : A 80 89: B 70 79: C 60 69: D <60: F

Test #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 information

Saturn and Planetary Rings 4/5/07

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

More information

Inner and Outer Planets

Inner and Outer Planets Inner and Outer Planets Inner Planets Terrestrial planets are those that are closest to the Sun. Terrestrial planets are made mostly of rock and have similar characteristics to Earth. There are four terrestrial

More information

Chapter 11 Jovian Planet Systems. Comparing the Jovian Planets. Jovian Planet Composition 4/10/16. Spacecraft Missions

Chapter 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 information

The Outermost Planets. The 7 Wanderers known since Antiquity. Uranus and Neptune distinctly Blue-ish!

The Outermost Planets. The 7 Wanderers known since Antiquity. Uranus and Neptune distinctly Blue-ish! The Outermost Planets The 7 Wanderers known since Antiquity. Uranus and Neptune distinctly Blue-ish! Uranus Uranus and 3 of its moons, barely visible from Earth. Discovered by William Herschel 1781. (Accidentally!)

More information

Inner and Outer Planets

Inner and Outer Planets Inner and Outer Planets SPI 0607.6.2 Explain how the relative distance of objects from the earth affects how they appear. Inner Planets Terrestrial planets are those that are closest to the Sun. Terrestrial

More information

Lecture 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. 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 information

The Fathers of the Gods: Jupiter and Saturn

The Fathers of the Gods: Jupiter and Saturn The Fathers of the Gods: Jupiter and Saturn Learning Objectives! Order all the planets by size and distance from the Sun! How are clouds on Jupiter (and Saturn) different to the Earth? What 2 factors drive

More information

Chapter 10 Worlds of Gas and Liquid- The Giant Planets. 21st CENTURY ASTRONOMY Fifth EDITION Kay Palen Blumenthal

Chapter 10 Worlds of Gas and Liquid- The Giant Planets. 21st CENTURY ASTRONOMY Fifth EDITION Kay Palen Blumenthal Chapter 10 Worlds of Gas and Liquid- The Giant Planets 21st CENTURY ASTRONOMY Fifth EDITION Kay Palen Blumenthal What is a storm on Saturn like? The Giant Planets, Part 1 Jupiter, Saturn, Uranus, and Neptune

More information

Exploring The Planets: Jupiter

Exploring The Planets: Jupiter Exploring The Planets: Jupiter By Encyclopaedia Britannica, adapted by Newsela staff on 08.28.17 Word Count 691 Level 800L New Horizons spacecraft took this collection of images of Jupiter and Io in 2007.

More information

Chapter 11 Jovian Planet Systems. Jovian Planet Composition. Are jovian planets all alike? Density Differences. Density Differences

Chapter 11 Jovian Planet Systems. Jovian Planet Composition. Are jovian planets all alike? Density Differences. Density Differences Chapter 11 Jovian Planet Systems 11.1 A Different Kind of Planet Our goals for learning Are jovian planets all alike? What are jovian planets like on the inside? What is the weather like on jovian planets?

More information

Starting from closest to the Sun, name the orbiting planets in order.

Starting 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 information

Astronomy. physics.wm.edu/~hancock/171/ A. Dayle Hancock. Small 239. Office hours: MTWR 10-11am. Page 1

Astronomy.  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 information

Chapter 11 Jovian Planet Systems

Chapter 11 Jovian Planet Systems Chapter 11 Jovian Planet Systems 11.1 A Different Kind of Planet Our goals for learning: Are jovian planets all alike? What are jovian planets like on the inside? What is the weather like on jovian planets?

More information

Astronomy Ch. 11 Jupiter. MULTIPLE CHOICE. Choose the one alternative that best completes the statement or answers the question.

Astronomy Ch. 11 Jupiter. MULTIPLE CHOICE. Choose the one alternative that best completes the statement or answers the question. Name: Period: Date: Astronomy Ch. 11 Jupiter MULTIPLE CHOICE. Choose the one alternative that best completes the statement or answers the question. 1) Jupiter is noticeably oblate because: A) it has a

More information

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

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

More information

Chapter 11 Jovian Planet Systems. Jovian Planet Composition. Are jovian planets all alike? Density Differences. Density Differences

Chapter 11 Jovian Planet Systems. Jovian Planet Composition. Are jovian planets all alike? Density Differences. Density Differences Chapter 11 Jovian Planet Systems 11.1 A Different Kind of Planet Our goals for learning:! Are jovian planets all alike?! What are jovian planets like on the inside?! What is the weather like on jovian

More information

Chapter 11 Review Clickers. The Cosmic Perspective Seventh Edition. Jovian Planet Systems Pearson Education, Inc.

