'The UNOCCUPIED MISSION FIELDS of AFRICA and ASIA
Total Page:16
File Type:pdf, Size:1020Kb
Load more
Recommended publications
-
Planetary Geologic Mappers Annual Meeting
Program Lunar and Planetary Institute 3600 Bay Area Boulevard Houston TX 77058-1113 Planetary Geologic Mappers Annual Meeting June 12–14, 2018 • Knoxville, Tennessee Institutional Support Lunar and Planetary Institute Universities Space Research Association Convener Devon Burr Earth and Planetary Sciences Department, University of Tennessee Knoxville Science Organizing Committee David Williams, Chair Arizona State University Devon Burr Earth and Planetary Sciences Department, University of Tennessee Knoxville Robert Jacobsen Earth and Planetary Sciences Department, University of Tennessee Knoxville Bradley Thomson Earth and Planetary Sciences Department, University of Tennessee Knoxville Abstracts for this meeting are available via the meeting website at https://www.hou.usra.edu/meetings/pgm2018/ Abstracts can be cited as Author A. B. and Author C. D. (2018) Title of abstract. In Planetary Geologic Mappers Annual Meeting, Abstract #XXXX. LPI Contribution No. 2066, Lunar and Planetary Institute, Houston. Guide to Sessions Tuesday, June 12, 2018 9:00 a.m. Strong Hall Meeting Room Introduction and Mercury and Venus Maps 1:00 p.m. Strong Hall Meeting Room Mars Maps 5:30 p.m. Strong Hall Poster Area Poster Session: 2018 Planetary Geologic Mappers Meeting Wednesday, June 13, 2018 8:30 a.m. Strong Hall Meeting Room GIS and Planetary Mapping Techniques and Lunar Maps 1:15 p.m. Strong Hall Meeting Room Asteroid, Dwarf Planet, and Outer Planet Satellite Maps Thursday, June 14, 2018 8:30 a.m. Strong Hall Optional Field Trip to Appalachian Mountains Program Tuesday, June 12, 2018 INTRODUCTION AND MERCURY AND VENUS MAPS 9:00 a.m. Strong Hall Meeting Room Chairs: David Williams Devon Burr 9:00 a.m. -
Der Schwarze Tag”
CHAPTER XIV “DER SCHWARZE TAG” ’rHE Australian infantry winding along their numerous approach tracks, constantly passing black silent masses of waiting tanks and crowded guns, were excited with their own realisation of the facts to which Monash’s message referred- that at last all five divisions of their national army were attack- ing together, that the Canadian force was attacking beside them, and that this time they were not to be stopped short of the opposing guns-and also of the elating circumstance that, so far, the enemy showed no awareness of the blow about to fall. The infantry brigades started their approach at different hours, mostly between midnight and 1.30 a.m.; the troops of the two divisions that were to launch the first stages of attack (at 4.20) mostly passed through-and reached their jumping-off tapes before-those of the two divisions for the second objective. These then followed and assembled behind them.’ At 3 a.m. when most units of the leading divisions had thus assembled and lain down, but about half of the two rearward ones were still moving up the tracks close behind them,2 the air became dimmed by a morning mist which quickly thickened until at 3.30 it was difficult to see more than twenty yards on either side. “It was getting too foggy to be pleasant,” said Col. Sadler of the 17th Battalion afterwards describing the assembly. Men of Elliott’s 15th Brigade, then toiling up from Bois 1’AbbC to their starting lines by the brickfield in rear of the Australian right, have told how they were becoming anxious as to their direction when lights were suddenly seen in the mist ahead and there was the number of their battalion, 57, glowing above 1 In some places. -
Martian Crater Morphology
