Lecture 21. Outline Jupiter and Saturn –Orbit –Surface –Atmosphere –Rings –Moons.

Slides:



Advertisements
Similar presentations
Jupiter and Saturn: Lords of the Planets
Advertisements

Chapter 12 Saturn Chapter 12 opener. The number of known moons in the solar system increased rapidly during the late 1990s. Better telescopes enabled astronomers.
The Jovian Planets (“Gas Giants”): Jupiter, Saturn, Uranus, Neptune
The Sun 6.E.1.2 Explain why Earth sustains life while other planets do not based on their properties (including types of surface, atmosphere.
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.
Copyright © 2010 Pearson Education, Inc. Clicker Questions Chapter 7 The Jovian Planets.
Jupiter and Saturn’s Satellites of Fire and Ice Chapter Fifteen.
Jupiter Astronomy 311 Professor Lee Carkner Lecture 17.
Astronomy 1 – Winter 2011 Lecture 15; February
Saturn Astronomy 311 Professor Lee Carkner Lecture 18.
Uranus and Neptune Astronomy 311 Professor Lee Carkner Lecture 19.
METO 637 Lesson 22. Jupiter Jupiter and Saturn are known as the gas planets They do not have solid surfaces, their gaseous materials get denser with.
Jupiter Astronomy 311 Professor Lee Carkner Lecture 17.
Saturn Astronomy 311 Professor Lee Carkner Lecture 18.
Universe Eighth Edition Universe Roger A. Freedman William J. Kaufmann III CHAPTER 12 & 13 Jupiter, Saturn and their Moons CHAPTER 12 & 13 Jupiter, Saturn.
Chapter 7 The Outer Planets. What do you think? Is Jupiter a “failed star” or almost a star? What is Jupiter’s Great Red Spot? Does Jupiter have continents.
Jupiter Astronomy 311 Professor Lee Carkner Lecture 17.
The Gas Giants Astronomy 311 Professor Lee Carkner Lecture 16.
The Gas Giants Astronomy 311 Professor Lee Carkner Lecture 16.
By Julie Bingaman 5th Grade
Lecture Outlines Astronomy Today 8th Edition Chaisson/McMillan © 2014 Pearson Education, Inc. Chapter 11.
Lecture 34 The Outer Planets. The Moon. The Origin of the Moon The Outer Planet Family Chapter 16.9 
The Jovian Planets, Part II Saturn. SATURN The God of Agriculture.
Jupiter and Saturn: Lords of the Planets Chapter Fourteen.
The Gas Giant Planets Chapter 29 Section 3
Eight Planets A Write On Activity.
AST 111 Lecture 20 Jovian Worlds I. Jovian Worlds = 50 Earths.
Nine Planets A Write On Activity In this activity you will:  Learn about the solar system.  Practice your knowledge in an interactive game.  Select.
By: Ian McGorray Kevin Bhasin Gnana Umpathy Dean Bizga
Chapter 9 Lecture Outline
Copyright © 2010 Pearson Education, Inc. The Jovian Planets Jupiter, Saturn, Uranus, Neptune.
The Effects of the Jovian Planets on Bodies in the Solar System. Jiaqi Long, Evan Rauh, Maggie Aldworth, Will Fyfe.
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.
Jovian Planets: Jupiter and Saturn Shortened Version Feb 15, 2011.
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.
Greenhouse Effect Earth absorbs energy from the Sun and heats up Earth re-radiates the absorbed energy in the form of infrared radiation The infrared radiation.
Jupiter and Saturn: Lords of the Planets Chapter Fourteen.
A Transitional Fossil 375 Ma fish: flat nose, beginnings of limbs “Missing link” between fish and life on land.
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 Outer Planets The Gas Giants.
Interior - Internal Heating - Saturn reradiates three times as much energy as it absorbs; therefore, there must be an internal heat source.
Planets of the Solar system Section 4 Key Ideas Identify the basic characteristics that make the outer planets different from terrestrial planets. Compare.
Astronomy 1010 Planetary Astronomy Fall_2015 Day-35.
Jupiter and Saturn: Lords of the Planets. Guiding Questions 1.Why is the best month to see Jupiter different from one year to the next? 2.Why are there.
Copyright © 2010 Pearson Education, Inc. Lecture Outline Chapter 7 The Jovian Planets.
Universe Tenth Edition Chapter 12: Jupiter and Saturn: Lords of the Planets Roger Freedman Robert Geller William Kaufmann III.
Universe Tenth Edition Chapter 12 Jupiter and Saturn: Lords of the Planets Roger Freedman Robert Geller William Kaufmann III Clicker Questions.
Our Solar System Planets and other stuff!. The Sun Produces energy through nuclear fusion. ( 2 hydrogen nuclei fusing to make helium. Very hot: up to.
Saturn Astronomy 311 Professor Lee Carkner Lecture 18.
Universe Tenth Edition Chapter 14 Uranus, Neptune, Pluto and the Kuiper Belt: Remote Worlds Roger Freedman Robert Geller William Kaufmann III.
Copyright © 2010 Pearson Education, Inc. The Jovian Planets.
THE OUTER PLANETS.
Saturn In many ways, Saturn resembles a smaller version of Jupiter
Chapter 11 Section 3 Gas Giants.
© 2017 Pearson Education, Inc.
Section 3: The Outer Planets
Lecture 12.
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 Solar System Lesson 6 Jupiter and Saturn
Jupiter Astronomy 311 Professor Lee Carkner Lecture 17.
Jupiter and Saturn: Lords of the Planets
Jupiter and Saturn: Lords of the Planets
Section 3: The Outer Planets
Uranus.
Jupiter and Saturn – Size and Mass
The Atmospheres of the Outer Jovian Worlds
Jupiter and Saturn: Lords of the Planets
Presentation transcript:

