Lecture 14 Outline For Rest of Semester Oct. 29 th Chapter 9 (Earth) Nov 3 rd and 5 th Chapter 9 and...

58

Transcript of Lecture 14 Outline For Rest of Semester Oct. 29 th Chapter 9 (Earth) Nov 3 rd and 5 th Chapter 9 and...

Page 1: Lecture 14 Outline For Rest of Semester Oct. 29 th Chapter 9 (Earth) Nov 3 rd and 5 th Chapter 9 and Chapter 10 (Earth and Moon) Nov. 10 th and 12.
Page 2: Lecture 14 Outline For Rest of Semester Oct. 29 th Chapter 9 (Earth) Nov 3 rd and 5 th Chapter 9 and Chapter 10 (Earth and Moon) Nov. 10 th and 12.

Lecture 14

Page 3: Lecture 14 Outline For Rest of Semester Oct. 29 th Chapter 9 (Earth) Nov 3 rd and 5 th Chapter 9 and Chapter 10 (Earth and Moon) Nov. 10 th and 12.
Page 4: Lecture 14 Outline For Rest of Semester Oct. 29 th Chapter 9 (Earth) Nov 3 rd and 5 th Chapter 9 and Chapter 10 (Earth and Moon) Nov. 10 th and 12.

Outline For Rest of Semester• Oct. 29th Chapter 9 (Earth)• Nov 3rd and 5th Chapter 9 and Chapter 10 (Earth and Moon)• Nov. 10th and 12th Mars, Venus, and Mercury• Nov. 17th and 19th Jupiter and Saturn• Nov 24th Uranus and Neptune• Nov 26th Thanksgiving• Dec. 1st - Exam 3• Dec. 3rd – Pluto, and the Kuiper Belt• Dec. 8th and 10th – Chapter 7 and 8 (Comparative Planetology I and II)• Tuesday December 15th (7:30 am – 10:15 am) Final Exam• No Reading days are scheduled this semester. (Exam Period begins at

7:30 a.m. on Monday, December 14 and ends on December 21)

Page 5: Lecture 14 Outline For Rest of Semester Oct. 29 th Chapter 9 (Earth) Nov 3 rd and 5 th Chapter 9 and Chapter 10 (Earth and Moon) Nov. 10 th and 12.

Outline

• Quiz discussion• Review question• Neptune and Uranus

Page 6: Lecture 14 Outline For Rest of Semester Oct. 29 th Chapter 9 (Earth) Nov 3 rd and 5 th Chapter 9 and Chapter 10 (Earth and Moon) Nov. 10 th and 12.

Roche limit

Some of the small shepherd satellites within Saturn's ring system are also inside Saturn's Roche Limit. Why are they not torn apart by tidal forces due to Saturn's gravity?

1. The Roche Limit applies only to the ring particles, not to anything as large as a satellite2. The interaction between Saturn's strong magnetic field and the magnetic fields generated by the shepherd satellites helps to hold the satellites together.3. The Roche Limit only applies to objects held together by mutual gravitational attraction, not to chunks of rock like the shepherd satellites.4. Unlike the ring particles, the satellites are large enough to produce significant gravitational fields of their own, and these counteract the tidal forces.

Page 7: Lecture 14 Outline For Rest of Semester Oct. 29 th Chapter 9 (Earth) Nov 3 rd and 5 th Chapter 9 and Chapter 10 (Earth and Moon) Nov. 10 th and 12.

Opposition

Which planet will appear more often at opposition, Jupiter or Saturn?

1. Same2. Jupiter3. Saturn

Page 8: Lecture 14 Outline For Rest of Semester Oct. 29 th Chapter 9 (Earth) Nov 3 rd and 5 th Chapter 9 and Chapter 10 (Earth and Moon) Nov. 10 th and 12.

In-class quiz

• 15 quiz points for any answer

• Triple points if all answers today correct

Page 9: Lecture 14 Outline For Rest of Semester Oct. 29 th Chapter 9 (Earth) Nov 3 rd and 5 th Chapter 9 and Chapter 10 (Earth and Moon) Nov. 10 th and 12.

Earth, Moon, Sun, Venus, and Mars

Page 10: Lecture 14 Outline For Rest of Semester Oct. 29 th Chapter 9 (Earth) Nov 3 rd and 5 th Chapter 9 and Chapter 10 (Earth and Moon) Nov. 10 th and 12.

Register for quiz 3

Text to 41411:

astr111 3 rweigel

You will receive either one or two texts in response

Replace with your GMU email name

Page 11: Lecture 14 Outline For Rest of Semester Oct. 29 th Chapter 9 (Earth) Nov 3 rd and 5 th Chapter 9 and Chapter 10 (Earth and Moon) Nov. 10 th and 12.

