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CLASS 8 • SCIENCE • CHAPTER 13

Our Home: Earth, a Unique Life Sustaining Planet

Explore the published notes, key concepts and questions for this chapter.

Quick answer
Earth supports life through liquid water, suitable temperature, atmosphere, gravity, sunlight, protective ozone and magnetic field, and interacting ecosystems. Reproduction maintains life, while climate change, pollution and biodiversity loss threaten it.
Key points
  • Earth is the only planet currently confirmed to support life.
  • Liquid water and suitable temperature are crucial for habitability.
  • Venus is hottest because of its intense greenhouse effect.
  • Gravity helps retain the atmosphere and ozone absorbs harmful UV.
  • Earth's magnetic field deflects many charged solar particles.
  • Atmosphere, hydrosphere, geosphere and biosphere interact.
  • Asexual and sexual reproduction sustain life and produce variation.
  • Climate change, biodiversity loss and pollution form the triple planetary crisis.

Use these notes alongside your current textbook. Check important formulas, worked answers and syllabus coverage with your teacher or official learning material.

Our Home: Earth, a Unique Life Sustaining Planet — NCERT Class 8 Science Chapter 13

Direct answer: Earth supports life because it has liquid water, suitable temperatures, an atmosphere, gravity, sunlight, a protective magnetic field and interconnected ecosystems. Reproduction sustains lineages, while climate change, biodiversity loss and pollution threaten life.

Why is Venus hotter than Mercury? How can a potato sprout without seeds? What would humans need to survive on Mars? These questions connect astronomy, ecology, reproduction and environmental science.

Source: NCERT Curiosity Reprint 2026–27, Chapter 13, printed pages 210–228. All six main sections, three activities and 12 numbered textbook exercises are addressed. Exercise questions are paraphrased; additional practice is original.

Earth's uniqueness

Earth is the only planet confirmed to support life. Its liquid water, suitable temperatures, atmosphere, gravity, magnetic field, sunlight and ecosystems work together. The crust is thin compared with Earth's radius, like the skin of an apple.

Eight planets and greenhouse warming

Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus and Neptune orbit the Sun. The first four are rocky. Jupiter and Saturn are gas giants; Uranus and Neptune are ice giants. Venus is hotter than Mercury because its thick carbon-dioxide atmosphere produces intense greenhouse warming.

13.3.1 Position and habitable zone

The habitable zone is a range of distances where a planet with suitable atmospheric conditions could retain liquid surface water. Distance alone does not prove life exists. Earth is in this zone; Mars may once have had stable surface water, but extraterrestrial life remains unconfirmed.

13.3.2 Size, atmosphere and ozone

Earth's gravity helps retain atmospheric gases. Its atmosphere supports respiration, weather, pressure and heat regulation. Stratospheric ozone absorbs harmful ultraviolet radiation; ground-level ozone can harm health. Earth's seasons arise primarily from axial tilt, not distance from the Sun.

13.3.3 Magnetic field

Movements of conducting liquid metal in Earth's outer core generate its magnetic field. The magnetosphere deflects many charged solar particles, although atmospheric shielding is also important. A vanished magnetic field would increase exposure to space weather, not instantly eliminate all life.

13.4.1 Air, water and sunlight

Photosynthesis uses carbon dioxide, water and sunlight to produce sugars and release oxygen. The atmosphere contains gases; the hydrosphere includes oceans, groundwater, glaciers and vapour. The water cycle transports water between Earth's systems. Greenhouse gases absorb outgoing infrared radiation and help keep Earth warm.

13.4.2 Soil, rocks and minerals

The geosphere includes solid Earth, rocks, soil and minerals. Weathering and organic decay contribute to soil formation. Geodiversity describes the variety of landforms, soils, rocks and geological processes, distinct from biodiversity.

13.4.3 Living things and the biosphere

Plants, animals, fungi and microbes interact with each other and their environments. Producers make food, consumers eat organisms, and decomposers recycle nutrients. The biosphere is Earth's zone of life.

13.4.4 Balance among systems

Forest removal can raise local temperatures, reduce habitats, increase soil erosion and change water runoff. Ecosystem balance is dynamic. Protecting soil, air, water and biodiversity helps maintain life-support systems.

13.5 Reproduction and genes

Reproduction maintains lineages. Genes are hereditary DNA instructions that influence traits. Offspring resemble their parents but genetic recombination and mutations can produce variation. Evolutionary adaptation develops across populations over generations, not through deliberate change in one individual.

13.5.1 Asexual reproduction

Asexual reproduction normally involves one parent without gamete fusion. Potato tuber eyes, ginger rhizomes, sugarcane stems, money-plant cuttings and Bryophyllum leaf buds are examples of vegetative propagation. Hydra reproduces by budding and bacteria can divide by binary fission. Mutations mean offspring are not guaranteed perfectly identical.

