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Lakes on Mars (Paperback)
Loot Price: R3,100
Discovery Miles 31 000
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Lakes on Mars (Paperback)
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On Earth, lakes provide favorable environments for the development
of life and its preservation as fossils. They are extremely
sensitive to climate fluctuations and to conditions within their
watersheds. As such, lakes are unique markers of the impact of
environmental changes. Past and current missions have now
demonstrated that water once flowed at the surface of Mars early in
its history. Evidence of ancient ponding has been uncovered at
scales ranging from a few kilometers to possibly that of the Arctic
ocean. Whether life existed on Mars is still unknown; upcoming
missions may find critical evidence to address this question in
ancient lakebeds as clues about Mars' climate evolution and its
habitability potential are still preserved in their sedimentary
record. Lakes on Mars is the first review on this subject. It is
written by leading planetary scientists who have dedicated their
careers to searching and exploring the questions of water, lakes,
and oceans on Mars through their involvement in planetary
exploration, and the analysis of orbital and ground data beginning
with Viking up to the most recent missions. In thirteen chapters,
Lakes on Mars critically discusses new data and explores the role
that water played in the evolution of the surface of Mars, the past
hydrological provinces of the planet, the possibility of heated
lake habitats through enhanced geothermal flux associated with
volcanic activity and impact cratering. The book also explores
alternate hypotheses to explain the geological record. Topographic,
morphologic, stratigraphic, and mineralogic evidence are presented
that suggest successions of ancient lake environments in Valles
Marineris and Hellas. The existence of large lakes and/or small
oceans in Elysium and the Northern Plains is supported both by the
global distribution of deltaic deposits and by equipotential
surfaces that may reflect their past margins. Whether those
environments were conducive to life has yet to be demonstrated but
from comparison with our planet, their sedimentary deposits may
provide the best opportunity to find its record, if any. The final
chapters explore the impact of climate variability on declining
lake habitats in one of the closest terrestrial analogs to Mars at
the Noachian/Hesperian transition, identify the geologic,
morphologic and mineralogic signatures of ancient lakes to be
searched for on Mars, and present the case for landing the Mars
Science Laboratory mission in such an environment.
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