DOCSLIB.ORG

Lunar Polar Volatiles

Total Page：16

File Type：pdf, Size：1020Kb

Download full-text PDF Read full-text
Lunar Polar Volatiles Program and Abstracts Lunar Polar Volatiles August 7–9, 2018 • Laurel, Maryland Organizers Lunar and Planetary Institute Universities Space Research Association Johns Hopkins University, Applied Physics Laboratory Convener Kathleen Mandt John Hopkins University, Applied Physics Laboratory Science Organizing Committee Kathleen Mandt Johns Hopkins University, Applied Physics Laboratory William Farrell NASA Goddard Space Flight Center Elizabeth Fisher Brown University Andrew Jordan University of New Hampshire Rachel Klima Johns Hopkins University, Applied Physics Laboratory Paul Lucey University of Hawaii Lunar and Planetary Institute 3600 Bay Area Boulevard Houston TX 77058-1113 Abstracts for this meeting are available via the meeting website at https://www.hou.usra.edu/meetings/lunarvolatiles2018/ Abstracts can be cited as Author A. B. and Author C. D. (2018) Title of abstract. In Lunar Polar Volatiles, Abstract #XXXX. LPI Contribution No. 2087, Lunar and Planetary Institute, Houston. Guide to Sessions Tuesday, August 7, 2018 9:00 a.m. Bldg. 200, Room E-100 Lunar Polar Volatiles: Current Understanding, Recent Discoveries, and Future Exploration 10:45 a.m. Bldg. 200, Room E-100 Volatile Sources for the Lunar Poles: I 1:30 p.m. Bldg. 200, Room E-100 Volatile Sources for the Lunar Poles: II 3:00 p.m. Bldg. 200, Room E-100 Panel Discussion on Volatile Sources 4:00 p.m. Bldg. 200, Room E-100 Distribution Differences Between the Surface and Deeper Volatiles: I 5:00 p.m. Bldg. 200, Lobby Welcome Reception Wednesday, August 8, 2018 9:00 a.m. Bldg. 200, Room E-100 Distribution Differences Between the Surface and Deeper Volatiles: II 10:30 a.m. Bldg. 200, Room E-100 Panel Discussion on Distribution of Volatiles 1:00 p.m. Bldg. 200, Room E-100 Transport of Volatiles at the Poles and Processes that Influence Distribution: I 3:50 p.m. Bldg. 200, Room E-100 Panel Discussion on Transport and Processes: I 5:30 p.m. Bldg. 200, Room E-100 Poster Session: Lunar Polar Volatiles Workshop Thursday, August 9, 2018 9:00 a.m. Bldg. 200, Room E-100 Transport of Volatiles at the Poles and Processes that Influence Distribution: II 10:15 a.m. Bldg. 200, Room E-100 Panel Discussion on Transport and Processes: II 10:45 a.m. Bldg. 200, Room E-100 Composition of Lunar Polar Volatiles: It’s More Than Just Water! 11:45 a.m. Bldg. 200, Room E-100 Panel Discussion for Composition of Lunar Polar Volatiles: It’s More Than Just Water! 1:20 p.m. Bldg. 200, Room E-100 Future Steps 4:00 p.m. Bldg. 200, Room E-100 Panel Discussion on Future Steps Program Tuesday, August 7, 2018 LUNAR POLAR VOLATILES: CURRENT UNDERSTANDING, RECENT DISCOVERIES, AND FUTURE EXPLORATION 9:00 a.m. Bldg. 200, Room E-100 Chair: Kathleen Mandt 9:00 a.m. Mandt K. * Welcome and Logistics 9:15 a.m. Hayne P. O. * Lunar Polar Volatiles: Current Understanding, Recent Discoveries, and Future Exploration [#5017] Recent observations and models have provided new insights into the nature and origins of lunar polar volatiles. I will provide a summary of current understanding of lunar volatiles and possible future directions for addressing outstanding questions. 10:15 a.m. Coffee Break VOLATILE SOURCES FOR THE LUNAR POLES: I 10:45 a.m. Bldg. 200, Room E-100 Chair: David Blewett 10:45 a.m. Lucey P. G. * Hurley D. Farrell W. Petro N. E. Cable M. Dyar D. Orlando T. McCanta M. Fisher E. Hibbitts K. Prem P. Benna M. Hayne P. Green R. Pieters C. M. Mandt K. Horyani M. Haleakas J. Li S. The Lunar Volatile System in Space and Time: Supplies to the Lunar Poles [#5015] Volatile sources for the poles vary in space and time. Now, meteorites and solar wind dominate the inputs; in the past volcanic eruptions and impacts overwhelmed the current sources. Major gaps in understanding persist regarding all epochs. 