THE FIFTEENTH GENERAL ASSEMBLY Cassegrairi Telescope
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Chandrayaan-2 Completes a Year Around the Moon
One-year completion of Chandrayaan-2 Lunar orbit insertion (August 20, 2019) Chandrayaan-2 completes a year around the Moon The Moon provides the best linkage to understand Earth’s early history and offers an undisturbed record of the inner Solar system environment. It could also be a base for future human space exploration of the solar system and a unique laboratory, unlike any on Earth, for fundamental physics investigations. In spite of several missions to the Moon, there remains several unanswered questions. Continued high resolution studies of its surface, sub-surface/interior and its low-density exosphere, are essential to address diversities in lunar surface composition and to trace back the origin and evolution of the Moon. The clear evidence from India’s first mission to the Moon, Chandrayaan-1, on the extensive presence of surface water and the indication for sub- surface polar water-ice deposits, argues for more focused studies on the extent of water on the surface, below the surface and in the tenuous lunar exosphere, to address the true origin and availability of water on Moon. With the goal of expanding the lunar scientific knowledge through detailed studies of topography, mineralogy, surface chemical composition, thermo-physical characteristics and the lunar exosphere, Chandrayaan-2 was launched on 22nd July 2019 and inserted into the lunar orbit on 20th August 2019, exactly one year ago. Though the soft-landing attempt was not successful, the orbiter, which was equipped with eight scientific instruments, was successfully placed in the lunar orbit. The orbiter completed more than 4400 orbits around the Moon and all the instruments are currently performing well. -
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. -
General Disclaimer One Or More of the Following Statements May Affect
General Disclaimer One or more of the Following Statements may affect this Document This document has been reproduced from the best copy furnished by the organizational source. It is being released in the interest of making available as much information as possible. This document may contain data, which exceeds the sheet parameters. It was furnished in this condition by the organizational source and is the best copy available. This document may contain tone-on-tone or color graphs, charts and/or pictures, which have been reproduced in black and white. This document is paginated as submitted by the original source. Portions of this document are not fully legible due to the historical nature of some of the material. However, it is the best reproduction available from the original submission. Produced by the NASA Center for Aerospace Information (CASI) ^i e I !emote sousing sad eeolegio Studies of the llaistary Crusts Bernard Ray Hawke Prince-1 Investigator a EL r Z^ .99 University of Hawaii Hawaii Institute of Geophysics Planetary Geosciences Division Honolulu, Hawaii 96822 ^y 1i i W. December 1983 (NASA —CR-173215) REMOTE SENSING AND N84-17092 GEOLOGIC STUDIES OF THE PLANETARY CRUSTS Final Report ( Hawaii Inst. of Geophysics) 14 p HC A02/MF 101 CSCL 03B Unclas G3/91 11715 Gy -2- ©R1GNAL OF POOR QUALITY Table of Contents Page I. Remote Sensing and Geologic Studies cf Volcanic Deposits . • . 3 A. Spectral reflectance studies of dark-haloed craters. • . 3 B. Remote s^:sing studies of regions which were sites of ancient volcanisa . 3 C. [REEP basalt deposits in the Imbrium Region. -
Tourism Snowy Mountains
Attachment 1 Tourism Snowy Briefing Note Mountains Tourism Snowy Mountains Contact Tourism Snowy Mountains Jo Hearne Executive Officer PO Box 663 JINDABYNE NSW 2627 Email [email protected] Phone 02 6457 2751 Mob 0431 247 994 Web www.snowymountains.com.au Tourism Snowy Mountains - overview The role of Tourism Snowy Mountains (TSM) is first and foremost, that of leadership. TSM aims to achieve tourism growth through creating opportunities for the region as a whole. This will be achieved by strong alliances with key industry, regional partners and government stakeholders. TSM has a vision that The Snowy Mountains will be the best mountain experience in Australia The Snowy Mountains region covers the Local Government Areas of: Snowy River Shire, Cooma-Monaro Shire, Tumbarumba Shire