GSA TODAY February and University of California, Berkeley Serves to Strengthen PEP by Providing Vol
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History of Geology
FEBRUARY 2007 PRIMEFACT 563 (REPLACES MINFACT 60) History of geology Mineral Resources Early humans needed a knowledge of simple geology to enable them to select the most suitable rock types both for axe-heads and knives and for the ornamental stones they used in worship. In the Neolithic and Bronze Ages, about 5000 to 2500 BC, flint was mined in the areas which are now Belgium, Sweden, France, Portugal and Britain. While Stone Age cultures persisted in Britain until after 2000 BC, in the Middle East people began to mine useful minerals such as iron ore, tin, clay, gold and copper as early as 4000 BC. Smelting techniques were developed to make the manufacture of metal tools possible. Copper was probably the earliest metal to be smelted, that is, extracted from its ore by melting. Copper is obtained easily by reducing the green copper carbonate mineral malachite, itself regarded as a precious stone. From 4000 BC on, the use of clay for brick-making became widespread. The Reverend William Branwhite Clarke (1798-1878), smelting of iron ore for making of tools and the ‘father’ of geology in New South Wales weapons began in Asia Minor at about 1300 BC but did not become common in Western Europe until Aristotle believed volcanic eruptions and nearly 500 BC. earthquakes were caused by violent winds escaping from the interior of the earth. Since earlier writers had ascribed these phenomena to The classical period supernatural causes, Aristotle's belief was a By recognising important surface processes at marked step forward. Eratosthenes, a librarian at work, the Greek, Arabic and Roman civilisations Alexandria at about 200 BC, made surprisingly contributed to the growth of knowledge about the accurate measurements of the circumference of earth. -
Of Vertebrate Fossils from the Middle Eocene Oil Shale of Messel, Germany: Implications for Their Taphonomy and Palaeoenvironment
Palaeogeography, Palaeoclimatology, Palaeoecology 416 (2014) 92–109 Contents lists available at ScienceDirect Palaeogeography, Palaeoclimatology, Palaeoecology journal homepage: www.elsevier.com/locate/palaeo Isotope compositions (C, O, Sr, Nd) of vertebrate fossils from the Middle Eocene oil shale of Messel, Germany: Implications for their taphonomy and palaeoenvironment Thomas Tütken ⁎ Steinmann-Institut für Geologie, Mineralogie und Paläontologie, Universität Bonn, Poppelsdorfer Schloss, 53115 Bonn, Germany article info abstract Article history: The Middle Eocene oil shale deposits of Messel are famous for their exceptionally well-preserved, articulated 47- Received 15 April 2014 Myr-old vertebrate fossils that often still display soft tissue preservation. The isotopic compositions (O, C, Sr, Nd) Received in revised form 30 July 2014 were analysed from skeletal remains of Messel's terrestrial and aquatic vertebrates to determine the condition of Accepted 5 August 2014 geochemical preservation. Authigenic phosphate minerals and siderite were also analysed to characterise the iso- Available online 17 August 2014 tope compositions of diagenetic phases. In Messel, diagenetic end member values of the volcanically-influenced 12 Keywords: and (due to methanogenesis) C-depleted anoxic bottom water of the meromictic Eocene maar lake are isoto- Strontium isotopes pically very distinct from in vivo bioapatite values of terrestrial vertebrates. This unique taphonomic setting al- Oxygen isotopes lows the assessment of the geochemical preservation of the vertebrate fossils. A combined multi-isotope Diagenesis approach demonstrates that enamel of fossil vertebrates from Messel is geochemically exceptionally well- Enamel preserved and still contains near-in vivo C, O, Sr and possibly even Nd isotope compositions while bone and den- Messel tine are diagenetically altered. -
Alaska Regional Directors Offices Director Email Address Contact Numbers Supt
