Chapter 8 Part 1 The Giants: Jupiter and Saturn

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

If your plan is for one year, plant rice. If your plan is for 100 years, educate children. Confucius

The Fathers of the Gods: Jupiter and Saturn

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

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

Inner and Outer Planets

Our Planetary System. Chapter 7

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

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

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

Chapter 11 Jovian Planet Systems

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

Overview of Solar System

Inner and Outer Planets

11.2 A Wealth of Worlds: Satellites of Ice and Rock

ASTR-1010: Astronomy I Course Notes Section X

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

What s in Our Solar System?

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)

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

Jupiter & Saturn. Moons of the Planets. Jupiter s Galilean satellites are easily seen with Earth-based telescopes. The Moons

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

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

SOLAR SYSTEM B Division

The Outer Planets (pages )

Motion of the planets

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

Chapter 8 Jovian Planet Systems

The Solar System. Tour of the Solar System

The Solar System 6/23

Astronomy 1140 Quiz 4 Review

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

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

Chapter 8 Jovian Planet Systems

Announcement Test 2. is coming up on Mar 19. Start preparing! This test will cover the classes from Feb 27 - Mar points, scantron, 1 hr.

Chapter 8 Jovian Planet Systems

Moons of Sol Lecture 13 3/5/2018

Jupiter and Saturn s Satellites of Fire and Ice. Chapter Fifteen. Guiding Questions

Jovian Planet Systems

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

9/22/ A Brief Tour of the Solar System. Chapter 6: Formation of the Solar System. What does the solar system look like?

The Outer Planets. Video Script: The Outer Planets. Visual Learning Company

CVtpf 2-1. Section 1 Review. 3. Describe How did the process of outgassing help shape Earth's atmosphere?

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

Similarities & Differences to Inner Planets

Chapter 11 Jovian Planet Systems

ASTR 380 Possibilities for Life in the Outer Solar System

3. The moon with the most substantial atmosphere in the Solar System is A) Iapetus B) Io C) Titan D) Triton E) Europa

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

Object Type Moons Rings Planet Terrestrial none none. Max Distance from Sun. Min Distance from Sun. Avg. Distance from Sun 57,910,000 km 0.

Chapter 7 Our Planetary System

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

Jovian (Jupiter like) Planets

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

NSCI SEARCHING FOR LIFE IN OUR SOLAR SYSTEM: MOONS OF THE OUTER PLANETS PLUS: WHY IS PLUTO NO LONGER CNSIDERED A PLANET?

Chapter 10 The Outer Planets

3. The name of a particularly large member of the asteroid belt is A) Halley B) Charon C) Eris D) Ceres E) Triton

Jupiter and Saturn s Satellites of Fire and Ice. Chapter Fifteen

Joy of Science Experience the evolution of the Universe, Earth and Life

The Jovian Planets and Their Moons

Phys 214. Planets and Life

UNIT 3: Chapter 8: The Solar System (pages )

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..

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

Label next 2 pages in ISN Gas Giants. Make sure the following assignments are turned in:

Exploring The Planets: Jupiter

Chapter 8 Jovian Planet Systems

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

2. Which of the following planets has exactly two moons? A) Venus B) Mercury C) Uranus D) Mars E) Neptune

Chapter 8 Jovian Planet Systems

Chapter 8 Jovian Planet Systems

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

1. Cosmology is the study of. a. The sun is the center of the Universe. b. The Earth is the center of the Universe

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

Jupiter: Giant of the Solar System

When you have completed this workbook, you should know and understand the following:

OUR SOLAR SYSTEM. James Martin. Facebook.com/groups/AstroLSSC Twitter.com/AstroLSSC

The Jovian Planets. Why do we expect planets like this in the outer reaches of the solar system?(lc)

Class Announcements. Solar System. Objectives for today. Will you read Chap 32 before Wed. class? Chap 32 Beyond the Earth

Chapter Outline. Earth and Other Planets. The Formation of the Solar System. Clue #1: Planetary Orbits. Clues to the Origin of the Solar System

Celestial Objects. Background Questions. 1. What was invented in the 17 th century? How did this help the study of our universe? 2. What is a probe?

Did you know that ALL Jovian Planets have rings??

AST Section 2: Test 2

Universe Now. 4. Solar System II: Jovian planets

NSCI 314 LIFE IN THE COSMOS

Jupiter and its Moons

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

Distance of Mercury to the Sun or the Orbital Radius

Announcements THE OUTER PLANETS

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

Spacecraft to the Outer Solar System

STUDENT RESOURCE 1.1 INFORMATION SHEET. Vocabulary

Our Created Solar System Video

Chapter 23: Touring Our Solar System

Directed Reading B. Section: The Outer Planets

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.

