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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. -
Nanosims Pb/Pb Dating of Tranquillityite in High-Ti Lunar Basalts
1 Revision 1 2 NanoSIMS Pb/Pb dating of tranquillityite in high-Ti lunar basalts: 3 Implications for the chronology of high-Ti volcanism on the Moon 4 5 Romain Tartèse1, Mahesh Anand1,2 and Thomas Delhaye3 6 7 1Planetary and Space Sciences, The Open University, Walton Hall, Milton Keynes, MK7 8 6AA, United Kingdom 9 2Department of Earth Sciences, The Natural History Museum, Cromwell Road, London, SW7 10 5BD, United Kingdom 11 3Plateforme ONIS/NanoSIMS, Université de Rennes 1, Campus de Beaulieu, 35042 Rennes 12 Cedex, France 13 14 15 16 17 18 19 20 21 22 23 24 25 26 Abstract 27 In this study, we carried out Pb/Pb dating of tranquillityite in high-Ti mare basalts 10044, 28 75055 and 74255, using a Cameca NanoSIMS 50 at a spatial resolution of ~ 3 µm. The 29 analyses yielded 207Pb/206Pb dates of 3722 ± 11 Ma for sample 10044, 3772 ± 9 Ma for 30 sample 75055 and 3739 ± 10 Ma for sample 74255, at 95% confidence level. These dates are 31 consistent with previously determined crystallization and emplacement ages of these samples 32 using different radiogenic systems. These high-precision ages allow refinement of the timing 33 of some of the high-Ti basaltic volcanism on the Moon. Crystallization ages of three different 34 high-Ti basalt units, integrating these new Pb/Pb ages with previous Rb-Sr and Sm-Nd age 35 determinations, are consistent with previous estimates but associated with uncertainties 3 to 5 36 times lower. In addition, the data obtained in this study confirm that tranquillityite contains 37 very low amounts of initial common Pb and has a high Pb ionization efficiency, making it an 38 excellent candidate for Pb/Pb dating by ion microprobe. -
74275 Oriented Ilmenite Basalt 1493 Grams
74275 Oriented Ilmenite Basalt 1493 grams 74275 Figure 1: Location of basalt sample 74275 at Shorty Crater - also see 74220. (falce color) AS17-137-20990 Introduction 1981). This sample has proven useful to studies that 74275 is a fine-grained, high-Ti mare basalt with require known lunar orientation with extended significant armalcolite content (Hodges and Kushiro exposure history to the extra-lunar environment 1974; Neal and Taylor 1993). It contains vesicles, vugs (micrometeorites, cosmic rays, solar irradiation). The and unusual olivine megacrysts (Fo82) (Meyer and sample is relatively flat 17 by 12 cm and 4 cm thick. Wilshire 1974). The top (T1) surface is somewhat rounded and has many micrometeorite pits (figure 4), while the bottom 74275 was collected from the rim of Shorty Crater (B1) surface is flat and angular and without any (figure 1) and was photographed both on the lunar evidence of exposure to the micrometeorites (figure surface and in the laboratory (with similar lighting) to 5). Fink et al. (1998) have carefully considered the document the exact lunar orientation. (Wolfe et al. exact orientation (30 deg tilt), shielding (nearby Lunar Sample Compendium C Meyer 2011 boulder) and detailed exposure history (complex) of 74275 74275. Di Hd This basalt has been determined to be very old (> 3.8 b.y.). Based on trace element analysis it is a type C Apollo 17 basalt. Petrography Perhaps the best petrographic description of 74275 is En Fs given by Hodges and Kushiro (1974): “Rock 74275 is a fine-grained ilmenite basalt with microphenocrysts Fo Fa of olivine (Fo80-71), titanaugite (up to 6.8 wt. -
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. -
Appendix a Apollo 15: “The Problem We Brought Back from the Moon”
Appendix A Apollo 15: “The Problem We Brought Back From the Moon” Postal Covers Carried on Apollo 151 Among the best known collectables from the Apollo Era are the covers flown onboard the Apollo 15 mission in 1971, mainly because of what the mission’s Lunar Module Pilot, Jim Irwin, called “the problem we brought back from the Moon.” [1] The crew of Apollo 15 carried out one of the most complete scientific explorations of the Moon and accomplished several firsts, including the first lunar roving vehicle that was operated on the Moon to extend the range of exploration. Some 81 kilograms (180 pounds) of lunar surface samples were returned for anal- ysis, and a battery of very productive lunar surface and orbital experiments were conducted, including the first EVA in deep space. [2] Yet the Apollo 15 crew are best remembered for carrying envelopes to the Moon, and the mission is remem- bered for the “great postal caper.” [3] As noted in Chapter 7, Apollo 15 was not the first mission to carry covers. Dozens were carried on each flight from Apollo 11 onwards (see Table 1 for the complete list) and, as Apollo 15 Commander Dave Scott recalled in his book, the whole business had probably been building since Mercury, through Gemini and into Apollo. [4] People had a fascination with objects that had been carried into space, and that became more and more popular – and valuable – as the programs progressed. Right from the start of the Mercury program, each astronaut had been allowed to carry a certain number of personal items onboard, with NASA’s permission, in 1 A first version of this material was issued as Apollo 15 Cover Scandal in Orbit No. -
Expanded Listings for Wskg Hdtv
