Uranus & Neptune, The Ice Giants

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

Lecture Outlines. Chapter 13. Astronomy Today 7th Edition Chaisson/McMillan Pearson Education, Inc.

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

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

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

Astronomy. Uranus Neptune & Remote Worlds

Uranus, Neptune, and Pluto. Outer Worlds 4/19/07

Lecture 25: The Outer Planets

Earth, Uranus, Neptune & Pluto

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

Saturn. Slightly smaller 1/3 the mass density 700 kg/m 3. Interior - light elements, lack of rocky materials. Voyager 2, NASA

Chapter 11 Jovian Planet Systems

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

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

Similarities & Differences to Inner Planets

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

ASTR-1010: Astronomy I Course Notes Section X

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

The Outer Planets (pages )

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

Jovian Planet Systems

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)

The Fathers of the Gods: Jupiter and Saturn

Universe Now. 4. Solar System II: Jovian planets

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

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

Traveler s Guide to the Planets Uranus & Neptune

Did you know that ALL Jovian Planets have rings??

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

Astro 101 Lecture 12 The Jovian Planets

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

Our Planetary System. Chapter 7

Saturn and Planetary Rings 4/5/07

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.

Page Uranus. Uranus's Structure

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 8 Jovian Planet Systems

Chapters 7&8. ASTRONOMY 202 Spring 2007: Solar System Exploration. Class 21: Solar System [3/12/07] Announcements.

A medium-sized star. The hottest object found in our solar system.

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

Chapter 8 Jovian Planet Systems

The Solar System. Tour of the Solar System

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

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

The Giant Planets [10]

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

Unusual Moon Information

Jupiter and its Moons

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

Astronomy 1140 Quiz 4 Review

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

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

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

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

By Andrew Hartsel. and. Evelyne Ridinger

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

Announcements THE OUTER PLANETS

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

The Gas Giants Astronomy Lesson 13

Directed Reading B. Section: The Outer Planets

Astronomy 1001/1005 Midterm (200 points) Name:

The Jovian Planets (Gas Giants)

Moons of Sol Lecture 13 3/5/2018

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

Solar System Research Teacher Notes The Sun

Chapter 8 Jovian Planet Systems

Pluto, the Kuiper Belt, and Trans- Neptunian Objects

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

Physical Science 1 Chapter 16 INTRODUCTION. Astronomy is the study of the universe, which includes all matter, energy, space and time.

Physics Homework 4 Fall 2015

ASTRO 120 Sample Exam

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

Earth & Space Science ~ The Solar System

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

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

Chapter 10 The Outer Planets

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

Ag Earth Science Chapter 23

11/11/08 Announce: Chapter 9. Jupiter. The Outer Worlds. Jupiter s Interior. Jupiter 11/11/2008. The Outer Planets

GIANT PLANETS & PLANETARY ATMOSPHERES

Chapter 8 Jovian Planet Systems

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

The Jovian Planets and Their Moons

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

SOLAR SYSTEM. planet feature cards

Physics 1305 Notes: The Outer Solar System

23.1 The Solar System. Orbits of the Planets. Planetary Data The Solar System. Scale of the Planets The Solar System

Chapter 8 Jovian Planet Systems

Chapter 8 Jovian Planet Systems

Unit 8. The Outer Planets

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

Jovian (Jupiter like) Planets

ASTR 380 Possibilities for Life in the Outer Solar System

Today. Jovian planets

Astro 1: Introductory Astronomy

Chapter 7 Our Planetary System

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

11.2 A Wealth of Worlds: Satellites of Ice and Rock

Transcription:

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 moons and rings like? What is special about Triton, Neptune s moon? How are these worlds unique in the SS?

