An Economic Analysis of Mars Exploration and Colonization Clayton Knappenberger Depauw University
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Wind Measurements of Martian Dust Devils from Hirise
EPSC Abstracts Vol. 6, EPSC-DPS2011-570, 2011 EPSC-DPS Joint Meeting 2011 c Author(s) 2011 Wind Measurements of Martian Dust Devils from HiRISE D. S. Choi (1) and C. M. Dundas (2) (1) Department of Planetary Sciences, University of Arizona, Tucson, AZ, USA ([email protected]) (2) United States Geological Survey, Flagstaff, AZ, USA Abstract servation crosses an active feature such as a dust devil, changes in the active feature are apparent from the We report direct measurements of the winds within three separate views. Treating the dust clouds as pas- Martian dust devils from HiRISE imagery. The cen- sive tracers of motion then allows for the direct mea- tral color swath of the HiRISE instrument observes surement of wind velocities. the surface by using separate CCDs and color filters in We utilize measurements from manual (hand-eye) rapid cadence. Active features, such as a dust devil, tracking of the clouds through image blinking, as appear in motion when serendipitously captured by well as automated correlation methods [9]. Typically, this region of the instrument. Our measurements re- manual measurements are more successful than au- veal clear circulation within the vortices, and that the tomated measurements. The relatively diffuse dust majority of overall wind magnitude within a dust devil clouds, combined with the static background terrain, 1 is between 10 and 30 m s− . cause the automated software to incorrectly report the movement as stationary. Successful automated results were obtained from images with more substantial dust 1. Introduction clouds and relatively featureless background terrain. Direct measurements of the winds within a Martian dust devil [1] are challenging to obtain. -
Stairway to Heaven? Geographies of the Space Elevator in Science Fiction
ISSN 2624-9081 • DOI 10.26034/roadsides-202000306 Stairway to Heaven? Geographies of the Space Elevator in Science Fiction Oliver Dunnett Outer space is often presented as a kind of universal global commons – a space for all humankind, against which the hopes and dreams of humanity have been projected. Yet, since the advent of spaceflight, it has become apparent that access to outer space has been limited, shaped and procured in certain ways. Geographical approaches to the study of outer space have started to interrogate the ways in which such inequalities have emerged and sustained themselves, across environmental, cultural and political registers. For example, recent studies have understood outer space as increasingly foreclosed by certain state and commercial actors (Beery 2012), have emphasised narratives of tropical difference in understanding geosynchronous equatorial satellite orbits (Dunnett 2019) and, more broadly, have conceptualised the Solar System as part of Earth’s environment (Degroot 2017). It is clear from this and related literature that various types of infrastructure have been a significant part of the uneven geographies of outer space, whether in terms of long-established spaceports (Redfield 2000), anticipatory infrastructures (Gorman 2009) or redundant space hardware orbiting Earth as debris (Klinger 2019). collection no. 003 • Infrastructure on/off Earth Roadsides Stairway to Heaven? 43 Having been the subject of speculation in both engineering and science-fictional discourses for many decades, the space elevator has more recently been promoted as a “revolutionary and efficient way to space for all humanity” (ISEC 2017). The concept involves a tether lowered from a position in geostationary orbit to a point on Earth’s equator, along which an elevator can ascend and arrive in orbit. -
A Theory of Mars Introduction Over the Last 10 Years Or So I Have Been
