Easy2Siksha Sample Paper
GNDU Most Repeated (Important) Quesons
B.A. 1st Semester
Geography (Physical Geography-I: Geomorphology) (2022-2024)
Must-Prepare Quesons (80-100% Probability)
SECTION-A (Origin of Earth & Structure)
1. 󷄧󼿒 Origin of Earth Theories (Nebular/Tidal/Connental Dri) (4 mes)
2. 󷄧󼿒 Structure of Earth with layers (2 mes)
󹵍󹵉󹵎󹵏󹵐 2025 Smart Predicon Table
Based on 4-Year Queson Paper Analysis + Latest Set
SECTION-A (Origin & Structure of Earth)
Queson Topic
Repeats
Years Appeared
Priority
Origin of Earth (Nebular/Tidal
Hypothesis)
4 Times
2021 (Q1), 2022 (Q1), 2023 (Q1),
2024 (implied)
󹻦󹻧 Very
High
Connental Dri Theory
(Wegener)
2 Times
2022 (Q2), 2024 (Q2-Plate
Tectonics link)
󽁗 High
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High Probability Quesons (60-80%)
Connental Dri Theory detailed explanaon (2 mes)
󷘹󷘴󷘵󷘶󷘷󷘸 2025 Predicon Summary
Almost Guaranteed (Pracce These First!):
1. 󷄧󼿒 Origin of Earth (Nebular or Tidal Hypothesis)
2. 󷄧󼿒 Folds - All types with diagrams
GNDU Most Repeated (Important) Answer
B.A. 1st Semester
Geography (Physical Geography-I: Geomorphology) (2022-2024)
Must-Prepare Quesons (80-100% Probability)
SECTION-A (Origin of Earth & Structure)
1. Origin of Earth Theories (Nebular/Tidal/Connental Dri) (4 mes)
Ans: The Origin of the Earth A Story from Dust to a Living Planet
Long, long ago before trees, oceans, or even the Sun as we know it there was only
a vast, dark emptiness. Imagine a cold cosmic night filled with swirling clouds of dust and
gas. No planets, no stars, no sound just silence and mystery.
And yet, from this nothingness, our beautiful Earth was born. The story of Earth’s origin
is not just about rocks and gases; it’s a story of transformation from chaos to
creation, from dust to life. Scientists have spent centuries trying to understand how our
planet came to be. Over time, many theories have been proposed. Among them, three
important ones stand out:
1. The Nebular Hypothesis
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2. The Tidal Hypothesis
3. The Continental Drift Theory
Let’s take a journey through each — like turning the pages of the universe’s own
storybook.
1. The Nebular Hypothesis The Cosmic Cloud that Became Home
Our story begins about 4.6 billion years ago. Scientists believe that our Solar System
including the Earth formed from a giant rotating cloud of gas and dust, known as a
nebula.
This theory, called the Nebular Hypothesis, was first suggested by Immanuel Kant
(1755) and later refined by Pierre-Simon Laplace (1796).
Now, let’s imagine it…
There was once a massive nebula floating in space made mostly of hydrogen, helium,
and tiny dust particles. It was quietly spinning for millions of years. Then, something
happened maybe a nearby star exploded (a supernova), sending shock waves that
made the nebula start to collapse under its own gravity.
As it shrank, it spun faster and faster just like a skater spins faster when pulling in
their arms. The center of this spinning disk became very hot and dense, eventually
forming our Sun.
The leftover gas and dust began sticking together small particles clumped to form
pebbles, pebbles became rocks, and rocks collided to form planetesimals (tiny planets).
Through millions of such collisions, Earth was born a glowing ball of molten matter
slowly cooling down.
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At first, Earth was a fiery world its surface a sea of molten lava. Slowly, it cooled
down. Heavier elements like iron and nickel sank to the center forming the core, while
lighter materials formed the crust. Water vapor condensed into rain, filling depressions
to form oceans. Gases like nitrogen, carbon dioxide, and oxygen formed the
atmosphere.
From that humble nebular cloud, a living planet emerged.
2. The Tidal Hypothesis A Fiery Encounter in Space
But not everyone agreed with the Nebular idea. In the early 20th century, two scientists
Sir James Jeans and Harold Jeffreys proposed another dramatic story called the
Tidal Hypothesis.
