Midterm Flashcards
what factors does Earth’s surface temperature depend on?
- Radiation from the sun
- Earth’s reflectivity (albedo, 30%)
- Warming provided by shifts in atmospheric composition (greenhouse effect)
What is radiation from the sun?
Radiation from the sun is essentially energy that travels through space and reaches the Earth in the form of light and heat. This energy is crucial for life on Earth, as it provides warmth and powers photosynthesis in plants.
When this radiation hits the Earth’s surface, it warms it. However, not all of this energy stays on the surface. Some is absorbed and some is reflected back into space. The absorbed energy heats the Earth and is eventually re-radiated back into the atmosphere as infrared radiation, or heat.
What is Earth’s reflectivity (albedo)?
Earth’s reflectivity, or albedo, is basically how much of the Sun’s light is reflected back into space without being absorbed. You can think of it like wearing a white shirt on a sunny day; the shirt reflects most of the sunlight and keeps you cooler compared to a dark shirt, which absorbs more light and makes you feel warmer.
The Earth’s surface has different colors and textures, like oceans, forests, ice caps, and deserts, each with its own albedo. Snow and ice, for instance, are very good at reflecting sunlight, which helps keep those areas cooler. Darker surfaces like oceans or forests absorb more sunlight and get warmer.
What is warming provided by shifts in atmospheric composition (greenhouse effect)?
The warming provided by shifts in atmospheric composition, also known as the greenhouse effect, is like wrapping a blanket around Earth. Our atmosphere has gases in it, called greenhouse gases, which include carbon dioxide, methane, and water vapor, among others. These gases act like the glass of a greenhouse, letting sunlight in to warm the Earth’s surface but then trapping some of the heat as it tries to escape back into space.
When the composition of the atmosphere changes, like when there are more greenhouse gases, the ‘blanket’ gets thicker. A thicker blanket means less heat can escape, which makes the Earth’s surface warmer over time.
what are the main atmospheric components?
N2 (78.08% by volume),
O2 (20.95%),
water vapor (concentration is highly variable, from 0% to 4%),
trace amounts of CO2, O3, and other gases,
aerosols
what are the aerosols?
Aerosols are tiny particles or droplets that are so small they can float in the air. Imagine when you use a spray can, the fine mist that comes out is similar to aerosols. These can be made of different things like dust, sea salts, volcanic ash, smoke from fires, and even tiny droplets from spray cans.
Aerosols are important because they can affect the weather and climate. For example, they can help clouds form; the water droplets in clouds actually form around these tiny particles. They can also reflect sunlight back into space, which can cool down the Earth’s surface. However, some aerosols can absorb heat and make the atmosphere warmer.
what is the water vapor?
Water vapor is just water in its gas form. It’s what you see when you boil water and steam comes up, or the invisible moisture in the air when it feels really humid. Water vapor is also created when the Sun heats up water from oceans, lakes, and rivers, and it turns into an invisible gas that goes up into the sky.
what are trace amounts of CO2, O3 and other gases?
CO2, or carbon dioxide, is one of these trace gases. Even though it’s only a small part of the atmosphere, it has a big job: it traps heat from the sun, which helps keep the Earth warm enough for us to live. This is part of the greenhouse effect.
O3, or ozone, is another trace gas. Ozone high up in the atmosphere acts like sunscreen for the Earth, protecting us from too much harmful ultraviolet (UV) light from the sun.
What are variables and increasing gases in the last couple of years?
Nitrogen and oxygen concentrations experience little change, but carbon dioxide, methane, nitrous oxides, and chlorofluorocarbons are greenhouse gases experiencing discernable increases in concentration.
What is Planetary albedo for Earth?
30%
what makes contribution into planetary albedo?
Clouds (20%): This means that clouds are responsible for reflecting 20% of the total sunlight that bounces back into space. Clouds can be very reflective, especially thick, fluffy ones, and they cover a large part of the Earth at any given time.
Earth’s Surface (4%): This is telling us that the actual ground, water, ice, and other surfaces of the Earth reflect about 4% of the sunlight that hits them back into space. Different surfaces have different reflectivities; for instance, ice and snow are highly reflective (high albedo), while forests and oceans are much less so (low albedo).
