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Monadnock Vol. 45 | June 1971
THE MONADNOCK I - L. .RK UNIVERSITY Vol. XLV )GRAPHICAL SOCIETY June, 1971 THE MQNADNOCK Volume XIN Editor, Edwin T. Wei5e, Jr. Aaooite Editor5 James FOnSeOa Kirsten Haring David Seairøn Photoqzapher, Ernie Wight ypists Ronnie Mason Phyllis sczynski 323812 ii ‘7f THE MONADNOCK CONTENTs . 2 DIRECT0I MESSAGE THE JESUITS IN NORTH AMERICA: A STUDY . IN ENVIRONMENTAL COCEUALIZATI Eenry Aay 4 STRUCTURE IN TRANSACTION SYSTEMS. .Christopher Clayton 9 CULTURE AND AGRICULTURE ON THE ANEPJCAN NTIER Brad Baltensperger 22 THE PROBABILISTIC APPROACH TO SPATIAL THEORY Kang-tsung Chang 30 AROHITECTURE AND GEOGRAPHICAL STUDIES: A REVIEW Stephen Hobart 36 AN ESSAY ON GROWTH POLE THEORY B. David Miller 40 MIND, MEANING, AND MILIEU: PSYCHOLOGICAL NEED AND DESIGRED ENVIRONMENTS Ernest A. Wight Jr 43 SPATIAL DYNAMICS IN CLASSICAL LOCATION THEORY Alfred Hecht 52 THE GRADUATE SCHOOL OF GEOGRAPHY 56 ALUMNI NEWS 65 A N(YTE ON THE QUESTIONNAIRE 80 :1 DIRECTOR’S MESSAGE This academic year is very special for Geography at Clark, marking the fiftieth year of the founding of the Graduate School of Geography by Wallace W. Atwood. Dedication of the new Geography facilities — with special recognition to the memory of John K. Wright, Historical Geographer and Geosophist, an adopted son of Clark — is one appropriate mode of celebration. Another mark of the occasion is the honor accorded to two major figures in American Geography: Clark could not have chosen two more distinguished geographers than Richard Hartshorne and Samuel Van Valkenburg on whom were bestowed .1 . - Honorary Doctorates of Law at the anniversary ceremonies of April .17th. Very different in their contributions and their characters, Richard Hartshorne provided American geography with its philosophic and method ological rationale and Dr. -
Crater Lake Reflections Summer-Fall 2018
Crater Lake National Park National Park Service Crater Lake U.S. Department of the Interior Refections Visitor Guide Summer/Fall 2018 Park News 2 ... Camping, Lodging, Food Discovering Crater Lake 3 ... Ranger Programs f Water Restrictions in Effect Please help us conserve water during 12 Great Ways to Enjoy Your Stay 4 ... Hiking Trails your visit. In March, the state of 5 ... Driving Map Oregon declared a drought emergency The frst European-American to see Crater Lake was lucky to ... In the News: Bull Trout for our county. In 8 of the past 10 survive the experience. On June 12, 1853, gold prospector John 6 years, the park has received less snow Wesley Hillman was riding his mule up a long, sloping mountain. 7 ... Feature Article: Lake Level than normal. Last winter’s snow total He was lost, tired, and not paying attention to the terrain ahead. was 15 feet below average. While 8 ... Climate Chart Suddenly, his mule stopped. Hillman sat up and found himself you’re here, please take short showers, on the edge of a clif, gazing in astonishment at “the bluest and don’t run the tap, and reuse towels most beautiful body of water I had ever seen.” He added: “If and sheets if staying overnight in park Look Inside! I had been riding a blind mule, I frmly believe I would have lodging. Thanks for your help! ridden over the edge to death and destruction.” f Leave Your Drone at Home While mules—no matter how sharp their eyesight—are no longer Operating remote-controlled aircraft permitted to approach the rim of Crater Lake, there are many in the park is prohibited. -
Geoscience and a Lunar Base