11:05 a.m. Needham D. H. * Kring D. A. A Volcanic Source for Lunar Polar Volatiles [#5009] Ancient eruptions of lunar mare basalts released significant masses of volatiles around the Moon. These internally sourced volatiles may have migrated to the lunar poles, forming a substantial component of currently observed polar volatile deposits. 11:25 a.m. Tucker O. J. * Killen R. M. Saxena P. Johnson R. E. Prem P. Lifetime of a Transient Atmosphere Produced by Lunar Volcanism [#5039] We estimate the thermal escape lifetime of a volcanically produced early Moon atmosphere for comparison to the Needham and Kring (2017), Earth and Planet. Sci., study. 11:45 a.m. Orlando T. M. * Jones B. M. Alexandrov A. B. Hibbitts C. A. Dyar M. D. A Solar Wind Source of Water in the Polar Regions of the Moon? [#5008] We address formation of water via thermally activated recombinative desorption of hydroxyls in proton irradiated regolith. This temperature dependent process can lead to limited water build-up at the poles or in permanently shadowed regions. 12:05 p.m. Lunch Tuesday, August 7, 2018 VOLATILE SOURCES FOR THE LUNAR POLES: II 1:30 p.m. Bldg. 200, Room E-100 Chair: David Blewett 1:30 p.m. Mandt K. E. * Luspay-Kuti A. Comets and Meteorites as Sources of Lunar Polar Volatiles [#5041] Volatiles stored in the lunar polar region could provide a time-line of volatile delivery to the Moon. We will review composition tracers for comets and meteorites that can be used to evaluate the history of volatile delivery to the Moon. 1:50 p.m. Schorghofer N. * Transport in the Lunar Water Exosphere [#5004] A surface-bounded exosphere has a non-exponential vertical density distribution. Delivery of water to the polar cold traps is dramatically more efficient on the Moon than on Mercury and Ceres. Uncertainties lie with the surface interaction. 2:10 p.m. Taylor G. J. * Kring D. A. Needham D. H. The Lunar Interior as a Source of Polar Water [#5007] Water released from the lunar crust by moonquakes and impacts each account for between 100 and 10,000 kg of water per year, at least three orders of magnitude less than contributed by solar wind or impact of water-bearing projectiles. 2:30 p.m. Coffee Break PANEL DISCUSSION ON VOLATILE SOURCES 3:00 p.m. Bldg. 200, Room E-100 Moderator: Adrienn Luspay-Kuti Panel Members: Kathleen Mandt Jeff Taylor Debra Needham O. J. Tucker Tuesday, August 7, 2018 DISTRIBUTION DIFFERENCES BETWEEN THE SURFACE AND DEEPER VOLATILES: I 4:00 p.m. Bldg. 200, Room E-100 Chair: John Gruener 4:00 p.m. Siegler M. A. * Keane J. T. Paige D. A. Subsurface Ice Stability on the Moon [#5038] The Moon has about 26,000 km2 of surface area in the large shadowed regions near the poles where ice could be stable. However, over 240,000 km2 of area in the upper meter alone that could hide subsurface ice. Much of the lunar ice may be at depth. 4:20 p.m. Jordan A. P. * Wilson J. K. Schwadron N. A. Spence H. E. Petro N. E. A Framework to Determine the History of the Moon’s Polar Ice [#5003] We describe a framework for interpreting the large-scale distribution of water ice in the polar regions of the Moon, and we show how this framework can help constrain the history of the ice as a function of depth. 