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Relevant bibliographies by topics / Mars craters

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Academic literature on the topic 'Mars craters'

Author: Grafiati

Published: 4 June 2021

Last updated: 1 February 2022

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Journal articles on the topic "Mars craters"

1

Francis, Alistair, Jonathan Brown, Thomas Cameron, et al. "A Multi-Annotator Survey of Sub-km Craters on Mars." Data 5, no. 3 (2020): 70. http://dx.doi.org/10.3390/data5030070.

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We present here a dataset of nearly 5000 small craters across roughly 1700 km2 of the Martian surface, in the MC-11 East quadrangle. The dataset covers twelve 2000-by-2000 pixel Context Camera images, each of which is comprehensively labelled by six annotators, whose results are combined using agglomerative clustering. Crater size-frequency distributions are centrally important to the estimation of planetary surface ages, in lieu of in-situ sampling. Older surfaces are exposed to meteoritic impactors for longer and, thus, are more densely cratered. However, whilst populations of larger craters

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Zimbelman, James R., and Stephen P. Scheidt. "Hesperian Age for Western Medusae Fossae Formation, Mars." Science 336, no. 6089 (2012): 1683. http://dx.doi.org/10.1126/science.1221094.

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The Medusae Fossae Formation (MFF) on Mars is an intensely eroded deposit north of the cratered highlands. It is widely thought that MFF materials were emplaced through ignimbrite eruptions. Recent geologic mapping of western MFF identified outliers of MFF materials well beyond the previously mapped western extent for the deposit, including outliers close to Gale crater. We report counts of impact craters on the MFF units that have implications for our understanding of the general history of MFF and the uppermost layered materials on the Gale crater mound.

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Hardy, Stuart. "Discrete Element Modelling of Pit Crater Formation on Mars." Geosciences 11, no. 7 (2021): 268. http://dx.doi.org/10.3390/geosciences11070268.

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Pit craters are now recognised as being an important part of the surface morphology and structure of many planetary bodies, and are particularly remarkable on Mars. They are thought to arise from the drainage or collapse of a relatively weak surficial material into an open (or widening) void in a much stronger material below. These craters have a very distinctive expression, often presenting funnel-, cone-, or bowl-shaped geometries. Analogue models of pit crater formation produce pits that typically have steep, nearly conical cross sections, but only show the surface expression of their initi

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Jia, Yutong, Gang Wan, Lei Liu, et al. "Split-Attention Networks with Self-Calibrated Convolution for Moon Impact Crater Detection from Multi-Source Data." Remote Sensing 13, no. 16 (2021): 3193. http://dx.doi.org/10.3390/rs13163193.

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Impact craters are the most prominent features on the surface of the Moon, Mars, and Mercury. They play an essential role in constructing lunar bases, the dating of Mars and Mercury, and the surface exploration of other celestial bodies. The traditional crater detection algorithms (CDA) are mainly based on manual interpretation which is combined with classical image processing techniques. The traditional CDAs are, however, inefficient for detecting smaller or overlapped impact craters. In this paper, we propose a Split-Attention Networks with Self-Calibrated Convolution (SCNeSt) architecture,

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Hsu, Chia-Yu, Wenwen Li, and Sizhe Wang. "Knowledge-Driven GeoAI: Integrating Spatial Knowledge into Multi-Scale Deep Learning for Mars Crater Detection." Remote Sensing 13, no. 11 (2021): 2116. http://dx.doi.org/10.3390/rs13112116.

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This paper introduces a new GeoAI solution to support automated mapping of global craters on the Mars surface. Traditional crater detection algorithms suffer from the limitation of working only in a semiautomated or multi-stage manner, and most were developed to handle a specific dataset in a small subarea of Mars’ surface, hindering their transferability for global crater detection. As an alternative, we propose a GeoAI solution based on deep learning to tackle this problem effectively. Three innovative features are integrated into our object detection pipeline: (1) a feature pyramid network

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Chen, Zihao, and Jie Jiang. "Crater Detection and Recognition Method for Pose Estimation." Remote Sensing 13, no. 17 (2021): 3467. http://dx.doi.org/10.3390/rs13173467.

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A crater detection and recognition algorithm is the key to pose estimation based on craters. Due to the changing viewing angle and varying height, the crater is imaged as an ellipse and the scale changes in the landing camera. In this paper, a robust and efficient crater detection and recognition algorithm for fusing the information of sequence images for pose estimation is designed, which can be used in both flying in orbit around and landing phases. Our method consists of two stages: stage 1 for crater detection and stage 2 for crater recognition. In stage 1, a single-stage network with dens

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Barata, T., E. I. Alves, A. Machado, and G. A. Barberes. "Characterization of palimpsest craters on Mars." Planetary and Space Science 72, no. 1 (2012): 62–69. http://dx.doi.org/10.1016/j.pss.2012.09.015.

