Question
The nebular hypothesis by Kant suggests A cloud of dust and gas, known as the
each other, eventually forming planets and the Sun.
V
, formed separate particles that
each other, eventually forming planets and the Sun.
V
, formed separate particles that
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The nebular hypothesis, originally suggested by Immanuel Kant and later expanded by Pierre-Simon Laplace, proposes that the Solar System formed from a vast cloud of dust and gas, known as a **solar nebula**. According to this hypothesis, this nebula underwent gravitational collapse, leading to the formation of a rotating disk. Over time, particles within this disk began to clump together due to gravitational attraction, forming larger bodies through a process known as accretion.
As these separate particles collided and merged, they eventually formed protoplanets. The central region of the disk accumulated enough mass to become the Sun, while the remaining material coalesced into the planets, moons, and other bodies in the Solar System. This process explains the current configuration and characteristics of our Solar System, including the orbital patterns and the differentiation between terrestrial and gas giant planets.
As these separate particles collided and merged, they eventually formed protoplanets. The central region of the disk accumulated enough mass to become the Sun, while the remaining material coalesced into the planets, moons, and other bodies in the Solar System. This process explains the current configuration and characteristics of our Solar System, including the orbital patterns and the differentiation between terrestrial and gas giant planets.
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