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Reyk (talk · contribs) Asteroids, small moons, history of the solar system, and anything that's not well understood; RSStockdale (talk · contribs) all; Ruslik0 (talk · contribs) Outer planets and satellites. Serendipodous (talk · contribs) Now focusing on the solar system featured topic, though Definition of planet has become an issue yet ...
Solar System project pages are rated as Project-Class on the Wikipedia 1.0 Assessment Scale. Add items to this category by typing {{WPSS|class=Project|importance=NA}} on the project page's talk page.
Solar System models, especially mechanical models, called orreries, that illustrate the relative positions and motions of the planets and moons in the Solar System have been built for centuries. While they often showed relative sizes, these models were usually not built to scale.
The following is a version of the five-planet Nice model that results in an early instability and reproduces a number of aspects of the current Solar System. Although in the past the giant planet instability has been linked to the Late Heavy Bombardment , a number of recent studies indicate that the giant planet instability occurred early .
The Solar System remains in a relatively stable, slowly evolving state by following isolated, gravitationally bound orbits around the Sun. [28] Although the Solar System has been fairly stable for billions of years, it is technically chaotic, and may eventually be disrupted. There is a small chance that another star will pass through the Solar ...
People around the world will have a chance this weekend to catch what could be the year’s most stunning view of the largest planet in our solar system. Jupiter on Saturday will shine at its ...
The original core of the Nice model is a triplet of papers published in the general science journal Nature in 2005 by an international collaboration of scientists. [4] [5] [6] In these publications, the four authors proposed that after the dissipation of the gas and dust of the primordial Solar System disk, the four giant planets (Jupiter, Saturn, Uranus, and Neptune) were originally found on ...
Later versions of the Nice model begin with the giant planets in a series of resonances. This change reflects some hydrodynamic models of the early Solar System.In these models, interactions between the giant planets and the gas disk result in the giant planets migrating toward the central star, in some cases becoming hot Jupiters. [11]
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