Movement of Surveyor 3 Spacecraft

Total Page:16

File Type:pdf, Size:1020Kb

Movement of Surveyor 3 Spacecraft VOl,. 76, NO. 14 JOURNAL OF GEOPHYSICAL RESEARCH MAY 10, 1971 BriefReport Movementof Surveyor3 Spacecraft R. F. $corrrr,T.-D. Lu, .aNDK. A. Ztrcxcga•tAN Division o• Engineeringand Applied Science California Institute of Technology, Pasadena 91109 An examinationof the positionof the Surveyor3 spacecraftas it appearedin the photo- graphs taken by astronautsC. Conrad and A. Bean of the Apollo 12 lunar mission in Novem- ber 1969 suggestedthat some changeshad occurred in the spacecraft'sattitude since the Surveyoroperation of April 1967.A detailedstudy was made by simulatingin the laboratory the position of one of the Surveyor spacecraft'sfootpads and its imprints in the lunar surface. Photographswere taken both from the location of the original Surveyor television camera and from the estimated position of the astronauts.It was found to be impossibleto match the footpad and imprint positionsand attitude in picturestaken from the two points of view. Consequently,it is tentatively concludedthat the Surveyor spacecraft moved a few inches at some time between May, 1967 and November 1969. It seemsmost likely that this movement occurred as a result of a relatively sudden failure of one or two of the shock absorbers on Surveyor'slanding gear, since2 out of the 3 shock absorberswere collapsedat the time of the astronauts' visit. The Surveyor 3 spacecraft landed on the served; the footpad had plowed downhill moon on April 20, 1967, and was operateduntil throughthe soil, and in its final positionthe May 3, 1967. The scientific and engineering visible part of its top surfacewas a few inches results of its sojourn on the lunar surfacehave above the soil level. been reported [Surveyor 3 Mission Report, On November 19, 1969, the Lunar Module 1967]; thosepertinent to this discussionwill be of the Apollo 12 spacecraftcarrying astronauts repeated briefly here. C. Conradand A. Beanlanded near Surveyor 3, No communication was returned from the and in the second of their two excursions on spacecraft after its first lunar night. At the the lunar surface the two astronauts visited their termination of its multiple impact touchdown, precursor.They took a numberof photographs the spacecraftcame to rest on the inner eastern of Surveyor and removed several spacecraft slope of a 200-meter-diameter crater. The components for return to earth. Some of the ground slope was approximately 10ø to 12ø , photographs,when comparedwith the original and the inclination of the spacecraft'svertical Surveyor pictures,suggest that, at sometime axis from lunar vertical was determined to be betweenSurveyor 3 shutdownon May 3, 1967, 12.4ø. One of the vehicle'sfootpads (number 2) and the time the photographswere taken by was within the field of view of the television Conrad and Bean, the Surveyor spacecraft camera;another (number3) was partly visible; moved a few inches. and the third was obscuredby spacecraftcom- ponents.In the last stagesof landing, footpad MOVEMENT STUDY 2 left an impressionon the lunar surfacea few On their way toward Surveyor3, Conrad inches from its final location. The appearance and Bean took the photographshown here as of this apparently penultimatecontact and the Figure 2. If the mast anglein this pictureis footpad itself from the point of view of the measured with respect to the visible lunar Surveyortelevision camera is shownin Figure 1. horizon,it is found to be about 15ø , in the Only the right sideof footpad3 couldbe ob- planeof the picture.The maximumdownslope angleof tilt wouldbe somewhatgreater. If the Copyright ¸ 1971 by the American Geophysical Union. lunar horizon differs from the true horizontal 3414 BRIEF REPORT 3415 in this picture by less than 2.5ø, it would shock absorber of leg 3 in Figure 