A Theory of Mars Introduction Over the last 10 years or so I have been researching the idea there might be alien artifacts on Mars. Over this time there have been many interesting discoveries by myself and others, and some candidate artifacts have been found to be likely natural. So far proof remains elusive but some evidence has grown stronger. As more and more of these candidate artifacts have been found, similarities have begun to emerge, pointing at a more plausible theory for their origin. So in this paper I am explaining this theory, with the caveat that nothing is proven at this stage. If more candidate artifacts are found and they also support this theory then this will be additional evidence for artificiality. The reason is formations of randomly appearing similar to artifacts should also randomly seem to fit in with many different contradictory theories. To explain this theory I will need to start at the beginning of this story, which is likely to be at least several hundred million years and possibly over a billion years ago. So these artifacts, if they exist at all, are likely to be incredibly old and only have survived because erosion on Mars is very small. The main reason for this is the near vacuum on Mars prevents most erosion because most of the atmosphere is frozen at the poles. This subject then is far removed from such things as UFOs or Von Daniken like theories of extra terrestrials visiting us today. By contrast any evidence of visitation from so long ago is likely to be archeological with little more than ruins to be found. -
Cubesats to the Moon | the Planetary Society
8/1/2019 CubeSats to the Moon | The Planetary Society Casey Dreier • September 2, 2015 CubeSats to the Moon An interview with the scientist behind NASA’s newest planetary exploration mission On Tuesday, NASA announced its selection of two CubeSats to ¼y beyond Earth as part of its Small, Innovative Missions for Planetary Exploration (SIMPLEx) program. The CubeSats were limited to a total budget of $5.6 million (though they were encouraged to be cheaper), and will ride along on the ¹rst ¼ight of the Space Launch System (SLS) in 2018. They were competitively selected from a number of proposals submitted by the scienti¹c community. The Lunar Polar Hydrogen Mapper (LunaH-Map) was one of the two missions selected. Led by 33-year-old planetary scientist Dr. Craig Hardgrove, a post- doctoral scholar at Arizona State University, it will attempt to map the distribution of water-ice over the south pole of the Moon at high resolutions. www.planetary.org/blogs/casey-dreier/2015/0902-cubesats-to-the-moon.html 1/11 8/1/2019 CubeSats to the Moon | The Planetary Society Sean Amidan / ASU / SpaceTREx LUNAR POLAR HYDROGEN MAPPER (LUNAH-MAP) Artist's concept of the Lunar Polar Hydrogen Mapper (LunaH-Map), an Arizona State University-built CubeSat about the size of a shoebox that will be used to produce a map of the water resources on the Moon for future human exploration. I interviewed Dr. Hardgrove about his lunar CubeSat, how it came together, and how NASA’s support for small missions are important for early career scientists like himself. -
By: Rahmat Hidayat 40300115045 ENGLISH and LITERATURE
The Influence of Writer’s Habitus in Made The Martian Novel. Thesis Submitted in Partial Fulfillment of the Requirements for the Degree of SarjanaHumaniora in English and Literature Department of Adab and Humanities Faculty of Alauddin State Islamic University of Makassar By: Rahmat Hidayat 40300115045 ENGLISH AND LITERATURE DEPARTMENT ADAB AND HUMANITIES FACULTY ALAUDDIN STATE ISLAMIC UNIVERSITY OF MAKASSAR 2019 i PERNYATAAN KEASLIAN SKRIPSI Dengan penuh kesadaran, penulis yang bertandatangan dibawah ini menyatakan bahwa skripsi ini benar-benar adalah hasil karya penulis sendiri, dan jika dikemudian hari terbukti merupakan duplikat, tiruan, plagiat, atau dibuat oleh orang lain secara keseluruhan ataupun sebagian, maka skripsi ini dang elar yang diperoleh batal demi hukum. Romang Polong, 7 November 2019 Penulis, Rahmat Hidayat 4030011504 ii iii iv v ACKNOWLEDGEMENT Alhamdulillah RabbilAlamin, all praises and thanks to the Almighty Allah SWT for His uncountable graces, faiths, and helps always stand behind the writer, show writer the right way, and carry the writer out to the final step of this thesis writing. Shalawat and salam are addressed to our prophet Muhammad SAW, the greatest one who has shared inspiration, spirit, and power to the human. The writer realizes that this thesis could not complete without getting assistance, guidance, understanding and encouragement from many people. Therefore the writer would like to express the deepest gratitude to the following: 1. The writer’s beloved parents, Syamsuddin and Nuraeni for their loves, cares, supports and prayers for the writer’s safety and successful. 2. The writer’s beloved big family for their support and sincere prayer for the writer’s success. -
