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Planets --- Geology. --- Earth (Planet) --- Mars (Planet) --- Surface. --- Geology --- Earth analogs. --- Planetary geology --- Astrogeology --- Crust
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Mars (Planet) --- Geology. --- Geological mapping. --- Cartographie géologique. --- Planets --- Planetary geology --- Astrogeology --- Geologic mapping --- Cartography
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Solar system --- Planets --- Planetology --- Planètes --- Planétologie --- Geology --- Géologie --- Geology. --- -Geology --- Planetary science. --- Planètes --- Planétologie --- Géologie --- Planetary geology --- Astrogeology --- Astronomie --- Planets - Geology.
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This book describes the tectonic landforms resulting from major internal and external forces acting on the outer layers of solid bodies throughout the Solar System. It presents a detailed survey of tectonic structures at a range of length scales found on Mercury, Venus, the Moon, Mars, the outer planet satellites, and asteroids. A diverse range of models for the sources of tectonic stresses acting on silicate and icy crusts is outlined, comparing processes acting throughout the Solar System. Rheological and mechanical properties of planetary crusts and lithospheres are discussed to understand how and why tectonic stresses manifest themselves differently on various bodies. Results from fault population data are assessed in detail. The book provides methods for mapping and analysing planetary tectonic features, and is illustrated with diagrams and spectacular images returned by manned and robotic spacecraft. It forms an essential reference for researchers and students in planetary geology and tectonics.
Geology, Structural. --- Plate tectonics. --- Tectonics, Plate --- Geodynamics --- Geotectonics --- Structural geology --- Tectonics (Geology) --- Physical geology --- Solar system. --- Milky Way --- Planets --- Planetary geology --- Astrogeology --- Geology.
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Solar system --- Planets --- Geology --- 523.4 --- -Planets and their satellites. Planetology --- Internal structure --- -523.4 Planets and their satellites. Planetology --- Planets and their satellites. Planetology --- Planetary geology --- Astrogeology --- 523.4 Planets and their satellites. Planetology --- Domaine extra-terrestre --- Geologie regionale
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Frozen ground --- Planets --- Glaciology --- Cryosphere --- Cryosphere. --- Frozen ground. --- Glaciology. --- Geology --- Geology. --- Cold regions --- Cold regions. --- Planetary geology --- Cryology --- Geology, Glacial --- Glacial geology --- Glaciogeology --- Frozen soil --- Chinosphere --- Astrogeology --- Hydrology --- Glaciers --- Soils --- Cryopedology --- Earth (Planet)
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Given the fundamental importance of and universal interest in whether extraterrestrial life has developed or could eventually develop in our solar system and beyond, it is vital that an examination of planetary habitability goes beyond simple assumptions such as, "Where there is water, there is life." This book has resulted from a workshop at the International Space Science Institute (ISSI) in Bern, Switzerland (5-9 September 2005) that brought together planetary geologists, geophysicists, atmospheric scientists, and biologists to discuss the multi-faceted problem of how the habitability of a planet co-evolves with the geology of the surface and interior, the atmosphere, and the magnetosphere. Each of the six chapters has been written by authors with a range of expertise so that each chapter is itself multi-disciplinary, comprehensive, and accessible to scientists in all disciplines. These chapters delve into what life needs to exist and ultimately to thrive, the early environments of the young terrestrial planets, the role of volatiles in habitability, currently habitable (but possibly not inhabited) geologic environments, the connection between a planet's inner workings and the habitability of its surface, and the effects on planetary atmospheres of solar evolution and the presence or absence of a magnetosphere. This book serves as a useful reference for those who plan missions that will hunt for biomarkers (especially on Mars), for biologists and geoscientists who seek a broader view of the story, and for researchers and upper level students interested in an in-depth review of the geologic evolution of terrestrial planets, from their cores to their magnetospheres, and how that evolution shapes the habitability of the planetary surface.
