Earth from space with land, oceans and cloud systems visible in a NASA DSCOVR EPIC image.

Earth as a System: Energy, Matter, and Life | Class 9 NCERT Science

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Class 9 Science · NCERT Exploration · Chapter 13

Earth as a System: Energy, Matter, and Life

Earth is made of connected systems. Energy flows through them, matter cycles between them, and a change in one part can affect life in many others.

This visual study guide follows the main ideas of the NCERT Exploration chapter. Use it with the official textbook activities, figures and end-of-chapter questions.

Earth from space with land, oceans and cloud systems visible in a NASA DSCOVR EPIC image
Earth photographed by the NASA/NOAA DSCOVR EPIC camera on July 12, 2026. Source: NASA EPIC archive.

What This Chapter Covers

01 · Earth systems

Five interacting spheres

Geosphere, hydrosphere, cryosphere, atmosphere and biosphere interact continuously.

02 · Energy

Solar radiation and albedo

See how radiation, surface colour and Earth’s shape change the amount of heating.

03 · Movement

Winds and ocean currents

Uneven heating creates pressure differences that move air and water.

04 · Matter

Biogeochemical cycles

Water, carbon, nitrogen and oxygen move through living and non-living systems.

05 · People

Human impact

Learn how land use, pollution and greenhouse-gas emissions can alter Earth systems.

Earth Is an Interconnected System

Energy and matter move between five connected spheres. Their interactions sustain life and shape weather, landforms, water availability and ecosystems. A disturbance in one sphere can produce effects in others.

Earth system GeosphereRocks, soil and land HydrosphereLiquid water AtmosphereAir and gases CryosphereIce and snow BiosphereLife and habitats
The five spheres interact. For example, snowfall (cryosphere) feeds lakes (hydrosphere), which support plants and animals (biosphere).
Key idea: The Earth system is connected, not a collection of isolated parts. Warming sea water can affect evaporation and monsoon rainfall; forest loss can change soil, runoff and river flow.

13.1 Uneven Heating of the Earth

The Sun is Earth’s main energy source. Solar radiation travels through the vacuum of space as electromagnetic waves. Its speed in vacuum is approximately 3 × 108 m/s. Solar radiation reaching Earth is concentrated mainly in ultraviolet (UV), visible and infrared (IR) wavelengths.

UV

Ultraviolet

The ozone layer absorbs much of the harmful ultraviolet radiation. Excess exposure can damage skin and eyes.

Visible

Visible light

Supplies the light used in photosynthesis and contributes to heating Earth’s surface.

Infrared

Infrared

Earth’s warmed surface emits infrared radiation. Greenhouse gases absorb some of this outgoing heat.

Sun Incoming solar radiation Some energy reflected Surface absorbs energy and warms Outgoing infrared heat
Some incoming radiation is reflected or absorbed by the atmosphere and clouds; the surface absorbs some energy and later emits heat.

Insolation, the solar constant and albedo

Insolation is the solar radiation received at Earth’s surface. The solar constant is the average solar power per unit area perpendicular to the Sun’s rays at the top of the atmosphere; NCERT gives an approximate value of 1.4 kW/m². Under clear-sky conditions, surface insolation can be about 1 kW/m².

Albedo is the fraction of incoming solar radiation reflected by a surface. Snow and ice have relatively high albedo and reflect more sunlight; dark surfaces often have lower albedo and absorb more.

SurfaceApproximate albedo from NCERTImplication
Snow0.80–0.90Reflects a large fraction of incoming radiation.
Ice0.50–0.70Reflects more solar radiation than many dark surfaces.
Crushed rock0.25–0.30Reflects a smaller fraction than snow.

Why heating is uneven

Land and water heat at different rates. The Earth’s spherical shape also makes sunlight strike different latitudes at different angles: sunlight is concentrated over a smaller area near the equator and spread over a larger area toward the poles. The atmosphere filters some radiation and helps retain outgoing infrared heat through the greenhouse effect.

Worked example: If insolation is 1 kW/m² over an area of 1 m² for one hour, then energy received is E = intensity × area × time = 1000 × 1 × 3600 = 3.6 × 106 J.

13.2 Uneven Heating Causes Wind and Ocean Currents

Sunlight heats Earth’s surface unevenly. Warm air often rises and produces lower pressure, while cooler, denser air sinks. Air moves from higher pressure toward lower pressure, producing wind. Uneven heating of land and water helps create local breezes; on a larger scale, it helps drive planetary winds and ocean currents.

