4. Lunar Architecture

Total Page:16

File Type:pdf, Size:1020Kb

4. Lunar Architecture 4. Lunar Architecture 4.1 Summary and Recommendations As defined by the Exploration Systems Architecture Study (ESAS), the lunar architecture is a combination of the lunar “mission mode,” the assignment of functionality to flight elements, and the definition of the activities to be performed on the lunar surface. The trade space for the lunar “mission mode,” or approach to performing the crewed lunar missions, was limited to the cislunar space and Earth-orbital staging locations, the lunar surface activities duration and location, and the lunar abort/return strategies. The lunar mission mode analysis is detailed in Section 4.2, Lunar Mission Mode. Surface activities, including those performed on sortie- and outpost-duration missions, are detailed in Section 4.3, Lunar Surface Activities, along with a discussion of the deployment of the outpost itself. The mission mode analysis was built around a matrix of lunar- and Earth-staging nodes. Lunar-staging locations initially considered included the Earth-Moon L1 libration point, Low Lunar Orbit (LLO), and the lunar surface. Earth-orbital staging locations considered included due-east Low Earth Orbits (LEOs), higher-inclination International Space Station (ISS) orbits, and raised apogee High Earth Orbits (HEOs). Cases that lack staging nodes (i.e., “direct” missions) in space and at Earth were also considered. This study addressed lunar surface duration and location variables (including latitude, longi- tude, and surface stay-time) and made an effort to preserve the option for full global landing site access. Abort strategies were also considered from the lunar vicinity. “Anytime return” from the lunar surface is a desirable option that was analyzed along with options for orbital and surface loiter. The duration, location, and centralization of lunar surface activities were analyzed by first determining the content of the science, resource utilization, Mars-forward technology demon- strations, and operational tests that could be performed during the lunar missions. The study team looked at high-priority landing sites and chose a reference site in order to further inves- tigate the operations at a permanent outpost. With the scientific and engineering activities defined, concept-level approaches for the deployment and buildup of the outpost were created. A comprehensive definition of lunar surface elements and infrastructure was not performed because development activities for lunar surface elements are still years in the future. There- fore, the ESAS team concentrated its recommendations on those elements that had the greatest impact on near-term decisions. 4. Lunar Architecture 75 The mission architecture decisions that most greatly affect near-term NASA development activities are mission mode, propulsion system types, and mission duration. The ESAS team recommends the use of an Earth Orbit Rendezvous-Lunar Orbit Rendezvous (EOR–LOR) mission mode. This mission mode, which can be executed with a combination of the launch of separate crew and cargo vehicles, was found to result in a Low Life Cycle Cost (LCC) and the highest crew safety and mission reliability combination. Further, the study found that pressure-fed Liquid Oxygen (LOX)/methane propulsion should be used for the lander ascent stage as well as the Crew Exploration Vehicle (CEV) Service Module (SM), which should be sized to perform the Trans-Earth Injection (TEI) propulsive maneuver for a lunar mission. The study also concluded that the lunar lander should use a LOX/hydrogen throttleable propulsion system for Lunar Orbit Insertion (LOI) and landing. The two-stage lander should include an airlock and be sized to support a 7-day surface mission with four crew members. 