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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 the Solar System is formed from gas and dust orbiting the Sun which clumped up together to form the planets.
The nebular hypothesis says that the Solar System formed from the gravitational collapse of a fragment of a giant molecular cloud, [10] most likely at the edge of a Wolf-Rayet bubble. [11] The cloud was about 20 parsecs (65 light years) across, [ 10 ] while the fragments were roughly 1 parsec (three and a quarter light-years ) across. [ 12 ]
One other problem is the detailed features of the planets. The solar nebula hypothesis predicts that all planets will form exactly in the ecliptic plane. Instead, the orbits of the classical planets have various small inclinations with respect to the ecliptic. Furthermore, for the gas giants, it is predicted that their rotations and moon ...
Solar Systems - Discusses solar systems and how they are formed. Includes topics such as the solar nebula theory and the detection of far away planets through the use of Doppler spectroscopy . The Terrestrial Planets - Details The formation and evolution of the Earth compared to other terrestrial planets.
A widely accepted theory of planet formation, the planetesimal hypothesis of Viktor Safronov, states that planets form from cosmic dust grains that collide and stick to form ever-larger bodies. Once a body reaches around a kilometer in size, its constituent grains can attract each other directly through mutual gravity , enormously aiding ...
As this collapsing cloud, called a solar nebula, becomes denser, 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 radius decreases. This rotation causes the cloud to flatten out—much like ...
At their distance from the Sun, accretion was too slow to allow planets to form before the solar nebula dispersed, because the initial disc lacked enough mass density to consolidate into a planet. The Kuiper belt lies between 30 and 55 AU from the Sun, while the farther scattered disc extends to over 100 AU, [ 43 ] and the distant Oort cloud ...
Formation and evolution of the Solar System; This page is a redirect. The following categories are used to track and monitor this redirect: From a page move: This is ...