40
LECTURE 12, OCTOBER 5, 2010 ASTR 101, SECTION 3 INSTRUCTOR, JACK BRANDT [email protected] 1 ASTR 101-3, FALL 2010

LECTURE 12, OCTOBER 5, 2010 ASTR 101, SECTION 3 INSTRUCTOR, JACK BRANDT [email protected] 1ASTR 101-3, FALL 2010

Embed Size (px)

Citation preview

Page 1: LECTURE 12, OCTOBER 5, 2010 ASTR 101, SECTION 3 INSTRUCTOR, JACK BRANDT jcbrandt@unm.edu 1ASTR 101-3, FALL 2010

ASTR 101-3, FALL 2010 1

LECTURE 12, OCTOBER 5, 2010

ASTR 101, SECTION 3INSTRUCTOR, JACK BRANDT

[email protected]

Page 2: LECTURE 12, OCTOBER 5, 2010 ASTR 101, SECTION 3 INSTRUCTOR, JACK BRANDT jcbrandt@unm.edu 1ASTR 101-3, FALL 2010

ASTR 101-3, FALL 2010 2

Page 3: LECTURE 12, OCTOBER 5, 2010 ASTR 101, SECTION 3 INSTRUCTOR, JACK BRANDT jcbrandt@unm.edu 1ASTR 101-3, FALL 2010

ASTR 101-3, FALL 2010 3

Page 4: LECTURE 12, OCTOBER 5, 2010 ASTR 101, SECTION 3 INSTRUCTOR, JACK BRANDT jcbrandt@unm.edu 1ASTR 101-3, FALL 2010

ASTR 101-3, FALL 2010 4

Page 5: LECTURE 12, OCTOBER 5, 2010 ASTR 101, SECTION 3 INSTRUCTOR, JACK BRANDT jcbrandt@unm.edu 1ASTR 101-3, FALL 2010

ASTR 101-3, FALL 2010 5

Page 6: LECTURE 12, OCTOBER 5, 2010 ASTR 101, SECTION 3 INSTRUCTOR, JACK BRANDT jcbrandt@unm.edu 1ASTR 101-3, FALL 2010

ASTR 101-3, FALL 2010 6

Page 7: LECTURE 12, OCTOBER 5, 2010 ASTR 101, SECTION 3 INSTRUCTOR, JACK BRANDT jcbrandt@unm.edu 1ASTR 101-3, FALL 2010

ASTR 101-3, FALL 2010 7

Page 8: LECTURE 12, OCTOBER 5, 2010 ASTR 101, SECTION 3 INSTRUCTOR, JACK BRANDT jcbrandt@unm.edu 1ASTR 101-3, FALL 2010

ASTR 101-3, FALL 2010 8

Page 9: LECTURE 12, OCTOBER 5, 2010 ASTR 101, SECTION 3 INSTRUCTOR, JACK BRANDT jcbrandt@unm.edu 1ASTR 101-3, FALL 2010

ASTR 101-3, FALL 2010 9

Page 10: LECTURE 12, OCTOBER 5, 2010 ASTR 101, SECTION 3 INSTRUCTOR, JACK BRANDT jcbrandt@unm.edu 1ASTR 101-3, FALL 2010

ASTR 101-3, FALL 2010 10

Page 11: LECTURE 12, OCTOBER 5, 2010 ASTR 101, SECTION 3 INSTRUCTOR, JACK BRANDT jcbrandt@unm.edu 1ASTR 101-3, FALL 2010

The surface of which jovian moon most resembles the pack ice of the Arctic Ocean?

Question 2

a) Europa b) Ioc) Amalthead) Ganymedee) Callisto

Page 12: LECTURE 12, OCTOBER 5, 2010 ASTR 101, SECTION 3 INSTRUCTOR, JACK BRANDT jcbrandt@unm.edu 1ASTR 101-3, FALL 2010

The surface of which jovian moon most resembles the pack ice of the Arctic Ocean?

Question 2

Ice-filled surface cracks

indicate an ocean may lie

below.

a) Europab) Ioc) Amalthead) Ganymedee) Callisto

Page 13: LECTURE 12, OCTOBER 5, 2010 ASTR 101, SECTION 3 INSTRUCTOR, JACK BRANDT jcbrandt@unm.edu 1ASTR 101-3, FALL 2010

What is thought to cause Io’s volcanism?

