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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. -
An Economic Analysis of Mars Exploration and Colonization Clayton Knappenberger Depauw University
DePauw University Scholarly and Creative Work from DePauw University Student research Student Work 2015 An Economic Analysis of Mars Exploration and Colonization Clayton Knappenberger DePauw University Follow this and additional works at: http://scholarship.depauw.edu/studentresearch Part of the Economics Commons, and the The unS and the Solar System Commons Recommended Citation Knappenberger, Clayton, "An Economic Analysis of Mars Exploration and Colonization" (2015). Student research. Paper 28. This Thesis is brought to you for free and open access by the Student Work at Scholarly and Creative Work from DePauw University. It has been accepted for inclusion in Student research by an authorized administrator of Scholarly and Creative Work from DePauw University. For more information, please contact [email protected]. An Economic Analysis of Mars Exploration and Colonization Clayton Knappenberger 2015 Sponsored by: Dr. Villinski Committee: Dr. Barreto and Dr. Brown Contents I. Why colonize Mars? ............................................................................................................................ 2 II. Can We Colonize Mars? .................................................................................................................... 11 III. What would it look like? ............................................................................................................... 16 A. National Program ......................................................................................................................... -
MMM #278 Since December 1986 SEPTEMBER 2014 – P 1
MMM #278 Since December 1986 SEPTEMBER 2014 – p 1 Two worlds of the Inner Solar System that present enormous challenges for human visitors, explorers, and settlers Feature Articles: 2 In Focus: Venus & Mercury: Why Limit Human Frontiers to Moon and Mars? 3 Venus: The Sources of Radical Transformation are already “on Location” 5 Mercury: Discovery of a hidden Settlement Sweet Spot; “Location, Location, Location” 7 Moon Base Costs: Dave Dietzler Below: Previous Articles about Venus have focused on “Aerostat stations” high above the surface, where air pressure and temperatures are human-friendly Above left: a Venus aerostat station - right: at an altitude where temperatures and pressures are benign For past articles, Visit http://www.moonsociety.org/publications/mmm_classics/ or /mmm_themes/ MMM #278 Since December 1986 SEPTEMBER 2014 – p 2 About Moon Miners’ Manifesto - “The Moon - it’s not Earth, but it’s Earth’s!” • MMM’s VISION: “expanding the human economy through of-planet resources”; early heavy reliance on Lunar materials; early use of Mars system and asteroid resources; and permanent settlements supporting this economy. • MMM’s MISSION: to encourage “spin-up” entrepreneurial development of the novel technologies needed and promote the economic-environmental rationale of space and lunar settlement. • Moon Miners’ Manifesto CLASSICS: The non-time-sensitive articles and editorials of MMM’s first twenty years plus have been re-edited, reillustrated, and republished in 23 PDF format volumes, for free downloading from this location: http://www.MoonSociety.org/publications/mmm_classics/ • MMM THEME Issues: 14 collections of articles according to themes: ..../publications/mmm_themes/ • MMM Glossary: new terms, old terms/new meanings: www.moonsociety.org/publications/m3glossary.html • MMM retains its editorial independence and serves many groups, each with its own philosophy, agenda, and programs. -
Environmental Philosophy and the Ethics of Terraforming Mars
ENVIRONMENTAL PHILOSOPHY AND THE ETHICS OF TERRAFORMING MARS: ADDING THE VOICES OF ENVIRONMENTAL JUSTICE AND ECOFEMINISM TO THE ONGOING DEBATE Robert Heath French Thesis Prepared for the Degree of MASTER OF ARTS UNIVERSITY OF NORTH TEXAS August 2013 APPROVED: Robert Figueroa, Committee Chair Eugene Hargrove, Committee Member Adam Briggle, Committee Member Patricia Glazebrook, Chair of the Department of Philosophy and Religion Studies Mark Wardell, Dean of the Toulouse Graduate School French, Robert Heath. Environmental Philosophy and the Ethics of Terraforming Mars: Adding the Voices of Environmental Justice and Ecofeminism to the Ongoing Debate. Master of Arts (Philosophy), August 2013, 133 pp., 1 table, bibliography, 78 titles. Questions concerning the ethics of terraforming Mars have received some attention from both philosophers and scientists during recent decades. A variety of theoretical approaches have been supplied by a number of authors, however research pursuant to this thesis has indicated at least two major blindspots in the published literature on the topic. First, a broad category of human