PTYS/ASTR 206Outer Worlds 4/19/07 The Outer Worlds: Uranus, Neptune, and Pluto.

Slides:



Advertisements
Similar presentations
Survey of Astronomy Astro1010-lee.com Chapter 13 Uranus & Neptune.
Advertisements

The Outer Planets Chap 16, Sec 4.
THE OUTER PLANETS. The first four outer planets- Jupiter, Saturn, Uranus, and Neptune- are much larger and more massive than Earth, and they do not have.
Neptune. Discovery John Couch Adams, Cambridge mathematician, predicted the existence of an unseen planet. Uranus was being pulled slightly out of position.
Chapter 10: Worlds of Gas and Liquid- The Giant Planets.
Remote Worlds Chapter Fourten. ASTR 111 – 003 Fall 2007 Lecture 12 Nov. 19, 2007 Introducing Astronomy (chap. 1-6) Introduction To Modern Astronomy I:
Uranus and Neptune Astronomy 311 Professor Lee Carkner Lecture 19.
The Outer Solar System Note the different scale of the inner and outer solar system. Note that Mercury and Pluto have the largest orbital inclinations.
Uranus and Neptune Astronomy 311 Professor Lee Carkner Lecture 19.
Uranus and Neptune Astronomy 311 Professor Lee Carkner Lecture 19.
Section 4: The Outer Planets. Objectives  After completing the lesson, students will be able to...  Describe the main characteristics of the gas giant.
4-4 The Outer Planets The Solar System – Course 3.
Lecture 34 The Outer Planets. The Moon. The Origin of the Moon The Outer Planet Family Chapter 16.9 
Planets of the Solar system Section 4 Section 4: The Outer Planets Preview Key Ideas The Outer Planets Gas Giants Jupiter Saturn Uranus Neptune Objects.
The Gas Giant Planets Chapter 29 Section 3
Jovian Planets - Different than Terrestrial Planets Bigger & more massive Lower density, different composition All have rings All have many moons.
Ch The Outer Planets.
Lesson 4, Chapter 3.  The four outer planets – Jupiter, Saturn, Uranus, and Neptune are much larger and more massive than Earth and they do not have.
Neptune By: Megan Tharpe And Ashley Elder. Neptune Facts Neptune is the 8 th planet from the sun Its orbit: 4,504,000,000 km from sun Diameter: 49,532.
While viewing Jupiter, he discovered four satellites orbiting around the planet Jupiter was the chief of the gods for the Romans, the way Zeus was for.
Copyright © 2010 Pearson Education, Inc. The Jovian Planets Jupiter, Saturn, Uranus, Neptune.
ASTR178 Other Worlds A/Prof. Orsola De Marco
The Gas Giant Planets. Jupiter Origin of name: From the king of the gods, Zeus or Jupiter.
The Planet Uranus Uranus It was discovered by William Herschel on March 13, 1781 and was the first planet discovered in modern times. It is also the.
I.Uranus and Neptune: Discoveries, atmospheres, interiors, rotation, magnetic fields, moons, rings, Uranus’ axis tilt and seasons. II.Pluto and Charon:
3 rd brightest object in night sky Alternating light & dark bands Giant Red Spot Galilean moons (Io, Callisto, Ganymede, Europa)
ASTRO 101 Principles of Astronomy. Instructor: Jerome A. Orosz (rhymes with “boris”) Contact: Telephone:
The Outer Worlds Chapter Sixteen. Guiding Questions 1.How did Uranus and Neptune come to be discovered? 2.What gives Uranus its distinctive greenish-blue.
Uranus and Neptune Uranus: general information –Discovered in 1781 (Herschel) –Radius about 4x that of Earth –Mass about 14.5x that of Earth –Nearly featureless.
Gas Giants. The four outer planets are: Jupiter Saturn Uranus Neptune.
