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  • Geography Notes For W.B.C.S Examination-The Origin and Evolution of the Earth
    Posted on October 30th, 2018 in Geography
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    Geography Notes For W.B.C.S Examination-The Origin and Evolution of the Earth

    The origin and evolution of the earth notes

    Nebular Hypothesis

    • Immanuel Kant, a German philosopher gave this theory.Continue Reading Geography Notes For W.B.C.S Examination-The Origin and Evolution of the Earth .
    • In 1796, a mathematician Pierre-Simon Laplace reexamined it.
    • According to this hypothesis, the planets were moulded out of a cloud of material associated with a young sun, which was rotating slowly.

    Binary theories

    • As per these theories, the sun had a companion.

    Revised Nebular Hypothesis

    • Revised Nebular Hypothesis was propounded by Carl Weizascar in Germany and Otto Schmidt in Russia.
    • They regarded that a solar nebula surrounded the sun and that the nebula comprised of chiefly hydrogen, helium and something called dust.
    • The collision of particles and the friction caused a disk-shaped cloud to be formed and then the planets were created via the accretion process.

    Big Bang Theory

    • Alternatively called the expanding universe hypothesis.
    • As per this theory, in the beginning, all matter or substance forming this universe existed at one place as a tiny ball. This tiny ball had an extremely small volume, infinite density and temperature.
    • At the Big Bang, this ball blasted fiercely and forcefully and started a substantial process of expansion which continues to this day.
    • Now it is accepted that this event took place 13.7 billion years ago.

    Origin of Earth 

    Formation of Planets

    The following are regarded as the stages in the planets’ development:

    • The stars are localised gas lumps inside a nebula.
    • A core to the gas cloud as well as a spinning disc of dust and gas are created because of the gravitational force within the lumps.
    • After this, the cloud of gas condenses and the matter over the core is changed into tiny rounded objects.
    • These small round objects develop into what are called planetesimals by a cohesion process.
    • The smaller objects start forming larger bodies by colliding with one another and they stick together because of gravitational force.
    • In the last stage, these large number of small planetesimals aggregate to develop into a smaller number of large bodies called planets.

     

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