considerations involving risks, dangers, and social, political, and economic inequalities that would likely be associated with efforts to terraform Mars have been woefully overlooked in the published literature to date. I attempt to rectify that oversight by employing the interpretive lens of environmental justice to address questions of environmental colonialism, equality in terms of political participation and inclusion in decision making structures, risks associated with technological progressivism, and responses to anthropogenic climate change. Only by including the historically marginalized and politically disenfranchised “voices,” of both humans and nonhumans, can any future plan to terraform Mars be deemed ethical, moral or just according to the framework provided by environmental justice. -
First Life in Primordial-Planet Oceans: the Biological Big Bang Gibson/Wickramasinghe/Schild First Life in Primordial-Planet Oceans: the Biological Big Bang
Journal of Cosmology First life in primordial-planet oceans: the biological big bang Gibson/Wickramasinghe/Schild First life in primordial-planet oceans: the biological big bang Carl H. Gibson 1,2 1 University of California San Diego, La Jolla, CA 92093-0411, USA [email protected], http://sdcc3.ucsd.edu/~ir118 N. Chandra Wickramasinghe3,4 3Cardiff Centre for Astrobiology, 24 Llwynypia Road, Lisvane, Cardiff CF14 0SY [email protected] Rudolph E. Schild5,6 5 Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA 6 [email protected] Abstract: A scenario is presented for the formation of first life in the universe based on hydro- gravitational-dynamics (HGD) cosmology. From HGD, the dark matter of galaxies is H-He gas dominated planets (primordial-fog-particle PFPs) in million solar mass clumps (protoglobularstar- cluster PGCs), which formed at the plasma to gas transition temperature 3000 K. Stars result from mergers of these hot-gas-planets. Over-accretion causes stars to explode as supernovae that scatter life-chemicals (C, N, O, P, S, Ca, Fe etc.) to other planets in PGC clumps and beyond. These chemicals were first collected gravitationally by merging PFPs to form H-saturated, high-pressure, dense oceans of critical-temperature 647 K water over iron-nickel cores at ~ 2 Myr. Stardust fertil- izes the formation of first life in a cosmic hot-ocean soup kitchen comprised of all planets and their moons in meteoric communication, > 10100 kg in total. Ocean freezing at 273 K slows this biologi- cal big bang at ~ 8 Myr. HGD cosmology confirms that the evolving seeds of life are scattered on intergalactic scales by Hoyle-Wickramasinghe cometary panspermia. -
Origins of Life: a Problem for Physics
Origins of Life: A Problem for Physics Sara Imari Walker School of Earth and Space Exploration and Beyond Center for Fundamental Concepts in Science, Arizona State University, Tempe AZ USA; Blue Marble Space Institute of Science, Seattle WA USA E-mail: [email protected] Abstract. The origins of life stands among the great open scientific questions of our time. While a number of proposals exist for possible starting points in the pathway from non-living to living matter, these have so far not achieved states of complexity that are anywhere near that of even the simplest living systems. A key challenge is identifying the properties of living matter that might distinguish living and non-living physical systems such that we might build new life in the lab. This review is geared towards covering major viewpoints on the origin of life for those new to the origin of life field, with a forward look towards considering what it might take for a physical theory that universally explains the phenomenon of life to arise from the seemingly disconnected array of ideas proposed thus far. The hope is that a theory akin to our other theories in fundamental physics might one day emerge to explain the phenomenon of life, and in turn finally permit solving its origins. arXiv:1705.08073v1 [q-bio.PE] 23 May 2017 CONTENTS 2 Contents 1 Introduction 2 2 Knowns and unknowns in solving the origin of life 4 2.1 One planet, one sample: The significance of anthropic bias . .5 2.2 Two paths to a solution . -
Moon-Miners-Manifesto-Mars.Pdf
