Earth’s Energy Budget Lesson Plan 2 – Day 2. Bell Work: We know that if the Sun kept inputting energy and it didn't go anywhere, then we would eventually.
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Presentation on theme: "Earth’s Energy Budget Lesson Plan 2 – Day 2. Bell Work: We know that if the Sun kept inputting energy and it didn't go anywhere, then we would eventually."— Presentation transcript:
Radiation Energy in the form of invisible waves or rays All objects emit (give- off) radiation. The amount and wavelength range is dependent on the temperature of the object.
Objects Radiate Heat Earth absorbs and re-radiates energy In Earth’s Energy Budget, all of Earth is considered together – Air (Atmosphere) – Land (Lithosphere) – Ice (Cryosphere) – Ocean/Water (Hydrosphere) – Life (Biosphere)
Radiation If energy is absorbed by an object (rocks, water, building), then the temperature of that object increases. As the temperature increases (hotter), the peak wavelength emitted by the object decreases (becomes shorter wavelengths).
What can you say about re-radiated heat from the Earth? It comes in a range of LONG wavelengths
Sun emits radiation Earth intercepts sunlight Input = Sunlight on one side of Earth Output = absorbed and re-radiated 30% is reflected
Another variable in Energy Budget A small part of the atmosphere is made of heat-trapping gases. These gases absorb long wave radiation. They are called greenhouse gases. Examples: Water Vapor (H 2 O), Carbon Dioxide (CO 2 )