Local winds

Sea and land breezes

Land heats and cools faster than water, so the direction of the breeze can change between day and night.

Mountain regions

Valley and mountain breezes

During the day, warmed air over sunlit slopes rises and cooler air moves upslope. After sunset, cooler dense air can flow downslope.

Planetary winds

Large-scale circulation

Heating differences between equator and poles create pressure belts; Earth’s rotation deflects moving air.

Ocean currents

Heat transport

Winds and pressure patterns help move ocean water, transporting heat and nutrients and influencing climate.

Ocean currents can reduce temperature differences across regions. In India, changes in sea temperature and atmospheric circulation are important to the southwest monsoon and patterns of rainfall.

Think it through: How might unusually warm Arabian Sea water affect evaporation, cloud formation and the southwest monsoon? Consider how the atmosphere, hydrosphere and biosphere are linked.

13.3 Biogeochemical Cycles

Matter is continuously exchanged between living organisms and non-living parts of Earth. Water, carbon, nitrogen and oxygen cycle between air, water, soil, rocks and organisms, keeping essential materials available to support life.

Water cycle

Water moves between spheres

Evaporation and transpiration add water vapour to the air; condensation forms clouds; precipitation returns water to land and water bodies; runoff and groundwater move it onward.

Carbon cycle

Carbon in living and non-living systems

Photosynthesis takes in carbon dioxide. Respiration and decomposition return carbon to the atmosphere. Over long timescales, carbon can be stored in rocks and fossil fuels; burning fuels releases CO₂.

Nitrogen cycle

Making nitrogen usable

Bacteria convert atmospheric nitrogen into compounds that plants can absorb. Nitrogen passes through food webs and returns to soil and atmosphere through decomposition and denitrification.

Oxygen cycle

Oxygen circulates

Photosynthesis releases oxygen; respiration and combustion use oxygen. These exchanges connect the atmosphere, oceans, land and living organisms.

Water body Condensation Precipitation Evaporation Runoff Transpiration
The water cycle moves water through the atmosphere, land, groundwater, living organisms and water bodies.
Important distinction: Energy flows through Earth systems and is eventually dispersed, while matter is recycled through biogeochemical cycles.

13.4 Human Impact on Earth’s Processes

Human actions can change energy flows and matter cycles. Burning fossil fuels increases carbon dioxide emissions; deforestation reduces vegetation and alters soil, runoff and habitats; air and water pollution can disrupt living systems. Excess nutrient inputs can cause algal blooms, while additional greenhouse gases enhance warming.

Climate

Greenhouse warming

Greenhouse gases absorb some outgoing infrared radiation. More greenhouse gas emissions can intensify warming and disturb climate patterns.

Land and water

Deforestation and runoff

Removing forests can change infiltration, erosion, river flow and the conditions needed by plants and animals.

Air quality

Pollution and ozone

Air pollutants harm health. Ozone in the stratosphere protects life from UV radiation, while ground-level ozone is harmful.

Solutions

Local and global action

Cleaner energy, ecosystem protection and international cooperation can help reduce damage and support recovery.

The chapter’s examples show that Earth-system problems are connected. A change to one sphere may affect weather, water availability, biodiversity, food production and human communities.

Quick Revision

TermRemember
Earth systemFive interacting spheres: geosphere, hydrosphere, cryosphere, atmosphere and biosphere.
AlbedoFraction of incoming solar radiation reflected by a surface.
Solar constantAbout 1.4 kW/m² at the top of Earth’s atmosphere, as stated in NCERT.
InsolationSolar radiation reaching Earth’s surface.
WindAir movement driven by pressure differences, commonly caused by uneven heating.
Biogeochemical cyclesRecycling of matter such as water, carbon, nitrogen and oxygen across Earth spheres.

NCERT-Style Practice Questions

Try each question before revealing the self-check answer.

Q1. Name the five interacting spheres of Earth.

Q2. What is albedo, and why does snow often remain cooler than dark soil?

Q3. How does uneven heating lead to wind?

Q4. Name two processes in the carbon cycle that return carbon dioxide to the atmosphere.

Q5. State two ways human activities can disturb Earth systems.