Alaska Regional Directors Offices Director Email Address Contact Numbers Supt. Phone Fax Code ABLI RegionType Unit U.S Fish and Wildlife Service (FWS) Alaska Region (FWS) HASKETT,GEOFFREY [email protected] 1011 East Tudor Road Phone: 907‐ 786‐3309 Anchorage, AK 99503 Fax: 907‐ 786‐3495 Naitonal Park Service(NPS) Alaska Region (NPS) MASICA,SUE [email protected] 240 West 5th Avenue,Suite 114 Phone:907‐644‐3510 Anchoorage,AK 99501 Bureau of Indian Affairs(BIA) Alaska Region (BIA) VIRDEN,EUGENE [email protected] Bureau of Indian Affairs Phone: 907‐586‐7177 PO Box 25520 Telefax: 907‐586‐7252 709 West 9th Street Juneau, AK 99802 Anchorage Agency Phone: 1‐800‐645‐8465 Bureau of Indian Affairs Telefax:907 271‐4477 3601 C Street Suite 1100 Anchorage, AK 99503‐5947 Telephone: 1‐800‐645‐8465 Bureau of Land Manangement (BLM) Alaska State Office (BLM) CRIBLEY,BUD [email protected] Alaska State Office Phone: 907‐271‐5960 222 W 7th Avenue #13 FAX: 907‐271‐3684 Anchorage, AK 99513 United States Geological Survey(USGS) Alaska Area (USGS) BARTELS,LESLIE lholland‐[email protected] 4210 University Dr., Anchorage, AK 99508‐4626 Phone:907‐786‐7055 Fax: 907‐ 786‐7040 Bureau of Ocean Energy Management(BOEM) Alaska Region (BOEM) KENDALL,JAMES [email protected] 3801 Centerpoint Drive Phone: 907‐ 334‐5208 Suite 500 Anchorage, AK 99503 Ralph Moore [email protected] c/o Katmai NP&P (907) 246‐2116 ANIA ANTI AKR NPRES ANIAKCHAK P.O. Box 7 King Salmon, AK 99613 (907) 246‐3305 (907) 246‐2120 Jeanette Pomrenke [email protected] P.O. -
No. 40. the System of Lunar Craters, Quadrant Ii Alice P
NO. 40. THE SYSTEM OF LUNAR CRATERS, QUADRANT II by D. W. G. ARTHUR, ALICE P. AGNIERAY, RUTH A. HORVATH ,tl l C.A. WOOD AND C. R. CHAPMAN \_9 (_ /_) March 14, 1964 ABSTRACT The designation, diameter, position, central-peak information, and state of completeness arc listed for each discernible crater in the second lunar quadrant with a diameter exceeding 3.5 km. The catalog contains more than 2,000 items and is illustrated by a map in 11 sections. his Communication is the second part of The However, since we also have suppressed many Greek System of Lunar Craters, which is a catalog in letters used by these authorities, there was need for four parts of all craters recognizable with reasonable some care in the incorporation of new letters to certainty on photographs and having diameters avoid confusion. Accordingly, the Greek letters greater than 3.5 kilometers. Thus it is a continua- added by us are always different from those that tion of Comm. LPL No. 30 of September 1963. The have been suppressed. Observers who wish may use format is the same except for some minor changes the omitted symbols of Blagg and Miiller without to improve clarity and legibility. The information in fear of ambiguity. the text of Comm. LPL No. 30 therefore applies to The photographic coverage of the second quad- this Communication also. rant is by no means uniform in quality, and certain Some of the minor changes mentioned above phases are not well represented. Thus for small cra- have been introduced because of the particular ters in certain longitudes there are no good determi- nature of the second lunar quadrant, most of which nations of the diameters, and our values are little is covered by the dark areas Mare Imbrium and better than rough estimates. -
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. -
Peer Review Draft Synthesis and Assessment Product 4.2 Thresholds
1 Peer Review Draft 2 Synthesis and Assessment Product 4.2 3 Thresholds of Change in Ecosystems 4 Authors: Daniel B. Fagre (lead author), Colleen W. Charles, Craig 5 D. Allen, Charles Birkeland, F. Stuart Chapin, III, Peter M. 6 Groffman, Glenn R. Guntenspergen, Alan K. Knapp, A. David 7 McGuire, Patrick J. Mulholland, Debra P.C. Peters, Daniel D. 8 Roby, and George Sugihara 9 Contributing authors: Brandon T. Bestelmeyer, Julio L. 10 Betancourt, Jeffrey E. Herrick, and Douglas S. Kenney 11 U.S. Climate Change Science Program 12 Draft 5.0 SAP 4.2 9/26/2008 1 1 Table of Contents 2 Executive Summary............................................................................................................ 5 3 Introduction................................................................................................................... 