4:40 p.m. McClanahan T. P. * Mitrofanov I. G. Boynton W. V. Chin G. Livengood T. A. Sanin A. Litvak M. Parsons A. Hamara D. Harshman K. Starr R. Su J. J. Lunar Regolith Geochemistry Variation May Explain the Polar Wander Observations [#5012] We examine recently recalibrated Lunar Exploration Neutron Detector (LEND) polar observations and the observation of polar wander. Preliminary studies suggest that regolith geochemistry variation could explain the polar wander observation. Wednesday, August 8, 2018 DISTRIBUTION DIFFERENCES BETWEEN THE SURFACE AND DEEPER VOLATILES: II 9:00 a.m. Bldg. 200, Room E-100 Chair: Susan Klem 9:00 a.m. Fisher E. A. * Lucey P. G. Lemelin M. Greenhagen B. T. Siegler M. A. Mazarico E. Aharonson O. Williams J. Hayne P. O. Neumann G. A. Paige D. A. Smith D. E. Zuber M. T. Evidence for Surface Water Ice in the Lunar Polar Regions Using Reflectance Measurements from the Lunar Orbiter Laser Altimeter and Temperature Measurements from the Diviner Lunar Radiometer Experiment [#5011] We study LOLA derived normal albedo as a function of Diviner maximum temperature, to see if lunar permanently shadowed regions cold enough (<110K) to preserve surface water frost over geologic timescales show increased reflectance. 9:20 a.m. Li S. * Lucey P. G. Milliken R. E. Hayne P. O. Fisher E. Williams J. P. Hurley D. Elphic R. C. Direct Detections of Surface Exposed Water Ice in the Lunar Polar Regions [#5010] IR absorptions of ice near 1.3, 1.5, and 2.0-µm were detected using the M3 data near the lunar polar regions, which is the first direct evidence for surface exposed water ice on the Moon. The distribution and formation of ice are also discussed. 9:40 a.m. Raut U. * Karnes P. L. Retherford K. D. Czajka E. Poston M. J. Davis M. W. Liu Y. Patrick E. L. Gladstone G. R. Greathouse T. K. Hendrix A. R. Mokashi P. Investigating Far-ultraviolet hydration signatures in the Southwest Ultraviolet Reflectance Chamber (SwURC) in support of LRO-LAMP observations [#5037] We will present results from our laboratory investigations on far-ultraviolet reflectance measurements of dry and water vapor-exposed Apollo soils made in support of LRO-LAMP observations. 10:00 a.m. Coffee Break PANEL DISCUSSION ON DISTRIBUTION OF VOLATILES 10:30 a.m.
Load more

Recommended publications
  • 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.
    [Show full text]
  • Green Diamond Forest Habitat Conservation Plan Appendix B
    B-1 Appendix B. Profile of the Covered Species TABLE OF CONTENTS APPENDIX B. PROFILE OF THE COVERED SPECIES ................................................... B-1 B.1 NORTHERN SPOTTED OWL (STRIX OCCIDENTALIS CAURINA) .......................................... B-3 B.2 LISTING STATUS ......................................................................................................... B-3 B.2.1 Range and Distribution .......................................................................................... B-3 B.2.2 Life History ............................................................................................................ B-4 B.2.3 Habitat Requirements ............................................................................................ B-5 B.3 FISHER (PEKANIA PENNANTI) ....................................................................................... B-5 B.3.1 Listing Status ......................................................................................................... B-5 B.3.2 Range and Distribution .......................................................................................... B-6 B.3.3 Life History ............................................................................................................ B-8 B.3.4 Habitat Requirements ............................................................................................ B-9 B.3.5 Resting and Denning Habitat ............................................................................... B-10 B.3.6 Foraging Habitat .................................................................................................
