The nebular model explains
The nebular hypothesis is the most widely accepted model in the field of cosmogony to explain the formation and evolution of the Solar System (as well as other planetary systems). It suggests that the Solar System formed from nebulous material.
The nebular model posits that the solar system formed from a rotating cloud of gas and dust, known as a solar nebula. Under the influence of gravity, this nebula collapsed, leading to the formation of the Sun at its center while the remaining material flattened into a protoplanetary disk. As particles within the disk collided and coalesced, they formed planetesimals, which eventually became the planets, moons, and other celestial bodies. This model explains the orderly motion of planets and their composition, as well as the presence of a variety of objects in the solar system.
The protoplanetary nebular model is a theory that describes how planetary systems form from a disk of gas and dust surrounding a young star. According to this model, the planets form as material within the disk accretes onto planetesimals, which eventually grow into planets through collisions and gravitational interactions. This model is widely accepted in planetary science for explaining the formation of our own solar system and others.
The nebular hypothesis explains the formation of the solar system from a rotating cloud of gas and dust, known as a nebula. Approximately 4.6 billion years ago, gravitational forces caused this nebula to collapse, leading to the formation of the Sun at its center, while the surrounding material coalesced into planets, moons, asteroids, and other celestial bodies. This model accounts for the observed distribution of mass and angular momentum in the solar system, as well as the differences between terrestrial and gas giant planets.
The most widely accepted model for the formation of the solar system is the nebular hypothesis. This theory suggests that the solar system formed from a rotating mass of gas and dust known as the solar nebula, which collapsed under its own gravity to form the Sun and surrounding planets approximately 4.6 billion years ago.
The nebular hypothesis is the most widely accepted model in the field of cosmogony to explain the formation and evolution of the Solar System (as well as other planetary systems). It suggests that the Solar System formed from nebulous material.
It was first proposed in 1734 by Emanuel Swedenborg. Originally applied only to our own Solar System, this method of planetary system formation is now thought to be at work throughout the universe. The widely accepted modern variant of the nebular hypothesis is Solar Nebular Disk Model (SNDM) or simply Solar Nebular Model.
Planets do not evolve in the Darwinian sense, but they do form and change over time. The model describing how they form is the Nebular Hypothesis, first formulated by Emanuel Swedenborg and Immanuel Kant.
It is -------------------------- if your so smart why don't yopu look it up and not by the enternet :)
The Big Bang is a theory that discusses the origin of the universe (from a single point source of incredible density and energy) while the Nebular Hypothesis is a theory that discusses the origins of stars and their planetary systems (through the accretion of interstellar gas).
nebular
The nebular hypothesis is the most widely accepted model explaining the formation and evolution of the Solar System.
The creation of stars and planets into solar systems by condensation, concretion, and gravitational collapse.
There is evidence that the Nebular hypothesis was first proposed in 1734 by Emanuel Swedenborg.Immanuel Kant, who was familiar with Swedenborg's work, developed the theory further in 1755. A similar model was proposed in 1796 by Pierre-Simon Laplace.
The protoplanetary nebular model is a theory that describes how planetary systems form from a disk of gas and dust surrounding a young star. According to this model, the planets form as material within the disk accretes onto planetesimals, which eventually grow into planets through collisions and gravitational interactions. This model is widely accepted in planetary science for explaining the formation of our own solar system and others.
a nebular creates stars as it caves in by its own gravity!
nebular