The Case for Renewed Human Exploration of the Moon
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Russia's Posture in Space
Russia’s Posture in Space: Prospects for Europe Executive Summary Prepared by the European Space Policy Institute Marco ALIBERTI Ksenia LISITSYNA May 2018 Table of Contents Background and Research Objectives ........................................................................................ 1 Domestic Developments in Russia’s Space Programme ............................................................ 2 Russia’s International Space Posture ......................................................................................... 4 Prospects for Europe .................................................................................................................. 5 Background and Research Objectives For the 50th anniversary of the launch of Sputnik-1, in 2007, the rebirth of Russian space activities appeared well on its way. After the decade-long crisis of the 1990s, the country’s political leadership guided by President Putin gave new impetus to the development of national space activities and put the sector back among the top priorities of Moscow’s domestic and foreign policy agenda. Supported by the progressive recovery of Russia’s economy, renewed political stability, and an improving external environment, Russia re-asserted strong ambitions and the resolve to regain its original position on the international scene. Towards this, several major space programmes were adopted, including the Federal Space Programme 2006-2015, the Federal Target Programme on the development of Russian cosmodromes, and the Federal Target Programme on the redeployment of GLONASS. This renewed commitment to the development of space activities was duly reflected in a sharp increase in the country’s launch rate and space budget throughout the decade. Thanks to the funds made available by flourishing energy exports, Russia’s space expenditure continued to grow even in the midst of the global financial crisis. Besides new programmes and increased funding, the spectrum of activities was also widened to encompass a new focus on space applications and commercial products. -
REASONS to MIND ASTEROIDS with the Rapid Progress Made In
ASTEROID MINING & ITS LEGAL IMPLICATIONS Neil Modi & Devanshu Ganatra Presentation ID- IAC- 16.E7.IP.23.x32357 REASONS TO MINE ASTEROIDS With the rapid progress made in technology, humans are taking huge steps in space today. There is huge potential in space, and particularly in asteroid mining. ENERGY CRISIS RARE EARTH METALS • Non-renewable fossil fuels like coal, oil currently account for 81% of • Many of the metals widely used in almost all industrial products the world’s primary energy. were always limited and are now in SHORT SUPPLY leading to skyrocketing manufacturing costs. • EARLIER, renewable energy could not compete with non-renewable sources because it relied on metals in short supply. Resources found • These include Platinum Group Metals (PMGS) and others like on asteroids would solve this problem completely. gold, cobalt, iron, molybdenum etc. Image Credit-The U.S. Energy Image Credit- FuelSpace.org- ‘How Asteroids Can Information Administration Save Mankind’ PROJECTED SCARCITY OF RESOURCES ON EARTH Image Credit-Shackleton Energy Company Image Credit- Chris Clugston’s ‘An Oil Drum- An Analysis’ (2010) THE NEED FOR WATER 1. SUPPORT SYSTEM FOR ASTRONAUTS- Since the main constituents of water HYDRATION AND OXYGEN are hydrogen and oxygen, it is a source of oxygen for life support. TO ASTRONAUTS 2. PROTECTION FROM RADIATION- Water absorbs and blocks infrared radiation, which means that by storing heat it helps to maintain temperature. 3. ROCKET FUEL- Rocket propellant is hydrogen and oxygen based, with a large percentage of the weight of a spacecraft taken up by fuel. 4. SPACE EXPLORATION- A GAS STATION IN SPACE KEY TO SPACE BLOCKS EXPLORATION WATER RADIATION Today billions of dollars are spent in rocket fuel to sustain space explorations. -
The Cassini Robot