    [Show full text]
  • Terrestrial Impact Structures Provide the Only Ground Truth Against Which Computational and Experimental Results Can Be Com­ Pared
    Ann. Rev. Earth Planet. Sci. 1987. 15:245-70 Copyright([;; /987 by Annual Reviews Inc. All rights reserved TERRESTRIAL IMI!ACT STRUCTURES ··- Richard A. F. Grieve Geophysics Division, Geological Survey of Canada, Ottawa, Ontario KIA OY3, Canada INTRODUCTION Impact structures are the dominant landform on planets that have retained portions of their earliest crust. The present surface of the Earth, however, has comparatively few recognized impact structures. This is due to its relative youthfulness and the dynamic nature of the terrestrial geosphere, both of which serve to obscure and remove the impact record. Although not generally viewed as an important terrestrial (as opposed to planetary) geologic process, the role of impact in Earth evolution is now receiving mounting consideration. For example, large-scale impact events may hav~~ been responsible for such phenomena as the formation of the Earth's moon and certain mass extinctions in the biologic record. The importance of the terrestrial impact record is greater than the relatively small number of known structures would indicate. Impact is a highly transient, high-energy event. It is inherently difficult to study through experimentation because of the problem of scale. In addition, sophisticated finite-element code calculations of impact cratering are gen­ erally limited to relatively early-time phenomena as a result of high com­ putational costs. Terrestrial impact structures provide the only ground truth against which computational and experimental results can be com­ pared. These structures provide information on aspects of the third dimen­ sion, the pre- and postimpact distribution of target lithologies, and the nature of the lithologic and mineralogic changes produced by the passage of a shock wave.
    [Show full text]
  • General Index
    General Index Italicized page numbers indicate figures and tables. Color plates are in- cussed; full listings of authors’ works as cited in this volume may be dicated as “pl.” Color plates 1– 40 are in part 1 and plates 41–80 are found in the bibliographical index. in part 2. Authors are listed only when their ideas or works are dis- Aa, Pieter van der (1659–1733), 1338 of military cartography, 971 934 –39; Genoa, 864 –65; Low Coun- Aa River, pl.61, 1523 of nautical charts, 1069, 1424 tries, 1257 Aachen, 1241 printing’s impact on, 607–8 of Dutch hamlets, 1264 Abate, Agostino, 857–58, 864 –65 role of sources in, 66 –67 ecclesiastical subdivisions in, 1090, 1091 Abbeys. See also Cartularies; Monasteries of Russian maps, 1873 of forests, 50 maps: property, 50–51; water system, 43 standards of, 7 German maps in context of, 1224, 1225 plans: juridical uses of, pl.61, 1523–24, studies of, 505–8, 1258 n.53 map consciousness in, 636, 661–62 1525; Wildmore Fen (in psalter), 43– 44 of surveys, 505–8, 708, 1435–36 maps in: cadastral (See Cadastral maps); Abbreviations, 1897, 1899 of town models, 489 central Italy, 909–15; characteristics of, Abreu, Lisuarte de, 1019 Acequia Imperial de Aragón, 507 874 –75, 880 –82; coloring of, 1499, Abruzzi River, 547, 570 Acerra, 951 1588; East-Central Europe, 1806, 1808; Absolutism, 831, 833, 835–36 Ackerman, James S., 427 n.2 England, 50 –51, 1595, 1599, 1603, See also Sovereigns and monarchs Aconcio, Jacopo (d. 1566), 1611 1615, 1629, 1720; France, 1497–1500, Abstraction Acosta, José de (1539–1600), 1235 1501; humanism linked to, 909–10; in- in bird’s-eye views, 688 Acquaviva, Andrea Matteo (d.