http://www.moonsociety.org/mars/ Let’s make the right choice - Mars and the Moon! Advantages of a low profile for shielding Mars looks like Arizona but feels like Antarctica Rover Opportunity at edge of Endeavor Crater Designing railroads and trains for Mars Designing planes that can fly in Mars’ thin air Breeding plants to be “Mars-hardy” Outposts between dunes, pulling sand over them These are just a few of the Mars-related topics covered in the past 25+ years. Read on for much more! Why Mars? The lunar and Martian frontiers will thrive much better as trading partners than either could on it own. Mars has little to trade to Earth, but a lot it can trade with the Moon. Both can/will thrive together! CHRONOLOGICAL INDEX MMM THEMES: MARS MMM #6 - "M" is for Missing Volatiles: Methane and 'Mmonia; Mars, PHOBOS, Deimos; Mars as I see it; MMM #16 Frontiers Have Rough Edges MMM #18 Importance of the M.U.S.-c.l.e.Plan for the Opening of Mars; Pavonis Mons MMM #19 Seizing the Reins of the Mars Bandwagon; Mars: Option to Stay; Mars Calendar MMM #30 NIMF: Nuclear rocket using Indigenous Martian Fuel; Wanted: Split personality types for Mars Expedition; Mars Calendar Postscript; Are there Meteor Showers on Mars? MMM #41 Imagineering Mars Rovers; Rethink Mars Sample Return; Lunar Development & Mars; Temptations to Eco-carelessness; The Romantic Touch of Old Barsoom MMM #42 Igloos: Atmosphere-derived shielding for lo-rem Martian Shelters MMM #54 Mars of Lore vs. Mars of Yore; vendors wanted for wheeled and walking Mars Rovers; Transforming Mars; Xities -
V Isysphere Mars: Terraforming Meets Eng Ineered Life Adaptation MSS
Visysphere mars: Terraforming meets engineered life adaptation MSS/MSM 2005 Visysphere Mars Terraforming Meets Engineered Life Adaptation International Space University Masters Program 2005 © International Space University. All Rights Reserved. Front Cover Artwork: “From Earth to Mars via technology and life”. Connecting the two planets through engineering of technology and life itself to reach the final goal of a terraformed Mars. The Executive Summary, ordering information and order forms may be found on the ISU web site at http://www.isunet.edu/Services/library/isu_publications.htm. Copies of the Executive Summary and the Final Report can also be ordered from: International Space University Strasbourg Central Campus Parc d’Innovation 1 rue Jean-Dominique Cassini 67400 Illkirch-Graffenstaden France Tel. +33 (0)3 88 65 54 32 Fax. +33 (0)3 88 65 54 47 e-mail. [email protected] ii International Space University, Masters 2005 Visysphere Mars Acknowledgements ACKNOWLEDGEMENTS The International Space University and the students of the Masters Program 2005 would like to thank the following people for their generous support and guidance: Achilleas, Philippe Hill, Hugh Part-Time Faculty Faculty, Space Science International Space University International Space University IDEST, Université Paris Sud, France Lapierre, Bernard Arnould, Jacques Coordinator “Ethics Applied to Special Advisor to the President Engineering” course. CNES Ecole Polytechnique of Montreal Averner, Mel Marinova, Margarita Program Manager, Fundamental Planetary -
Primordial Planets, Comets and Moons Foster Life in the Cosmos
Primordial planets, comets and moons foster life in the cosmos Carl H. Gibsona*, N. Chandra Wickramasingheb and Rudolph E. Schildc a UCSD, La Jolla, CA, 92093-0411, USA; b Cardiff Univ., Cardiff, UK; c Harvard, Cambridge, MA, USA ABSTRACT A key result of hydrogravitational dynamics cosmology relevant to astrobiology is the early formation of vast numbers of hot primordial-gas planets in million-solar-mass clumps as the dark matter of galaxies and the hosts of first life. Photon viscous forces in the expanding universe of the turbulent big bang prevent fragmentations of the plasma for mass scales smaller than protogalaxies. At the plasma to gas transition 300,000 years after the big bang, the 107 decrease in kinematic viscosity ν explains why ~3x107 planets are observed to exist per star in typical galaxies like the Milky Way, not eight or nine. Stars form by a binary accretional cascade from Earth-mass primordial planets to progressively larger masses that collect and recycle the stardust chemicals of life produced when stars overeat and explode. The astonishing complexity of molecular biology observed on Earth is possible to explain only if enormous numbers of primordial planets and their fragments have hosted the formation and wide scattering of the seeds of life virtually from the beginning of time. Geochemical and biological evidence suggests that life on Earth appears at the earliest moment it can survive, in highly evolved forms with complexity requiring a time scale in excess of the age of the galaxy. This is quite impossible within standard cold-dark-matter cosmology where planets are relatively recent, rare and cold, completely lacking mechanisms for intergalactic transport of life forms. -
Planetary Protection