76 4. Lunar Architecture 4.2 Lunar Mission Mode The lunar mission mode is the fundamental lunar architecture decision that defines where space flight elements come together and what functions each of these elements perform. Mission mode analysis had its genesis early in the design of the Apollo Program, with notable NASA engineers and managers such as Wernher Von Braun, John Houbolt, Joe Shea, and Robert Seamans contributing to the decision to use LOR as the Apollo mission mode. This study built on the foundation of the Apollo decision but sought to question whether the LOR decision and overall Apollo mission approach were still valid, given new missions require- ments and technology. The ESAS team researched many of the Apollo lunar landing mode comparison studies as well as more recent studies performed by both NASA and industry. One study of interest, performed by a Massachusetts Institute of Technology (MIT)-Draper Laboratory team as part of a “Concept Exploration and Refinement” (CE&R) contract to NASA, suggested that the Apollo mission mode was no longer valid and that NASA should consider “direct return” modes for future human lunar missions. The ESAS team took special note of this study and sought to challenge all of the Apollo mission assumptions. 4.2.1 Previous Lunar Architecture Study Results Since its inception, NASA has conducted or sponsored numerous studies of human explo- ration beyond LEO. These studies have been used to understand requirements for human exploration of the Moon and Mars in the context of other space missions and Research and Development (R&D) programs. Each exploration architecture provides an end-to-end mission baseline against which other mission and technology concepts can be compared. The results from the architecture studies were used to: • Derive technology R&D plans; • Define and prioritize requirements for precursor robotic missions; • Define and prioritize flight experiments and human exploration mission elements, such as those involving the Space Shuttle, ISS, and other Space Transportation Systems (STSs); • Open a discussion with international partners in a manner that allows identification of participants’ potential interests in specialized aspects of the missions; and • Describe to the public, media, and Government stakeholders the feasible, long-term visions for space exploration. 4. Lunar Architecture 77 Each architecture study emphasized one or more critical aspects of human exploration in order to determine basic feasibility and technology needs. Examples of architectural areas of emphasis include: • Destination: Moon ↔ Mars ↔ Libration Points ↔ Asteroids; • System Reusability: Expendable ↔ Reusable; • Architecture Focus: Sorties ↔ Colonization; • Surface Mobility: Local ↔ Global; • Launch Vehicles (LVs): Existing ↔ New Heavy-Lift; • Transportation: Numerous stages and technologies traded; • LEO Assembly: None ↔ Extensive; • Transit Modes: Zero-gravity ↔ Artificial-gravity; • Surface Power: Solar ↔ Nuclear; • Crew Size: 4 ↔ 24; and • In Situ Resource Utilization (ISRU): None ↔ Extensive. The ESAS team extensively scrutinized the NASA studies that led to the Apollo Program, most notably studies to determine the shape of the Apollo capsule and the mode used for the Apollo missions. Additionally, the team reviewed the findings of human lunar and Mars mission studies performed over the past 15 years. A summary of these studies is shown in Table 4-1. Office of Exploration (OExP) - 1988 Case Studies First Lunar Outpost - 1993 Human Expedition to Phobos Early Lunar Resource Utilization - 1993 Human Expedition to Mars Human Lunar Return - 1996 Lunar Observatory Lunar Outpost to Early Mars Evolution Mars Exploration Missions Design Reference Mission Version 1.0 - 1994 Office of Exploration (OExP) - 1989 Case Studies Design Reference Mission Version 3.0 - 1997 Lunar Evolution Design Reference Mission Version 4.0 - 1998 Mars Evolution Mars Combo Lander (Johnson Space Center (JSC)) - 1999 Mars Expedition Dual Landers – 1999 NASA 90-Day Study - 1989 Decadal Planning Team (DPT)/NASA Exploration Team (NExT) - 2000–2002 Approach A - Moon as testbed for Mars missions Earth’s Neighborhood Architecture Approach B - Moon as testbed for early Mars missions Asteroid Missions Approach C - Moon as testbed for Mars Outposts Mars Short and Long Stay Approach D - Relaxed mission dates Exploration Blueprint - 2002 Approach E - Lunar outpost followed by Mars missions Space Architect - 2003 America at the Threshold - “The Synthesis Group” - 1991 Exploration Systems