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Transcript
4/21/2014
Chapter 21 Section 2
The Inner Planets
Objectives
• Explain the difference between a planet’s
period of rotation and period of revolution.
• Describe the difference between prograde and
retrograde rotation
• Describe the individual characteristics of
Mercury, Venus, Earth, & Mars
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Measuring Interplanetary Distance
Astronomical Unit – average
distance between the Earth and
the sun
• 150 million kilometers
Speed of light
• 300,000 km/s
• Light minute = light travels 18
million km in one minute.
• Light from the sun takes 8.3 light
minutes to reach Earth.
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Terrestrial Planets
Terrestrial Planets
• Small
• Dense
• Rocky
• Near the sun
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Mercury: Closest to the Sun
Mercury
• Less massive = less gravity
• One day = 59 Earth days
– Period of rotation = 59 days long
• One year = 88 Earth days
– Period of revolution = 88 days
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Venus: Earth’s Twin
Venus
• Similar to Earth: mass and density
• Different: Sun rises in west and sets in East
– Prograde rotation: counterclockwise when viewed
from N. Pole
• Earth
– Retrograde rotation: clockwise when viewed from N.
Pole
• Venus
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Venus: Earth’s Twin
Venus (continued)
• Atmosphere
– Dense! 90 times the
pressure of Earth’s
– Carbon dioxide,
destructive acids,
– Hot! 867.2oF
• Carbon dioxide traps heat
• Surface
– Mapped the surface with
radar waves
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Mars: Our Intriguing Neighbor
Mars
• Less mass = less density (38% of Earth’s gravity)
• Thin atmosphere = cold
– Summer temps: a high of 8.6oF
– No ozone = liquid water would quickly boil away
• Has frozen water
4
4/21/2014
Chapter 21 Section 3
The Outer Planets
Objectives
1. Explain how gas giants are different from
terrestrial planets.
2. Describe the individual characteristics of
Jupiter, Saturn, Uranus, and Neptune
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Gas Giants!
Gas Giants
• Deep, massive atmosphere
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Jupiter: A Giant Among Giants
Jupiter
• Largest
• Hydrogen & helium
• Atmosphere = clouds of water, methane, &
ammonia
• Radiates more energy than it receives from
the sun.
6
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