    [Show full text]
  • Select Letters of Percy Bysshe Shelley
    ENGLISH CLÀSSICS The vignette, representing Shelleÿs house at Great Mar­ lou) before the late alterations, is /ro m a water- colour drawing by Dina Williams, daughter of Shelleÿs friend Edward Williams, given to the E ditor by / . Bertrand Payne, Esq., and probably made about 1840. SELECT LETTERS OF PERCY BYSSHE SHELLEY EDITED WITH AN INTRODUCTION BY RICHARD GARNETT NEW YORK D.APPLETON AND COMPANY X, 3, AND 5 BOND STREET MDCCCLXXXIII INTRODUCTION T he publication of a book in the series of which this little volume forms part, implies a claim on its behalf to a perfe&ion of form, as well as an attradiveness of subjeâ:, entitling it to the rank of a recognised English classic. This pretensión can rarely be advanced in favour of familiar letters, written in haste for the information or entertain­ ment of private friends. Such letters are frequently among the most delightful of literary compositions, but the stamp of absolute literary perfe&ion is rarely impressed upon them. The exceptions to this rule, in English literature at least, occur principally in the epistolary litera­ ture of the eighteenth century. Pope and Gray, artificial in their poetry, were not less artificial in genius to Cowper and Gray ; but would their un- their correspondence ; but while in the former premeditated utterances, from a literary point of department of composition they strove to display view, compare with the artifice of their prede­ their art, in the latter their no less successful cessors? The answer is not doubtful. Byron, endeavour was to conceal it. Together with Scott, and Kcats are excellent letter-writers, but Cowper and Walpole, they achieved the feat of their letters are far from possessing the classical imparting a literary value to ordinary topics by impress which they communicated to their poetry.
    [Show full text]
  • Special Catalogue Milestones of Lunar Mapping and Photography Four Centuries of Selenography on the Occasion of the 50Th Anniversary of Apollo 11 Moon Landing
    Special Catalogue Milestones of Lunar Mapping and Photography Four Centuries of Selenography On the occasion of the 50th anniversary of Apollo 11 moon landing Please note: A specific item in this catalogue may be sold or is on hold if the provided link to our online inventory (by clicking on the blue-highlighted author name) doesn't work! Milestones of Science Books phone +49 (0) 177 – 2 41 0006 www.milestone-books.de [email protected] Member of ILAB and VDA Catalogue 07-2019 Copyright © 2019 Milestones of Science Books. All rights reserved Page 2 of 71 Authors in Chronological Order Author Year No. Author Year No. BIRT, William 1869 7 SCHEINER, Christoph 1614 72 PROCTOR, Richard 1873 66 WILKINS, John 1640 87 NASMYTH, James 1874 58, 59, 60, 61 SCHYRLEUS DE RHEITA, Anton 1645 77 NEISON, Edmund 1876 62, 63 HEVELIUS, Johannes 1647 29 LOHRMANN, Wilhelm 1878 42, 43, 44 RICCIOLI, Giambattista 1651 67 SCHMIDT, Johann 1878 75 GALILEI, Galileo 1653 22 WEINEK, Ladislaus 1885 84 KIRCHER, Athanasius 1660 31 PRINZ, Wilhelm 1894 65 CHERUBIN D'ORLEANS, Capuchin 1671 8 ELGER, Thomas Gwyn 1895 15 EIMMART, Georg Christoph 1696 14 FAUTH, Philipp 1895 17 KEILL, John 1718 30 KRIEGER, Johann 1898 33 BIANCHINI, Francesco 1728 6 LOEWY, Maurice 1899 39, 40 DOPPELMAYR, Johann Gabriel 1730 11 FRANZ, Julius Heinrich 1901 21 MAUPERTUIS, Pierre Louis 1741 50 PICKERING, William 1904 64 WOLFF, Christian von 1747 88 FAUTH, Philipp 1907 18 CLAIRAUT, Alexis-Claude 1765 9 GOODACRE, Walter 1910 23 MAYER, Johann Tobias 1770 51 KRIEGER, Johann 1912 34 SAVOY, Gaspare 1770 71 LE MORVAN, Charles 1914 37 EULER, Leonhard 1772 16 WEGENER, Alfred 1921 83 MAYER, Johann Tobias 1775 52 GOODACRE, Walter 1931 24 SCHRÖTER, Johann Hieronymus 1791 76 FAUTH, Philipp 1932 19 GRUITHUISEN, Franz von Paula 1825 25 WILKINS, Hugh Percy 1937 86 LOHRMANN, Wilhelm Gotthelf 1824 41 USSR ACADEMY 1959 1 BEER, Wilhelm 1834 4 ARTHUR, David 1960 3 BEER, Wilhelm 1837 5 HACKMAN, Robert 1960 27 MÄDLER, Johann Heinrich 1837 49 KUIPER Gerard P.
