40
Chapter 7 : Mentos

Chapter 7 : Mentos

  • Upload
    vondra

  • View
    66

  • Download
    2

Embed Size (px)

DESCRIPTION

Chapter 7 : Mentos. Chapter 7 The Jovian Planets. Units of Chapter 7. Observations of Jupiter and Saturn The Discoveries of Uranus and Neptune Bulk Properties of the Jovian Planets Jupiter’s Atmosphere The Atmospheres of the Outer Jovian Worlds Jovian Interiors Summary of Chapter 7. - PowerPoint PPT Presentation

Citation preview

Page 1: Chapter 7 :  Mentos

Chapter 7 : Mentos

Page 2: Chapter 7 :  Mentos

Chapter 7 The Jovian Planets

Page 3: Chapter 7 :  Mentos

Observations of Jupiter and SaturnThe Discoveries of Uranus and NeptuneBulk Properties of the Jovian PlanetsJupiter’s AtmosphereThe Atmospheres of the Outer Jovian WorldsJovian InteriorsSummary of Chapter 7

Units of Chapter 7

Page 4: Chapter 7 :  Mentos

Jupiter can be imaged well from Earth, even with a small telescope.Here: Jupiter with its Galilean moons

7.1 Observations of Jupiter and Saturn

Page 5: Chapter 7 :  Mentos

True-color image of Jupiter

Page 6: Chapter 7 :  Mentos

Natural-color image of Saturn

Page 7: Chapter 7 :  Mentos

Cassini image of Jupiter, true color

Page 8: Chapter 7 :  Mentos

Uranus, in natural color. Note the absence of features.

7.2 The Discoveries of Uranus and Neptune

Page 9: Chapter 7 :  Mentos

Neptune in natural color

Page 10: Chapter 7 :  Mentos

The Jovian planets are large and much less dense than the terrestrial planets; Saturn is less dense than water!

7.3 Bulk Properties of the Jovian Planets

Page 11: Chapter 7 :  Mentos

Jovian planets, compared to Earth

Page 12: Chapter 7 :  Mentos

Peculiarity of Uranus: Axis of rotation lies almost in the plane of its orbit. Seasonal variations are extreme.

Page 13: Chapter 7 :  Mentos

Atmosphere has bright zones and dark belts.Zones are cooler, and are higher than belts.Stable flow underlies zones and bands, called zonal flow.Simplified model:

7.4 Jupiter’s Atmosphere

Page 14: Chapter 7 :  Mentos

No solid surface; take top of troposphere to be 0 km.Lowest cloud layer cannot be seen by optical telescopes.Measurements by Galileo probe show high wind speeds even at great depth – probably due to heating from planet, not from Sun.

Page 15: Chapter 7 :  Mentos

The Galileo probe descended into Jupiter’s atmosphere and returned valuable data. The arrow indicates its entry point.

Page 16: Chapter 7 :  Mentos

Major visible features:Bands of clouds; Great Red Spot

Page 17: Chapter 7 :  Mentos

Two examples of smaller storms merging, first into a smaller red spot, second into existing Great Red Spot

Page 18: Chapter 7 :  Mentos

The atmosphere of Saturn is similar to that of Jupiter, except that Saturn is somewhat colder and its atmosphere is thicker.

7.5 The Atmospheres of the Outer Jovian Worlds

Page 19: Chapter 7 :  Mentos

Saturn’s atmosphere is similar to Jupiter’s, except pressure is lower.It has three cloud layers.Cloud layers are thicker than Jupiter’s; see only top layer.

Page 20: Chapter 7 :  Mentos

Saturn also has large storms, and bands.

Page 21: Chapter 7 :  Mentos

Storms near Saturn’s equator

Page 22: Chapter 7 :  Mentos

Enormous thunderstorm on Saturn

Page 23: Chapter 7 :  Mentos

Rotation of Uranus can be measured by watching storms.

