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  1. Dec 12, 2017 · Heating and cooling. Like all planets, Mars became hot as it formed because of the energy from these collisions. The planet's interior melted and denser elements such as iron sank to the center ...

  2. When the solar system settled into its current layout about 4.5 billion years ago, Mars formed when gravity pulled swirling gas and dust in to become the fourth planet from the Sun. Mars is about half the size of Earth, and like its fellow terrestrial planets, it has a central core, a rocky mantle, and a solid crust.

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  3. Jun 5, 2013 · Debates in the scientific community focus on how the interior and crust of Mars formed and how they differ from those of Earth. To investigate the history of Martian water and other volatiles, scientists at JSC, the Carnegie Institution in Washington, and the Lunar and Planetary Institute in Houston compared water concentrations and hydrogen isotopes trapped in crystals within the meteorites.

  4. en.wikipedia.org › wiki › MarsMars - Wikipedia

    Mars is the fourth planet from the Sun. The surface of Mars is orange-red because it is covered in iron (III) oxide dust, giving it the nickname " the Red Planet ". [22][23] Mars is among the brightest objects in Earth's sky, and its high-contrast albedo features have made it a common subject for telescope viewing.

  5. When the solar system settled into its current layout about 4.5 billion years ago, Mars formed when gravity pulled swirling gas and dust in to become the fourth planet from the Sun. Mars is about half the size of Earth, and like its fellow terrestrial planets, it has a central core, a rocky mantle, and a solid crust. Structure. Structure

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  7. With a radius of 2,106 miles, Mars is the seventh largest planet in our solar system and about half the diameter of Earth. Its surface gravity is 37.5 percent of Earth’s. Mars rotates on its ...

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