and Tumut Shire which encompasses all of Kosciuszko National Park. To deliver on this vision TSM provides leadership and direction to the region by encouraging innovative activities for both marketing and product development that grow visitation. As the peak tourism body in the region TSM has a dual role in promoting the Snowy Mountains Region as having the best mountain experience in Australia. This is achieved by TSM having both an external focus and an operational role. The external focus is to • Lift and maintain the profile of the Snowy Mountains Region with Federal, State and Local Governments and their agencies to ensure that the Snowy Mountains region is top of mind as tourism destination • Be a spokesperson for the Snowy Mountains Region on regional -
CIE Final Report NSW Regional Snowy
FINAL REPORT Economic development in the Snowy SAP Prepared for Department of Regional NSW April 2021 THE CENTRE FOR INTERNATIONAL ECONOMICS www.TheCIE.com.au The Centre for International Economics is a private economic research agency that provides professional, independent and timely analysis of international and domestic events and policies. The CIE’s professional staff arrange, undertake and publish commissioned economic research and analysis for industry, corporations, governments, international agencies and individuals. © Centre for International Economics 2021 This work is copyright. Individuals, agencies and corporations wishing to reproduce this material should contact the Centre for International Economics at one of the following addresses. CANBERRA SYDNEY Centre for International Economics Centre for International Economics Ground Floor, 11 Lancaster Place Level 7, 8 Spring Street Canberra Airport ACT 2609 Sydney NSW 2000 Telephone +61 2 6245 7800 Telephone +61 2 9250 0800 Facsimile +61 2 6245 7888 Email [email protected] Email [email protected] Website www.TheCIE.com.au Website www.TheCIE.com.au DISCLAIMER While the CIE endeavours to provide reliable analysis and believes the material it presents is accurate, it will not be liable for any party acting on such information. Economic development in the Snowy SAP iii Contents Executive summary 1 1 Socio-economic profile of the Snowy Mountains SAP 7 Mapping the Snowy Mountains SAP to current ABS identifiers 7 Labour force analysis 7 Property sales and local development 16 Economic -
Skiing in New South Wales
SKIING IN NEW SOUTH WALES Located within Kosciuszko National Park in the Snowy Mountains, NSW’s four snow resorts – Perisher, Thredbo, Charlotte Pass and Selwyn Snow Resort – each has their own style and personality. The resorts have invested heavily in recent years to extend the Winter snow and make sure skiers and boarders have optimal conditions. All-inclusive deals that bundle accommodation with transport, lift passes and equipment hire are a great way to stretch your dollar. The season generally begins on the June long weekend (the second weekend of the month), with loads of fun events planned throughout the weekend. Now is the time to start planning your Winter holiday – all you have to do is decide where to go. PERISHER The largest ski resort in the southern hemisphere, Perisher covers more than 12 square kilometres across seven peaks and four distinct resort areas – Perisher Valley, Blue Cow, Smiggin Holes and Guthega. It’s great for all ages and abilities with more than 1,200 hectares of skiable terrain, hundreds of runs, 100km of cross country trails, 47 lifts, five terrain parks and two halfpipes. 240 Current as at 8 February 2019 snow cannons ensure there’s a coating of fresh powder for the whole season. The large resort village has lots of places to eat and drink, and other restaurants are spread across the mountains. Once the lifts have closed for the day, there are plenty of welcoming bars and clubs. Enjoy comedy night at the Sundeck Hotel or, for something more refined, you can ski to the piano bar at the Base 1720 Bar and Restaurant or Curve Bar. -
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 -
Australian Alps Education Kit – Teacher's Notes