THE CASSINI–HUYGENS MISSION LESSON The Cassini Robot 5 Students begin by examining their prior 3–4 hrs notions of robots and then consider the characteristics and capabilities of a robot like the Cassini–Huygens spacecraft that would be sent into space to explore another planet. Students compare robotic functions to human body functions. The lesson MEETS NATIONAL SCIENCE EDUCATION prepares students to design, build, diagram, STANDARDS: and explain their own models of robots for Unifying Concepts and Processes space exploration in the Saturn system. A computer-generated rendering of Cassini–Huygens. • Form and function PREREQUISITE SKILLS BACKGROUND INFORMATION Science and Drawing and labeling diagrams Background for Lesson Discussion, page 122 Technology • Abilities of Assembling a spacecraft model Questions, page 127 technological Some familiarity with the Saturn Answers in Appendix 1, page 225 design system (see Lesson 1) 56–63: The Cassini–Huygens Mission 64–69: The Spacecraft 70–76: The Science Instruments 81–94: Launch and Navigation 95–101: Communications and Science Data EQUIPMENT, MATERIALS, AND TOOLS For the teacher Materials to reproduce Photocopier (for transparencies & copies) Figures 1–6 are provided at the end of Overhead projector this lesson. Chart paper (18" × 22") FIGURE TRANSPARENCY COPIES Markers; clear adhesive tape 1 1 per group 21 For each group of 3 to 4 students 3 1 1 per student Chart paper (18" × 22") 4 1 per group Markers 51 Scissors 6 (for teacher only) Clear adhesive tape or glue Various household objects: egg cartons, yogurt cartons, film canisters, wire, aluminum foil, construction paper 121 Saturn Educator Guide • Cassini Program website — http://www.jpl.nasa.gov/cassini/educatorguide • EG-1998-12-008-JPL Background for Lesson Discussion LESSON craft components and those of human body 5 The definition of a robot parts. -
NASA's Lunar Atmosphere and Dust Environment Explorer (LADEE)
Geophysical Research Abstracts Vol. 13, EGU2011-5107-2, 2011 EGU General Assembly 2011 © Author(s) 2011 NASA’s Lunar Atmosphere and Dust Environment Explorer (LADEE) Richard Elphic (1), Gregory Delory (1,2), Anthony Colaprete (1), Mihaly Horanyi (3), Paul Mahaffy (4), Butler Hine (1), Steven McClard (5), Joan Salute (6), Edwin Grayzeck (6), and Don Boroson (7) (1) NASA Ames Research Center, Moffett Field, CA USA ([email protected]), (2) Space Sciences Laboratory, University of California, Berkeley, CA USA, (3) Laboratory for Atmospheric and Space Physics, University of Colorado, Boulder, CO USA, (4) NASA Goddard Space Flight Center, Greenbelt, MD USA, (5) LunarQuest Program Office, NASA Marshall Space Flight Center, Huntsville, AL USA, (6) Planetary Science Division, Science Mission Directorate, NASA, Washington, DC USA, (7) Lincoln Laboratory, Massachusetts Institute of Technology, Lexington MA USA Nearly 40 years have passed since the last Apollo missions investigated the mysteries of the lunar atmosphere and the question of levitated lunar dust. The most important questions remain: what is the composition, structure and variability of the tenuous lunar exosphere? What are its origins, transport mechanisms, and loss processes? Is lofted lunar dust the cause of the horizon glow observed by the Surveyor missions and Apollo astronauts? How does such levitated dust arise and move, what is its density, and what is its ultimate fate? The US National Academy of Sciences/National Research Council decadal surveys and the recent “Scientific Context for Exploration of the Moon” (SCEM) reports have identified studies of the pristine state of the lunar atmosphere and dust environment as among the leading priorities for future lunar science missions. -
Exploration of the Moon
Exploration of the Moon The physical exploration of the Moon began when Luna 2, a space probe launched by the Soviet Union, made an impact on the surface of the Moon on September 14, 1959. Prior to that the only available means of exploration had been observation from Earth. The invention of the optical telescope brought about the first leap in the quality of lunar observations. Galileo Galilei is generally credited as the first person to use a telescope for astronomical purposes; having made his own telescope in 1609, the mountains and craters on the lunar surface were among his first observations using it. NASA's Apollo program was the first, and to date only, mission to successfully land humans on the Moon, which it did six times. The first landing took place in 1969, when astronauts placed scientific instruments and returnedlunar samples to Earth. Apollo 12 Lunar Module Intrepid prepares to descend towards the surface of the Moon. NASA photo. Contents Early history Space race Recent exploration Plans Past and future lunar missions See also References External links Early history The ancient Greek philosopher Anaxagoras (d. 428 BC) reasoned that the Sun and Moon were both giant spherical rocks, and that the latter reflected the light of the former. His non-religious view of the heavens was one cause for his imprisonment and eventual exile.[1] In his little book On the Face in the Moon's Orb, Plutarch suggested that the Moon had deep recesses in which the light of the Sun did not reach and that the spots are nothing but the shadows of rivers or deep chasms. -
