Last Class. Jupiter. Today s Class

Similar documents
Last Class. Today s Class 11/28/2017

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

Chapter 11 Jovian Planet Systems

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

Juno. Fran Bagenal University of Colorado

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

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

Chapter 11 Jovian Planet Systems

11.2 A Wealth of Worlds: Satellites of Ice and Rock

Scott Bolton OPAG February 1, 2016

Chapter 8 Jovian Planet Systems

Jupiter and its Moons

Chapter 8 Jovian Planet Systems

Chapter 8 Jovian Planet Systems

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

Chapter 7 Our Planetary System

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

Jovian Planet Systems

Chapter 8 Jovian Planet Systems

Chapter 8 Jovian Planet Systems

Chapter 8 Jovian Planet Systems

The Fathers of the Gods: Jupiter and Saturn

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

Jovian (Jupiter like) Planets

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

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

Spacecraft to the Outer Solar System

Chapter 11 Lecture. The Cosmic Perspective Seventh Edition. Jovian Planet Systems

ESA s Juice: Mission Summary and Fact Sheet

Moons of Sol Lecture 13 3/5/2018

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

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

Overview of Solar System

Announcements. Writing assignment early deadline next Tuesday!

Welcome to the Solar System

Juno Status and Earth Flyby Plans. C. J. Hansen

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

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

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

The Jovian Planets. Huge worlds, heavily mantled in gas at the time of the formation of the Solar System.

Jet Propulsion Laboratory California Institute of Technology. Juno Update

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

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

Juno Update for OPAG. Steve Levin Juno Project Scien8st September 7, 2017

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

The Solar System. Sun. Rotates and revolves around the Milky Way galaxy at such a slow pace that we do not notice any effects.

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

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

The Galilean Moons. ENV235Y1 Yin Chen (Judy)

NSCI 314 LIFE IN THE COSMOS

Outline. Characteristics of Jupiter. Exploration of Jupiter. Data and Images from JUNO spacecraft

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

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

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.

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

The Moons of the Solar System

Astronomy 1140 Quiz 4 Review

Astronomy 1140 Quiz 3 Review

ASTR-1010: Astronomy I Course Notes Section X

The Galilean Satellites. Jupiter has four planetary-sized moons first seen by Galileo and easily visible in binoculars.

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

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

Phys 214. Planets and Life

Our Planetary System. Chapter 7

ASTRO 120 Sample Exam

The Outer Planets (pages )

Mimas, moon of Saturn and Death Star impersonator responsible for several gaps in Saturn s ring system

Inner and Outer Planets

The Solar System. Tour of the Solar System

Terrestrial Bodies of the Solar System. Valerie Rapson

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

The Sun and Planets Lecture Notes 6.

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

The Solar System 6/23

Chapter 11 The Jovian Planets

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

Outer Solar System. Jupiter. PHY outer-solar-system - J. Hedberg

Class Exercise. Today s Class. Overview of Mercury. Terrestrial Planet Interiors. Today s Class: Mercury & Venus

JUpiter Icy Moons Explorer (JUICE) Status report for OPAG. N. Altobelli (on behalf of O. Witasse) JUICE artist impression (Credits ESA, AOES)

ASTR 2020, Spring 2018

Omnis, in exitu eius, pulchrimma

Chapter 8 2/19/2014. Lecture Outline. 8.1 The Galilean Moons of Jupiter. Moons, Rings, and Plutoids. 8.1 The Galilean Moons of Jupiter

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?

The Jovian Planets and Their Moons

The observations. The deductions. Determine the density of the Galilean satellites. Two classes of Galilean satellites

19 October 2012! Moons of Jupiter! So many moons, so little

Earth 110 Exploration of the Solar System Assignment 4: Jovian Planets Due in class Tuesday, Feb. 23, 2016

Inner Planets (Part II)

Astronomy November, 2016 Introduction to Astronomy: The Solar System. Mid-term Exam 3. Practice Version. Name (written legibly):

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

ASTR 200 : Lecture 6 Introduction to the Solar System Pearson Education Inc., publishing as Addison-Wesley

Universe Now. 4. Solar System II: Jovian planets

1 of 5 4/21/2015 6:40 PM

The escape speed for an object leaving the surface of any celestial body of mass M and radius d is

Announcements THE OUTER PLANETS

Life in the outer Solar System. AST 309 part 2: Extraterrestrial Life

see disks around new stars in Orion nebula where planets are probably being formed 3

