The Earth was formed approximately 4.6 billion years ago from cosmic dust and gas through processes including planetary accretion. This chapter explores theories of Earth's formation, the structure of its layers, major geological time periods, and the cooling and differentiation of the Earth. Additionally, it discusses the formation of continents and oceans, as well as the ongoing geological processes that continue to shape the planet today.
You've not yet enrolled in this course. Please enroll for free to listen to audio lessons, classroom podcasts and take mock test.
References
g11-2.pdfClass Notes
Memorization
What we have learnt
Final Test
Revision Tests
Chapter FAQs
Term: Planetary Accretion
Definition: The process by which dust and gas in the solar system gradually came together under gravitational attraction to form planets.
Term: Geological Time Scale
Definition: A timeline that divides Earth's history into eons, eras, periods, and epochs based on significant geological and biological events.
Term: Plate Tectonics
Definition: A theory explaining the movement of Earth's lithosphere divided into tectonic plates that shape the Earth's surface.
Term: Differentiation
Definition: The process by which heavier materials sink to the center of the Earth while lighter materials rise to form the mantle and crust.