Earth’s Atmosphere
Chapter 1: Earth’s Changing Atmosphere
Section 1.2: The sun supplies the atmosphere’s
energy.
I. Vocabulary
A. radiation- energy that travels across distances in the form of certain
types of waves
B. conduction- the transfer of heat energy from one substance to another by
direct contact
C. convection- the transfer of energy from place to place by the motion of
a gas or liquid
II. Energy from the sun heats the
atmosphere
A. Two things may happen to the sunlight
that reaches the Earth
1. Sunlight is reflected (this is how you see
things around you)
2. Sunlight is absorbed
B. The sunlight that we see is one type of
radiation
1. About 30% of the solar radiation that
hits the Earth is reflected
a. Clouds, icecaps are white, so they
reflect a lot of light
b. Air reflects light also
2. About 70% of the solar radiation that
hits the Earth is absorbed
a. Oceans, landforms, and living things
absorb most light
b. Absorbed energy heats Earth’s surface
3. Absorption/reflection breakdown
III. The atmosphere moves energy
A. Radiation- sunlight warms the ground
B. Conduction- the warm ground heats the air
C.
Convection- cold, dense air
sinks downward and pushes warm air out of the way; warm air rushes energy
upward
**Differences in density produce the motion of convection (textbook page
19)
IV. The atmosphere has temperature layers
A. Troposphere
1. Layer of the atmosphere nearest to the
Earth’s surface
2. Contains about 80% of the total mass of
the atmosphere, and almost all the water vapor
3. Temperature is highest at ground level
and decreases 6.5o C every km you rise
4. All weather occurs in the troposphere
B. Stratosphere
1. Clear, dry layer sitting above the
troposphere
2. Contains the ozone
layer, which absorbs harmful solar radiation and heats the surrounding air
3. Temperature increases as you go up
C. Mesosphere
1. Layer of extremely thin air above the
stratosphere
2. Contains less than 0.1% of the
atmosphere’s mass
3. Most meteors that enter the
atmosphere burn up here
D. Thermosphere
1. Starts about 56 miles above the Earth’s
surface, atop the mesosphere
2. Grows less and less dense, for many
miles, until it fades to outer space
3. Air high in this layer is very hot
because it absorbs a certain type of solar radiation
4. It would still feel cold to us, though,
since molecules are so spread out
5. Temperature here increases as you rise