chapter 8 the solar system. how was it formed the nebular theory started as nebula about 5 billion...
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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
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
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
• Jupiter’s gravity stopped a planet from forming• Oort Cloud- Near the edge clumps of matter-
home of comets.
The Origin of the Moon Giant Impact Hypothesis
A very large body crashed into the Earth. Debris from the impact made a moon.
• 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
• 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.
Why Do We Think This?
• The moon has no iron– Earth’s 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
Surface Features on the Moon
Two types of Surfaces– Highlands
• More heavily cratered surface is older.
– Maria (“Seas”)• Less heavily cratered
surface is younger.
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.
Centrifugal Force
• unequal masses of Earth and Moon – center of rotation lies beneath the Earth’s
surface.
• second tidal bulge– ocean shifts away from center of rotation
Special Features of the Planets
• Mercury
• Many Craters– no atmosphere– no erosion
• Slow rotation makes it hot and cold
Venus• Thick atmosphere of
carbon dioxide
• Sulfuric acid clouds
• Greenhouse effect– carbon dioxide traps
heat.– Makes Venus hotter
than Mercury
• Retrograde rotation - rotates backward
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
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
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
Uranus
• Twice as far from the sun as Saturn.
• Covered with ocean of superheated water
• Tilted on axis• Rings of methane ice• Many moons
Neptune
• Like Uranus• Hydrogen and
helium atmosphere
• Surface of water and methane
• Rings made of dust
• Eight moons
Triton
• Large moon
• Thought to be captured
• Retrograde revolution
• out of plane of Neptune’s rotation
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
The Sun• An average star
• Over 1 million earth’s would fit inside
• 1/4 the density of the Earth
• made of 4 layers
Corona- Outermost layer•Temp-1,700,000ºC•Few particlesChromosphere-middle of atmosphere•Temp-27,800ºC•1000’s of km thick
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
Meteorites
• Leave a crater where they hit the ground
• Meteorite Crater in Arizona
• Evidence of meteorites from the moon and from Mars
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