Chapter 11 Review Clickers. The Cosmic Perspective Seventh Edition. Jovian Planet Systems Pearson Education, Inc. Review Clickers The Cosmic Perspective Seventh Edition Jovian Planet Systems If Jupiter was the size of a basketball, Earth would be the size of a(n) a) bacterium. b) grain of rice. c) marble. d) orange.

More information

Investigating Astronomy Timothy F. Slater, Roger A. Freeman Chapter 7 Observing the Dynamic Giant Planets

Investigating Astronomy Timothy F. Slater, Roger A. Freeman Chapter 7 Observing the Dynamic Giant Planets Investigating Astronomy Timothy F. Slater, Roger A. Freeman Chapter 7 Observing the Dynamic Giant Planets Observing Jupiter and Saturn The disk of Jupiter at opposition appears about two times larger than

More information

Chapter 11 Lecture. The Cosmic Perspective Seventh Edition. Jovian Planet Systems Pearson Education, Inc.

Chapter 11 Lecture. The Cosmic Perspective Seventh Edition. Jovian Planet Systems Pearson Education, Inc. Chapter 11 Lecture The Cosmic Perspective Seventh Edition Jovian Planet Systems Jovian Planet Systems 11.1 A Different Kind of Planet Our goals for learning: Are jovian planets all alike? What are jovian

More information

Chapter 11 The Jovian Planets

Chapter 11 The Jovian Planets Chapter 11 The Jovian Planets The Jovian planets: Jupiter, Saturn, Uranus and Neptune Using Venus transit it was possible to get a good value of the AU (1639). Knowing the AU, it is possible to calculate

More information

A star is a massive sphere of gases with a core like a thermonuclear reactor. They are the most common celestial bodies in the universe are stars.

A star is a massive sphere of gases with a core like a thermonuclear reactor. They are the most common celestial bodies in the universe are stars. A star is a massive sphere of gases with a core like a thermonuclear reactor. They are the most common celestial bodies in the universe are stars. They radiate energy (electromagnetic radiation) from a

More information

Chapter 11 Jovian Planet Systems

Chapter 11 Jovian Planet Systems Chapter 11 Jovian Planet Systems 11.1 A Different Kind of Planet Our goals for learning: Are jovian planets all alike? What are jovian planets like on the inside? What is the weather like on jovian planets?

More information

Jovian Planet Systems

Jovian Planet Systems Jovian Planet Systems Reading: Chapter 14.1-14.5 Jovian Planet Systems Voyager 1 and 2 explored the outer planets in the 1970s and 1980s. The Galileo spacecraft circled Jupiter dozens of times in the late

More information

The scientific theory I like best is that the rings of. Saturn are composed entirely of lost airline luggage. Mark Russell

The scientific theory I like best is that the rings of. Saturn are composed entirely of lost airline luggage. Mark Russell The scientific theory I like best is that the rings of Saturn are composed entirely of lost airline luggage. Mark Russell What We Will Learn Today Why does Saturn have such a low density and how does that

More information

A Star is born: The Sun. SNC1D7-Space

A Star is born: The Sun. SNC1D7-Space A Star is born: The Sun SNC1D7-Space Exploring the Sun Our Sun, a star, is the most important celestial object for life on Earth. The solar nebula theory is the current theory used to explain the formation

More information

Astronomy 1 Winter Lecture 15; February

Astronomy 1 Winter Lecture 15; February Astronomy 1 Winter 2011 Lecture 15; February 9 2011 Previously on Astro-1 Mercury, Venus, Mars (and Earth) Size and composition Crusts and cores Volcanism and internal activity Stargazing Events Santa

More information

Our Planetary System. Chapter 7

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

More information

Jupiter is the most massive object in the Solar System (300x bigger than the Earth). It actually weighs as much as all the other

