Life on earth - Monelison Middle Schoolmms.amherst.k12.va.us/sites/default/files/Atmosphere chpt...
Transcript of Life on earth - Monelison Middle Schoolmms.amherst.k12.va.us/sites/default/files/Atmosphere chpt...
ATOMOSPHERE
a thin layer of air that forms a protective
covering around the planet
Contains mixture of gases(O2 ), solids (dust,
pollen, salt), and liquids (water vapor)
circulated by winds
What would happen if there was no atmosphere?
Cold nights
Hot days
IMPORTANCE OF THE ATMOSPHERE
1-Balances the amount of heat absorbed and
the amount of heat escaping back to space
This heat comes from the Sun
2-Protects life forms from Sun’s harmful rays
How was it created?
MAKE-UP OF THE ATMOSPHERE
Time line:
Volcanoes producing nitrogen and carbon
dioxide
Cyanobacteria living in ocean photosynthesized
to release oxygen into atmosphere
MAKE-UP OF THE ATMOSPHERE
Time line:
Volcanoes producing nitrogen and carbon
dioxide
Cyanobacteria living in ocean photosynthesized
to release oxygen into atmosphere
Ozone came about from oxygen in atmosphere
MAKE-UP OF THE ATMOSPHERE
Time line:
Volcanoes producing nitrogen and carbon
dioxide
Cyanobacteria living in ocean photosynthesized
to release oxygen into atmosphere
Ozone came about from oxygen in atmosphere
Plants were then protected from Sun and
produced oxygen for respirating organisms
MAKE-UP OF THE ATMOSPHERE
Time line:
Volcanoes producing nitrogen and carbon
dioxide
Cyanobacteria living in ocean photosynthesized
to release oxygen into atmosphere
Ozone came about from oxygen in atmosphere
Plants were then protected from Sun
HOW WE CHANGE THE ATMOSPHERE
Car emissions adds CO2 to the atmosphere
Dangerous b/c CO2 is #1 greenhouse gas
Producing CFCs - chlorofluorocarbons
LAYERS OF THE ATMOSPHERE
characterized by abrupt temperature changes
Temp. changes due to difference in solar
energy absorption
LAYERS OF THE ATMOSPHERE
Troposphere
The inner most layer
Weather, clouds, we are here
Temperature decreases as you go up
Climbing a mountain
Tropopause
Boundary between the troposphere and the stratosphere
Temperature stabilizes
Limits mixing between the two layers
Stratosphere
Ozone layer – global sunscreen
absorbs energy from the sun heating the air
Aircraft flight in lower level
LAYERS OF THE ATMOSPHERE
Mesosphere
Meteoroids start to burn
Ionosphere exists here
Noctilucent clouds
Ionosphere – a layer of electrically charged particles located between the mesosphere and the thermosphere
It allows radio waves to travel across the country to other cities
Thermosphere
Auroras – reaction
between solar wind and
magnetic field where e-
are excited emitting
photons of light
International Space
Station
Exosphere
Region where atoms and molecules can escape
gravity and exit into space
Exosphere is the outer layer
of the atmosphere in which
the space shuttle flies.
Brain Pop Video on Atmosphere
OZONE
Ozone layer – a layer made of oxygen in the
stratosphere that absorbs most of the
ultraviolet radiation from the sun
3 types of suns rays – UVA, UVB, UVC sunglasses block A
and B ozone blocks C
Ultraviolet radiation – one type of energy that
comes to the Earth from the Sun
Causes skin damage and cancer
CFCs
Chlorofluorocarbons – an air pollutant that
destroys the ozone layer composed of Chlorine,
Fluorine, and carbon,
Used in some refrigerators, air conditioners (Freon),
aerosol cans (propellants), foam packaging
Good because non-flammable, odorless, cheap,
nontoxic, non-corrosive
Page 432
THE OZONE HOLE
Ultraviolet radiation breaks down CFCs causing
the depletion of ozone molecules leaving holes
in the ozone layer
THE OZONE HOLE
Sun breaks down CFC creating a free Chlorine atom
That chlorine atom breaks up O3 (ozone) when the
chlorine atom joins with 1 oxygen atom leaving 2
oxygen atoms together
The chlorine and oxygen molecule break up when
come in contact with another free oxygen atom and
the oxygen atoms hook-up
Now that free chlorine atom will find another ozone
molecule to break apart
Air pressure
The weight of the
air/atmosphere above
you causes air pressure.
ATMOSPHERIC PRESSURE
Air density (# of air
molecules in a given space)
is greatest at the surface
and decreases as you go up
Measuring Air Pressure Tool used to measure air pressure is a
barometer.
Air pressure pushes down on the surface of the
mercury in the dish, causing the mercury in the
tube to rise. The air pressure is greater on the
barometer on the right, so the mercury is higher
in the tube.
ENERGY TRANSFER IN THE ATOMOSPHERE
What happens to the heat from the sun?
Absorbed by earth
Reflected by the earth’s surface
Absorbed by atmosphere
Reflected by atmosphere
ENERGY TRANSFER IN THE ATMOSPHERE
Heat flows from high temperatures to low
temperatures
Sun heats earth, earth heats atmosphere
Heat transfers through the atmosphere
in three ways: radiation, conduction,
and convection
RADIATION
energy transferred in the form of rays or waves.
Ex: holding your hand over a stove burner
CONDUCTION
the transfer of energy that occurs when
molecules bump into one another.
Ex: burner warming pot
RADIATION, CONDUCTION, OR CONVECTION?
Popping popcorn on the stove
Popping popcorn in electric popper
Microwave popcorn
What are the molecules doing?
Why does heat rise?
When air is warmed, the molecules move apart and
the air becomes less dense.
Air density decreases because there are fewer
molecules in one space.
What are the air molecules doing?
Why does cold air sink?
cold air molecules move close together becoming
more dense
https://www.youtube.com/watch?v=yUEPGMnRqGs
HYDROLOGIC (WATER) CYCLE
Hydrosphere – a term that describes all the
water on earth’s surface
Evaporation/transpiration – sun’s energy causes water
to change from a liquid to a gas
Precipitation – rain, sleet, snow, hail
Condensation – when the water vapor
cools it changes back into a liquid
AIR MOVEMENT
Radiation from sun is received on Earth in different amounts because its curved
The equator gets more radiation than the poles because the rays are more direct
Warmer less dense air rises and the cooler air falls creating convection currents
CORIOLIS EFFECT
Coriolis effect – causes
moving air to turn left in
the S. Hemisphere and
turn right in the N.
Hemisphere due to
Earth’s rotation
Picture pg. 440, 441
CONVECTION CURRENTS Trade winds – blow to the west as the cooled air flows
back to the equator between 0˚ and 30˚N and S
latitude
Called the trade winds because early sailors used the
patterns to navigate the oceans.
Polar Easterlies – between 60˚N and S latitude
to the N and S poles blow from the east away
from poles
WINDS IN THE UPPER TROPOSPHERE
Jet Stream – narrow
belts of strong winds
that blow near the
troposphere
LOCAL WIND SYSTEMS
Sea breezes- created during
the day because land is
warmed faster than water.
Land breezes – created
during the night because
water cools slower than land