Relevant bibliographies by topics / Mars (Planet) – Geology – Earth analogs

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  1. Journal articles
  2. Dissertations / Theses
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Academic literature on the topic 'Mars (Planet) – Geology – Earth analogs'

Author: Grafiati
Published: 4 June 2021
Last updated: 3 February 2022

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Journal articles on the topic "Mars (Planet) – Geology – Earth analogs"

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Shaller, Philip J., Macan Doroudian, and Michael W. Hart. "The Eureka Valley Landslide: Evidence of a Dual Failure Mechanism for a Long-Runout Landslide." Lithosphere 2020, no. 1 (2020): 1–26. http://dx.doi.org/10.2113/2020/8860819.

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Abstract Long-runout landslides are well-known and notorious geologic hazards in many mountainous parts of the world. Commonly encompassing enormous volumes of debris, these rapid mass movements place populations at risk through both direct impacts and indirect hazards, such as downstream flooding. Despite their evident risks, the mechanics of these large-scale landslides remain both enigmatic and controversial. In this work, we illuminate the inner workings of one exceptionally well-exposed and well-preserved long-runout landslide of late Pleistocene age located in Eureka Valley, east-central
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Chan, Marjorie A., Brenda Beitler Bowen, W. T. Parry, Jens Ormö, and Goro Komatsu. "Red rock and red planet diagenesis: Comparisons of Earth and Mars concretions." GSA Today 15, no. 8 (2005): 4. http://dx.doi.org/10.1130/1052-5173(2005)015[4:rrarpd]2.0.co;2.

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Chan, Marjorie A., Brenda Beitler Bowen, W. T. Parry, Jens Ormö, and Goro Komatsu. "Red rock and red planet diagenesis: Comparisons of Earth and Mars concretions." GSA Today 15, no. 8 (2005): 4. http://dx.doi.org/10.1130/1052-5173(2005)15[4:rrarpd]2.0.co;2.

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Rubin, David M., A. G. Fairén, J. Martínez-Frías, et al. "Fluidized-sediment pipes in Gale crater, Mars, and possible Earth analogs." Geology 45, no. 1 (2016): 7–10. http://dx.doi.org/10.1130/g38339.1.

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Sakon, John J., and Robert L. Burnap. "An analysis of potential photosynthetic life on Mars." International Journal of Astrobiology 5, no. 2 (2006): 171–80. http://dx.doi.org/10.1017/s1473550406003144.

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This project researched the possibility of photosynthetic life on Mars. Cyanobacteria were used as potential analogs and were subjected to various Martian-simulated conditions. Synechocystis sp. PCC 6803 was exposed to low pressure, ultraviolet radiation and Martian-simulated atmospheric composition, and proved resistant to the combination of these stresses. However, this organism could neither grow within Martian Regolith Simulant, owing to the lack of soluble nitrogen, nor could it grow in cold temperatures. As a result, later research focused on psychrotolerant cyanobacteria capable of util
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Klimczak, Christian, Paul K. Byrne, A. M. Celâl Şengör, and Sean C. Solomon. "Principles of structural geology on rocky planets." Canadian Journal of Earth Sciences 56, no. 12 (2019): 1437–57. http://dx.doi.org/10.1139/cjes-2019-0065.

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Although Earth is the only known planet on which plate tectonics operates, many small- and large-scale tectonic landforms indicate that deformational processes also occur on the other rocky planets. Although the mechanisms of deformation differ on Mercury, Venus, and Mars, the surface manifestations of their tectonics are frequently very similar to those found on Earth. Furthermore, tectonic processes invoked to explain deformation on Earth before the recognition of horizontal mobility of tectonic plates remain relevant for the other rocky planets. These connections highlight the importance of
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Osinski, Gordon. "The geology of Mars: Evidence from Earth-based analogs, edited by M. G. Chapman." Meteoritics & Planetary Science 42, no. 10 (2007): 1855–56. http://dx.doi.org/10.1111/j.1945-5100.2007.tb00543.x.

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Kedar, S., H. K. M. Tanaka, C. J. Naudet, C. E. Jones, J. P. Plaut, and F. H. Webb. "Muon radiography for exploration of Mars geology." Geoscientific Instrumentation, Methods and Data Systems Discussions 2, no. 2 (2012): 829–53. http://dx.doi.org/10.5194/gid-2-829-2012.

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Abstract. Muon radiography is a technique that uses naturally occurring showers of muons (penetrating particles generated by cosmic rays) to image the interior of large scale geological structures in much the same way as standard X-ray radiography is used to image the interior of smaller objects. Recent developments and application of the technique to terrestrial volcanoes have demonstrated that a low-power, passive muon detector can peer deep into geological structures up to several kilometers in size, and provide crisp density profile images of their interior at ten meter scale resolution. P
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Kedar, S., H. K. M. Tanaka, C. J. Naudet, C. E. Jones, J. P. Plaut, and F. H. Webb. "Muon radiography for exploration of Mars geology." Geoscientific Instrumentation, Methods and Data Systems 2, no. 1 (2013): 157–64. http://dx.doi.org/10.5194/gi-2-157-2013.

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Abstract. Muon radiography is a technique that uses naturally occurring showers of muons (penetrating particles generated by cosmic rays) to image the interior of large-scale geological structures in much the same way as standard X-ray radiography is used to image the interior of smaller objects. Recent developments and application of the technique to terrestrial volcanoes have demonstrated that a low-power, passive muon detector can peer deep into geological structures up to several kilometers in size, and provide crisp density profile images of their interior at ten meter scale resolution. P
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Di Bella, Marcella, Franco Pirajno, Giuseppe Sabatino, et al. "Rolling Ironstones from Earth and Mars: Terrestrial Hydrothermal Ooids as a Potential Analogue of Martian Spherules." Minerals 11, no. 5 (2021): 460. http://dx.doi.org/10.3390/min11050460.

