Lunar Rover with Multiple Science Payload Handling Capability
Total Page:16
File Type:pdf, Size:1020Kb
Load more
Recommended publications
-
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. -
350 International Atlas of Lunar Exploration 8 January 1973
:UP/3-PAGINATION/IAW-PROOFS/3B2/978«52181«5(M.3D 350 [7428] 19.8.20073:28PM 350 International Atlas of Lunar Exploration 8 January 1973: Luna 21 and Lunokhod 2 (Soviet Union) The 4850 kg Luna 21 spacecraft was launched from Baikonur at 06:56 UT on a Proton booster, placed in a low Earth parking orbit and then put on a lunar trajec tory. Power problems required that the Lunokhod solar panel be opened in flight to augment power, and stowed again for the trajectory correction and orbit insertion burns and for landing. On 12 January Luna 21 entered a 90 km by 100 km lunar orbit inclined 60° to the equator. After a day in orbit the low point was reduced to 16 km, and on 15 January after 40 orbits the vehicle braked and dropped to just 750 m above the surface. Then the main thrusters slowed the descent, and at :UP/3-PAGINATION/IAW-PROOFS/3B2/978«52181«5(M.3D 351 [7428] 19.8.20073:28PM Chronological sequence of missions and events 351 22 m a set of secondary thrusters took over until the After landing, Lunokhod 2 surveyed its surround spacecraft was only 1.5 meters high, when the thrusters ings. A rock partly blocked the west-facing ramp so the were shut off. Landing time was 23:35 UT. rover was driven east across a shallow crater, leaving the The site was in Le Monnier crater on the eastern edge lander at 01:14 UT on 16 January. It rested 30 m from of Mare Serenitatis, 180 km north of the Apollo 17 land the descent stage to recharge its batteries until 18 ing site, at 25.85° N, 30.45° E (Figure 327A). -
Searching for Lunar Horizon Glow with the Lunar Orbiter Laser Altimeter (LOLA)
Searching for lunar horizon glow with the lunar orbiter laser altimeter (LOLA) M. K. Barker, D. Smith, T. McClanahan, E. Mazarico, X. Sun, M. T. Zuber, G. A. Neumann, M. H. Torrence, J. W. Head DAP-2017 Boulder, CO Jan. 11-13, 2017 Lunar Horizon Glow • Surveyor landers, Lunokhod-2 lander, Apollo 17 astronaut sketches (Rennilson & Criswell 1974, Severnyi et al. 1975, McCoy & Criswell 1974, Zook & McCoy 1991) ==> Electrostatic levitation, dynamic lofting (Stubbs et al. 2006, Farrell et al. 2007) • Apollo 15 photographs at dawn: LHG extending ~30 km above horizon, N~103-105 cm-2 for grain r = 0.1 µm (McCoy 1976, Glenar et al. 2011) ==> Meteor stream impact ejecta could initiate a saltation-like cascade process • Recent searches with Clementine Star Trackers, LRO/LAMP, and LADEE/LDEX gave limits on dust density ~100x lower than A15 (Glenar et al. 2014, Feldman et al. 2014, Szalay & Horányi 2015, Horányi et al. 2015) Glenar et al. (2011) Lunar Orbiter ~65 m Diffractive Optical Element Laser Altimeter (LOLA) •5-beam time-of-flight laser altimeter onboard the Lunar Reconnaissance 50 m Orbiter (LRO) 5-m diameter •28 Hz laser, 140 measurements/sec observation area (red) •Each shot provides: • up to 5 ranges to surface (10 cm prec.) 20-m FOV (green) • footprint-scale surface roughness • footprint-scale slope 10 to 12 m apart • 1064-nm reflectance of surface along track •Detectors: 5 fiber optically-coupled avalanche photodiodes LOLA has two radiometric modes: (1) Active radiometry: LOLA laser is the light source. 1064-nm normal albedo Lemelin et al. (2016) (2) Passive radiometry: Sun is the light source. -
SOIL Xecfinics RESULTS of LUNA 16