Planets --- Habitable planets. --- Life on other planets. --- Geology. --- Extraterrestrial life --- Fermi's paradox --- Earth-like planets --- Earthlike planets --- Extrasolar planets --- Exobiology --- Planetary geology --- Astrogeology --- Astrophysics. --- Astrobiology. --- Planetology. --- Space Sciences (including Extraterrestrial Physics, Space Exploration and Astronautics). --- Planetary sciences --- Planetology --- Astronomical physics --- Astronomy --- Cosmic physics --- Physics --- Astrobiology --- Biology --- Habitable planets --- Life --- Origin --- Space sciences. --- Science and space --- Space research --- Cosmology --- Science
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In the early days of planetary observation, oceans were thought to exist in all corners of the Solar System. Carbonated seas percolated beneath the clouds of Venus. Features on the Moon's surface were given names such as "the Bay of Rainbows” and the "Ocean of Storms." With the advent of modern telescopes and spacecraft exploration these ancient concepts of planetary seas have been replaced by the reality of something even more exotic. Alien Seas serves up the current research, past beliefs, and new theories to offer a rich array of the "seas" on other worlds. It is organized by location and by the material composing the oceans under discussion, with expert authors penning chapters on their specialty. Each chapter features new original art depicting alien seas, as well as the latest ground-based and spacecraft images. With the contributors as guides, readers can explore the wild seas of Jupiter's watery satellite Europa, believed similar in composition to battery acid. Saturn's planet-sized moon Titan seems to be subject to methane or ethane rainfall that become vast lakes and, perhaps, seasonal oceans. Titan and Mars have seas of sand, large shifting dunes covering huge plains, while Venus may have ‘oceans’ of frozen lava. The possibilities are excitingly endless and ripe for exploration. Contributors: Kevin Baines Jeffrey Bennett James Cameron Michael Carroll Mona Delitsky David Grinspoon Rosaly Lopes Christopher P. McKay Karl Mitchell Robert Pappalardo Timothy Parker Jani Radebaugh John Spencer.
Planets --- Seas --- Ocean --- Astronomy & Astrophysics --- Physical Sciences & Mathematics --- Astrophysics --- Surfaces --- Water --- Surfaces. --- Geology. --- Planetary geology --- Surfaces, Planet --- Physics. --- Planetology. --- Space sciences. --- Astronomy. --- Extraterrestrial Physics, Space Sciences. --- Popular Science in Astronomy. --- Astrogeology --- Astrophysics. --- Space Sciences (including Extraterrestrial Physics, Space Exploration and Astronautics). --- Planetary sciences --- Planetology --- Astronomical physics --- Astronomy --- Cosmic physics --- Physics --- Science and space --- Space research --- Cosmology --- Science
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523.4 --- Geophysics --- Planets --- -Planets --- -Geological physics --- Terrestrial physics --- Earth sciences --- Physics --- Planets and their satellites. Planetology --- Figure --- Geology --- Internal structure --- Geophysics. --- Figure. --- Geology. --- Internal structure. --- -Planets and their satellites. Planetology --- 523.4 Planets and their satellites. Planetology --- Geological physics --- Planetary geology --- Astrogeology
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Basalt. --- Volcanism. --- Planets --- Planetary volcanism. --- Geology. --- 552.3 --- Basalt --- Planetary volcanism --- Volcanism --- Basaltic rocks --- Igneous rocks --- 552.3 Magmatic rocks. Igneous rocks --- Magmatic rocks. Igneous rocks --- Geology --- Planetary geology --- Volcanicity --- Vulcanism --- Astrogeology --- Geodynamics --- Volcanology --- DOMAINE EXTRA-TERRESTRE --- GEOLOGIE REGIONALE --- PETROLOGIE ROCHES IGNEES --- ROCHES IGNEES BASIQUES, ULTRA-BASIQUES --- PETROLOGIE ROCHES CRISTALLINES
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