NASA's Apollo and Artemis Missions to the Moon
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Index Abulfeda crater chain (Moon), 97 Aphrodite Terra (Venus), 142, 143, 144, 145, 146 Acheron Fossae (Mars), 165 Apohele asteroids, 353–354 Achilles asteroids, 351 Apollinaris Patera (Mars), 168 achondrite meteorites, 360 Apollo asteroids, 346, 353, 354, 361, 371 Acidalia Planitia (Mars), 164 Apollo program, 86, 96, 97, 101, 102, 108–109, 110, 361 Adams, John Couch, 298 Apollo 8, 96 Adonis, 371 Apollo 11, 94, 110 Adrastea, 238, 241 Apollo 12, 96, 110 Aegaeon, 263 Apollo 14, 93, 110 Africa, 63, 73, 143 Apollo 15, 100, 103, 104, 110 Akatsuki spacecraft (see Venus Climate Orbiter) Apollo 16, 59, 96, 102, 103, 110 Akna Montes (Venus), 142 Apollo 17, 95, 99, 100, 102, 103, 110 Alabama, 62 Apollodorus crater (Mercury), 127 Alba Patera (Mars), 167 Apollo Lunar Surface Experiments Package (ALSEP), 110 Aldrin, Edwin (Buzz), 94 Apophis, 354, 355 Alexandria, 69 Appalachian mountains (Earth), 74, 270 Alfvén, Hannes, 35 Aqua, 56 Alfvén waves, 35–36, 43, 49 Arabia Terra (Mars), 177, 191, 200 Algeria, 358 arachnoids (see Venus) ALH 84001, 201, 204–205 Archimedes crater (Moon), 93, 106 Allan Hills, 109, 201 Arctic, 62, 67, 84, 186, 229 Allende meteorite, 359, 360 Arden Corona (Miranda), 291 Allen Telescope Array, 409 Arecibo Observatory, 114, 144, 341, 379, 380, 408, 409 Alpha Regio (Venus), 144, 148, 149 Ares Vallis (Mars), 179, 180, 199 Alphonsus crater (Moon), 99, 102 Argentina, 408 Alps (Moon), 93 Argyre Basin (Mars), 161, 162, 163, 166, 186 Amalthea, 236–237, 238, 239, 241 Ariadaeus Rille (Moon), 100, 102 Amazonis Planitia (Mars), 161 COPYRIGHTED -
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. -
A Comparative Analysis of the Geology Tools Used During the Apollo Lunar Program and Their Suitability for Future Missions to the Om on Lindsay Kathleen Anderson
University of North Dakota UND Scholarly Commons Theses and Dissertations Theses, Dissertations, and Senior Projects January 2016 A Comparative Analysis Of The Geology Tools Used During The Apollo Lunar Program And Their Suitability For Future Missions To The oM on Lindsay Kathleen Anderson Follow this and additional works at: https://commons.und.edu/theses Recommended Citation Anderson, Lindsay Kathleen, "A Comparative Analysis Of The Geology Tools Used During The Apollo Lunar Program And Their Suitability For Future Missions To The oonM " (2016). Theses and Dissertations. 1860. https://commons.und.edu/theses/1860 This Thesis is brought to you for free and open access by the Theses, Dissertations, and Senior Projects at UND Scholarly Commons. It has been accepted for inclusion in Theses and Dissertations by an authorized administrator of UND Scholarly Commons. For more information, please contact [email protected]. A COMPARATIVE ANALYSIS OF THE GEOLOGY TOOLS USED DURING THE APOLLO LUNAR PROGRAM AND THEIR SUITABILITY FOR FUTURE MISSIONS TO THE MOON by Lindsay Kathleen Anderson Bachelor of Science, University of North Dakota, 2009 A Thesis Submitted to the Graduate Faculty of the University of North Dakota in partial fulfillment of the requirements for the degree of Master of Science Grand Forks, North Dakota May 2016 Copyright 2016 Lindsay Anderson ii iii PERMISSION Title A Comparative Analysis of the Geology Tools Used During the Apollo Lunar Program and Their Suitability for Future Missions to the Moon Department Space Studies Degree Master of Science In presenting this thesis in partial fulfillment of the requirements for a graduate degree from the University of North Dakota, I agree that the library of this University shall make it freely available for inspection. -
Apollo 14 Press