" t N_iSA Conference Pubhcatmn 3070 " i J Geoscience and a Lunar Base A Comprehensive Plan for Lunar Explora, tion unclas HI/VI 02907_4 at ,unar | !' / | .... ._-.;} / [ | -- --_,,,_-_ |,, |, • • |,_nrrr|l , .l -- - -- - ....... = F _: .......... s_ dd]T_- ! JL --_ - - _ '- "_r: °-__.......... / _r NASA Conference Publication 3070 Geoscience and a Lunar Base A Comprehensive Plan for Lunar Exploration Edited by G. Jeffrey Taylor Institute of Meteoritics University of New Mexico Albuquerque, New Mexico Paul D. Spudis U.S. Geological Survey Branch of Astrogeology Flagstaff, Arizona Proceedings of a workshop sponsored by the National Aeronautics and Space Administration, Washington, D.C., and held at the Lunar and Planetary Institute Houston, Texas August 25-26, 1988 IW_A National Aeronautics and Space Administration Office of Management Scientific and Technical Information Division 1990 PREFACE This report was produced at the request of Dr. Michael B. Duke, Director of the Solar System Exploration Division of the NASA Johnson Space Center. At a meeting of the Lunar and Planetary Sample Team (LAPST), Dr. Duke (at the time also Science Director of the Office of Exploration, NASA Headquarters) suggested that future lunar geoscience activities had not been planned systematically and that geoscience goals for the lunar base program were not articulated well. LAPST is a panel that advises NASA on lunar sample allocations and also serves as an advocate for lunar science within the planetary science community. LAPST took it upon itself to organize some formal geoscience planning for a lunar base by creating a document that outlines the types of missions and activities that are needed to understand the Moon and its geologic history. -
Qiao Et Al., Sosigenes Pit Crater Age 1/51
Qiao et al., Sosigenes pit crater age 1 2 The role of substrate characteristics in producing anomalously young crater 3 retention ages in volcanic deposits on the Moon: Morphology, topography, 4 sub-resolution roughness and mode of emplacement of the Sosigenes Lunar 5 Irregular Mare Patch (IMP) 6 7 Le QIAO1,2,*, James W. HEAD2, Long XIAO1, Lionel WILSON3, and Josef D. 8 DUFEK4 9 1Planetary Science Institute, School of Earth Sciences, China University of 10 Geosciences, Wuhan 430074, China. 11 2Department of Earth, Environmental and Planetary Sciences, Brown University, 12 Providence, RI 02912, USA. 13 3Lancaster Environment Centre, Lancaster University, Lancaster LA1 4YQ, UK. 14 4School of Earth and Atmospheric Sciences, Georgia Institute of Technology, Atlanta, 15 Georgia 30332, USA. 16 *Corresponding author E-mail: [email protected] 17 18 19 20 Key words: Lunar/Moon, Sosigenes, irregular mare patches, mare volcanism, 21 magmatic foam, lava lake, dike emplacement 22 23 24 25 1/51 Qiao et al., Sosigenes pit crater age 26 Abstract: Lunar Irregular Mare Patches (IMPs) are comprised of dozens of small, 27 distinctive and enigmatic lunar mare features. Characterized by their irregular shapes, 28 well-preserved state of relief, apparent optical immaturity and few superposed impact 29 craters, IMPs are interpreted to have been formed or modified geologically very 30 recently (<~100 Ma; Braden et al. 2014). However, their apparent relatively recent 31 formation/modification dates and emplacement mechanisms are debated. We focus in 32 detail on one of the major IMPs, Sosigenes, located in western Mare Tranquillitatis, 33 and dated by Braden et al. -
Glossary Glossary