4 showed appear that the spacecraft has increasedits that the latter shock absorber is also collapsed inclination downslopesince 1967. More positive All the shock absorberswere extended during evidencefor this is apparent in Figures3 and 4 the landing and communicationlife of Surveyor of legs I and 3, respectively,also taken by the 3 in 1967. The shock absorbers contained helium astronauts.In this picture, the shock absorbers gas at high pressure;the gas was retained by of legs I and 3 are seento have collapsed.Their seals that can fail. It is concluded that the normally extended position can be seen from shockabsorbers on legs I and 3 of Surveyor 3 the position of the leg 2 shock absorber in collapsed at some time after the terminalion Figure 2. Here the extended shock absorber of communicationwith the spacecraft. and its supportingstrut form a straight line, in An indication that the failure of the shock comparisonwith the angle visible in Figure 3 absorber on leg 3, at least, may have been of leg 1. Study of the positionof the leg 2 shock suddenis seen in Figure 4, taken by the astro- absorber in Figure 2 and comparisonwith the nauts and showingfootpad 3. This picture indi- ... Fig. 1. Picture of footpad 2 from Surveyor 3 television camera, April 21, 1967. The imageis hazy becausea film of lunar dust was depositedon the mirror of the cameraduring the landing (GMT day 111, 07h 43m 38s). 3416 SCOTT,Lu, AND ZUCKERMAN caresthat the edge of footpad 3 not visible to white were a light tan color at the time of the Surveyor 3 camera dug into the lunar soil their visit. This observation was subsequently so that its upper surfacebecame covered with confirmedby examinationof the returnedspace- soil. However, a lighter shadingappears around craft parts [Benson et al., 1970]. It is con- the edgeof the pile of soil on the footpad.This jectured, therefore, that the footpad receiveda was at first interpreted [Scott et al., 1970], it partial coveringof soil in the landing in April is now thought erroneously,as being lunar soil 1967; this soil protected the underlying foot- of a lighter color. pad surfacefrom a processthat either coated However, the astronauts reported that the or, more probably, altered the white surfaceto exposedspacecraft parts Ihat were originally tan in an unknown length of time. When the ..•:.... :.4... .:. ",.•.•'• - •":•''•'•.•?.-:.•',.-'.-•.i•-' :.•::•,.-'•,.-.•:::•:,+.-.•.•: ......................•..:.....:.......... ........ -..' .:.......... •:............ •. :.:.:::....:.::.•:i•:•.:"•:•ii::•::...•?`.•...:•..:•?.•``..•...`.........::•?.?`::::..`...•:?...:.:•::.•:'•...:.-gi.?•4•:;::;:':::•..•'.:': ........ .•. .•.'.i•:•:.,..:.:..::.5•{:•i'"":,,""':•*•::.•:•'•:D:}:•::i:{•-'.- "•..::.•-.•:i•i!i•.-,?•...•..:•::{i:-'-'..-'•::::i•::!:•" .....•:•"-•'--';.-'-".-'•i:•.::.,•.<•::2•:-•.•i'r•:•:•:•::}•,•:•i•:::.•:.-:.-:{{..i••..... ..::i::i•:{•.:.-.-•.•-...:•...::,•..:.•:•'.,,•.•,•,,•.•.::...•:i•:•,• • ........"•--.•.••.'•••.•.............,••....•'..'z,..•:"•:'•'•.••,•, - • ' •-....... ......• ::'...:.......• '?::•...•._•.::..::,•.•.•,•.q•.•..•:.•.. ...........................•......... ...................... ;•:!•!:•-•....... .::::{:{•',•.•.....,,x.•,•_.:..•::,::::•!i.....'-:!-- .:..:i:...?•.':.,•..-•.,_•:.•:..>... .........'.•::•-..}'-.•::..,.g..,•:.:.:.*..>...:• ......•-:.--.- •: .......... --...•:•:•i!:. • .......- ....• ........i:...... •-.•.'•......:•'•-. :..•. ..................::-•.•[:•.•. •. .. ....•....•:•,•::...-::,..-..-.•g•:i•....;,.-•.z,.•.::--' -'5'• ..... - -:.. •(• .... ...........:.- ...... .-..:.-.•..•,-...•.. .......... .,•..½.•'•ß .•..•:•....*.. --- .. ................... •.... ..:•:•:..•::!z?ß............. '.' ...:'-:.z?....:.::•%•i:i•.:.:.i½-'-:--::•:..•4•-,: .:• "•:-• .........•........ - .........:.•!i•" ..•:'"•:•::•.:."'{•:•ß': ' ' .............. '.•'..