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Cheat Sheet: Energy Matter And Life

1. Earth as a System: Energy, Matter, and Life

1.1 Earth System and Spheres

SphereDefinition
GeosphereSolid rocks, soil, landforms and the Earth's interior
HydrosphereLiquid water including oceans, rivers, lakes and groundwater
CryosphereSolid water forms such as glaciers, snow and polar ice caps
AtmosphereAir surrounding Earth held by gravity
BiosphereAll living organisms and their environments

1.2 Solar Energy and Electromagnetic Radiation

TermDefinition / Value
Primary energy sourceThe Sun
Speed of electromagnetic waves3 × 10^8 m/s
Electromagnetic spectrumRange of EM radiation; most solar energy reaching Earth is in UV, visible and IR (~99%)
High-frequency EMGamma rays and X-rays; high energy; harmful
Low-frequency EMInfrared and radio waves; lower energy
Ultraviolet (UV) range100 nm-400 nm
Visible lightReaches surface and provides energy for photosynthesis
Infrared (IR)Heats Earth's surface; surface emits IR back to atmosphere
InsolationAmount of solar radiation reaching Earth's surface
Solar constant≈1.4 kW/m² (≈1400 J/s/m²) at top of atmosphere perpendicular to Sun's rays
Maximum surface insolation≈1 kW/m² under clear skies
Anna ManiMapped solar insolation across India (1950s); published Solar Radiation Over India (1981)

1.3 Interaction of Solar Radiation on Earth's Surface

TermDefinition
AlbedoFraction of solar radiation reflected by a surface (Latin: whiteness)
MaterialAlbedo
Snow0.80-0.90
Ice0.50-0.70
Crushed rock0.25-0.30
  • Dark surfaces absorb more sunlight; light surfaces reflect more and remain cooler
  • Urban heat island effect: built materials absorb and retain heat, raising city temperatures relative to rural areas

1.4 Latitude and Earth's Shape

  • Sunlight concentrated at equator; spread over larger area at poles
  • Uneven heating causes temperature differences between equator and poles
  • Axial tilt and Earth's shape produce seasons and varying day lengths
  • Uneven insolation drives global winds and ocean currents

1.5 Role and Structure of the Atmosphere

CompositionNitrogen 78%; Oxygen 21%; small amounts of argon, carbon dioxide, water vapor and other gases
LayerApproximate altitudes and features
Troposphere0-12 km; weather formation; heated by Earth's surface; temperature decreases with height (~6.5 °C/km); thickest over equator, thinnest over poles
Stratosphere12-50 km; contains ozone layer that absorbs UV; temperature increases with height; restricts vertical mixing
MesosphereAbove stratosphere; minor role in climate
ThermosphereAbove mesosphere; minor role in climate
ExosphereOutermost layer; minor role in climate
  • Atmosphere partly absorbs incoming solar radiation (ozone blocks harmful UV)
  • Atmosphere traps outgoing heat via greenhouse effect, keeping Earth warm enough for life
  • Outer space begins at about 100 km above Earth

2. Uneven Heating Causes Wind and Ocean Currents

2.1 Local Winds

  • Valley breeze (daytime): mountain slopes heat faster than valley floor; warm air rises along slopes; cooler valley air moves up
  • Mountain breeze (after sunset): slopes cool faster; cooler dense air flows down into the valley

2.2 Planetary Winds

  • Equatorial low: warm air rises near equator and moves poleward aloft
  • Sub-tropical highs (~30° N/S): sinking cooled air creates high pressure belts
  • Sub-polar lows (~60° N/S): rising air where polar and mid-latitude air converge
  • Polar highs (~90° N/S): cold sinking air produces polar high pressure belts
  • Coriolis effect: winds curve to the right in Northern Hemisphere and to the left in Southern Hemisphere

2.3 Ocean Currents

TermDefinition / Role
Ocean currentsContinuous movement of large water masses driven by winds, temperature and salinity differences, Earth's rotation and land mass layout
  • Temperature and salinity: warm equatorial waters move poleward at surface; cold denser waters return toward equator at depth
  • Low salinity water stays near surface; high salinity water sinks
  • Gyres: large circular current patterns; clockwise in Northern Hemisphere; counterclockwise in Southern Hemisphere
  • Role: redistribute heat from equator to poles and transport nutrients, regulating climate and supporting marine ecosystems
  • North Atlantic Drift: carries warm water from the southern North American east coast to northwestern Europe, keeping many ports ice-free in winter