Jupiter is the most massive object in the Solar System (300x bigger than the Earth). It actually weighs as much as all the other Chapter 8 Part 1 The Giants: Jupiter and Saturn 5th Planet: Jupiter the Massive Jupiter is the most massive object in the Solar System (300x bigger than the Earth). It actually weighs as much as all the

More information

Lesson 3 THE SOLAR SYSTEM

Lesson 3 THE SOLAR SYSTEM Lesson 3 THE SOLAR SYSTEM THE NATURE OF THE SUN At the center of our solar system is the Sun which is a typical medium sized star. Composed mainly of Hydrogen (73% by mass), 23% helium and the rest is

More information

The Universe and Galaxies

The Universe and Galaxies The Universe and Galaxies 16.1 http://dingo.care-mail.com/cards/flash/5409/galaxy.swf Universe The sum of all matter and energy that exists, that has ever existed, and that will ever exist. We will focus

More information

MULTIPLE CHOICE. Choose the one alternative that best completes the statement or answers the question.

MULTIPLE CHOICE. Choose the one alternative that best completes the statement or answers the question. Homework Ch 7, 8, 9 Name MULTIPLE CHOICE. Choose the one alternative that best completes the statement or answers the question. 1) Our most detailed knowledge of Uranus and Neptune comes from 1) A) the

More information

Chapter 8 Part 1 The Giants: Jupiter and Saturn

Chapter 8 Part 1 The Giants: Jupiter and Saturn 5th Planet: Jupiter the Massive Chapter 8 Part 1 The Giants: Jupiter and Saturn Jupiter is the most massive object in the Solar System (300x bigger than the Earth). It actually weighs as much as all the

More information

Solar System Physics I

Solar System Physics I Department of Physics and Astronomy Astronomy 1X Session 2006-07 Solar System Physics I Dr Martin Hendry 6 lectures, beginning Autumn 2006 Lectures 4-6: Key Features of the Jovian and Terrestrial Planets

More information

Lecture 16 Dwarf Planets and Comets January 8a, 2014

Lecture 16 Dwarf Planets and Comets January 8a, 2014 1 Lecture 16 Dwarf Planets and Comets January 8a, 2014 2 Pluto -- Basic Information Discovered by Clyde Tombaugh in 1930 Period: P orb = 248 years Distance: a = 39.5 AU 3 moons (Charon, Nix, Hydra) Demoted

More information

Our Sun. The centre of our solar system

Our Sun. The centre of our solar system Our Sun The centre of our solar system Nicolaus Copernicus Our Sun The sun represents 99.86% of the mass in our solar system. It is ¾ hydrogen and ¼ helium. More than 1 million Earths can fit inside the

More information

The Solar System 6/23

The 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 information

Lecture 23: Jupiter. Solar System. Jupiter s Orbit. The semi-major axis of Jupiter s orbit is a = 5.2 AU

Lecture 23: Jupiter. Solar System. Jupiter s Orbit. The semi-major axis of Jupiter s orbit is a = 5.2 AU Lecture 23: Jupiter Solar System Jupiter s Orbit The semi-major axis of Jupiter s orbit is a = 5.2 AU Jupiter Sun a Kepler s third law relates the semi-major axis to the orbital period 1 Jupiter s Orbit

More information

days to rotate in its own axis km in diameter ( 109 diameter of the Earth ) and kg in mass ( mass of the Earth)

days to rotate in its own axis km in diameter ( 109 diameter of the Earth ) and kg in mass ( mass of the Earth) The Sun - It is located at the centre of our solar system with all planets and objects (comets and asteroids) revolving around it Page 1 of 6 - It s gravitational pull keeps the planets and other objects

More information

10/6/16. Observing the Universe with Gravitational Waves

10/6/16. Observing the Universe with Gravitational Waves Lecture Outline Observing the Universe with Gravitational Waves Thursday, October 13 7:00 PM Bell Museum Auditorium This event is free and open to the public, and will be followed by telescope observing.