Page 24: Chapter 7 :  Mentos

Neptune has storm systems similar to those on Jupiter, but fewer. The large storm system at top has disappeared in recent years.

Page 25: Chapter 7 :  Mentos

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.

7.6 Jovian Interiors

Page 26: Chapter 7 :  Mentos

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:

Page 27: Chapter 7 :  Mentos

Jupiter’s magnetosphere:Intrinsic field strength is 20,000 times that of Earth.Magnetosphere can extend beyond the orbit of Saturn.

Page 28: Chapter 7 :  Mentos

Aurorae are seen on Jupiter, and have the same cause as those on Earth – the interaction of solar wind particles with the magnetosphere.

Page 29: Chapter 7 :  Mentos

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.

Page 30: Chapter 7 :  Mentos

How do we know what the internal structures of the Jovian planets are like?A. Probes have been sent into the

interiors of the planets and have returned data about the conditions.

B. Astronomers use the Earth's internal structure as a basis of comparison.

C. Astronomers examine the composition of the satellites of these planets.

D. Astronomers use information about the physical characteristics as well as laws of physics to obtain theoretical models.

Page 31: Chapter 7 :  Mentos

Which of the following statements is FALSE?A. Interior heating in the Jovian planets

contribute to convection in the atmospheres.

B. Slow rotation rates lead to very strong coriolis forces.

C. The circulation patterns tend to be in very elongated bands that encircle the planets.

D. The circulation speeds increase towards the equator.

Page 32: Chapter 7 :  Mentos

Near the core of Jupiter, hydrogen isA. a low temperature gas.B. a high temperature gas.C. a solid.D. a liquid.E. a liquid metal.

Page 33: Chapter 7 :  Mentos

The great red spot of Jupiter is thought to be

A. caused by an enormous volcano.B. a region of hotter gases.C. a long-lasting cyclonic storm.D. an opening through the high level

clouds revealing a portion of the atmosphere nearer the surface. 

Page 34: Chapter 7 :  Mentos

Which of the following are true about Jupiter's belts (dark) and zones(light)

A. belts are rising while zones are sinking.

B. belts are sinking while zones are rising.

C. both belts and zones are rising.D. both belts and zones are sinking. 

Page 35: Chapter 7 :  Mentos

Jupiter's magnetic field probably originates

A. in the liquid metallic hydrogen region.

B. from the solar wind.C. in the vicinity of Io.D. from the motion of the

Galilean satellites.

Page 36: Chapter 7 :  Mentos

Compared to Earth, the expected seasonal changes on Uranus because of its orbital and spin-axis alignments will be

A. much less.B. very much exaggerated.C. absent, because of the alignment

of the spin axis.D. the same .

Page 37: Chapter 7 :  Mentos

From the results of the voyager 2 mission of Uranus, we now know that the

A. planet has fewer rings than expected.

B. magnetic field has a large tilt to the spin axis.

C. larger moons have smooth surfaces and little evolution.

D. rings are made of objects hundreds of meters in radius. 

Page 38: Chapter 7 :  Mentos

Since Uranus has a higher average density than Saturn

A. it must rotate faster.B. it must have much more rocky

material.C. it must have a stronger magnetic

field.D. it must have a higher concentration

of icy materials.

Page 39: Chapter 7 :  Mentos

Summary of Chapter 7• Jupiter and Saturn were known to the ancients; Uranus was discovered by chance, and Neptune was predicted from anomalies in the orbit of Uranus.• Jovian planets are large but not dense; they are fluid and display differential rotation.• Cloud layers have light zones and dark bands; wind pattern, called zonal flow, is stable.

Page 40: Chapter 7 :  Mentos

Summary of Chapter 7, cont.• Storms appear with regularity; the Great Red Spot of Jupiter has lasted for hundreds of years (that we know of).• Due to conductive interiors and rapid rotation, Jovian planets have large magnetic fields.• Jupiter, Saturn, and Neptune radiate more energy than they receive from the Sun.