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The Solar System

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The Solar System How was it formed The Nebular Theory Started as nebula about 5 billion years ago Composed of hydrogen and helium Nearby supernova sent shock waves ... – PowerPoint PPT presentation

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Title: The Solar System


1
Chapter 8
  • The Solar System

2
How was it formed
  • The Nebular Theory
  • Started as nebula about 5 billion years ago
  • Composed of hydrogen and helium
  • Nearby supernova sent shock waves through galaxy
  • caused gases to be pulled inward
  • supplied new elements
  • Shrank to a spinning disk 10 billion kilometers
    across
  • Gravity heated center to protostar - the sun

3
How was it formed
  • Other matter spun around the new sun
  • gathered into clumps- protoplanets
  • Near the sun the light weight gases boiled away
  • Mercury, Venus, Earth, Mars
  • In those far away the gases did not boil away
  • Jupiter, Saturn, Uranus, Neptune
  • the gas giants

4
How was it formed
  • Around the protoplanets smaller clumps formed
    moons or satellites.
  • Pluto is thought to be a moon of Neptune that
    broke away.
  • Asteroid belt- clumps of rocks between Mars and
    Jupiter
  • Jupiters gravity stopped a planet from forming
  • Oort Cloud- Near the edge clumps of matter- home
    of comets.

5
The Origin of the Moon Giant Impact Hypothesis
  • A very large body crashed into the Earth. Debris
    from the impact made a moon.

6
  • 4.6 byr ago -- Moon formed, possibly due to
    collision of Earth and a large, Mars-sized
    object.
  • If Earth already differentiated, most material
    expelled would be mantle material, not iron core

7
  • Rock at impact heated, losing volatile elements
  • Some debris falls back to Earth, some forms Moon.
  • Earth and Moon each pulled back into spherical
    shape by gravity.

8
Why Do We Think This?
  • The moon has no iron
  • Earths iron had already concentrated in the core
    by the time of the impact
  • The iron core of the impactor melded with that of
    the Earth, leaving the moon with no iron of its
    own
  • The moon and Earth share isotopes of oxygen that
    are not found on other planets or objects far
    from Earth

9
Surface Features on the Moon
  • Two types of Surfaces
  • Highlands
  • More heavily cratered ? surface is older.
  • Maria (Seas)
  • Less heavily cratered ? surface is younger.

10
What causes tides?
2 Bulges from Gravitational Attraction
Centrifugal Force
11
Gravitational Attraction
  • All masses are drawn to each other.
  • The moon because of its closeness to the Earth
    exerts a greater gravitational effect on the
    Earth than the Sun, despite the fact that the Sun
    is much more massive than the Moon.

12
Centrifugal Force
  • unequal masses of Earth and Moon
  • center of rotation lies beneath the Earths
    surface.
  • second tidal bulge
  • ocean shifts away from center of rotation

13
Special Features of the Planets
  • Mercury
  • Many Craters
  • no atmosphere
  • no erosion
  • Slow rotation makes it hot and cold

14
Venus
  • Thick atmosphere of carbon dioxide
  • Sulfuric acid clouds
  • Greenhouse effect
  • carbon dioxide traps heat.
  • Makes Venus hotter than Mercury
  • Retrograde rotation - rotates backward

15
Mars
  • Red planet- covered by iron oxide (rust)
  • Mons Olympus -
  • Largest volcano in the solar system
  • Two ice caps
  • north - water -never melts
  • south -carbon dioxide melts in summer

16
Two moons of Mars
Phobos
Deimos
17
Jupiter
18
Jupiter
  • Largest of the gas giants
  • Huge storms - red spot
  • Small solid core
  • Liquid metal layer makes a huge magnetic field
  • Magnetosphere
  • Gives off more heat than it receives from the sun
  • Thin ring

19
16 moons
  • 4 seen by Galileo helped change science

20
Saturn
  • Similar to Jupiter
  • Clouds, magnetosphere, gives off heat
  • Rotates in 10 hours - makes it bulge in the
    middle and flat at the poles
  • Low density- would float in water

21
Saturn
  • Many rings
  • complex system
  • made of water
  • weave in and out

22
Saturn
  • Many moons -
  • Titan- the largest is like the early Earth.

23
Uranus
  • Twice as far from the sun as Saturn.
  • Covered with ocean of superheated water
  • Tilted on axis
  • Rings of methane ice
  • Many moons

24
Neptune
  • Like Uranus
  • Hydrogen and helium atmosphere
  • Surface of water and methane
  • Rings made of dust
  • Eight moons

25
Triton
  • Large moon
  • Thought to be captured
  • Retrograde revolution
  • out of plane of Neptunes rotation

26
Pluto
  • Moon sized
  • Made of methane
  • Pink atmosphere on the sunny side
  • Moon Charon 1/2 the size of Pluto
  • Scientists think it is a moon broken away from
    Neptune
  • Orbit crosses Neptune
  • Orbit not in plane with other planets

27
The Sun
  • An average star
  • Over 1 million earths would fit inside
  • 1/4 the density of the Earth
  • made of 4 layers

28
  • Corona- Outermost layer
  • Temp-1,700,000ºC
  • Few particles
  • Chromosphere-
  • middle of atmosphere
  • Temp-27,800ºC
  • 1000s of km thick

29
  • Photosphere-
  • Temp-6000ºC
  • 550 km thick
  • Surface of the sun

Core-
1,000,000ºC
15,000,000ºC
30
Activity on the Sun
  • Storms on the sun
  • Prominences- Loops or arches of gas that rise
    from the chromosphere
  • Solar Flares- Bright bursts of light, huge
    amounts of energy released
  • Sunspots- Dark areas on the suns surface
  • in the lower atmosphere
  • Motion shows the rotation of the sun
  • Interferes with radio

31
Meteorites
  • Leave a crater where they hit the ground
  • Meteorite Crater in Arizona
  • Evidence of meteorites from the moon and from Mars

32
Comets
  • Chunks of dust and gas from the Oort Cloud that
    orbit the sun
  • When it gets close to the sun it gets hotter
  • Some of the gas and dust form a cloud around the
    head called the coma
  • Solar wind pushes the gases away from the sun and
    make the tail
  • Tail is pushed by the solar wind
  • Tail always points way from the sun

33
Coma
Tail
Nucleus
34
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