Atmosphere and Weather

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Presentation transcript:

Atmosphere and Weather

Earth’s Atmosphere Atmosphere is the gas surrounding Earth (or any planet) The atmosphere today: ~78% Nitrogen (N2) ~21% oxygen (O2) ~1% all other gases The atmosphere did not always look like this, and was quite different while Earth was young

Earth’s Ancient Atmosphere Earth’s early atmosphere had little to no gaseous O2 It was mostly dominated by Hydrogen (H2)and Helium (H) Volcanoes began to spew gases like carbon dioxide (CO2), Ammonia (NH3), and Methane (CH4) This early atmosphere was known as the reduced atmosphere We know that there was no O2 because it would have caused the ancient iron rocks to rust, but no rust was found

Development of current atmosphere Early organisms (plants, protists, bacteria) absorbed the CO2 and produced O2 through biochemical cycles Photosynthesis being the primary one This also explains why the CO2 content of the current atmosphere is so low It is now an oxidizing atmosphere

Atmosphere basics Layers of the atmosphere: Troposphere Stratosphere Closest to the ground Where weather occurs 0-10km above ground Stratosphere Contains the ozone later 10-50 km above ground Mesosphere 50-100 km above ground Thermosphere Can be over 1000oC (1832oF) 100-500 km above ground Exosphere Outer space

Atmosphere and Weather Weather is the short-term variations in the atmosphere Caused by 3 main factors: Temperature Air Pressure Humidity

Temperature and Heating Earth SI unit is degrees Celsius Water freezes at 0oC and 32of Water boils at 100oC and 212oF Temperature vs. heat Temperature is the average amount of molecule movement Heat is the total amount of molecule movement Ex. Even though the Atlantic ocean is cold (low temperature), it has so much more mass that it has much more heat contained in it An oven is very hot to the touch because it has high temperature, but because it’s not as big as the ocean it has FAR less heat

Temperature and Heating Earth Transfer of heat Radiation is the transfer of energy through electromagnetic waves Conduction is transfer of energy through direct contact Convection is the transfer of energy through moving air or water As air or water is heated, it rises and the cooler air/water falls, creating loops of moving air/water

Temperature and Heating Earth

Temperature and Heating Earth The sun radiating energy to Earth transfers the energy driving weather patterns This transfer of energy is not equal among all of the earth at all times Depending on the angle the sun hits a part of the earth, it may transfer a lot of heat or very little This creates imbalances in the temperatures of different locations, and therefore imbalances of air pressure The re-balancing of these temperatures and pressures produces weather

Temperature and Heating Earth The more direct the sunlight, the more energy is transferred

Air Pressure Differences in air pressure cause wind Air pressure makes an enormous impact on weather forecasting The SI unit for air pressure is the Pascal (Pa) Since these are so tiny, usually air pressure is communicated in millibars. 1 millibar=10 pascals It is measured using a barometer Earliest types had atmospheric pressure pushing down on a dish of liquid mercury, which then pushes upward through a tube

Air Pressure Pressure/temperature/density relationship The higher the temperature, the less dense things are and the more they expand (ex. roasting marshmallows or hot dogs) If you have the system closed off (for example, a closed soda bottle), then increasing the heat will also increase the pressure Because the atmosphere closes off Earth, whenever a part gets heated it increases the pressure in that part

Humidity This is the amount of water vapor in the atmosphere at a given spot The air can only hold so much water at a given time If there’s more water than the air can hold, the air is saturated More humidity allows for more heat to be transferred through the air This is why lower temperatures and high humidity feels hotter than “dry heat” with little humidity and higher temperatures

Humidity When water turns from water vapor back into liquid water, that’s condensation Warm air can hold more water than cooler air without the water condensing back into liquid The temperature where the air becomes saturated is the dew point Condensation in the troposphere creates clouds The warm air from the surface rises, cools, and condenses high above the ground

Humidity The water molecules join around particles in the air like the picture above When the water condenses from the clouds and falls to the ground it’s called precipitation Coalescence is when the molecules group up into bigger and bigger droplets/snowflakes/hail pieces In severe weather the wind can create so much coalescence hailstones the size of baseballs can fall

Humidity

Air Masses and Fronts Air masses are large volumes of air that share similar temperature, humidity, and pressure They tend to move around a lot Because Earth is always spinning, when these masses move they don’t move in straight lines This curved movement is called the coriolis effect

Air Masses and Fronts

Air Masses and Fronts When two air masses collide it’s called a front Whichever mass is moving faster gives the front it’s name Cold fronts replace warm air with cold air and forces the warm air up Warm fronts replace cool air with warm air and rise above them Stationary fronts happen when 2 fronts collide and don’t go anywhere Occluded fronts push warm air up between 2 cooler air masses