ASTRONOMY 161 Introduction to Solar System Astronomy - PowerPoint PPT Presentation

1 / 38
About This Presentation
Title:

ASTRONOMY 161 Introduction to Solar System Astronomy

Description:

ASTRONOMY 161 Introduction to Solar System Astronomy – PowerPoint PPT presentation

Number of Views:288
Avg rating:3.0/5.0
Slides: 39
Provided by: astronomy
Category:

less

Transcript and Presenter's Notes

Title: ASTRONOMY 161 Introduction to Solar System Astronomy


1
ASTRONOMY 161Introduction to Solar System
Astronomy
Class 15
2
Midterm 2 (Friday, in class)
  • 1) Use the study guide.
  • 2) Know and understand the basic equations.
  • 3) Only material covered in class is required.
  • 4) Laws of motion are important.
  • 5) Properties of light are important.
  • Good luck!

3
Midterm Exam Sample Question
  • The masses of planets are measured from
  • A) their brightness.
  • B) their size and density.
  • C) acceleration their gravity produces on nearby
    objects.
  • D) infrared and radio emission.
  • E) their resistance to being gravitationally
    accelerated.

4
Midterm Exam Sample Questions
  • Name the planet which comes closest to the Earth
    (26 million miles)
  • A) Saturn
  • B) Jupiter
  • C) Venus
  • D) Uranus
  • E) Mercury

5
The Earth Wednesday, October 27
6
(No Transcript)
7
(No Transcript)
8
(No Transcript)
9
The Earth Physical characteristics
  • Mass 5.971024 kg
  • Mean radius 6,373 km
  • Polar radius 6,357 km
  • Density 5,515 kg/m³
  • Sidereal rotation period 0.9973 d (23.934 h)
  • Axial tilt 23.4

10
The Earth Key Concepts
  • (1) The study of seismic waves tells us about the
    Earths interior.
  • (2) The Earth is layered into crust, mantle,
    inner core, and outer core.
  • (3) The Earth is layered because it underwent
    differentiation when molten.
  • (4) The lithosphere is broken into plates that
    move relative to each other.
  • (5) The motion of liquid metal in the outer core
    produces a magnetic field.

11
(1) The study of seismic waves
tells us about the Earths interior.
  • How can we study the deep interior of the Earth?
  • Average density of the Earth 5500 kg/m3
  • Earth is too dense to be solid rock
    Basalt 3300 kg/m3 Granite
    2700 kg/m3

12
(No Transcript)
13
(No Transcript)
14
  • Earthquakes produce two types of seismic waves
  • P waves Primary, Pressure Sound waves travel
    through solids and liquids.
  • S waves Secondary, Shear Transverse
    (side-to-side) waves that do NOT travel through
    liquids.

15
(No Transcript)
16
  • Seismic waves radiating through the Earth after
    an earthquake
  • Note S waves do not travel through the outer
    core!

17
(2) The earth is layered into a crust, mantle,
inner core, and outer core.
  • From the outside in
  • 1) Crust
    solid rock
    5 km
    thick basalt (ocean floor)
    35 km thick granite (continents)
  • 2) Mantle
    partly solid rock, partly semisolid
    (plastic) rock 2900 km thick

18
  • 3) Outer (liquid) core
    molten iron and nickel
    2200 km thick
  • 4) Inner (solid) core
    solid iron and nickel
    1300 km in radius

19
  • The center of the Earth is as hot as the surface
    of the Sun.
  • Why doesnt the inner core melt??
  • The high pressure in the inner core keeps it
    solid.

20
(3) The Earth is layered because it underwent
differentiation when molten.
  • When young, the Earth was heated by the impact of
    planetesimals. For a while, the Earth was molten.
  • In a liquid, dense stuff sinks, low-density stuff
    floats.

21
  • When differentiation was complete, Earth cooled
    and (partly) solidified.
  • Crust of the ocean floor floats on the mantle
    like skin on cocoa lower-density continents
    are the marshmallows.

22
(4) The lithosphere is broken into plates
that move relative to each other.
  • The crust plus the upper mantle form the
    lithosphere (solid but brittle).
  • Beneath the lithosphere is the asthenosphere
    (plastic).
  • The asthenosphere, heated from below,
    undergoes convection.

23
Convection
24
  • Convection currents in the asthenosphere have
    broken the lithosphere into sections called
    plates.
  • There are 15 large plates.

25
  • Continuing convection in the asthenosphere causes
    plates to move relative to each other.
  • The study of plate motion is called plate
    tectonics.
  • The motion of continents
    was first suspected by
    Sir Francis Bacon
    (17th cent). Best
    known for leading the
    scientific revolution with his
    new 'observation and
    experimentation' theory.

26
  • America and Europe are moving apart by 3
    centimeters per year ( 30 km per million
    years).
  • This continental drift is measured using GPS
    (global positioning systems).

27
  • 200 million years ago, the Americas, Europe, and
    Africa formed a single supercontinent, PANGAEA.

28
  • The boundaries between plates are geologically
    active, with many volcanoes and earthquakes.
  • Example the Ring of Fire around the Pacific
    Ocean.

29
(No Transcript)
30
  • Types of plate boundaries
  • 1) Oceanic rift plates moving apart, new rock
    forming.
  • 2) Subduction zone plates moving together, ocean
    crust shoved under continent.
  • 3) Mountain-building zone plates moving
    together, continents collide buckle upward.
  • 4) Transverse fault plates slipping past each
    other, with lots of friction.

31
  • The summit of Mount Everest is made of marine
    limestone.
  • It has been lifted
    9 kilometers
    high!

32
  • Grand Tetons

33
  • Grand Tetons

34
  • The San Andreas
    transverse fault
  • Motion jumps
    during a quake

35
(5) The motion of liquid metal in the outer core
produces a magnetic field.
  • A compass points to the Earths North Magnetic
    Pole (not the true North Pole!)
  • Why is the Earth a giant magnet?

36
  • Remember Moving charged particles create a
    magnetic field.
  • Inside the Earth, convection currents exist
    within the liquid outer core. These currents
    carry electrons around, creating a magnetic field.

37
  • The Earths magnetic field stretches far beyond
    the surface.
  • Our magnetic field deflects the solar wind
    (electrons and protons streaming away from the
    Sun).

38
Few closing questions
  • 1) Are there earthquakes in Ohio?
  • 2) Are there any volcanoes in Ohio?
  • 3) Why is Ohio so boring?
  • 4) If you are at the North Pole, which way does
    the compass needle point?
Write a Comment
User Comments (0)
About PowerShow.com