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Saturn is the sixth planet from the Sun and the second largest in the Solar System, after Jupiter. ... Saturn has a hot interior, reaching 11,700 °C ...
On Saturn, this helium condensation occurs at certain pressures and temperatures when helium does not mix in with the liquid metallic hydrogen present on the planet. [20] Regions on Saturn where helium is insoluble allow the denser helium to form droplets and act as a source of energy, both through the release of latent heat and by descending ...
Most planets so mapped have been large and close-orbiting "hot Jupiters". Speculation on the appearances of unseen extrasolar planets currently relies upon computational models of the likely atmosphere of such a planet, for instance how the atmospheric temperature–pressure profile and composition would respond to varying degrees of insolation.
Something Weird Is Going On Inside Saturn We may have found water on Mars, but something far stranger is happening inside Saturn. Astronomers have noticed unusual movement in Saturn's rings.
A theoretical planet that may form via mass loss from a low-mass white dwarf. Helium planets are predicted to have roughly the same diameter as hydrogen–helium planets of the same mass. Hycean planet: A hypothetical type of habitable planet described as a hot, water-covered planet with a hydrogen-rich atmosphere. Ice giant
A giant planet, sometimes referred to as a jovian planet (Jove being another name for the Roman god Jupiter), is a diverse type of planet much larger than Earth. Giant planets are usually primarily composed of low- boiling point materials ( volatiles ), rather than rock or other solid matter, but massive solid planets can also exist.
Well, every 13-15 years, Saturn, the second largest planet in the solar system behind Jupiter, is angled in a way in which the edge of its thin rings are oriented toward Earth – effectively ...
Jupiter and Saturn most likely formed around previously existing rocky and/or icy bodies, rendering these previous primordial planets into gas-giant cores. [5] This is the planetary core accretion model of planet formation.