How is a planet form?

Answer 1

Leftover matter around the sun after the sun forms. It eventually falls together via gravitational forces to form planets.

Answer 2

Hi:

Watch the Show on the Science Channel entitled "The Planets" and "the Sun" or Get the book or DVD of "Cosmos" by the late Carl Segan that should answer your question quite well

other show to watch that will answer your question are:

The Mechanical Universe by Cal Tech Available from Cal Tech

"Hot Rock" - Science Channel

The History Channel - Meteors- Fire from the Sky


Get the Time Life Science Series entitled:

The Universe

The Planets

The Scientist

Matter

Answer 3

The planets formed from the material left over as a result of our sun's formation. As the nebulous cloud condensed and began to rotate, most of the gas condensed into what is now our sun. The remaining material formed what is now the planets and the other bodies in our solar system

Answer 4

A protoplanetary disk (or proplyd) is a rotating disk of dense gas surrounding a young newly formed star (a T Tauri star). The protoplanetary disk may be considered an accretion disk because gaseous material may be falling from the inner edge of the disk onto the surface of the star, but this process should not be confused with the accretion process thought to build up the planets themselves.

Protoplanetary disks around T Tauri stars differ from the discs surrounding the primary components of close binary systems in their size and temperature. Protoplanetary discs have radii up to 1000 astronomical units and are rather cool. Only their innermost parts reach temperatures above 1000 kelvins. They are very often accompanied by jets.

Protostars typically form from molecular clouds consisting primarily of molecular hydrogen. When a portion of a molecular cloud reaches a critical size, mass, or density, it begins to collapse under its own gravity. As this collapsing cloud, called a solar nebula, becomes more dense, random gas motions originally present in the cloud average out in favor of the direction of the nebula's net angular momentum. Conservation of angular momentum causes the rotation to increase as the nebula becomes smaller. This rotation causes the cloud to flatten out - much like forming a flat pizza out of dough - and take the form of a disk. The initial collapse takes about 100,000 years. After that time the star reaches a surface temperature similar to that of a main sequence star of the same mass and becomes visible. It is now a T Tauri star. Accretion of gas onto the star continues for another 10 million years, before the disk disappears, perhaps being blown away by the young star's solar wind, or perhaps simply ceasing to emit radiation after accretion has ended. The oldest protoplanetary disk ever discovered is 25 million years old.

The nebular theory of solar system formation describes how protoplanetary disks are thought to evolve into planetary systems. Electrostatic and gravitational interactions may cause the dust and ice grains in the disk to accrete into planetesimals. This process competes against the stellar wind, which drives the gas out of the system, and accretion, which pulls material into the central T Tauri star.

Protoplanetary disks have been observed around several young stars in our galaxy, the first being found around the star Beta Pictoris in 1984. Recent observations by the Hubble Space Telescope have shown proplyds and planetary discs to be forming within the Orion Nebula.

Astronomers have discovered large discs of material, which may themselves be protoplanetary discs, around the stars Vega, Alphecca and Fomalhaut, all of which are very close to the Sun.

The Castor co-moving group of stars containing Vega and Fomalhaut has recently been isolated. Using data from the Hipparcos satellite telescope the Castor group was found to have an estimated age of 200 ± 100 million years. This indicates that the infrared excesses seen around Vega and Fomalhaut are likely due to a disk of debris from colliding planetesimals rather than a protoplanetary disk. Successful imaging of Fomalhaut's disk by the Hubble Space Telescope confirms this.

Answer 5

bye nebula's once the particles of ice and dust come to gather a star will explode and throw a bunch off balls like a grenade.This will create a solar system. so your question should be how is a solar system is made?.

Answer 6

i guesse from the big bang there are alot of theroys i hear thata astteroid about the same size of earth a long time ago hit the earth and the asteroid broke in 2 some of it stuck to the earth the other became the moon but thats a theory and its not wat you wanted to know but hey

Answer 7

A planet is form with rocks....................

Answer 8

jesus/god farts