SPHERES Interact - Human-Machine Interaction Aboard the International Space Station
SPHERES Interact - Human-Machine Interaction aboard the International Space Station Enrico Stoll Steffen Jaekel Jacob Katz Alvar Saenz-Otero Space Systems Laboratory Massachusetts Institute of Technology 77 Massachusetts Avenue, Cambridge Massachusetts, 02139-4307, USA [email protected] [email protected] [email protected] [email protected] Renuganth Varatharajoo Department of Aerospace Engineering University Putra Malaysia 43400 Selangor, Malaysia [email protected] Abstract The deployment of space robots for servicing and maintenance operations, which are tele- operated from ground, is a valuable addition to existing autonomous systems since it will provide flexibility and robustness in mission operations. In this connection, not only robotic manipulators are of great use but also free-flying inspector satellites supporting the oper- ations through additional feedback to the ground operator. The manual control of such an inspector satellite at a remote location is challenging since the navigation in three- dimensional space is unfamiliar and large time delays can occur in the communication chan- nel. This paper shows a series of robotic experiments, in which satellites are controlled by astronauts aboard the International Space Station (ISS). The Synchronized Position Hold Engage Reorient Experimental Satellites (SPHERES) were utilized to study several aspects of a remotely controlled inspector satellite. The focus in this case study is to investigate different approaches to human-spacecraft interaction with varying levels of autonomy under zero-gravity conditions. 1 Introduction Human-machine interaction is a wide spread research topic on Earth since there are many terrestrial applica- tions, such as industrial assembly or rescue robots. Analogously, there are a number of possible applications in space such as maintenance, inspection and assembly amongst others. -
Global Exploration Roadmap
The Global Exploration Roadmap January 2018 What is New in The Global Exploration Roadmap? This new edition of the Global Exploration robotic space exploration. Refinements in important role in sustainable human space Roadmap reaffirms the interest of 14 space this edition include: exploration. Initially, it supports human and agencies to expand human presence into the robotic lunar exploration in a manner which Solar System, with the surface of Mars as • A summary of the benefits stemming from creates opportunities for multiple sectors to a common driving goal. It reflects a coordi- space exploration. Numerous benefits will advance key goals. nated international effort to prepare for space come from this exciting endeavour. It is • The recognition of the growing private exploration missions beginning with the Inter- important that mission objectives reflect this sector interest in space exploration. national Space Station (ISS) and continuing priority when planning exploration missions. Interest from the private sector is already to the lunar vicinity, the lunar surface, then • The important role of science and knowl- transforming the future of low Earth orbit, on to Mars. The expanded group of agencies edge gain. Open interaction with the creating new opportunities as space agen- demonstrates the growing interest in space international science community helped cies look to expand human presence into exploration and the importance of coopera- identify specific scientific opportunities the Solar System. Growing capability and tion to realise individual and common goals created by the presence of humans and interest from the private sector indicate and objectives. their infrastructure as they explore the Solar a future for collaboration not only among System. -
