Introduction: Writing About Twentieth Century Geology
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Timeline of Natural History
Timeline of natural history This timeline of natural history summarizes significant geological and Life timeline Ice Ages biological events from the formation of the 0 — Primates Quater nary Flowers ←Earliest apes Earth to the arrival of modern humans. P Birds h Mammals – Plants Dinosaurs Times are listed in millions of years, or Karo o a n ← Andean Tetrapoda megaanni (Ma). -50 0 — e Arthropods Molluscs r ←Cambrian explosion o ← Cryoge nian Ediacara biota – z ←Earliest animals o ←Earliest plants i Multicellular -1000 — c Contents life ←Sexual reproduction Dating of the Geologic record – P r The earliest Solar System -1500 — o t Precambrian Supereon – e r Eukaryotes Hadean Eon o -2000 — z o Archean Eon i Huron ian – c Eoarchean Era ←Oxygen crisis Paleoarchean Era -2500 — ←Atmospheric oxygen Mesoarchean Era – Photosynthesis Neoarchean Era Pong ola Proterozoic Eon -3000 — A r Paleoproterozoic Era c – h Siderian Period e a Rhyacian Period -3500 — n ←Earliest oxygen Orosirian Period Single-celled – life Statherian Period -4000 — ←Earliest life Mesoproterozoic Era H Calymmian Period a water – d e Ectasian Period a ←Earliest water Stenian Period -4500 — n ←Earth (−4540) (million years ago) Clickable Neoproterozoic Era ( Tonian Period Cryogenian Period Ediacaran Period Phanerozoic Eon Paleozoic Era Cambrian Period Ordovician Period Silurian Period Devonian Period Carboniferous Period Permian Period Mesozoic Era Triassic Period Jurassic Period Cretaceous Period Cenozoic Era Paleogene Period Neogene Period Quaternary Period Etymology of period names References See also External links Dating of the Geologic record The Geologic record is the strata (layers) of rock in the planet's crust and the science of geology is much concerned with the age and origin of all rocks to determine the history and formation of Earth and to understand the forces that have acted upon it. -
Argon Ages and Geochemistry of Lunar Breccias 67016 and 67455
Available online at www.sciencedirect.com Geochimica et Cosmochimica Acta 74 (2010) 763–783 www.elsevier.com/locate/gca Imbrium provenance for the Apollo 16 Descartes terrain: Argon ages and geochemistry of lunar breccias 67016 and 67455 M.D. Norman a,b,*, R.A. Duncan c, J.J. Huard c a Research School of Earth Sciences, Australian National University, Canberra 0200, Australia b Lunar and Planetary Institute, 3600 Bay Area Boulevard, Houston TX 77058, USA c College of Oceanic and Atmospheric Sciences, Oregon State University, Corvallis, OR 97331, USA Received 23 January 2009; accepted in revised form 16 September 2009; available online 21 October 2009 Abstract In order to improve our understanding of impact history and surface geology on the Moon, we obtained 40Ar–39Ar incre- mental heating age data and major + trace element compositions of anorthositic and melt breccia clasts from Apollo 16 feld- spathic fragmental breccias 67016 and 67455. These breccias represent the Descartes terrain, a regional unit often proposed to be ejecta from the nearby Nectaris basin. The goal of this work is to better constrain the emplacement age and provenance of the Descartes breccias. Four anorthositic clasts from 67016 yielded well-defined 40Ar–39Ar plateau ages ranging from 3842 ± 19 to 3875 ± 20 Ma. Replicate analyses of these clasts all agree within measurement error, with only slight evidence for either inheritance or youn- ger disturbance. In contrast, fragment-laden melt breccia clasts from 67016 yielded apparent plateau ages of 4.0–4.2 Ga with indications of even older material (to 4.5 Ga) in the high-T fractions. -
GSA TODAY • Employment Service, P
Vol. 7, No. 7 July 1997 INSIDE • Call for Editors, p. 15 GSA TODAY • Employment Service, p. 21 • 1997 GSA Annual Meeting, p. 28 A Publication of the Geological Society of America Evidence for Life in a Martian Meteorite? Harry Y. McSween, Jr. Department of Geological Sciences, University of Tennessee, Knoxville, TN 37996 ABSTRACT The controversial hypothesis that the ALH84001 mete- orite contains relics of ancient martian life has spurred new findings, but the question has not yet been resolved. Organic matter probably results, at least in part, from terrestrial contamination by Antarctic ice meltwater. The origin of nanophase magnetites and sulfides, suggested, on the basis of their sizes and morphologies, to be biogenic remains con- tested, as does the formation temperature of the carbonates that contain all of the cited evidence for life. The reported nanofossils may be magnetite whiskers and platelets, proba- bly grown from a vapor. New observations, such as the possi- ble presence of biofilms and shock metamorphic effects in the