According to them, billions of years ago, our Sun already existed a huge, burning star
in the middle of space. One day, another massive star passed very close to it. The pull of
this passing star created gigantic tidal waves on the Sun’s surface (like how the Moon
pulls tides on Earth, but much stronger).
These tidal waves stretched out hot gases from the Sun into space. Long fingers of fire
were pulled away some of these gaseous streams broke off and began to spin around
the Sun.
Over time, these fiery blobs cooled and condensed into planets, including our Earth.
Diagram: Tidal Hypothesis
Passing Star
Sun (tidal bulges)
Gaseous Matter Pulled Out
Planets formed from gases
In this version, the Earth was once a part of the Sun’s outer layer a burning fragment
that cooled down into a solid body.
Although this idea sounds exciting (almost like a cosmic tug-of-war!), later scientists
found problems with it. The main issue: it’s extremely rare for stars to pass that close
without completely destroying each other. Also, the matter pulled out would probably
disperse not form solid planets.
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So, the Nebular Hypothesis remained more accepted because it better explains the
shape and movement of the Solar System. But the Tidal theory is still admired as a bold
and creative explanation of planetary birth.
3. The Continental Drift Theory When Earth Itself Started Moving
Now that the Earth was formed, another great mystery appeared:
Why are continents shaped like puzzle pieces that seem to fit together?
If you look closely at a world map, the eastern coast of South America fits perfectly with
the western coast of Africa like two halves of a torn page. This observation led Alfred
Wegener, a German meteorologist, to propose the Continental Drift Theory in 1912.
Wegener believed that all continents were once joined together in a single massive
supercontinent called Pangaea (meaning “all Earth”). Surrounding it was one huge
ocean, Panthalassa.
Over millions of years, Pangaea began to break apart due to internal Earth forces. The
pieces drifted slowly across the surface forming the continents we know today.
Diagram: Continental Drift Theory
250 million years ago: Pangaea (single supercontinent)
200 million years ago: Drift begins
65 million years ago: Continents take shape
Present: Modern world map
Wegener used evidence such as:
Similar fossils found on different continents (e.g., Mesosaurus fossils in both
South America and Africa).
Matching mountain ranges (like the Appalachians and Caledonian Mountains).
Evidence of ancient glaciation across now-tropical regions.
At first, scientists rejected his theory because he couldn’t explain how continents
moved. Later, with the discovery of plate tectonics, his idea was proven right
continents indeed drift, floating slowly over molten rock beneath the crust.
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Today, we know that the Earth’s crust is divided into tectonic plates that move about 2
5 cm per year like slow-moving rafts on a molten sea. Wegener’s idea changed our
understanding of Earth forever.
The Beautiful Sequence of Creation
If we link all these theories together, we get a grand timeline of creation:
1. Nebular Hypothesis → Describes how the Earth and other planets formed from a
cloud of gas and dust.
2. Tidal Hypothesis A creative alternative explaining planet formation through
stellar encounters.
3. Continental Drift Theory → Explains how Earth’s surface continued evolving,
shaping continents and oceans.
Each theory, in its own time, brought us a step closer to understanding the miracle of
our planet.
In Simpler Words: The Earth’s Journey
Think of it like this:
The Nebular Hypothesis is about the birth of Earth how it came into existence.
The Tidal Hypothesis is an alternate story a different imagination of that birth.
The Continental Drift Theory is about Earth’s life after birth how it changed,
moved, and took the shape we see today.
So, the Earth’s story is a continuous dance — from dust to planet, from fire to water,
from one supercontinent to seven.
Conclusion A Living Planet from Cosmic Dust
Our Earth’s origin is a tale of mystery, imagination, and science woven together. From a
swirling nebula to a glowing planet and finally to a blue-green world filled with life the
journey took billions of years.
Each theory Nebular, Tidal, or Continental Drift contributed a piece of the grand
puzzle. And together, they remind us how small we are, yet how special our planet is.
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Every grain of sand, every mountain, every ocean wave carries the memory of that
ancient cosmic beginning. Earth isn’t just a rock in space it’s a living story, written
over 4.6 billion years, and still being written today.