The Outer Worlds. Update! International Astronomical Union (IAU) voted on the re- definition of planets in Prague on Aug. 24, Pluto is no longer.
Uranus and Neptune Astronomy 311 Professor Lee Carkner Lecture 19.
Uranus. Uranus Uranus is the seventh planet from the Sun and the third-largest and fourth most massive planet in the Solar System. It is named after the.
THE PLANETS OF OUR SOLAR SYSTEM
Atmosphere - Uranus’ clouds are featureless blue. Neptune’s clouds show more variety and contrast than Uranus’.
The Outer Planets Know about Jupiter Know about Saturn
Outer Planets  Comparative Giant Planets  Jupiter  Saturn  Uranus  Neptune  Gravity  Tidal Forces Sept. 25, 2002.
The Jovian Planets, Part III Uranus and Neptune. URANUS The God of the Heavens.
The Outer Planets The Gas Giants.
Planets of the Solar system Section 4 Key Ideas Identify the basic characteristics that make the outer planets different from terrestrial planets. Compare.
Uranus.
Lecture Outlines Astronomy Today 8th Edition Chaisson/McMillan © 2014 Pearson Education, Inc. Chapter 13.
The Outer Planets Section Standard e. Students know the appearance, general composition, relative position and size, an motion of objects.
Chapter 13 Uranus and Neptune. Uranus was discovered in 1781 by Herschel; first planet to be discovered in more than 2000 years Little detail can be seen.
Copyright © 2010 Pearson Education, Inc. Lecture Outline Chapter 7 The Jovian Planets.
The Jovian Planets Jupiter Saturn (from Cassini probe!) Uranus Neptune (roughly to scale)
Uranus Neptune And their moons. Uranus Statistics Radius: 3.98 times Earth’s (25,559 km) Mass: times Earth’s (8.68 x 10^25 kg ) Density: 1.32 g/cm³.
Chapter 23 The Solar System Section 2 Outer Planets Notes 23-4.
Neptune Shaniya Malcolm General Science.  Surface Of Neptune  The Space Shuttle/ Voyager 2  Composition  Winds  When Discovered  Facts  Symbols.
Review: What did Kepler study? What is an ellipse? Why is Mars called the red planet? Why is Venus called Earth’s twin? What do the four terrestrial planets.
Universe Tenth Edition Chapter 14 Uranus, Neptune, Pluto and the Kuiper Belt: Remote Worlds Roger Freedman Robert Geller William Kaufmann III.
The Outer Worlds Chapter Sixteen. Introducing Astronomy (chap. 1-6) Introduction To Modern Astronomy I Planets and Moons (chap. 7-17) ASTR 111 – 003 Fall.
Unit 5 Lesson 2. Vocabulary  Solar System: A star and all the planets and other objects that revolve around it.  Planet: A body that revolves around.
I.Uranus and Neptune: Discoveries, atmospheres, interiors, rotation, magnetic fields, moons, rings, Uranus’ axis tilt and seasons. II.Pluto and Charon:
Chapter 14 Section 4. GAS GIANTS Jupiter, Saturn, Uranus, and Neptune Don’t’ have solid surfaces Atmospheres composed of mainly hydrogen and helium Thick.
THE OUTER PLANETS.
Section 3: The Outer Planets
14.4 The Solar System Outer Planets (page 562)
Bell work Every planet that has an atmosphere has weather. Jupiter's Great Red Spot appears to be very similar to a hurricane system on Earth, but it has.
The Outer Planets.
Section 4 – pg 562 The Outer Planets
The Planets of our solar system Part Two: Outer Gas Giants.
Section 3: The Outer Planets
Uranus, Neptune and Pluto
Uranus.
The Gas Giants...and Pluto
The Planets of our solar system Part Two: Outer Gas Giants.
THE OUTER PLANETS.
Neptune And their moons
Neptune And their moons
Presentation transcript:

PTYS/ASTR 206Outer Worlds 4/19/07 The Outer Worlds: Uranus, Neptune, and Pluto

PTYS/ASTR 206Outer Worlds 4/19/07 Announcements Reading Assignment –Finish Chapter 17 6 th homework due on Tuesday, April 24 Quiz on Tuesday, April 24 (will cover all lectures since the last exam and Chapters 14-17) Final Activity next Thursday –Come prepared with 2 multiple-choice final exam questions Next study-group session is Monday, April 23, from 10:30AM- 12:00Noon – in room 330. Public lecture – Tuesday, April 24 7:30PM (this room) Movie Night – Monday, April 23, 6:30PM (this room)

PTYS/ASTR 206Outer Worlds 4/19/07 Discovery of Uranus “Discovered” by William Herschel in 1781 (discovered by chance) –Herschel was an English musician and amateur astronomer –He used a 6.5” homemade reflector (it took him over 200 attempts to make it!) –Prior to its discovery, Uranus had been seen, but not recognized as a planet (it had been designated 34 Tauri) Herschel made many contributions to astronomy, including the discovery of binary star systems, and the motion of the solar system in space

PTYS/ASTR 206Outer Worlds 4/19/07 Discovery of Neptune The problem: –Uranus’s orbit didn’t match Newton’s Laws, with the forces from all known planets at that time Proposed solution – there must be another planet ! –Bode’s Law gives the distance to be 39 AU –Its mass must be about the same as Uranus

PTYS/ASTR 206Outer Worlds 4/19/07 Neptune’s Discovery John Couch Adams (English student) –Predicted its location in 1843 (using Newton’s Laws including the its force on Uranus to explain Uranus’s orbit) –George Airy (Astronomer Royal) wouldn’t look! Wanted a few more details worked out

PTYS/ASTR 206Outer Worlds 4/19/07 Neptune’s Discovery Urbain Le Verrier (French Professor) –Predicted its location in 1846 – published it –Airy (now interested) did not have good enough star charts –Johann Galle (German astronomer) did have good star charts –LeVerrier convinced Galle to look for it

PTYS/ASTR 206Outer Worlds 4/19/07 Neptune’s Discovery Galle found it in 30 minutes ! Galle is often credited for being the discoverer, although Adams and Le Verrier were the first to predict its presence –Instructors note: Why did Adams get credit? He never published it !

PTYS/ASTR 206Outer Worlds 4/19/07 Uranus and Neptune from Earth Uranus is visible with the naked eye under good (dark sky) conditions Neptune is not visible to the naked eye Both can be seen as planets with moderate-sized telescopes (rather than a point-like star) No surface features are visible without a filter –Only recently were a ground- based telescope able to discern surface features on Uranus using an IR filter and adaptive optics Uranus Neptune

PTYS/ASTR 206Outer Worlds 4/19/07 Uranus: Basic Facts Equatorial diameter of 51,800 kilometers –about 4 Earth diameters Mass is about 14.5 Earth masses Density =1.3 g/cm 3 Orbital period is years –About the average lifespan of a human average distance from the Sun is about 19 AU Retrograde rotation Rotational period is 17 hours 14 minutes. It has 27 moons –The two largest are Titania and Oberon –Both are about ½ the size of our moon

PTYS/ASTR 206Outer Worlds 4/19/07 Neptune: Basic Facts Equatorial diameter of 49,500 kilometers –Nearly 4 Earth diameters –A little bit smaller than Uranus Mass is about 17 Earth masses –A little bit more massive than Uranus Density = 1.7 g/cm 3 Orbital period is about 165 years It is about 29.8 AU from the Sun Rotational period is about 16 hours Has 13 moons –The largest is Triton which is about 3/4 the size of our moon

PTYS/ASTR 206Outer Worlds 4/19/07 Uranus’s Composition and Appearance The atmosphere of Uranus is composed of –83% hydrogen, –15% helium, –2% methane Methane absorbs red light, giving Uranus its blue-green color. –Methane on Uranus is 5 times more abundant than on Jupiter and Saturn It lacks an appreciable internal heat source, thus there are no visible surface features

PTYS/ASTR 206Outer Worlds 4/19/07 Uranus’s Atmosphere Visibly, Uranus appears as a virtually featureless hazy blue ball. –Lack of internal heat. –Clouds on Uranus are cold and don't billow up above the top haze layer. Seen in false color (at the right), Uranus reveals atmospheric features The atmosphere is arranged into clouds running at constant latitudes (like Jupiter and Saturn)

PTYS/ASTR 206Outer Worlds 4/19/07 Uranus has an unusual tilt Herschel discovered that moons were orbiting in a plane perpendicular to its orbit –Moons orbit about their parent body’s equator Uranus’s rotation axis is tilted 98 o with respect to the plane of its orbit about the Sun Thought to be the result of a collision with a planet sized body early in the solar system formation