Glossary Glossary Albedo A measure of an object’s reflectivity. A pure white reflecting surface has an albedo of 1.0 (100%). A pitch-black, nonreflecting surface has an albedo of 0.0. The Moon is a fairly dark object with a combined albedo of 0.07 (reflecting 7% of the sunlight that falls upon it). The albedo range of the lunar maria is between 0.05 and 0.08. The brighter highlands have an albedo range from 0.09 to 0.15. Anorthosite Rocks rich in the mineral feldspar, making up much of the Moon’s bright highland regions. Aperture The diameter of a telescope’s objective lens or primary mirror. Apogee The point in the Moon’s orbit where it is furthest from the Earth. At apogee, the Moon can reach a maximum distance of 406,700 km from the Earth. Apollo The manned lunar program of the United States. Between July 1969 and December 1972, six Apollo missions landed on the Moon, allowing a total of 12 astronauts to explore its surface. Asteroid A minor planet. A large solid body of rock in orbit around the Sun. Banded crater A crater that displays dusky linear tracts on its inner walls and/or floor. 250 Basalt A dark, fine-grained volcanic rock, low in silicon, with a low viscosity. Basaltic material fills many of the Moon’s major basins, especially on the near side. Glossary Basin A very large circular impact structure (usually comprising multiple concentric rings) that usually displays some degree of flooding with lava. The largest and most conspicuous lava- flooded basins on the Moon are found on the near side, and most are filled to their outer edges with mare basalts. -
Planetary Surfaces
Chapter 4 PLANETARY SURFACES 4.1 The Absence of Bedrock A striking and obvious observation is that at full Moon, the lunar surface is bright from limb to limb, with only limited darkening toward the edges. Since this effect is not consistent with the intensity of light reflected from a smooth sphere, pre-Apollo observers concluded that the upper surface was porous on a centimeter scale and had the properties of dust. The thickness of the dust layer was a critical question for landing on the surface. The general view was that a layer a few meters thick of rubble and dust from the meteorite bombardment covered the surface. Alternative views called for kilometer thicknesses of fine dust, filling the maria. The unmanned missions, notably Surveyor, resolved questions about the nature and bearing strength of the surface. However, a somewhat surprising feature of the lunar surface was the completeness of the mantle or blanket of debris. Bedrock exposures are extremely rare, the occurrence in the wall of Hadley Rille (Fig. 6.6) being the only one which was observed closely during the Apollo missions. Fragments of rock excavated during meteorite impact are, of course, common, and provided both samples and evidence of co,mpetent rock layers at shallow levels in the mare basins. Freshly exposed surface material (e.g., bright rays from craters such as Tycho) darken with time due mainly to the production of glass during micro- meteorite impacts. Since some magnetic anomalies correlate with unusually bright regions, the solar wind bombardment (which is strongly deflected by the magnetic anomalies) may also be responsible for darkening the surface [I]. -
National History Bee: Round 3 Tournament Room Division Round Moderator Scorer 3 (Circle 1) V JV
Final Final JV score 35 V 34 33 8 points 32 Division (circle 1) 31 30 . 3 29 28 9 points 27 incorrect interrupt), place running running place incorrect interrupt), rd Round 26 25 24 23 10 points 10 22 21 20 19 Room 18 11 points 11 17 16 15 14 12 pts 13 Scorer 12 13 Make column scoresplace sure the to in forcorrect the question 11 10 14 9 8 7 . 6 ifscore no change. 