lecture 13, october 7, 2010 astr 101, section 3 instructor, jack brandt [email protected] 1astr...

33
LECTURE 13, OCTOBER 7, 2010 ASTR 101, SECTION 3 INSTRUCTOR, JACK BRANDT [email protected] 1 ASTR 101-3, FALL 2010

Upload: kory-holbrooks

Post on 02-Apr-2015

214 views

Category:

Documents


0 download

TRANSCRIPT

Page 1: LECTURE 13, OCTOBER 7, 2010 ASTR 101, SECTION 3 INSTRUCTOR, JACK BRANDT jcbrandt@unm.edu 1ASTR 101-3, FALL 2010

ASTR 101-3, FALL 2010 1

LECTURE 13, OCTOBER 7, 2010

ASTR 101, SECTION 3INSTRUCTOR, JACK BRANDT

[email protected]

Page 2: LECTURE 13, OCTOBER 7, 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 13, OCTOBER 7, 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 13, OCTOBER 7, 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 13, OCTOBER 7, 2010 ASTR 101, SECTION 3 INSTRUCTOR, JACK BRANDT jcbrandt@unm.edu 1ASTR 101-3, FALL 2010

ASTR 101-3, FALL 2010 5

HALLEY’S COMET

• First comet to have its return predicted. Occurred in 1759 AD, a triumph of celestial mechanics

• Seen at nearly every apparition since 239 BC• Returns on average every 76 years• Last return was in 1986 AD & 5 spacecraft were

sent to its vicinity• Next return is in 2061 AD

Page 6: LECTURE 13, OCTOBER 7, 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 13, OCTOBER 7, 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 13, OCTOBER 7, 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 13, OCTOBER 7, 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 13, OCTOBER 7, 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 13, OCTOBER 7, 2010 ASTR 101, SECTION 3 INSTRUCTOR, JACK BRANDT jcbrandt@unm.edu 1ASTR 101-3, FALL 2010

ASTR 101-3, FALL 2010 11

PROCESSES IN COMETS-1

• The basic process is sublimation, the direct transition from solid water ice to vapor

• Produces water vapor and releases dust particles and other gases trapped in the ice

• All cometary phenomena ultimately originate with material in the nucleus

• Energy source is solar radiation as the nucleus approaches the sun

Page 12: LECTURE 13, OCTOBER 7, 2010 ASTR 101, SECTION 3 INSTRUCTOR, JACK BRANDT jcbrandt@unm.edu 1ASTR 101-3, FALL 2010

ASTR 101-3, FALL 2010 12

PROCESSES IN COMETS-2

• Gas and dust emission comes from localized areas on the surface of the nucleus

• After sublimation occurs from the surface layers, a loose, dust crust remains. Confirmed by Deep Impact

• Dust and gas (atoms & molecules) flow outward to form the coma and hydrogen cloud

Page 13: LECTURE 13, OCTOBER 7, 2010 ASTR 101, SECTION 3 INSTRUCTOR, JACK BRANDT jcbrandt@unm.edu 1ASTR 101-3, FALL 2010

ASTR 101-3, FALL 2010 13

PROCESSES IN COMETS-3

• Solar radiation pressure pushes dust particles anti-sunward to make the dust tail

• Some molecules are ionized (electrically charged) and are carried anti-sunward by the solar wind to form the ion/plasma tail

Page 14: LECTURE 13, OCTOBER 7, 2010 ASTR 101, SECTION 3 INSTRUCTOR, JACK BRANDT jcbrandt@unm.edu 1ASTR 101-3, FALL 2010

ASTR 101-3, FALL 2010 14

TEXT PROBLEM, PAGE 111, ETC.

• The text statement: “Both types of tails are in all cases directed away from the Sun by the solar wind, an invisible steam of matter and radiation of escaping from the Sun.”

• This is wrong. See previous slide. Also, the solar wind is composed of particles and magnetic fields, but not radiation.

Page 15: LECTURE 13, OCTOBER 7, 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 13, OCTOBER 7, 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 13, OCTOBER 7, 2010 ASTR 101, SECTION 3 INSTRUCTOR, JACK BRANDT jcbrandt@unm.edu 1ASTR 101-3, FALL 2010

ASTR 101-3, FALL 2010 17

Question 9

Compared to asteroids, comets show all of these properties EXCEPT

a) their densities are higher.b) their orbits tend to be more elliptical.c) they tend to be made of ice.d) they can look fuzzy, whereas asteroids

appear as moving points of light.e) their average distances from the Sun

are far greater.

