Major Theme: The Earth as a basis of comparison for understanding the terrestrial planets.
Learning Objectives
- Identify the processes that cause primary and secondary atmospheres to be formed, retained, and lost.
- Compare the strength of the greenhouse effect and differences in the atmospheres of Earth, Venus, Mars
- Describe the layers of the atmospheres on Earth, Venus, and Mars, and explain how Earth’s atmosphere has been reshaped by the presence of life.
- Compare the atmosphere of Venus and Mars with the atmosphere of Earth.
- Describe how comparative planetology contributes to a better understanding of the changes in Earth’s climate.
- Identify the processes that cause primary and secondary atmospheres to be formed, retained, and lost.
- Compare the strength of the greenhouse effect and differences in the atmospheres of Earth, Venus, Mars
- Describe the layers of the atmospheres on Earth, Venus, and Mars, and explain how Earth’s atmosphere has been reshaped by the presence of life.
- Compare the atmosphere of Venus and Mars with the atmosphere of Earth.
- Describe how comparative planetology contributes to a better understanding of the changes in Earth’s climate.
Outline
Atmospheres change over time.
- Formation and loss of primary atmosphere
- Formation of the secondary atmosphere
Secondary atmospheres evolve
- The effect of planetary mass on a planet’s atmosphere
- The atmosphere greenhouse effect
- Thermal energy transfer into the atmosphere
- Similarities and differences among the terrestrial planets
Earth’s atmosphere has detailed structure
- Life and the composition of Earth’s atmosphere: Nitrogen, Oxygen, Ozone, CO2, Water Vapor
- The layers of Earth’s atmosphere
- Earth’s magnetosphere
- Wind and water
The atmospheres of Venus and Mars differ from Earth’s
- Venus and Mars
- Mercury and the Moon
Greenhouse gases affect global climates.
The giant planets are large, cold, and massive.
- Characteristics of the giant planets.
- Composition of the giant planets
- Days and seasons on the giant planets
The giant planets have clouds and weather.
- The structure below the cloud tops.
- Winds and weather: Jupiter, Saturn, Neptune.
The interiors of the giant planets are hot and dense.
- The cores of Jupiter and Saturn
- The cores of Uranus and Neptune
The giant planets are magnetic powerhouses
- The size and shape of the magnetosphere
- Radiation belts and auroras of the giant planets
The planets of our solar system might not be typical
- Different types of “Jupiters”
- Super-Earths to Mini-Neptunes
Activities:
- Read textbook: Chapter 10.3, Chapter 11
- Topic class notes
- Phet: Greenhouse gases
- Lecture Tutorial: Greenhouse Effect (pair and share).
- Lab 8: Planetary Atmospheres (see lab manual): see the Phet Greenhouse simulation and NASA’s Climate Change website.
- ClassAction: Jovian Planets, lessons 9-14
Extra Stuff:
- Star Chart of the Month
- The evidence for climate change: Decoding the Weather Machine
- Open House: Chamberlain Observatory