Mining on the Moon; Yes, It’S Really Going to Happen
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Craters in Shadow
Section 3: Craters in Shadow Kepler Copernicus Eratosthenes Seen it Clavius Seen it Section 3: Craters in Shadow Visibility: A pair of binoculars is the minimum requirement to see these features. When: Look for them when the terminator’s close by, typically a day before last quarter. Not all craters are best seen when the Sun is high in the lunar sky - in fact most aren’t! If craters aren’t par- ticularly bright or dark, they tend to disappear into the background when the Moon’s phase is close to full. These craters are best seen when the ‘terminator’ is nearby, or when the Sun is low in the lunar sky as seen from the crater. This causes oblique lighting to fall on the crater and create exaggerated shadows. Ultimately, this makes the crater look more dramatic and easier to see. We’ll use this effect for the next section on lunar mountains, but before we do, there are a couple of craters that we’d like to bring to your attention. Actually, the Moon is covered with a whole host of wonderful craters that look amazing when the lighting is oblique. During the summer and into the early autumn, it’s the later phases of the Moon are best positioned in the sky - the phases following full Moon. Unfortunately, this means viewing in the early hours but don’t worry as we’ve kept things simple. We just want to give you a taste of what a shadowed crater looks like for this marathon, so the going here is really pretty easy! First, locate the two craters Kepler and Copernicus which were marathon targets pointed out in Section 2. -
Project Horizon Report
Volume I · SUMMARY AND SUPPORTING CONSIDERATIONS UNITED STATES · ARMY CRD/I ( S) Proposal t c• Establish a Lunar Outpost (C) Chief of Ordnance ·cRD 20 Mar 1 95 9 1. (U) Reference letter to Chief of Ordnance from Chief of Research and Devel opment, subject as above. 2. (C) Subsequent t o approval by t he Chief of Staff of reference, repre sentatives of the Army Ballistic ~tissiles Agency indicat e d that supplementar y guidance would· be r equired concerning the scope of the preliminary investigation s pecified in the reference. In particular these r epresentatives requested guidance concerning the source of funds required to conduct the investigation. 3. (S) I envision expeditious development o! the proposal to establish a lunar outpost to be of critical innportance t o the p. S . Army of the future. This eva luation i s appar ently shar ed by the Chief of Staff in view of his expeditious a pproval and enthusiastic endorsement of initiation of the study. Therefore, the detail to be covered by the investigation and the subs equent plan should be as com plete a s is feas ible in the tin1e limits a llowed and within the funds currently a vailable within t he office of t he Chief of Ordnance. I n this time of limited budget , additional monies are unavailable. Current. programs have been scrutinized r igidly and identifiable "fat'' trimmed awa y. Thus high study costs are prohibitive at this time , 4. (C) I leave it to your discretion t o determine the source and the amount of money to be devoted to this purpose. -
List of Missions Using SPICE (PDF)
1/7/20 Data Restorations Selected Past Users Current/Pending Users Examples of Possible Future Users Apollo 15, 16 [L] Magellan [L] Cassini Orbiter NASA Discovery Program Mariner 2 [L] Clementine (NRL) Mars Odyssey NASA New Frontiers Program Mariner 9 [L] Mars 96 (RSA) Mars Exploration Rover Lunar IceCube (Moorehead State) Mariner 10 [L] Mars Pathfinder Mars Reconnaissance Orbiter LunaH-Map (Arizona State) Viking Orbiters [L] NEAR Mars Science Laboratory Luna-Glob (RSA) Viking Landers [L] Deep Space 1 Juno Aditya-L1 (ISRO) Pioneer 10/11/12 [L] Galileo MAVEN Examples of Users not Requesting NAIF Help Haley armada [L] Genesis SMAP (Earth Science) GOLD (LASP, UCF) (Earth Science) [L] Phobos 2 [L] (RSA) Deep Impact OSIRIS REx Hera (ESA) Ulysses [L] Huygens Probe (ESA) [L] InSight ExoMars RSP (ESA, RSA) Voyagers [L] Stardust/NExT Mars 2020 Emmirates Mars Mission (UAE via LASP) Lunar Orbiter [L] Mars Global Surveyor Europa Clipper Hayabusa-2 (JAXA) Helios 1,2 [L] Phoenix NISAR (NASA and ISRO) Proba-3 (ESA) EPOXI Psyche