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The nebular hypothesis explains how our solar system probably formed from a giant cloud of gases and dispersed solid particles.
What is Nebular hypothesis?
The most widely accepted theory in cosmogony to explain how the solar system formed and evolved is the nebular hypothesis. It implies that gas and dust orbiting the sun are what created the solar system.
Following are the steps in nebular theory:
- As part of the cloud of gas and dust condenses into a core and becomes a protostar, the nebula changes into a solar nebula.
- The material condensing might have been brought on by a nearby supernova shockwave.
- An accretion disk is formed as the protostar's surrounding material disintegrates.
How did the solar system form, according to the nebular hypothesis?
The nebular hypothesis states that enormous clouds of hydrogen and helium imploded. The cloud's center heated up significantly after collapsing. The system then started to rotate as it became hotter and more compressed. The formation of the solar system started at this point.
Learn more about solar system here:
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