Register for quiz 3

Text to 41411:

astr111 3 rweigel-jsmith1-hjones7

You will receive either one or two texts in response

Separate group member names with hyphen

Late students may not work in group

Page 12: Lecture 14 Outline For Rest of Semester Oct. 29 th Chapter 9 (Earth) Nov 3 rd and 5 th Chapter 9 and Chapter 10 (Earth and Moon) Nov. 10 th and 12.

3 1 a

3 1 b 3 1 c

3 1 d

If you think the black dots best represent configuration in photo, text 3 1 d

Which case, blue, red, green, or black, best represents the configuration in the photo?

Page 13: Lecture 14 Outline For Rest of Semester Oct. 29 th Chapter 9 (Earth) Nov 3 rd and 5 th Chapter 9 and Chapter 10 (Earth and Moon) Nov. 10 th and 12.

3 1 a

3 1 b 3 1 c

3 1 d

If you think the black dots best represent configuration in photo, text 3 1 d

Which case, blue, red, green, or black, best represents the configuration in the photo?

Page 14: Lecture 14 Outline For Rest of Semester Oct. 29 th Chapter 9 (Earth) Nov 3 rd and 5 th Chapter 9 and Chapter 10 (Earth and Moon) Nov. 10 th and 12.

3 2 b

3 2 a

Where is the best placement of moon?

3 2 c

3 2 d

Page 15: Lecture 14 Outline For Rest of Semester Oct. 29 th Chapter 9 (Earth) Nov 3 rd and 5 th Chapter 9 and Chapter 10 (Earth and Moon) Nov. 10 th and 12.

b

ac

d

Page 16: Lecture 14 Outline For Rest of Semester Oct. 29 th Chapter 9 (Earth) Nov 3 rd and 5 th Chapter 9 and Chapter 10 (Earth and Moon) Nov. 10 th and 12.

Suggested Reading

• Chapters on Uranus and Neptune

Page 17: Lecture 14 Outline For Rest of Semester Oct. 29 th Chapter 9 (Earth) Nov 3 rd and 5 th Chapter 9 and Chapter 10 (Earth and Moon) Nov. 10 th and 12.

Neptune and Uranus

Page 18: Lecture 14 Outline For Rest of Semester Oct. 29 th Chapter 9 (Earth) Nov 3 rd and 5 th Chapter 9 and Chapter 10 (Earth and Moon) Nov. 10 th and 12.

Doubling the Solar System

Page 19: Lecture 14 Outline For Rest of Semester Oct. 29 th Chapter 9 (Earth) Nov 3 rd and 5 th Chapter 9 and Chapter 10 (Earth and Moon) Nov. 10 th and 12.

• How can you tell the difference between a planet and a distant star? (assume the both span the same angular distance)

a. Planet always moves in retrograde

b. Star always appears at same position in sky

c. Star position repeats after one year, planet does not

d. Planet position repeats after on year, star does not

3 3

3 3

3 3

3 3

Page 20: Lecture 14 Outline For Rest of Semester Oct. 29 th Chapter 9 (Earth) Nov 3 rd and 5 th Chapter 9 and Chapter 10 (Earth and Moon) Nov. 10 th and 12.

Uranus

• Hershel “discovered” it

A Short History of Nearly EverythingBy Bill Bryson (Travel Writer and Humorist)

Page 21: Lecture 14 Outline For Rest of Semester Oct. 29 th Chapter 9 (Earth) Nov 3 rd and 5 th Chapter 9 and Chapter 10 (Earth and Moon) Nov. 10 th and 12.

Neptune’s discovery

• A triumph of modern science

+ =

Page 22: Lecture 14 Outline For Rest of Semester Oct. 29 th Chapter 9 (Earth) Nov 3 rd and 5 th Chapter 9 and Chapter 10 (Earth and Moon) Nov. 10 th and 12.

The Pioneer anomaly

• Is history repeating itself?

Pioneer plaque

Page 23: Lecture 14 Outline For Rest of Semester Oct. 29 th Chapter 9 (Earth) Nov 3 rd and 5 th Chapter 9 and Chapter 10 (Earth and Moon) Nov. 10 th and 12.

http://www.guardian.co.uk/science/2004/sep/12/spaceexploration.research

• Some researchers say unseen 'dark matter' may permeate the universe and that this is affecting the Pioneers' passage. Others say flaws in our understanding of the laws of gravity best explain the crafts' wayward behaviour.

