Swri IR&D Program 2016
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Annotated List of Works Cited Primary Sources Newspapers “Apollo 11 se Vraci na Zemi.” Rude Pravo [Czechoslovakia] 22 July 1969. 1. Print. This was helpful for us because it showed how the U.S. wasn’t the only ones effected by this event. This added more to our project so we had views from outside the US. Barbuor, John. “Alunizaron, Bajaron, Caminaron, Trabajaron: Proeza Lograda.” Excelsior [Mexico] 21 July 1969. 1. Print. The front page of this newspaper was extremely helpful to our project because we used it to see how this event impacted the whole world not just America. Beloff, Nora. “The Space Race: Experts Not Keen on Getting a Man on the Moon.” Age [Melbourne] 24 April 1962. 2. Print. This was an incredibly important article to use in out presentation so that we could see different opinions. This article talked about how some people did not want to go to the moon; we didn’t find many articles like this one. In most everything we have read it talks about the advantages of going to the moon. This is why this article was so unique and important. Canadian Press. “Half-billion Watch the Moon Spectacular.” Gazette [Montreal] 21 July 1969. 4. Print. This source gave us a clear idea about how big this event really was, not only was it a big deal in America, but everywhere else in the world. This article told how Russia and China didn’t have TV’s so they had to find other ways to hear about this event like listening to the radio. -
PEANUTS and SPACE FOUNDATION Apollo and Beyond
Reproducible Master PEANUTS and SPACE FOUNDATION Apollo and Beyond GRADE 4 – 5 OBJECTIVES PAGE 1 Students will: ö Read Snoopy, First Beagle on the Moon! and Shoot for the Moon, Snoopy! ö Learn facts about the Apollo Moon missions. ö Use this information to complete a fill-in-the-blank fact worksheet. ö Create mission objectives for a brand new mission to the moon. SUGGESTED GRADE LEVELS 4 – 5 SUBJECT AREAS Space Science, History TIMELINE 30 – 45 minutes NEXT GENERATION SCIENCE STANDARDS ö 5-ESS1 ESS1.B Earth and the Solar System ö 3-5-ETS1 ETS1.B Developing Possible Solutions 21st CENTURY ESSENTIAL SKILLS Collaboration and Teamwork, Communication, Information Literacy, Flexibility, Leadership, Initiative, Organizing Concepts, Obtaining/Evaluating/Communicating Ideas BACKGROUND ö According to NASA.gov, NASA has proudly shared an association with Charles M. Schulz and his American icon Snoopy since Apollo missions began in the 1960s. Schulz created comic strips depicting Snoopy on the Moon, capturing public excitement about America’s achievements in space. In May 1969, Apollo 10 astronauts traveled to the Moon for a final trial run before the lunar landings took place on later missions. Because that mission required the lunar module to skim within 50,000 feet of the Moon’s surface and “snoop around” to determine the landing site for Apollo 11, the crew named the lunar module Snoopy. The command module was named Charlie Brown, after Snoopy’s loyal owner. These books are a united effort between Peanuts Worldwide, NASA and Simon & Schuster to generate interest in space among today’s younger children. -
Design Your Mission Patch 1
Activities: 9. Design Your Mission Patch 1 Design Your Mission Patch Suggested Grade Level: 3–9 Summary 1. Students will work in teams to design a space mission patch. 2. In order to design the patch, the teams will use the Mission Patch Checklist to select a mission type, destination, mission goal(s), science objective(s), and mission name. Standards NM Science Content Standards: Strand III, Science and Society NM Arts Content Standards 2, 4, and 5 NM Career Readiness Standard 5 National Science Education Standards: Standard G, History and Nature of Science Background Information A space mission requires hundreds (sometimes thousands) of people working together in a variety of jobs. Construction workers, truck drivers, spacecraft designers, engineers, planetary geologists, chemists, physicists, and astronauts may all work together to create a successful mission. One of the things that holds this group together is a well-defined understanding of their mission goals and objectives and pride in their achievement. The mission patch is the graphic representation of their common goal. Each mission patch is unique and is frequently designed by the people involved in the mission to represent the important aspects of the mission. Suggested Materials Mission Patch Checklist accompanying this activity Color or black and white copies of a variety of mission patches (included) White drawing paper Pens, crayons, or markers Preparation 1. Print and photocopy the Mission Patch Checklist and Mission Patch Examples for each team of students. 