teacher’s notes for THE AUSTRALIAN ALPS The Australian Alps, in all their richness, complexity and power to engage, are presented here as a resource for secondary students and their teachers who are studying... • Aboriginal Studies • Geography • Australian History • Biology • Tourism • Outdoor and Environmental Science ...with resources grouped within a series of facts sheets on soils, climate, vegetation, fauna, fire, Aboriginal people, mining, grazing, water catchment recreation and tourism, conservation. EDUCATION RESOURCE TEACHER’S NOTES 1/7 teacher’s notes This is an education resource catering for the curriculum needs of students at Year 7 through 12, across New South Wales, the Australian Capital Territory and Victoria. The following snap- shots show the Australian Alps as an effective focus for study. • The alpine and sub-alpine terrain in Australia is extremely small, unique and highly valued as a water supply as well as for its environmental, cultural, historic and recrea- tional significance. • Most of the Australian Alps lie within national parks with state and federal governments working cooperatively to manage these reserves as one bio-geographical area. • Climate, landforms and soils vary as altitude increases and so create a variety of envi- ronments where different plants grow together in communities. These in turn provide habitats for a wide range of wildlife. Many of these plants and animals are found nowhere else in the world and some are considered threatened or endangered. • The Alps reflect a history of diverse uses and connections including Aboriginal occupation, European exploration, grazing, mining, timber saw milling, water harvesting, conservation, recreation and tourism. Retaining links with this past is an important part of managing the region. -
Sensitivity of the Orographic Precipitation Across the Australian Snowy Mountains to Regional Climate Indices
CSIRO PUBLISHING Journal of Southern Hemisphere Earth Systems Science, 2019, 69, 196–204 https://doi.org/10.1071/ES19014 Sensitivity of the orographic precipitation across the Australian Snowy Mountains to regional climate indices Fahimeh SarmadiA,B,E, Yi HuangC,D, Steven T. SiemsA,B and Michael J. MantonA ASchool of Earth, Atmosphere and Environment, 9 Rainforest Walk, Monash University, Melbourne, Vic. 3800, Australia. BAustralian Research Council (ARC) Centre of Excellence for Climate System Science, Monash University, Melbourne, Vic., Australia. CSchool of Earth Sciences, The University of Melbourne, Melbourne, Vic., Australia. DAustralian Research Council Centre of Excellence for Climate Extremes, Melbourne, Vic., Australia. ECorresponding author. Email: [email protected] Abstract. The wintertime (May–October) precipitation across south-eastern Australia, and the Snowy Mountains, was studied for 22 years (1995–2016) to explore the sensitivity of the relationships between six established climate indices and the precipitation to the orography, both regionally and locally in high-elevation areas. The high-elevation (above 1100 m) precipitation records were provided by an independent network of rain gauges maintained by Snowy Hydro Ltd. These observations were compared with the Australian Water Availability Project (AWAP) precipitation analysis, a commonly used gridded nationwide product. As the AWAP analysis does not incorporate any high-elevation sites, it is unable to capture local orographic precipitation processes. The analysis demonstrates that the alpine precipitation over the Snowy Mountains responds differently to the indices than the AWAP precipitation. In particular, the alpine precipitation is found to be most sensitive to the position of the subtropical ridge and less sensitive to a number of other climate indices tested. -
Landing Sites”
NationalNational Aeronautics Aeronautics and Space and Administration Space Administration SKGs, & ISECG “Landing Sites” Ben Bussey Chief Exploration Scientist Human Exploration & Operations Mission Directorate, NASA HQ 1 Strategic Knowledge Gaps • SKGs define information that is useful/mandatory for designing human spaceflight architecture • Perception is that SKGs HAVE to be closed before we can go to a destination, i.e. they represent Requirements • In reality, there is very little information that is a MUST HAVE before we go somewhere with humans. What SKGs do is buy down risk, allowing you to design simpler/cheaper systems. • There are three flavors of SKGs 1. Have to have – Requirements 2. Buys down risk – LM foot pads 3. Mission enhancing – Resources • Four sets of SKGs – Moon, Phobos & Deimos, Mars, NEOs www.nasa.gov/exploration/library/skg.html 2 Lunar Science-Exploration SKGs • Revisited