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  2. Geological history of Mars - Wikipedia

    en.wikipedia.org/wiki/Geological_history_of_Mars

    The same methodology was later applied to the Moon [1] and then to Mars. [2] Another stratigraphic principle used on planets where impact craters are well preserved is that of crater number density. The number of craters greater than a given size per unit surface area (usually a million km 2) provides a relative age for that surface. Heavily ...

  3. Tectonics of Mars - Wikipedia

    en.wikipedia.org/wiki/Tectonics_of_Mars

    The Valles Marineris trough system, which is over 4000 km long, 600 km wide, and up to 7 km deep, would, if located on Earth, extend all the way across North America. [4] The study indicates that the Ius-Melas-Coprates fault zone is a left-slip transtensional system similar to that of the Dead Sea fault zone on Earth. [5]

  4. Geology of Mars - Wikipedia

    en.wikipedia.org/wiki/Geology_of_Mars

    For example, the peak discharge required to carve the 28-km-wide Ares Vallis is estimated to have been 14 million cubic metres (500 million cu ft) per second, over ten thousand times the average discharge of the Mississippi River. [41] Mars Orbital Laser Altimeter (MOLA) derived image of Planum Boreum. Vertical exaggeration is extreme.

  5. Timeline of natural history - Wikipedia

    en.wikipedia.org/wiki/Timeline_of_natural_history

    Geologic time is the timescale used to calculate dates in the planet's geologic history from its origin (currently estimated to have been some 4,600 million years ago) to the present day. Radiometric dating measures the steady decay of radioactive elements in an object to determine its age. It is used to calculate dates for the older part of ...

  6. Noachian - Wikipedia

    en.wikipedia.org/wiki/Noachian

    The lunar cratering record suggests that the rate of impacts in the Inner Solar System 4000 million years ago was 500 times higher than today. [44] During the Noachian, about one 100-km diameter crater formed on Mars every million years, [ 3 ] with the rate of smaller impacts exponentially higher.

  7. Mars carbonate catastrophe - Wikipedia

    en.wikipedia.org/wiki/Mars_carbonate_catastrophe

    The Mars carbonate catastrophe was an event that happened on Mars in its early history. Evidence shows Mars was once warmer and wet about 4 billion years ago, that is about 560 million years after the formation of Mars. Mars quickly, over a 1 to 12 million year time span, lost its water, becoming cold and very dry.

  8. One Scientist Believes We May Have Found Life On Mars 50 ...

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  9. Amazonian (Mars) - Wikipedia

    en.wikipedia.org/wiki/Amazonian_(Mars)

    Notes (Mars) Eonothem: Eon: not used for Mars Erathem: Era: not used for Mars System: Period: 3 total; 10 8 to 10 9 years in length Series: Epoch: 8 total; 10 7 to 10 8 years in length Stage: Age: not used for Mars Chronozone: Chron: smaller than an age/stage; not used by the ICS timescale