    [Show full text]
  • The Minor Planet Bulletin
    THE MINOR PLANET BULLETIN OF THE MINOR PLANETS SECTION OF THE BULLETIN ASSOCIATION OF LUNAR AND PLANETARY OBSERVERS VOLUME 36, NUMBER 3, A.D. 2009 JULY-SEPTEMBER 77. PHOTOMETRIC MEASUREMENTS OF 343 OSTARA Our data can be obtained from http://www.uwec.edu/physics/ AND OTHER ASTEROIDS AT HOBBS OBSERVATORY asteroid/. Lyle Ford, George Stecher, Kayla Lorenzen, and Cole Cook Acknowledgements Department of Physics and Astronomy University of Wisconsin-Eau Claire We thank the Theodore Dunham Fund for Astrophysics, the Eau Claire, WI 54702-4004 National Science Foundation (award number 0519006), the [email protected] University of Wisconsin-Eau Claire Office of Research and Sponsored Programs, and the University of Wisconsin-Eau Claire (Received: 2009 Feb 11) Blugold Fellow and McNair programs for financial support. References We observed 343 Ostara on 2008 October 4 and obtained R and V standard magnitudes. The period was Binzel, R.P. (1987). “A Photoelectric Survey of 130 Asteroids”, found to be significantly greater than the previously Icarus 72, 135-208. reported value of 6.42 hours. Measurements of 2660 Wasserman and (17010) 1999 CQ72 made on 2008 Stecher, G.J., Ford, L.A., and Elbert, J.D. (1999). “Equipping a March 25 are also reported. 0.6 Meter Alt-Azimuth Telescope for Photometry”, IAPPP Comm, 76, 68-74. We made R band and V band photometric measurements of 343 Warner, B.D. (2006). A Practical Guide to Lightcurve Photometry Ostara on 2008 October 4 using the 0.6 m “Air Force” Telescope and Analysis. Springer, New York, NY. located at Hobbs Observatory (MPC code 750) near Fall Creek, Wisconsin.
    [Show full text]
  • COURT of CLAIMS of THE
    REPORTS OF Cases Argued and Determined IN THE COURT of CLAIMS OF THE STATE OF ILLINOIS VOLUME 39 Containing cases in which opinions were filed and orders of dismissal entered, without opinion for: Fiscal Year 1987 - July 1, 1986-June 30, 1987 SPRINGFIELD, ILLINOIS 1988 (Printed by authority of the State of Illinois) (65655--300-7/88) PREFACE The opinions of the Court of Claims reported herein are published by authority of the provisions of Section 18 of the Court of Claims Act, Ill. Rev. Stat. 1987, ch. 37, par. 439.1 et seq. The Court of Claims has exclusive jurisdiction to hear and determine the following matters: (a) all claims against the State of Illinois founded upon any law of the State, or upon an regulation thereunder by an executive or administrative ofgcer or agency, other than claims arising under the Workers’ Compensation Act or the Workers’ Occupational Diseases Act, or claims for certain expenses in civil litigation, (b) all claims against the State founded upon any contract entered into with the State, (c) all claims against the State for time unjustly served in prisons of this State where the persons imprisoned shall receive a pardon from the Governor stating that such pardon is issued on the grounds of innocence of the crime for which they were imprisoned, (d) all claims against the State in cases sounding in tort, (e) all claims for recoupment made by the State against any Claimant, (f) certain claims to compel replacement of a lost or destroyed State warrant, (g) certain claims based on torts by escaped inmates of State institutions, (h) certain representation and indemnification cases, (i) all claims pursuant to the Law Enforcement Officers, Civil Defense Workers, Civil Air Patrol Members, Paramedics and Firemen Compensation Act, (j) all claims pursuant to the Illinois National Guardsman’s and Naval Militiaman’s Compensation Act, and (k) all claims pursuant to the Crime Victims Compensation Act.
