Ms. Terkper's Digital Classroom

Energy Flow in Global Systems — Ms. Terkper's Digital Classroom
Science 10 Units
Unit A: Chemistry Unit B: Physics Unit C: Biology Unit D: Biosphere
Energy Flow in Global Systems — Unit D
Overview Solar Energy Global Transfer Heat Calculations Biomes Climate Change Practice
Alberta Science 10 — Unit D

Energy Flow in Global Systems

Ms. Terkper's Digital Classroom — Social and Environmental Contexts Emphasis

Focusing Questions

"Are there relationships between solar energy, global energy transfer processes, climate and biomes? What evidence suggests our climate may be changing more rapidly than living species can adapt? Is human activity causing climate change? How can we reduce our impact on the biosphere and on global climate, while still meeting human needs?"

Program Outcomes

Outcome 1: Describe how solar energy input, terrestrial energy output and energy flow within the biosphere affect humans and other species.
Outcome 2: Analyze the relationships among net solar energy, global energy transfer processes (radiation, convection, hydrologic cycle) and climate.
Outcome 3: Relate climate to the characteristics of the world's major biomes and compare biomes in different regions.
Outcome 4: Investigate and interpret the role of environmental factors on global energy transfer and climate change.

Key Concepts

Solar Radiation Budget Greenhouse Effect Climate Zones Coriolis Effect Hydrologic Cycle Albedo 6 Major Biomes Heat Transfer (Q = mcΔt) Human Activity & Climate IPCC

Unit Overview

Solar energy sustains all life on Earth and drives global climate systems. The absorption and transfer of thermal energy at and near Earth's surface produces climate zones and biomes. The IPCC states the balance of evidence suggests a human influence on global climate, and scientists are studying the potential impact on biomes.

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Solar Energy & Earth's Energy Systems

Earth's Major Spheres

Atmosphere

Layer of gases surrounding Earth. Contains N2 (78%), O2 (21%), Ar, CO2, H2O vapor, and trace greenhouse gases. Layers: troposphere, stratosphere, mesosphere, thermosphere.

Hydrosphere

All water on Earth: oceans (~97%), ice caps and glaciers (~2%), freshwater lakes, rivers, groundwater. Oceans cover ~71% of Earth's surface. Stores and transports thermal energy.

Lithosphere

Solid outer layer of Earth including the crust and upper mantle. Contains rocks, soil, and minerals. Influences climate through topography, mountain ranges, and land surface albedo.

Biosphere

The zone of life on Earth — all ecosystems from ocean floor to mountain tops. Depends on inputs from all other spheres. Interacts with climate through respiration, photosynthesis and transpiration.

Solar Radiation Budget — What Happens to 100% of Incoming Solar Energy?
Total solar energy incoming
100%
Shortwave radiation from the Sun
Reflected by clouds & aerosols
21%
Scattered back to space
Reflected by Earth's surface
9%
Albedo of land and ice
Absorbed by atmosphere
20%
By ozone, H2O vapor, clouds
Absorbed by Earth's surface
50%
Heats land, water; drives weather
Re-emitted as infrared (longwave)
~70%
Terrestrial radiation back to space
Net radiant energy (absorbed)
~30%
Net surplus that drives climate systems
The Greenhouse Effect

The greenhouse effect is the process by which greenhouse gases in the atmosphere trap outgoing infrared (longwave) radiation from Earth's surface, warming the planet.

1
Shortwave solar radiation passes through the atmosphere and is absorbed by Earth's surface.
2
Earth's surface re-emits energy as longwave infrared radiation (heat).
3
Greenhouse gases (CO2, CH4, H2O vapour, N2O) absorb this outgoing radiation.
4
Some energy is re-radiated back toward Earth's surface, warming it further.

Natural vs Enhanced Greenhouse Effect

The natural greenhouse effect keeps Earth ~33°C warmer than it would otherwise be. The enhanced greenhouse effect is caused by human activity increasing greenhouse gas concentrations, leading to additional warming beyond the natural baseline.