1 Follow the Black, homeless queer Join a team of archaeologists as and trans youth who call NY's they examine one of the most Christopher Street Pier their home. significant Viking graves ever 11:30pm Amanpour and found. Company 11pm Amanpour and Company 12:30am History with David 12am BBC World News WSKG-HD Rubenstein 12:30am Articulate with Jim Cokie Roberts Cotter August 2021 An interview with the late Cokie Finding Meaning Roberts, political commentator and Timothy Showalter uses music to expanded listings author, is showcased. survive a tumultuous world. John 3 Tuesday Jarboe wants to help change it. 1 Sunday 8pm Finding Your Roots 5 Thursday 9pm Unforgotten Season 4 On Freedom Tales 8pm W1a Masterpiece S. Epatha Merkerson and Michael 8:30pm W1a Episode 4 Strahan learn stories that challenge 9pm Downton Abbey Season 5 Cassie and Sunny discover Walsh assumptions about black history. On Masterpiece was chased by all four suspects on 9pm Jesse Owens: American Episode One the night in question. Experience A working-class prime minister is 10pm Professor T The athlete's life and his victories in elected. Robert is snubbed by the Mother Love the face of Nazi racism at the 1936 village. Edith plays with fire. Professor T is called upon to help Olympics are explored. 10:25pm Downton Abbey Season investigate the disappearance of a 10pm Fight: American 5 On Masterpiece six year-old girl. Experience Episode Two 11pm Halifax: Retribution Examine the impact of the historic Rose hits on a strategy to get a 12am Secrets of Royal Travel bout between heavyweight Joe radio in the house. -
Spacecraft Deliberately Crashed on the Lunar Surface
A Summary of Human History on the Moon Only One of These Footprints is Protected The narrative of human history on the Moon represents the dawn of our evolution into a spacefaring species. The landing sites - hard, soft and crewed - are the ultimate example of universal human heritage; a true memorial to human ingenuity and accomplishment. They mark humankind’s greatest technological achievements, and they are the first archaeological sites with human activity that are not on Earth. We believe our cultural heritage in outer space, including our first Moonprints, deserves to be protected the same way we protect our first bipedal footsteps in Laetoli, Tanzania. Credit: John Reader/Science Photo Library Luna 2 is the first human-made object to impact our Moon. 2 September 1959: First Human Object Impacts the Moon On 12 September 1959, a rocket launched from Earth carrying a 390 kg spacecraft headed to the Moon. Luna 2 flew through space for more than 30 hours before releasing a bright orange cloud of sodium gas which both allowed scientists to track the spacecraft and provided data on the behavior of gas in space. On 14 September 1959, Luna 2 crash-landed on the Moon, as did part of the rocket that carried the spacecraft there. These were the first items humans placed on an extraterrestrial surface. Ever. Luna 2 carried a sphere, like the one pictured here, covered with medallions stamped with the emblem of the Soviet Union and the year. When Luna 2 impacted the Moon, the sphere was ejected and the medallions were scattered across the lunar Credit: Patrick Pelletier surface where they remain, undisturbed, to this day. -
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. -
The Lunar Dust-Plasma Environment Is Crucial
TheThe LunarLunar DustDust --PlasmaPlasma EnvironmentEnvironment Timothy J. Stubbs 1,2 , William M. Farrell 2, Jasper S. Halekas 3, Michael R. Collier 2, Richard R. Vondrak 2, & Gregory T. Delory 3 [email protected] Lunar X-ray Observatory(LXO)/ Magnetosheath Explorer (MagEX) meeting, Hilton Garden Inn, October 25, 2007. 1 University of Maryland, Baltimore County 2 NASA Goddard Space Flight Center 3 University of California, Berkeley TheThe ApolloApollo AstronautAstronaut ExperienceExperience ofof thethe LunarLunar DustDust --PlasmaPlasma EnvironmentEnvironment “… one of the most aggravating, restricting facets of lunar surface exploration is the dust and its adherence to everything no matter what kind of material, whether it be skin, suit material, metal, no matter what it be and it’s restrictive friction-like action to everything it gets on. ” Eugene Cernan, Commander Apollo 17. EvidenceEvidence forfor DustDust AboveAbove thethe LunarLunar SurfaceSurface Horizon glow from forward scattered sunlight • Dust grains with radius of 5 – 6 m at about 10 to 30 cm from the surface, where electrostatic and gravitational forces balance. • Horizon glow ~10 7 too bright to be explained by micro-meteoroid- generated ejecta [Zook et al., 1995]. Composite image of morning and evening of local western horizon [Criswell, 1973]. DustDust ObservedObserved atat HighHigh AltitudesAltitudes fromfrom OrbitOrbit Schematic of situation consistent with Apollo 17 observations [McCoy, 1976]. Lunar dust at high altitudes (up to ~100 km). 0.1 m-scale dust present Gene Cernan sketches sporadically (~minutes). [McCoy and Criswell, 1974]. InIn --SituSitu EvidenceEvidence forfor DustDust TransportTransport Terminators Berg et al. [1976] Apollo 17 Lunar Ejecta and Meteorites (LEAM) experiment. PossiblePossible DustyDusty HorizonHorizon GlowGlow seenseen byby ClementineClementine StarStar Tracker?Tracker? Above: image of possible horizon glow above the lunar surface. -
