Origin of Earth – NDA Geography Notes

Exam Relevance: Low-Moderate Frequency | Big Bang vs Nebular Hypothesis, Geological Eras, Dinosaur Extinction, Pleistocene Epoch, Palaeoclimatology

Reading Time: 20–25 minutes | Last Updated: 2025

How did the Earth form? How old is it? When did life first appear? These are questions that scientists have been trying to answer for centuries. This chapter covers the theories about the origin of the Universe and the Earth, the geological time scale, and the major eras of Earth’s history.

NDA does not ask many questions from this chapter, but the ones it does ask are very specific, particularly about which era dinosaurs lived in, what happened in the Pleistocene epoch, and the geological time scale. These questions are straightforward if you know the basic framework clearly.


How Did the Universe Begin?

Most scientists today accept the Big Bang Theory as the best explanation for the origin of the Universe.

About 13.8 billion years ago, the entire Universe existed as an incredibly hot and dense single point. In a massive explosion, the Big Bang, this point expanded rapidly. Space, time, matter, and energy all came into existence at that moment. The Universe has been expanding ever since. [NDA 2019-II]

As the Universe expanded and cooled, hydrogen and helium, the simplest elements, formed first. Over billions of years, gravity pulled these gases together to form stars. Inside stars, nuclear reactions created heavier elements like carbon, oxygen, and iron. When massive stars exploded at the end of their lives, they scattered these elements into space. New stars and planets, including our Solar System, formed from this enriched material.


How Did the Earth Form?

The Earth formed about 4.6 billion years ago from the same cloud of gas and dust that formed the Sun and the rest of the Solar System.

As the Sun formed at the centre of this cloud, the remaining material began to clump together. Small particles collided and stuck, gradually building up larger bodies that eventually became the planets.

The early Earth was extremely hot. The interior was entirely molten. Heavier materials like iron and nickel sank toward the centre, forming the core. Lighter materials rose and cooled to form the crust. Over billions of years, the Earth cooled further, oceans formed, and eventually life appeared.


Theories About Earth’s Origin

Nebular Hypothesis was proposed by Kant and Laplace. A rotating cloud of gas and dust (called a nebula) cooled and contracted, throwing off rings of material that condensed into planets. This was an early theory that has since been refined.

Planetesimal Hypothesis was proposed by Chamberlin. A passing star pulled material from the Sun. This material formed small solid bodies called planetesimals. These collided and gradually built up into planets.

IMPORTANT The Big Bang Theory explains the origin of the Universe (13.8 billion years ago). The Nebular and Planetesimal hypotheses explain the origin of the Solar System (4.6 billion years ago). These are different events. Do not confuse them. [NDA 2019-II]

The Geological Time Scale

The geological time scale organises Earth’s 4.6-billion-year history into named time periods. Scientists determined this by studying rock layers and the fossils found within them. Older rocks are generally found below newer rocks. Different fossils appear in different layers, helping scientists identify when different forms of life existed.

Divisions from largest to smallest: Eons → Eras → Periods → Epochs

The Four Major Eons

EonTimeKey Feature
Hadean4.6 to 4.0 billion years agoNo life; molten surface
Archean4.0 to 2.5 billion years agoFirst simple life (bacteria)
Proterozoic2.5 billion to 541 million years agoSimple multicellular life begins
Phanerozoic541 million years ago to presentComplex life; divided into three eras

The Three Major Eras of the Phanerozoic Eon

EraTimeKnown AsKey Life
Palaeozoic541–252 MaAge of Ancient LifeMarine invertebrates → fish → amphibians → reptiles
Mesozoic252–66 MaAge of ReptilesDinosaurs
Cenozoic66 Ma–presentAge of MammalsMammals → Humans

Palaeozoic Era (541 to 252 million years ago)

Palaeozoic means “ancient life.” This era saw the explosion of complex marine life, followed by the appearance of fish, amphibians, reptiles, and land plants.

Cambrian Period: the first explosion of complex invertebrates (trilobites, molluscs). Life was almost entirely in the sea.

Permian Period: the era ended with the largest mass extinction in Earth’s history, wiping out about 96% of all marine species.