•,:•:::[.:::..'.,::-:' c{::•-...........:•.•......... ...•.•.:.•;•:.2-'. ......ß:---S:•:p:....:;r'•: .....:':g:•.......:.•,:..•.'•..:• ............:.:.:........... .:2:..•.:•:•,...-.:-•!'..:i ß:::::::•.-'..-.':.•:• ............?.•":•: "'::.:.:•.:ß.•!:-{::.'.•'.-"•!'•:ß..•::.:.::.• ............-':•.•..:.'ßß..;...?'•.....,}•...::•::•. .-.>:•'i.:;!:'/-...' .'.'::.".'""?.,:• ..... :::-:-::"'ß.-::......,•::•:•{-.'-:Ji'.".'};..•:•' %::-' .....•.:•+?::•:•.•.•..r::•}:.:•.5•:.:•.`.•::•:::..•:.•.:•:::?.•f•.*..?:..}......•.•... • .• ß•..• .::•:.:.•4.•:::.•,.:•:a,•r•.•. ..........---'-'•--'•--:-•••'•-- c:': '•':'-'•::::•.--•---. ....". ..'• '.".•.. ' :".....-::?': "':::;.'.......•:&:.." ":•:?.-'•.:':•.?' "• ""••'' "'•••••i•'•::•'• "•'• ••••••••••:'..•...:.?::?'.::'::•,•..•....- .::.:•:.•:-•?.....•..... -•":--:.-.%•---='...'•..•:..:•;11::::-•:•:•:•::::::::.*-•.•i•:::•}.:-:•:-"•:. ' .....r-'.': •ø•'"•{•:•:--::•.'-.:.;?:::2:"•.---. •" ".---,.•; ...... :• :•:!::• ........ ::.:.-' :.-:..":•:>•4•ii::::::::?:i:'.'::•.'!-.-.::.:.::":•::•i ;•-•---'-:'::...:..--/.ß,•i}':•-:-•!•{•::{•::{-":,:•./..."•j::i•ß'•-•:•'•:..,,•:•... -".....:.... •.'i..::.:_q•.:::::•::•-:• . '•'-: •*:•.'•..•.:-•.':':::::::::-.... :•. ':.,•,' -:'::::•:•'•::•'-. ....-:....•...•.. •ß.....• . ß................ -...... :--- .. -½:.-:::-•.:.•::;•.::•.-...'-•:-.•k•:•-.:.•:.::•:•-.......•:;•-:.-•,•.•:'::•':•'•-.'-:-•:• ::.?.•?-:•r:-..•.r4-x •:.-•...... ... •. - ....•**-•:"•:•:..-...--.::.:...•.::.::::•-•..<.•:+:::4.: ':..:,.•:::.:.:•.• ..:-:•....-.•....,/• - 'J.:':" : •.-•.•:.•'-'-,---:->•.• •z::•:•:::•.`...}•z•:::•:::•.::•::r•}!•z.•:.•`::.•.•:.:::..:.::•::•:::•.i•.-.'•.•.!:•;•...-.....:•:,•.-.•..:.•..-.•:..-• •.:•:. • •...•: .•*:•'.:.'•.*•- .•__:...•.•.:•. '•'*•*•'-"' ": ß r• -'• .......... '•::i.t•."•.'i_••:.•...::r:•.... -::•....... :'•}.•i:..'•.:•!::.•: . ......::.-.-.-:•: :.-.-.•.....•-•,e..•.m:•.:.•-...e-.. '•.:..:,•. .......ß'-:•'•-" "•-.-D.....-:•:'":::::-"-'::•':'":':'-:...:•"-:'"" .''" .::':9-•"* .'::'•':-•:..5•
Recommended publications
  • Protecting & Preserving Apollo Program Lunar Landing Sites
    PROTECTING & PRESERVING APOLLO PROGRAM LUNAR LANDING SITES & ARTIFACTS In accordance with the NASA TRANSITION AUTHORIZATION ACT OF 2017 Product of the OFFICE OF SCIENCE AND TECHNOLOGY POLICY MARCH 2018 PROTECTING & PRESERVING APOLLO PROGRAM LUNAR LANDING SITES & ARTIFACTS Background The Moon continues to hold great significance around the world. The successes of the Apollo missions still represent a profound human technological achievement almost 50 years later and continue to symbolize the pride of the only nation to send humans to an extraterrestrial body. The Apollo missions reflect the depth and scope of human imagination and the desire to push the boundaries of humankind’s existence. The Apollo landing sites and the accomplishments of our early space explorers energized our Nation's technological prowess, inspired generations of students, and greatly contributed to the worldwide scientific understanding of the Moon and our Solar System. Additionally, other countries have placed hardware on the Moon which undoubtedly has similar historic, cultural, and scientific value to their country and to humanity. Three Apollo sites remain scientifically active and all the landing sites provide the opportunity to learn about the changes associated with long-term exposure of human-created systems in the harsh lunar environment. These sites offer rich opportunities for biological, physical, and material sciences. Future visits to the Moon’s surface offer opportunities to study the effects of long-term exposure to the lunar environment on materials and articles, including food left behind, paint, nylon, rubber, and metals. Currently, very little data exist that describe what effect temperature extremes, lunar dust, micrometeoroids, solar radiation, etc.