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Edgett, Kenneth S., Steven G. Banham, Kristen A. Bennett, et al. "Extraformational sediment recycling on Mars." Geosphere 16, no. 6 (2020): 1508–37. http://dx.doi.org/10.1130/ges02244.1.

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Abstract Extraformational sediment recycling (old sedimentary rock to new sedimentary rock) is a fundamental aspect of Earth’s geological record; tectonism exposes sedimentary rock, whereupon it is weathered and eroded to form new sediment that later becomes lithified. On Mars, tectonism has been minor, but two decades of orbiter instrument–based studies show that some sedimentary rocks previously buried to depths of kilometers have been exposed, by erosion, at the surface. Four locations in Gale crater, explored using the National Aeronautics and Space Administration’s Curiosity rover, exhibi

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Carporzen, Laurent, Stuart A. Gilder, and Rodger J. Hart. "Palaeomagnetism of the Vredefort meteorite crater and implications for craters on Mars." Nature 435, no. 7039 (2005): 198–201. http://dx.doi.org/10.1038/nature03560.

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MCEWEN, A., B. PREBLICH, E. TURTLE, et al. "The rayed crater Zunil and interpretations of small impact craters on Mars." Icarus 176, no. 2 (2005): 351–81. http://dx.doi.org/10.1016/j.icarus.2005.02.009.

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Dissertations / Theses on the topic "Mars craters"

1

De, Villiers Germari Marzen Luke J. King David T. "Remote sensing of shallow-marine impact craters on Mars." Auburn, Ala., 2007. http://hdl.handle.net/10415/1343.

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Kukkonen, S. (Soile). "Small impact craters in crater counting:evolution studies of the eastern Hellas outflow channels, Mars." Doctoral thesis, Oulun yliopisto, 2018. http://urn.fi/urn:isbn:9789526218779.

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Abstract Crater counting is a method which allows us to estimate the surface ages of the planetary bodies, from which the sampling and sample delivery to laboratories on Earth are difficult or impossible. Because the number of craters on a surface unit increases over the time the surface has been exposed to space, old, geologically stable units have more craters than young and active units. When the crater production rate as a function of time is known, the absolute age of the surface unit can be determined based on its crater density. The purpose of this thesis is to investigate the role of s

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Chee, Yenlai. "Remote sensing analysis of cratered surfaces Mars landing hazard assessment, comparison to terrestrial crater analogs, and Mars crater dating models /." To access this resource online via ProQuest Dissertations and Theses @ UTEP, 2007. http://0-proquest.umi.com.lib.utep.edu/login?COPT=REJTPTU0YmImSU5UPTAmVkVSPTI=&clientId=2515.

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BARLOW, NADINE GAIL. "RELATIVE AGES AND THE GEOLOGIC EVOLUTION OF MARTIAN TERRAIN UNITS (MARS, CRATERS)." Diss., The University of Arizona, 1987. http://hdl.handle.net/10150/184013.

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Existing martian relative age chronologies rely entirely or predominantly on Mariner 9 images, extrapolated numbers of craters, and craters 500(DEGREES)K) for the planet are consistent with the derived chronology.

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Daubar, Ingrid Justine. "New Dated Craters On Mars And The Moon: Studies Of The Freshest Craters In The Solar System." Diss., The University of Arizona, 2014. http://hdl.handle.net/10150/337303.

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New, dated impacts discovered on Mars and the Moon provide direct observations of modern bombardment in the inner Solar System and the freshest available examples of recent craters. Their population, morphology, formation and modification processes relate to issues with secondaries and help calibrate cratering chronology models. I use a subset of the new impacts to measure the current production function at Mars. The resulting production function is a factor of approximately four lower than widely-used models, and the size frequency distribution has a shallower slope. This discrepancy between

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Bamberg, Marlene. "Planetary mapping tools applied to floor-fractured craters on Mars." Phd thesis, Universität Potsdam, 2014. http://opus.kobv.de/ubp/volltexte/2014/7210/.

