2007 Pearson Education Inc., publishing as Pearson Addison-Wesley. The Jovian Planets



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

Our Planetary System. Earth, as viewed by the Voyager spacecraft Pearson Education, Inc.

Chapter 7 Our Planetary System. What does the solar system look like? Thought Question How does the Earth-Sun distance compare with the Sun s radius

Chapter 7 Our Planetary System. Agenda. Intro Astronomy. Intro Astronomy. What does the solar system look like? A. General Basics

Chapter 6 Formation of Planetary Systems Our Solar System and Beyond

Solar System Fact Sheet

Solar System Overview

NOTES: GEORGIA HIGH SCHOOL SCIENCE TEST THE SOLAR SYSTEM

THE SOLAR SYSTEM - EXERCISES 1

UNIT V. Earth and Space. Earth and the Solar System

Related Standards and Background Information

Cosmic Journey: A Solar System Adventure General Information

Asteroids. Earth. Asteroids. Earth Distance from sun: 149,600,000 kilometers (92,960,000 miles) Diameter: 12,756 kilometers (7,926 miles) dotted line

Name: João Fernando Alves da Silva Class: 7-4 Number: 10

Summary: Four Major Features of our Solar System

A Solar System Coloring Book

CHARACTERISTICS OF THE SOLAR SYSTEM

Science 9 Worksheet 13-1 The Solar System

Name Date THE OUTER PLANETS

Lab 7: Gravity and Jupiter's Moons

A SOLAR SYSTEM COLORING BOOK

Lesson 6: Earth and the Moon

DESCRIPTION ACADEMIC STANDARDS INSTRUCTIONAL GOALS VOCABULARY BEFORE SHOWING. Subject Area: Science

Study Guide due Friday, 1/29

The Solar System. Olivia Paquette

WELCOME to Aurorae In the Solar System. J.E. Klemaszewski

The Layout of the Solar System

The atmospheres of different planets

Europa and Titan: Oceans in the Outer Solar System? Walter S. Kiefer, Lunar and Planetary Institute, Houston TX

Discover the planets of our solar system. In 90 minutes through the universe. On a hiking path between Ehrenfriedensdorf and Drebach

Lecture 12: The Solar System Briefly

Copyright 2006, Astronomical Society of the Pacific

Geol 116 The Planet Class 7-1 Feb 28, Exercise 1, Calculate the escape velocities of the nine planets in the solar system

Chapter 12 Asteroids, Comets, and Dwarf Planets. Asteroid Facts. What are asteroids like? Asteroids with Moons Asteroids and Meteorites

The Earth, Sun, and Moon

Solar Nebula Theory. Basic properties of the Solar System that need to be explained:

Solar System Formation

Chapter 8 Formation of the Solar System. What theory best explains the features of our solar system? Close Encounter Hypothesis

California Standards Grades 9 12 Boardworks 2009 Science Contents Standards Mapping

Class 2 Solar System Characteristics Formation Exosolar Planets

Earth Is Not the Center of the Universe

Chapter 8 Welcome to the Solar System

Perspective and Scale Size in Our Solar System

Probing for Information

Solar System Fundamentals. What is a Planet? Planetary orbits Planetary temperatures Planetary Atmospheres Origin of the Solar System

The Main Point. Lecture #34: Solar System Origin II. Chemical Condensation ( Lewis ) Model. How did the solar system form? Reading: Chapter 8.

LER Ages. Grades. Solar System. A fun game of thinking & linking!

Lecture 7 Formation of the Solar System. Nebular Theory. Origin of the Solar System. Origin of the Solar System. The Solar Nebula

4 HOW OUR SOLAR SYSTEM FORMED 750L

Chapter 8 Formation of the Solar System Agenda

Chapter 9 Asteroids, Comets, and Dwarf Planets. Their Nature, Orbits, and Impacts

Earth Sciences -- Grades 9, 10, 11, and 12. California State Science Content Standards. Mobile Climate Science Labs

Titan: The Solar System s Abiotic Petroleum Factory


Assignment 5. Multiple Choice Identify the letter of the choice that best completes the statement or answers the question.

The Solar System. Source

1 A Solar System Is Born

STUDY GUIDE: Earth Sun Moon

SGL 101 MATERIALS OF THE EARTH Lecture 1 C.M.NYAMAI LECTURE ORIGIN, STRUCTURE AND COMPOSITION OF THE EARTH

L3: The formation of the Solar System

Introduction and Origin of the Earth

KINDERGARTEN 1 WEEK LESSON PLANS AND ACTIVITIES

Background Information Students will learn about the Solar System while practicing communication skills.

Name Class Date. true

25 MS The Solar System Chapter Outline

Lecture 10 Formation of the Solar System January 6c, 2014

Unit 8 Lesson 2 Gravity and the Solar System

The Inner Solar System by Leslie Cargile

TO GO TO ANY OF THE PAGES LISTED BELOW, CLICK ON ITS TITLE

Rosaly Lopes, Jet Propulsion Laboratory, California Institute of Technology

Voyage: A Journey through our Solar System. Grades 5-8. Lesson 1: Our Solar System

Orbital Dynamics. Orbital Dynamics 1/29/15

3 rd Grape from the Sun Activity Timeline and Notes Nicholas McConnell, UC Berkeley, Intro and Group Assignments (10 minutes)

Atmospheric Layers. Ionosphere. Exosphere. Thermosphere. Mesosphere. Stratosphere. Troposphere. mi (km) above sea level 250 (400) 50 (80) 30 (50)

Georgia Performance Standards Framework for Science Grade 6. Unit Organizer: UNIVERSE AND SOLAR SYSTEM (Approximate Time 3 Weeks)

Introduction to the Solar System

Astronomy Notes for Educators

Study Guide: Solar System

Section 1 The Earth System

Our Solar System!!! Solar System scaled to accurate size, not distance from the Sun.

