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  2. Jupiter - Wikipedia

    en.wikipedia.org/wiki/Jupiter

    Jupiter's helium abundance is 80% of the Sun's, similar to Saturn's composition. The ongoing contraction of Jupiter's interior generates more heat than the planet receives from the Sun. Its internal structure is believed to consist of an outer mantle of fluid metallic hydrogen and a diffuse inner core of

  3. Exoplanet interiors - Wikipedia

    en.wikipedia.org/wiki/Exoplanet_interiors

    Another proposed interior is a chthonian planet, a gas giant like a "hot Jupiter" that has had the outer hydrogen and helium layers stripped away leaving what looks like a rocky planet behind. [20] There are no confirmed examples of these proposed interior structures.

  4. Portal:Solar System/Selected article/10 - Wikipedia

    en.wikipedia.org/wiki/Portal:Solar_System/...

    Jupiter's helium abundance is 80% of the Sun's, similar to Saturn's composition. The ongoing contraction of Jupiter's interior generates more heat than the planet receives from the Sun. Its internal structure is believed to consist of an outer mantle of fluid metallic hydrogen and a diffuse inner core of

  5. Juno (spacecraft) - Wikipedia

    en.wikipedia.org/wiki/Juno_(spacecraft)

    Obtain a better estimate of Jupiter's core mass, which will also help distinguish among prevailing theories linking Jupiter's formation to the Solar System. Precisely map Jupiter's gravitational field to assess the distribution of mass in Jupiter's interior, including properties of its structure and dynamics.

  6. File:Jupiter diagram.svg - Wikipedia

    en.wikipedia.org/wiki/File:Jupiter_diagram.svg

    English: Diagram of Jupiter, its interior, surface features, rings, and inner moons. A 3D renderer was used to make the skeleton for this picture so everything is drawn to scale (except the aurorae). F-stop used is estimated at f/0.308. Sources: 1, 2, 3, and the wikipedia articles Jupiter & Rings of Jupiter.

  7. Atmosphere of Jupiter - Wikipedia

    en.wikipedia.org/wiki/Atmosphere_of_Jupiter

    While Jupiter has a small obliquity of about 3°, and its poles receive much less solar radiation than its equator, the tropospheric temperatures do not change appreciably from the equator to poles. One explanation is that Jupiter's convective interior acts like a thermostat, releasing more heat near the poles than in the equatorial region.

  8. NASA's stunning new photo of Jupiter looks like a work of art

    www.aol.com/article/news/2018/06/25/nasas...

    Jupiter may be best known as the planetary titan of our solar system with a comparatively small red mark — that still dwarfs the entirety of Earth — and rows of striations going from pole to pole.

  9. Planetary core - Wikipedia

    en.wikipedia.org/wiki/Planetary_core

    The internal structure of the inner planets. The internal structure of the outer planets. A planetary core consists of the innermost layers of a planet. [1] Cores may be entirely liquid, or a mixture of solid and liquid layers as is the case in the Earth. [2]