NATIONAL AERONAUTICS AND SPACE ADMINISTRATION WO 2-4155 WASHINGT0N.D.C. 20546 lELS.wo 36925 RELEASE NO: 71-3K FOR RELEASE: THURSDAY A. M . January 21, 1971 P R E S S K I T -more - 1/11/71 2 -0- NATIONAL AERONAUTICS AND SPACE ADMINISTRATION (m2) 962-4155 N E w s WASHINGTON,D.C. 20546 mu: (202) 963-6925 FOR RELEASE: THURSDAY A..M. January 21:, 1971 RELEASE NO: 71-3 APOLLO 14 LAUNCH JAN. 31 Apollo 14, the sixth United States manned flight to the Moon and fourth Apollo mission with an objective of landing men on the Moon, is scheduled for launch Jan. 31 at 3:23 p.m. EST from Kennedy Space Center, Fla. The Apollo 14 lunar module is to land in the hilly upland region north of the Fra Mauro crater for a stay of about 33 hours, during whick, the landing crew will leave the spacecraft twice to set up scientific experiments on the lunar surface and to continue geological explorations. The two earlier Apollo lunar landings were Apollo 11 at Tranquillity Base and Apollo 12 at Surveyor 3 crater in the Ocean of Storms. Apollo 14 prime crewmen are Spacecraft Commander Alan B. Shepard, Jr., Command Module Pilot Stuart A. Roosa, and Lunar Module Pilot Edgar I). Mitchell. Shepard is a Navy car-sain Roosa an Air Force major and Mitchell a Navy commander. -more- 1/8/71 -2- Lunar materials brought- back from the Fra Mauro formation are expected to yield information on the early history of the Moon, the Earth and the solar system--perhaps as long ago as five billion years. -
Conceptual Human-System Interface Design for a Lunar Access Vehicle
Conceptual Human-System Interface Design for a Lunar Access Vehicle Mary Cummings Enlie Wang Cristin Smith Jessica Marquez Mark Duppen Stephane Essama Massachusetts Institute of Technology* Prepared For Draper Labs Award #: SC001-018 PI: Dava Newman HAL2005-04 September, 2005 http://halab.mit.edu e-mail: [email protected] *MIT Department of Aeronautics and Astronautics, Cambridge, MA 02139 TABLE OF CONTENTS 1 INTRODUCTION..................................................................................................... 1 1.1 THE GENERAL FRAMEWORK................................................................................ 1 1.2 ORGANIZATION.................................................................................................... 2 2 H-SI BACKGROUND AND MOTIVATION ........................................................ 3 2.1 APOLLO VS. LAV H-SI........................................................................................ 3 2.2 APOLLO VS. LUNAR ACCESS REQUIREMENTS ...................................................... 4 3 THE LAV CONCEPTUAL PROTOTYPE............................................................ 5 3.1 HS-I DESIGN ASSUMPTIONS ................................................................................ 5 3.2 THE CONCEPTUAL PROTOTYPE ............................................................................ 6 3.3 LANDING ZONE (LZ) DISPLAY............................................................................. 8 3.3.1 LZ Display Introduction................................................................................. -
Gao-21-330, Nasa Lunar Programs
Report to Congressional Committees May 2021 NASA LUNAR PROGRAMS Significant Work Remains, Underscoring Challenges to Achieving Moon Landing in 2024 GAO-21-330 May 2021 NASA LUNAR PROGRAMS Significant Work Remains, Underscoring Challenges to Achieving Moon Landing in 2024 Highlights of GAO-21-330, a report to congressional committees Why GAO Did This Study What GAO Found In March 2019, the White House The National Aeronautics and Space Administration (NASA) has initiated eight directed NASA to accelerate its plans lunar programs since 2017 to help NASA achieve its goal of returning humans to for a lunar landing