The Reference Mission of the NASA Mars Exploration Study Team
NASA Special Publication 6107 Human Exploration of Mars: The Reference Mission of the NASA Mars Exploration Study Team Stephen J. Hoffman, Editor David I. Kaplan, Editor Lyndon B. Johnson Space Center Houston, Texas July 1997 NASA Special Publication 6107 Human Exploration of Mars: The Reference Mission of the NASA Mars Exploration Study Team Stephen J. Hoffman, Editor Science Applications International Corporation Houston, Texas David I. Kaplan, Editor Lyndon B. Johnson Space Center Houston, Texas July 1997 This publication is available from the NASA Center for AeroSpace Information, 800 Elkridge Landing Road, Linthicum Heights, MD 21090-2934 (301) 621-0390. Foreword Mars has long beckoned to humankind interest in this fellow traveler of the solar from its travels high in the night sky. The system, adding impetus for exploration. ancients assumed this rust-red wanderer was Over the past several years studies the god of war and christened it with the have been conducted on various approaches name we still use today. to exploring Earth’s sister planet Mars. Much Early explorers armed with newly has been learned, and each study brings us invented telescopes discovered that this closer to realizing the goal of sending humans planet exhibited seasonal changes in color, to conduct science on the Red Planet and was subjected to dust storms that encircled explore its mysteries. The approach described the globe, and may have even had channels in this publication represents a culmination of that crisscrossed its surface. these efforts but should not be considered the final solution. It is our intent that this Recent explorers, using robotic document serve as a reference from which we surrogates to extend their reach, have can continuously compare and contrast other discovered that Mars is even more complex new innovative approaches to achieve our and fascinating—a planet peppered with long-term goal. -
A Future Mars Environment for Science and Exploration
Planetary Science Vision 2050 Workshop 2017 (LPI Contrib. No. 1989) 8250.pdf A FUTURE MARS ENVIRONMENT FOR SCIENCE AND EXPLORATION. J. L. Green1, J. Hol- lingsworth2, D. Brain3, V. Airapetian4, A. Glocer4, A. Pulkkinen4, C. Dong5 and R. Bamford6 (1NASA HQ, 2ARC, 3U of Colorado, 4GSFC, 5Princeton University, 6Rutherford Appleton Laboratory) Introduction: Today, Mars is an arid and cold world of existing simulation tools that reproduce the physics with a very thin atmosphere that has significant frozen of the processes that model today’s Martian climate. A and underground water resources. The thin atmosphere series of simulations can be used to assess how best to both prevents liquid water from residing permanently largely stop the solar wind stripping of the Martian on its surface and makes it difficult to land missions atmosphere and allow the atmosphere to come to a new since it is not thick enough to completely facilitate a equilibrium. soft landing. In its past, under the influence of a signif- Models hosted at the Coordinated Community icant greenhouse effect, Mars may have had a signifi- Modeling Center (CCMC) are used to simulate a mag- cant water ocean covering perhaps 30% of the northern netic shield, and an artificial magnetosphere, for Mars hemisphere. When Mars lost its protective magneto- by generating a magnetic dipole field at the Mars L1 sphere, three or more billion years ago, the solar wind Lagrange point within an average solar wind environ- was allowed to directly ravish its atmosphere.[1] The ment. The magnetic field will be increased until the lack of a magnetic field, its relatively small mass, and resulting magnetotail of the artificial magnetosphere its atmospheric photochemistry, all would have con- encompasses the entire planet as shown in Figure 1. -
The Analysis of Life Struggle in Andy Weir's