    [Show full text]
  • June 9, 2020 LIST of ABSENTEE VOTERS HOLDING BALLOTS – NAMES
    WARSAW CENTRAL SCHOOL BUDGET/BOARD VOTE – June 9, 2020 LIST OF ABSENTEE VOTERS HOLDING BALLOTS – NAMES Abbasey, Salman Aumer, Andrew J. Bauer, James E. Abbott, John Axtell, Paula A. Bauer, Janet M. Ackerman, James Backlas, Frederick A. Jr Bauer, Michael Ackerman, Susan M. Bagg , Robert L. Bauer, Michelle Adolf, Jeremy J. Bagg, Kenneth G. Baxter, Susan Agrawal, Rajendra Bagg, Patty Bayliss, Bruce A. Aguado, Andrew E. Bagley, Raymond F. Bayoumi, Ahmed Ahl, Florence Bailey, Betty J. Beach, Douglas A. Aker, James D. Bailey, Judith L. Beach, Robert L. Akin, Claudia J. Bailey, Lyndsay Beals, Duane M. Alband, Jeffrey L. Bailey, Richard L. Beals, Shane Alcaraz, Christina M. Bailey, Stephen Beardsley, Peter G. Alderson, Donald P. Bailey, Stephen Beck, Michael J. Aldinger, Suzanne Bailey, Tara L. Beckstrand, Benjamine C. Aldrich, Heather L. Baize, Mary A. Beckstrand, Denise C. Aldrich, Jordan A. Baker, Arlene W. Beilein, Paul T. Aldrich, Kathryn J. Baker, Charles O. Beinhauer, Joseph F. Alexander, Christopher J. Baker, Frederic Belden, Barbara A. Alexander, Tara Baker, Gregory S. Belden, James C. Allen, Patricia A. Baker, Karen Bell, David K. Allison, Eddie R. Baker, Kirk E. Bell, Kathleen D. Almeter, David J Baker, Kristina Bell, Lorraine F. Almeter, George Anna Baker, Nichlos Bell, Milda Almeter, Nathan A. Baker, Peggy J. Bell, Mildred E. Almeter, Steven A. Baker, Roger O. Bellaire, Donald Ames, Gregory K. Baker, Shawn R. Bellaire, Donald W. Sr Ames, Richard A. Bakowski, Christopher Belles, Cody J. Andalora, Ingeburg Ballard, Joanne R. Bellinger, Heather Andalora, Orah Ballerstein, Lisa Bender, Gloria Andrews, Lee H. Ballew, Marjorie Bender, Sidney Antinore, Hope Bannister, Jeffrey H.
    [Show full text]
  • Planning a Mission to the Lunar South Pole
    Lunar Reconnaissance Orbiter: (Diviner) Audience Planning a Mission to Grades 9-10 the Lunar South Pole Time Recommended 1-2 hours AAAS STANDARDS Learning Objectives: • 12A/H1: Exhibit traits such as curiosity, honesty, open- • Learn about recent discoveries in lunar science. ness, and skepticism when making investigations, and value those traits in others. • Deduce information from various sources of scientific data. • 12E/H4: Insist that the key assumptions and reasoning in • Use critical thinking to compare and evaluate different datasets. any argument—whether one’s own or that of others—be • Participate in team-based decision-making. made explicit; analyze the arguments for flawed assump- • Use logical arguments and supporting information to justify decisions. tions, flawed reasoning, or both; and be critical of the claims if any flaws in the argument are found. • 4A/H3: Increasingly sophisticated technology is used Preparation: to learn about the universe. Visual, radio, and X-ray See teacher procedure for any details. telescopes collect information from across the entire spectrum of electromagnetic waves; computers handle Background Information: data and complicated computations to interpret them; space probes send back data and materials from The Moon’s surface thermal environment is among the most extreme of any remote parts of the solar system; and accelerators give planetary body in the solar system. With no atmosphere to store heat or filter subatomic particles energies that simulate conditions in the Sun’s radiation, midday temperatures on the Moon’s surface can reach the stars and in the early history of the universe before 127°C (hotter than boiling water) whereas at night they can fall as low as stars formed.
