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  2. Volcanism on Mars - Wikipedia

    en.wikipedia.org/wiki/Volcanism_on_Mars

    However, the largest volcano on the planet, Olympus Mons, is thought to have formed when the plates were not moving. Olympus Mons may have formed just after the plate motion stopped. The mare-like plains on Mars are roughly 3 to 3.5 billion years old. [72] The giant shield volcanoes are younger, formed between 1 and 2 billion years ago.

  3. Water frost detected on Mars volcanoes in ‘unexpected’ first

    www.aol.com/water-frost-detected-mars-volcanoes...

    Using cameras fitted on probes orbiting Mars, researchers have observed morning frost forming inside the calderas of the planet’s volcanoes for the first time. Water frost detected on Mars ...

  4. Hecates Tholus - Wikipedia

    en.wikipedia.org/wiki/Hecates_Tholus

    The eruption which formed the caldera of Hecates Tholus took place 350 million years ago. [8] However, the volcano itself dates back to the Hesperian period of Mars' history, [9] and is at least 3.8 billion years old. [10] Volcanic activity lasted until at least 335 million years ago, [10] and potentially as recent as 100 million years ago ...

  5. Geological history of Mars - Wikipedia

    en.wikipedia.org/wiki/Geological_history_of_Mars

    Pre-Noachian: the interval from the accretion and differentiation of the planet about 4.5 billion years ago to the formation of the Hellas impact basin, between 4.1 and 3.8 Gya. [13] Most of the geologic record of this interval has been erased by subsequent erosion and high impact rates.

  6. Mud volcanoes on Mars hint at ancient water reservoirs

    www.aol.com/mud-volcanoes-mars-hint-ancient...

    Arsia Mons once spewed molten rock across the surface of Mars, but some smaller volcanic features may have come from another source. In a select few places on Earth, mud erupts rather than molten ...

  7. Common surface features of Mars - Wikipedia

    en.wikipedia.org/wiki/Common_surface_features_of...

    Volcanoes, wind, or water can produce layers. [8] A detailed discussion of layering with many Martian examples can be found in Sedimentary Geology of Mars. [9] Layers can be hardened by the action of groundwater. Martian ground water probably moved hundreds of kilometers, and in the process it dissolved many minerals from the rock it passed ...

  8. Perseverance rover will uncover mysterious Martian history ...

    www.aol.com/perseverance-rover-prepares...

    The team suspects the bedrock was broken by an impact that occurred when a celestial body slammed into Mars 3.9 billion years ago, creating a 745-mile-wide (1,200-kilometer) basin that scattered ...

  9. Elysium Mons - Wikipedia

    en.wikipedia.org/wiki/Elysium_Mons

    Elysium Mons / ɪ ˈ l ɪ z i ə m ˈ m ɒ n z / is a volcano on Mars located in the volcanic province Elysium, at , in the Martian eastern hemisphereIt stands about 12.6 km (41,000 ft) above its base, [2] and about 14.1 km (46,000 ft) above the Martian datum, [2] making it the third tallest Martian mountain in terms of relief and the fourth highest in elevation.