2. For more information about NASA mission patches, log on to www.hq.nasa.gov/ office/pao/History/mission_patches.html or have students access this site prior to the activity. -
A Functional Approach to Finding Answer Sets
A Functional Approach to Finding Answer Sets Bryant Nelson, Josh Archer, and Nelson Rushton Texas Tech Dept. of Computer Science (bryant.nelson | josh.archer | nelson.rushton) @ ttu.edu Texas Tech University Department of Computer Science Box 43104 Lubbock, TX 79409-3104 we have been convinced of Hughes’ hypothesis. We set out to further test this Submitted to FCS 2013 hypothesis by encoding an Answer Set Solver in SequenceL. We hypothesize that Keywords: Functional Programming, a functional language would allow the Answer Set Prolog, Logic Programming programmer to implement an Answer Set Solver more quickly than a procedural Abstract: A naive answer set solver was language, and that the resulting program implemented in the functional programming would be more readable and language SequenceL, and its performance understandable. compared to mainstream solvers on a set of standard benchmark problems. Finding answer sets is an NP-Complete Implementation was very rapid (25 person problem, and over the last few decades a hours) and the resulting program only 400 few solvers have been developed that lines of code. Nonetheless, the algorithm tackle this problem. The current juggernauts was tractable and obtained parallel in this area are the DLV, CLASP, and speedups. Performance, though not SMODELS solvers, all of which are very pathologically poor, was considerably efficient. The problem would seem to benefit slower (around 20x) than that of mainstream from a parallelized solver, yet CLASP only solvers (CLASP, Smodels, and DLV) on all has a branch (CLASPar) dedicated to this, but one benchmark problem. and DLV has been “experimenting” with parallelization in their grounder [DLVPar]. -
Variations of Solar Wind Parameters Over a Solar Cycle: Expectations for NASA’S Solar Terrestrial Relations Observatory (STEREO) Mission
Variations of Solar Wind Parameters over a Solar Cycle: Expectations for NASA’s Solar TErrestrial RElations Observatory (STEREO) Mission Catherine C. Walker Mount Holyoke College 2007 Department of Astronomy Advisors: Professor M. Darby Dyar Department of Astronomy Mount Holyoke College Antoinette B. Galvin Department of Physics STEREO/PLASTIC Principal Investigator Space Science Center Institute for the Study of Earth, Oceans, and Space University of New Hampshire Mark A. Popecki STEREO/PLASTIC Co-Investigator Space Science Center Institute for the Study of Earth, Oceans, and Space University of New Hampshire ii ACKNOWLEDGEMENTS To start off, I would like to thank Dr. George Hurtt of the Complex Systems Center at the University of New Hampshire’s Institute for the Study of Earth, Oceans, and Space for allowing me to have such a wonderful research opportunity through the UNH-NASA Research & Discover Program. It has become apparent to me that the experience and connections that I gained through this program have brought me closer to my goal than I thought I would be at this point in life! In that vein, I need to express my sincere gratitude to Dr. Antoinette Galvin and Dr. Mark Popecki, first of all for taking me as a Research & Discover intern. Second, I need to thank them for allowing me to continue my research with them throughout the year, allowing me to become part of the UNH- PLASTIC team, flying me down to see the launch of STEREO, and accompanying me to the American Geophysical Union Fall meeting in San Francisco where I was able to present my research. -
The Early Geological History of the Moon Inferred from Ancient Lunar Meteorite Miller Range 13317
