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  2. Planetary core - Wikipedia

    en.wikipedia.org/wiki/Planetary_core

    All of the rocky inner planets, as well as the moon, have an iron-dominant core. Venus and Mars have an additional major element in the core. Venus’ core is believed to be iron-nickel, similarly to Earth. Mars, on the other hand, is believed to have an iron-sulfur core and is separated into an outer liquid layer around an inner solid core. [20]

  3. Composition of Mars - Wikipedia

    en.wikipedia.org/wiki/Composition_of_Mars

    Mars is differentiated, which—for a terrestrial planet—implies that it has a central core made up of high density matter (mainly metallic iron and nickel) surrounded by a less dense, silicate mantle and crust. [4] Like Earth, Mars appears to have a molten iron core, or at least a molten outer core. [5]

  4. Lava planet - Wikipedia

    en.wikipedia.org/wiki/Lava_planet

    Artist's impression of CoRoT-7b, likely a lava exoplanet. A lava planet is a type of terrestrial planet, with a surface mostly or entirely covered by molten lava.Situations where such planets could exist include a young terrestrial planet just after its formation, a planet that has recently suffered a large collision event, or a planet orbiting very close to its star, causing intense ...

  5. Geology of solar terrestrial planets - Wikipedia

    en.wikipedia.org/wiki/Geology_of_solar...

    The terrestrial planets all have roughly the same structure: a central metallic core, mostly iron, with a surrounding silicate mantle. The Moon is similar, but lacks a substantial iron core. [ 1 ] Three of the four solar terrestrial planets (Venus, Earth, and Mars) have substantial atmospheres ; all have impact craters and tectonic surface ...

  6. List of planet types - Wikipedia

    en.wikipedia.org/wiki/List_of_planet_types

    A class of extrasolar planets whose characteristics are similar to Jupiter, but that have high surface temperatures because they orbit very close—between approximately 0.015 and 0.5 AU (2.2 × 10 ^ 6 and 74.8 × 10 ^ 6 km)—to their parent stars, whereas Jupiter orbits its parent star (the Sun) at 5.2 AU (780 × 10 ^ 6 km), causing low ...

  7. Internal heating - Wikipedia

    en.wikipedia.org/wiki/Internal_heating

    Internal heat is the heat source from the interior of celestial objects, such as stars, brown dwarfs, planets, moons, dwarf planets, and (in the early history of the Solar System) even asteroids such as Vesta, resulting from contraction caused by gravity (the Kelvin–Helmholtz mechanism), nuclear fusion, tidal heating, core solidification (heat of fusion released as molten core material ...

  8. Astronomers find the biggest known batch of planet ... - AOL

    www.aol.com/news/astronomers-biggest-known-batch...

    The diameter of this colossal disk is roughly 3,300 times the distance between Earth and the sun, with enough gas and dust to form super-sized planets in far-flung orbits, the U.S. and German ...

  9. Planetary differentiation - Wikipedia

    en.wikipedia.org/wiki/Planetary_differentiation

    The Earth's core is primarily composed Fe-Ni alloys. Based on the studies of short lived radionuclides, the results suggest that core formation process occurred during an early stage of the solar system. [4] Siderophile elements such as, sulfur, nickel, and cobalt can dissolve in molten iron; these elements help the differentiation of iron ...