Question 3

a) Jupiter’s magnetosphereb) Jupiter’s rapid rotationc) tidal stress from Jupiter and Europad) radioactive decay from its coree) Io’s large mass and tectonic activity

Page 14: LECTURE 12, OCTOBER 5, 2010 ASTR 101, SECTION 3 INSTRUCTOR, JACK BRANDT jcbrandt@unm.edu 1ASTR 101-3, FALL 2010

What is thought to cause Io’s volcanism?

Question 3

a) Jupiter’s magnetosphereb) Jupiter’s rapid rotationc) tidal stress from Jupiter and Europad) radioactive decay from its coree) Io’s large mass and tectonic activity

Io is constantly “squeezed” by its huge neighbor as well as by companion

moons, heating its interior.

Page 15: LECTURE 12, OCTOBER 5, 2010 ASTR 101, SECTION 3 INSTRUCTOR, JACK BRANDT jcbrandt@unm.edu 1ASTR 101-3, FALL 2010

ASTR 101-3, FALL 2010 15

Page 16: LECTURE 12, OCTOBER 5, 2010 ASTR 101, SECTION 3 INSTRUCTOR, JACK BRANDT jcbrandt@unm.edu 1ASTR 101-3, FALL 2010

ASTR 101-3, FALL 2010 16

Page 17: LECTURE 12, OCTOBER 5, 2010 ASTR 101, SECTION 3 INSTRUCTOR, JACK BRANDT jcbrandt@unm.edu 1ASTR 101-3, FALL 2010

ASTR 101-3, FALL 2010 17

Page 18: LECTURE 12, OCTOBER 5, 2010 ASTR 101, SECTION 3 INSTRUCTOR, JACK BRANDT jcbrandt@unm.edu 1ASTR 101-3, FALL 2010

ASTR 101-3, FALL 2010 18

Page 19: LECTURE 12, OCTOBER 5, 2010 ASTR 101, SECTION 3 INSTRUCTOR, JACK BRANDT jcbrandt@unm.edu 1ASTR 101-3, FALL 2010

ASTR 101-3, FALL 2010 19

Page 20: LECTURE 12, OCTOBER 5, 2010 ASTR 101, SECTION 3 INSTRUCTOR, JACK BRANDT jcbrandt@unm.edu 1ASTR 101-3, FALL 2010

ASTR 101-3, FALL 2010 20

Page 21: LECTURE 12, OCTOBER 5, 2010 ASTR 101, SECTION 3 INSTRUCTOR, JACK BRANDT jcbrandt@unm.edu 1ASTR 101-3, FALL 2010

ASTR 101-3, FALL 2010 21

Page 22: LECTURE 12, OCTOBER 5, 2010 ASTR 101, SECTION 3 INSTRUCTOR, JACK BRANDT jcbrandt@unm.edu 1ASTR 101-3, FALL 2010

Question 8

a) our Moonb) Phobosc) Europad) Titane) Triton

Which moon in the solar system shows a dense atmosphere?

Page 23: LECTURE 12, OCTOBER 5, 2010 ASTR 101, SECTION 3 INSTRUCTOR, JACK BRANDT jcbrandt@unm.edu 1ASTR 101-3, FALL 2010

Question 8

a) our Moonb) Phobosc) Europad) Titane) Triton

Which moon in the solar system shows a dense atmosphere?

The Huygens probe, deployed by the Cassini spacecraft in 2005, showed that

Titan’s atmosphere has a complex organic chemistry.

Page 24: LECTURE 12, OCTOBER 5, 2010 ASTR 101, SECTION 3 INSTRUCTOR, JACK BRANDT jcbrandt@unm.edu 1ASTR 101-3, FALL 2010

ASTR 101-3, FALL 2010 24

Page 25: LECTURE 12, OCTOBER 5, 2010 ASTR 101, SECTION 3 INSTRUCTOR, JACK BRANDT jcbrandt@unm.edu 1ASTR 101-3, FALL 2010

ASTR 101-3, FALL 2010 25

Page 26: LECTURE 12, OCTOBER 5, 2010 ASTR 101, SECTION 3 INSTRUCTOR, JACK BRANDT jcbrandt@unm.edu 1ASTR 101-3, FALL 2010

ASTR 101-3, FALL 2010 26

Page 27: LECTURE 12, OCTOBER 5, 2010 ASTR 101, SECTION 3 INSTRUCTOR, JACK BRANDT jcbrandt@unm.edu 1ASTR 101-3, FALL 2010

ASTR 101-3, FALL 2010 27

Page 28: LECTURE 12, OCTOBER 5, 2010 ASTR 101, SECTION 3 INSTRUCTOR, JACK BRANDT jcbrandt@unm.edu 1ASTR 101-3, FALL 2010