Exploration Timeline A
HOW DID OUR MOON FORM? MEET A LUNAR GEOLOGIST — Dr. Jeff Taylor, University of Hawaii What do you do? —— How did you get interested in this field? What is the most interesting question about the Moon that scientists are trying to solve? Do you want to go to the Moon? If someone wants to become a scientist, what should they do? EVOLUTION OF OUR MOON TRY THIS — What’s Needed Early Stages: A Magma Ocean — Make an Impact! Students model impact events and develop an understanding of the processes that cause cratering on the lunar surface. Getting Started Big Impacts, Big Basins — What features do they observe? Do they see the large round areas that have smooth dark interiors? Do they see smaller circular features? How might these have formed? What to Do Basin Filling — What do they observe? Can they identify different features of the crater? How do craters help geologists “see into” the inside of a planet? How did impactors traveling at different “velocities” influence the crater size or distribution of ejecta? Do the crater sizes or depths change? Wrapping Up Recent History — Can they identify impact basins, craters, and rays? EXPLORATIONXPLORATION TIMELINEIMELINE HINA MOVES TO THE MOON: Humans have been asking questions about our Moon since we first looked up at it in the sky. A HAWAIIAN STORY ABOUT OUR MOON WhatWhat isis oourur MMoonoon mmadeade oof?f? WWhathat aarere tthehe llightight aandnd ddarkark mmarkings?arkings? DDoesoes tthehe MMoonoon hhaveave ooceansceans aandnd aann aatmosphere?tmosphere? As telescopes became ever more powerful, the Moon’s rugged surface was revealed in increasing detail, but observations from Earth could not answer many scientific questions. -
Next-Generation Laser Retroreflectors for the Science and Exploration of the Moon, Mars and Beyond
3rd International Workshop on Instrumentation for Planetary Missions (2016) 4074.pdf Next-Generation Laser Retroreflectors for the Science and Exploration of the Moon, Mars and Beyond. S. Dell’Agnello1 for the SCF_Lab Team, D. Currie2, R. Richards3, J. Chandler4 1Istituto Nazionale di Fisica Nucleare – Laboratori Nazionali di Frascati (INFN-LNF), via E. Fermi, Frascati (Rome), Italy, email [email protected] 2University of Maryland (UMD) at College Park, MD, USA 3Moon Express Inc (MEI), 19-2060 N Akron Rd, Moffett Field, CA 94035 4Harvard-Smithsonian Center for Astrophysics (CfA), MA, USA Introduction. We developed next-generation laser retroreflectors for solar system science and exploration in the framework of the Affiliation membership of INFN to NASA/SSERVI (Solar System Exploration Virtual Institute), INFN National Science Committees n. 5 (devoted to R&D) and n. 2 (devoted to science) [1] and in collaboration with ASI, the Italian Space Agen- cy. Applications cover landing and roving missions to the Moon, Mars (ExoMars 2016 lander, ExoMars 2020 Figure 1: MoonLIGHT (4”), Apollo (1.5”) reflectors Rover and Mars 2020 Rover) to future or proposed missions to Phobos/Deimos (sample return), icy/rocky INFN, UMD and MEI signed a private-public partner- moons of Jupiter/Saturn and asteroids/comets (ESA’s ship, multi-mission agreement to deploy MoonLIGHT AIM). These retroreflectors have been or will be fully on the Moon (1st mission: end 2017/early 2018). The characterized at the SCF_Lab (Satellite/lunar/gnss la- results of an optical performace characterization of ser ranging/altimetry Cube/microsat Characterization MoonLIGHT carried out at the SCF_Lab is in Fig. -
Celebrate Apollo
National Aeronautics and Space Administration Celebrate Apollo Exploring The Moon, Discovering Earth “…We go into space because whatever mankind must undertake, free men must fully share. … I believe that this nation should commit itself to achieving the goal before this decade is out, of landing a man on the moon and returning him safely to Earth. No single space project in this period will be more exciting, or more impressive to mankind, or more important for the long-range exploration of space; and none will be so difficult or expensive to accomplish …” President John F. Kennedy May 25, 1961 Celebrate Apollo Exploring The Moon, Discovering Earth Less than five months into his new administration, on May 25, 1961, President John F. Kennedy, announced the dramatic