ANALYSIS OF THE DEPTH-DIAMETER RELATIONSHIP OF MARTIAN CRATERS A Capstone Experience Thesis Presented by Jared Howenstine Completion Date: May 2006 Approved By: Professor M. Darby Dyar, Astronomy Professor Christopher Condit, Geology Professor Judith Young, Astronomy Abstract Title: Analysis of the Depth-Diameter Relationship of Martian Craters Author: Jared Howenstine, Astronomy Approved By: Judith Young, Astronomy Approved By: M. Darby Dyar, Astronomy Approved By: Christopher Condit, Geology CE Type: Departmental Honors Project Using a gridded version of maritan topography with the computer program Gridview, this project studied the depth-diameter relationship of martian impact craters. The work encompasses 361 profiles of impacts with diameters larger than 15 kilometers and is a continuation of work that was started at the Lunar and Planetary Institute in Houston, Texas under the guidance of Dr. Walter S. Keifer. Using the most ‘pristine,’ or deepest craters in the data a depth-diameter relationship was determined: d = 0.610D 0.327 , where d is the depth of the crater and D is the diameter of the crater, both in kilometers. This relationship can then be used to estimate the theoretical depth of any impact radius, and therefore can be used to estimate the pristine shape of the crater. With a depth-diameter ratio for a particular crater, the measured depth can then be compared to this theoretical value and an estimate of the amount of material within the crater, or fill, can then be calculated. The data includes 140 named impact craters, 3 basins, and 218 other impacts. The named data encompasses all named impact structures of greater than 100 kilometers in diameter. -
Download Just Choose the Ones I Can Afford and Take to Have Some Grasp of Whereabouts in the and Own – Any Big Finish Production
WWW.BIGFINISH.COM • NEW AUDIO ADVENTURES REUNITING THE REBELS IN WARSHIP WHAT’S IN STORE IN GALLIFREY V ISSUE 48 • FEBRUARY 2013 ANIMATING THE REIGN OF TERROR PLUS CHASE MASTERSON DISCUSSES VIENNA VORTEX MAGAZINE | PAGE 1 VORTEX MAGAZINE | PAGE 2 SNEAK PREVIEWS EDITORIAL AND WHISPERS ello! You were expecting Nick Briggs weren’t you? I’m H afraid he’s in a booth at the minute, hissing and growling. This is not a condition brought on by overwork… Oh no, he’s back in the armour of an Ice Warrior, acting away for the recording of Doctor Who – The Lost Stories: Lords of the Red Planet. The six-part story, which was originally devised by Brian Hayles for TV back in 1968, will be out on audio in November – and form another part of Big Finish’s massive fiftieth anniversary celebrations. And what celebrations they will be! As I write, we’re well into recording our multi-Doctor special The Light at the End, and it’s been a blast. Admittedly it’s been strange to DOCTOR WHO: THE LIGHT AT THE END see the Doctors in the studio at the same time. We’re so used to them being in separately, and suddenly they’re ‘We want something special from Big Finish for here together! But there’s been a real sense of this being the fiftieth anniversary,’ they said. a massive party – the green room chatter has been really We like a challenge, so we went to town jolly and vibrant. It’s so nice to see that all these actors love with this one – eight Doctors (yes, incarnations Doctor Who just as much as we do. -
Journey to Southern Zanskar Trekking -NEC Travels and Tours