SOIL XECfiNICS RESULTS OF LUNA 16 Stewart bl. Johnson U. David Carrier, I11 1172-14896 (NASA-TI-I-67 566) SOIL lECAANICS R OF LUWA 16 AN D LUYOKHOD 1: A PBELI RSPORT S.Y. Johnson, nt a1 (HASA) Unclas 1971 13 p NASA-Manned Spacecraft Center .Houston, Texas 77058 9 June 1'971 The Ninth International Symposium on Space Technology and Science was held in Tokyo, Jcpan May 17-22, 1971. At this meeting two papers ? (Ref. 1 and 2) were presented giving results of the Luna 16 and Lunokhod-I experiments. These reports, whi ch were presented by representatives of the Academy of Sclence of the USSR, concentrateci on nechanical ard physicai properties of the luaar soil. In addition to these two papers, there were two 20-mi nute films shown on Luna 16 and Lc.~okhodI. The overall impression was that the USSR has performed a nuch more extensive soi l mechanics i'nvestigation on thei r returned lunar-~&~~leand as part of the Lunokhod traver;a than has been- - perfomed by the U.S. to date in the Apol lo program. Apparently the aussian soil nechanics investigations are being conducted with the vf e-d that datbcollected now will be valuable in future exploratidn of- - the 1unar surface. It was suggested that later versions of Lunokhod would Ce used to explore t!e far side of the Roan and would have a data ,storage capabi 1i ty to use while cut of communication with eart!!. - At the meeting in Tokyo, results were presented for ths Lunokhod-I penetrometer and analyses of the interactions between the vehicle wheds and the lunar soi 1. -
Aerogel Background Slides
Aerogels Background Information Version 052917.1 Overview The following slides present background information on aerogel and its role in nanotechnology. They may be presented as part of a lecture introducing the Aerogel activity. Aerogel’s nickname: “Solid blue smoke” Aerogel resembles a hologram. Is it there or not? Aerogel is a highly porous, solid material. Aerogel has the lowest density of any solid known to man. It is one thousand times less dense than glass. NASA Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California Aerogel is a Product of Nanotechnology Aerogels are made of 10nm silica spheres. They weigh only slightly more than air. In fact, one form is 99.8% air. About 8,000 of these air Scanning electron microscope image of aerogel bubbles would fit across a single human hair Why is Aerogel Blue? The size of the air bubbles is similar in size to the molecules in air and the air pockets in glaciers. They all scatter blue light more than red, making them look blue. NASA Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California Gray Glacier, Torres del Paine National Park Chile How is Aerogel Made? • Labs make aerogels by suspending silicon dioxide in alcohol and water to form a gel. • The liquid is removed with carbon dioxide under high pressure and temperature. • Aerogels are expensive to make. Extreme Physical Properties of Aerogel Property Silica Aerogel Silica Glass Density (kgm3) 5-200 2300 Specific Surface area 500-800 0.1 (m2/g) Optical Transmission 90% 99% at 632.8nm -
The Soviet Space Program
C05500088 TOP eEGRET iuf 3EEA~ NIE 11-1-71 THE SOVIET SPACE PROGRAM Declassified Under Authority of the lnteragency Security Classification Appeals Panel, E.O. 13526, sec. 5.3(b)(3) ISCAP Appeal No. 2011 -003, document 2 Declassification date: November 23, 2020 ifOP GEEAE:r C05500088 1'9P SloGRET CONTENTS Page THE PROBLEM ... 1 SUMMARY OF KEY JUDGMENTS l DISCUSSION 5 I. SOV.IET SPACE ACTIVITY DURING TfIE PAST TWO YEARS . 5 II. POLITICAL AND ECONOMIC FACTORS AFFECTING FUTURE PROSPECTS . 6 A. General ............................................. 6 B. Organization and Management . ............... 6 C. Economics .. .. .. .. .. .. .. .. .. .. .. ...... .. 8 III. SCIENTIFIC AND TECHNICAL FACTORS ... 9 A. General .. .. .. .. .. 9 B. Launch Vehicles . 9 C. High-Energy Propellants .. .. .. .. .. .. .. .. .. 11 D. Manned Spacecraft . 12 E. Life Support Systems . .. .. .. .. .. .. .. .. 15 F. Non-Nuclear Power Sources for Spacecraft . 16 G. Nuclear Power and Propulsion ..... 16 Te>P M:EW TCS 2032-71 IOP SECl<ET" C05500088 TOP SECRGJ:. IOP SECREI Page H. Communications Systems for Space Operations . 