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Planetary research is often user-based and requires considerable skill, time, and effort. Unfortunately, self-defined boundary conditions, definitions, and rules are often not documented or not easy to comprehend due to the complexity of research. This makes a comparison to other studies, or an extension of the already existing research, complicated. Comparisons are often distorted, because results rely on different, not well defined, or even unknown boundary conditions. The purpose of this research is to develop a standardized analysis method for planetary surfaces, which is adaptable to sev

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Perälä, Jesper. "Pit Craters of Arsia Mons Volcano, Mars, and Their Relation to Regional Volcano-tectonism." Thesis, Uppsala universitet, Institutionen för geovetenskaper, 2015. http://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-255563.

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Pit crater and pit crater chains associated to the volcano Arsia Mons on Mars have been mapped to analyse their spatial pattern and to conclude about their formation. For the mapping, high resolution satellite data gathered during the Mars Express mission were used. The spatial distribution of the pit craters was then compared with typical patterns of magmatic sheet intrusions within volcanoes as they are known from Earth. The results show that the pattern of the mapped pit craters and pit crater chains are in good agreement with these sheet intrusions and are therefore likely related to Marti

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Viola, Donna, and Donna Viola. "Expanded Craters on Mars: Implications for Shallow, Mid-Latitude Excess Ice." Diss., The University of Arizona, 2017. http://hdl.handle.net/10150/625594.

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Understanding the age and distribution of shallow ice on Mars is valuable for interpreting past and present climate conditions, and has implications on habitability and future in situ resource utilization. Many ice-related features, such as lobate debris aprons and concentric crater fill, have been studied using a range of remote sensing techniques. Here, I explore the distribution of expanded craters, a form of sublimation thermokarst where shallow, excess ice has been destabilized and sublimated following an impact event. This leads to the collapse of the overlying dry regolith to produce th

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Breton, Sylvain. "Dynamique des surfaces planétaires actives : quantification des paysages, modélisation et inversion." Thesis, Lyon, 2019. http://www.theses.fr/2019LYSE1280.

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Les cratères d'impact sont indispensables dans l'étude des surfaces planétaires. D'une part, les statistiques de leur nombre permet de dater les surfaces planétaires, d'autre part, leur forme révèle les processus de surface qu'ils ont connu. Cette thèse propose de coupler les études statistiques et morphologiques afin d'étudier la temporalité et l'importance des processus sédimentaires et/ou volcaniques des surfaces planétaires. L'utilisation de la profondeur des cratères permet de rajouter une dimension aux distributions avec l'introduction des distributions en fréquence de taille et de profo

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Viola, D., and A. S. McEwen. "Geomorphological Evidence for Shallow Ice in the Southern Hemisphere of Mars." AMER GEOPHYSICAL UNION, 2018. http://hdl.handle.net/10150/627126.

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The localized loss of near-surface excess ice on Mars by sublimation (and perhaps melting) can produce thermokarstic collapse features such as expanded craters and scalloped depressions, which can be indicators of the preservation of shallow ice. We demonstrate this by identifying High Resolution Imaging Science Experiment images containing expanded craters south of Arcadia Planitia (25-40 degrees N) and observe a spatial correlation between regions with thermokarst and the lowest-latitude ice-exposing impact craters identified to date. In addition to widespread thermokarst north of 35 degrees

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Books on the topic "Mars craters"

1

Grant, John A. Advances in planetary geology. NASA, 1987.

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2

Bridges, John C. Evolution of the Martian Crust. Oxford University Press, 2017. http://dx.doi.org/10.1093/acrefore/9780190647926.013.18.

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This is an advance summary of a forthcoming article in the Oxford Encyclopedia of Planetary Science. Please check back later for the full article.Mars, which has a tenth of the mass of Earth, has cooled as a single lithospheric plate. Current topography gravity maps and magnetic maps do not show signs of the plate tectonics processes that have shaped the Earth’s surface. Instead, Mars has been shaped by the effects of meteorite bombardment, igneous activity, and sedimentary—including aqueous—processes. Mars also contains enormous igneous centers—Tharsis and Elysium, with other shield volcanoes

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Reimold, Wolf Uwe, and Christian Koeberl, eds. Large Meteorite Impacts and Planetary Evolution VI. Geological Society of America, 2021. http://dx.doi.org/10.1130/spe550.

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This volume represents the proceedings of the homonymous international conference on all aspects of impact cratering and planetary science, which was held in October 2019 in Brasília, Brazil. This volume contains a sizable suite of contributions dealing with regional impact records (Australia, Sweden), impact craters and impactites, early Archean impacts and geophysical characteristics of impact structures, shock metamorphic investigations, post-impact hydrothermalism, and structural geology and morphometry of impact structures—on Earth and Mars. These contributions are authored by many of the

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E, Wieprecht David, and Sako Maurice K, eds. Elevations and descriptions for leveling bench marks at Newberry Crater, Oregon. U.S. Dept. of the Interior, U.S. Geological Survey, 1995.