Mission Directorate (ESMD) 2004–2005 Mars Exploration Science Emphasis for the Moon and Mars The Moon to Stay and Mars Exploration Space Resource Utilization Table 4-1. Summary of Previous NASA Architecture Studies 78 4. Lunar Architecture 4.2.1.1 Summary of Previous Studies 4.2.1.1.1 Office of Exploration Case Studies (1988) In June 1987, the NASA Administrator established the Office of Exploration (OExP) in response to an urgent national need for a long-term goal to reenergize the U.S. civilian space program. The OExP originated as a result of two significant assessments conducted prior to its creation. In 1986, the National Commission on Space, as appointed by the President and charged by the Congress, formulated a bold agenda to carry America’s civilian space enter- prise into the 21st century (number 1 in Section 4.5, Endnotes). Later that year, the NASA Administrator asked scientist and astronaut Sally Ride to lead a task force to look at potential long-range goals of the U.S. civilian space program. The subsequent task force report, “Lead- ership and America’s Future in Space,” (number 2 in Section 4.5, Endnotes) outlined four initiatives which included both human and robotic exploration of the solar system. In response to the task force report, the OExP conducted
Recommended publications
  • Reference System Issues in Binary Star Calculations
    Reference System Issues in Binary Star Calculations Poster for Division A Meeting DAp.1.05 George H. Kaplan Consultant to U.S. Naval Observatory Washington, D.C., U.S.A. [email protected] or [email protected] IAU General Assembly Honolulu, August 2015 1 Poster DAp.1.05 Division!A! !!!!!!Coordinate!System!Issues!in!Binary!Star!Computa3ons! George!H.!Kaplan! Consultant!to!U.S.!Naval!Observatory!!([email protected][email protected])! It!has!been!es3mated!that!half!of!all!stars!are!components!of!binary!or!mul3ple!systems.!!Yet!the!number!of!known!orbits!for!astrometric!and!spectroscopic!binary!systems!together!is! less!than!7,000!(including!redundancies),!almost!all!of!them!for!bright!stars.!!A!new!genera3on!of!deep!allLsky!surveys!such!as!PanLSTARRS,!Gaia,!and!LSST!are!expected!to!lead!to!the! discovery!of!millions!of!new!systems.!!Although!for!many!of!these!systems,!the!orbits!may!be!poorly!sampled!ini3ally,!it!is!to!be!expected!that!combina3ons!of!new!and!old!data!sources! will!eventually!lead!to!many!more!orbits!being!known.!!As!a!result,!a!revolu3on!in!the!scien3fic!understanding!of!these!systems!may!be!upon!us.! The!current!database!of!visual!(astrometric)!binary!orbits!represents!them!rela3ve!to!the!“plane!of!the!sky”,!that!is,!the!plane!orthogonal!to!the!line!of!sight.!!Although!the!line!of!sight! to!stars!constantly!changes!due!to!proper!mo3on,!aberra3on,!and!other!effects,!there!is!no!agreed!upon!standard!for!what!line!of!sight!defines!the!orbital!reference!plane.!! Furthermore,!the!computa3on!of!differen3al!coordinates!(component!B!rela3ve!to!A)!for!a!given!date!must!be!based!on!the!binary!system’s!direc3on!at!that!date.!!Thus,!a!different!
    [Show full text]
  • Sentinel-1 Constellation SAR Interferometry Performance Verification
    Sentinel-1 Constellation SAR Interferometry Performance Verification Dirk Geudtner1, Francisco Ceba Vega1, Pau Prats2 , Nestor Yaguee-Martinez2 , Francesco de Zan3, Helko Breit3, Andrea Monti Guarnieri4, Yngvar Larsen5, Itziar Barat1, Cecillia Mezzera1, Ian Shurmer6 and Ramon Torres1 1 ESA ESTEC 2 DLR, Microwaves and Radar Institute 3 DLR, Remote Sensing Technology Institute 4 Politecnico Di Milano 5 Northern Research Institute (Norut) 6 ESA ESOC ESA UNCLASSIFIED - For Official Use Outline • Introduction − Sentinel-1 Constellation Mission Status − Overview of SAR Imaging Modes • Results from the Sentinel-1B Commissioning Phase • Azimuth Spectral Alignment Impact on common − Burst synchronization Doppler bandwidth − Difference in mean Doppler Centroid Frequency (InSAR) • Sentinel-1 Orbital Tube and InSAR Baseline • Demonstration of cross S-1A/S-1B InSAR Capability for Surface Deformation Mapping ESA UNCLASSIFIED - For Official Use ESA Slide 2 Sentinel-1 Constellation Mission Status • Constellation of two SAR C-band (5.405 GHz) satellites (A & B units) • Sentinel-1A launched on 3 April, 2014 & Sentinel-1B on 25 April, 2016 • Near-Polar, sun-synchronous (dawn-dusk) orbit at 698 km • 12-day repeat cycle (each satellite), 6 days for the constellation • Systematic SAR data acquisition using a predefined observation scenario • More than 10 TB of data products daily (specification of 3 TB) • 3 X-band Ground stations (Svalbard, Matera, Maspalomas) + upcoming 4th core station in Inuvik, Canada • Use of European Data Relay System (EDRS) provides