Meteoritics & Planetary Science 54, Nr 7, 1401–1430 (2019) doi: 10.1111/maps.13295 The early geological history of the Moon inferred from ancient lunar meteorite Miller Range 13317 N. M. CURRAN 1,2,*, K. H. JOY1, J. F. SNAPE3, J. F. PERNET-FISHER1, J. D. GILMOUR 1, A. A. NEMCHIN4, M. J. WHITEHOUSE3, and R. BURGESS1 1School of Earth and Environmental Sciences, University of Manchester, Oxford Road, Manchester M13 9PL, UK 2NASA Goddard Space Flight Center, 8800 Greenbelt Road, Greenbelt, Maryland 20771, USA 3Department of Geosciences, Swedish Museum of Natural History, SE-104 05 Stockholm, Sweden 4Department of Applied Geology, Curtin University, Perth, Western Australia 6845, Australia *Corresponding author. E-mail: [email protected] (Received 17 October 2018; revision accepted 14 March 2019) Abstract–Miller Range (MIL) 13317 is a heterogeneous basalt-bearing lunar regolith breccia that provides insights into the early magmatic history of the Moon. MIL 13317 is formed from a mixture of material with clasts having an affinity to Apollo ferroan anorthosites and basaltic volcanic rocks. Noble gas data indicate that MIL 13317 was consolidated into a breccia between 2610 Æ 780 Ma and 1570 Æ 470 Ma where it experienced a complex near- surface irradiation history for ~835 Æ 84 Myr, at an average depth of ~30 cm. The fusion crust has an intermediate composition (Al2O3 15.9 wt%; FeO 12.3 wt%) with an added incompatible trace element (Th 5.4 ppm) chemical component. Taking the fusion crust to be indicative of the bulk sample composition, this implies that MIL 13317 originated from a regolith that is associated with a mare-highland boundary that is KREEP-rich (i.e., K, rare earth elements, and P). -
Constraining the Evolutionary History of the Moon and the Inner Solar System: a Case for New Returned Lunar Samples
Space Sci Rev (2019) 215:54 https://doi.org/10.1007/s11214-019-0622-x Constraining the Evolutionary History of the Moon and the Inner Solar System: A Case for New Returned Lunar Samples Romain Tartèse1 · Mahesh Anand2,3 · Jérôme Gattacceca4 · Katherine H. Joy1 · James I. Mortimer2 · John F. Pernet-Fisher1 · Sara Russell3 · Joshua F. Snape5 · Benjamin P. Weiss6 Received: 23 August 2019 / Accepted: 25 November 2019 / Published online: 2 December 2019 © The Author(s) 2019 Abstract The Moon is the only planetary body other than the Earth for which samples have been collected in situ by humans and robotic missions and returned to Earth. Scien- tific investigations of the first lunar samples returned by the Apollo 11 astronauts 50 years ago transformed the way we think most planetary bodies form and evolve. Identification of anorthositic clasts in Apollo 11 samples led to the formulation of the magma ocean concept, and by extension the idea that the Moon experienced large-scale melting and differentiation. This concept of magma oceans would soon be applied to other terrestrial planets and large asteroidal bodies. Dating of basaltic fragments returned from the Moon also showed that a relatively small planetary body could sustain volcanic activity for more than a billion years after its formation. Finally, studies of the lunar regolith showed that in addition to contain- ing a treasure trove of the Moon’s history, it also provided us with a rich archive of the past 4.5 billion years of evolution of the inner Solar System. Further investigations of samples returned from the Moon over the past five decades led to many additional discoveries, but also raised new and fundamental questions that are difficult to address with currently avail- able samples, such as those related to the age of the Moon, duration of lunar volcanism, the Role of Sample Return in Addressing Major Questions in Planetary Sciences Edited by Mahesh Anand, Sara Russell, Yangting Lin, Meenakshi Wadhwa, Kuljeet Kaur Marhas and Shogo Tachibana B R. -
Mission Task Checklist