Q6. Calculate the solar energy received by a 1 m² area in one hour at an intensity of 1 kW/m².

Study tip: Use the original NCERT figures to practise explaining connections between Earth’s spheres. Many questions are easier when you trace how an initial change affects air, water, land and living organisms.

Source alignment: NCERT Class 9 Science, Exploration, Chapter 13, “Earth as a System: Energy, Matter, and Life.” This page is an original study guide and summary; use the official chapter for the textbook’s full activities and exercises.

Open the official NCERT Chapter 13 PDF · Back to Class 9 topics

PhysicsQnA · NCERT Class 9 Science · Chapter 13

Classwork notebook notes

Write in Your Copy: Earth as a System: Energy, Matter, and Life

Suggested notebook notes aligned with the lesson. The Earth system has five interconnected spheres; include labelled diagrams of the spheres and cycles.

Date: __________Subject: ScienceChapter: 13

1. The Five Earth Systems

Earth is an interconnected system in which energy and matter move between living and non-living parts. A change in one sphere may affect the others.

  1. Atmosphere: The layer of gases surrounding Earth.
  2. Hydrosphere: Liquid water in oceans, rivers, lakes and groundwater.
  3. Cryosphere: Frozen water, including glaciers, ice sheets, sea ice and snow.
  4. Geosphere: The solid Earth, including rocks, soil and landforms.
  5. Biosphere: Living organisms and the environments in which they live.

2. Solar Energy, Insolation and Albedo

  • The Sun is Earth’s main external energy source. Solar radiation can travel through the vacuum of space.
  • Insolation: Incoming solar radiation reaching Earth’s surface.
  • Albedo: The fraction of incoming solar radiation reflected by a surface. Snow and ice generally reflect more radiation than darker surfaces.
  • The solar constant is about 1.4 kW/m² at the top of Earth’s atmosphere (approximate textbook value).
  • Earth receives uneven heating because of its shape, the angle of sunlight, season and differences among surfaces.
  • Land heats and cools faster than water. Uneven heating creates temperature and pressure differences that help drive winds and ocean currents.

3. Energy Flow and Greenhouse Effect

Solar radiation warms Earth’s surface. Earth emits energy outward mainly as infrared radiation. Greenhouse gases absorb some outgoing infrared radiation and re-emit it, helping warm the lower atmosphere. Increased greenhouse-gas emissions strengthen this warming effect.

Energy flows through Earth systems, while matter is recycled through natural cycles.

4. Biogeochemical Cycles

  • Water cycle: Evaporation and transpiration → condensation → precipitation → runoff, infiltration and groundwater flow.
  • Carbon cycle: Carbon moves among air, oceans, living things and rocks through photosynthesis, respiration, decomposition, ocean exchange and combustion.
  • Nitrogen cycle: Nitrogen is converted into forms usable by plants, moves through food chains and returns to soil and atmosphere through processes such as decomposition and denitrification.
  • Oxygen cycle: Photosynthesis releases oxygen; respiration, decomposition and combustion use oxygen and return compounds to the environment.

5. Human Impact and Examples of Interconnection

  • Burning fossil fuels increases atmospheric carbon dioxide.
  • Deforestation reduces vegetation and carbon storage and can change runoff, soil and habitats.
  • Air and water pollution affect organisms and ecosystems.
  • Melting ice can change the cryosphere, sea level and ocean properties.
  • Protecting habitats, reducing pollution and using resources carefully can help maintain resilient Earth systems.

6. Solved / Explanation Example

How can deforestation affect more than one sphere? It reduces the biosphere (trees and habitats), can expose the geosphere (soil erosion), may change water movement in the hydrosphere, and reduces carbon uptake from the atmosphere.

7. Classwork Questions

  1. Name the five major Earth spheres and give one example of each.
  2. Define insolation and albedo.
  3. Explain how uneven heating can cause winds and ocean currents.
  4. Describe the water and carbon cycles.
  5. How do greenhouse gases affect Earth’s energy balance?

8. Homework

  1. Draw and label the five Earth spheres and use arrows to show interactions.
  2. Draw the water cycle and label its main stages.
  3. Write one short paragraph on the nitrogen cycle and one on the oxygen cycle.
  4. Describe two human activities that affect Earth systems and one action that can reduce each impact.

Teacher’s check: all five spheres, insolation/albedo definitions, cycle diagrams, and examples of human impact.

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