Key Greenhouse Gases
GasFormulaSourceWarming Potential
Water VapourH2OEvaporationNatural; ~50% of total GH effect
Carbon DioxideCO2Combustion, deforestationGWP = 1 (reference)
MethaneCH4Livestock, landfills, wetlandsGWP = 28–36 (over 100 yr)
Nitrous OxideN2OFertilizers, combustionGWP = ~265
OzoneO3Chemical reactions in atm.Complex; also shields UV
Greenhouse Gas Effect Simulator
Estimated Avg Surface Temp
+15.0°C
Current atmospheric conditions. Pre-industrial average temperature was approximately +14.0°C.
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Global Energy Transfer Processes

Factors Affecting Solar Energy at Earth's Surface

  • Angle of inclination: Low-angle sunlight is spread over a larger area, delivering less energy per m² (explains why poles are cooler)
  • Length of daylight: More hours of sunlight = more energy absorbed (seasons)
  • Cloud cover: Clouds reflect incoming shortwave radiation; also trap outgoing infrared
  • Albedo: Fraction of solar energy reflected; snow/ice high (~80%), ocean low (~6%)
  • Aerosols & particulates: Volcanic ash and pollution scatter and absorb radiation

The Hydrologic Cycle

The continuous movement of water through the Earth's systems. Transfers enormous amounts of thermal energy through phase changes (evaporation, condensation, melting, freezing).

Evaporation
Liquid → gas; absorbs energy
Condensation
Gas → liquid; releases energy
Precipitation
Rain, snow, sleet, hail
Runoff
Water flows back to oceans

Global Wind Patterns

90°NNorth PolePolar High
60°NPolar Front (Low pressure)Westerlies (SW)
60–30°NPrevailing WesterliesBlow W to E
30°NSubtropical High (Horse Latitudes)Calm / dry
30–0°NTrade Winds (NE)Blow NE to SW
Intertropical Convergence Zone (ITCZ)Calm / rainy
0–30°STrade Winds (SE)Blow SE to NW
30°SSubtropical HighCalm / dry
60–30°SPrevailing WesterliesBlow W to E
90°SSouth PolePolar High

Coriolis Effect

Earth's rotation deflects moving air and water to the right in the Northern Hemisphere and to the left in the Southern Hemisphere. This creates the curved paths of winds and ocean currents. It also causes cyclones to rotate counterclockwise in the Northern Hemisphere.

Albedo — Surface Reflectivity Explorer

Click a surface type to see its albedo (reflectivity) and relative contribution to heating or cooling. Higher albedo = more reflection = less warming.

Fresh Snow
Albedo: ~80%
Ice / Glacier
Albedo: ~60%
Desert Sand
Albedo: ~25%
Forest
Albedo: ~15%
Open Ocean
Albedo: ~8%
Grassland
Albedo: ~20%
Dark Pavement
Albedo: ~12%
White Roof
Albedo: ~70%
Fresh SnowFresh snow reflects up to 80% of incoming solar radiation. This is why Arctic and Antarctic regions stay cold — most solar energy is reflected away.
Absorbed: 20%
Reflected: 80%
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Heat Transfer Calculations

Q = mcΔt
Q = heat (J)  |  m = mass (g)  |  c = specific heat capacity  |  Δt = temp change (°C)
Hfus = Q / n
Hfus = heat of fusion (kJ/mol)  |  Q = heat (kJ)  |  n = moles
Hvap = Q / n
Hvap = heat of vaporization (kJ/mol)  |  Water: 40.7 kJ/mol
Specific Heat Capacity Reference Values
Substancec (J/g·°C)Significance
Water (liquid)4.18Very high c — oceans act as a giant heat buffer, moderating coastal climates
Ice2.09Lower than liquid water; glaciers warm faster than oceans
Steam (water vapour)2.01Important in atmospheric energy transfer
Dry Air1.01Low c — air heats and cools quickly over land
Sand / Soil~0.84Very low c — deserts have extreme temperature swings day/night
Granite (rock)0.79Rocks heat and cool rapidly; amplifies temperature range in continents

Why Water Has Such High Specific Heat

Water molecules form strong hydrogen bonds. A large amount of energy is needed to break these bonds and increase temperature. This makes water an excellent thermal buffer — oceans and large lakes resist large temperature changes, which is why coastal cities have milder climates than inland cities at the same latitude.

Key Values for Water:
  • Hfus = 6.01 kJ/mol (melting ice at 0°C)
  • Hvap = 40.7 kJ/mol (boiling water at 100°C)
  • c(liquid) = 4.18 J/g·°C

Sensible Heat Calculator

Q = mcΔt  —  Calculate the heat energy absorbed or released when temperature changes.
Heat Energy (Q)
104,500
Joules (J)
Q = 500 g × 4.18 J/g·°C × 50°C = 104,500 J

Heat of Fusion

Q = n × Hfus  —  Energy to melt (or freeze) ice at 0°C. Hfus(water) = 6.01 kJ/mol. Molar mass of water = 18.02 g/mol.
Moles of water
5.55
mol
n = 100 / 18.02 = 5.55 mol
Heat required (Q)
33.4
kJ
Q = 5.55 × 6.01 = 33.4 kJ

Heat of Vaporization

Q = n × Hvap  —  Energy to boil (or condense) water at 100°C. Hvap(water) = 40.7 kJ/mol. Note: vaporization requires ~6.8× more energy than fusion!
Moles of water
11.10
mol
n = 200 / 18.02 = 11.10 mol
Heat required (Q)
451.8
kJ
Q = 11.10 × 40.7 = 451.8 kJ
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World's Major Biomes

A biome is an open system characterized by specific climatic conditions (temperature, precipitation, sunlight, wind) and topography. Biomes with similar characteristics can exist at similar latitudes anywhere in the world.

