A whirling cloud of gas or dust that becomes a planet by condensation during formation of a solar system. As the central body, or protostar, of the system contracts and heats up
The leading scientific theory on the origin of the moon suggests that it formed from debris left over after a giant impact between Earth and a Mars-sized protoplanet called Theia around 4.5 billion years ago. This collision resulted in the debris coalescing to form the moon in orbit around Earth.
The three main theories on the origin of the Earth are the nebular hypothesis, the giant impact hypothesis, and the core accretion theory. The nebular hypothesis proposes that the solar system formed from a rotating cloud of dust and gas, while the giant impact hypothesis suggests that Earth formed from a collision between a Mars-sized protoplanet and the early Earth. The core accretion theory posits that planets formed from the gradual accumulation of solid particles in a protoplanetary disk.
Some scientific theories explaining the origin of Earth include the nebular hypothesis, which suggests that the solar system formed from a rotating disk of gas and dust, and the giant impact hypothesis, which proposes that the Moon formed from debris created by a collision between Earth and a Mars-sized protoplanet. Other theories include the core accretion model for planet formation and the theory of planetary migration.
The Earth never collapsed. In the beginning of formation (about 4.6 billion years ago), however, it is theorized that a protoplanet, the size of Mars, sideswiped the Earth and caused a portion of both to break apart. The pieces came together and formed the Moon. It is also theorized that the Earth became a snow ball twice. There were also asteroid impacts on Earth, some severe enough to end most of life, but the Earth itself stayed intact.
The oldest moon rocks are actually older than the oldest Earth rocks. The moon formed from accreted material that resulted from a collision between Earth and a Mars sized protoplanet. Both the Earth and the moon were molten for a period after the collision. Because of the moon's smaller size, it's surface cooled very quickly compared to the Earth. The solidified magma (rock) that formed the moon's crust has been dated at roughly 4.4 billion years of age. Even though no Earth rock has been found to date this old, we can still reasonably assume that the Earth is at least that old due to the fact that the moon is formed from accreted material from the previously mentioned collision.
An early collision by (proto) Earth with a large protoplanet..
The protoplanet hypothesis describes the formation of planets from the dust and gas present in the early solar system. It suggests that small planetesimals collided and merged to form larger celestial bodies, eventually leading to the creation of the planets we see today.
Yes, that is how Earth's formed, it hit a large protoplanet called Theia.
Currently, the most accepted theory is that it resulted from a crash between a large planetoid (or "protoplanet") and Earth.
There are several, but one of the more popular is that a protoplanet about the size of Mars originally shared Earth's orbit. It crashed into Earth, and threw off a gigantic cloud of debris that coalesced into the Moon. If you'd like to read more about this, look up "Theia", the name given to this hypothetical protoplanet.
I think you mean "protoplanet hypothesis". In fact, astronomers usually call it the Nebular Hypothesis A protoplanet is a planet-like object that hasn't fully developed into a planet. Why that hypothesis? It's because it is the best we have to describe the origin of the solar system according to the Laws of Physics.
The protoplanet underwent differentiation, where heat caused materials to separate based on their density. The heavy elements sank to the core, while lighter materials floated to the surface, forming layers. This process is important in planetary formation as it leads to the creation of distinct layers within a planet.
An asteroid is a minor planet that can lean towards terrestrial objects such as the rocky protoplanet-asteroids of Vesta and Pallas.
No one was around at the time, so we're not really sure, but the current hypothesis in favor is called the "Giant Impact Hypothesis." It posits that a protoplanet about the same size as the current planet Mars struck the proto-Earth while it was still forming, and "splashed" a lot of rock off. This eventually formed the Moon, while the rest of this protoplanet (named Theia) joined with the Earth.
The primary sources of heat for protoplanets during their formation were gravitational collapse, radioactive decay of elements within the planet, and impacts from other celestial bodies. These heat sources contributed to melting the protoplanet's interior and driving geological processes like differentiation and magma ocean formation.
The planet Mercury originated from the protoplanet closest to the sun. It is one of the four rocky inner planets in our solar system.
The hypothesis states that during the formation of a star, the original nebula disk may be so massive that upon further contraction and flattening, it breaks into separate clouds (vortices) or protoplanets.