Parker Solar Probe GRAIL Lucy EUMETSAT GEO satellites [L] DAWN Lunar Reconnaissance Orbiter MOM (ISRO) Messenger Mars Express (ESA) Chandrayan-2 (ISRO) Phobos Sample Return (RSA) ExoMars 2016 (ESA, RSA) Solar Orbiter (ESA) Venus Express (ESA) Akatsuki (JAXA) STEREO [L] Rosetta (ESA) Korean Pathfinder Lunar Orbiter (KARI) Spitzer Space Telescope [L] [L] = limited use Chandrayaan-1 (ISRO) New Horizons Kepler [L] [S] = special services Hayabusa (JAXA) JUICE (ESA) Hubble Space Telescope [S][L] Kaguya (JAXA) Bepicolombo (ESA, JAXA) James Webb Space Telescope [S][L] LADEE Altius (Belgian earth science satellite) ISO [S] (ESA) Armadillo (CubeSat, by UT at Austin) Last updated: 1/7/20 Smart-1 (ESA) Deep Space Network Spectrum-RG (RSA) NAIF has or had project-supplied funding to support mission operations, consultation for flight team members, and SPICE data archive preparation. -
Go for Lunar Landing Conference Report
CONFERENCE REPORT Sponsored by: REPORT OF THE GO FOR LUNAR LANDING: FROM TERMINAL DESCENT TO TOUCHDOWN CONFERENCE March 4-5, 2008 Fiesta Inn, Tempe, AZ Sponsors: Arizona State University Lunar and Planetary Institute University of Arizona Report Editors: William Gregory Wayne Ottinger Mark Robinson Harrison Schmitt Samuel J. Lawrence, Executive Editor Organizing Committee: William Gregory, Co-Chair, Honeywell International Wayne Ottinger, Co-Chair, NASA and Bell Aerosystems, retired Roberto Fufaro, University of Arizona Kip Hodges, Arizona State University Samuel J. Lawrence, Arizona State University Wendell Mendell, NASA Lyndon B. Johnson Space Center Clive Neal, University of Notre Dame Charles Oman, Massachusetts Institute of Technology James Rice, Arizona State University Mark Robinson, Arizona State University Cindy Ryan, Arizona State University Harrison H. Schmitt, NASA, retired Rick Shangraw, Arizona State University Camelia Skiba, Arizona State University Nicolé A. Staab, Arizona State University i Table of Contents EXECUTIVE SUMMARY..................................................................................................1 INTRODUCTION...............................................................................................................2 Notes...............................................................................................................................3 THE APOLLO EXPERIENCE............................................................................................4 Panelists...........................................................................................................................4 -
10Great Features for Moon Watchers
Sinus Aestuum is a lava pond hemming the Imbrium debris. Mare Orientale is another of the Moon’s large impact basins, Beginning observing On its eastern edge, dark volcanic material erupted explosively and possibly the youngest. Lunar scientists think it formed 170 along a rille. Although this region at first appears featureless, million years after Mare Imbrium. And although “Mare Orien- observe it at several different lunar phases and you’ll see the tale” translates to “Eastern Sea,” in 1961, the International dark area grow more apparent as the Sun climbs higher. Astronomical Union changed the way astronomers denote great features for Occupying a region below and a bit left of the Moon’s dead lunar directions. The result is that Mare Orientale now sits on center, Mare Nubium lies far from many lunar showpiece sites. the Moon’s western limb. From Earth we never see most of it. Look for it as the dark region above magnificent Tycho Crater. When you observe the Cauchy Domes, you’ll be looking at Yet this small region, where lava plains meet highlands, con- shield volcanoes that erupted from lunar vents. The lava cooled Moon watchers tains a variety of interesting geologic features — impact craters, slowly, so it had a chance to spread and form gentle slopes. 10Our natural satellite offers plenty of targets you can spot through any size telescope. lava-flooded plains, tectonic faulting, and debris from distant In a geologic sense, our Moon is now quiet. The only events by Michael E. Bakich impacts — that are great for telescopic exploring. -
JAXA's Space Exploration Activities