13.5.2 Sexual reproduction

Gametes combine at fertilisation to form a zygote. In flowering plants, pollen grains contain cells that produce male gametes and the ovule contains an egg cell; pollination transfers pollen to a stigma. Fertilisation is different from pollination. In frogs, fertilisation often occurs externally; birds and most mammals use internal fertilisation. Birds lay eggs, while most mammals develop embryos internally.

13.6 Threats to life

Climate change, biodiversity loss and pollution form the triple planetary crisis. Fossil-fuel emissions increase greenhouse warming. Habitat destruction reduces biodiversity; pollution damages air, water and soil. The Montreal Protocol addresses ozone-depleting chemicals; the Paris Agreement addresses greenhouse-gas emissions. Cleaner energy, conservation and sustainable resource use help reduce risks.

Tables for revision

Earth systemIncludesImportance
AtmosphereGasesWeather and temperature
HydrosphereWater, ice, vapourWater cycle and life
GeosphereRocks and soilLand and minerals
BiosphereOrganismsFood webs and nutrient cycles
FeatureAsexualSexual
Gamete fusionNoYes
Typical genetic similarityHighVariable
ExamplesPotato, HydraFlowering plants, frogs
PlanetTypeAtmospheric note
MercuryRockyExtremely thin exosphere
VenusRockyThick CO₂, very hot
EarthRockyNitrogen and oxygen
MarsRockyThin CO₂
Jupiter and SaturnGas giantsMostly hydrogen and helium
Uranus and NeptuneIce giantsHydrogen, helium, methane

Activities 13.1–13.3

Activity 13.1: What makes Earth special?

List gravity, breathable air, liquid water, fertile soil and protection from radiation. Explain how each supports life; compare observations with classmates.

Activity 13.2: Compare the eight planets

Prepare a table of planet temperatures, relative radii and atmospheres from reliable sources. Note that gas-giant temperatures are often cloud-top values and not directly comparable with rocky-planet surfaces.

Activity 13.3: Observe vegetative propagation

Place a money-plant cutting in water, a sprouted potato piece in soil and a ginger rhizome in moist soil. Supply suitable light and water. Record actual dates for roots, shoots and first leaves. Never invent observations.

NCERT Keep the Curiosity Alive — complete worked solutions

Question 1. What is a major reason Mars cannot currently support life like Earth?

Step-by-step explanation: Its thin atmosphere and lack of stable abundant surface liquid water make Earth-like conditions difficult.

Final answer: Option (iii): it lacks a thick atmosphere and liquid water.

Question 2. Which is geodiversity: bird calls, different landforms, changing weather or fish species?

Step-by-step explanation: Geodiversity concerns rocks, landforms, soils and geological processes.

Final answer: Option (ii): mountains, valleys and deserts.

Question 3. What happens to atmospheric retention if Earth were much smaller at the same density?

Step-by-step explanation: Reduced mass gives weaker gravity, allowing more gases to escape over time.

Final answer: Option (ii): gases could escape into space.

Question 4. Why do offspring from sexual reproduction differ from parents?

Step-by-step explanation: They inherit mixed genetic information from gametes.

Final answer: Option (iv): mixed genes from both parents.

Question 5. Why do tiny plants grow in wall cracks after monsoon, and how did seeds arrive?

Step-by-step explanation: Birds, wind or other animals can deposit seeds; rain supplies moisture, while dust, light and air support growth.

Final answer: Seeds arrive by dispersal and germinate under favourable conditions.

Question 6. What effects might forest clearing for a city have on climate, biodiversity and water?

Step-by-step explanation: Less shade and evapotranspiration can warm the area; habitats disappear; runoff and erosion may increase and groundwater recharge may decline.

Final answer: Higher local heat, biodiversity loss and potential water-quality and availability problems.

Question 7. How would you respond to a friend who says modern global warming is merely natural because climates changed in the past?

Step-by-step explanation: Past natural changes occurred, but current long-term warming is primarily driven by human greenhouse-gas emissions, supported by multiple scientific measurements.

Final answer: Natural historical variation does not explain away human-caused warming today.

Question 8. What could happen if Earth's magnetic field suddenly disappeared?

Step-by-step explanation: Charged particles could affect satellites and the upper atmosphere more strongly; long-term atmospheric loss could increase. The atmosphere still provides protection.

Final answer: Greater space-weather hazards and possible long-term atmospheric effects, not immediate extinction.

Question 9. What three Earth-like requirements must a Mars settlement recreate, and which is hardest?

Step-by-step explanation: Provide pressurised breathable air, reliable water and food-producing systems with radiation protection. A self-sustaining ecosystem must recycle resources reliably.

Final answer: Air/pressure, water and food systems; sustaining a closed ecosystem is especially challenging.

Question 10. A village has rising temperatures and unpredictable rain. What might cause it, and suggest two adaptations.

Step-by-step explanation: Climate change and local land-use changes can contribute. Rainwater harvesting stores water; drought-tolerant crops or efficient irrigation reduce vulnerability.