Lecture 21

Outline Jupiter and Saturn –Orbit –Surface –Atmosphere –Rings –Moons

Outline Jupiter and Saturn –Orbit –Surface –Atmosphere –Rings –Moons

Why is the ecliptic at an angle with respect to the horizon?

Inferior planets superior planets

A planet’s synodic period is measured with respect to the Earth and the Sun (for example, from one opposition to the next)

Periods Rotational Orbital Sidereal Synodic Measured with respect to something that is not rotating or orbiting

Orbit

Question Which is longer, Jupiter’s synodic or orbital period? Which is longer, Jupiter’s synodic or Saturn’s synodic period? Guess Jupiter’s and Saturn’s synodic period.

Question As seen from Earth, does Jupiter or Saturn undergo retrograde motion more frequently?

Kepler’s Third Law P 2 = a 3 P = planet’s sidereal period, in years a = planet’s semimajor axis, in AU

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

The best time to observe Saturn from Earth is when it is A.at opposition and it is midnight at your location on Earth. B.at opposition and it is sunset or sunrise at your location on Earth. C.at conjunction and it is midnight at your location on Earth. D.at conjunction and it is sunset or sunrise at your location on Earth. E.at opposition and it is just before sunrise at your location on Earth.

Outline Jupiter and Saturn –Orbit –Surface –Atmosphere –Rings –Moons

What happens to ornaments when hoop is spun? hoop

A B C D

The oblateness of Jupiter and Saturn reveals their rocky cores Jupiter probably has a rocky core several times more massive than the Earth The core is surrounded by a layer of liquid “ices” (water, ammonia, methane, and associated compounds)

The oblateness of Jupiter and Saturn reveals their rocky cores On top of this is a layer of helium and liquid metallic hydrogen and an outermost layer composed primarily of ordinary hydrogen and helium Saturn’s internal structure is similar to that of Jupiter, but its core makes up a larger fraction of its volume and its liquid metallic hydrogen mantle is shallower than that of Jupiter

