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Announcements The last Dark Sky Observing Night is tonight. Starts at 7:30pm at the APSU Observatory on “The Farm”. Try to arrive a little early so your.

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Presentation on theme: "Announcements The last Dark Sky Observing Night is tonight. Starts at 7:30pm at the APSU Observatory on “The Farm”. Try to arrive a little early so your."— Presentation transcript:

1 Announcements The last Dark Sky Observing Night is tonight. Starts at 7:30pm at the APSU Observatory on “The Farm”. Try to arrive a little early so your lights don’t interfere with the observing in progress. Since there is a high chance tonight will be cancelled, we will try again tomorrow night (Tuesday). There is also a Dark Sky Alternative posted in www.apsu.edu/astronomy/dark-sky- observing-nightwww.apsu.edu/astronomy/dark-sky- observing-night

2 The Greenhouse Effect Lecture-Tutorial The greenhouse gasses are mostly CO 2 and H 2 O but CH 4 and a few others also contribute

3 iClicker Question The main reason Earth’s average temperature is not below 0°C is because a)volcanoes heat the atmosphere. b)solar radiation alone is enough. c)the greenhouse effect warms the ground above what it would otherwise be. d)continental drift and tectonics adds heat to the atmosphere.

4 Another iClicker Question The greenhouse effect is caused mostly by a)the aurora borealis. b)pesticides. c)depletion of the ozone layer by manmade CFC’s. d)carbon dioxide and water vapor in the atmosphere

5 One More iClicker Question The Earth’s surface absorbs energy from sunlight and then radiates the same amount of energy back into space. The best proof for this fact is that the average annual surface temperature on Earth is a)warming rapidly. b)not changing much. c)cooling rapidly. d)fluctuating wildly.

6 Earth’s Atmosphere is layered like an onion The layers are due to how the temperature changes with altitude. Mars and Venus don’t show the same kind of layering.

7 The way temperature changes is due to energy transport In the troposphere convection is driven by heat from the ground In the stratosphere and thermosphere energy is absorbed directly from the sun

8 Just as in the interior of the planets, convection is important to atmospheres Rotation and the Coriolis effect are also important

9 Magnetic fields are also very important to atmospheres Earth’s relatively strong magnetic field protects our atmosphere from erosion by the solar wind

10 The weak or non-existent magnetic fields of Venus and Mars lead to strong erosion by the solar winds

11 iClicker Question ClassAction website Terrestrial Planets module Magnetic Fields and Atmospheres

12 Another iClicker Question If its mass was closer to that of Earth and Venus, Mars might a) still have an active interior. b) have a thick atmosphere. c) have abundant liquid water and larger ice caps. d) have a strong magnetic field. e) All of the above.

13 Is mankind changing Earth’s atmosphere? Man?

14 Each spring in Antarctica a hole develops in the ozone layer

15 Ozone depletion is caused by CFC’s CFC’s are Chlorofluorocarbon molecules which are man made compounds. They do not occur naturally

16 The solution: stop using CFC’s The 1987 Montreal Treaty gradually reduces the production and consumption of CFC’s worldwide

17 Is the Ozone Hole getting worse or better?

18 Our actions have led to an increase in the level of a number of greenhouse gases Unfortunately, we can’t stop producing these gases as easily as we stopped producing CFC’s

19 Deforestation has a major impact Earth’s atmosphere

20 Deforestation removes the trees that remove CO 2 The cut trees are usually burned which adds more CO 2 to the atmosphere

21 There is a direct relationship between the level of CO 2 and the global average temperature

22 One model of where it will get hot in the future based on increases in CO 2 levels

23 All models predict that it will get warmer

24 We are performing an experiment on our atmosphere. What the outcome will be we don’t yet know


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