5 National History Bee: Round 3 History Round Bee: National 4 15 points 15 3 2 1 ) Cross out entire columnCross entire out include school . Remove student from round. In “Final score” column, place student’s total score (refer to the bottom row for the question on which +8 was Remove from was student +8 score” score “Final (referwhich column, In total on round. bottom student’s forplace to the question the row For correct answers, place new running total in student’s row for the corresponding question. For -1’s (3 for question. corresponding the row student’s in total running For correct new place answers, and Cross remainder out of row student’s circle it Moderator full name Total pts for +8 reaching Student namesStudent ( Tournament INSTRUCTIONS: SCORING: and total +8: REACHING reached). NHBB Nationals Bee 2017-2018 Bee Round 3 Bee Round 3 Regulation Questions (1) This empire's naval commanders included the native Dutchman Jan Janszoon. In the 18th century, this empire's capital was briefly taken over by the sailor Patrona Halil. This empire's other naval commanders included Dragut, who served as a galley slave after this empire lost a pivotal battle. -
Hyde Park Historical Record (Vol
' ' HYDE PARK ' ' HISTORICAL RECORD ^ ^ VOLUME IV : 1904 ^ ^ ISe HYDE PARK HISTORICAL SOCIETY j< * HYDE PARK, MASSACHUSETTS * * HYDE PARK HISTORICAL RECORD Volume IV— 1904 PUBLISHED BY THE HYDE PARK HISTORICAL SOCIETY HYDE PARK, MASS. PRESS OF . THE HYDE PARK GAZETTE . 1904 . OFFICERS FOR J904 President Charles G. Chick Recording Secretary Fred L. Johnson Corresponding Secretary and Librarian Henry B. Carrington, 19 Summer Street, Hyde Park, Mass. Treasurer Henry B. Humphrey Editor William A. Mowry, 17 Riverside Square, Hyde Park, Mass. Curators Amos H. Brainard Frank B. Rich George L. Richardson J. Roland Corthell. George L. Stocking Alfred F. Bridgman Charles F. Jenney Henry B, Carrington {ex ofido) CONTENTS OF VOLUME IV. THEODORE DWIGHT WELD 5-32 IVi'lliam Lloyd Garrison, "J-r., Charles G. Chick, Henry B. Carrington, Mrs. Albert B. Bradley, Mrs. Cordelia A. Pay- son, Wilbur H. Po'vers, Francis W. Darling; Edtvard S. Hathazvay. JOHN ELIOT AND THE INDIAN VILLAGE AT NATICK . 33-48 Erastus Worthington. GOING WEST IN 1820. George L. Richardson .... 49-67 EDITORIAL. William A. Mowry 68 JACK FROST (Poem). William A. Mo-vry 69 A HYDE PARK MEMORIAL, 18SS (with Ode) .... 70-75 Henry B- Carrington. HENRY A. RICH 76, 77 William y. Stuart, Robert Bleakie, Henry S. Bunton. DEDICATION OF CAMP MEIGS (1903) 78-91 Henry B. Carrington, Augustus S. Lovett, BetiJ McKendry. PROCEEDINGS OF THE SOCIETY SINCE 1892 . 92-100 Fred L. 'Johnso7i. John B. Bachelder. Henry B- Carrington, Geo. M. Harding, yohn y. E7ineking ..... 94, 95 Gov. F. T. Greenhalge. C. Fred Allen, John H. ONeil . 96 Annual Meeting, 1897. Charles G. -
Science Concept 5: Lunar Volcanism Provides a Window Into the Thermal and Compositional Evolution of the Moon
Science Concept 5: Lunar Volcanism Provides a Window into the Thermal and Compositional Evolution of the Moon Science Concept 5: Lunar volcanism provides a window into the thermal and compositional evolution of the Moon Science Goals: a. Determine the origin and variability of lunar basalts. b. Determine the age of the youngest and oldest mare basalts. c. Determine the compositional range and extent of lunar pyroclastic deposits. d. Determine the flux of lunar volcanism and its evolution through space and time. INTRODUCTION Features of Lunar Volcanism The most prominent volcanic features on the lunar surface are the low albedo mare regions, which cover approximately 17% of the lunar surface (Fig. 5.1). Mare regions are generally considered to be made up of flood basalts, which are the product of highly voluminous basaltic volcanism. On the Moon, such flood basalts typically fill topographically-low impact basins up to 2000 m below the global mean elevation (Wilhelms, 1987). The mare regions are asymmetrically distributed on the lunar surface and cover about 33% of the nearside and only ~3% of the far-side (Wilhelms, 1987). Other volcanic surface features include pyroclastic deposits, domes, and rilles. These features occur on a much smaller scale than the mare flood basalts, but are no less important in understanding lunar volcanism and the internal evolution of the Moon. Table 5.1 outlines different types of volcanic features and their interpreted formational processes. TABLE 5.1 Lunar Volcanic Features Volcanic Feature Interpreted Process -