Journey to Southern Zanskar Trekking https://www.nectravels.com/package/journey-to-southern-zanskar/ Trekking is a popular adventure sport in India and has attracted many enthusiasts across the nation and the globe. India is home to some of the most dangerous and challenging mountainous terrains and valleys which are full of scenic and ethereal beauty. These mountain ranges are hotspots for trekking expeditions providing the chills and frills of an adventurous journey. Unmatched in their flora and fauna these high altitude terrains are worth visiting at least once in a life time. People who love to experience strenuous ventures and unexplored territories must try out exploring the Ladakh region situated in the North-Easter region of Jammu and Kashmir. Zanskar is an inviting mountaineering destination that will not only test your physical and mental limits but it is also an opportunity to tread in to the serene uncharted territories, places where very few men have set foot and also a chance to conquer the massive mountains by scaling high altitude peaks. Southern Zanskar with its vivid ecology, cascading waterfalls, silent valleys, clear rivers and snow covered peaks guarantees to be one of your finest trekking experiences. Zanskar is located in the eastern part of Jammu and Kashmir along the banks of the river Zanskar at an average altitude of 3500m-7000m. Its geography is scattered with passes and valleys like the Shingo la which locals say is one of the most thankless and sordid routes with no natural grandeur. In the north eastern part of Zanskar lies the Zanskar mountain range where a variety of wildlife like the snow leopard, bear, white yak, ibex etc are in abundance. -
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, -
Orbital Evidence for More Widespread Carbonate- 10.1002/2015JE004972 Bearing Rocks on Mars Key Point: James J
PUBLICATIONS Journal of Geophysical Research: Planets RESEARCH ARTICLE Orbital evidence for more widespread carbonate- 10.1002/2015JE004972 bearing rocks on Mars Key Point: James J. Wray1, Scott L. Murchie2, Janice L. Bishop3, Bethany L. Ehlmann4, Ralph E. Milliken5, • Carbonates coexist with phyllosili- 1 2 6 cates in exhumed Noachian rocks in Mary Beth Wilhelm , Kimberly D. Seelos , and Matthew Chojnacki several regions of Mars 1School of Earth and Atmospheric Sciences, Georgia Institute of Technology, Atlanta, Georgia, USA, 2The Johns Hopkins University/Applied Physics Laboratory, Laurel, Maryland, USA, 3SETI Institute, Mountain View, California, USA, 4Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, California, USA, 5Department of Geological Sciences, Brown Correspondence to: University, Providence, Rhode Island, USA, 6Lunar and Planetary Laboratory, University of Arizona, Tucson, Arizona, USA J. J. Wray, [email protected] Abstract Carbonates are key minerals for understanding ancient Martian environments because they Citation: are indicators of potentially habitable, neutral-to-alkaline water and may be an important reservoir for Wray, J. J., S. L. Murchie, J. L. Bishop, paleoatmospheric CO2. Previous remote sensing studies have identified mostly Mg-rich carbonates, both in B. L. Ehlmann, R. E. Milliken, M. B. Wilhelm, Martian dust and in a Late Noachian rock unit circumferential to the Isidis basin. Here we report evidence for older K. D. Seelos, and M. Chojnacki (2016), Orbital evidence for more widespread Fe- and/or Ca-rich carbonates exposed from the subsurface by impact craters and troughs. These carbonates carbonate-bearing rocks on Mars, are found in and around the Huygens basin northwest of Hellas, in western Noachis Terra between the Argyre – J. -
Observations of the Marker Bed at Gale Crater with Recommendations for Future Exploration by the Curiosity Rover