and ambitious goal of sending an American safely to the moon before the end of the decade. Coming just three weeks after Mercury astronaut Alan Shepard became the first American in space, Kennedy’s bold challenge that historic spring day set the nation on a journey unparalleled in human history. Just eight years later, on July 20, 1969, Apollo 11 commander Neil Armstrong stepped out of the lunar module, taking “one small step” in the Sea of Tranquility, thus achieving “one giant leap for mankind,” and demonstrating to the world that the collective will of the nation was strong enough to overcome any obstacle. It was an achievement that would be repeated five other times between 1969 and 1972. By the time the Apollo 17 mission ended, 12 astronauts had explored the surface of the moon, and the collective contributions of hundreds of thousands of engineers, scientists, astronauts and employees of NASA served to inspire our nation and the world. -
Space Technology Mission Directorate
Space Technology Mission Directorate Innovation and Opportunity Conference 2018 Therese Griebel, Deputy Associate Administrator for STMD Programs | 11.07.18 TECHNOLOGY DRIVES EXPLORATION sparking enabling exploration investing in innovation and discovery America embracing competition engaging the and public-private NASA Pre-decisional – Internal Use Only – Do brightest minds partnerships 2 Not Distribute Partnerships & Technology Transfer SBIR/STTR • Technology Transfer • Prizes and Challenges Early Stage Innovation • iTech • NASA Innovative Advanced Concepts • Space Tech Research Grants Technology Demonstrations • Center Innovation Fund/Early Mid TRL • Technology Demonstration Career Initiative Missions • Small Spacecraft High TRL Technology Technology Maturation • Flight Opportunities • Game Changing Low TRL Development 3 FY 2018 Key Accomplishments Station Explorer for X-ray Timing and Navigation Technology (SEXTANT) Aboard ISS demonstrated fully autonomous X-ray navigation in space — a capability that could revolutionize NASA’s ability in the Small Spacecraft future to pilot robotic spacecraft to Two small spacecraft (Integrated the far reaches of the solar Solar Array and Reflect Antenna and system and beyond. Optical Communication and Sensor Demonstration) missions were successfully launched aboard Orbital ATK’s Cygnus spacecraft. Kilopower Testing successfully completed on 1 kW ground demonstration system- could be used for an Solar Electric affordable fission nuclear power In Space Robotics Propulsion system to enable long-duration -
Autonomous Robotic Systems for Mars Exploration Dr. Andrew E
Autonomous Robotic Systems for Mars Exploration Dr. Andrew E. Johnson Jet Propulsion Laboratory California Institute of Technology Robotic spacecraft that land on and rove over the surface of Mars must be designed to overcome many challenges due to the hostile and uncertain environment. Winds and dust buffet landers as they descend rapidly to the surface. Rocks, scarps, dunes and slopes must be avoided during landing and rover traverse. Temperature extremes, radiation, shock and vibration stress mechanical designs and computing must recover gracefully from hardware and software failures. The round-trip light time precludes direct tele-operation so all vehicle motion is executed autonomously on-board given high level commands from earth. Autonomous robotic systems are increasingly used to mitigate these challenges while also extending the capabilities of the spacecraft. The objective of robotic Mars missions is to advance scientific discovery. Science return is greater when there is geological diversity and stratigraphy near the landing site, but these create terrain that is risky for landing. To mitigate these risks autonomous robotic systems are being developed for safe landing in these hazardous terrains. Algorithms have been developed that estimate the pose of the lander relative to known landmarks and automatically detect and avoid landing hazards. These algorithms are being combined with sensors and high performance computing to create bolt-on systems for safe and pin-point landing. Landing is fully autonomous and failure is not recoverable, so these systems are designed to be self- checking and as simple as possible while also dealing with environmental factors like illumination variations, dust and terrain relief.