by 4 years, to 2024. the Moon. NASA plans to conduct this mission, known as Artemis III, in 2024. Accomplishing this goal will require NASA has made progress by completing some early lunar program development extensive coordination across lunar activities including initial contract awards, but an ambitious schedule decreases programs and contractors to ensure the likelihood of NASA achieving its goal. For example, NASA’s planned pace to systems operate together seamlessly develop a Human Landing System, shown below, is months faster than other and safely. In December 2019, GAO spaceflight programs, and a lander is inherently more complex because it found that NASA had begun making supports human spaceflight. decisions related to requirements, cost, and schedule for individual lunar Notional Human Landing System programs but was behind in taking these steps for the Artemis III mission. The House Committee on Appropriations included a provision in 2018 for GAO to review NASA’s proposed lunar-focused programs. This is the second such report. -
Stereo Reconstruction from Apollo 15 and 16 Metric Camerazachary
42nd Lunar and Planetary Science Conference (2011) 2267.pdf Stereo Reconstruction from Apollo 15 and 16 Metric Camera Zachary Moratto1, Ara Nefian1,2, Taemin Kim1, Michael Broxton1,2, Ross Beyer1,3, and Terry Fong1, 1NASA Ames Research Center, MS 269-3, Moffett Field, CA, USA ([email protected]), 2Carnegie Mellon University, 3Carl Sagan Center SETI Introduction saic, DIM, and precision maps are produced for both This paper presents the production of digital terrain mod- missions separately. els (DTMs) and digital image mosaics (DIMs) of the Lu- The DTM mosaic is formed by a weighted average of nar surface that cover a large portion of the near-side of the stereo pair DTMs. Input DTMs were weighted max- the Moon at 40 m/px and 10 m/px respectively. These imum value at their centers and then feathered to zero at data products, produced under direction of the NASA the edges. The DTM mosaics are shown in Fig. 1 and 2. ESMD Lunar Mapping and Modeling Project (LMMP), The DIM was created by projecting the original res- are based on 2600 stereo image pairs from the Apollo olution images onto the 40 m/px DTMs, creating indi- 15 and 16 missions that were digitized at high resolution vidual orthoimages. Those orthoimages were then mo- from the original mission films [1]. Our reconstruction saicked by a process described in [5] without reflectance. was carried out using the highly automated Ames Stereo Therefore, only the final image mosaic and time expo- Pipeline software [2], which runs on NASA’s Pleiades sures were calculated. -
Apollo 13 Mission Review
APOLLO 13 MISSION REVIEW HEAR& BEFORE THE COMMITTEE ON AERONAUTICAL AND SPACE SCIENCES UNITED STATES SENATE NINETY-FIRST CONGRESS SECOR’D SESSION JUR’E 30, 1970 Printed for the use of the Committee on Aeronautical and Space Sciences U.S. GOVERNMENT PRINTING OFFICE 47476 0 WASHINGTON : 1970 COMMITTEE ON AEROKAUTICAL AND SPACE SCIENCES CLINTON P. ANDERSON, New Mexico, Chairman RICHARD B. RUSSELL, Georgia MARGARET CHASE SMITH, Maine WARREN G. MAGNUSON, Washington CARL T. CURTIS, Nebraska STUART SYMINGTON, bfissouri MARK 0. HATFIELD, Oregon JOHN STENNIS, Mississippi BARRY GOLDWATER, Arizona STEPHEN M.YOUNG, Ohio WILLIAM B. SAXBE, Ohio THOJfAS J. DODD, Connecticut RALPH T. SMITH, Illinois HOWARD W. CANNON, Nevada SPESSARD L. HOLLAND, Florida J4MES J. GEHRIG,Stad Director EVERARDH. SMITH, Jr., Professional staffMember Dr. GLENP. WILSOS,Professional #tad Member CRAIGVOORHEES, Professional Staff Nember WILLIAMPARKER, Professional Staff Member SAMBOUCHARD, Assistant Chief Clerk DONALDH. BRESNAS,Research Assistant (11) CONTENTS Tuesday, June 30, 1970 : Page Opening statement by the chairman, Senator Clinton P. Anderson-__- 1 Review Board Findings, Determinations and Recommendations-----_ 2 Testimony of- Dr. Thomas 0. Paine, Administrator of NASA, accompanied by Edgar M. Cortright, Director, Langley Research Center and Chairman of the dpollo 13 Review Board ; Dr. Charles D. Har- rington, Chairman, Aerospace Safety Advisory Panel ; Dr. Dale D. Myers, Associate Administrator for Manned Space Flight, and Dr. Rocco A. Petrone, hpollo Director -___________ 21, 30 Edgar 11. Cortright, Chairman, hpollo 13 Review Board-------- 21,27 Dr. Dale D. Mvers. Associate Administrator for Manned SDace 68 69 105 109 LIST OF ILLUSTRATIOSS 1. Internal coinponents of oxygen tank So. 2 ---_____-_________________ 22 2. -
Map the Six Apollo Moon Landing Sites
1 Based on: Earthrise – My Adventures as an Apollo 14 Astronaut By Edgar Mitchell, Chicago Review Press, 2014 Map the Apollo Moon Landing Sites Photo of the Moon from Apollo 11, Courtesy NASA There were six Apollo missions that landed astronauts on the Moon including: Apollo 11, Apollo 12, Apollo 14, Apollo 15, Apollo 16, and Apollo 17. Each Moon mission explored a different part of the Moon and had a specific landing site. Apollo 13 was heading to the Moon, but returned to Earth due to a spacecraft malfunction. For this activity, draw a picture of the Moon and indicate where each mission landed. Approximate age range: fifth to eighth grade Objective: To help young people learn about the Apollo missions. You’ll Need: * Computer with Internet access * Poster board (20 by 24 inches, 50.8 by 60.9 cm) * Pen or Pencil * Colored pencils * Markers 1. For overviews of Apollo missions 11, 12, 14, 15, 16, and 17, check out: Apollo 11: http://nssdc.gsfc.nasa.gov/planetary/lunar/apollo11info.html Apollo 12: http://nssdc.gsfc.nasa.gov/planetary/lunar/apollo12info.html Apollo 14: http://nssdc.gsfc.nasa.gov/planetary/lunar/apollo14info.html Apollo 15: http://nssdc.gsfc.nasa.gov/planetary/lunar/apollo15info.html © 2016 Ellen Mahoney 2 Apollo 16: http://nssdc.gsfc.nasa.gov/planetary/lunar/apollo16info.html Apollo 17: http://nssdc.gsfc.nasa.gov/planetary/lunar/apollo17info.html 2. For each Apollo mission, write down the name of the mission, the names of the astronauts and their titles, the launch date, when the lunar module landed on the Moon, the name of the Landing Site, and the date the astronauts returned to Earth. -
In Situ Propellant Production: Alternatives for Mars Exploration
https://ntrs.nasa.gov/search.jsp?R=19930008610 2020-03-17T09:20:19+00:00Z mira IN SITU PROPELLANT PRODUCTION: ALTERNATIVES FOR MARS EXPLORATION NASA CR 187192 Report No. SAIC-91/1052 Study No. SAIC 1-120-631-$28 by Michael L. Stancati Mark K. Jacobs Kevin J. Cole John T. Collins Science Applications International Corporation 1515 E. Woodfield Road Schaumburg, IL 60173 for Space Propulsion Technology Division NASA Lewis Research Center Cleveland, Ohio Contract NAS3-25809 "qB" October 1991 lWr_ IIm _ IW i m i!i W m m _ 1p m II mmm I z MI qw II - m_ mm_ h ii m_ i PREFACE This study was completed between May 1990 and April 1991 by members of the Advanced Planntng and Analysis Division of Science Applications International Corporation. The study was sponsored by the Space Propulsion Technology Division of NASA Lewis Research Center, and conducted as a task order under contract number NAS3-25809. SAIC acknowledges the contributions of several reviewers who offered valuable insight and commentary w on recovery of raw materials, in situ processing, and propellant utilization strategies. Dr. Robert L. Ash of Old Dominion University examined our characterization of propellant recovery and processing options, and suggested key areas for technology development and early testing of candidate processes. Mr. James R. French of JRF Engineering Services provided a systems-level critique of the assessment approach and alternative utilization strategies, and reviewed the results of performance trades. Dr. Kumar Ramohaili of the Center for Utilization of Lunar and Planetary Resources at the University of Arizona reviewed the infrastructure assessment approach that we proposed, and offered suggestions on presentation of this material. -