Page 18: LECTURE 13, OCTOBER 7, 2010 ASTR 101, SECTION 3 INSTRUCTOR, JACK BRANDT jcbrandt@unm.edu 1ASTR 101-3, FALL 2010

ASTR 101-3, FALL 2010 18

Question 9

Compared to asteroids, comets show all of these properties EXCEPT

Comets have densities much lower than asteroids or

planets.

a) their densities are higher.b) their orbits tend to be more elliptical.c) they tend to be made of ice.d) they can look fuzzy, whereas asteroids

appear as moving points of light.e) their average distances from the Sun

are far greater.

Page 19: LECTURE 13, OCTOBER 7, 2010 ASTR 101, SECTION 3 INSTRUCTOR, JACK BRANDT jcbrandt@unm.edu 1ASTR 101-3, FALL 2010

ASTR 101-3, FALL 2010 19

DISCONNECTION EVENTS

• Occasionally, the entire ion/plasma tail disconnects from the head region

• A new ion/plasma tail is formed• Produced by a specific feature in the solar

wind

Page 20: LECTURE 13, OCTOBER 7, 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 13, OCTOBER 7, 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 13, OCTOBER 7, 2010 ASTR 101, SECTION 3 INSTRUCTOR, JACK BRANDT jcbrandt@unm.edu 1ASTR 101-3, FALL 2010

ASTR 101-3, FALL 2010 22

Page 23: LECTURE 13, OCTOBER 7, 2010 ASTR 101, SECTION 3 INSTRUCTOR, JACK BRANDT jcbrandt@unm.edu 1ASTR 101-3, FALL 2010

ASTR 101-3, FALL 2010 23

Page 24: LECTURE 13, OCTOBER 7, 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 13, OCTOBER 7, 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 13, OCTOBER 7, 2010 ASTR 101, SECTION 3 INSTRUCTOR, JACK BRANDT jcbrandt@unm.edu 1ASTR 101-3, FALL 2010

ASTR 101-3, FALL 2010 26

What causes a meteor shower?

Question 10a) A comet and an asteroid collide.b) Earth runs into a stray swarm of asteroids.c) Earth runs into the debris of an old comet littering

its orbit. d) Meteorites are ejected from the Moon.e) Debris from a supernova enters Earth’s

atmosphere

Page 27: LECTURE 13, OCTOBER 7, 2010 ASTR 101, SECTION 3 INSTRUCTOR, JACK BRANDT jcbrandt@unm.edu 1ASTR 101-3, FALL 2010

ASTR 101-3, FALL 2010 27

What causes a meteor shower?

Question 10

Meteor showers can generate a few shooting stars, to hundreds of thousands, seen in an hour.

a) A comet and an asteroid collide.b) Earth runs into a stray swarm of asteroids.c) Earth runs into the debris of an old comet littering

its orbit. d) Meteorites are ejected from the Moon.e) Debris from a supernova enters Earth’s

atmosphere

Page 28: LECTURE 13, OCTOBER 7, 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 13, OCTOBER 7, 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 13, OCTOBER 7, 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 13, OCTOBER 7, 2010 ASTR 101, SECTION 3 INSTRUCTOR, JACK BRANDT jcbrandt@unm.edu 1ASTR 101-3, FALL 2010

ASTR 101-3, FALL 2010 31

Question 12

a) a cold terrestrial planet.b) a small jovian planet.c) a large Kuiper belt object.d) a wandering moon.e) a captured comet.

Many astronomers believe Pluto is perhaps best classified as

Page 32: LECTURE 13, OCTOBER 7, 2010 ASTR 101, SECTION 3 INSTRUCTOR, JACK BRANDT jcbrandt@unm.edu 1ASTR 101-3, FALL 2010

ASTR 101-3, FALL 2010 32

Many astronomers believe Pluto is perhaps best classified as

Question 12

a) a cold terrestrial planet.b) a small jovian planet.c) a large Kuiper belt object.d) a wandering moon.e) a captured comet.

Several other large Kuiper belt objects have been

discovered, including the largest known, called Eris.

Page 33: LECTURE 13, OCTOBER 7, 2010 ASTR 101, SECTION 3 INSTRUCTOR, JACK BRANDT jcbrandt@unm.edu 1ASTR 101-3, FALL 2010

ASTR 101-3, FALL 2010 33