Interiors of Worlds and Heat loss

Life in the Outer Solar System

Transcription:

Today s Class: Jupiter & Its Waterworld Moons 1. Reading for Next Class: Saturn and its moons Chapter 11 in Cosmic Perspective. 2. Homework #8 will be due next Wednesday, April 18. 3. Need 2 more volunteers for Space in the News. Last Class The atmosphere of Venus. Greenhouse Effect on Venus & Earth. How did Earth s atmosphere end up so different from Venus? Effects of water and carbon Dangers of human activity Clicker Question: What is the leading hypothesis for Venus lack of water? Clicker Question: What is the leading hypothesis for Venus lack of water? a) It s water molecules were broken apart, and hydrogen was lost to space. b) Venus formed closer to the Sun and accreted very little water. c) Its water is locked away in the crust along with carbon. d) Active volcanoes absorbed all the water early in the evolution of Venus. a) It s water molecules were broken apart, and hydrogen was lost to space. b) Venus formed closer to the Sun and accreted very little water. c) Its water is locked away in the crust along with carbon. d) Active volcanoes absorbed all the water early in the evolution of Venus. Today s Class Inside Jupiter Source of heat Magnetosphere NASA s JUNO mission The moons of Jupiter Io: Active volcanoes Europa: Possible ocean & life? Jupiter Much farther from Sun than inner planets Mostly H/He; no solid surface 300 times more massive than Earth Many moons, rings 1

Jupiter s moons Io (shown here): active volcanoes all over Europa: possible subsurface ocean Ganymede: largest moon in solar system Callisto: a large, cratered "ice ball" Jupiter's moons can be as interesting as planets themselves, especially Jupiter's four Galilean moons. Inside Jupiter High pressures inside Jupiter cause phase of hydrogen to change with depth. Hydrogen acts like a metal at great depths because its electrons move freely. Jupiter's Internal Heat Jupiter radiates twice as much energy as it receives from the Sun. Energy probably comes from slow contraction of interior (releasing potential energy). Clicker Question: Jupiter does not have a large metal core like the Earth. How can it have a magnetic field? a) The magnetic field is left over from when Jupiter accreted. b) Its magnetic field comes from the Sun. c) It has metallic hydrogen inside, which circulates and makes a magnetic field. d) Its core creates a magnetic field, but it is very weak. Clicker Question: Jupiter does not have a large metal core like the Earth. How can it have a magnetic field? Jupiter's Magnetosphere a) The magnetic field is left over from when Jupiter accreted. b) Its magnetic field comes from the Sun. c) It has metallic hydrogen inside, which circulates and makes a magnetic field. d) Its core creates a magnetic field, but it is very weak. Jupiter's strong magnetic field (20,000 times Earth!) gives it an enormous magnetosphere. Gases escaping Io feed the donut-shaped Io torus. 2

Juno Solar-powered, spinning spacecraft 8 Science instruments Proposed/selected 2005 Launched Aug 5th 2011 Arrived Jul 4th 2016 The Juno Spacecraft Juno s key components: Solar arrays 2m x 7.5m arrays producing ~300 W Sun-pointed, spinning 2 rpm Waves Radio & plasma Spacecraft & Payload JunoCam camera UVS UV spectrometer JIRAM IR spectrometer Gravity Science MWR Microwaves SPACECRAFT DIMENSIONS Diameter: 66 feet (20 m) Height: 15 feet (4.5 m) JEDI High-energy particles JADE Low-energy particles Magnetometer Juno: Close Polar Orbit is Key 35 polar orbits Duck under radiation belts Skim above clouds Why are Jupiter's Galilean moons so geologically active? From JunoCam an education & public outreach instrument 3

Io's Volcanoes Io's Volcanic Activity Volcanic eruptions continue to change Io's surface. Io is the most volcanically active body in the solar system, but why? Tidal Heating Europa's Ocean: Waterworld? Io is squished and stretched as it orbits Jupiter. NASA/JPL/DLR Tidal stresses crack Europa's surface ice Europa's interior also warmed by tidal heating 4

Possible Robotic Mission to Europa Goal: JPL s Europa Clipper - investigate whether the icy moon could harbor conditions suitable for life. Investigation of Europa using a radiationtolerant spacecraft that would perform close flybys of the icy moon from a looping orbit around Jupiter. What did we learn Today? Inside Jupiter Source of heat Magnetosphere NASA s JUNO mission The moons of Jupiter Io: Active volcanoes Europa: Possible ocean & life? 5