Origin of the Solar System
Nebular Hypothesis
Encounter Hypothesis
Tidal Theory
In this scenario, a rogue star passes close to the Sun about 5 billion years ago. Material, in the form of hot gas, is tidally stripped from the Sun and the rogue star.
the passage of a massive star past the Sun would raise a huge solar tidal bulge from which matter would escape in the form of a filament.
cloud collapse,
Sir James H. Jeans (1877–1946) and Sir Harold Jeffreys.
formation of a protoplanetary disk,
growth
of planets.
Solar System
Hypothetically, a shockwave from a supernova or the effect of a passing star may cause a cloud collapse. The collapse at the center of the cloud due to gravity occurs when gas pressure becomes insufficient to support the mass of the cloud. The collapsed cloud of interstellar gas and dust results in a smaller radius which means it will spin faster.
Planetesimals are small celestial bodies that combine under the force of gravity forming protoplanets. Planetesimals are small celestial bodies that combine under the force of gravity forming protoplanets.
The proponents of the nebular theory are Emanuel Swedenborg, Immanuel Kant, and Pierre-Simon Laplace.
Planets
Terrestrial
asteroids
Comets
Accretion
Jovian
It is the gradual accumulation of matter which results in an increase in size.
Planetesimal Theory
Planetesimal Theory is a form of encounter theory. It proposes that a passing star termed as an intruding star nearly collided with the
protosun.
The planetesimal theory is also known as the Chamberlin-Moulton Hypothesis, after its proponents Thomas Chowder Chamberlin and Forest Ray Moulton.