Final answer: Rainwater harvesting and climate-resilient farming.

Question 11. What would happen to life, temperature and water if Earth had no atmosphere?

Step-by-step explanation: Breathable air and normal atmospheric pressure would disappear; temperature extremes and radiation exposure would increase; stable surface water would be difficult.

Final answer: Most current life could not survive and Earth's water and temperature systems would change drastically.

Question 12. Discuss five examples of vegetative propagation.

Step-by-step explanation: Potato grows from tuber eyes; ginger from rhizome buds; sugarcane from stem nodes; money plant from cuttings; Bryophyllum from leaf plantlets.

Final answer: Potato, ginger, sugarcane, money plant and Bryophyllum.

Additional original practice questions and solutions

Question Original 1. Why is Venus hotter than Mercury?

Step-by-step explanation: Venus's thick CO₂ atmosphere absorbs outgoing infrared radiation.

Final answer: Intense greenhouse effect.

Question Original 2. What is the habitable zone?

Step-by-step explanation: It describes where surface liquid water might exist with suitable planetary conditions.

Final answer: Potential liquid-water region around a star.

Question Original 3. Why is the ozone layer important?

Step-by-step explanation: Stratospheric ozone absorbs harmful ultraviolet radiation.

Final answer: It shields living organisms from much UV.

Question Original 4. Distinguish hydrosphere and geosphere.

Step-by-step explanation: Hydrosphere includes water; geosphere includes solid Earth and soils.

Final answer: Water system versus solid-Earth system.

Question Original 5. What is the difference between pollination and fertilisation?

Step-by-step explanation: Pollination transfers pollen; fertilisation unites gametes.

Final answer: Pollen transfer versus gamete fusion.

Question Original 6. Why are asexual offspring not always genetically identical?

Step-by-step explanation: Mutations can occur during replication.

Final answer: Genetic variation is possible.

Question Original 7. Name the triple planetary crisis.

Step-by-step explanation: It describes three linked environmental threats.

Final answer: Climate change, biodiversity loss and pollution.

Question Original 8. Why can plants not simply be grown outdoors on Mars?

Step-by-step explanation: Very low air pressure, extreme cold and lack of stable liquid water prevent normal crop growth.

Final answer: Controlled habitats are necessary.

Question Original 9. How does soil support ecosystems?

Step-by-step explanation: It stores water and nutrients and provides habitat for roots and organisms.

Final answer: It supports plants and nutrient cycling.

Question Original 10. Why do siblings often look different?

Step-by-step explanation: Different combinations of inherited alleles arise during reproduction.

Final answer: They inherit different gene combinations.

Question Original 11. What is the role of decomposers?

Step-by-step explanation: They break down dead material and release nutrients.

Final answer: Nutrient recycling.

Question Original 12. Does being in the habitable zone prove a planet has life?

Step-by-step explanation: Atmosphere, chemistry, water and planetary history also matter.

Final answer: No.

Figures and diagram guidance

Fig. 13.1 compares the crust to apple skin. Fig. 13.2 shows greenhouse warming. Fig. 13.4 shows the habitable zone. Fig. 13.7 depicts Mangalyaan, launched in 2013 and placed in Mars orbit in 2014. Fig. 13.11 illustrates potato and ginger propagation. Fig. 13.13 shows anther and ovule; Fig. 13.14 shows fertilisation and zygote formation. These text descriptions do not reproduce the original figures.

MCQs, HOTS and exam revision

MCQ: Which planet has the hottest surface? Venus. MCQ: What does a gamete contribute? Hereditary information. HOTS: Why does location in the habitable zone not guarantee life? Atmosphere, water, chemistry and history also matter. Common mistakes: Ozone depletion and greenhouse warming are distinct; pollination is not fertilisation; not all mammals give live birth.

Discover, Design and Debate

Design an Earth survival kit for another planet, propose a controlled plant-growth experiment using simulated lunar soil, investigate how flowers attract pollinators, and compare egg numbers and parental care among animals. Distinguish planned missions from completed missions and cite scientific sources.

Official NCERT Chapter 13 PDF

Frequently asked questions

Why is Earth unique?

It is the only planet currently known to support life.

What is the habitable zone?

A region where surface liquid water may exist on a suitable planet.

Why is Venus hotter than Mercury?

Venus has an intense greenhouse effect.

What does ozone do?

Stratospheric ozone absorbs harmful ultraviolet radiation.

Why is Earth's magnetic field important?

It deflects many charged particles.

What is the hydrosphere?

All Earth's water in its different states.

What is geodiversity?

Variety of landforms, rocks, soils and geological processes.

What is vegetative propagation?

Asexual reproduction using plant parts.

What is a gamete?

A reproductive cell contributing hereditary material.

What is fertilisation?

Fusion of gametes forming a zygote.

What is the triple planetary crisis?

Climate change, biodiversity loss and pollution.

Is life confirmed on Mars?

No confirmed extraterrestrial life has been found.

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