THE ANALYSIS OF LIFE STRUGGLE IN ANDY WEIR‘S NOVEL THE MARTIAN A THESIS BY ALEMINA BR KABAN REG. NO. 140721012 DEPARTMENT OF ENGLISH FACULTY OF CULTURAL STUDIES UNIVERSITY OF SUMATERA UTARA MEDAN 2018 UNIVERSITAS SUMATERA UTARA THE ANALYSIS OF LIFE STRUGGLE IN ANDY WEIR‘S NOVEL THE MARTIAN A THESIS BY ALEMINA BR KABAN REG. NO. 140721012 SUPERVISOR CO-SUPERVISOR Drs. Parlindungan Purba,M.Hum. Riko Andika Pohan, S.S., M.Hum. NIP.1963021619 89031003001 NIP. 1984060920150410010016026 Submitted to Faculty of Cultural Studies University of Sumatera Utara Medan in partial fulfilment of the requirements for the degree of Sarjana Sastra from Department of English DEPARTMENT OF ENGLISH FACULTY OF CULTURAL STUDIES UNIVERSITY OF SUMATERA UTARA MEDAN 2018 UNIVERSITAS SUMATERA UTARA Approved by the Department of English, Faculty of Cultural Studies University of Sumatera Utara (USU) Medan as thesis for The Sarjana Sastra Examination. Head, Secretary, Prof. T.Silvana Sinar,Dipl.TEFL,MA.,Ph.D Rahmadsyah Rangkuti, M.A. Ph.D. NIP. 19571117 198303 2 002 NIP. 19750209 200812 1 002 UNIVERSITAS SUMATERA UTARA Accepted by the Board of Examiners in partial fulfillment of requirements for the degree of Sarjana Sastra from the Department of English, Faculty of Cultural Studies University of Sumatera Utara, Medan. The examination is held in Department of English Faculty of Cultural Studies University of Sumatera Utara on July 6th, 2018 Dean of Faculty of Cultural Studies University of Sumatera Utara Dr. Budi Agustono, M.S. NIP.19600805 198703 1 001 Board of Examiners Rahmadsyah Rangkuti, M.A., Ph.D __________________ Drs. Parlindungan Purba, M.Hum. -
Design of a Human Settlement on Mars Using In-Situ Resources
46th International Conference on Environmental Systems ICES-2016-151 10-14 July 2016, Vienna, Austria Design of a Human Settlement on Mars Using In-Situ Resources Marlies Arnhof1 Vienna University of Technology, Vienna, 1040, Austria Mars provides plenty of raw materials needed to establish a lasting, self-sufficient human colony on its surface. Due to the planet's vast distance from Earth, it is neither possible nor economically reasonable to provide permanent, interplanetary supply. In-situ resource utilization (ISRU) will be necessary to keep the Earth launch burden and mission costs as low as possible, and to provide – apart from propellant and life support – a variety of construction material. However, to include outposts on other planets into the scope of human spaceflight also opens up new psychological and sociological challenges. Crews will live in extreme environments under isolated and confined conditions for much longer periods of time than ever before. Therefore, the design of a Mars habitat requires most careful consideration of physiological as well as psychosocial conditions of living in space. In this design for a Martian settlement, the author proposes that – following preliminary automated exploration – a basic surface base brought from Earth would be set up. Bags of unprocessed Martian regolith would be used to provide additional shielding for the habitat. Once the viability of the base and its production facilities are secured, the settlement would be expanded, using planetary resources. Martian concrete – processed regolith with a polymeric binder – would be used as main in-situ construction material. To provide optimum living and working conditions, the base would respond to the environment and the residents' number and needs, thereby evolving and growing continuously. -
Lafayette - 800 Grams Nakhlite
Lafayette - 800 grams Nakhlite Figure 1. Photograph showing fine ablation features Figure 2. Photograph of bottom surface of Lafayette of fusion crust on Lafayette meteorite. Sample is meteorite. Photograph from Field Museum Natural shaped like a truncated cone. This is a view of the top History, Chicago, number 62918. of the cone. Sample is 4-5 centimeters across. Photo- graph from Field Museum Natural History, Chicago, number 62913. Introduction According to Graham et al. (1985), “a mass of about 800 grams was noticed by Farrington in 1931 in the geological collections in Purdue University in Lafayette Indiana.” It was first described by Nininger (1935) and Mason (1962). Lafayette is very similar to the Nakhla and Governador Valadares meteorites, but apparently distinct from them (Berkley et al. 1980). Lafayette is a single stone with a fusion crust showing Figure 3. Side view of Lafayette. Photograph from well-developed