JAXA’s Space Exploration Activities Jun Gomi, Deputy Director General, JAXA Hayabusa 2 ✓ Asteroid Explorer of the C-type asteroid ✓ Launched in December, 2014 ✓ Reached target asteroid “Ryugu” in 2018 ✓ First successful touchdown to Ryugu on February 22, 2019 ✓ Return to Earth in 2020 (162173) Ryugu 2 Hayabusa 2 (c) JAXA, University of Tokyo, Kochi University, Rikkyo University, (c) JAXA, University of Tokyo, Kochi University, Rikkyo University, Nagoya University, Chiba Institute of Technology, Meiji University, Nagoya University, Chiba Institute of Technology, Meiji University, University of Aizu and AIST. University of Aizu, AIST Asteroid Ryugu photographed from a Asteroid Ryugu from an altitude of 6km. distance of about 20 km. The image Image was captured with the Optical was taken on June 30, 2018. Navigation Camera on July 20, 2018. Hayabusa 2 4 JAXA’s Plan for Space Exploration International • Utilization of ISS/Kibo • Cis-Lunar Platform (Gateway) Cooperation • Lunar exploration and beyond Industry & • JAXA Space Exploration Innovation Academia Hub Partnerships • Science Community discussions JAXA’s Overall Scenario for International Space Exploration Mars, others ★ Initial Exploration ★ Full Fledge Exploration MMX: JFY2024 • Science and search for life • Utilization feasibility exam. Kaguya Moon ©JAXA ©JAXA ©JAXA ©JAXA ©JAXA Full-fledged Exploration & SLIM Traversing exploration(2023- ) Sample Return(2026- ) Utilization (JFY2021) • Science exploration • S/R from far side • Cooperative science/resource • Water prospecting • Technology demo for human mission exploration by robotic and human HTV-X der.(2026- ) • Small probe deploy, data relay etc. Gateway Phase 1 Gateway (2022-) Phase 2 • Support for Lunar science Earth • Science using deep space Promote Commercialization International Space Station 6 SLIM (Smart Lander for Investigating Moon) ✓ Demonstrate pin-point landing on the moon. -
Relative Ages
CONTENTS Page Introduction ...................................................... 123 Stratigraphic nomenclature ........................................ 123 Superpositions ................................................... 125 Mare-crater relations .......................................... 125 Crater-crater relations .......................................... 127 Basin-crater relations .......................................... 127 Mapping conventions .......................................... 127 Crater dating .................................................... 129 General principles ............................................. 129 Size-frequency relations ........................................ 129 Morphology of large craters .................................... 129 Morphology of small craters, by Newell J. Fask .................. 131 D, method .................................................... 133 Summary ........................................................ 133 table 7.1). The first three of these sequences, which are older than INTRODUCTION the visible mare materials, are also dominated internally by the The goals of both terrestrial and lunar stratigraphy are to inte- deposits of basins. The fourth (youngest) sequence consists of mare grate geologic units into a stratigraphic column applicable over the and crater materials. This chapter explains the general methods of whole planet and to calibrate this column with absolute ages. The stratigraphic analysis that are employed in the next six chapters first step in reconstructing -
The Systematic Identification and Articulation of Content Standards and Benchmarks. Update. INSTITUTION Mid-Continent Regional Educational Lab., Aurora, CO
DOCUMENT RESUME ED 403 308 TM 026 040 AUTHOR Kendall, John S.; Marzano, Robert J. TITLE The Systematic Identification and Articulation of Content Standards and Benchmarks. Update. INSTITUTION Mid-Continent Regional Educational Lab., Aurora, CO. SPONS AGENCY Office of Educational Research and Improvement (ED), Washington, DC. PUB DATE Mar 95 CONTRACT RP91002005 NOTE 598p. AVAILABLE FROM Superintendent of Documents, U.S. Government Printing Office, Washington, DC 20402. PUB TYPE Legal/Legislative/Regulatory Materials (090) Reports Descriptive (141) EDRS PRICE MF03/PC24 Plus Postage. DESCRIPTORS Art; *Course Content; *Educational Improvement; Elementary Secondary