Pluto Data: Numbers. 14b. Pluto, Kuiper Belt & Oort Cloud. Pluto Data (Table 14-5)

AP Environmental Science Graph Prep

THE SOLAR SYSTEM AND THE UNIVERSE

Grade 6 Standard 3 Unit Test A Astronomy. 1. The four inner planets are rocky and small. Which description best fits the next four outer planets?

4 HOW OUR SOLAR SYSTEM FORMED 890L

The spectacular eruption of a volcano, the magnificent scenery of a

Journey to other celestial objects. learning outcomes

Lecture 23: Terrestrial Worlds in Comparison. This lecture compares and contrasts the properties and evolution of the 5 main terrestrial bodies.

The Solar System. Unit 4 covers the following framework standards: ES 10 and PS 11. Content was adapted the following:

4 HOW OUR SOLAR SYSTEM FORMED 1020L

CHAPTER 6 THE TERRESTRIAL PLANETS

Use the following information to deduce that the gravitational field strength at the surface of the Earth is approximately 10 N kg 1.

Composition of the Atmosphere. Outline Atmospheric Composition Nitrogen and Oxygen Lightning Homework

Solar System Facts & Fun

astronomy A planet was viewed from Earth for several hours. The diagrams below represent the appearance of the planet at four different times.

Lecture 13. Gravity in the Solar System

Transcription:

The Jovian Planets

The Jovian planets are gas giants - much larger than Earth

Sizes of Jovian Planets Planets get larger as they get more massive up to a point... Planets more massive than Jupiter are expected to shrink. There comes a point where gravity wins: adding more mass causes contraction.

Jovian Planet Composition Jupiter and Saturn Mostly H and He gas these are the most common elements in the Universe Gas Giants Uranus and Neptune Mostly hydrogen compounds: water (H 2 O), methane (CH 4 ), ammonia (NH 3 ) Some H, He, and rock Ice Giants

Interiors of Jovian Planets

Inside Jupiter High pressure inside of Jupiter causes the phase of hydrogen to change with depth. Hydrogen acts like a metal at great depths because its electrons move freely.

Inside Jupiter The core is thought to be made of rock, metals, and hydrogen compounds. The core is about the same size as Earth but 10 times as massive.

Comparing Jovian Interiors Models suggest that cores of jovian planets have similar composition. Lower pressures inside Uranus and Neptune mean no metallic hydrogen.

Jupiter s Atmosphere Hydrogen compounds in Jupiter form clouds. Different cloud layers correspond to freezing points of different hydrogen compounds. Other jovian planets have similar cloud layers.

Jupiter s Colors Ammonium sulfide clouds (NH 4 SH) reflect red/brown. Ammonia, the highest, coldest layer, reflects white.

Saturn s Colors Saturn s layers are similar but are deeper in and farther from the Sun more subdued.

Methane on Uranus and Neptune Methane gas on Neptune and Uranus absorbs red light but transmits blue light. Blue light reflects off methane clouds, making those planets look blue.

Weather on Jovian Planets All the jovian planets have strong winds and storms. The great red spot on Jupiter is a storm larger than Earth that has persisted for centuries.

Jovian planets are Big massive and cold, they can retain light elements like hydrogen and helium Escape Speed Jovian planets Hydrogen retained Terrestrial planets Oxygen retained Temperature

Jovian planets are Big massive and cold, they can retain light elements like hydrogen and helium their composition is like that of the stars the smaller terrestrial planets are the abnormal planets in terms of composition Like miniature solar systems moons rings Escape Speed Temperature

The moons of the Jovian planets Galilean moons of Jupiter ( Medici stars )

Sizes of Moons Small moons (< 300 km) No geological activity Medium-sized moons (300 1,500 km) Geological activity in past Large moons (> 1,500 km) Ongoing geological activity

Medium and Large Moons Enough self-gravity to be spherical Have substantial amounts of ice - as important as rock to overall composition Formed in orbit around jovian planets Circular orbits mostly in the same direction as planet rotation

Small Moons Far more numerous than the medium and large moons Not enough gravity to be spherical: potato-shaped

Some interesting cases: Io Io is the most volcanically active body in the solar system.

Tidal Heating Io is squished and stretched as it orbits Jupiter. Orbit is elliptical because of orbital resonances with other moons

Orbital Resonances The tugs add up over time, making all three orbits elliptical. Every 7 days, these three moons line up.

Volcanic eruptions continue to change Io s surface.

Europa Icy surface cracks driven by some geological activity Liquid ocean beneath? popular spot to speculate about the potential for life

Ganymede Largest moon in the solar system Clear evidence of geological activity Tidal heating plus heat from radioactive decay?

Saturn s large moon Titan Titan is the only moon in the solar system which has a thick atmosphere. It consists mostly of nitrogen with some argon, methane, and ethane.

Titan s Surface The Huygens probe provided a first look at Titan s surface in early 2005. It had liquid methane, rocks made of ice.

Neptune s Moon Triton Similar to Pluto, but larger Evidence for past geological activity orbits retrograde unique for such a large moon

Saturn s rings

What are Saturn s rings like? They are made up of numerous, small, icy particles. They orbit over Saturn s equator. They are very thin.

Artist s Conception in Ring

Elaborate structure in rings controlled by the gravity of shepherd moons Pan Prometheus 32

Newly discovered outer ring 33

34

Iapetus 35

actual data 36

Jovian Ring Systems All four jovian planets have ring systems. Others have smaller, darker ring particles than does Saturn. Rings and moons ubiquitous around Jovian planets like small solar systems.