5 4 Definitions.....................................................................................................................5 5 Development of Threshold Concepts............................................................................ 6 6 Principles of Thresholds ............................................................................................... 7 7 Case Studies.................................................................................................................. 8 8 Potential Management Responses............................................................................... 10 9 Recommendations...................................................................................................... -
Feature of the Month - August 2006
RECENT BACK ISSUES: http://www.zone-vx.com/tlo_back.html A PUBLICATION OF THE LUNAR SECTION OF THE A.L.P.O. EDITED BY: William M. Dembowski, F.R.A.S. - [email protected] Elton Moonshine Observatory - http://www.zone-vx.com 219 Old Bedford Pike (Elton) - Windber, PA 15963 FEATURE OF THE MONTH - AUGUST 2006 RHEITA E Sketch and text by Robert H. Hays, Jr. - Worth, Illinois, USA March 5, 200 - 01:15 to 01:45 UT 15cm Newtonian - 170x - Seeing 7-8/10 I sketched this crater and vicinity on the evening of March 4, 2006 after observing two occultations. This feature is located amid a jumble of craters south of Mare Fecunditatis. This is an elongated crater that appears to be the result of at least three impacts. The north and south lobes are about the same size, but the southern lobe is definitely deeper. The central portion is about the size of the north and south lobes combined. There are some bits of shadow on the floor, but I saw no obvious hills or craters there. I have drawn the shadowing within and around Rheita E as I saw it. There is an obvious ridge extending westward from the south lobe. The crater Rheita F is adjacent to the south lobe of Rheita E, and has a strip of shadow parallel to the ridge from Rheita E. Rheita M is the large, shallow crater east of Rheita E's south end, and Rheita N is the small, shallow pit between them. Stevinus D is the slightly smaller, but deeper crater north of Rheita M. -
Obituary 1967
OBITUARY INDEX 1967 You can search by clicking on the binoculars on the adobe toolbar or by Pressing Shift-Control-F Request Form LAST NAME FIRST NAME DATE PAGE # Abbate Barbara F. 6/6/1967 p.1 Abbott William W. 9/22/1967 p.30 Abel Dean 11/27/1967 p.24 Abel Francis E. 9/25/1967 p.24 Abel Francis E. 9/27/1967 p.10 Abel Frederick B. 11/11/1967 p.26 Abel John Hawk 12/7/1967 p.42 Abel John Hawk 12/11/1967 p.26 Abel William E. 7/10/1967 p.28 Abel William E. 7/12/1967 p.12 Aber George W. 3/14/1967 p.24 Abert Esther F. 7/26/1967 p.14 Abrams Laura R. Hoffman 8/14/1967 p.28 Abrams Laura R. Hoffman 8/17/1967 p.28 Abrams Pearl E. 10/19/1967 p.28 Abrams Pearl E. 10/20/1967 p.10 Achenbach Helen S. 11/6/1967 p.36 Achenbach Helen S. 11/8/1967 p.15 Ackerman Calvin 5/22/1967 p.34 Ackerman Calvin 5/25/1967 p.38 Ackerman Fritz 11/27/1967 p.24 Ackerman Harold 10/27/1967 p.26 Ackerman Harold 10/28/1967 p.26 Ackerman Hattie Mann 4/14/1967 p.21 Ackerman Hattie Mann 4/19/1967 p.14 Adamczyk Bennie 5/3/1967 p.14 Adamo Margaret M. 3/15/1967 p.15 Adamo Margaret M. 3/20/1967 p.28 Adams Anna 6/17/1967 p.22 Adams Anna 6/20/1967 p.17 Adams Harriet C. -
By DWG Arthur, Alice P. Agnieray, Ruth H. Pellicori, CA Wood, and T
No. 50 THE SYSTEM OF LUNAR CRATERS, QUADRANT III by D. W. G. Arthur, Alice P. Agnieray, Ruth H. Pellicori, C. A. Wood, and T. Weller February 25, 1965 ABSTRACT The designation, diameter, position, central peak information, and state of completeness are listed for each discernible crater with a diameter exceeding 3.5 km in the third lunar quadrant. The catalog contains about 5200 items and is illustrated by a map in 11 sections. on the averted lunar hemisphere, and therefore, these Thistem Communication of Lunar Craters, is the which third is part a catalog of The in Sys four are not listed in the catalog. parts of all craters recognizable with reasonable The approximate positions and diameters for certainty on photographs and having a diameter these craters are: greater than 3.5 km. It is thus a continuation of the work in Comm. LPL Nos. 30 and 40, and the same Long. Lat. Diam, (.00Ir) Hausen -91?5 - 6 5 ? 