Education; Geography Instruction; Health Education; History Instruction; *Identification; Language Arts; Mathematics Education; Science Education; *Standards; Thinking Skills IDENTIFIERS *Benchmarking; *Subject Content Knowledge ABSTRACT The project described in this paper addresses the major issues surrounding content standards, provides a model for their identification, and applies this model to identify standards and benchmarks in subject areas. This update includes a revision of content standards and benchmarks published in, earlier updates and the synthesis and identification of standards in new areas. Standards and benchmarks are provided for science, mathematics, history, geography, the arts, the language arts, and health. Also included are standards in thinking and reasoning and an analysis and description of knowledge and skills considered important for the workplace. Following an introduction, the second section presents an overview of the current efforts towards standards in each of these subject areas. Section 3 describes the technical and conceptual differences that have been apparent in the standards movement and the model adopted for this study. Section 4 presents key questions that should be addressed by schools and districts interested in a standards-based strategy. -
Astrophysics
National Aeronautics and Space Administration Astrophysics Committee on NASA Science Paul Hertz Mission Extensions Director, Astrophysics Division NRC Keck Center Science Mission Directorate Washington DC @PHertzNASA February 1-2, 2016 Why Astrophysics? Astrophysics is humankind’s scientific endeavor to understand the universe and our place in it. 1. How did our universe 2. How did galaxies, stars, 3. Are We Alone? begin and evolve? and planets come to be? These national strategic drivers are enduring 1972 1982 1991 2001 2010 2 Astrophysics Driving Documents http://science.nasa.gov/astrophysics/documents 3 Astrophysics Programs Physics of the Cosmos Cosmic Origins Exoplanet Exploration Program Program Program 1. How did our universe 2. How did galaxies, stars, 3. Are We Alone? begin and evolve? and planets come to be? Astrophysics Explorers Program Astrophysics Research Program James Webb Space Telescope Program (managed outside of Astrophysics Division until commissioning) 4 Astrophysics Programs and Missions Physics of the Cosmos Cosmic Origins Exoplanet Exploration Program Program Program Chandra Hubble Spitzer Kepler/K2 XMM-Newton (ESA) Herschel (ESA) WFIRST Fermi SOFIA Planck (ESA) LISA Pathfinder (ESA) Astrophysics Explorers Program Euclid (ESA) NuSTAR Swift Suzaku (JAXA) Athena (ESA) ASTRO-H (JAXA) NICER TESS L3 GW Obs (ESA) 3 SMEX and 2 MO in Phase A James Webb Space Telescope Program: Webb 5 Astrophysics Programs and Missions Physics of the Cosmos Cosmic Origins Exoplanet Exploration Program Program Program Missions in extended phase Chandra Hubble Spitzer Kepler/K2 XMM-Newton (ESA) Herschel (ESA) WFIRST Fermi SOFIA Planck (ESA) LISA Pathfinder (ESA) Astrophysics Explorers Program Euclid (ESA) NuSTAR Swift Suzaku (JAXA) Athena (ESA) ASTRO-H (JAXA) NICER TESS L3 GW Obs (ESA) 3 SMEX and 2 MO in Phase A James Webb Space Telescope Program: Webb 6 Astrophysics Mission Portfolio • NASA Astrophysics seeks to advance NASA’s strategic objectives in astrophysics as well as the science priorities of the Decadal Survey in Astronomy and Astrophysics. -
State Da Vinci Decathlon 2016 Practice Tasks
Knox Grammar School STATE DA VINCI DECATHLON 2016 PRACTICE TASKS CELEBRATING THE ACADEMIC GIFTS OF STUDENTS IN YEARS 9, 10 & 11 Task developed by Karen Yager, Knox Grammar School, 2016 An academic gala day for Years 9, 10 & 11 Team Number _____________ Task developed by Karen Yager, Knox Grammar School, 2016 Background information The poet T.S. Eliot wrote “We shall not cease from exploration, and the end of all our exploring will be to arrive where we started and know the place for the first time”. Throughout history humanity has yearned to explore new worlds. However, many after travelling to new places discover that they long to return to their home. They see home in a fresh light and question why they left it in the first place. Homer’s legendary hero Odysseus explored new countries and met fascinating people and creatures