    [Show full text]
  • Domi Inter Astra
    Team members Alice Sueko Müller | Anshoo Mehra | Chaitnya Chopra | Ekaterina Seltikova Isabel Alonso Serrano | James Xie | Jay Kamdar | Julie Pradel | Kunal Kulkarni Matej Poliaček | Myles Harris | Nitya Jagadam | Richal Abhang | Ruvimbo Samanga | Sagarika Rao Valluri Sanket Kalambe | Sejal Budholiya | Selene Cannelli Space Generation Advisory Council Team 1 Contents Society and Culture 3 Tourist Attractions 3 Astronaut and Tourist Selection 3 Architecture 4 Module 1: Greenhouse, Guest Amenities, Medicine, and Environmental Control 5 Module 2: Social Space and Greenhouse 5 Module 3: Kitchen, Fitness, Hygiene, and Social 6 Module 3: Sky-view 6 Module 4: Crew Bedrooms and Private Social Space 6 Module 5: Workspace 6 Management and Politics 7 Governance, Ownership, and Intellectual Property 7 Crew Operations 7 Base Management System 8 Safety & Emergency Planning 8 Engineering 9 Landing & Settlement Site 9 Settlement Structure 10 Robotics and Extravehicular Activities (EVAs) 10 Construction Timeline 11 Communications System 12 Critical Life Support (Air & Water) Systems 12 Thermal System 13 Food & Human Waste Recycling 14 Other Waste 14 Technical Floor Plan 14 Power Generation & Storage 14 Economy 16 Capital & Operating Costs 16 Revenue Generation 17 Tourism & Outreach 17 Commercial Activities 18 Lunar Manufacturing 18 References 20 ntariksha, aptly meaning ‘the universe’ in to be a giant leap for all the young girls around the Sanskrit, is an avid stargazer fascinated world, and she knew something incredible is waiting by the blanket of splurging stars she saw to be known. from her village in North East India. To- day, her joy knew no bounds upon learn- “Each civilization must become space-faring or ex- ingA that she would get a chance to visit Domi Inter tinct”.
    [Show full text]
  • Circular Orbits
    ANALYSIS AND MECHANIZATION OF LAUNCH WINDOW AND RENDEZVOUS COMPUTATION PART I. CIRCULAR ORBITS Research & Analysis Section Tech Memo No. 175 March 1966 BY J. L. Shady Prepared for: NATIONAL AERONAUTICS AND SPACE ADMINISTRATION / GEORGE C. MARSHALL SPACE FLIGHT CENTER AERO-ASTRODYNAMICS LABORATORY Prepared under Contract NAS8-20082 Reviewed by: " D. L/Cooper Technical Supervisor Director Research & Analysis Section / NORTHROP SPACE LABORATORIES HUNTSVILLE DEPARTMENT HUNTSVILLE, ALABAMA FOREWORD The enclosed presents the results of work performed by Northrop Space Laboratories, Huntsville Department, while )under contract to the Aero- Astrodynamfcs Laboratory of Marshall Space Flight Center (NAS8-20082) * This task was conducted in response to the requirement of Appendix E-1, Schedule Order No. PO. Technical coordination was provided by Mr. Jesco van Puttkamer of the Technical and Scientific Staff (R-AERO-T) ABS TRACT This repart presents Khe results of an analytical study to develop the logic for a digrtal c3mp;lrer sclbrolrtine for the automatic computationof launch opportunities, or the sequence of launch times, that rill allow execution of various mades of gross ~ircuiarorbit rendezvous. The equations developed in this study are based on tho-bady orb:taf chmry. The Earch has been assumed tcr ha.:e the shape of an oblate spheroid. Oblateness of the Earth has been accounted for by assuming the circular target orbit to be space- fixed and by cosrecring che T ational raLe of the EarKh accordingly. Gross rendezvous between the rarget vehicle and a maneuverable chaser vehicle, assumed to be a standard 3+ uprated Saturn V launched from Cape Kennedy, is in this srudy aecomplfshed by: .x> direct ascent to rendezvous, or 2) rendezvous via an intermediate circG1a.r parking orbit.