    [Show full text]
  • Mapping the Surveyor III Crater Large-Scale Maps May Be Produced from Lunar Oribiter Photographs
    FIG. 1. The Surveyor I II Crater. CHARLES W. SHULL t LYNN A. SCHENK U. S. Army TOPOCOM Washington, D. C.20315 Mapping the Surveyor III Crater large-scale maps may be produced from lunar Oribiter photographs (Abstract on next page) INRODUCTlON Because of the inclination of the camera, lunar features were viewed more clearly than URVEYOR III spacecraft was launched Son April 17, 1967 toward the moon on a would have been possible on flat terrain. mission to explore possible Apollo landing This crater, then, became an object of in­ sites. On April 19 the Surveyor landed on the tense interest to the scientific community, moon's Ocean of Storms and almost imme­ especially to astrogeologists who had the diately began transmitting television pictures unique opportunity of observing high quality back to Earth. When the lunar day ended pictures of the interior of a lunar crater for on May 3, over 6,300 photographs had been the first time. Because of this unusual characteristic, the received from Surveyor III by the Jet Pro­ pulsion Laboratory.* ational Aeronautics and Space Administra­ vVhen the spacecraft landed, it came to tion (NASA) requested that the Department of Defense prepare two maps of the crater rest on the inside slope of crater giving it a 12.40 tilt from the local vertical (Figure 1). and surrounding areas. The request was for a photo mosaic at 1 :2,000 scale with 10-meter t Presented at the Annual Convention of the contours and a shaded relief map with con­ American Society of Photogrammetry in Washing­ tours at the smallest interval possible.
    [Show full text]
  • 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.
    [Show full text]
  • 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.
    [Show full text]
  • Photographs Written Historical and Descriptive
    CAPE CANAVERAL AIR FORCE STATION, MISSILE ASSEMBLY HAER FL-8-B BUILDING AE HAER FL-8-B (John F. Kennedy Space Center, Hanger AE) Cape Canaveral Brevard County Florida PHOTOGRAPHS WRITTEN HISTORICAL AND DESCRIPTIVE DATA HISTORIC AMERICAN ENGINEERING RECORD SOUTHEAST REGIONAL OFFICE National Park Service U.S. Department of the Interior 100 Alabama St. NW Atlanta, GA 30303 HISTORIC AMERICAN ENGINEERING RECORD CAPE CANAVERAL AIR FORCE STATION, MISSILE ASSEMBLY BUILDING AE (Hangar AE) HAER NO. FL-8-B Location: Hangar Road, Cape Canaveral Air Force Station (CCAFS), Industrial Area, Brevard County, Florida. USGS Cape Canaveral, Florida, Quadrangle. Universal Transverse Mercator Coordinates: E 540610 N 3151547, Zone 17, NAD 1983. Date of Construction: 1959 Present Owner: National Aeronautics and Space Administration (NASA) Present Use: Home to NASA’s Launch Services Program (LSP) and the Launch Vehicle Data Center (LVDC). The LVDC allows engineers to monitor telemetry data during unmanned rocket launches. Significance: Missile Assembly Building AE, commonly called Hangar AE, is nationally significant as the telemetry station for NASA KSC’s unmanned Expendable Launch Vehicle (ELV) program. Since 1961, the building has been the principal facility for monitoring telemetry communications data during ELV launches and until 1995 it processed scientifically significant ELV satellite payloads. Still in operation, Hangar AE is essential to the continuing mission and success of NASA’s unmanned rocket launch program at KSC. It is eligible for listing on the National Register of Historic Places (NRHP) under Criterion A in the area of Space Exploration as Kennedy Space Center’s (KSC) original Mission Control Center for its program of unmanned launch missions and under Criterion C as a contributing resource in the CCAFS Industrial Area Historic District.
    [Show full text]
  • 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.
