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  1. 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.

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

    The geological history of Mars can be split into many periods, but the following are the three primary periods: Noachian period: Formation of the oldest extant surfaces of Mars, 4.5 to 3.5 billion years ago. Noachian age surfaces are scarred by many large impact craters.

    • 24.07 km/s, (86700 km/h; 53800 mph)
    • 1.025957 d, 24ʰ 37ᵐ 22.7ˢ
    • 241 m/s, (870 km/h; 540 mph)
  3. Mars is one of the most explored bodies in our solar system, and it's the only planet where we've sent rovers to explore the alien landscape. NASA missions have found lots of evidence that Mars was much wetter and warmer, with a thicker atmosphere, billions of years ago. Explore with Us

  4. 21 de ago. de 2023 · By Michael Greshko. 11 min read. The red planet Mars, named for the Roman god of war, has long been an omen in the night sky. And in its own way, the planet’s rusty red surface tells a story of...

  5. 10 min read. Mars has captivated humans since we first set eyes on it as a star-like object in the night sky. Early on, its reddish hue set the planet apart from its shimmering siblings, each...

  6. 1 de sept. de 2019 · The geological history of Mars has been divided into three main periods, each named after a region of Mars: Noachian, Hesperian, and Amazonian. An earlier, Pre-Noachian, period has also been identified, even though no physical evidence for its existence remains.