    [Show full text]
  • Gryphon: a Flexible Lunar Lander Design to Support a Semi-Permanent Lunar Outpost
    AIAA SPACE 2007 Conference & Exposition AIAA 2007-6169 18 - 20 September 2007, Long Beach, California The Gryphon: A Flexible Lunar Lander Design to Support a Semi-Permanent Lunar Outpost Dale Arney1, Joseph Hickman,1 Philip Tanner,1 John Wagner,1 Marc Wilson,1 and Dr. Alan Wilhite2 Georgia Institute of Technology/National Institute of Aerospace, Hampton, VA, 23666 A lunar lander is designed to provide safe, reliable, and continuous access to the lunar surface by the year 2020. The NASA Exploration System Architecture is used to initially define the concept of operations, architecture elements, and overall system requirements. The design evaluates revolutionary concepts and technologies to improve the performance and safety of the lunar lander while minimizing the associated cost using advanced systems engineering capabilities and multi-attribute decision making techniques. The final design is a flexible (crew and/or cargo) lander with a side-mounted minimum ascent stage and a separate stage to perform lunar orbit insertion. Nomenclature ACC = Affordability and Cost Criterion AFM = Autonomous Flight Manager AHP = Analytic Hierarchy Process ALHAT = Autonomous Landing and Hazard Avoidance Technology ATP = Authority to Proceed AWRS = Advanced Air & Water Recovery System CDR = Critical Design Review CER = Cost Estimating Relationship CEV = Crew Exploration Vehicle CH4 = Methane DDT&E = Design, Development, Testing and Evaluation DOI = Descent Orbit Insertion DSM = Design Structure Matrix ECLSS = Environmental Control & Life Support System
    [Show full text]
  • Glossary Glossary
    Glossary Glossary Albedo A measure of an object’s reflectivity. A pure white reflecting surface has an albedo of 1.0 (100%). A pitch-black, nonreflecting surface has an albedo of 0.0. The Moon is a fairly dark object with a combined albedo of 0.07 (reflecting 7% of the sunlight that falls upon it). The albedo range of the lunar maria is between 0.05 and 0.08. The brighter highlands have an albedo range from 0.09 to 0.15. Anorthosite Rocks rich in the mineral feldspar, making up much of the Moon’s bright highland regions. Aperture The diameter of a telescope’s objective lens or primary mirror. Apogee The point in the Moon’s orbit where it is furthest from the Earth. At apogee, the Moon can reach a maximum distance of 406,700 km from the Earth. Apollo The manned lunar program of the United States. Between July 1969 and December 1972, six Apollo missions landed on the Moon, allowing a total of 12 astronauts to explore its surface. Asteroid A minor planet. A large solid body of rock in orbit around the Sun. Banded crater A crater that displays dusky linear tracts on its inner walls and/or floor. 250 Basalt A dark, fine-grained volcanic rock, low in silicon, with a low viscosity. Basaltic material fills many of the Moon’s major basins, especially on the near side. Glossary Basin A very large circular impact structure (usually comprising multiple concentric rings) that usually displays some degree of flooding with lava. The largest and most conspicuous lava- flooded basins on the Moon are found on the near side, and most are filled to their outer edges with mare basalts.
    [Show full text]
  • Apollo Program 1 Apollo Program
    Apollo program 1 Apollo program The Apollo program was the third human spaceflight program carried out by the National Aeronautics and Space Administration (NASA), the United States' civilian space agency. First conceived during the Presidency of Dwight D. Eisenhower as a three-man spacecraft to follow the one-man Project Mercury which put the first Americans in space, Apollo was later dedicated to President John F. Kennedy's national goal of "landing a man on the Moon and returning him safely to the Earth" by the end of the 1960s, which he proposed in a May 25, 1961 address to Congress. Project Mercury was followed by the two-man Project Gemini (1962–66). The first manned flight of Apollo was in 1968 and it succeeded in landing the first humans on Earth's Moon from 1969 through 1972. Kennedy's goal was accomplished on the Apollo 11 mission when astronauts Neil Armstrong and Buzz Aldrin landed their Lunar Module (LM) on the Moon on July 20, 1969 and walked on its surface while Michael Collins remained in lunar orbit in the command spacecraft, and all three landed safely on Earth on July 24. Five subsequent Apollo missions also landed astronauts on the Moon, the last in December 1972. In these six spaceflights, 12 men walked on the Moon. Apollo ran from 1961 to 1972, and was supported by the two-man Gemini program which ran concurrently with it from 1962 to 1966. Gemini missions developed some of the space travel techniques that were necessary for the success of the Apollo missions.
