ARES Biennial Report 2012 FinalSince the return of the first lunar samples, what is now the Astromaterials Research and Exploration Science (ARES) Directorate has had curatorial responsibility for all NASA-held extraterrestrial materials. Originating during the Apollo Program (1960s), this capability at Johnson Space Center (JSC) included scientists who were responsible for the science planning and training of astronauts for lunar surface activities as well as experts in the analysis and preservation of the precious returned samples. Today, ARES conducts research in basic and applied space and planetary science, and its scientific staff represents a broad diversity of expertise in the physical sciences (physics, chemistry, geology, astronomy), mathematics, and engineering organized into three offices (figure 1): Astromaterials Research (KR), Astromaterials Acquisition and Curation (KT), and Human Exploration Science (KX). Scientists within the Astromaterials Acquisition and Curation Office preserve, protect, document, and distribute samples of the current astromaterials collections. Since the return of the first lunar samples, ARES has been assigned curatorial responsibility for all NASA-held extraterrestrial materials (Apollo lunar samples, Antarctic meteorites - some of which have been confirmed to have originated on the Moon and on Mars - cosmic dust, solar wind samples, comet and interstellar dust particles, and space-exposed hardware). The responsibilities of curation consist not only of the longterm care of the samples, but also the support and planning for future sample collection missions and research and technology to enable new sample types. Curation provides the foundation for research into the samples. The Lunar Sample Facility and other curation clean rooms, the data center, laboratories, and associated instrumentation are unique NASA resources that, together with our staff's fundamental understanding of the entire collection, provide a service to the external research community, which relies on access to the samples. The curation efforts are greatly enhanced by a strong group of planetary scientists who conduct peerreviewed astromaterials research. Astromaterials Research Office scientists conduct peer-reviewed research as Principal or Co-Investigators in planetary science (e. g., cosmochemistry, origins of solar systems, Mars fundamental research, planetary geology and geophysics) and participate as Co-Investigators or Participating Scientists in many of NASA's robotic planetary missions. Since the last report, ARES has achieved several noteworthy milestones, some of which are documented in detail in the sections that follow. Within the Human Exploration Science Office, ARES is a world leader in orbital debris research, modeling and monitoring the debris environment, designing debris shielding, and developing policy to control and mitigate the orbital debris population. ARES has aggressively pursued refinements in knowledge of the debris environment and the hazard it presents to spacecraft. Additionally, the ARES Image Science and Analysis Group has been recognized as world class as a result of the high quality of near-real-time analysis of ascent and on-orbit inspection imagery to identify debris shedding, anomalies, and associated potential damage during Space Shuttle missions. ARES Earth scientists manage and continuously update the database of astronaut photography that is predominantly from Shuttle and ISS missions, but also includes the results of 40 years of human spaceflight. The Crew Earth Observations Web site (http://eol.jsc.nasa.gov/Education/ESS/crew.htm) continues to receive several million hits per month. ARES scientists are also influencing decisions in the development of the next generation of human and robotic spacecraft and missions through laboratory tests on the optical qualities of materials for windows, micrometeoroid/orbital debris shielding technology, and analog activities to assess surface science operations. ARES serves as host to numerous students and visiting scientists as part of the services provided to the research community and conducts a robust education and outreach program. ARES scientists are recognized nationally and internationally by virtue of their success in publishing in peer-reviewed journals and winning competitive research proposals. ARES scientists have won every major award presented by the Meteoritical Society, including the Leonard Medal, the most prestigious award in planetary science and cosmochemistry; the Barringer Medal, recognizing outstanding work in the field of impact cratering; the Nier Prize for outstanding research by a young scientist; and several recipients of the Nininger Meteorite Award. One of our scientists received the Department of Defense (DoD) Joint Meritorious Civilian Service Award (the highest civilian honor given by the DoD). ARES has established numerous partnerships with other NASA Centers, universities, and national laboratories. ARES scientists serve as journal editors, members of advisory panels and review committees, and society officers, and several scientists have been elected as Fellows in their professional societies. This biennial report summarizes a subset of the accomplishments made by each of the ARES offices and highlights participation in ongoing human and robotic missions, development of new missions, and planning for future human and robotic exploration of the solar system beyond low Earth orbit.