Waltham on the Moon, Apollo 15 and the Search for the Holy Grail
Waltham on the Moon, Apollo 15 and the Search for the Holy Grail. Post contains Pict... Page 1 of 3 [ View Thread ] [ Return to Index ] [ Read Prev Msg ] [ Read Next Msg ] 'Poor Man's' Watch Forum ARCHIVE Waltham on the Moon, Apollo 15 and the Search for the Holy Grail. Posted By: Kelly M. Rayburn <[email protected]> Date: Wednesday, 27 August 2003, at 2:21 a.m. (Reto was kind enough to ask me to repost my earlier post on the above topic for the archives on the new server. It contains nothing new except the post script. If you have already read the post, please disregard.) Hi all: In preparation for purchasing an Omega Speedmaster Professional, I have done the obligatory research on the use of the Speedmaster in the NASA space program. Chuck Maddox's excellent article on Omega's history with the Apollo program revealed some interesting facts that I did not know. In brief: The cal. 321 Speedmasters were purchased by NASA for the astronauts' use prior to the introduction of the cal. 861 movement in 1968. Apparently it is generally accepted that only the cal. 321 Speedmasters were worn on the moon during the various moon missions, as the initial procurement of these watches around 1965 was distributed to all astonauts at that time (two each) with as many as twenty still left in inventory and never used following the final Apollo 17 mission in 1972. Apparently, there is no evidence that a cal. 861 Speedmaster was worn by any of the moonwalkers or that NASA had procured any cal. -
The Moon After Apollo
ICARUS 25, 495-537 (1975) The Moon after Apollo PAROUK EL-BAZ National Air and Space Museum, Smithsonian Institution, Washington, D.G- 20560 Received September 17, 1974 The Apollo missions have gradually increased our knowledge of the Moon's chemistry, age, and mode of formation of its surface features and materials. Apollo 11 and 12 landings proved that mare materials are volcanic rocks that were derived from deep-seated basaltic melts about 3.7 and 3.2 billion years ago, respec- tively. Later missions provided additional information on lunar mare basalts as well as the older, anorthositic, highland rocks. Data on the chemical make-up of returned samples were extended to larger areas of the Moon by orbiting geo- chemical experiments. These have also mapped inhomogeneities in lunar surface chemistry, including radioactive anomalies on both the near and far sides. Lunar samples and photographs indicate that the moon is a well-preserved museum of ancient impact scars. The crust of the Moon, which was formed about 4.6 billion years ago, was subjected to intensive metamorphism by large impacts. Although bombardment continues to the present day, the rate and size of impact- ing bodies were much greater in the first 0.7 billion years of the Moon's history. The last of the large, circular, multiringed basins occurred about 3.9 billion years ago. These basins, many of which show positive gravity anomalies (mascons), were flooded by volcanic basalts during a period of at least 600 million years. In addition to filling the circular basins, more so on the near side than on the far side, the basalts also covered lowlands and circum-basin troughs.