MISSION TASK CHECKLIST Entryway Discovery (page 2) Astronaut Encounter (page 3) Astronaut Autograph (page 3) Where in the World? (page 4) Mission Patch (page 5) Wild Neighbors (page 6) NASA Speak (page 7) Journey To Mars: Explorers Wanted (page 7) The Orion spacecraft is the Science On A Sphere (page 8) crew vehicle NASA is Move the Galaxy (page 8) currently developing for future deep-space missions. Mapping Survey (page 9) Crew Conference (page 10) Shuttle Launch Experience (page 15) EXPEDITION Bus Tour (page16) Touch the Moon (page16) LOGBOOK Energy for the Future (page 11-12) From Sketchpad to Launchpad (page 13) Team Name: ______________________________ ISS Live! (page 14) Rocket Garden Rap (page 17) Commander (teacher): ______________________ Rocket Search (page 18) Pilot (chaperone): __________________________ Mission Specialist 1 (MS1): ________________________ For more cool information and activities, visit www.nasa.gov and click on the “For Students” tab! Mission Specialist 2 (MS2): ________________________ Mission Specialist 3 (MS3): ________________________ Mission Specialist 4 (MS4): ________________________ MISSION TASK: Rocket Search LOCATION: Rocket Garden Expedition 321 YOU ARE GO FOR LAUNCH The rockets on display here are real, space worthy rockets left over from the early days of space exploration. Unlike the space shuttle, they are all “expendable” rockets, which means they were designed to be used only once. Some of these were Welcome the Kennedy Space Center Visitor Complex, the only place surplus, while others were designed for missions that were later canceled. on Earth where human beings have left the planet, traveled to Find the following items in the Rocket Garden and in the Word Search puzzle. -
An Evolving Astrobiology Glossary
Bioastronomy 2007: Molecules, Microbes, and Extraterrestrial Life ASP Conference Series, Vol. 420, 2009 K. J. Meech, J. V. Keane, M. J. Mumma, J. L. Siefert, and D. J. Werthimer, eds. An Evolving Astrobiology Glossary K. J. Meech1 and W. W. Dolci2 1Institute for Astronomy, 2680 Woodlawn Drive, Honolulu, HI 96822 2NASA Astrobiology Institute, NASA Ames Research Center, MS 247-6, Moffett Field, CA 94035 Abstract. One of the resources that evolved from the Bioastronomy 2007 meeting was an online interdisciplinary glossary of terms that might not be uni- versally familiar to researchers in all sub-disciplines feeding into astrobiology. In order to facilitate comprehension of the presentations during the meeting, a database driven web tool for online glossary definitions was developed and participants were invited to contribute prior to the meeting. The glossary was downloaded and included in the conference registration materials for use at the meeting. The glossary web tool is has now been delivered to the NASA Astro- biology Institute so that it can continue to grow as an evolving resource for the astrobiology community. 1. Introduction Interdisciplinary research does not come about simply by facilitating occasions for scientists of various disciplines to come together at meetings, or work in close proximity. Interdisciplinarity is achieved when the total of the research expe- rience is greater than the sum of its parts, when new research insights evolve because of questions that are driven by new perspectives. Interdisciplinary re- search foci often attack broad, paradigm-changing questions that can only be answered with the combined approaches from a number of disciplines. -
Gsnca Patch Program out of This World
gsnca patch program Out of this World Requirements 1. Identify a former Girl Scout who went on to become a NASA astronaut. Name five facts about her. Visit spaceflightsystems.grc.nasa.gov/girlscouts/gsusa_astro.html. 2. Read astronaut Suni Williams’ answers to questions from Girl Scouts. Visit nasa.gov/ mission_pages/station/expeditions/expedition15/girl_scout_questions.html. 3. Visit the Women@NASA website and watch at least one of the videos to see how women at NASA are leading the way in STEM (science, technology, engineering and mathematics), and learn about the awe-inspiring projects they’re pursuing. Visit women.nasa.gov/. 4. Choose one mission from each of the following three space programs: Mercury, Gemi- ni and Apollo. Name the crew, vehicle used, purpose of the mission and one interesting fact about each mission. Objectives: 5. Choose a mission from the Space Shuttle program (STS). Name the crew, vehicle used, purpose of the mission and one interesting fact about that mission. This patch is designed to help girls learn more 6. Choose a mission from the International Space Station (ISS) program. Name the crew, about the history of manned space flight, how vehicle used to get them to and from the space station, purpose of the mission and humans adapt to living in space and women’s one interesting fact about that mission. roles in aerospace. 