PTYS/ASTR 206Outer Worlds 4/19/07

PTYS/ASTR 206Outer Worlds 4/19/07 Neptune’s Atmosphere Neptune's atmosphere is made up of hydrogen, helium, and methane. Neptune's has clouds and storm systems that revolve around the planet, but with wind speeds of 300 m/sec (700 mi/hr These winds are driven by an internal heat source (unlike Uranus)

PTYS/ASTR 206Outer Worlds 4/19/07 Neptune’s Clouds The clouds seen on Neptune are frozen methane in the atmosphere Much more cloud activity is seen on Neptune than on Uranus This is because Uranus lacks a substantial internal heat source while Neptune does –Neptune radiates more than twice the energy it receives from the Sun

PTYS/ASTR 206Outer Worlds 4/19/07 The Giant Dark Spot on Neptune Similar to Jupiter’s Giant Red Spot (GRS) However, the giant dark spot on Neptune is not as long-lived as the GRS on Jupiter –Disappeared in 1994 –Another re-appeared in the northern hemisphere in 1995 Rotates counterclockwise, as does the GRS on Jupiter

PTYS/ASTR 206Outer Worlds 4/19/07 Uranus and Neptune contain a higher proportion of heavy elements than Jupiter and Saturn Both Uranus and Neptune may have a rocky core (about the size of Earth) surrounded by a mantle of water and ammonia (like Windex!) Electric currents in the mantles may generate the magnetic fields of the planets

PTYS/ASTR 206Outer Worlds 4/19/07 The Origin of Magnetic Fields on Uranus and Neptune Not massive enough to possess a liquid metallic hydrogen layer like Jupiter H 2 O in the interior is under enough pressure to induce ionization –Ionization increases its electrical conductivity –An ionized-water dynamo!

PTYS/ASTR 206Outer Worlds 4/19/07 The magnetic axes of both Uranus and Neptune are steeply inclined from their axes of rotation The magnetic and rotational axes of all the other planets are more nearly parallel The magnetic fields of Uranus and Neptune are also offset from the centers of the planets

PTYS/ASTR 206Outer Worlds 4/19/07 Uranus and Neptune each have a system of thin, dark rings

PTYS/ASTR 206Outer Worlds 4/19/07

PTYS/ASTR 206Outer Worlds 4/19/07

PTYS/ASTR 206Outer Worlds 4/19/07 Triton (Moon of Neptune) Discovered by William Lassell only a month after Neptune was discovered Orbits Neptune in a retrograde orbit ! –opposite to the rotation direction of Neptune –The only large moon to do this The orbit is also highly inclined relative to Neptune’s equator Density = 2066 kg/m 3 –More rock than in Saturn’s moons Probably a captured asteroid!

PTYS/ASTR 206Outer Worlds 4/19/07 Triton (Moon of Neptune) Shows evidence of geological activity –Lacks large craters – it is a very young surface –Probably tidal heating from Neptune –Perhaps extreme tidal heating in the past It also has a tenuous nitrogen (N 2 ) atmosphere –70,000 times less atmospheric pressure than Earth –about 500 times thinner than the Martian atmosphere

PTYS/ASTR 206Outer Worlds 4/19/07 Pluto and Charon How was Pluto Discovered? What is the nature of the planet and its moon? Is Pluto a planet?

PTYS/ASTR 206Outer Worlds 4/19/07 Planet “X” Percival Lowell repeated Adams & Le Verrier calculations for planet “X” –He looked, but never found it After Lowell Died, there was a tedious search

PTYS/ASTR 206Outer Worlds 4/19/07 Lowell hired Clyde Tombaugh who discovered Pluto in 1930 Pluto was named after the lord of Hades (in Greek mythology), “PL” are the initials of Percival Lowell

PTYS/ASTR 206Outer Worlds 4/19/07 Pluto’s Discovery Only “planet” found by an American, and only planet found in the 20 th century Too small to effect the orbits of other planets –The calculations of Lowell didn’t matter

PTYS/ASTR 206Outer Worlds 4/19/07