Field Trials of a Prototype Lunar Rover Under Multi-Sensor Safeguarded Teloperation Control
In Proc Seventh- ANS- Topical Meeting on lC.,a# -* 7='- v I GA Field Trials of a Prototype Lunar Rover under Multi-Sensor Safeguarded Teleoperation Control E. Krotkov, M. Hebert, L. Henriksen, P. Levin, M. Maimone, R. Simmons, and J. Teza Robotics Institute, School of Computer Science Carnegie Mellon University, Pittsburgh, PA 152 13 Abstract - This paper presents the results of field trials of a prototype lunar rover traveling over natural terrain under safe- guarded teleoperation control. Both the rover and the safeguard- ing approach have been used in previous work. The original contributions of this paper are the development and integration of a laser sensing system, and extensive field testing of the overall system. The laser system, which complements an existing stereo vision system, is based on a line-scanning laser ranger viewing the area 1 meter in front of the rover. The laser system has demon- strated excellent performance: zero misses and few false alarms operating at 4 Hz. The overall safeguarding system guided the rover 43 km over lunar analogue terrain with 0.8 failures per kilo- meter. 1 Introduction The hazard detection system described in this paper has been developed under CMU's Lunar Rover Initiative, whose goal is to develop and demonstrate techniques enabling plane- tary rover missions. The initiative has targeted a mission to land two rovers on the surface of the Moon, where they will navigate semi-autonomously for 1,OOO km, visiting historic sites and places of geological interest (Krotkov 1994). For such a mission, a spectrum of navigation modes are applicable. -
Apollo Over the Moon: a View from Orbit (Nasa Sp-362)
chl APOLLO OVER THE MOON: A VIEW FROM ORBIT (NASA SP-362) Chapter 1 - Introduction Harold Masursky, Farouk El-Baz, Frederick J. Doyle, and Leon J. Kosofsky [For a high resolution picture- click here] Objectives [1] Photography of the lunar surface was considered an important goal of the Apollo program by the National Aeronautics and Space Administration. The important objectives of Apollo photography were (1) to gather data pertaining to the topography and specific landmarks along the approach paths to the early Apollo landing sites; (2) to obtain high-resolution photographs of the landing sites and surrounding areas to plan lunar surface exploration, and to provide a basis for extrapolating the concentrated observations at the landing sites to nearby areas; and (3) to obtain photographs suitable for regional studies of the lunar geologic environment and the processes that act upon it. Through study of the photographs and all other arrays of information gathered by the Apollo and earlier lunar programs, we may develop an understanding of the evolution of the lunar crust. In this introductory chapter we describe how the Apollo photographic systems were selected and used; how the photographic mission plans were formulated and conducted; how part of the great mass of data is being analyzed and published; and, finally, we describe some of the scientific results. Historically most lunar atlases have used photointerpretive techniques to discuss the possible origins of the Moon's crust and its surface features. The ideas presented in this volume also rely on photointerpretation. However, many ideas are substantiated or expanded by information obtained from the huge arrays of supporting data gathered by Earth-based and orbital sensors, from experiments deployed on the lunar surface, and from studies made of the returned samples. -
Floris Heyne Joel Meter Simon Phillipson Delano Steenmeijer
Floris Heyne Joel Meter Simon Phillipson Delano Steenmeijer Edited by Neil Pearson With a special foreword by Apollo 7 astronaut Walt Cunningham “When you get back… you will be a national hero. But your photographs… they will live forever. Your only key to immortality is the quality of your photography.” Richard W. Underwood NASA Chief of Photography for Mercury, Gemini and Apollo 4 Small steps. Giant leaps. The English word ‘photograph’ is made up of the The early exploration of space is one such historical ancient Greek words ‘photos’ and ‘graphos’ which event, unrivaled among humanity’s achievements. literally mean ‘light writing’. At the time of the Apollo Fortunately space travelers were able to bring back program, that meant exposing a chemically-treated beautiful, moving and instantly recognizable images film to patterns of light and it was this process which to depict it. Those images add a new understanding made it possible to seize moments in time and share to what it means to be human, what it means to them with the world. live on a delicate little orb circling the Sun since time immemorial. A single photograph can tell a story to billions of people. It transcends language barriers, physical Not only did Apollo bring us this photographic barriers and requires no prior knowledge of testimony but many major advancements in the subject. This is the beauty of photography: photographic technology date back to the extensive it reaches out to all people and everybody can research and engineering that was part of the hugely intuitively understand its form and content.