7. The International Space Station was not the first space station to orbit earth. Identify Grade Level Requirements: at least two other space stations that came before the ISS. Identify when they were in orbit, what country they belonged to and at least one interesting fact about each of To earn this patch, everyone must complete them. -
Lunar Cold Spots and Crater Production on the Moon 10.1029/2018JE005652 J.-P
Journal of Geophysical Research: Planets RESEARCH ARTICLE Lunar Cold Spots and Crater Production on the Moon 10.1029/2018JE005652 J.-P. Williams1 , J. L. Bandfield2 , D. A. Paige1, T. M. Powell1, B. T. Greenhagen3, S. Taylor1, 4 5 6 7,8 Key Points: P. O. Hayne , E. J. Speyerer , R. R. Ghent , and E. S. Costello • We measure diameters of craters 1 2 associated with cold spots. Their Earth, Planetary, and Space Sciences, University of California, Los Angeles, CA, USA, Space Science Institute, Boulder, CO, USA, size-frequency distribution indicates 3Applied Physics Laboratory, Johns Hopkins University, Laurel, MD, USA, 4Department of Astrophysical & Planetary Sciences, cold spots survive a few hundred kyr University of Colorado, Boulder, Boulder, CO, USA, 5School of Earth and Space Exploration, Arizona State University, Tempe, AZ, • fl The distribution of cold spots re ects USA, 6Earth Sciences, University of Toronto, Toronto, ON, Canada, 7Department of Geology and Geophysics, University of ’ the Moon s synchronous rotation ’ ā 8 with cold spots focused on the apex Hawai iatM noa, Honolulu, HI, USA, Hawaii Institute of Geophysics and Planetology, Honolulu, HI, USA of motion • The largest cold spots with source craters larger than 800 m are Abstract Mapping of lunar nighttime surface temperatures has revealed anomalously low nighttime concentrated on the trailing side of temperatures around recently formed impact craters on the Moon. The thermophysically distinct “cold the moon spots” provide a way of identifying the most recently formed impact craters. Over 2,000 cold spot source craters were measured with diameters ranging from 43 m to 2.3 km. -
JJ Gillis K. Righter Elphic RC
Lunar and Planetary Science XXXIII (2002) sess39.pdf Wednesday, March 13, 2002 LUNAR BASALTS: THE WIND CRIES MARE 8:30 a.m. Salon A Chairs: J. J. Gillis K. Righter Elphic R. C.* Lawrence D. J. Maurice S. Feldman W. C. Prettyman T. H. Gasnault O. M. Binder A. B. Lucey P. G. An Index for Evolved Lithologies on the Lunar Surface: Lunar Prospector Thorium-to-REE Ratio [#2009] Using Lunar Prospector neutron and gamma ray spectrometer data, we develop an “evolved lithology index” based on the ratio of thorium to rare earth element abundance. This is useful in identifying exotic compositions. Gasnault O.* Lawrence D. J. Vaniman D. T. Elphic R. C. Feldman W. C. Systematics on Thorium in Lunar Basalts [#2010] We study the thorium content in lunar mare basalts. A severe selection is made to make sure that the studied sub-dataset is representative of basaltic flows. The thorium distribution in those basalts presents strong patterns. Relation with iron, age, and topography are investigated. Vaniman D.* Lawrence D. Gasnault O. Reedy R. Extending the Th-FeO Sampling Range at Apollo 14: Under the Footprint of Lunar Prospector [#1404] Using measured FeO and using K as a Th surrogate, glasses in Apollo 14 regolith breccias provide a wider sampling than other Apollo 14 samples. The range of variation compares broadly with that found by Lunar Prospector for the whole Moon. Gillis J. J.* Jolliff B. L. Korotev R. L. Lawrence D. J. The Origin of Elevated Th in the Eratosthenian Lava Flows in the Procellarum KREEP Terrane [#1934] Clementine spectral reflectance and compositional data, Lunar Prospector gamma ray and neutron spectrometer data, and sample analysis of lunar soils are used to examine the origin of high-Th in Eratosthenian basalts of the Procellarum KREEP Terrane Lawrence D.