Phys 214. Planets and Life

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

Lesson 3 The Outer Planets

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

Transcription:

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 other planets together. The movie 2010 aside, it is far below the mass needed to begin nuclear fusion and become a brown dwarf star. Jupiter s Vital Stats Jupiter s Clouds It rotates in about 10 hrs and takes 12 years to revolve around the Sun. It has a slightly eccentric orbit and high albedo. The high albedo is due to the beautiful high cloud structures. This closeup pic shows the swirling on the edges as clouds in darker areas sink and brighter ones rise. This happens while the whole atmosphere rotates around Jupiter every 10 hours. Jupiter s Cloud Bands Are Permanent and Changing Jupiter s Great Red Spot One notably long-lived feature is the Great Red Spot, which Cassini first spotted in the 1600s. It seems to be a large, permanent hurricane in this one cloud band. Over the past 10 years, it has begun to fade slightly, although it is just as big. 1

Jupiter in Cross-section We believe that Jupiter is made up of three cloud layers on top of a deep band of hydrogen/helium clouds. Notice that below the clouds, the temp and pressure quickly rise beyond what life could support. Comet Shoemaker-Levy Impact Sites We got more data on Jupiter s cloud structure from a cometary impact in 1994. We learned that the winds at the top of the clouds move at about Mach 3! Vital Stats on Galilean Moons Galilean Moon Surfaces Notice that Jupiter s moons are as big or bigger than the Moon and Mercury. They also are as heavy or heavier than the Moon they have iron in their cores that the Moon lacks. They are also as far out from Jupiter as the Moon is from Earth, but rotate much faster! They are set up above moving farther out from Jupiter, beginning with Io. Notice that t as you move out (right), the moons get smoother, grayer and icier Jupiter is a hot and active planet that boils away water. Europa is the only moon that might have life in a liquid water ocean under its icy surface. Cross-Section of Jupiter s Moons Io: Innermost and Volcanic Io is innermost and takes a beating from Jupiter s magnetic field. Jupiter keeps the mantle of Io stirred up and causes numerous gas volcanoes. Io is the most volcanically active place in the Solar System. 2

Europa May Have Life The presence of a large, warmish (60s F) ocean of liquid water leads many to believe that this is the most likely spot for life in the Solar System. While it is not likely, l conditions have been constant like this for billions of years and life may exist beneath the ice. There is no atmosphere above it, so life would have to be constrained to the deeper parts of the ocean. Ganymede: Grooved but not Dead Ganymede is the largest moon in the Solar System, but seems like a small planet in makeup. It is not volcanically active, but it does have an iron core and mantle like the Earth. It cooled long ago and now has a covering beneath its dusty surface. The ice heaves and settles producing halfmile high grooves on the surface. Callisto: Frozen at Impact Farthest out is Callisto which bears the scars of large impacts on its icy surface. Too far out for volcanism, Callisto s surface is coated with a shallow layer of ice that highlights past impacts. The largest impact crater, Valhalla, is almost 1500 miles across! Where is Bruce Willis when you need him? Other Moons of Jupiter Jupiter has at least a dozen more moons, but most of them look like lumpy Amalthea (compare to Mars moons, Phobos and Deimos). Jupiter also has a faint ring with small shepherd moons and some smaller moons that look like captured asteroids. Rings Around Jupiter Jupiter also has a faint ring inside the orbit of Io. Since Jupiter is so massive and gravitationally strong, it probably bl absorbed b most of the dust that could have made the rings bigger what we see today is just a hint of what the rings could have been. 6th Planet: Saturn the Ringed With the largest ring system among the planets, Saturn is one of the most recognizable planets. Smaller and lighter than Jupiter, it has far less gravitational and magnetic influence than its massive neighbor. 3

Saturn s Vital Stats Saturn and Auroras Saturn is incredibly light less dense than water! It rotates in less than 11 hrs and also has a very high albedo (mostly due to the cloud layers). This view of Saturn shows high-altitude auroras at both poles on Saturn. You can also see that there are some bands in the atmosphere, but not as much as Jupiter probably due to lower gravity on Saturn. Comparing Jupiter and Saturn Jupiter is 4x more massive, but only 20% bigger than Saturn. This lower mass translates to a lower compression of the hydrogen around Saturn s core and thus produces a weaker magnetic field. Its rocky core is larger but less dense this is mostly because it is not being compressed as much as Jupiter s core. Views of Saturn s Rings The angle of the rings are fixed by Saturn s magnetic field. So, as it revolves, the rings appear to change their shape as seen from the Earth. Every 15 years, the rings appear edge-on and are almost invisible next time is 2014. The Rings Have Internal Structure Wow! The rings are not solid, but made up of many smaller rings of various thicknesses and widths. Here you can see some of fthe gaps and rings in the Cassini and Encke divisions of the rings. These gaps are probably caused by small shepherd moons (more later). 4

Titan: A Moon with Atmosphere Haze on Titan Titan, the most massive Saturnian moon, is the only moon in the Solar System with an atmosphere. The atmosphere is very hazy and impossible to see through. We do know that it is very cold (200 F below 0) and probably can t support any forms of life. The Hubble ST took this pic in infra-red to look at heat on Titan s surface. Notice that there are features, but we can t tell if they are on the surface or beneath the highest clouds. What are probably seeing is an ocean of liquid ethane and these are warm spots in the moonwide ocean. Shepherd Moons of Saturn This image shows 2 of the 22 known Saturnian moons around one of the outer rings. These moons shepherd the ring particles, using their gravitational influence to keep the ring together and distinct. 5