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Week 8 Day Announcements Grades First iClicker scores have posted (from 4 classes) Participation scores will be up to date after Spring Break Email Dr. Saul if there are discrepancies (include your iClicker number) Homework: Homework assignments for Chs 4 & 5 will post tomorrow Cannot do homework without Mastering Astronomy Homework counts for 22% of your grade NOT DOING HOMEWORK REDUCES YOUR CHANCES OF A GOOD GRADE IN THIS CLASS Extensions • Since Extensions remove late penalties, you can keep working on your homework assignments while waiting for an extension to be granted Email

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Page 1: Week 8 Day Announcements Grades First iClicker scores have posted (from 4 classes) Participation scores will be up to date after Spring Break Email Dr

Week 8 Day AnnouncementsGrades

• First iClicker scores have posted (from 4 classes)• Participation scores will be up to date after Spring Break• Email Dr. Saul if there are discrepancies (include your iClicker number)

Homework:• Homework assignments for Chs 4 & 5 will post tomorrow• Cannot do homework without Mastering Astronomy• Homework counts for 22% of your grade• NOT DOING HOMEWORK REDUCES YOUR CHANCES OF A

GOOD GRADE IN THIS CLASS

Extensions• Since Extensions remove late penalties, you can keep working on your

homework assignments while waiting for an extension to be granted

Email• Make sure you include ASTR 101 in email subject and your name at the

end of the message text.

Page 2: Week 8 Day Announcements Grades First iClicker scores have posted (from 4 classes) Participation scores will be up to date after Spring Break Email Dr

a) beyond the orbit of Neptune.

b) between Earth and the Sun.

c) between Mars and Jupiter.

d) in the orbit of Jupiter, but 60 degrees ahead or behind it.

e) orbiting the jovian planets in captured, retrograde orbits.

Most asteroids are found

Question 7

Page 3: Week 8 Day Announcements Grades First iClicker scores have posted (from 4 classes) Participation scores will be up to date after Spring Break Email Dr

a) beyond the orbit of Neptune.

b) between Earth and the Sun.

c) between Mars and Jupiter.

d) in the orbit of Jupiter, but 60 degrees ahead or behind it.

e) orbiting the jovian planets in captured, retrograde orbits.

Question 7

Most asteroids are found

The Asteroid Belt is located between

2.1 and 3.3 A U from the Sun.

Page 4: Week 8 Day Announcements Grades First iClicker scores have posted (from 4 classes) Participation scores will be up to date after Spring Break Email Dr

The Structure of the Solar System

~ 45 AU~ 5 AU

L4

L5

L3

Page 5: Week 8 Day Announcements Grades First iClicker scores have posted (from 4 classes) Participation scores will be up to date after Spring Break Email Dr

Lagrange Points

Page 6: Week 8 Day Announcements Grades First iClicker scores have posted (from 4 classes) Participation scores will be up to date after Spring Break Email Dr

Interplanetary Matter: Asteroids

The inner solar system, showing the asteroid belt, Earth-crossing asteroids, and Trojan asteroids

Page 7: Week 8 Day Announcements Grades First iClicker scores have posted (from 4 classes) Participation scores will be up to date after Spring Break Email Dr

Interplanetary Matter: Asteroids

Large picture: The path of Icarus, an Earth-crossing asteroid

Inset: Ceres, the largest asteroid

Page 8: Week 8 Day Announcements Grades First iClicker scores have posted (from 4 classes) Participation scores will be up to date after Spring Break Email Dr

Asteroids and meteoroids have rocky composition; asteroids are bigger.

(above) Asteroid Ida with its moon, Dactyl

(below) Asteroid Gaspra

(above) Asteroid Mathilde

Interplanetary Matter: Asteroids

Page 9: Week 8 Day Announcements Grades First iClicker scores have posted (from 4 classes) Participation scores will be up to date after Spring Break Email Dr

Interplanetary Matter: Asteroids

Asteroid Eros

Page 10: Week 8 Day Announcements Grades First iClicker scores have posted (from 4 classes) Participation scores will be up to date after Spring Break Email Dr

Comets are icy, with some rocky parts.