16 I. Command and Control for Space Operations . 17 IV. FUTURE PROSPECTS ....................................... 18 A. General ............... ... ···•· ................. ····· ... 18 B. Manned Space Station . 19 C. Planetary Exploration . ........ 19 D. Unmanned Lunar Exploration ..... 21 E. Manned Lunar Landfog ... 21 F. Applied Satellites ......... 22 G. Scientific Satellites ........................................ 24 V. INTERNATIONAL SPACE COOPERATION ............. 24 A. USSR-European Nations .................................... 24 B. USSR-United States 25 ANNEX A. SOVIET SPACE ACTIVITY ANNEX B. SOVIET SPACE LAUNCH VEHICLES ANNEX C. SOVIET CHRONOLOGICAL SPACE LOG FOR THE PERIOD 24 June 1969 Through 27 June 1971 TCS 2032-71 IOP SLClt~ 70P SECRE1- C05500088 TOP SEGR:R THE SOVIET SPACE PROGRAM THE PROBLEM To estimate Soviet capabilities and probable accomplishments in space over the next 5 to 10 years.' SUMMARY OF KEY JUDGMENTS A. -
Lunar Laser Ranging: the Millimeter Challenge
REVIEW ARTICLE Lunar Laser Ranging: The Millimeter Challenge T. W. Murphy, Jr. Center for Astrophysics and Space Sciences, University of California, San Diego, 9500 Gilman Drive, La Jolla, CA 92093-0424, USA E-mail: [email protected] Abstract. Lunar laser ranging has provided many of the best tests of gravitation since the first Apollo astronauts landed on the Moon. The march to higher precision continues to this day, now entering the millimeter regime, and promising continued improvement in scientific results. This review introduces key aspects of the technique, details the motivations, observables, and results for a variety of science objectives, summarizes the current state of the art, highlights new developments in the field, describes the modeling challenges, and looks to the future of the enterprise. PACS numbers: 95.30.Sf, 04.80.-y, 04.80.Cc, 91.4g.Bg arXiv:1309.6294v1 [gr-qc] 24 Sep 2013 CONTENTS 2 Contents 1 The LLR concept 3 1.1 Current Science Results . 4 1.2 A Quantitative Introduction . 5 1.3 Reflectors and Divergence-Imposed Requirements . 5 1.4 Fundamental Measurement and World Lines . 10 2 Science from LLR 12 2.1 Relativity and Gravity . 12 2.1.1 Equivalence Principle . 13 2.1.2 Time-rate-of-change of G ....................... 14 2.1.3 Gravitomagnetism, Geodetic Precession, and other PPN Tests . 14 2.1.4 Inverse Square Law, Extra Dimensions, and other Frontiers . 16 2.2 Lunar and Earth Physics . 16 2.2.1 The Lunar Interior . 16 2.2.2 Earth Orientation, Precession, and Coordinate Frames . 18 3 LLR Capability across Time 20 3.1 Brief LLR History . -
Aerogel Fact Sheet
The NASA Vision The NASA Mission To improve life here, To understand and protect our home planet, To extend life to there, To explore the universe and search for life, To find life beyond To inspire the next generation of explorers Aerogel ...as only NASA can Mystifying Blue Smoke At first sight, aerogel resembles a hologram. An JPL’s second application of aerogel is spacecraft in- excellent insulator, aerogel has the lowest density sulation. Because aerogel is mostly air, an effective Property Silica Aerogel Silica Glass of any known solid — one form of this extraordi- thermal insulator is contained within its porous nary substance is actually 99.8 percent air and silica network. This presents an excellent thermal Density (kgm3) 5 – 200 2300 0.2 percent silica dioxide (by volume). Aerogels barrier to protect the spacecraft against the ex- Specific Surface Area 500 – 800 0.1 have open-pore structures similar to honeycomb, treme cold of deep space. The Mars Pathfinder (m2/g) but in fact they are low-density, solid materials mission used aerogel to protect the electronics Refractive Index at with extremely fine microstructures. Typically sili- of the Sojourner rover against the frigid Martian 1.002 – 1.046 1.514 – 1.644 632.8 nm con-based like ordinary glass, or carbon-based like environment during Sojourner’s 1997 travels on common organic synthetics, aerogels possess the red planet. Each of the twin Mars Exploration Optical unique physical properties (see table). The unique Rovers, scheduled to land on Mars in early 2004, Transmittance 90% 99% characteristics of aerogels are being applied to employs aerogel for thermal insulation of the bat- at 632.8 nm tery, electronics, and computer in the chassis, or meet new technological demands. -