    [Show full text]
  • Apollo Space Suit
    APOLLO SPACE S UIT 1962–1974 Frederica, Delaware A HISTORIC MECHANICAL ENGINEERING LANDMARK SEPTEMBER 20, 2013 DelMarVa Subsection Histor y of the Apollo Space Suit This model would be used on Apollo 7 through Apollo 14 including the first lunar mission of Neil Armstrong and Buzz International Latex Corporation (ILC) was founded in Aldrin on Apollo 11. Further design improvements were made to Dover, Delaware in 1937 by Abram Nathanial Spanel. Mr. Spanel improve mobility for astronauts on Apollo 15 through 17 who was an inventor who became proficient at dipping latex material needed to sit in the lunar rovers and perform more advanced to form bathing caps and other commercial products. He became mobility exercises on the lunar surface. This suit was known as famous for ladies apparel made under the brand name of Playtex the model A7LB. A slightly modified ILC Apollo suit would also go that today is known worldwide. Throughout WWII, Spanel drove on to support the Skylab program and finally the American-Soyuz the development and manufacture of military rubberized products Test Program (ASTP) which concluded in 1975. During the entire to help our troops. In 1947, Spanel used the small group known time the Apollo suit was produced, manufacturing was performed as the Metals Division to develop military products including at both the ILC plant on Pear Street in Dover, Delaware, as well as several popular pressure helmets for the U.S. Air Force. the ILC facility in Frederica, Delaware. In 1975, the Dover facility Based upon the success of the pressure helmets, the Metals was closed and all operations were moved to the Frederica plant.
    [Show full text]
  • Gao-21-306, Nasa
    United States Government Accountability Office Report to Congressional Committees May 2021 NASA Assessments of Major Projects GAO-21-306 May 2021 NASA Assessments of Major Projects Highlights of GAO-21-306, a report to congressional committees Why GAO Did This Study What GAO Found This report provides a snapshot of how The National Aeronautics and Space Administration’s (NASA) portfolio of major well NASA is planning and executing projects in the development stage of the acquisition process continues to its major projects, which are those with experience cost increases and schedule delays. This marks the fifth year in a row costs of over $250 million. NASA plans that cumulative cost and schedule performance deteriorated (see figure). The to invest at least $69 billion in its major cumulative cost growth is currently $9.6 billion, driven by nine projects; however, projects to continue exploring Earth $7.1 billion of this cost growth stems from two projects—the James Webb Space and the solar system. Telescope and the Space Launch System. These two projects account for about Congressional conferees included a half of the cumulative schedule delays. The portfolio also continues to grow, with provision for GAO to prepare status more projects expected to reach development in the next year. reports on selected large-scale NASA programs, projects, and activities. This Cumulative Cost and Schedule Performance for NASA’s Major Projects in Development is GAO’s 13th annual assessment. This report assesses (1) the cost and schedule performance of NASA’s major projects, including the effects of COVID-19; and (2) the development and maturity of technologies and progress in achieving design stability.
    [Show full text]
  • Surveyor 1 Space- Craft on June 2, 1966 As Seen by the Narrow Angle Camera of the Lunar Re- Connaissance Orbiter Taken on July 17, 2009 (Also See Fig
    i “Project Surveyor, in particular, removed any doubt that it was possible for Americans to land on the Moon and explore its surface.” — Harrison H. Schmitt, Apollo 17 Scientist-Astronaut ii Frontispiece: Landing site of the Surveyor 1 space- craft on June 2, 1966 as seen by the narrow angle camera of the Lunar Re- connaissance Orbiter taken on July 17, 2009 (also see Fig. 13). The white square in the upper photo outlines the area of the enlarged view below. The spacecraft is ca. 3.3 m tall and is casting a 15 m shadow to the East. (NASA/LROC/ ASU/GSFC photos) iii iv Surveyor I: America’s First Moon Landing by William F. Mellberg v © 2014, 2015 William F. Mellberg vi About the author: William Mellberg was a marketing and public relations representative with Fokker Aircraft. He is also an aerospace historian, having published many articles on both the development of airplanes and space vehicles in various magazines. He is the author of Famous Airliners and Moon Missions. He also serves as co-Editor of Harrison H. Schmitt’s website: http://americasuncommonsense.com Acknowledgments: The support and recollections of Frank Mellberg, Harrison Schmitt, Justin Rennilson, Alexander Gurshstein, Paul Spudis, Ronald Wells, Colin Mackellar and Dwight Steven- Boniecki is gratefully acknowledged. vii Surveyor I: America’s First Moon Landing by William F. Mellberg A Journey of 250,000 Miles . December 14, 2013. China’s Chang’e 3 spacecraft successfully touched down on the Moon at 1311 GMT (2111 Beijing Time). The landing site was in Mare Imbrium, the Sea of Rains, about 25 miles (40 km) south of the small crater, Laplace F, and roughly 100 miles (160 km) east of its original target in Sinus Iridum, the Bay of Rainbows.