2. Structure of Earth with layers (2 mes)
Ans: The Story of Earth’s Structure
Imagine you are an explorer standing on the surface of our planet. The ground beneath
your feet feels solid, but what if you could dig deeper and deeperthrough rocks,
molten rivers, and fiery cores? You would discover that the Earth is not a single solid
ball, but a layered world, each layer with its own character, composition, and role.
Let’s begin this journey layer by layer.
The Earth as a Layered Cake
Think of Earth like a giant cake with multiple layers:
1. Crust the thin outer icing.
2. Mantle the thick sponge beneath.
3. Outer Core the liquid chocolate filling.
4. Inner Core the solid, glowing cherry at the center.
Each layer is unique, and together they make Earth the living planet we call home.
1. The Crust Earth’s Skin
Thickness: 570 km (thinnest under oceans, thickest under mountains).
Composition: Rocks like granite (continental crust) and basalt (oceanic crust).
Temperature: Relatively cool compared to deeper layers (up to 400°C).
Story Analogy: The crust is like the skin of an apple—thin, fragile, but essential. It’s
where we live, build cities, grow crops, and walk every day.
Types of Crust
1. Continental Crust: Thick, less dense, made of granite.
2. Oceanic Crust: Thin, denser, made of basalt.
2. The Mantle The Giant Middle Layer
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Thickness: About 2,900 km (the thickest layer).
Composition: Silicate rocks rich in magnesium and iron.
Temperature: 500°C near the crust to 4,000°C near the core.
Story Analogy: The mantle is like the sponge of the cakethick, soft in parts, and slowly
moving.
Upper Mantle & Asthenosphere
The upper mantle is partly molten and flows slowly.
This movement drives plate tectonicsthe shifting of continents and
earthquakes.
Lower Mantle
More rigid due to high pressure, but still capable of slow flow.
3. The Outer Core The Fiery Ocean of Metal
Thickness: About 2,200 km.
State: Liquid.
Composition: Molten iron and nickel.
Temperature: 4,0005,000°C.
Story Analogy: Imagine a swirling ocean of liquid metal deep inside the Earth. This is the
outer core.
Importance
The movement of molten iron here generates Earth’s magnetic field, which
protects us from harmful solar radiation.
Without it, life on Earth would be exposed to deadly cosmic rays.
4. The Inner Core The Glowing Heart
Radius: About 1,220 km.
State: Solid (due to immense pressure).
Composition: Iron and nickel.
Temperature: Around 5,0006,000°Chotter than the surface of the Sun!
Story Analogy: At the very center lies a glowing metal ball, like a cherry at the heart of
the cake. It is solid not because it’s cool, but because the pressure is so immense that
atoms are locked tightly together.
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Diagram of Earth’s Layers
Two Ways to Classify Earth’s Layers
Scientists classify Earth’s structure in two ways:
1. Chemical Composition (What it’s made of):
Crust → Silicates (granite, basalt).
Mantle → Silicates with magnesium & iron.
Core → Iron and nickel.
2. Physical Properties (How it behaves):
Lithosphere → Rigid (crust + upper mantle).
Asthenosphere → Semi-molten, flows slowly.
Mesosphere → Strong lower mantle.
Outer Core → Liquid.
Inner Core → Solid.
Comparative Table of Earth’s Layers
Layer
Thickness
State
Temperature
Special Role
Crust
570 km
Solid
Up to 400°C
Supports life
Mantle
2,900 km
Semi-
solid
5004000°C
Drives plate
tectonics
Outer
Core
2,200 km
Liquid
40005000°C
Creates magnetic
field
Inner
Core
1,220 km
Solid
50006000°C
Earth’s solid heart
Why Earth’s Structure Matters
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1. Plate Tectonics: Movement in the mantle causes earthquakes, volcanoes, and
mountain building.
2. Magnetic Field: Generated by the outer core, it shields life from solar winds.
3. Life on Crust: The thin crust supports ecosystems, agriculture, and human
civilization.
4. Scientific Exploration: Understanding Earth’s layers helps in mining, oil
exploration, and predicting natural disasters.
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