52nd Lunar and Planetary Science Conference 2021 (LPI Contrib. No. 2548) 1484.pdf OBSERVATIONS OF THE MARKER BED AT GALE CRATER WITH RECOMMENDATIONS FOR FUTURE EXPLORATION BY THE CURIOSITY ROVER. C. M. Weitz1, J. L. Bishop2, B. J. Thomson3, K. D. Seelos4, K. Lewis5, I. Ettenborough3, and R. E. Arvidson6. 1Planetary Science Institute, 1700 East Fort Lowell, Tuc- son, AZ ([email protected]); 2SETI Institute, Carl Sagan Center, Mountain View, CA; 3Dept. of Earth and Planetary Sciences, Univ. Tennessee, Knoxville, TN; 4Planetary Exploration Group, JHU Applied Physics Laboratory, Laurel, MD; 5Dept Earth and Planetary Sciences, John Hopkins University, Baltimore, MD; 6Dept Earth and Planetary Sci- ences, Washington University, St. Louis, Missouri. Introduction: A dark-toned marker bed is ob- pearance across the mound. Most of the sulfates served within the sulfates at Gale crater [1,2]. This above/below the marker bed are stratified, heavily marker bed is characterized by a dark-toned, smooth fractured, and erode into boulder-size blocks, but there surface that appears more indurated and retains more are examples where the sulfates appear massive with craters relative to the sulfate-bearing layers above and limited fracturing and no boulders eroding from the below it. The bed has a distinct physical appearance unit (Fig. 3a). from the sulfates in which it occurs, suggesting a change in the environment or geochemistry for a brief period of time within the depositional sequence that formed the sulfates or post-deposition alteration. In this study, we utilized HiRISE and CTX images to identify and map the occurrence of the marker bed throughout Aeolis Mons. -
1 Jonathan Demenge
Jonathan Demenge (IDS, Brighton) In the Shadow of Zanskar: The Life of a Nepali Migrant Published in Ladakh Studies, July 2009 This article is a tribute to Thinle, a Nepali worker who died last September (2008) in Chilling. He was a driller working on the construction of the road between Nimu and Padum, along the Zanskar River. Like most other similar stories, the story of Thinle could have remained undocumented, mainly because migrants’ presence in Ladakh remains widely unstudied. The story of Thinle has a lot to tell about the living conditions of migrants who build the roads in Ladakh, their relationship to the environment – physical and imagined – and their relationship to danger. Starting from the biography of a man and his family, I attempt to understand the larger social matrix in which this history is embedded. Using the concept of structural violence (Galtung 1969; Farmer 1997; 2004) I try to shed light on the wider socio-political forces at work in this tragedy. At the same time I point to a striking reality: despite the long and important presence of working migrants in Ladakh, they remain unstudied. In spite of their substantial contribution to Ladakh’s history and development, both literally and figuratively, in the field and in the literature, migrants remain at the margin, or in the shade. The life of Thinle Sherpa I started researching road construction and road workers in Ladakh about three years ago. Thinle was one of the workers I learnt to know while I was conducting fieldwork in Chilling. Thinle and his family were very engaging people, and those who met them will surely remember them. -
Pre-Mission Insights on the Interior of Mars Suzanne E
Pre-mission InSights on the Interior of Mars Suzanne E. Smrekar, Philippe Lognonné, Tilman Spohn, W. Bruce Banerdt, Doris Breuer, Ulrich Christensen, Véronique Dehant, Mélanie Drilleau, William Folkner, Nobuaki Fuji, et al. To cite this version: Suzanne E. Smrekar, Philippe Lognonné, Tilman Spohn, W. Bruce Banerdt, Doris Breuer, et al.. Pre-mission InSights on the Interior of Mars. Space Science Reviews, Springer Verlag, 2019, 215 (1), pp.1-72. 10.1007/s11214-018-0563-9. hal-01990798 HAL Id: hal-01990798 https://hal.archives-ouvertes.fr/hal-01990798 Submitted on 23 Jan 2019 HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. Open Archive Toulouse Archive Ouverte (OATAO ) OATAO is an open access repository that collects the wor of some Toulouse researchers and ma es it freely available over the web where possible. This is an author's version published in: https://oatao.univ-toulouse.fr/21690 Official URL : https://doi.org/10.1007/s11214-018-0563-9 To cite this version : Smrekar, Suzanne E. and Lognonné, Philippe and Spohn, Tilman ,... [et al.]. Pre-mission InSights on the Interior of Mars. (2019) Space Science Reviews, 215 (1). -