but after the tragic loss of all of his men he realised that he wanted to return home to Penelope and the life he led in Ithaca: Many cities of men he saw and learned their minds, many pains he suffered, heartsick on the open sea, fighting to save his life and bring his comrades home. Driven by curiosity many have left home to explore new worlds: the sailors who sailed across unknown, treacherous seas to explore new lands; young country boys who enlisted during the world wars to escape their country homes and explore foreign places; scientists who are planning to travel to Mars knowing that there will be no return; and even many young people who long to leave their home after school and explore new worlds but after extensive travelling discover that their home was a wonderful place. -
Extending NASA™S Exploration Systems Architecture Towards Long
SpaceOps 2006 Conference AIAA 2006-5746 Extending NASA’s Exploration Systems Architecture towards Long - term Crewed Moon and Mars Operations Wilfried K. Hofstetter *, Paul D. Wooster †, Edward F. Crawley ‡ Massac husetts Institute of Technology 77 Massachusetts Avenue , Cambridge, MA, 02139 This pape r presents a baseline strategy for extending lunar crew transportation system operations as outlined in NASA’s Exploration Systems Architecture Study (ESAS) report towards longer -stay lunar surface operations and conjunction class Mars missions. The analys is of options for commonality between initial lunar sortie operations and later Moon and Mars exploration missions is essential for reducing life -cycle cost and pr oviding low - investment / high -return options for extending exploration capabilities soon afte r the 7 th human lunar landing . The analysis is also intended to inform the development of the human lunar lander and other exploration system elements by identifying enabling requirements for extension of the lunar crew tr ansportation system. The baseline strategy outlined in this paper was generated using a three -step process : the analysis of exploration objectives and scenarios, identification of functional and operational extension options , and the conceptual design of a set of preferred extension option s. Extension options include (but are not limited to) the use of the human lunar lander as outpost for extended stays, and Mars crew transportation using evolved Crew Exploration Vehicle ( CEV ) and human lander crew compartments. Although t he results presen ted in this paper are based on the ES AS elements , the conclusions drawn in this paper are generally applicable provided the same l unar transportation mode (lunar orbit rendezvous) is used . -
Securing Japan an Assessment of Japan´S Strategy for Space
Full Report Securing Japan An assessment of Japan´s strategy for space Report: Title: “ESPI Report 74 - Securing Japan - Full Report” Published: July 2020 ISSN: 2218-0931 (print) • 2076-6688 (online) Editor and publisher: European Space Policy Institute (ESPI) Schwarzenbergplatz 6 • 1030 Vienna • Austria Phone: +43 1 718 11 18 -0 E-Mail: [email protected] Website: www.espi.or.at Rights reserved - No part of this report may be reproduced or transmitted in any form or for any purpose without permission from ESPI. Citations and extracts to be published by other means are subject to mentioning “ESPI Report 74 - Securing Japan - Full Report, July 2020. All rights reserved” and sample transmission to ESPI before publishing. ESPI is not responsible for any losses, injury or damage caused to any person or property (including under contract, by negligence, product liability or otherwise) whether they may be direct or indirect, special, incidental or consequential, resulting from the information contained in this publication. Design: copylot.at Cover page picture credit: European Space Agency (ESA) TABLE OF CONTENT 1 INTRODUCTION ............................................................................................................................. 1 1.1 Background and rationales ............................................................................................................. 1 1.2 Objectives of the Study ................................................................................................................... 2 1.3 Methodology