March 21–25, 2016
FORTY-SEVENTH LUNAR AND PLANETARY SCIENCE CONFERENCE PROGRAM OF TECHNICAL SESSIONS MARCH 21–25, 2016 The Woodlands Waterway Marriott Hotel and Convention Center The Woodlands, Texas INSTITUTIONAL SUPPORT Universities Space Research Association Lunar and Planetary Institute National Aeronautics and Space Administration CONFERENCE CO-CHAIRS Stephen Mackwell, Lunar and Planetary Institute Eileen Stansbery, NASA Johnson Space Center PROGRAM COMMITTEE CHAIRS David Draper, NASA Johnson Space Center Walter Kiefer, Lunar and Planetary Institute PROGRAM COMMITTEE P. Doug Archer, NASA Johnson Space Center Nicolas LeCorvec, Lunar and Planetary Institute Katherine Bermingham, University of Maryland Yo Matsubara, Smithsonian Institute Janice Bishop, SETI and NASA Ames Research Center Francis McCubbin, NASA Johnson Space Center Jeremy Boyce, University of California, Los Angeles Andrew Needham, Carnegie Institution of Washington Lisa Danielson, NASA Johnson Space Center Lan-Anh Nguyen, NASA Johnson Space Center Deepak Dhingra, University of Idaho Paul Niles, NASA Johnson Space Center Stephen Elardo, Carnegie Institution of Washington Dorothy Oehler, NASA Johnson Space Center Marc Fries, NASA Johnson Space Center D. Alex Patthoff, Jet Propulsion Laboratory Cyrena Goodrich, Lunar and Planetary Institute Elizabeth Rampe, Aerodyne Industries, Jacobs JETS at John Gruener, NASA Johnson Space Center NASA Johnson Space Center Justin Hagerty, U.S. Geological Survey Carol Raymond, Jet Propulsion Laboratory Lindsay Hays, Jet Propulsion Laboratory Paul Schenk, -
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. -
Diamond Craters Oregon's Geologic
Text by Ellen M. Benedict, 1985 Features at stops correspond to points on a clock ago, a huge mass of hot gases, volcanic ashes, bits face. Imagine that you are standing in the middle of a of pumice and other pyroclastics (fire-broken rock) Travel And Hiking Hints clock face. Twelve o’clock is the road in front of you violently erupted. The blast – greater than the May and 6 o’clock the road behind. If you always align the 18, 1980, eruption of Mt. St. Helens – deposited a Diamond Craters is located in the high desert country clock face with the road, you should be able to locate layer of pyroclastics 30 to 130 feet thick over an area about 55 miles southeast of Burns, Oregon. It’s an the features. almost 7,000 square miles! isolated place and some precautions should be taken . when traveling in the area. Start Tour. Mileage begins halfway Pyroclastics are between milepost 40 and 41 on State normal behavior Diamond Craters has no tourist facilities. The nearest Highway 205 at the junction to Diamond. for magmas place where gasoline is sold is at Frenchglen. Turn left. (subsurface That’s the opinion held by scores of molten rocks) Keep your scientists and educators who have visited Diamond, Oregon, a small ranching community, was of rhyolitic (a vehicle on named in 1874 for Mace McCoy’s Diamond brand. volcanic material and studied the area. It has the “best and hard-packed The nearby craters soon became known as Diamond related to granite) most diverse basaltic volcanic features in the road surfaces Craters.