Investigation of Carbon Nanotube Grafted Graphene Oxide Hybrid Aerogel for Polystyrene Composites with Reinforced Mechanical Performance
polymers Article Investigation of Carbon Nanotube Grafted Graphene Oxide Hybrid Aerogel for Polystyrene Composites with Reinforced Mechanical Performance Yanzeng Sun †, Hui Xu †, Zetian Zhao, Lina Zhang, Lichun Ma, Guozheng Zhao, Guojun Song * and Xiaoru Li * Institute of Polymer Materials, School of Material Science and Engineering, Qingdao University, No. 308 Ningxia Road, Qingdao 266071, China; [email protected] (Y.S.); [email protected] (H.X.); [email protected] (Z.Z.); [email protected] (L.Z.); [email protected] (L.M.); [email protected] (G.Z.) * Correspondence: [email protected] (G.S.); [email protected] (X.L.) † Yanzeng Sun and Hui Xu are co-first authors. Abstract: The rational design of carbon nanomaterials-reinforced polymer matrix composites based on the excellent properties of three-dimensional porous materials still remains a significant challenge. Herein, a novel approach is developed for preparing large-scale 3D carbon nanotubes (CNTs) and graphene oxide (GO) aerogel (GO-CNTA) by direct grafting of CNTs onto GO. Following this, styrene was backfilled into the prepared aerogel and polymerized in situ to form GO–CNTA/polystyrene (PS) nanocomposites. The results of X-ray photoelectron spectroscopy (XPS) and Raman spectroscopy indicate the successful establishment of CNTs and GO-CNT and the excellent mechanical properties of the 3D frameworks using GO-CNT aerogel. The nanocomposite fabricated with around 1.0 wt% GO- CNT aerogel displayed excellent thermal conductivity of 0.127 W/m·K and its mechanical properties Citation: Sun, Y.; Xu, H.; Zhao, Z.; Zhang, L.; Ma, L.; Zhao, G.; Song, G.; were significantly enhanced compared with pristine PS, with its tensile, flexural, and compressive Li, X. -
Mapping and GIS-Analyses of the Lunokhod-1 Landing Site
43rd Lunar and Planetary Science Conference (2012) 1750.pdf Mapping and GIS-Analyses of the Lunokhod-1 Landing Site. E. Gusakova1, I. Karachevtseva1, K.Shingareva1, J. Oberst1,2,3, O. Peters2, M.Wählisch2, and M. S. Robinson4. 1Moscow State University of Geodesy and Cartography (MIIGAiK), Gorokhovskiy per., 4, 105064, Moscow, Russia; 2German Aerospace Center (DLR); 3 Technical Uni- versity of Berlin, Germany; 4Arizona State University, USA Introduction: The Soviet spacecraft Luna 17 was small craters, which could be compare with results of launched towards the Moon in November 1970 and mapping that had been carried out during the Lunok- deployed Lunokhod-1, the first rover to explore an hod-1 mission. We conclude that LRO NAC images extraterrestrial surface. Until October 1971, Lunokhod- can be used for cartography support at high level of 1 acquired about 20,000 TV pictures and 206 stereo detail for characterization of future landing sites such images along its traverse [1]. Using recent new high as LUNA-GLOB and LUNA-RESOURCE. resolution images we mapped the landing site and tra- Reference: [1] Barsukov V.L. et. al. (1978) Pe- verse route, using automated GIS-oriented mapping. redvijnaya laboratoriya na Lune Lunokhod-1, Vol. 2. Sources: We used high resolution Digital Eleva- Nauka (in Russian). [2] Oberst J. et al. (2010) LPSC tion Model (DEM) and orthoimage from photogram- XLI, Abstract #2051. [3] Kneissl T. et al. (2011) Pla- metric processing of Lunar Reconnaissance Orbiter net. Space Sci., 59, 1243-1254. [4] Karachevtseva I. et Camera (LROC) Narrow Angle Camera (NAC) stereo al. (2011) The Book of Abstracts of the 2-nd Moscow images [2] with a spatial resolution of 0.5 m/pixel Solar System Symposium (2M-S3), Space Research (M150749234, M150756018). -