• As a result, scientists are to press a European Space Agency (Esa) meeting, called Cosmic Visions, in Paris this week for backing for a mission that would follow the Pioneers and pinpoint the cause of their erratic movements.

Page 24: Lecture 14 Outline For Rest of Semester Oct. 29 th Chapter 9 (Earth) Nov 3 rd and 5 th Chapter 9 and Chapter 10 (Earth and Moon) Nov. 10 th and 12.

• The reasons for the anomaly have caused a rift among physicists, … 'Unless there is really good evidence to the contrary, we should stick to simple ideas like these and not go around blaming strange new types of particle or flaws in general relativity,' said Professor Martin Barstow, of Leicester University.

• One proposal put forward is that Newton's idea that the force of gravity weakens as distance increases may be incorrect over very large spaces, and may drop off over very long distances.

Page 25: Lecture 14 Outline For Rest of Semester Oct. 29 th Chapter 9 (Earth) Nov 3 rd and 5 th Chapter 9 and Chapter 10 (Earth and Moon) Nov. 10 th and 12.

Neptune• Galileo missed it – noted something that

star seemed to have moved in relation to other stars.

Yo-hooOver here

Page 26: Lecture 14 Outline For Rest of Semester Oct. 29 th Chapter 9 (Earth) Nov 3 rd and 5 th Chapter 9 and Chapter 10 (Earth and Moon) Nov. 10 th and 12.

Neptune’s orbit

• Uranus is at about 20 AU and Neptune is at about 30 AU. The ratio is 3:2. Does this mean anything?

Page 27: Lecture 14 Outline For Rest of Semester Oct. 29 th Chapter 9 (Earth) Nov 3 rd and 5 th Chapter 9 and Chapter 10 (Earth and Moon) Nov. 10 th and 12.

Neptune’s orbit

• Uranus is at about 20 AU and Neptune is at about 30 AU. The ratio is 3:2. Does this mean anything?

• Saturn’s orbit is 9.5 AU, Jupiter’s orbit is at 5.2 AU.

• Mercury is at 0.38 AU, Venus is at 0.73 AU, Earth is at 1 AU, Mars is at 1.5 AU.

Page 28: Lecture 14 Outline For Rest of Semester Oct. 29 th Chapter 9 (Earth) Nov 3 rd and 5 th Chapter 9 and Chapter 10 (Earth and Moon) Nov. 10 th and 12.
Page 29: Lecture 14 Outline For Rest of Semester Oct. 29 th Chapter 9 (Earth) Nov 3 rd and 5 th Chapter 9 and Chapter 10 (Earth and Moon) Nov. 10 th and 12.
Page 30: Lecture 14 Outline For Rest of Semester Oct. 29 th Chapter 9 (Earth) Nov 3 rd and 5 th Chapter 9 and Chapter 10 (Earth and Moon) Nov. 10 th and 12.

Atmosphere

Page 31: Lecture 14 Outline For Rest of Semester Oct. 29 th Chapter 9 (Earth) Nov 3 rd and 5 th Chapter 9 and Chapter 10 (Earth and Moon) Nov. 10 th and 12.

• Both Uranus and Neptune have atmospheres composed primarily of hydrogen, helium, and a few percent methane

• What colors does methane absorb?

Page 32: Lecture 14 Outline For Rest of Semester Oct. 29 th Chapter 9 (Earth) Nov 3 rd and 5 th Chapter 9 and Chapter 10 (Earth and Moon) Nov. 10 th and 12.

• What colors does methane absorb?

• Methane is a greenhouse gas

• Greenhouse gasses tend to absorb long wavelength photons, which Earth’s surface emits

• Is the color of Uranus consistent with this?

Page 33: Lecture 14 Outline For Rest of Semester Oct. 29 th Chapter 9 (Earth) Nov 3 rd and 5 th Chapter 9 and Chapter 10 (Earth and Moon) Nov. 10 th and 12.

• Methane is a greenhouse gas• Greenhouse gasses tend to absorb long

wavelength photons, which Earth’s surface emits• Is the color of Uranus consistent with this?

–Red has long wavelength, blue short.

–So methane absorbing long wavelength photons is consistent with it being a greenhouse gas

Page 34: Lecture 14 Outline For Rest of Semester Oct. 29 th Chapter 9 (Earth) Nov 3 rd and 5 th Chapter 9 and Chapter 10 (Earth and Moon) Nov. 10 th and 12.

Bizarro tilt on Uranus

Page 35: Lecture 14 Outline For Rest of Semester Oct. 29 th Chapter 9 (Earth) Nov 3 rd and 5 th Chapter 9 and Chapter 10 (Earth and Moon) Nov. 10 th and 12.