ASTR 101-3, FALL 2010 28

Page 29: LECTURE 12, OCTOBER 5, 2010 ASTR 101, SECTION 3 INSTRUCTOR, JACK BRANDT jcbrandt@unm.edu 1ASTR 101-3, FALL 2010

ASTR 101-3, FALL 2010 29

Page 30: LECTURE 12, OCTOBER 5, 2010 ASTR 101, SECTION 3 INSTRUCTOR, JACK BRANDT jcbrandt@unm.edu 1ASTR 101-3, FALL 2010

ASTR 101-3, FALL 2010 30

Page 31: LECTURE 12, OCTOBER 5, 2010 ASTR 101, SECTION 3 INSTRUCTOR, JACK BRANDT jcbrandt@unm.edu 1ASTR 101-3, FALL 2010

The Roche limit is defined as the critical

Question 5

a) distance from a planet, inside of which a moon can be tidally destroyed.

b) density that a moon can have and be solid.c) distance from a planet that a moon can experience

synchronous rotation.d) mass a moon can have and still be classified as a

moon.

Page 32: LECTURE 12, OCTOBER 5, 2010 ASTR 101, SECTION 3 INSTRUCTOR, JACK BRANDT jcbrandt@unm.edu 1ASTR 101-3, FALL 2010

The Roche limit is defined as the critical

Question 5

a) distance from a planet, inside of which a moon can be tidally destroyed.

b) density that a moon can have and be solid.c) distance from a planet that a moon can experience

synchronous rotation.d) mass a moon can have and still be classified as a

moon.

Saturn’s rings, as well as those of the other jovian planets, lie within

its planet’s Roche limit.

Page 33: LECTURE 12, OCTOBER 5, 2010 ASTR 101, SECTION 3 INSTRUCTOR, JACK BRANDT jcbrandt@unm.edu 1ASTR 101-3, FALL 2010

Why are the rings of Saturn so bright?

Question 7

a) They are made of frozen metallic hydrogen.b) They contain glassy beads expelled by volcanoes

on Enceladus.c) They contain shiny bits of iron.d) Titan and other moons reflect additional glow onto

the rings. e) They are made of relatively new ice.

Page 34: LECTURE 12, OCTOBER 5, 2010 ASTR 101, SECTION 3 INSTRUCTOR, JACK BRANDT jcbrandt@unm.edu 1ASTR 101-3, FALL 2010

Why are the rings of Saturn so bright?

Question 7

a) They are made of frozen metallic hydrogen.b) They contain glassy beads expelled by volcanoes

on Enceladus.c) They contain shiny bits of iron.d) Titan and other moons reflect an additional glow

onto the rings. e) They are made of relatively new ice.

Saturn’s rings are perhaps only 50 million years old, the result of a small moon coming within

the planet’s Roche limit.

Page 35: LECTURE 12, OCTOBER 5, 2010 ASTR 101, SECTION 3 INSTRUCTOR, JACK BRANDT jcbrandt@unm.edu 1ASTR 101-3, FALL 2010

ASTR 101-3, FALL 2010 35

Page 36: LECTURE 12, OCTOBER 5, 2010 ASTR 101, SECTION 3 INSTRUCTOR, JACK BRANDT jcbrandt@unm.edu 1ASTR 101-3, FALL 2010

ASTR 101-3, FALL 2010 36

Page 37: LECTURE 12, OCTOBER 5, 2010 ASTR 101, SECTION 3 INSTRUCTOR, JACK BRANDT jcbrandt@unm.edu 1ASTR 101-3, FALL 2010

ASTR 101-3, FALL 2010 37

Page 38: LECTURE 12, OCTOBER 5, 2010 ASTR 101, SECTION 3 INSTRUCTOR, JACK BRANDT jcbrandt@unm.edu 1ASTR 101-3, FALL 2010

ASTR 101-3, FALL 2010 38

Page 39: LECTURE 12, OCTOBER 5, 2010 ASTR 101, SECTION 3 INSTRUCTOR, JACK BRANDT jcbrandt@unm.edu 1ASTR 101-3, FALL 2010

ASTR 101-3, FALL 2010 39

Page 40: LECTURE 12, OCTOBER 5, 2010 ASTR 101, SECTION 3 INSTRUCTOR, JACK BRANDT jcbrandt@unm.edu 1ASTR 101-3, FALL 2010

ASTR 101-3, FALL 2010 40