Apollo 17 Mission (AS-5 12)
Total Page:16
File Type:pdf, Size:1020Kb
Load more
Recommended publications
-
Subject Index
SUBJECT INDEX Accretion of the Moon Aphelion 34 (chemistry) 419 Apogee 57 Aeronautical Chart and Apollo 5, 8, 596–598, 602, 603, 605 Information Center Apollo 11 30, 609, 611–613 (ACIC) 60 geology 613 Age dating 134 landing site 611, 612 highland rocks 218, 219, 225, 228, 245, 250, Apollo 12 610, 614–616 253, 255, 256 geology 616 mare basalts 208, 209 landing site 614, 615 methods 134, 223 Apollo 14 31, 610, 617–619 Agglutinates 288, 296–299, 301, 339, 414 geology 619 and siderophile elements 414 landing site 617, 618 chemistry 299 Apollo 15 33, 36, 37, 337, 348, 620– description 296 622 F3 model 299 geology 622 genesis 298 heat flow 36, 37 mineralogy 297 landing site 620, 621 native Fe in 154 Apollo 16 32, 341, 351, 623–625, 631 petrography 298 geology 625 physical properties 296 landing site 623, 624 solar-wind elements in 301 Apollo 17 35, 37, 341, 348, 626–628, Akaganeite 150 631 Albedo 59, 558, 560, 561 geology 628 absorption coefficient 561 heat flow 37 Bond albedo 560 landing site 626, 627 geometrical albedo 560 Apollo command module normal albedo 560 experiments 596 scattering coefficient 561 Apollo Lunar Module (LM) 22, 476 single scattering albedo 560 Apollo Lunar Sample Return spherical albedo 560 Containers (ALSRC) 22 Albite 127, 363, 368 Apollo Lunar Sounder Aldrin, Edwin E., Jr. 27–30 Experiment (ALSE) 564 Alkali anorthosite 228, 381, 398, 399 Apollo Self-Recording high strontium, gallium Penetrometer (SRP) 508, 512, 591 content 399 Apollo Simple Penetrometer Alkali gabbro 370 (ASP) 506 Alkali gabbronorite 230, 368 Apollo -
3 2__ Cryptomarcdeposit
/,c, - c/C. ._; 3 2__ _d"/7--- Cryptomare Delineations using Craters as Probes to Lunar Stratigraphy: Use of Multispectral Clementine Data as a Tool; I. Antonenko, J. W. Head, C. M. Pieters. Dept. Geol., Brown Univ., Providence, RI 02912 USA, [email protected]. Hidden mare deposits, or cryptomare, present strong mafic component, and surprisingly, only a evidence of ancient mare volcanism [1], and thus merit portion of the wall of the large subdued crater appears furtherstudy. We have addressed issues of cryptomare to have a strong mafic component. identification [2], and presented techniques for Our analysis can be extended by considering 5- determining cryptomare geometry using dark halo channel spectra taken from key areas in the image. We impact craters (DHCs) which punch through overlying collectedaverage 3X3 pixel spectra for the locations ejecta to excavate underlying mare material [3]. These shown in Fig 1. Representative spectra of fresh techniques have been applied to a study area on the materials, gathered from the slopes of various small western limb of the Moon, using rectified Earth-based craters and in a traverse around the slopes of the large telescopic images and Zond data. The resolution and degraded crater, are shown in Fig 4: Craters whose coverage of these data sets, however, is fairly limiting. spectra exhibit a ferrous absorption feature near 1 gm Furthermore, visual identification of DHCs requires areinterlmm_astapping high-Ca pyroxene-rich that the soils developed on the crater ejecta be material indicating buried basalt (Fig 4A). Those that spectrally mature. The Clemenfine data set, with global exhibit a shorter wavelength absorption or a very weak coverage, improved resolution, and multiple channels, absorption are interpreted as tapping primarily highland presents a new opportunity to expand our studies, material (Fig 4B). -