2000 Ladakh and Zanskar-The Land of Passes
1 LADAKH AND ZANSKAR -THE LAND OF PASSES The great mountains are quick to kill or maim when mistakes are made. Surely, a safe descent is as much a part of the climb as “getting to the top”. Dead men are successful only when they have given their lives for others. Kenneth Mason, Abode of Snow (p. 289) The remote and isolated region of Ladakh lies in the state of Jammu and Kashmir, marking the western limit of the spread of Tibetan culture. Before it became a part of India in the 1834, when the rulers of Jammu brought it under their control, Ladakh was an independent kingdom closely linked with Tibet, its strong Buddhist culture and its various gompas (monasteries) such as Lamayuru, Alchi and Thiksey a living testimony to this fact. One of the most prominent monuments is the towering palace in Leh, built by the Ladakhi ruler, Singe Namgyal (c. 1570 to 1642). Ladakh’s inhospitable terrain has seen enough traders, missionaries and invading armies to justify the Ladakhi saying: “The land is so barren and the passes are so high that only the best of friends or worst of enemies would want to visit us.” The elevation of Ladakh gives it an extreme climate; burning heat by day and freezing cold at night. Due to the rarefied atmosphere, the sun’s rays heat the ground quickly, the dry air allowing for quick cooling, leading to sub-zero temperatures at night. Lying in the rain- shadow of the Great Himalaya, this arid, bare region receives scanty rainfall, and its primary source of water is the winter snowfall. -
Cartes De Trekking LADAKH & ZANSKAR Trekking Maps
Cartes de trekking LADAKH & ZANSKAR Trekking Maps Index des noms de lieux Index of place names NORTH CENTER SOUTH abram pointet www.abram.ch Ladakh & Zanskar Cartes de trekking / Trekking Maps Editions Olizane A Arvat E 27 Bhardas La C 18 Burma P 11 Abadon B 1 Arzu N 11 Bhator D 24 Burshung O 19 Abale O 5 Arzu N 11 Bhutna A 19 C Abran … Abrang Arzu Lha Khang N 11 Biachuthasa A 7 Cerro Kishtwar C 19 Abrang C 16 Ashur Togpo H 8 Biachuthusa … Biachuthasa Cha H 20 Abuntse D 7 Askuta F 11 Biadangdo G 3 Cha H 20 Achina Lungba D 6 Askuta Togpo F 11 Biagdang Gl. G 2 Cha Gonpa H 20 Achina Lungba Gonpa D 6 Ating E 17 Biama … Beama Chacha Got C 26 Achina Thang C 7 Ayi K 3 Biar Malera A 24 Chacham Togpo K 14 Achina Thang Gonpa D 7 Ayu M 11 Biarsak F 2 Chachatapsa D 7 Achinatung … Achina Thang B Bibcha F 19 Chagangle V 24 Achirik I 11 Bagioth F 27 Bibcha Lha Khang F 19 Chagar Tso S 12 Achirik Lha Khang I 11 Bahai Nala B 22 Bidrabani Sarai A 22 Chagarchan La U 24 Agcho C 15 Baihali Jot C 25 Bilargu D 5 Chagdo W 9 Agham O 8 Bakartse C 16 Billing Nala G 27 Chaghacha E 9 Agsho B 17 Bakula Bao I 13 Bima E 27 Chaglung C 7 Agsho Gl. B 17 Baldar Gl. B 13 Birshungle V 26 Chagra U 11 Agsho La B 17 Baldes B 5 Bishitao A 22 Chagra U 11 Agyasol A 19 Baleli Jot E 22 Bishur B 25 Chagri F 9 Ajangliung J 7 Balhai Nala C 25 Bod Kharbu C 8 Chagtsang M 15 Akeke R 18 Balthal Got C 26 Bog I 27 Chagtsang La M 15 Akling L 11 Bangche Togpo G 15 Bokakphule V 27 Chakharung B 5 Aksaï Chin V 10 Bangche Togpo F 14 Boksar Gongma F 13 Chakrate T 16 Alam H 12 Bangongsho X 16 Boksar Yokma G 13 Chali Gali E 27 Alchi I 10 Banku G 8 Bolam L 11 Chaluk J 13 Alchi H 10 Banon D 23 Bong La M 21 Chalung U 21 Alchi Brok H 10 Banraj Gl.