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- W97190641 abstract "Because of its many similarities to Earth, including its potential as an abode for past or present life, Mars has been the subject of intense international robotic space exploration over the past four decades. Here we summarize the major observations and results from these missions that pertain to the planet's surface and interior. Evidence exists for the long-term action of impacts, volcanism, tectonism, and erosion shaping the planet's geology and topography. Variations in the relative magnitude and influence of these processes have been used to define a simple geologic timescale for Mars that ranges from a warmer and wetter earliest ∼500 million years (Noachian), to a volcanically-dominated middle transitional period over the next ∼1 billion years (Hesperian), to the arid, wind-dominated regime of the last ∼3 billion years (Amazonian). Close-up observations by landers and rovers of a small number of carefully selected areas indicate that Mars once had the liquid water and energy sources required to make the surface habitable. Ongoing and future missions will focus on the associated search for the elements, molecules, and environments required to support past or present surface or subsurface life." @default.
- W97190641 created "2016-06-24" @default.
- W97190641 creator A5062630223 @default.
- W97190641 date "2014-01-01" @default.
- W97190641 modified "2023-09-25" @default.
- W97190641 title "Mars" @default.
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- W97190641 doi "https://doi.org/10.1016/b978-0-12-415845-0.00017-7" @default.
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