young stars are found to have hot disks that surround them.
your welcome
The Solar Nebula Hypothesis was developed independently by Soviet astrophysicist Victor Safronov and American astrophysicist Carl Woese in the 1960s. They proposed that the solar system formed from a swirling cloud of gas and dust called the solar nebula.
The hypothesis on how the solar system was formed is known as the solar nebula theory. This theory posits that the solar system formed from a massive, rotating cloud of gas and dust called the solar nebula. Over time, gravity caused the material in the nebula to clump together, eventually forming the sun and the planets.
The nebular hypothesis suggests that the solar system formed from a rotating cloud of gas and dust, known as a solar nebula. As this nebula collapsed under its own gravity, it spun faster and flattened into a disk, causing material to clump together and form the Sun at its center, while planets, moons, and other celestial bodies formed from the remaining material. This theory explains the observed patterns of motion and composition in the solar system.
It was found by a German man named Seemore Butts. He had a hairy face and chest and butt.
The Solar nebula hypothesis is supported by several lines of evidence, including the observation of protoplanetary disks around young stars, which resemble the proposed structure of our early solar system. Additionally, the distribution of angular momentum in the solar system, with the Sun containing most of the mass and planets forming a flat disk, aligns with predictions of the hypothesis. The chemical composition of the planets, which reflects the solar nebula's materials, further corroborates this model. Lastly, computer simulations of the collapse of gas and dust clouds consistently produce outcomes that resemble the formation of our solar system.
your welcome
The Solar Nebula Hypothesis was developed independently by Soviet astrophysicist Victor Safronov and American astrophysicist Carl Woese in the 1960s. They proposed that the solar system formed from a swirling cloud of gas and dust called the solar nebula.
The hypothesis on how the solar system was formed is known as the solar nebula theory. This theory posits that the solar system formed from a massive, rotating cloud of gas and dust called the solar nebula. Over time, gravity caused the material in the nebula to clump together, eventually forming the sun and the planets.
The super nebula hypothesis proposes that massive stars can form in areas where the gas density is high enough to trigger the formation of multiple stars within a single giant molecular cloud complex. This hypothesis suggests that these super nebulas are responsible for the formation of massive star clusters seen in the universe.
The nebular hypothesis suggests that the solar system formed from a rotating cloud of gas and dust, known as a solar nebula. As this nebula collapsed under its own gravity, it spun faster and flattened into a disk, causing material to clump together and form the Sun at its center, while planets, moons, and other celestial bodies formed from the remaining material. This theory explains the observed patterns of motion and composition in the solar system.
The correct term is planetary nebula. Such nebulae form when a low to medium mass star dies.
It was found by a German man named Seemore Butts. He had a hairy face and chest and butt.
The hypothesis you're referring to is the Nebular Hypothesis. It proposes that the solar system formed from a giant rotating cloud of gas and dust, known as a solar nebula. As this nebula collapsed under its own gravity, it spun faster and flattened into a disk, leading to the formation of the Sun at its center and the planets from the surrounding material. This process explains the structure and composition of the solar system as we observe it today.
The nebular hypothesis attempts to explain the formation and evolution of the solar system. It posits that the solar system formed from a rotating cloud of gas and dust, known as a solar nebula, which collapsed under its own gravity. As the nebula contracted, it spun faster, flattening into a disk and eventually leading to the formation of the Sun at its center and the planets from the remaining material. This hypothesis addresses the structure and dynamics of planetary systems and their development over time.
The nebular hypothesis suggests that our solar system evolved from a huge rotating cloud of gas and dust, known as a solar nebula. Over time, this cloud collapsed under its own gravity, leading to the formation of the Sun at its center and the planets, moons, and other celestial bodies from the remaining material. This process involved the condensation, accretion, and differentiation of matter within the nebula.
The nebular hypothesis is a widely-accepted theory that explains the formation of the solar system. It suggests that the Sun and planets formed from a spinning disk of gas and dust called a solar nebula. As the nebula contracted due to gravity, it flattened into a disk and the Sun formed at the center, while planets and other celestial bodies formed from material in the disk.