Scattering by Air Molecules (6%): The remaining 6% of the reflected sunlight is scattered back into space by the tiny molecules that make up Earth’s atmosphere. This is the light that gets bounced off in different directions as it hits the gases in the air, and some of it escapes back into space.
Provide examples of albedo
Fresh snow (75-95%)
Clouds (30-90%)
Ice (30-40%)
Grassy fields (10-30%)
water (10%)
forest (3-10%)
What are Milankovic cycles?
Milankovitch cycles are like Earth’s dance moves around the Sun, which change slowly over thousands of years and affect how much sunlight different parts of our planet receive.
What three main types of Milankoovic cycles?
- Orbit eccentricity - Earth’s orbit around the Sun isn’t a perfect circle, it’s more like an ellipse. About every 100,000 years, the shape of this orbit stretches out a bit and then becomes more circular again. When the orbit is more stretched, there’s a bigger difference in the amount of sunlight we get when we’re closer to the Sun versus when we’re farther away.
- Axial tilt - Earth is tilted on its axis. This tilt changes between more tilted and less tilted about every 41,000 years. The more the Earth is tilted, the more extreme our seasons are because the Sun’s light hits different parts more directly or more at an angle.
- Axial precession - Earth also wobbles like a spinning top. This wobble changes the direction Earth’s axis is pointing and cycles about every 26,000 years. This wobble can affect when in its orbit Earth experiences the seasons.
Does Milankovic cycle is the reason of today’s climate change?
No
What are the astronomical causes of climate change?
11-year and 206-year cycles: These are periods when the amount of sunspots (dark spots on the sun that are cooler than other parts) increases or decreases. Sunspots are associated with solar activity, which can affect the amount of energy the Earth receives from the Sun.
21,000-year cycle: This is about the wobble in the way Earth spins on its axis and the shape of its orbit around the Sun. It changes how sunlight is distributed on Earth’s surface, which can lead to climate changes over long periods.
41,000-year cycle: This refers to the slight changes in how much Earth is tilted on its axis. A greater tilt means more extreme seasons, and a smaller tilt means milder seasons.
100,000-year cycle: This is about changes in the shape of Earth’s orbit from more circular to more elongated and back again, which affects how much sunlight Earth gets.
Asteroid impacts: When a large asteroid hits Earth, it can throw up a lot of dust and particles into the air, blocking sunlight and causing the climate to change.
What are the atmospheric causes of climate change?
Heat retention (Greenhouse effect): Gases like water vapor (as a gas, not droplets), carbon dioxide, and methane trap heat in the Earth’s atmosphere, which keeps the planet warmer than it would be otherwise.
Solar reflectivity: Things like clouds, volcanic ash, and ice caps can reflect sunlight away from Earth, which can cool down the planet’s surface.
What are the tectonic causes of climate change?
Landmass distribution (Continental drift): Continents move around on Earth’s surface over millions of years. When there’s a large landmass at one of the poles, it can lead to the formation of ice caps and ice ages.
Undersea ridge activity (Sea floor spreading): This is when the ocean floors spread apart, creating more space on the ocean floor. This can change the volume of the oceans and affect the flow of ocean currents, which in turn can impact the climate.
What is effective radiative forcing (ERF)?
This is a fancy term for changes in how much energy from the sun is kept by the Earth versus how much is sent back out into space. Changes in this balance can warm up or cool down the planet.
What is the summary of the change in ERF graph?
Based on the graph you’ve provided, the most effective ERF (Effective Radiative Forcing) from 1750 to 2019 appears to be from carbon dioxide (CO2). This is indicated by the longest bar extending to the right, which shows the greatest positive value in watts per square meter (W/m²). The exact value is not clear without seeing the specific numbers, but it’s evident that CO2 has the largest influence on radiative forcing, contributing to an increase in Earth’s temperature.
The other factors also contribute to ERF but to a lesser extent than CO2. Methane (CH4), nitrous oxide (N2O), and halogenated compounds are significant contributors as well but with shorter bars than CO2, indicating a smaller forcing effect.
Aerosols appear to have a negative forcing (cooling effect), as their bars extend to the left. However, their impact is less than the warming effects of the greenhouse gases.
The total anthropogenic ERF, which is the combined effect of all human-related factors, shows a substantial positive forcing, reinforcing the dominant role of human activities in changing Earth’s climate.