    [Show full text]
  • Project Horizon Report
    Volume I · SUMMARY AND SUPPORTING CONSIDERATIONS UNITED STATES · ARMY CRD/I ( S) Proposal t c• Establish a Lunar Outpost (C) Chief of Ordnance ·cRD 20 Mar 1 95 9 1. (U) Reference letter to Chief of Ordnance from Chief of Research and Devel opment, subject as above. 2. (C) Subsequent t o approval by t he Chief of Staff of reference, repre­ sentatives of the Army Ballistic ~tissiles Agency indicat e d that supplementar y guidance would· be r equired concerning the scope of the preliminary investigation s pecified in the reference. In particular these r epresentatives requested guidance concerning the source of funds required to conduct the investigation. 3. (S) I envision expeditious development o! the proposal to establish a lunar outpost to be of critical innportance t o the p. S . Army of the future. This eva luation i s appar ently shar ed by the Chief of Staff in view of his expeditious a pproval and enthusiastic endorsement of initiation of the study. Therefore, the detail to be covered by the investigation and the subs equent plan should be as com­ plete a s is feas ible in the tin1e limits a llowed and within the funds currently a vailable within t he office of t he Chief of Ordnance. I n this time of limited budget , additional monies are unavailable. Current. programs have been scrutinized r igidly and identifiable "fat'' trimmed awa y. Thus high study costs are prohibitive at this time , 4. (C) I leave it to your discretion t o determine the source and the amount of money to be devoted to this purpose.
    [Show full text]
  • Materials for Liquid Propulsion Systems
    https://ntrs.nasa.gov/search.jsp?R=20160008869 2019-08-29T17:47:59+00:00Z CHAPTER 12 Materials for Liquid Propulsion Systems John A. Halchak Consultant, Los Angeles, California James L. Cannon NASA Marshall Space Flight Center, Huntsville, Alabama Corey Brown Aerojet-Rocketdyne, West Palm Beach, Florida 12.1 Introduction Earth to orbit launch vehicles are propelled by rocket engines and motors, both liquid and solid. This chapter will discuss liquid engines. The heart of a launch vehicle is its engine. The remainder of the vehicle (with the notable exceptions of the payload and guidance system) is an aero structure to support the propellant tanks which provide the fuel and oxidizer to feed the engine or engines. The basic principle behind a rocket engine is straightforward. The engine is a means to convert potential thermochemical energy of one or more propellants into exhaust jet kinetic energy. Fuel and oxidizer are burned in a combustion chamber where they create hot gases under high pressure. These hot gases are allowed to expand through a nozzle. The molecules of hot gas are first constricted by the throat of the nozzle (de-Laval nozzle) which forces them to accelerate; then as the nozzle flares outwards, they expand and further accelerate. It is the mass of the combustion gases times their velocity, reacting against the walls of the combustion chamber and nozzle, which produce thrust according to Newton’s third law: for every action there is an equal and opposite reaction. [1] Solid rocket motors are cheaper to manufacture and offer good values for their cost.