More information

Solar System revised.notebook October 12, 2016 Solar Nebula Theory

Solar 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 information

Directed Reading B. Section: The Outer Planets

Directed Reading B. Section: The Outer Planets Skills Worksheet Directed Reading B Section: The Outer Planets 1. What is one way that gas giants differ from the terrestrial planets? a. They are much smaller. b. They are rocky and icy. c. They are made

More information

Overview of Solar System

Overview of Solar System Overview of Solar System The solar system is a disk Rotation of sun, orbits of planets all in same direction. Most planets rotate in this same sense. (Venus, Uranus, Pluto are exceptions). Angular momentum

More information

The Jovian Planets and Their Moons

The 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 information

Unit 3 Lesson 5 The Gas Giant Planets. Copyright Houghton Mifflin Harcourt Publishing Company

Unit 3 Lesson 5 The Gas Giant Planets. Copyright Houghton Mifflin Harcourt Publishing Company Florida Benchmarks SC.8.E.5.3 Distinguish the hierarchical relationships between planets and other astronomical bodies relative to solar system, galaxy, and universe, including distance, size, and composition.

More information

Uranus & Neptune: The Ice Giants. Discovery of Uranus. Bode s Law. Discovery of Neptune

Uranus & Neptune: The Ice Giants. Discovery of Uranus. Bode s Law. Discovery of Neptune Uranus & Neptune: The Ice Giants Discovery of Uranus Discovery of Uranus & Neptune Properties Density & Composition Internal Heat Source Magnetic fields Rings Uranus Rotational Axis by William Herschel

More information

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

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

More information

Universe Now. 4. Solar System II: Jovian planets

Universe Now. 4. Solar System II: Jovian planets Universe Now 4. Solar System II: Jovian planets An overview of the known Solar System The Sun 4 terrestrial planets: Mercury, Venus, The Earth, Mars 4 Jovian planets: Jupiter, Saturn, Uranus, Neptune 5

More information

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? 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 information

Astronomy 1001/1005 Midterm (200 points) Name:

Astronomy 1001/1005 Midterm (200 points) Name: Astronomy 1001/1005 Midterm (00 points) Name: Instructions: Mark your answers on this test AND your bubble sheet You will NOT get your bubble sheet back One page of notes and calculators are allowed Use

More information

Space Notes 2. Covers Objectives 3, 4, and 8

Space 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 information

Today. Jovian planets

Today. Jovian planets Today Jovian planets Global Wind Patterns Heat transport Global winds blow in distinctive patterns: Equatorial: E to W Mid-latitudes: W to E High latitudes: E to W 2014 Pearson Education, Inc. Circulation

More information

Motion of the planets

Motion 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 information

Unusual Moon Information

Unusual 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

Similarities & Differences to Inner Planets

Similarities & 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 information

ASTR 1050: Survey of Astronomy Fall 2012 PRACTICE Exam #2 Instructor: Michael Brotherton Covers Solar System and Exoplanet Topics

ASTR 1050: Survey of Astronomy Fall 2012 PRACTICE Exam #2 Instructor: Michael Brotherton Covers Solar System and Exoplanet Topics ASTR 1050: Survey of Astronomy Fall 2012 PRACTICE Exam #2 Instructor: Michael Brotherton Covers Solar System and Exoplanet Topics Instructions This exam is closed book and closed notes, although you may

More information

Uranus & Neptune, The Ice Giants

Uranus & Neptune, The Ice Giants Uranus & Neptune, The Ice Giants What We Will Learn Today How & When were Uranus & Neptune discovered? How are the interiors and weather on these planets? Why is Neptune as warm as Uranus? What are their

More information

Jupiter. Notes compiled by Paul Woodward Department of Astronomy

Jupiter. Notes compiled by Paul Woodward Department of Astronomy Jupiter Notes compiled by Paul Woodward Department of Astronomy We will spend about one week on the outer, gaseous planets, focusing first on Jupiter, then on Saturn. We will not spend time on Uranus and

More information

Which of the following statements best describes the general pattern of composition among the four jovian

Which 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 information

WHAT WE KNOW. Scientists observe that every object in the universe is moving away from each other. Objects furthest away are moving the fastest. So..

