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The prograde rotation of the collapsing cloud of gas and dust results in conservation of angular momentum, causing the material to flatten into a disk shape. This disk of material, known as a protoplanetary disk, is where planets are thought to form through the process of accretion and gravitational interactions.
An accretion disk forms around a massive object, such as a black hole or a young star, when material falls into its gravitational pull. The material spirals inward due to angular momentum conservation, forming a disk-shaped structure as it moves closer to the central object. Friction within the disk causes the material to heat up and emit energy in the form of radiation.
accretion disk
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.
solar system Material that is in orbit around a massive central body is an accretion disk. This disk can eventually turn into a white dwarf star. An accretion disc may eventually form planets such as the ones in our solar system.
from when an objects crashed into earth and an chunk of rock form
from when an objects crashed into earth and an chunk of rock form
from when an objects crashed into earth and an chunk of rock form
In a way, yes. The material that makes up the "disk" in a floppy is Mylar, a magnetic substance. Data is stored on the Mylar disk in the form of magnetic charges.
A protoplanetary disk is a concentration of gas and dust around a young star that eventually comes together to form planets. As the material in the disk begins to clump together due to gravity, it forms planetesimals which then grow into planets through accretion and collisions.
solar system Material that is in orbit around a massive central body is an accretion disk. This disk can eventually turn into a white dwarf star. An accretion disc may eventually form planets such as the ones in our solar system.
The solar disk formed from a rotating cloud of gas and dust, known as the solar nebula, approximately 4.6 billion years ago. Under the influence of gravity, the material in the nebula collapsed, leading to the formation of the Sun at its center. As the surrounding material continued to coalesce, it flattened into a protoplanetary disk, where particles collided and stuck together, ultimately forming planets, moons, and other bodies in the solar system. This process is a fundamental aspect of star and planetary formation in the universe.