    [Show full text]
  • Commercial Lunar Propellant Architecture a Collaborative Study of Lunar Propellant Production
    Commercial Lunar Propellant Architecture A Collaborative Study of Lunar Propellant Production 1 To the Memory of: Dr. Paul D. Spudis (1952–2018) Dr. Spudis earned his master’s degree from Brown University and his Ph.D. from Arizona State University in Geology with a focus on the Moon. His career included work at the US Geological Survey, NASA, John Hopkins University Applied Physics Laboratory, and the Lunar and Planetary Institute advocating for the exploration and the utilization of lunar resources. His work will continue to inspire and guide us all on our journey to the Moon. “By going to the Moon we can learn how to extract what we need in space from what we find in space. Fundamentally that is a skill that any spacefaring civilization has to master. If you can learn to do that, you’ve got a skill that will allow you to go to Mars and beyond.” ii Authors David Kornuta, United Launch Alliance, CisLunar Project Lead1 Angel Abbud-Madrid, Colorado School of Mines, Professor of Space Resources Jared Atkinson, Honeybee Robotics, Senior Geophysical Engineer Jonathan Barr, United Launch Alliance, Program Manager Gary Barnhard, Xtraordinary Innovative Space Partnership, CEO Dallas Bienhoff, Cislunar Space Development Company LLC, Founder Brad Blair, NewSpace Analytics, Managing Partner Vanessa Clark, Atomos Nuclear and Space, Chief Executive and Technology Officer Justin Cyrus, Lunar Outpost, CEO Blair DeWitt, Lunar Station Corporation, CEO and Co-Founder Chris Dreyer, Colorado School of Mines, Professor of Space Resources Barry Finger, Paragon
    [Show full text]
  • Location #1: Peary/Whipple Crater
    Location, Location, Location A Lunar Investment Strategy Hoyt Davidson Near Earth LLC June 2017 ISU's International Institute of Space Commerce Lunar Economic Action Plan (LEAP) Space and Questions from 1960 Still Relevant Today Economic Development • How can we utilize our dynamic system of competitive private enterprise in space, as on earth, to make newly discovered resources useful to man? • How can private enterprise and private capital make their maximum contribution? Philosophy and Policy The ultimate goal is not to impress others, or merely to explore our planetary system, but to use accessible space for the benefit of humankind. It is a goal that is not confined to a decade or a century. Nor is it confined to a single nearby destination, or to a fleeting dash to plant a flag. The idea is to begin preparing now for a future in which the material trapped in the Sun's vicinity is available for incorporation into our way of life. Dr. John Marburger, Head of the Office of Science and Technology Policy 2006 3 The Investment Premise • Just as on Earth, lunar real estate “value” is driven by location, location, location Rank Location Why Valuable 1 Peary Crater Best 1st industrial base and settlement 2 Sinus Medii Good cargo port & space elevator site 3 Largest skylights / lava tubes Best large scale settlements 4 Tsiolkovskiy crater, dark side Prime radio astronomy site 5 High helium-3 concentrations Potential high value mining 6 Lipsky Crater Space elevator site for Earth-Moon L2 7 Aristillus High Thorium concentrations • Lunar real
    [Show full text]
  • Mobile Lunar and Planetary Base Architectures
    Space 2003 AIAA 2003-6280 23 - 25 September 2003, Long Beach, California Mobile Lunar and Planetary Bases Marc M. Cohen, Arch.D. Advanced Projects Branch, Mail Stop 244-14, NASA-Ames Research Center, Moffett Field, CA 94035-1000 TEL 650 604-0068 FAX 650 604-0673 [email protected] ABSTRACT This paper presents a review of design concepts over three decades for developing mobile lunar and planetary bases. The idea of the mobile base addresses several key challenges for extraterrestrial surface bases. These challenges include moving the landed assets a safe distance away from the landing zone; deploying and assembling the base remotely by automation and robotics; moving the base from one location of scientific or technical interest to another; and providing sufficient redundancy, reliability and safety for crew roving expeditions. The objective of the mobile base is to make the best use of the landed resources by moving them to where they will be most useful to support the crew, carry out exploration and conduct research. This review covers a range of surface mobility concepts that address the mobility issue in a variety of ways. These concepts include the Rockwell Lunar Sortie Vehicle (1971), Cintala’s Lunar Traverse caravan, 1984, First Lunar Outpost (1992), Frassanito’s Lunar Rover Base (1993), Thangavelu’s Nomad Explorer (1993), Kozlov and Shevchenko’s Mobile Lunar Base (1995), and the most recent evolution, John Mankins’ “Habot” (2000-present). The review compares the several mobile base approaches, then focuses on the Habot approach as the most germane to current and future exploration plans.
    [Show full text]