flow features from ablation in the Field Museum Natural History, Chicago, number Earth’s atmosphere (figures 1,2,3). The specimen is 62917. shaped like a rounded cone with a blunt bottom end. It was apparently oriented during entry into the Earth’s that the water released during stepwise heating of atmosphere. Note that the fine ablation features seen Lafayette was enriched in deuterium. The alteration on Lafayette have not been reported on any of the assemblages in Lafayette continue to be an active field Nakhla specimens. of research, because it has been shown that the alteration in Lafayette occurred on Mars. Karlsson et al. (1992) found that Lafayette contained the most extra-terrestrial water of any Martian Lafayette is 1.32 b.y. -
The Case for Mars Subsurface Exploration
Ninth International Conference on Mars 2019 (LPI Contrib. No. 2089) 6279.pdf THE CASE FOR MARS SUBSURFACE EXPLORATION. L. W. Beegle1, V. Stamenković1, K. Zacny2.1Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109 USA. 2Honeybee Robotics, New York, NY, USA. The Martian subsurface is of enormous interest for Orbiters, landers and rovers, especially the two astrobiology, geochemistry, climatology, and In Situ MERs and Curiosity, have delivered data that have revo- Resource Utilization (ISRU) objectives, which cannot lutionized our understanding of ancient Martian surface be addressed with surface missions alone. Specifically, environments. Those data support a rich history of subsurface data are needed to continue the search for groundwater flow and a diverse, and from the surface extinct of extant life started by the Viking landers more very different, world hiding beneath the oxidized surficial than forty years ago and to prepare for human explora- regolith. InSight and future missions like the ExoMars tion. If Mars ever had life, whether it emerged on or and Mars 2020 rovers will aim to extend our knowledge of ancient habitable surface environments, to produce below the surface, then as the atmosphere thinned and unprecedented data on global large-scale interior proper- global temperatures dropped[1], life may have fol- ties, and to inform us about the very shallow Martian lowed the groundwater table to progressively greater regolithic subsurface. However, questions, in particular depths where stable liquid water could persist. At such about whether there ever was or is still life on Mars, how depths, life could have been sustained by hydrothermal the Martian climate changed over long periods of time, activity and rock-water reactions. -
Why NASA Consistently Fails at Congress
W&M ScholarWorks Undergraduate Honors Theses Theses, Dissertations, & Master Projects 6-2013 The Wrong Right Stuff: Why NASA Consistently Fails at Congress Andrew Follett College of William and Mary Follow this and additional works at: https://scholarworks.wm.edu/honorstheses Part of the Political Science Commons Recommended Citation Follett, Andrew, "The Wrong Right Stuff: Why NASA Consistently Fails at Congress" (2013). Undergraduate Honors Theses. Paper 584. https://scholarworks.wm.edu/honorstheses/584 This Honors Thesis is brought to you for free and open access by the Theses, Dissertations, & Master Projects at W&M ScholarWorks. It has been accepted for inclusion in Undergraduate Honors Theses by an authorized administrator of W&M ScholarWorks. For more information, please contact [email protected]. The Wrong Right Stuff: Why NASA Consistently Fails at Congress A thesis submitted in partial fulfillment of the requirement for the degree of Bachelors of Arts in Government from The College of William and Mary by Andrew Follett Accepted for . John Gilmour, Director . Sophia Hart . Rowan Lockwood Williamsburg, VA May 3, 2013 1 Table of Contents: Acknowledgements 3 Part 1: Introduction and Background 4 Pre Soviet Collapse: Early American Failures in Space 13 Pre Soviet Collapse: The Successful Mercury, Gemini, and Apollo Programs 17 Pre Soviet Collapse: The Quasi-Successful Shuttle Program 22 Part 2: The Thin Years, Repeated Failure in NASA in the Post-Soviet Era 27 The Failure of the Space Exploration Initiative 28 The Failed Vision for Space Exploration 30 The Success of Unmanned Space Flight 32 Part 3: Why NASA Fails 37 Part 4: Putting this to the Test 87 Part 5: Changing the Method.