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5

Byrne, Charles J. The Moon's Largest Craters and Basins: Images and Topographic Maps from LRO, GRAIL, and Kaguya. Springer, 2016.

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Byrne, Charles J. The Moon's Largest Craters and Basins: Images and Topographic Maps from LRO, GRAIL, and Kaguya. Springer, 2015.

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7

Survey, United States Geological. Geologic map of the MTM -15182 and MTM -15187 quadrangles, Gusev Crater-Ma'adim Vallis Region, Mars. For sale by USGS Information Services, 2000.

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8

Washington, Oregon: Includes Maps of Portland, Seattle, Crater Lake NP, Mount Rainier NP. Not Avail, 2004.

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9

Cogenetic rock fragments from a lunar soil: Evidence of a ferroan noritic-anorthosite pluton on the moon. National Aeronautics and Space Administration, 1995.

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10

Verne, Jules. Journey to the Centre of the Earth. Translated by William Butcher. Oxford University Press, 2008. http://dx.doi.org/10.1093/owc/9780199538072.001.0001.

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Journey to the Centre of the Earth has been consistently praised for its style and its vision of the world. It explores the prehistory of the globe, but can also be read as a psychological quest, for the journey itself is as important as arrival or discovery. Professor Lidenbrock and his nephew Axel travel across Iceland, and then down through an extinct crater towards a sunless sea where they enter a living past and are confronted with the origins of man. A classic of nineteenth-century French literature, the novel's distinctive combination of realism and Romanticism has marked figures as div

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Book chapters on the topic "Mars craters"

1

Vetro, Rosanne, and Dan A. Simovici. "Entropic Quadtrees and Mining Mars Craters." In Advances in Data Mining. Applications and Theoretical Aspects. Springer Berlin Heidelberg, 2010. http://dx.doi.org/10.1007/978-3-642-14400-4_17.

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Chapman, Clark R., and David Morrison. "Craters on the Moon and Mars." In Cosmic Catastrophes. Springer US, 1989. http://dx.doi.org/10.1007/978-1-4899-6553-0_4.

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Barata, Teresa, E. Ivo Alves, José Saraiva, and Pedro Pina. "Automatic Recognition of Impact Craters on the Surface of Mars." In Lecture Notes in Computer Science. Springer Berlin Heidelberg, 2004. http://dx.doi.org/10.1007/978-3-540-30126-4_60.

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Marques, Jorge S., and Pedro Pina. "An Algorithm for the Delineation of Craters in Very High Resolution Images of Mars Surface." In Pattern Recognition and Image Analysis. Springer Berlin Heidelberg, 2013. http://dx.doi.org/10.1007/978-3-642-38628-2_25.

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Hargitai, Henrik. "Pedestal Crater (Mars)." In Encyclopedia of Planetary Landforms. Springer New York, 2014. http://dx.doi.org/10.1007/978-1-4614-9213-9_257-1.

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Hargitai, Henrik. "Pedestal Crater (Mars)." In Encyclopedia of Planetary Landforms. Springer New York, 2015. http://dx.doi.org/10.1007/978-1-4614-3134-3_257.

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Airo, Alessandro. "Crater Lakes (Mars)." In Encyclopedia of Astrobiology. Springer Berlin Heidelberg, 2014. http://dx.doi.org/10.1007/978-3-642-27833-4_3244-2.

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Airo, Alessandro. "Crater Lakes (Mars)." In Encyclopedia of Astrobiology. Springer Berlin Heidelberg, 2015. http://dx.doi.org/10.1007/978-3-662-44185-5_3244.

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Cattermole, Peter. "The Ancient Cratered Terrain." In Mars. Springer Netherlands, 1992. http://dx.doi.org/10.1007/978-94-011-2306-8_6.

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El-Maarry, Mohamed Ramy, Richard Soare, and Ákos Kereszturi. "Crater-Floor Polygons (Mars)." In Encyclopedia of Planetary Landforms. Springer New York, 2014. http://dx.doi.org/10.1007/978-1-4614-9213-9_72-2.

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Conference papers on the topic "Mars craters"

1

Schultz, Peter H. "MISSING MARS: CLUES FROM RELICT CRATERS." In GSA Annual Meeting in Seattle, Washington, USA - 2017. Geological Society of America, 2017. http://dx.doi.org/10.1130/abs/2017am-306336.

