Volatiles in the Martian Crust is a vital reference for future missions - including ESA’s EXO Mars and NASA’s Mars2020 rover - looking for evidence of life on Mars and the potential for habitability and human exploration of the Martian crust. Mars science is a rapidly evolving topic with new data returned from the planet on a daily basis. The book presents chapters written by well-established experts who currently focus on the topic, providing the reader with a fresh, up-to-date and accurate view. Organized into two main sections, the first half of the book focuses on the Martian meteorites and specific volatile elements. The second half of the book explores processes and locations on the crust, including what we have learned about volatile mobility in the Martian crust. Coverage includes data from orbiter and in situ rovers and landers, geochemical and geophysical modeling, and combined data from the SNC meteorites. Presents information about the nature, relationship, and reactivity of chemical elements and compounds on Mars Explores the potential habitability of Mars Provides a comprehensive view of volatiles in the Martian crust from studies of actual samples as well as from the variety of landed missions, including the MER and Curiosity rovers Delivers a vital reference for ongoing and future missions to Mars while synthesizing large data sets and research on volatiles in the Martian atmosphere Concludes with an informative summary chapter that looks to future Mars missions and what might be learned
This new volume brings together the many new ideas about the atmosphere and climate system that have emerged, including the complex interplay of the volatile and dust cycles, the atmosphere-surface interactions that connect them over time, ...
Filiberto J., McCubbin F. M., and Taylor G. J. (2019) Volatiles in martian magmas and the interior: Inputs of volatiles into the crust and atmosphere. In Volatiles in the Martian Crust, Filibert J., and Schwenzer S., editors., pp.
But the global system includes much more than the volatiles – volcanic outpourings , impacts , and crustal fracturing are all a part of the story , as is the Sun and the cosmic dance of the planets . NIX OLYMPICA Mariner 9's first ...
From this, the majority of the Tharsis crust is constructed in the Noachian [26], but where extensive volcanic ... from the Martian highland crust required a rapid release of volatiles from the interior, forming an early atmosphere of ...
There are geological formations of Mars which are more peculiar to the Earth , rather than to the Moon or Mercury . ... The presence of volatiles in the Martian crust also becomes apparent in the eolian nature of the surface substance .
Mars Geological Enigmas: From the Late Noachian Epoch to the Present Day presents outstanding questions on the geology of Mars and divergent viewpoints based on varying interpretations and analyses.
One of Springer’s Major Reference Works, this book gives the reader a truly global perspective. It is the first major reference work in its field.
As mentioned earlier, the Proterozoic was warm during its middle part but extremely cold on both ends. Indeed, both the Paleoproterozoic and Neoproterozoic glaciations are thought by some geologists to have been “Snowball Earth” ...
A comprehensive guide to carbon inside Earth - its quantities, movements, forms, origins, changes over time and impact on planetary processes. This title is also available as Open Access on Cambridge Core.
These issues will be addressed by examining the different types of water worn features and what they might imply about the hydrologic history of the planet. Three classes of likely water worn features are recognized. Outflow channels ...