Mesozoic Era (252 to 66 million years ago)

Mesozoic means “middle life.” This is the famous Age of Reptiles, the era of dinosaurs.

Dinosaurs first appeared in the Triassic Period (252 to 201 million years ago). They dominated the Earth through the Jurassic and Cretaceous periods. The Mesozoic Era ended about 66 million years ago with a mass extinction, most likely caused by a large asteroid striking the Earth, which wiped out the dinosaurs and about 75% of all species.

Appeared in Triassic. Went extinct at end of Cretaceous. Dinosaurs did not go extinct in the Triassic. They only first appeared there.

Cenozoic Era (66 million years ago to present)

Cenozoic means “recent life.” After the extinction of dinosaurs, mammals rapidly diversified and became the dominant animals, the Age of Mammals.


Important Epochs of the Cenozoic

Palaeocene Epoch (66 to 56 million years ago), the first epoch of the Cenozoic. Early mammals spread rapidly after the dinosaurs disappeared.

Pleistocene Epoch (2.6 million to 11,700 years ago). This is when the Ice Ages occurred, periods when large parts of the Earth were covered in glaciers. Early humans (the genus Homo) appeared during this epoch. The Karewas of Kashmir, the flat-topped lacustrine deposits, formed during the Pleistocene when the Kashmir Valley was a large lake.

Holocene Epoch (11,700 years ago to present), the current epoch. The Ice Ages ended. Human civilisation began. All of recorded history falls within the Holocene.

EpochTimeKey Event
Palaeocene66–56 MaEarly mammals spread after dinosaur extinction
Pleistocene2.6 Ma–11,700 years agoIce Ages; early humans (Homo); Karewas formed
Holocene11,700 years ago–presentCurrent epoch; all recorded history

Palaeoclimatology

Palaeoclimatology is the study of ancient climates: what the Earth’s climate was like in the distant past. Scientists use ice cores, fossil pollen, tree rings, and ocean sediments to reconstruct past climates. [NDA 2022-II]


How Do We Know the Age of the Earth?

The answer: 4.6 billion years: comes from a technique called radiometric dating.

Certain elements are radioactive. They slowly change from one element to another at a known, fixed rate. For example, uranium slowly changes into lead. By measuring how much uranium and how much lead are in a rock, scientists can calculate how long the rock has been forming. The oldest rocks found on Earth are about 4 billion years old. Meteorites give ages of about 4.6 billion years. This tells us the Solar System formed about 4.6 billion years ago.


Quick Revision

ORIGIN THEORIES

TheoryWhat It ExplainsProposed ByNDA Tag
Big Bang TheoryOrigin of the Universe (13.8 billion years ago)[NDA 2019-II]
Nebular HypothesisOrigin of Solar System (4.6 billion years ago)Kant and Laplace
Planetesimal HypothesisOrigin of Solar SystemChamberlin

GEOLOGICAL TIME: DIVISIONS Eons → Eras → Periods → Epochs

THREE MAJOR ERAS (oldest → newest)

EraTime (Ma)AgeKey PeriodKey Event
Palaeozoic541–252Ancient lifeCambrian; PermianInvertebrates → reptiles; Permian mass extinction
Mesozoic252–66Age of ReptilesTriassic → Jurassic → CretaceousDinosaurs appear (Triassic); extinct (end Cretaceous)
Cenozoic66–presentAge of MammalsPalaeocene; Pleistocene; HoloceneMammals diversify; humans appear

KEY EPOCHS

  • Palaeocene = first epoch of Cenozoic; early mammals
  • Pleistocene = Ice Ages; early humans (Homo); Karewas of Kashmir
  • Holocene = current epoch; all recorded history (last 11,700 years)

OTHER KEY FACTS

  • Earth’s age = 4.6 billion years (radiometric dating: uranium → lead)
  • Palaeoclimatology = study of ancient climates [NDA 2022-II]
  • Early Earth: iron and nickel sank to form core; lighter material rose to form crust

Related Topics

Universe and Solar System Interior of the Earth Physical Division of India

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