The basic components of a comet

Interplanetary Matter: Comets

Page 11: Week 8 Day Announcements Grades First iClicker scores have posted (from 4 classes) Participation scores will be up to date after Spring Break Email Dr

Interplanetary Matter: Comets

The solar wind means the ion tail always points away from the Sun.

The dust tail also tends to point away from the Sun, but the dust particles are more massive and lag somewhat, forming a curved tail.

Page 12: Week 8 Day Announcements Grades First iClicker scores have posted (from 4 classes) Participation scores will be up to date after Spring Break Email Dr

Interplanetary Matter: Comets

The internal structure of the cometary nucleus

Page 13: Week 8 Day Announcements Grades First iClicker scores have posted (from 4 classes) Participation scores will be up to date after Spring Break Email Dr

Oort Cloud

The size, shape, and orientation of cometary orbits depend on their location. Oort cloud comets rarely enter the inner solar system.

Page 14: Week 8 Day Announcements Grades First iClicker scores have posted (from 4 classes) Participation scores will be up to date after Spring Break Email Dr

Meteor Showers

Meteor showers are associated with comets – they are the debris left over when a comet breaks up.

Page 15: Week 8 Day Announcements Grades First iClicker scores have posted (from 4 classes) Participation scores will be up to date after Spring Break Email Dr

Meteor Showers

Page 16: Week 8 Day Announcements Grades First iClicker scores have posted (from 4 classes) Participation scores will be up to date after Spring Break Email Dr

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 17: Week 8 Day Announcements Grades First iClicker scores have posted (from 4 classes) Participation scores will be up to date after Spring Break Email Dr

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 18: Week 8 Day Announcements Grades First iClicker scores have posted (from 4 classes) Participation scores will be up to date after Spring Break Email Dr

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 19: Week 8 Day Announcements Grades First iClicker scores have posted (from 4 classes) Participation scores will be up to date after Spring Break Email Dr

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 20: Week 8 Day Announcements Grades First iClicker scores have posted (from 4 classes) Participation scores will be up to date after Spring Break Email Dr

Chapter 5: The Earth

Page 21: Week 8 Day Announcements Grades First iClicker scores have posted (from 4 classes) Participation scores will be up to date after Spring Break Email Dr

Pale Blue Dot

Earth as seen from Voyager 1, when it was 6 billion km from home.

Page 22: Week 8 Day Announcements Grades First iClicker scores have posted (from 4 classes) Participation scores will be up to date after Spring Break Email Dr

General Features

Mass: MEarth

= 6 x 1027 g

Radius: REarth

= 6378 km

Density: p = 5.5 g/cm3

Age: 4.6 billion years

Page 23: Week 8 Day Announcements Grades First iClicker scores have posted (from 4 classes) Participation scores will be up to date after Spring Break Email Dr

Earth's Internal Structure

Crust: thin. Much Si and Al(lots of granite). Two-thirds covered by oceans.

How do we know? Earthquakes. See later

Mantle is mostly solid, mostly basalt (Fe, Mg, Si). Cracks in mantle allow molten material to rise => volcanoes.

Core temperature is 6000 K. Metallic - mostly nickel and iron. Outer core molten, innercore solid.

Atmosphere very thin

Page 24: Week 8 Day Announcements Grades First iClicker scores have posted (from 4 classes) Participation scores will be up to date after Spring Break Email Dr

Earth's Atmosphere

78% Nitrogen21% Oxygen

gas is ionized by solar radiation

ozone is O3 , which

absorbs solar UV efficiently, thusheating stratosphere

commercial jet altitudes

temperature on a cool day

Original gases disappeared. Atmosphere is mostly due to volcanoes and plants!

