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Origin of the Earth
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Origin of the Earth
Early Theories
A large number of hypotheses were put forth by different philosophers and scientists regarding the origin of the 
earth.
One of the earlier and popular arguments was by German philosopher Immanuel Kant. Mathematician Laplace 
revised it in 1796. It is known as Nebular Hypothesis.
The hypothesis considered that the planets were formed out of a cloud of material associated with a youthful sun, 
which was slowly rotating.
Page 3


Origin of the Earth
Early Theories
A large number of hypotheses were put forth by different philosophers and scientists regarding the origin of the 
earth.
One of the earlier and popular arguments was by German philosopher Immanuel Kant. Mathematician Laplace 
revised it in 1796. It is known as Nebular Hypothesis.
The hypothesis considered that the planets were formed out of a cloud of material associated with a youthful sun, 
which was slowly rotating.
Nebular Hypothesis
Proposed by Immanuel Kant and revised by Laplace in 1796
Planets formed from a cloud of material around a young, slowly rotating sun
Revised Theories (1950)
Otto Schmidt in Russia and Carl Weizascar in Germany revised the 'nebular hypothesis'
They proposed that the sun was surrounded by solar nebula containing mostly hydrogen 
and helium along with dust
The friction and collision of particles led to formation of a disk-shaped cloud
The planets were formed through the process of accretion
Page 4


Origin of the Earth
Early Theories
A large number of hypotheses were put forth by different philosophers and scientists regarding the origin of the 
earth.
One of the earlier and popular arguments was by German philosopher Immanuel Kant. Mathematician Laplace 
revised it in 1796. It is known as Nebular Hypothesis.
The hypothesis considered that the planets were formed out of a cloud of material associated with a youthful sun, 
which was slowly rotating.
Nebular Hypothesis
Proposed by Immanuel Kant and revised by Laplace in 1796
Planets formed from a cloud of material around a young, slowly rotating sun
Revised Theories (1950)
Otto Schmidt in Russia and Carl Weizascar in Germany revised the 'nebular hypothesis'
They proposed that the sun was surrounded by solar nebula containing mostly hydrogen 
and helium along with dust
The friction and collision of particles led to formation of a disk-shaped cloud
The planets were formed through the process of accretion
Modern Theories
The Big Bang Theory was introduced by Edwin Hubble in 
1920
It offers a contemporary explanation for Earth's origin
Also known as the Expanding Universe Hypothesis
States that the universe continuously expands
Suggests all universal matter was initially concentrated at 
its center in an extremely hot, dense point
Around 13.7 billion years ago, a massive explosion occurred
This explosion triggered atom formation
Eventually energy was converted into matter
Page 5


Origin of the Earth
Early Theories
A large number of hypotheses were put forth by different philosophers and scientists regarding the origin of the 
earth.
One of the earlier and popular arguments was by German philosopher Immanuel Kant. Mathematician Laplace 
revised it in 1796. It is known as Nebular Hypothesis.
The hypothesis considered that the planets were formed out of a cloud of material associated with a youthful sun, 
which was slowly rotating.
Nebular Hypothesis
Proposed by Immanuel Kant and revised by Laplace in 1796
Planets formed from a cloud of material around a young, slowly rotating sun
Revised Theories (1950)
Otto Schmidt in Russia and Carl Weizascar in Germany revised the 'nebular hypothesis'
They proposed that the sun was surrounded by solar nebula containing mostly hydrogen 
and helium along with dust
The friction and collision of particles led to formation of a disk-shaped cloud
The planets were formed through the process of accretion
Modern Theories
The Big Bang Theory was introduced by Edwin Hubble in 
1920
It offers a contemporary explanation for Earth's origin
Also known as the Expanding Universe Hypothesis
States that the universe continuously expands
Suggests all universal matter was initially concentrated at 
its center in an extremely hot, dense point
Around 13.7 billion years ago, a massive explosion occurred
This explosion triggered atom formation
Eventually energy was converted into matter
Stages of the Big Bang Theory
Singularity
All matter and energy existed in a "tiny ball" (singular atom) with infinite temperature and density.
Big Bang Explosion
The "tiny ball" exploded violently 13.7 billion years ago, leading to rapid expansion. Some energy 
converted into matter. Rapid expansion within fractions of a second; first atoms formed within three 
minutes.
Cooling and Atomic Matter Formation
300,000 years after the Big Bang, temperature dropped to 4,500K. Atomic matter formed, and the 
universe became transparent.
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FAQs on PPT: Origin of the Earth - Geography Class 11 - Humanities/Arts

1. What are the primary theories about the origin of the Earth?
Ans. The primary theories regarding the origin of the Earth include the nebular hypothesis, which suggests that the Earth formed from a rotating cloud of gas and dust in space. Another significant theory is the planetesimal hypothesis, which posits that Earth formed through the gradual accumulation of smaller bodies called planetesimals. Additionally, some scientists consider the giant impact hypothesis, which proposes that a Mars-sized body collided with the early Earth, leading to the formation of the Moon.
2. How did early geological processes shape the Earth’s surface?
Ans. Early geological processes such as volcanism, tectonic activity, and erosion significantly shaped the Earth’s surface. Volcanic eruptions released gases and molten rock, creating landforms like mountains and islands. Tectonic activity led to the formation of continents and ocean basins through the movement of tectonic plates. Erosion from wind, water, and ice gradually sculpted these landforms, contributing to the diverse landscapes we see today.
3. What role did water play in the development of the Earth?
Ans. Water played a crucial role in the development of the Earth by facilitating the formation of oceans, which are essential for sustaining life. It helped in the weathering of rocks, which contributed to soil formation and the cycling of nutrients. Additionally, water’s presence in various forms (liquid, ice, vapor) influenced the planet's climate and atmosphere, creating a stable environment for life to emerge.
4. What are some significant milestones in the Earth’s geological history?
Ans. Significant milestones in the Earth’s geological history include the formation of the Earth approximately 4.5 billion years ago, the appearance of the first simple life forms around 3.5 billion years ago, and the Cambrian explosion about 541 million years ago, which marked a rapid diversification of life. Other milestones include the formation of supercontinents like Pangaea and significant extinction events that reshaped biodiversity.
5. How does the study of the Earth’s origin contribute to our understanding of other celestial bodies?
Ans. The study of the Earth’s origin provides insights into the processes that govern planetary formation and evolution, which can be applied to other celestial bodies in our solar system and beyond. By understanding the conditions that led to the Earth’s formation, scientists can make inferences about the potential for life on other planets, the composition of their atmospheres, and their geological histories, enhancing our knowledge of the universe.
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