WHAT WE KNOW. Scientists observe that every object in the universe is moving away from each other. Objects furthest away are moving the fastest. So.. ASTRONOMY THE BIG BANG THEORY WHAT WE KNOW Scientists observe that every object in the universe is moving away from each other. Objects furthest away are moving the fastest. So.. WHAT DOES THIS MEAN? If

More information

FCAT Review Space Science

FCAT Review Space Science FCAT Review Space Science The Law of Universal Gravitation The law of universal gravitation states that ALL matter in the universe attracts each other. Gravity is greatly impacted by both mass and distance

More information

World Book at NASA. 12/29/2010 NASA - Jupiter. nasa.gov/ /jupiter_worldbook_prt.htm 1/5

World Book at NASA. 12/29/2010 NASA - Jupiter. nasa.gov/ /jupiter_worldbook_prt.htm 1/5 Print Close World Book at NASA Jupiter is the largest planet in the solar system. Its diameter is 88,846 miles (142,984 kilometers), more than 11 times that of Earth, and about one-tenth that of the sun.

More information

Earth, Uranus, Neptune & Pluto. 14a. Uranus & Neptune. The Discovery of Uranus. Uranus Data: Numbers. Uranus Data (Table 14-1)

Earth, Uranus, Neptune & Pluto. 14a. Uranus & Neptune. The Discovery of Uranus. Uranus Data: Numbers. Uranus Data (Table 14-1) 14a. Uranus & Neptune The discovery of Uranus & Neptune Uranus is oddly tilted & nearly featureless Neptune is cold & blue Uranus & Neptune are like yet dislike Jupiter The magnetic fields of Uranus &

More information

Lecture #11: Plan. Terrestrial Planets (cont d) Jovian Planets

Lecture #11: Plan. Terrestrial Planets (cont d) Jovian Planets Lecture #11: Plan Terrestrial Planets (cont d) Jovian Planets Mercury (review) Density = 5.4 kg / liter.. ~ Earth s Rocky mantle + iron/nickel core Slow spin: 59 days (orbital period = 88 days) No satellites

More information

1781: Uranus Discovered. The Outer Worlds. 1846: Neptune Discovered. Distance Comparison. Uranus Rotates Sideways. Exaggerated Seasons On Uranus

1781: Uranus Discovered. The Outer Worlds. 1846: Neptune Discovered. Distance Comparison. Uranus Rotates Sideways. Exaggerated Seasons On Uranus The Outer Worlds 1781: Discovered (accidentally!) by William Herschel using a 6 inch telescope [he thought it was a comet!] 2 Draft 12/03/2006 Updated May 05, 2011 1846: Discovered Le Verrier: proposed

More information

Earth Science 11 Learning Guide Unit Complete the following table with information about the sun:

Earth 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 information

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 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 information

Uranus and Neptune. Uranus and Neptune Properties. Discovery of Uranus

Uranus 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 information

Radiation - a process in which energy travels through vacuum (without a medium) Conduction a process in which energy travels through a medium

Radiation - a process in which energy travels through vacuum (without a medium) Conduction a process in which energy travels through a medium SOLAR SYSTEM NOTES ENERGY TRANSFERS Radiation - a process in which energy travels through vacuum (without a medium) Conduction a process in which energy travels through a medium Convection - The transfer

More information

The Outer Planets (pages )

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

More information

The Solar Nebula Theory. This lecture will help you understand: Conceptual Integrated Science. Chapter 28 THE SOLAR SYSTEM

The 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 information

Astronomy Unit Notes Name:

Astronomy Unit Notes Name: Astronomy Unit Notes Name: (DO NOT LOSE!) To help with the planets order 1 My = M 2 V = Venus 3 Eager = E 4 M = Mars 5 Just = J 6 Served = Saturn 7 Us = Uranus 8 N = N 1 Orbit: The path (usually elliptical)

More information

Solution for Homework# 3. Chapter 5 : Review & Discussion

Solution for Homework# 3. Chapter 5 : Review & Discussion Solution for Homework# 3 Chapter 5 : Review & Discussion. The largest telescopes are reflecting telescopes, primarily because of 3 distinct disadvantages of the refracting telescope. When light passes

More information

Jupiter and Saturn. Guiding Questions. Long orbital periods of Jupiter and Saturn cause favorable viewing times to shift

Jupiter 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 information

Did you know that ALL Jovian Planets have rings??