    [Show full text]
  • Commercial Lunar Propellant Architecture a Collaborative Study of Lunar Propellant Production
    Commercial Lunar Propellant Architecture A Collaborative Study of Lunar Propellant Production 1 To the Memory of: Dr. Paul D. Spudis (1952–2018) Dr. Spudis earned his master’s degree from Brown University and his Ph.D. from Arizona State University in Geology with a focus on the Moon. His career included work at the US Geological Survey, NASA, John Hopkins University Applied Physics Laboratory, and the Lunar and Planetary Institute advocating for the exploration and the utilization of lunar resources. His work will continue to inspire and guide us all on our journey to the Moon. “By going to the Moon we can learn how to extract what we need in space from what we find in space. Fundamentally that is a skill that any spacefaring civilization has to master. If you can learn to do that, you’ve got a skill that will allow you to go to Mars and beyond.” ii Authors David Kornuta, United Launch Alliance, CisLunar Project Lead1 Angel Abbud-Madrid, Colorado School of Mines, Professor of Space Resources Jared Atkinson, Honeybee Robotics, Senior Geophysical Engineer Jonathan Barr, United Launch Alliance, Program Manager Gary Barnhard, Xtraordinary Innovative Space Partnership, CEO Dallas Bienhoff, Cislunar Space Development Company LLC, Founder Brad Blair, NewSpace Analytics, Managing Partner Vanessa Clark, Atomos Nuclear and Space, Chief Executive and Technology Officer Justin Cyrus, Lunar Outpost, CEO Blair DeWitt, Lunar Station Corporation, CEO and Co-Founder Chris Dreyer, Colorado School of Mines, Professor of Space Resources Barry Finger, Paragon
    [Show full text]
  • Planetary Science : a Lunar Perspective
    APPENDICES APPENDIX I Reference Abbreviations AJS: American Journal of Science Ancient Sun: The Ancient Sun: Fossil Record in the Earth, Moon and Meteorites (Eds. R. 0.Pepin, et al.), Pergamon Press (1980) Geochim. Cosmochim. Acta Suppl. 13 Ap. J.: Astrophysical Journal Apollo 15: The Apollo 1.5 Lunar Samples, Lunar Science Insti- tute, Houston, Texas (1972) Apollo 16 Workshop: Workshop on Apollo 16, LPI Technical Report 81- 01, Lunar and Planetary Institute, Houston (1981) Basaltic Volcanism: Basaltic Volcanism on the Terrestrial Planets, Per- gamon Press (1981) Bull. GSA: Bulletin of the Geological Society of America EOS: EOS, Transactions of the American Geophysical Union EPSL: Earth and Planetary Science Letters GCA: Geochimica et Cosmochimica Acta GRL: Geophysical Research Letters Impact Cratering: Impact and Explosion Cratering (Eds. D. J. Roddy, et al.), 1301 pp., Pergamon Press (1977) JGR: Journal of Geophysical Research LS 111: Lunar Science III (Lunar Science Institute) see extended abstract of Lunar Science Conferences Appendix I1 LS IV: Lunar Science IV (Lunar Science Institute) LS V: Lunar Science V (Lunar Science Institute) LS VI: Lunar Science VI (Lunar Science Institute) LS VII: Lunar Science VII (Lunar Science Institute) LS VIII: Lunar Science VIII (Lunar Science Institute LPS IX: Lunar and Planetary Science IX (Lunar and Plane- tary Institute LPS X: Lunar and Planetary Science X (Lunar and Plane- tary Institute) LPS XI: Lunar and Planetary Science XI (Lunar and Plane- tary Institute) LPS XII: Lunar and Planetary Science XII (Lunar and Planetary Institute) 444 Appendix I Lunar Highlands Crust: Proceedings of the Conference in the Lunar High- lands Crust, 505 pp., Pergamon Press (1980) Geo- chim.
    [Show full text]