The Atmospheres of the Outer Jovian Worlds Enormous

Saturn North Pole(Hexagonal Storm) Copyright © 2010 Pearson Education, Inc.

The Atmospheres of the Outer Jovian Worlds Rotation of Uranus can be measured by

The Atmospheres of the Outer Jovian Worlds Neptune has storm systems similar to those

Jovian Interiors No direct information is available about Jupiter’s interior, but its main components,

Jovian Interiors Uranus and Neptune both have substantial magnetic fields, but at a large

Jovian Interiors Jupiter’s magnetosphere: Intrinsic field strength is 20, 000 times that of Earth.

Jovian Interiors Magnetic fields of Uranus and Neptune must not be produced by dynamos,

Jovian Interiors Aurorae are seen on Jupiter, and have the same cause as those

Question 1 Both Jupiter and Saturn Copyright © 2010 Pearson Education, Inc. a) b)

Question 2 Jovian planets share all of the following traits EXCEPT Copyright © 2010

Question 2 Jovian planets share all of the following traits EXCEPT a) a low-density

Question 3 Jupiter and the other jovian planets are noticeably oblate because they have

Question 4 What is the probable source of the variations in Jupiter’s belts and

Question 5 What is the source of Jupiter’s large magnetic field? Copyright © 2010

Question 8 Which of these is TRUE about the seasons on Uranus? Copyright ©

Question 7 The two outer jovian planets appear bluish in color because Copyright ©

Question 9 The magnetic fields of which two planets are most unusual? Copyright ©

Question 9 The magnetic fields of which two planets are most unusual? a) Jupiter

Slides: 26

Download presentation

The Atmospheres of the Outer Jovian Worlds Neptune has storm systems similar to those on Jupiter, but fewer. The large storm system at top has disappeared in recent years. Copyright © 2010 Pearson Education, Inc.

Jovian Interiors No direct information is available about Jupiter’s interior, but its main components, hydrogen and helium, are quite well understood. The central portion is thought to be a rocky core. Copyright © 2010 Pearson Education, Inc.

Jovian Interiors Uranus and Neptune both have substantial magnetic fields, but at a large angle to their rotation axes. The rectangle within each planet shows a bar magnet that would produce a similar field. Note that both Uranus’s and Neptune’s are significantly off center. Copyright © 2010 Pearson Education, Inc.

Jovian Interiors Magnetic fields of Uranus and Neptune must not be produced by dynamos, as the other planets’ fields are. Interior structure of Uranus and Neptune, compared to that of Jupiter and Saturn: Copyright © 2010 Pearson Education, Inc.

Question 1 Both Jupiter and Saturn Copyright © 2010 Pearson Education, Inc. a) b) c) d) e) have liquid metallic hydrogen in their interiors. have rings. emit more energy than they absorb from the Sun. rotate very rapidly. All of the above.

Question 2 Jovian planets share all of the following traits EXCEPT Copyright © 2010 Pearson Education, Inc. a) a low-density gaseous core. b) large magnetic fields. c) lots of hydrogen & helium gas. d) many moons. e) differential rotation.

Question 2 Jovian planets share all of the following traits EXCEPT a) a low-density gaseous core. b) large magnetic fields. c) lots of hydrogen & helium gas. d) many moons. e) differential rotation. All of the jovian planets have dense, compact cores more massive than Earth, surrounded by liquid and gaseous layers. Copyright © 2010 Pearson Education, Inc.

Question 3 Jupiter and the other jovian planets are noticeably oblate because they have Copyright © 2010 Pearson Education, Inc. a) very strong magnetic fields. b) powerful gravity pulling on the poles. c) rapid rotation and a fluid interior. d) many moons that tidally distort their shapes. e) All of the above.

Question 3 Jupiter and the other jovian planets are noticeably oblate because they have a) very strong magnetic fields. b) powerful gravity pulling on the poles. c) rapid rotation and a fluid interior. d) many moons that tidally distort their shapes. e) All of the above. All of the jovian planets are larger than Earth, all spin faster, all have lower density, and all show a flattened, “oblate” shape. Copyright © 2010 Pearson Education, Inc.

Question 4 What is the probable source of the variations in Jupiter’s belts and zones? Copyright © 2010 Pearson Education, Inc. a) convection of ammonia ice upward b) differential rotation and underlying zonal flow c) oblateness due to low density d) thermonuclear fusion e) Jupiter’s huge magnetosphere

Question 5 What is the source of Jupiter’s large magnetic field? Copyright © 2010 Pearson Education, Inc. a) charged particles moving in the atmosphere b) thermonuclear fusion in Jupiter’s core c) the gravitational attraction of Jupiter’s many large moons d) the Great Red Spot e) metallic hydrogen swirling in its interior

Question 8 Which of these is TRUE about the seasons on Uranus? Copyright © 2010 Pearson Education, Inc. a) Its strange tilt produces extreme seasonal variations. b) With its tilt of 29°, Uranus has four seasons similar to those on Earth. c) It never shows any weather in its bland clouds. d) It spins so fast all seasons are the same.

Question 7 The two outer jovian planets appear bluish in color because Copyright © 2010 Pearson Education, Inc. a) gaseous ammonia in their atmospheres absorbs blue light. b) methane absorbs red light. c) cold hydrogen reflects blue light. d) dust in their atmospheres scatters blue light, similar to Earth.

Question 9 The magnetic fields of which two planets are most unusual? Copyright © 2010 Pearson Education, Inc. a) Jupiter and Neptune b) Jupiter and Saturn c) Jupiter and Earth d) Saturn and Earth e) Uranus and Neptune

Question 9 The magnetic fields of which two planets are most unusual? a) Jupiter and Neptune b) Jupiter and Saturn c) Jupiter and Earth d) Saturn and Earth e) Uranus and Neptune Both Uranus and Neptune have fields that are off-center, and very inclined to their rotation axes. Copyright © 2010 Pearson Education, Inc.