Title: Earth and Other Planets
1Earth and Other Planets
Great Idea Earth, one of the planets that orbit
the Sun, formed 4.5 billion years ago from a
great cloud of dust.
2Chapter Outline
- The Formation of the Solar System
- Exploring the Solar System
3The Formation of the Solar System
4Clues to the Origin of the Solar System
- Solar system
- Objects gravitationally bound to Sun
- Deduction of origin
- Observations
- Earth
- Space
5Clue 1 Planetary Orbits
- Features of solar system
- All planets orbit in same direction
- Orbits in same plane
- Most rotate in direction of orbit
6Clue 2 Distribution of Mass
- Most material within Sun
- Two types of planets
- Terrestrial planets
- Jovian planets
- Other objects
- Moons, asteroids, comets
7The Nebular Hypothesis
- Nebular Hypothesis
- Cloud of dust and gas
- 99 H and He
- Collapse of nebula
- Planetary orbits
- Clumping of matter
- Planetesimals
- Temperature
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9The surface of Venus is shrouded in clouds, but
the Magellan spacecraft produced radar images
of the surface. In this computer-generated view
of a Venusian volcano, the vertical relief has
been greatly exaggerated.
10The Formation of Earth
- Planetesimals
- Combined to form earth
- Great bombardment
- Meteors
- Growth of planet
- 20 metric tons per day
11Differentiation
- Differentiation
- Heat from collisions
- Dense material sank to center
- Lighter material rose to surface
- Structure
- Core
- Mantle
- Crust
12Researchers attain high pressures, equivalent to
those deep inside the Earth and other planets,
using the diamond anvil cell. Looking through
such diamond cells you can observe pressurized
samples such as this high-pressure ice crystal
that was formed at room temperature by squeezing
water.
13Earths Atmosphere
- The temperature of the atmosphere is a
complicated function of altitude.
14Our Atmosphere 50 below 3.5 miles 90 below 10
miles 99 below 20 miles ozone hole global
warming
15The concentration of which gas is increasing in
our atmosphere leading to global warming?
A Clicker Question.
- water
- acetone
- carbon dioxide
- carbon monoxide
- tri-carbon
16Ozone and the Upper Atmosphere
- Ozone absorbs photons with a wavelength between
240 and 310 nm. - Most of the ozone is present in the stratosphere
- Between 30 and 90 km photodissociation of oxygen
is possible - O2(g) h? ? 2O(g)
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18Ozone and the Upper Atmosphere
- The oxygen atoms can collide with oxygen
molecules to form ozone - O(g) O2(g) ? O3(g)
19Ozone and the Upper Atmosphere
- Depletion of the Ozone Layer
- In 1974 Rowland and Molina showed that chlorine
from chlorofluorocarbons (CFCs) deplete the ozone
layer by catalyzing the formation of ClO and O2.
20The Formation of the Moon
- Big Splash
- Large object impacted earth
- Parts of mantle blown into orbit
- Moon formed from this material
21Planetary Idiosyncracies
- Cratering
- Mercury, Mars, Moon
- None on earth
- weathering
- Rotation
- Venus
- Earths axis
- Uranus
22The Evolution of Planetary Atmospheres
- Earths atmosphere
- Early
- Outgassing
- Atmosphere was N2, CO2, H2, H2O
- Gravitational escape
- Living organisms
23Exploring the Solar System
24The Inner Solar System
- Mercury, Venus, Mars
- Mercury and Venus too hot for life
- Mars Exploration
- Multiple missions
- Found evidence of water
25The Outer Solar System
- Jupiter, Saturn, Uranus, Neptune
- Layered structure
- No solid surface
- Jupiter
- Comet Shoemaker-Levy
- Galileo spacecraft
- Saturn
- Cassini spacecraft
26Moons and Rings of the Outer Planets
- Moons
- Io
- Europa
- Titan
- Rings
- Ice and rock
27Pluto
- Pluto
- Outermost planet
- .3 of earths mass
- Three moons
- Formation
- Captured comet or asteroid
- Still open to question
28A Tenth Planet?
- Xena
- Orbits sun every 560 years
- One moon
- Larger than Pluto
29Asteroids, Comets, and Meteors
- Asteroids
- Small rocky bodies
- Orbit sun
- Most in belt between Mars and Jupiter
- Comets
- Dirty snowballs
- Orbit outside Pluto
- Oort cloud
- Kuiper belt
- Halleys Comet
- Stardust and Deep Impact missions
- Meteoroids, Meteors, and Meteorites
- Meteor showers
- Original solar system material