Did you know that ALL Jovian Planets have rings?? Outer Planets Did you know that ALL Jovian Planets have rings?? Jupiter: faint, dusty rings Saturn: bright, spectacular rings Uranus: dark, thin rings Neptune: dark, thin rings & ring arcs PLANET DATA

More information

Unit 6 Lesson 4 What Are the Planets in Our Solar System? Copyright Houghton Mifflin Harcourt Publishing Company

Unit 6 Lesson 4 What Are the Planets in Our Solar System? Copyright Houghton Mifflin Harcourt Publishing Company Unit 6 Lesson 4 What Are the Planets in Our Solar System? What other objects are near Earth in this part of space? Earth and millions of other objects make up our solar system. In Our Corner of Space A

More information

IX. 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

IX. 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 information

3. Titan is a moon that orbits A) Jupiter B) Mars C) Saturn D) Neptune E) Uranus

3. Titan is a moon that orbits A) Jupiter B) Mars C) Saturn D) Neptune E) Uranus Fall 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 well.

More information

What s in Our Solar System?

What s in Our Solar System? The Planets What s in Our Solar System? Our Solar System consists of a central star (the Sun), the main eight planets orbiting the sun, the dwarf planets, moons, asteroids, comets, meteors, interplanetary

More information

Welcome to the Solar System

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

More information

Developed in Consultation with Georgia Educators

Developed in Consultation with Georgia Educators Developed in Consultation with Georgia Educators Table of Contents Georgia Performance Standards Correlation Chart........... 7 Performance Standards Chapter 1 Earth and Space.............................

More information

Distance of Mercury to the Sun or the Orbital Radius

Distance of Mercury to the Sun or the Orbital Radius Distance of Mercury to the Sun or the Orbital Radius The minimum distance from the Sun to Mercury is about 45866304 kilometers and the maximum distance is about 70006464 kilometers. Space Station One Day

More information

Saturn. 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 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 information

Chapter 29. The Solar System. The Solar System. Section 29.1 Models of the Solar System notes Models of the Solar System

Chapter 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 information

Our Sun. & the Planets. Sun and Planets.notebook. October 18, Our Sun (a quick review) Hydrogen is the main fuel source

Our Sun. & the Planets. Sun and Planets.notebook. October 18, Our Sun (a quick review) Hydrogen is the main fuel source Sun and Planets.notebook October 18, 2016 Our Sun Our Sun (a quick review) Average size main sequence star Hydrogen is the main fuel source In about 5 billion years it will become a & the Planets red giant

More information

Name: Date: Hour: 179 degrees celsius. 5% of Earth A 70 pound person would weigh 27 pounds on Mercury.

Name: Date: Hour: 179 degrees celsius. 5% of Earth A 70 pound person would weigh 27 pounds on Mercury. Planet Exploration- http://www.kidsastronomy.com/solar_.htm Mercury 1 87.9 days 58.6 days 57 million Km 465 degrees celsius Minimum -184 degrees celsius 179 degrees celsius Moons Terrestrial or Gaseous?

More information

SOLAR SYSTEM NOTES. Scientists believe its at least 4.6 billion years old!!! 10/26/2017 ENERGY TRANSFERS RADIATION FROM THE SUN

SOLAR SYSTEM NOTES. Scientists believe its at least 4.6 billion years old!!! 10/26/2017 ENERGY TRANSFERS RADIATION FROM THE SUN SOLAR SYSTEM NOTES Our Solar System is composed of: 1. The Sun 2. The Planets 3. Asteroids 4. Comets 5. Meteors 6. Natural & Artificial satellites Remember: How old is our Solar System? Scientists believe

More information

Chapter 11. ASTRONOMY 202 Spring 2007: Solar System Exploration. Class 31: Jovian Planets [4/4/07] Announcements. Ice Ages and Global Warming

Chapter 11. ASTRONOMY 202 Spring 2007: Solar System Exploration. Class 31: Jovian Planets [4/4/07] Announcements. Ice Ages and Global Warming ASTRONOMY 202 Spring 2007: Solar System Exploration Instructor: Dr. David Alexander Web-site: www.ruf.rice.edu/~dalex/astr202_s07 Class 31: Jovian Planets [4/4/07] Announcements Ice Ages and Global Warming

More information