Metallic hydrogen inside Jupiter and Saturn endows the planets with strong magnetic fields Jupiter and Saturn have strong magnetic fields created by currents in the metallic hydrogen layer Jupiter’s huge magnetosphere contains a vast current sheet of electrically charged particles Saturn’s magnetic field and magnetosphere are much less extensive than Jupiter’s

Synchrotron Radiation Charged particles in the densest portions of Jupiter’s magnetosphere emit synchrotron radiation at radio wavelengths

Auroras on Jupiter and Saturn are caused by A.charged particles from the magnetosphere colliding with molecules in the upper atmosphere. B.ionized hydrogen. C.ionized helium. D.tidal interactions with the largest moons. E.gas circulating at the poles.

Outline Jupiter and Saturn –Orbit –Surface –Atmosphere –Rings –Moons

Atmospheres gravity and escape velocity

Atmospheres gravity and escape velocity

Atmospheres The visible “surfaces” of Jupiter and Saturn are actually the tops of their clouds

Atmospheres The rapid rotation of the planets twists the clouds into dark belts and light zones that run parallel to the equator

The chemical composition of Jupiter and Saturn is difficult to measure. Why?

Atmospheres The outer layers of both planets’ atmospheres show differential rotation –The equatorial regions rotate slightly faster than the polar regions

Atmospheres For both Jupiter and Saturn, the polar rotation rate is nearly the same as the internal rotation rate

Spacecraft images show remarkable activity in the clouds of Jupiter and Saturn

The internal heat of Jupiter and Saturn has a major effect on the planets’ atmospheres

Explain how Infrared and Visible (indicated on the previous slide) relate to the blackbody curves we studied.

A space probe has explored Jupiter’s deep atmosphere There are presumed to be three cloud layers in the atmospheres of Jupiter and Saturn The reasons for the distinctive colors of these different layers are not yet known The cloud layers in Saturn’s atmosphere are spread out over a greater range of altitude than those of Jupiter, giving Saturn a more washed-out appearance

Both Jupiter and Saturn emit more energy than they receive from the Sun. What does this tell us?

Jupiter radiates more energy into space than it receives from the Sun. What is the primary source of the excess energy that Jupiter radiates? A.Decay of radioactive materials in Jupiter's core B.Tidal forces from Jupiter's moons C.Jupiter is still contracting, and the contraction releases energy D.Jupiter's rotation is slowing down dramatically, and this slowdown releases energy E.All of the above are the energy sources

What can you say about these planets?

If Jupiter and Saturn formed at the same time, which should be emitting more heat?

Saturn’s atmosphere contains less helium than Jupiter’s atmosphere This lower abundance may be the result of helium raining downward into the planet Helium “rainfall” may also account for Saturn’s surprisingly strong heat output

Outline Jupiter and Saturn –Orbit –Surface –Atmosphere –Rings –Moons

Link

Something is Fishy How can a planet be solid?

Earth-based observations reveal three broad rings encircling Saturn

Saturn is circled by a system of thin, broad rings lying in the plane of the planet’s equator This system is tilted away from the plane of Saturn’s orbit, which causes the rings to be seen at various angles by an Earth-based observer over the course of a Saturnian year

Saturn’s rings are composed of numerous icy fragments, while Jupiter’s rings are made of small rocky particles The principal rings of Saturn are composed of numerous particles of ice and ice-coated rock ranging in size from a few micrometers to about 10 m Jupiter’s faint rings are composed of a relatively small amount of small, dark, rocky particles that reflect very little light

Most of its rings exist inside the Roche limit of Saturn, where disruptive tidal forces are stronger than the gravitational forces attracting the ring particles to each other Each of Saturn’s major rings is composed of a great many narrow ringlets

Saturn’s rings consist of thousands of narrow, closely spaced ringlets

Saturn’s inner satellites affect the appearance and structure of its rings

Outline Jupiter and Saturn –Orbit –Surface –Atmosphere –Rings –Moons

Preview Already discussed influence on Saturn’s rings. Jupiter’s moons are even more interesting