    [Show full text]
  • Surveyor Ill Mission Report Part I
    \ NAT IONAL AERONAUT ICS AND SPAC E ADMIN ISTRATION Technical Report 32-1177 Surveyor Ill Mission Report Part I. Mission Description and Performance JET PROPULSION LAB ORATOR Y CALIFORNIA INS TITUTE OF TECHNOLOGY PASAD E NA, CALIFORNIA September 1, 1967 NAT IONAL AERONA UT ICS AND SPAC E AD MINISTRAT ION Technical Report 32-1177 Surveyor Ill Mission Report Part I. Mission Description and Performance Approved for publication by: H. H. Haglund Surveyor Project Manager JET PROPULSION LAB ORA TOR Y CAL I FORNIA INSTITUTE OF TECHNOLO GY PASAD E NA, CAL I FORNI A September 1, 1967 TECHNICAL REPORT 32-1 177 Copyright © 7 196 Jet Propulsion laboratory California Institute of Technology Prepared Under Contract No. NAS 7-100 National Aeronautics Space Administration & Preface This three-part document constitutes the Surveyor III Mission Report. It describes the third in a series of unmanned missions designed to soft-land on the moon and return data from the lunar surface. Part I of this report consists of a technical description and an evaluation of engineering results of the systems utilized in the Surveyor III mission. Analysis of the data received from the Surveyor III mission is continuing, and it is expected that additional results will be obtained together with some improvement in accuracy. Part I was compiled using the contributions of many individuals in the major systems which support the Project. Some of the information for this report was obtained from other published documents; a list of these documents is con­ tained in a bibliography. Part II of this report presents the scientific data derived from the mission and the results of scientific analyses which have been conducted.
    [Show full text]
  • Open Research Online Oro.Open.Ac.Uk
    Open Research Online The Open University’s repository of research publications and other research outputs Analysis of Lunar Boulder Tracks: Implications for Trafficability of Pyroclastic Deposits Journal Item How to cite: Bickel, V. T.; Honniball, C. I.; Martinez, S. N.; Rogaski, A.; Sargeant, Hannah; Bell, S. K.; Czaplinski, E. C.; Farrant, B. E.; Harrington, E. M.; Tolometti, G. D. and Kring, D. A. (2019). Analysis of Lunar Boulder Tracks: Implications for Trafficability of Pyroclastic Deposits. Journal of Geophysical Research: Planets, 124(5) pp. 1296–1314. For guidance on citations see FAQs. c 2019 American Geophysical Union https://creativecommons.org/licenses/by-nc-nd/4.0/ Version: Version of Record Link(s) to article on publisher’s website: http://dx.doi.org/doi:10.1029/2018JE005876 Copyright and Moral Rights for the articles on this site are retained by the individual authors and/or other copyright owners. For more information on Open Research Online’s data policy on reuse of materials please consult the policies page. oro.open.ac.uk RESEARCH ARTICLE Analysis of Lunar Boulder Tracks: Implications 10.1029/2018JE005876 for Trafficability of Pyroclastic Deposits Key Points: V. T. Bickel1,2 , C. I. Honniball3, S. N. Martinez4, A. Rogaski5, H. M. Sargeant6, S. K. Bell7, • Bearing capacity of pyroclastic, 8 7 9 9 10,11 mare, and highland regions is E. C. Czaplinski , B. E. Farrant , E. M. Harrington , G. D. Tolometti , and D. A. Kring calculated based on measurements 1 2 of boulder tracks in orbital images Department Planets & Comets, Max
    [Show full text]
  • Shoot the Moon – 1967
    Video Transcript for Archival Research Catalog (ARC) Identifier 45011 Assignment: Shoot the Moon – 1967 Narrator: The assignment was specific: get photographs of the surface of the Moon that are good enough to determine whether or not it’s safe for a man to land there. But appearances can be deceiving, just as deceiving as trying to get a good picture of, well, a candy apple. Doesn’t seem to be too much of a problem, just set it up, light it, and snap the picture. Easy, quick, simple. But it can be tough. To begin with, the apple is some distance away, so you can’t get to it to just set it up, light it, and so on. To make things even more difficult, it isn’t even holding still; it’s moving around in circles. Now timing is important. You have to take your picture when the apple is nearest to you so you get the most detail and when the light that’s available is at the best angle for the photo. And even that’s not all. You are moving too, in circles. You’re both turning and circling about the apple. Now, about that assignment. As the technology of man in space was developing, it became more and more apparent that our knowledge of the Moon’s surface as a possible landing site was not sufficient. To land man safely on the Moon and get him safely off again, we had to know whether we could set up a precise enough trajectory to reach the Moon.
    [Show full text]