OPEN ACCESS Freelyavailableonline Journal of Astrobiology &Outreach Editorial Terraforming of Mars Environment * Pekka Janhunen Department of Astrobiology, Finnish Meteorological Institute, Space Research, Helsinki, Finland ABSTRACT Mars also features a history of being wet and plush. It has been theorized that when it had been first formed 4.2 billion years ago it had an environment and high amounts of water. Since Mars is far smaller than Earth, its internal core gradually hardened, which caused Mars to lose its magnetic flux? Without a protective magnetic flux, the solar radiation was ready to strip away most of the Martian atmosphere. The end result's that over subsequent 500 million years, Mars gradually transformed from a warm, wet planet to a chilly, dry planet. Around 3.7 billion years ago, Mars eventually became almost like the barren planet we all know of today. Despite this, there's evidence that water still exists on Mars. Water in the form of ice has been found at the poles and underground in the Utopia Plantain region of Mars. There is up to five million cubic kilometers of ice on Mars, and if this were to be spread evenly over everything of the surface of Mars it would submerge the planet under 35 meters of water. Keywords: Mars, Utopia plantain region, Martian atmosphere INTRODUCTION or her visual or olfactory qualities. This, unfortunately, pales in comparison to the 1.36 billion cubic If we are to urge an accurate picture of the potential wealth to be kilometers of water found on Earth, but it is a start. We are gained from the system, we must recognize the successive waves of currently on the hunt for life on Mars, but this has not been economic energy through which our civilization is passing. -
The Thermodynamics of Planetary Engineering on the Planet Mars
University of Central Florida STARS HIM 1990-2015 2014 The Thermodynamics of Planetary Engineering on the Planet Mars Christopher Barsoum University of Central Florida Part of the Aerospace Engineering Commons Find similar works at: https://stars.library.ucf.edu/honorstheses1990-2015 University of Central Florida Libraries http://library.ucf.edu This Open Access is brought to you for free and open access by STARS. It has been accepted for inclusion in HIM 1990-2015 by an authorized administrator of STARS. For more information, please contact [email protected]. Recommended Citation Barsoum, Christopher, "The Thermodynamics of Planetary Engineering on the Planet Mars" (2014). HIM 1990-2015. 1552. https://stars.library.ucf.edu/honorstheses1990-2015/1552 THE THERMODYNAMICS OF PLANETARY ENGINEERING ON THE PLANET MARS by CHRISTOPHER BARSOUM A thesis submitted in partial fulfillment of the requirements for the Honors in the Major Program in Aerospace Engineering in the College of Mechanical and Aerospace Engineering and in The Burnett Honors College at the University of Central Florida Orlando, Florida Spring Term 2014 Thesis Chair: Dr. Kuo-Chi Lin © 2014 Christopher Barsoum ii ABSTRACT Mars is a potentially habitable planet given the appropriate planetary engineering efforts. In order to create a habitable environment, the planet must be terraformed, creating quasi-Earth conditions. Benchmarks for minimum acceptable survivable human conditions were set by observing atmospheric pressures and temperatures here on Earth that humans are known to exist in. By observing a positive feedback reaction, it is shown how the sublimation of the volatile southern polar ice cap on Mars can increase global temperatures and pressures to the benchmarks set for minimum acceptable survivable human conditions. -
Mapping Disciplinary Relationships in Astrobiology: 2001-2012
Western Washington University Western CEDAR WWU Graduate School Collection WWU Graduate and Undergraduate Scholarship 2014 Mapping disciplinary relationships in Astrobiology: 2001-2012 Jason W. Cornell Western Washington University Follow this and additional works at: https://cedar.wwu.edu/wwuet Part of the Geography Commons Recommended Citation Cornell, Jason W., "Mapping disciplinary relationships in Astrobiology: 2001-2012" (2014). WWU Graduate School Collection. 387. https://cedar.wwu.edu/wwuet/387 This Masters Thesis is brought to you for free and open access by the WWU Graduate and Undergraduate Scholarship at Western CEDAR. It has been accepted for inclusion in WWU Graduate School Collection by an authorized administrator of Western CEDAR. For more information, please contact [email protected]. Mapping Disciplinary Relationships in Astrobiology: 2001 - 2012 By Jason W. Cornell Accepted in Partial Completion Of the Requirements for the Degree Master of Science Kathleen L. Kitto, Dean of the Graduate School ADVISORY COMMITTEE Chair, Dr. Gigi Berardi Dr. Linda Billings Dr. David Rossiter ! ! MASTER’S THESIS In presenting this thesis in partial fulfillment of the requirements for a master’s degree at Western Washington University, I grant to Western Washington University the non-exclusive royalty-free right to archive, reproduce, distribute, and display the thesis in any and all forms, including electronic format, via any digital library mechanisms maintained by WWU. I represent and warrant this is my original work, and does not infringe or violate any rights of others. I warrant that I have obtained written permission from the owner of any third party copyrighted material included in these files. I acknowledge that I retain ownership rights to the copyright of this work, including but not limited to the right to use all or part of this work in future works, such as articles or books.