Exaggerated Seasons On Uranus

• Uranus’s axis of rotation lies nearly in the plane of its orbit, producing greatly exaggerated seasonal changes on the planet

• This unusual orientation may be the result of a collision with a planetlike object early in the history of our solar system. Such a collision could have knocked Uranus on its side

Page 36: Lecture 14 Outline For Rest of Semester Oct. 29 th Chapter 9 (Earth) Nov 3 rd and 5 th Chapter 9 and Chapter 10 (Earth and Moon) Nov. 10 th and 12.
Page 37: Lecture 14 Outline For Rest of Semester Oct. 29 th Chapter 9 (Earth) Nov 3 rd and 5 th Chapter 9 and Chapter 10 (Earth and Moon) Nov. 10 th and 12.

• Which would you guess has a more active atmosphere?– Based on distance from Sun– Based on above pictures

Page 38: Lecture 14 Outline For Rest of Semester Oct. 29 th Chapter 9 (Earth) Nov 3 rd and 5 th Chapter 9 and Chapter 10 (Earth and Moon) Nov. 10 th and 12.

• Neptune looks more active• But its orbit is 30 AU compared to 20 AU

for Uranus. What is the difference between amount of energy they receive?

Page 39: Lecture 14 Outline For Rest of Semester Oct. 29 th Chapter 9 (Earth) Nov 3 rd and 5 th Chapter 9 and Chapter 10 (Earth and Moon) Nov. 10 th and 12.

• “Thanks to distance, Neptune receives less than one-half of the amount of solar energy than Uranus.”

• Where did the “one-half” number come from?

Page 40: Lecture 14 Outline For Rest of Semester Oct. 29 th Chapter 9 (Earth) Nov 3 rd and 5 th Chapter 9 and Chapter 10 (Earth and Moon) Nov. 10 th and 12.

• “Thanks to distance, Neptune receives less than one-half of the amount of solar energy than Uranus.”

• Where did the “one-half” number come from?

– Energy Flux ~ 1/r2

– Energy Flux Uranus ~ 1/202 = 1/400– Energy Flux Neptune ~ 1/302 = 1/900– Ratio is 400/900, which is a little less than 0.5

Page 41: Lecture 14 Outline For Rest of Semester Oct. 29 th Chapter 9 (Earth) Nov 3 rd and 5 th Chapter 9 and Chapter 10 (Earth and Moon) Nov. 10 th and 12.

Interior

Page 42: Lecture 14 Outline For Rest of Semester Oct. 29 th Chapter 9 (Earth) Nov 3 rd and 5 th Chapter 9 and Chapter 10 (Earth and Moon) Nov. 10 th and 12.

Uranus and Neptune contain a higher proportionof heavy elements than Jupiter and Saturn

• Both Uranus and Neptune may have a rocky core surrounded by a mantle of water and ammonia

• Electric currents in the mantles may generate the magnetic fields of the planets

Page 43: Lecture 14 Outline For Rest of Semester Oct. 29 th Chapter 9 (Earth) Nov 3 rd and 5 th Chapter 9 and Chapter 10 (Earth and Moon) Nov. 10 th and 12.

They should not exist

Page 44: Lecture 14 Outline For Rest of Semester Oct. 29 th Chapter 9 (Earth) Nov 3 rd and 5 th Chapter 9 and Chapter 10 (Earth and Moon) Nov. 10 th and 12.

Bizarro Magnetic Axis

The magnetic fields of both Uranus and Neptuneare oriented at unusual angles

Page 45: Lecture 14 Outline For Rest of Semester Oct. 29 th Chapter 9 (Earth) Nov 3 rd and 5 th Chapter 9 and Chapter 10 (Earth and Moon) Nov. 10 th and 12.

• 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

Page 46: Lecture 14 Outline For Rest of Semester Oct. 29 th Chapter 9 (Earth) Nov 3 rd and 5 th Chapter 9 and Chapter 10 (Earth and Moon) Nov. 10 th and 12.

Moons and Rings

• un14vi03.mov

Movie 16.3

Page 47: Lecture 14 Outline For Rest of Semester Oct. 29 th Chapter 9 (Earth) Nov 3 rd and 5 th Chapter 9 and Chapter 10 (Earth and Moon) Nov. 10 th and 12.

Uranus and Neptune each have a system of thin, dark rings

Movie 16.3

Page 48: Lecture 14 Outline For Rest of Semester Oct. 29 th Chapter 9 (Earth) Nov 3 rd and 5 th Chapter 9 and Chapter 10 (Earth and Moon) Nov. 10 th and 12.