Document ID
20140011750
Acquisition Source
Johnson Space Center
Document Type
Other
Authors
Stansbery, Eileen (NASA Johnson Space Center Houston, TX, United States)
IDRelationTitle20150003834WorkAnalyzing an Aging ISS20150003814WorkSolving Problems Caused by Small Micrometeoroid and Orbital Debris Impacts for Space-Walking Astronauts20150003805WorkSmall-Scale Impact Processes on Stony Asteroids20150003799WorkWater in the Oldest Lunar Rocks: Moon is "Wetter" than Previously Thought20150003817WorkOrbital Debris Mitigation Requirements and the GRAIL Spacecraft20150003827WorkCEO Sites Mission Management System (SMMS)20150003796WorkMars Habitability, Biosignature Preservation, and Mission Support20150003811WorkHuman Exploration Science Office (KX) Overview20150003825WorkThe 2012 Moon and Mars Analog Mission20150003808WorkGeoLab: A Geological Workstation for Future Missions20150003794WorkNew Martian Meteorite Is One of the Most Oxidized Found to Date20150003828WorkSTK Integrated Message Production List Editor (SIMPLE) for CEO Operations20150003800WorkMagnetic Nozzle Effects on Plasma Plumes20150003832WorkClearance Analysis of Node 3 Aft CBM to the Stowed FGB Solar Array20150003822WorkCoring the Wide-Field Planetary Camera 2 Radiator for Impactor Trace Residue Assessment20150003826WorkSeeing Earth Through the Eyes of an Astronaut20150003824WorkNASA Extreme Environment Mission Operations: Science Operations Development for Human Exploration20150003833WorkClearance Analysis of CTC2 (on ELC4) to S-TRRJ HRS Radiator Rotation Envelope20150003815WorkToughened Thermal Blankets for Micrometeoroid and Orbital Debris Protection20150003835WorkARES Education and Public Outreach20150003803WorkProbing Asteroid (4) Vesta, Part 1: Dawn Mission Science20150003816WorkShell-NASA Vibration-Based Damage Characterization20150003819WorkEffectiveness of Satellite Postmission Disposal to Limit Orbital Debris Population Growth in Low Earth Orbit20150003795WorkShock Effects on Cometary-Dust Simulants20150003792WorkAstromaterials Research Office (KR) Overview20150003812WorkImagery Integration Team20150003829WorkRewriting the Landform History of One of Africa's Three Largest Basins20150003830WorkMegafans and Trumpeter Bird Biodiversity-Psophia Phylogeography and Landscape Evolution in Amazonia20150003823WorkMulti-Purpose Crew Vehicle Camera Asset Planning: Imagery Previsualization20150003801WorkMagnetohydrodynamic Turbulence and the Geodynamo20150003793WorkImproved Measurement of Ejection Velocities From Craters Formed in Sand20150003831WorkThe International Space Station: A Unique Platform for Remote Sensing of Natural Disasters20150003813WorkAdvancements in Capsule Parachute Analysis20150003806WorkAstromaterials Acquisition and Curation Office (KT) Overview20150003820WorkAn Analysis of the FY-1C, Iridium 33, and Cosmos 2251 Fragments20150003809WorkDividing the Concentrator Target From the Genesis Mission20150003818WorkOrigin of the Inter-Agency Space Debris Coordination Committee20150003797WorkEarly Life on Earth and the Search for Extraterrestrial Biosignatures20150003810WorkThe Apollo Lunar Sample Image Collection: Digital Archiving and Online Access20150003807WorkCollecting Comet Samples by ER-2 Aircraft: Cosmic Dust Collection During the Draconid Meteor Shower in October 201220150003798WorkWater Content of Earth's Continental Mantle Is Controlled by the Circulation of Fluids or Melts20150003804WorkProbing Asteroid (4) Vesta, Part 2: Meteorites From Vesta20150003802WorkConstraining Early Planetary Differentiation: The Link Between Chondrites and Achondrites Revealed From the Study of Aubrite Meteorites20150003821WorkDetection of Optically Faint GEO Debris