Planet Details Property Uranus Neptune Semi-major axis 19.2 AU 30.1 AU Size (radius) 4.0 R Earth 3.9 R Earth Smallest Jovian Mass 14.5 M Earth 17.1 M Earth Average density 1.32 g/cc 1.64 g/cc Composition H, He, H-compounds H, He, H-compounds Cloud-top Temp 60 K 60 K As warm as Uranus! Moons > 27 > 13 Orbital period 84 years 165 years Rotation period * -17.3 hours Retrograde 16 hours Axis tilt 97.9 o Most extreme 29.6 o Orbital inclination 0.77 o 1.77 o Orbital eccentricity 0.046 0.010 * Measured based on rotation of magnetic field lines

Uranus & Neptune s Discovery First planets discovered using a telescope Uranus discovered in 1781 by William & Caroline Herschel Although faintly visible to naked-eye, does not wander as much due to its long 84 year orbit Discovered during a survey of the skies Careful observations of Uranus shows deviation in path vs. Newton s laws Adams & Leverrier independently predicted influence on Uranus from an unseen eighth planet Neptune discovered in 1846 by Galle based on Leverrier s prediction of its position!

Formation of Uranus & Neptune Similar to Jupiter and Saturn, core of about 10 M Earth formed from hydrogen compounds Accreted much smaller atmosphere Orbit around the Sun is much bigger Accretion slower as a result Solar wind blew away gas into interstellar space Stopped planet formation, leaving Uranus and Neptune less massive

Interior of Uranus & Neptune No liquid or metallic hydrogen Not enough pressure Rock & metal core Larger than Jupiter & Saturn as it is not weighed down by a large atmosphere Hydrogen compound layer Differentiated over rock & metal core unlike Jupiter & Saturn Gaseous hydrogen Visible clouds Uranus Cooled off and dull (as expected) Neptune Internal heat source! Perhaps due to ongoing contraction Like which other planet? Fig 11.5

Atmosphere & Weather ~ 84% H, 14% He, 2% CH 4 Methane condenses into snow flakes less than 100 km below the cloud tops Gives the blue color Methane gas above absorbs red light Methane clouds reflect blue light Why is Neptune bluer? Uranus has smog-like layer due to its extreme seasons Scatters blue light before reaching clouds Fig 11.7

Winds & Weather Uranus Voyager 2 saw no bands or clouds in 1986 Subsequent HST and AO observations reveal storms brewing Perhaps due to changing seasons NH seeing Sunlight after 42 years! Neptune Banded atmosphere with storms and clouds Great Dark Spot Lasted only about 6 years Fig 11.11 c, Keck IR image Fig 11.11 d

Magnetic Fields Moderate sized magnetosphere despite weak field Liquid core of metals and hydrogen compounds generate magnetic field Weaker solar wind pressure allows moderate sized magnetosphere Both magnetic axes are very tilted with respect to rotation axes Don t know why Fig 11.13

Uranus Medium Sized Moons All named after Shakespeare's characters Made mainly of ices (water, methane, ammonia) Voyager flyby gave us information and raised questions Ariel & Umbriel are virtual twins, but only Ariel shows evidence of volcanism & tectonics Titania & Oberon are also similar size, but only Titania shows geological activity Miranda, the smallest, shows many tectonic features and relatively few craters Perhaps due to past tidal heating Fig 11.28

Neptune s Captured Moons Many retrograde orbits, high inclinations Captured asteroids Triton is the largest captured object in the Solar System Coldest world in the solar system (high albedo) Once orbited the Sun as a KBO Larger than Pluto Retrograde orbit Spiraling into Neptune Will cross Roche Limit in about 100 million years Evidence of past geological activity Past eccentric orbit caused tidal heating Fig 11.29

Rings Uranus rings are tipped over Photo from HST in IR Neptune rings picture was taken by Voyager Fig 11.34

Unique Features of Uranus First SS planet to be discovered with a telescope Farthest naked eye planet, but not recognized as a planet The most tilted planet Moon and rings are like bulls-eye from the Sun/Earth Most extreme seasons 42 years of day and 42 years of night! The only gas giant to have no internal heat source

Unique Features of Neptune As warm as Uranus despite greater distance from the Sun Internal heat source Largest captured moon Retrograde orbit Many moons with wacky orbits Captured KBOs Triton is coldest world in the Solar System 35 K, -238 o C, -396 o F Smallest gas giant planet

Voyager Movies