Discovery of Uranian Rings

Page 49: Lecture 14 Outline For Rest of Semester Oct. 29 th Chapter 9 (Earth) Nov 3 rd and 5 th Chapter 9 and Chapter 10 (Earth and Moon) Nov. 10 th and 12.

Movie

1403002.swf

Movie 16.2

Page 50: Lecture 14 Outline For Rest of Semester Oct. 29 th Chapter 9 (Earth) Nov 3 rd and 5 th Chapter 9 and Chapter 10 (Earth and Moon) Nov. 10 th and 12.
Page 51: Lecture 14 Outline For Rest of Semester Oct. 29 th Chapter 9 (Earth) Nov 3 rd and 5 th Chapter 9 and Chapter 10 (Earth and Moon) Nov. 10 th and 12.

Some of Uranus’s satellites show evidence of past tidal heating

Uranus has five satellites similar to the moderate-sized moons of Saturn, plus at least 22 more small satellites

Page 52: Lecture 14 Outline For Rest of Semester Oct. 29 th Chapter 9 (Earth) Nov 3 rd and 5 th Chapter 9 and Chapter 10 (Earth and Moon) Nov. 10 th and 12.

• Heavily cratered• Dramatic

topography• Unfinished tidal

heating?

Page 53: Lecture 14 Outline For Rest of Semester Oct. 29 th Chapter 9 (Earth) Nov 3 rd and 5 th Chapter 9 and Chapter 10 (Earth and Moon) Nov. 10 th and 12.
Page 54: Lecture 14 Outline For Rest of Semester Oct. 29 th Chapter 9 (Earth) Nov 3 rd and 5 th Chapter 9 and Chapter 10 (Earth and Moon) Nov. 10 th and 12.

Triton is a frigid, icy world with a young surface and a tenuous atmosphere

• Neptune has 13 satellites, one of which (Triton) is comparable in size to our Moon or the Galilean satellites of Jupiter

• Triton has a young, icy surface indicative of tectonic activity

• The energy for this activity may have been provided by tidal heating that occurred when Triton was captured by Neptune’s gravity into a retrograde orbit

• Triton has a tenuous nitrogen atmosphere

Page 55: Lecture 14 Outline For Rest of Semester Oct. 29 th Chapter 9 (Earth) Nov 3 rd and 5 th Chapter 9 and Chapter 10 (Earth and Moon) Nov. 10 th and 12.

 Neptune was

a. predicted to exist through its gravitational effect on Uranus

b. discovered in ancient times because it is a naked-eye object.

c. found by accident during a search for comets.

d. predicted to exist through its gravitational effect on Saturn.

e. was discovered using a radio telescope.

3 4

3 4

3 4

3 4

3 4

Page 56: Lecture 14 Outline For Rest of Semester Oct. 29 th Chapter 9 (Earth) Nov 3 rd and 5 th Chapter 9 and Chapter 10 (Earth and Moon) Nov. 10 th and 12.

 Neptune was

a. predicted to exist through its gravitational effect on Uranus

b. discovered in ancient times because it is a naked-eye object.

c. found by accident during a search for comets.

d. predicted to exist through its gravitational effect on Saturn.

e. was discovered using a radio telescope.

3 4

3 4

3 4

3 4

3 4

Page 57: Lecture 14 Outline For Rest of Semester Oct. 29 th Chapter 9 (Earth) Nov 3 rd and 5 th Chapter 9 and Chapter 10 (Earth and Moon) Nov. 10 th and 12.

Which of the following statements correctly describes a currently proposed picture for the formation of Uranus and Neptune?

a. Uranus and Neptune formed where they are now with the mass and composition we see today.

b. Uranus and Neptune formed farther from the Sun than they are now and gradually spiraled inward to their present orbits.

c. Uranus and Neptune formed closer to the Sun than they are now and were pushed outward to their present orbits.

d. Uranus is a result of the collision of a Mars-sized object with Neptune.

3 5

3 5

3 5

3 5

Page 58: Lecture 14 Outline For Rest of Semester Oct. 29 th Chapter 9 (Earth) Nov 3 rd and 5 th Chapter 9 and Chapter 10 (Earth and Moon) Nov. 10 th and 12.

We know that Neptune contains a larger amount of heavier elements than Saturn. We know this because Neptune

a. is smaller than Saturn

b. has a higher density than Saturn

c. is farther from the Sun than Saturn

d. has a lower density than Saturn

e. is larger than Saturn.

3 6

3 63 6

3 6

3 6