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High-resolution images of Mars from National Aeronautics and Space Administration (NASA) rovers revealed mm-size loose haematite spherulitic deposits (nicknamed “blueberries”) similar to terrestrial iron-ooids, for which both abiotic and biotic genetic hypotheses have been proposed. Understanding the formation mechanism of these haematite spherules can thus improve our knowledge on the possible geologic evolution and links to life development on Mars. Here, we show that shape, size, fabric and mineralogical composition of the Martian spherules share similarities with corresponding iron spherul
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Dissertations / Theses on the topic "Mars (Planet) – Geology – Earth analogs"

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Smith, Amy Renee. "Subsurface Igneous Mineral Microbiology: Iron-Oxidizing Organotrophs on Olivine Surfaces and the Significance of Mineral Heterogeneity in Basalts." PDXScholar, 2011. https://pdxscholar.library.pdx.edu/open_access_etds/294.

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The subsurface igneous biome contains a vast portion of Earth's total biomass, yet we still know so little about it. Igneous environments such as iron-rich ocean crust and lava tubes may also host analogs to chemolithotrophically-driven life on other planets, so studying life in this biome is essential to understanding how life may survive on other planets. In this study, three igneous surface and subsurface environments were investigated for microbial preference for olivine, microbial physiologies and phylotypes present on olivine, and microbial growth on olivine in the laboratory via iron ox
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Murdock, Kathryn J. "Possible Terrestrial Basaltic Analogs for Highly Magnetized Martian Crustal Rocks." 2009. https://scholarworks.umass.edu/theses/342.

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Mars was assumed to be very similar to Earth in terms of topography, water, magnetic field, and even the existence of life. However, exploration of the planet in the 1960s by the Mariner missions showed us a very different planet, one very unlike our own. The later discovery by the Mars Global Surveyor (MGS) of the lack of a globally generated magnetic field proved just how different Mars is from Earth. The discovery of strong magnetic remanence (on the order of 20 – 30 A/m) on Mars implies that at some point in Mars’ history there was a magnetic field, and therefore a dynamo. Since a globally
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Books on the topic "Mars (Planet) – Geology – Earth analogs"

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SEPM (Society for Sedimentary Geology), ed. Sedimentary geology of Mars. SEPM (Society for Sedimentary Geology), 2012.

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2

Brandenburg, John. Death on Mars: The discovery of a planetary nuclear massacre. Adventures Unlimited Press, 2015.

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3

Rossbacher, Lisa A. Periglacial and glacial analogs for Martian landforms: Final technical report. National Aeronautics and Space Administration, 1992.

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Reykjavík, Iceland) International Symposium on Earth and Planetary Ice-Volcano Interactions (2006. Earth and planetary ice-volcano interactions: Papers from the International Symposium on Earth and Planetary Ice-Volcano Interactions : held in Reykjavík, Iceland, on 19-23 June, 2006. International Glaciological Society, 2007.

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5

The Mars mystery: The secret connection between earth and red planet. Crowns, 1998.

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6

G, Chapman Mary, ed. The geology of Mars: Evidence from Earth-based analogs. Cambridge University Press, 2007.

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7

A, Clarke Jonathan D., and American Astronautical Society, eds. Mars analog research. Published for the American Astronautical Society by Univelt, 2006.

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Mars Analog Research. Amer Astronautical Society, 2006.

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9

The Geology of Mars. Cambridge University Press, 2007.

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Chapman, Mary. The Geology of Mars: Evidence from Earth-Based Analogs (Cambridge Planetary Science). Cambridge University Press, 2007.

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Book chapters on the topic "Mars (Planet) – Geology – Earth analogs"

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Mohammadiha, Homayoon. "A View to Anorthosites." In Volcanology [Working Title]. IntechOpen, 2021. http://dx.doi.org/10.5772/intechopen.97787.

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It seems anorthosites are by far interested by geologists because they give us great information about Earth history and how it was evolved in planetary geology. Planetary geology is subject the geology of the celestial bodies such as the planets and their moons, asteroids, comets, and meteorites. It is nearly abundant in the moon. So, it seems studying of these rocks give us good information about planetary evolution and the own early time conditions. Anorthosites can be divided into few types on earth such as: Archean-age (between 4,000 to 2,500 million years ago) anorthosites, Proterozoic (2.5 billion years ago) anorthosite (also known as massif or massif-type anorthosite) – the most abundant type of anorthosite on Earth, Anorthosite xenoliths in other rocks (often granites, kimberlites, or basalts). Furthermore, Lunar anorthosites constitute the light-colored areas of the Moon’s surface and have been the subject of much research. According to the Giant-impact hypothesis the moon and earth were both originated from ejecta of a collision between the proto-Earth and a Mars-sized planetesimal, approximately 4.5 billion years ago. The geology of the Moon (lunar science) is different from Earth. The Moon has a lower gravity and it got cooled faster due to its small size. Also, it has no plate tectonics and due to lack of a true atmosphere it has no erosion and weathering alike the earth. However, Eric A.K. Middlemost believed the astrogeology will help petrologist to make better petrogenic models to understand the magma changing process despite some terms geological differences among the Earth and other extraterrestrial bodies like the Moon. So, it seems that these future studies will clarify new facts about planet formation in planetary and earth, too.
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Journal articles
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