3. Biogeochemical Cycles

3.1 Water Cycle

ComponentsProcesses
Key processesEvaporation; Transpiration; Condensation; Precipitation; Infiltration; Groundwater
  • Process sequence: evaporation from water bodies → condensation to clouds → precipitation → surface flow back to oceans → infiltration into ground
  • Water dissolves minerals during movement, transporting nutrients to terrestrial and marine organisms
  • Climate change effects: warmer atmosphere holds more moisture, causing heavier rainfall in some regions and droughts in others
  • Melting glaciers increase river water and sea level, threatening coastal cities such as Mumbai and Chennai
  • Intense rainfall increases runoff and soil erosion
  • Reduced infiltration decreases groundwater recharge and complicates agriculture during dry periods
  • Water cycle links cryosphere, hydrosphere, atmosphere, geosphere and biosphere; all affected by global warming

3.2 Carbon Cycle

AspectDetails
ReservoirsAtmosphere (CO₂); Biosphere (plants, animals); Geosphere (carbonate rocks, fossil fuels); Hydrosphere (dissolved CO₂ and marine shells)
Fast cyclePhotosynthesis converts atmospheric CO₂ into glucose; respiration returns CO₂; decomposition returns CO₂ to atmosphere
Slow cycleBurial of organic matter forms fossil fuels; combustion of fossil fuels releases carbon rapidly; ocean exchanges CO₂ forming carbonate and bicarbonate ions used by phytoplankton and shell-building organisms
Human impactAtmospheric CO₂ increased ~35% since 1960 (315 ppm → 420 ppm); excess CO₂ intensifies greenhouse effect, causing global warming, glacier and sea-ice melting and sea-level rise
MitigationExpansion of renewable energy sources reduces carbon released to atmosphere

3.3 Nitrogen Cycle

StepAgent / Description
Nitrogen fixationRhizobium (root nodules of legumes) and Azotobacter (soil) convert N₂ to ammonia (NH₃)
NitrificationNitrosomonas converts NH₃ → NO₂⁻; Nitrobacter converts NO₂⁻ → NO₃⁻
AssimilationPlants absorb nitrogen compounds from soil; animals obtain nitrogen by consuming plants or other animals
AmmonificationDecomposers (bacteria and fungi) break organic matter, returning ammonia to soil
DenitrificationPseudomonas converts nitrates back into N₂ gas
Other inputLightning produces nitrogen oxides contributing to fixation
Industrial fixationHaber-Bosch process (early 1900s) produces ammonia for fertilisers; process uses ~1-2% of global energy and has led to extensive fertiliser use

3.4 Oxygen Cycle

AspectDetails
Atmospheric fractionOxygen ≈21% of the atmosphere
FormsFree O₂ gas and combined forms in crust as metal oxides and minerals; oxygen also present in CO₂
Regulating processesRespiration and combustion consume O₂ and release CO₂; photosynthesis produces O₂ from CO₂, water and sunlight

4. Human Impact on Earth's Processes

4.1 Carbon and Ocean Impacts

  • Burning fossil fuels and deforestation raise atmospheric CO₂, intensifying the greenhouse effect and causing extreme weather and biodiversity loss
  • Increased atmospheric CO₂ leads to greater ocean CO₂ absorption, causing ocean acidification that threatens plankton and coral reefs
  • Warmer ocean water reduces the ocean's capacity to absorb CO₂
  • Natural carbon sinks (forests and oceans) become saturated by continued emissions

4.2 Nitrogen and Water Impacts

  • Overuse of fertilisers adds excessive nitrates to rivers and lakes causing eutrophication and fish kills

4.3 Land Use, Air Pollution and Restoration Steps

  • Deforestation reduces photosynthesis and transpiration, can decrease local rainfall, alters surface albedo, increases soil erosion and destroys habitats causing biodiversity decline
  • Vehicular emissions react with sunlight to form ground-level smog and ground-level ozone, which is harmful to health
  • Montreal Protocol initiated ozone-layer recovery by reducing CFCs
  • Kyoto Protocol and Paris Agreement aimed to reduce CO₂ emissions but have been less successful
  • Restoration measures: conserve energy; switch to renewable energy (solar, wind); plant trees; save water; practice sustainable farming
  • India actions: large-scale tree planting and expansion of solar and renewable energy; Mission LiFE introduced at the UN Climate Change Conference in 2021 to promote mindful, eco-friendly lifestyles
The document Cheat Sheet: Energy Matter And Life is a part of the Class 9 Course Science Class 9 New NCERT 2026-27 (New Syllabus).
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