The Origin and Evolution of the Earth

Class 11 Geography · Fundamentals of Physical Geography · Chapter 2

163 members in the CBSE community

View all
  • Marks booster + cheatsheet: key concepts in 2 lines each, common traps
  • 8 marks: Climate unit, Ch 7–10
  • 5 marks: map work, covered
  • 4 marks: ocean data as charts, Unit V
  • Heat budget and five air layers as charts
  • Common traps, corrected
Page 1 free about 8 min read, Full kit about 55 min read
  • Marks booster + cheatsheet: key concepts in 2 lines each, common traps
  • 12 marks: Climate, Vegetation (Unit III)
  • Full CBSE map-work list, chapter by chapter
  • Indus, Ganga, Brahmaputra river systems
  • Monsoon mechanism, onset and four seasons
  • Common traps, corrected
Page 1 free about 8 min read, Full kit about 55 min read
  • Marks booster + cheatsheet: key concepts in 2 lines each
  • 4 marks: Map Scale, conversions worked
  • 4 marks: Latitude, Longitude and Time
  • 4 marks: Topographical Maps, contours
  • 5 marks: practical file and viva
  • Conical and Mercator's construction steps
Page 1 free about 8 min read, Full kit about 55 min read
View all 44 amazing Marks Booster kits →

Summary

This chapter traces ideas about the origin of the earth and the universe. Early theories include the Nebular Hypothesis of Immanuel Kant (revised by Laplace in 1796), and the modern version by Otto Schmidt and Carl Weizsacker, who held that the sun was surrounded by a solar nebula of hydrogen and helium from which planets formed by accretion. The most popular modern view of the origin of the universe is the Big Bang Theory (expanding universe hypothesis); Edwin Hubble in 1920 provided evidence that the universe is expanding. The Big Bang occurred about 13.7 billion years ago when a "tiny ball" of infinite density exploded; within the first three minutes the first atoms began to form, and after 300,000 years atomic matter arose. Stars formed from clumps within nebulae about 5–6 billion years ago, and planets developed through stages: a rotating disc of gas and dust, the formation of planetesimals by cohesion, and finally accretion into larger planets. The earth began as a barren, hot, rocky body and acquired its layered structure (crust, mantle, outer core, inner core) through the process of differentiation, where heavier materials sank to the centre. The atmosphere evolved in three stages, including degassing from the interior and modification by photosynthesis; oceans formed about 4,000 million years ago and life began to evolve around 3,800 million years ago.

The Origin and Evolution of the Earth

Key terms

Nebular Hypothesis
the idea of Kant (revised by Laplace) that planets formed from a cloud of material around a youthful, slowly rotating sun.
Big Bang Theory
the expanding-universe hypothesis that all matter began in a tiny dense ball that exploded about 13.7 billion years ago.
Light year
a measure of distance: the distance light travels in one year, about 9.461 × \(10^12\) km.
Planetesimals
small rounded bodies formed by cohesion of matter that later accreted into planets.
Differentiation
the process by which heavier materials sank to the centre, separating the earth into layers.
Degassing
the process by which gases and water vapour were released from the earth's hot interior to build the early atmosphere.

Extra questions & answers

Try one from this chapter
The Nebular Hypothesis was first proposed by which philosopher?
Flashcards & interactive practice

Practice quiz · The Origin and Evolution of the Earth

Score on this chapter, climb the leaderboard, and get an AI diagnosis of your mistakes.

Double-checked questions Real exam pattern 1 free test every month, then ₹9 per test

#1

The Origin and Evolution of the Earth

Start here
Geography 10 Qs · ~10 min

Instant score, answer review and weak-topic diagnosis

Data & insights

Trending in Class 11 this weekThe chapters students are reading most right now
  1. 1The AdventureEnglish
  2. 2The Portrait of a LadyEnglish
  3. 3The AddressEnglish
See the full ranking