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Uranus - Wikipedia
Diagram of the interior of Uranus, listing each layer's composition. The extreme pressure and temperature deep within Uranus may break up the methane molecules, with the carbon atoms condensing into crystals of diamond that rain down through the mantle like hailstones. See more
Uranus orbits the Sun once every 84 years. As viewed against the background of stars, since being discovered in 1781, the planet has … See more
Although there is no well-defined solid surface within Uranus's interior, the outermost part of Uranus's gaseous envelope that is accessible to remote sensing is called its See more
Like the classical planets, Uranus is visible to the naked eye, but it was never recognised as a planet by ancient observers because of its dimness and slow orbit. See more
It is argued that the differences between the ice giants and the gas giants arise from their formation history. The Solar System is … See more
Uranus's mass is roughly 14.5 times that of Earth, making it the least massive of the giant planets. Its diameter is slightly larger than Neptune's at … See more
Wikipedia text under CC-BY-SA license Uranus | Facts, Moons, & Rings | Britannica
1 day ago · Uranus, seventh planet in distance from the Sun and the least massive of the solar system’s four giant, or Jovian, planets. Uranus has more than two dozen moons, five of which (Umbriel, Miranda, Ariel, Titania, and …
Uranus Facts - Science@NASA
Uranus is a very cold and windy world. The ice giant is surrounded by 13 faint rings and 28 small moons. Uranus rotates at a nearly 90-degree angle from the plane of its orbit. This unique tilt makes Uranus appear to spin sideways, …
Uranus - NASA Science
Uranus is a very cold and windy planet. It is surrounded by faint rings, and more than two dozen small moons as it rotates at a nearly 90-degree angle from the plane of its orbit. This unique tilt makes Uranus appear to spin on its side.
In Depth | Uranus – NASA Solar System Exploration
The interiors of Uranus and Neptune: current …
Nov 9, 2020 · Interior models of Uranus and Neptune assuming adiabatic temperature profiles with distinct layers have been presented by Nettelmann et al. . In these models, the planets are assumed to consist of a rocky core …
The interior of Uranus - Thermal profile, bulk composition, and the ...
The Interior of Uranus - Solar System
Our knowledge of the internal structure of Uranus is inferred from the planet's radius, mass, period of rotation, the shape of its gravitational field and the behavior of hydrogen, helium, and water at high pressure.
The interiors of Uranus and Neptune: current understanding and …
Uranus and Neptune: Origin, Evolution and Internal …
Mar 25, 2020 · Traditional interior models of Uranus and Neptune assume an “adiabatic” structure all the way to the interior, i.e., a temperature profile set by the specific entropy of hydrogen and helium measured in the atmosphere …