Shakespeare and Strategy Founder and Contributing Editor: Lyndon H
Executive Intelligence Review EIRJanuary 31, 2014 Vol. 41 No. 5 www.larouchepub.com $10.00 The Empire Lashes Out: Ukraine, Syria, Thailand Declaration of Independence of European Nations Strategic Implications of the Lunar Fusion Revolution Sense & Science, Again: Shakespeare and Strategy Founder and Contributing Editor: Lyndon H. LaRouche, Jr. Editorial Board: Lyndon H. LaRouche, Jr., Antony Papert, Gerald Rose, Dennis Small, Nancy Spannaus, Jeffrey Steinberg, William EI R Wertz Editor: Nancy Spannaus Managing Editor: Susan Welsh Technology Editor: Marsha Freeman From the Managing Editor Book Editor: Katherine Notley Graphics Editor: Alan Yue Photo Editor: Stuart Lewis Circulation Manager: Stanley Ezrol INTELLIGENCE DIRECTORS This week’s magazine is an unusual one. We begin with a “conversa- Counterintelligence: Jeffrey Steinberg, Michele tion” between Lyndon LaRouche and William Shakespeare on grand Steinberg Economics: John Hoefle, Marcia Merry Baker, strategy, and we end with a televised conversation among LaRouche Paul Gallagher History: Anton Chaitkin and his associates Natalie Lovegren and Creighton Jones, on how the Ibero-America: Dennis Small Chinese Moon landing opens the way to a science policy that could Russia and Eastern Europe: Rachel Douglas United States: Debra Freeman save the human race. INTERNATIONAL BUREAUS LaRouche was extremely happy about Lovegren’s report on the Bogotá: Javier Almario Berlin: Rainer Apel helium-3 on the Moon, the fascinating geology (lunology?) in which it Copenhagen: Tom Gillesberg is embedded, and how it can be utilized by man, including for con- Houston: Harley Schlanger Lima: Sara Madueño trolled thermonuclear fusion power. “This is of great strategic signifi- Melbourne: Robert Barwick Mexico City: Gerardo Castilleja Chávez cance,” he exclaimed. -
The Geologic Investigation of the Taurus-Littrow Valley: Apollo 17 Landing Site
The Geologic Investigation of the Taurus-Littrow Valley: Apollo 17 Landing Site GEOLOGICAL SURVEY PROFESSIONAL PAPER 1080 THE GEOLOGIC INVESTIGATION OF THE TAURUS-LITTROW VALLEY: APOLLO 17 LANDING SITE By EDWARD W. WOLFE, NORMAN G. BAILEY, BAERBEL K. LUCCHITTA, WILLIAM R. MUEHLBERGER, DAVID H. SCOTT, ROBERT L. SUTTON, and HOWARD G. WILSHIRE ABSTRACT canic ash form an unconsolidated surficial deposit with an average thickness of about 14 m, sufficiently thick to permit abnormally rapid degradation of the smaller Astronauts Cernan and Schmitt, of Apollo 17, landed in the Taurus-Littrow valley craters, especially those less than 200 m in diameter, so as to create a surface that of the Moon on December 11,1972. Their major objectives were (1) to sample very appears less cratered than other mare surfaces. Admixed volcanic ash gives the ancient lunar material such as might be found in pre-Imbrian highlands as distant as surface a distinctive dark color, which, in combination with the less cratered possible from the Imbrium basin and (2) to sample pyroclastic materials that had appearance, led to its interpretation before the mission as a young dark mantling been interpreted as significantly younger than the mare basalts returned from unit. previous Apollo landing sites. The crew worked approximately 22 hours on the lunar The uppermost part of the regolith over much of the landing area is basalt-rich surface; they traversed about 30 km, collected nearly 120 kg of samples, took more ejects from the clustered craters of the valley floor. Most of the valley-floor craters than 2,200 photographs, and recorded many direct geologic observations.