6 9 9 . 5 conventions and format are used. Boltzmann -96?0 - 7 5 ? 5 3 9 . 1 As in the earlier parts, it was found necessary S t e f a n - 9 4 ? 0 - 7 2 ? 0 7 8 . 0 to add names for large craters in the extreme limb regions. The new crater names for Quadrant III are: The above are mere additions to the Blagg and Miiller scheme. A more notable innovation, which Baade German-American astronomer has already been authorized by the International Boltzmann Austrian physicist Astronomical Union at its 1964 general meeting at Drygalski German geographer Hamburg, is the addition of the name Mare Cogni- Hartwig German selenodetist tum (the known sea) for the dark area between Krasnov Russian selenodetic observer Riphaeus and the crater Guerike. -
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, -
GSA TODAY • Radon in Water, P
Vol. 8, No. 11 November 1998 INSIDE • Field Guide Editor, p. 5 GSA TODAY • Radon in Water, p. 10 • Women Geoscientists, p. 12 A Publication of the Geological Society of America • 1999 Annual Meeting, p. 31 Gas Hydrates: Greenhouse Nightmare? Energy Panacea or Pipe Dream? Bilal U. Haq, National Science Foundation, Division of Ocean Science, Arlington, VA 22230 ABSTRACT Recent interest in methane hydrates has resulted from the recognition that they may play important roles in the global carbon cycle and rapid climate change through emissions of methane from marine sediments and permafrost into the atmosphere, and in causing mass failure of sediments and structural changes on the continental slope. Their presumed large volumes are also consid- ered to be a potential source for future exploitation of methane as a resource. Natural gas hydrates occur widely on continental slope and rise, stabilized in place by high hydrostatic pressure and frigid bottom-temperature condi- tions. Change in these conditions, Figure 1. This seismic profile, over the landward side of Blake Ridge, crosses a salt diapir; the profile has either through lowering of sea level or been processed to show reflection strength. The prominent bottom simulating reflector (BSR) swings increase in bottom-water temperature, upward over the diapir because of the higher conductivity of the salt. Note the very strong reflections of may trigger the following sequence of gas accumulations below the gas-hydrate stability zone and the “blanking” of energy above it. Bright events: dissociation of the hydrate at its Spots along near-vertical faults above the diapir represent conduits for gas venting. -
Origin of the Solar System
Creation Myths The rise of the monotheistic religions changed this view. When one of the gods got a higher Old Myths status than others (who in some cases became Speculation about the origin and evolution of demons or devils), he continued to increase in the earth and the celestial bodies is probably as prestige and power until he became the Supreme old as human thinking. During the millennia that Lord, the undisputed ruler of the whole world. are covered by the history of science, philosphy, Then it was not enough for him to create the world and religion we can distinguish three types of ap in the sense of organizing a preexisting chaos; he proach to this problem. had to create it all from nothing (ex nihilo) by The first is the "theocratic-myth" approach, pronouncing a magic word or by his will power. according to which the evolution of the world was This is the meaning of "creation" when we use it governed by gods who once upon a time created today, but it is a relatively new concept. It was it. However, we must remember that the meaning generally accepted in Christianity in the second of "creation" has changed. The earliest meaning century A.D. but the Genesis description of the of this term seems to have been that the gods Creation seems to have either meaning. The crea brought order into a preexisting chaos. The world tion ex nihilo was not generally accepted by the was "ungenerated and indestructible"-as Aris philosophical-scientific community until the syn totle puts it-and the gods were part of this world thesis by St.