and revised in 2016 • Architecture was unchanged, so SKG changes were based on new data since the previous SKG revision. • Effort led by LEAG. • Three Themes 1. Understand the lunar resource potential 2. Understand the lunar environment and its effect on human life 3. Understand how to work and live on the lunar surface 3 Findings • Recent missions produced data that was used to retire several of the SKGs defined by HAT and the 2011-2012 LEAG GAP-SAT analyses. • Thanks to these missions, there are no strategic knowledge gaps (SKG) that would inhibit the flight of any human mission (e.g., sortie or human-tended surface facility) <28 days duration. • However, there are several SKGs that should be addressed that would increase human safety not only at the Moon, but also in LEO, cislunar space, and beyond the Moon. -
Discoveries of Mass Independent Isotope Effects in the Solar System: Past, Present and Future Mark H
Reviews in Mineralogy & Geochemistry Vol. 86 pp. 35–95, 2021 2 Copyright © Mineralogical Society of America Discoveries of Mass Independent Isotope Effects in the Solar System: Past, Present and Future Mark H. Thiemens Department of Chemistry and Biochemistry University of California San Diego La Jolla, California 92093 USA [email protected] Mang Lin State Key Laboratory of Isotope Geochemistry Guangzhou Institute of Geochemistry, Chinese Academy of Sciences Guangzhou, Guangdong 510640 China University of Chinese Academy of Sciences Beijing 100049 China [email protected] THE BEGINNING OF ISOTOPES Discovery and chemical physics The history of the discovery of stable isotopes and later, their influence of chemical and physical phenomena originates in the 19th century with discovery of radioactivity by Becquerel in 1896 (Becquerel 1896a–g). The discovery catalyzed a range of studies in physics to develop an understanding of the nucleus and the properties influencing its stability and instability that give rise to various decay modes and associated energies. Rutherford and Soddy (1903) later suggested that radioactive change from different types of decay are linked to chemical change. Soddy later found that this is a general phenomenon and radioactive decay of different energies and types are linked to the same element. Soddy (1913) in his paper on intra-atomic charge pinpointed the observations as requiring the observations of the simultaneous character of chemical change from the same position in the periodic chart with radiative emissions required it to be of the same element (same proton number) but differing atomic weight. This is only energetically accommodated by a change in neutrons and it was this paper that the name “isotope” emerges. -
Winter 2010 Gems & Gemology
G EMS & G VOLUME XLVI WINTER 2010 EMOLOGY W INTER 2010 P AGES 259–336 V OLUME Synthetics Retrospective . Scapolite from Madagascar . Pietersite from China and Namibia . New Mexifire Synthetic Opal . Identifying Historic Gems 46 N O. 4 THE QUARTERLY JOURNAL OF THE GEMOLOGICAL INSTITUTE OF AMERICA 19922 GIA G&G Winter ‘10 Journal P BC 19922 GIA G&G Winter ‘10 Journal P FC Because Public Education Happens At The Counter. GIA’s Retailer Support Kit and website A $97.00 value, shipping symposium 2011 and handling extra. ADVANCING THE SCIENCE GIA’s Retailer Support Kit has been developed to help AND BUSINESS OF GEMS sales associates educate the public about diamonds, the 4Cs, and thoroughly explain a GIA grading report. Take full advantage of all that GIA has to off er by visiting MAY 29 – 30, 2011 www.retailer.gia.edu GIA World Headquarters Robert Mouawad Campus | Carlsbad, California To order your FREE kit, log on to www.retailer.gia.edu www.symposium2011.gia.edu GGWI10 Winter 2010 Volume 46, No. 4 ® EDITORIAL __________________ 259 A Fond Farewell Alice S. Keller FEATURE ARTICLE __________________ 260 Synthetic Gem Materials in the 2000s: A Decade in Review Nathan Renfro, John I. Koivula, Wuyi Wang, and Gary Roskin Looks back on an eventful decade in the synthetic gem industry, highlighted by the commercial introduction of faceted gem-quality CVD synthetic diamonds. NOTES & N EW TECHNIQUES ______________ pg. 262 274 Yellow Scapolite from Ihosy, Madagascar Margherita Superchi, Federico Pezzotta, Elena Gambini, and Emanuela Castaman Characterizes scapolite from this locality and examines established methods of calculating the gem’s chemical composition.