Alberta Connection

Alberta spans multiple biomes: the southern prairies are grassland, the northern half of the province transitions through taiga (boreal forest), and the Rocky Mountains create alpine tundra at high elevations. Climate change is already impacting all three of these biomes in Alberta, with particular concern for the shrinking of glaciers in the Rockies and permafrost thaw in the north.

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Human Activity & Climate Change

Human Actions Affecting Climate
1
Greenhouse gas emissions: Burning fossil fuels releases CO2; agriculture and landfills release CH4 and N2O. Concentrations rising rapidly since industrialization.
2
Deforestation: Removes CO2-absorbing forests. Replaces dark canopy with lighter cleared land, increasing albedo but eliminating carbon storage and evapotranspiration cooling.
3
Draining of wetlands: Wetlands store vast amounts of carbon. When drained, decomposition releases stored CO2 and CH4 rapidly.
4
Forest fires: Both natural and human-caused fires release stored carbon. Increasingly severe fire seasons due to warming create a positive feedback loop.
5
Urban expansion: Replaces natural surfaces with low-albedo pavement and buildings, creating urban heat islands.
Evidence for Past & Current Climate Change
Evidence TypeHow It WorksWhat It Shows
Ice Core SamplesAir bubbles trapped in ancient ice preserve samples of past atmospheresCO2 and temperature data going back 800,000 years; clear correlation
Tree Ring Analysis (Dendrochronology)Width and density of annual growth rings records climate conditionsDrought periods, temperature anomalies, past centuries of climate
Coral RecordsCoral skeletons record ocean temperature and chemistrySea surface temperatures and acidification over centuries
Sediment CoresLake and ocean bottom sediments preserve pollen and organismsPast vegetation and climate conditions
Satellite ImagingContinuous monitoring of ice extent, vegetation, sea levelMeasurable shrinkage of Arctic ice pack; rising sea levels

High-Risk Impacts

  • Arctic ice pack reduction — loss of polar bear habitat; impacts Inuit communities' traditional lifestyle and food security
  • Permafrost thaw — releases CH4; destabilizes infrastructure in northern communities
  • Rising sea levels — threatens coastal cities and low-lying nations
  • Coral reef bleaching — ocean warming and acidification
  • Increased extreme weather events (droughts, floods, heat waves)

Moderate-Risk Impacts

  • Shifts in biome boundaries as temperature zones move poleward
  • Changes to Alberta's agriculture seasons and crop suitability zones
  • Altered precipitation patterns; changing river flows
  • Species range shifts; mismatched migration/bloom timing

Multiple Perspectives on Climate Action

Gaia Hypothesis (James Lovelock, 1970s): Earth acts as a self-regulating system — living organisms interact with their inorganic environment to maintain conditions suitable for life.

Traditional Aboriginal Perspectives: Indigenous worldviews have long emphasized relational thinking — humans are part of the natural world, not separate from it. Practices of stewardship and reciprocity with the land are seen as responsibilities, not choices.

International Scientific Programs & Organizations
Organization / ProgramRole
IPCC — Intergovernmental Panel on Climate ChangeReviews and synthesizes global climate research; publishes assessment reports used by governments worldwide for policy decisions
WMO — World Meteorological OrganizationCoordinates global network of weather and climate observation; produces international weather standards
World Weather WatchGlobal system of weather observation, analysis and forecasting using satellites, ground stations and ocean buoys
Global Atmosphere Watch (GAW)Monitors greenhouse gases, ozone, aerosols and acid rain globally; provides long-term data trends
SHEBA ProjectSurface Heat Budget of the Arctic Ocean — studied how solar energy is absorbed by Arctic ice and open water; critical for understanding ice-albedo feedback
Paleoclimate ResearchStudies past climate using ice cores, sediments, tree rings; provides context for current changes and validates climate models
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Interactive Practice & Quizzes

Knowledge Check Quiz

Test your understanding of global energy systems, biomes and climate change.

Global Systems — Science 10

Question 1 of 10 0 / 0

Biome Characteristics Match

Match each biome on the left with its key characteristic on the right.

0 of 6 matched

Vocabulary Flashcards

Click card to flip. Use arrows to navigate all 20 terms.

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