Page 25: Week 8 Day Announcements Grades First iClicker scores have posted (from 4 classes) Participation scores will be up to date after Spring Break Email Dr

Ionosphere

Particles in the upper reaches of the atmosphere are ionized by the sun.

Radio signals below ~20 MHz can “bounce” off the ionosphere allowingCommunication “over the horizon” (or mountains)

Page 26: Week 8 Day Announcements Grades First iClicker scores have posted (from 4 classes) Participation scores will be up to date after Spring Break Email Dr

EarthquakesThey are vibrations in the solid Earth, or seismic waves.

Two kinds go through Earth, P-waves ("primary") and S-waves ("secondary"):

Page 27: Week 8 Day Announcements Grades First iClicker scores have posted (from 4 classes) Participation scores will be up to date after Spring Break Email Dr

How do they measure where Earthquakes are centered?

* *

*

seismic stations

Page 28: Week 8 Day Announcements Grades First iClicker scores have posted (from 4 classes) Participation scores will be up to date after Spring Break Email Dr

Like all waves, seismic waves bend when they encounter changes in density. If density change is gradual, wave path is curved.

S-waves are unable to travel in liquid.

Thus, measurement of seismic wave gives info on density of Earth's interior and which layers are solid/molten.

But faint P wavesseen in shadow zone,refracting off denseinner core

Curved paths ofP and S waves:density must slowlyincrease with depth

Zone with no S waves:must be a liquid corethat stops them

No P waves too:they must bend sharplyat core boundary

Page 29: Week 8 Day Announcements Grades First iClicker scores have posted (from 4 classes) Participation scores will be up to date after Spring Break Email Dr

Earth's Interior Structure

Average density

CrustMantleCore

5.5 g/cm3

3 g/cm3

5 g/cm3

11 g/cm3

Density increases with depth => "differentiation"

Earth must have been molten once, allowing denser material to sink, as it started to cool and solidify.

Page 30: Week 8 Day Announcements Grades First iClicker scores have posted (from 4 classes) Participation scores will be up to date after Spring Break Email Dr

Earthquakes and volcanoes are related, and also don't occur at random places. They outline plates.

Plates moving at a few cm/year. "Continental drift" or "plate tectonics"

Page 31: Week 8 Day Announcements Grades First iClicker scores have posted (from 4 classes) Participation scores will be up to date after Spring Break Email Dr

When plates meet...

1) Head-on collision (Himalayas)

2) "Subduction zone" (one slides under the other) (Andes)

3) "Rift zone" (two plates moving apart) (Mid-Atlantic Ridge)

4) They may just slide past each other (San Andreas Fault)

side view

top view

=> mountain ranges, trenches, earthquakes, volcanoes

Page 32: Week 8 Day Announcements Grades First iClicker scores have posted (from 4 classes) Participation scores will be up to date after Spring Break Email Dr

Clicker Question:

Sunlight absorbed by the Earth’s surface is reemitted in the form of?

A: radio waves

B: infrared radiation

C: visible radiation

D: ultraviolet radiation

E: X-ray radiation

Page 33: Week 8 Day Announcements Grades First iClicker scores have posted (from 4 classes) Participation scores will be up to date after Spring Break Email Dr

The Mid-Atlantic Ridge is a rift zone.

Page 34: Week 8 Day Announcements Grades First iClicker scores have posted (from 4 classes) Participation scores will be up to date after Spring Break Email Dr

What causes the drift?

Convection! Mantle slightly fluid and can support convection. Plates ride on top of convective cells. Lava flows through cell boundaries. Earth loses internal heat this way.

Cycles take ~108 years.

Plates form lithosphere (crust and solid upper mantle).Partially melted, circulating part of mantle is asthenosphere.

Page 35: Week 8 Day Announcements Grades First iClicker scores have posted (from 4 classes) Participation scores will be up to date after Spring Break Email Dr

Pangaea Theory: 200 million years ago, all the continents were together!