Planetary Rover Mobility on Loose Soil
PLANETARYROVERMOBILITYONLOOSESOIL: TERRAMECHANICSTHEORYFORSIDESLIPPREDICTION ANDCOMPENSATION nicolò carletti Supervisor: Prof. Michéle Lavagna Master of Science Space Engineering Department of Aerospace Science and Technology Politecnico di Milano December 2016 – 816663 ABSTRACT The aim of this thesis is to develop a model which can predict a mobile trajectory profile of the rover under loose soil condition. The study also encapsulates a traversal run in a sloped terrain without the skid characteristics. The geometry and features are defined to model the rover as known as Moonraker: the lunar rover of the team HAKUTO, competing for the Google Lunar XPRIZE. After a brief introduction of the working environment, a chapter is de- dicated to the modeling of the forces generated from the interaction between wheels with soil, depending on the slip ratio and the slip angle. The used model is the one proposed by G. Ishigami [6, 7, 8, 9], based on the work of M. G. Bekker [1, 2] and J. Y. Wong [3] and modi- fied, according to what proposed by M. Sutoh [11, 12, 13], to explicitly consider the grouser effect. The model is verified through One-Wheel tests. The equations of motion are retrieved and the numerical simulation with iterative loop is described. The desired state is reached imposing arbitrary inputs to the wheels. Two input strategies are discussed: torque input and velocity input. The resulting motion is compared with tests on both controlled (sand- box) and uncontrolled environment. The former is mainly used to ve- rify the precision of the model, and the latter to prove the sensibility to the ground properties. -
Workshop Report
WORKSHOP REPORT July 2019 This report was compiled by Andrew Petro, Anna Schonwald, Chris Britt, Renee Weber, Jeff Sheehy, Allison Zuniga, and Lee Mason. Contents Page EXECUTIVE SUMMARY AND RECOMMENDATIONS 2 WORKSHOP SUMMARY 5 Workshop Purpose and Scope 5 Background and Objectives 5 Workshop Agenda 6 Overview of Lunar Day/Night Environmental Conditions 7 Lessons Learned From Missions That Have Survived Lunar Night 8 Science Perspective 9 Exploration Perspective 10 Evolving Requirements from Survival to Continuous Operations for Science, 11 Exploration, and Commercial Activities Power Generation, Storage and Distribution - State of the Art, Potential 13 Solutions, and Technology Gaps Thermal Management Systems, Strategies, and Component Design Features - 16 State of the Art, Potential Solutions, and Technology Gaps The Economic Business Case for Creating Lunar Infrastructure Services and 18 Lunar Markets International Space University Summer Project “Lunar Night Survival” 20 Open Discussion Summary 21 APPENDIX A: Workshop Organizing Committee and Participants 23 APPENDIX B: Poster Session Participants 28 1 Survive and Operate Through the Lunar Night WORKSHOP REPORT June 2019 EXECUTIVE SUMMARY AND RECOMMENDATIONS The lunar day/night cycle, which at most locations on the Moon, includes fourteen Earth days of continuous sunlight followed by fourteen days of continuous darkness and extreme cold presents one of the most demanding environmental challenge that will be faced in the exploration of the solar system. Due to the lack of a moderating atmosphere, temperatures on the lunar surface can range from as high as +120 C during the day to as low as -180 C during the night. Permanently shadowed regions can be even colder.