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Wilson, Sharon A., and Alan D. Howard. "THE NATURE AND DISTRIBUTION OF POLLYWOG CRATERS ON MARS." In GSA Annual Meeting in Phoenix, Arizona, USA - 2019. Geological Society of America, 2019. http://dx.doi.org/10.1130/abs/2019am-339375.

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Kling, Corbin L., Paul K. Byrne, Danielle Y. Wyrick, Karl W. Wegmann, and Helena Mitasova. "THE FORMATION OF PIT CRATERS WITHIN NOCTIS LABYRINTHUS, MARS." In GSA Annual Meeting in Seattle, Washington, USA - 2017. Geological Society of America, 2017. http://dx.doi.org/10.1130/abs/2017am-307391.

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Golombek, M. P., N. H. Warner, Vamsi Ganti, and Julianne Sweeney. "DEGRADATION OF SMALL IMPACT CRATERS: EROSION RATES AND MARS CLIMATE." In GSA Annual Meeting in Seattle, Washington, USA - 2017. Geological Society of America, 2017. http://dx.doi.org/10.1130/abs/2017am-301049.

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Aoki, Risako, Akira Oyama, Koji Fujita, et al. "Conceptual Helicopter Design for Exploration of Pit craters and Caves on Mars." In 2018 AIAA SPACE and Astronautics Forum and Exposition. American Institute of Aeronautics and Astronautics, 2018. http://dx.doi.org/10.2514/6.2018-5362.

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Wilson, Sharon A., Alexander M. Morgan, and Alan D. Howard. "THE GLOBAL DISTRIBUTION OF CRATERS WITH ALLUVIAL FANS AND DELTAS ON MARS." In GSA 2020 Connects Online. Geological Society of America, 2020. http://dx.doi.org/10.1130/abs/2020am-359423.

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Newsom, Horton E. "Where Should We Look for Life on Mars: The Case for Impact Craters?" In SPACE TECHNOLOGY AND APPLICATIONS INTERNAT.FORUM-STAIF 2004: Conf.on Thermophys.in Microgravity; Commercial/Civil Next Gen.Space Transp.; 21st Symp.Space Nuclear Power & Propulsion; Human Space Explor.; Space Colonization; New Frontiers & Future Concepts. AIP, 2004. http://dx.doi.org/10.1063/1.1649658.

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Irwin, Rossman, and Edward Wolfe. "SPATIALLY AND TEMPORALLY VARIABLE EROSION OF THE LARGEST POST-NOACHIAN IMPACT CRATERS ON MARS." In GSA 2020 Connects Online. Geological Society of America, 2020. http://dx.doi.org/10.1130/abs/2020am-358202.

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Peel, Samantha E., and Devon M. Burr. "MAPPING LACUSTRINE, FLUVIAL, AND AEOLIAN DEPOSITS WITHIN CRATERS IN THE AEOLIS DORSA REGION OF MARS." In 67th Annual Southeastern GSA Section Meeting - 2018. Geological Society of America, 2018. http://dx.doi.org/10.1130/abs/2018se-312598.

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Harrison, Tanya N. "EVIDENCE FOR VOLCANISM IN MARTIAN FLOOR-FRACTURED CRATERS FROM THE MARS RECONNAISSANCE ORBITER CONTEXT CAMERA." In GSA Annual Meeting in Seattle, Washington, USA - 2017. Geological Society of America, 2017. http://dx.doi.org/10.1130/abs/2017am-308639.

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Reports on the topic "Mars craters"

1

Joseph, Rhawn. Mars: Algae, Lichens, Fossils, Minerals, Microbial Mats, and Stromatolites in Gale Crater. Journal of Astrobiology and Space Science, 2020. http://dx.doi.org/10.37720/jassr.03082020.

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Berger, B., D. Blaney, J. Bridges, et al. POSSIBLE ALTERATION OF ROCKS OBSERVED BY CHEMCAM ALONG THE TRAVERSE TO GLENELG IN GALE CRATER ON MARS. Office of Scientific and Technical Information (OSTI), 2013. http://dx.doi.org/10.2172/1077020.

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Geologic map of the MTM-15182 and MTM-15187 quadrangles, Gusev Crater-Ma'adim Vallis region, Mars. US Geological Survey, 2000. http://dx.doi.org/10.3133/i2666.

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Maps showing posteruption erosion, deposition, and dome growth in Mount St. Helens Crater, Washington, determined by a geographic information system. US Geological Survey, 1992. http://dx.doi.org/10.3133/i2297.

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