carbonates, have not yet been evaluated. Regardless of the ultimate conclusion, this controversy continues to help define strategies and sharpen tools that will be required for a Mars exploration program focused on the search for life. INTRODUCTION Since the intriguing proposal last summer that martian mete- orite Allan Hills (ALH) 84001 contains biochemical markers, bio- genic minerals, and microfossils (McKay et al., 1996), scientists and the public alike have been treated to a variety of claims sup- porting or refuting this hypothesis. Occasionally, the high visibil- ity of the controversy has overshadowed the research effort (e.g., Begley and Rogers, 1997), but I believe that science will benefit significantly from this experience. -
Workshop on Moon in Transition: Apollo 14, Kreep, and Evolved Lunar Rocks
WORKSHOP ON MOON IN TRANSITION: APOLLO 14, KREEP, AND EVOLVED LUNAR ROCKS (NASA-CR-I"'-- N90-I_02o rRAN31TION: APJLLN l_p KRFEP, ANu _VOLVFD LUNAR ROCKS (Lunar and Pl_net3ry !nst.) I_7 p C_CL O3B Unclas G3/91 0253133 LPI Technical Report Number 89-03 UNAR AND PLANETARY INSTITUTE 3303 NASA ROAD 1 HOUSTON, TEXAS 77058-4399 7 WORKSHOP ON MOON IN TRANSITION: APOLLO 14, KREEP, AND EVOLVED LUNAR ROCKS Edited by G. J. Taylor and P. H. Warren Sponsored by Lunar and Planetary Institute NASA Johnson Space Center November 14-16, 1988 Houston, Texas Lunar and Planetary Institute 330 ?_NASA Road 1 Houston, Texas 77058-4399 LPI Technical Report Number 89-03 Compiled in 1989 by the LUNAR AND PLANETARY INSTITUTE The Institute is operated by Universities Space Research Association under Contract NASW-4066 with the National Aeronautics and Space Administration. Material in this document may be copied without restraint for Library, abstract service, educational, or personal research purposes; however, republication of any portion requires the written permission of the authors as well as appropriate acknowledgment of this publication. This report may be cited as: Taylor G. J. and Warren PI H., eds. (1989) Workshop on Moon in Transition: Apo{l_ 14 KREEP, and Evolved Lunar Rocks. [PI Tech. Rpt. 89-03. Lunar and Planetary Institute, Houston. 156 pp. Papers in this report may be cited as: Author A. A. (1989) Title of paper. In W_nkshop on Moon in Transition: Ap_llo 14, KREEP, and Evolved Lunar Rocks (G. J. Taylor and P. H. Warren, eds.), pp. xx-yy. LPI Tech. Rpt. -
Famous Geologist Fact Sheet Your Job Is to Research Information About
Famous Geologist Fact Sheet Your job is to research information about one of the geologists on the list and arrange the information you find into a fact sheet about that person. The fact sheet should only be one side of an 8 ½ x 11 inch paper. Include all of the following information about the scientist. You may turn your project into a wanted poster if you want starting your paper with “Be on the lookout for this man/woman. Wanted for ___________.” You may use bulleted lists where appropriate. A. Give the scientists full name – first, middle, last B. When they were born and when they died (if applicable) C. Where they were born – country, state, city D. Where they grew up if different from where they were born E. Family information – parents, siblings, wife, children F. Where they went to school – elementary, high school, college G. What they did for a job H. What they studied – field of expertise - give a complete description of what they studied I. What they are famous for specifically – include how their contributions affect us now and/or will in the future J. A quote from your scientist if you can find one K. Any other interesting facts about your scientist L. A picture of the scientist – not a cartoon M. A picture pertaining to what they are famous for N. List of important publications by the scientist O. List any awards given and the dates they were given to your scientist for their contributions to science P. Cite your source or sources according to the MLA Style Your grade will be determined by: * Overall presentation, neatness and creativity. -
Workshop on Geology of the Apollo 17 Landing Site
NASA-CR-191637 \ WORKSHOP ON GEOLOGY OF THE APOLLO 17 LANDING SITE (NASA-CR-191637) WORKSHOP ON N93-18786 GEOLOGY OF THE APOLLO 17 LANDING --THRU-- SITE (Lunar Science Inst.) 70 p N93-18817 Unclas G3/91 0141290 __ LPI Technical Report Number 92-09, Part 1 LUNAR AND PLANETARY INSTITUTE 3600 BAY AREA BOULEVARD HOUSTON TX 77058-1113 LPI/TR--92-09, Part 1 WORKSHOP ON GEOLOGY OF THE APOLLO 17 LANDING SITE Edited by G. Ryder, H. H. Schmitt, and P. D. Spudis Held at Houston, Texas December 2-4, 1992 Sponsored by Lunar and Planetary Sample Team Lunar and Planetary Institute Lunar and Planetary Institute 3600 Bay Area Boulevard Houston TX 77058-1113 LPI Technical Report Number 92-09, Part 1 LPI/TR--92-09, Part 1 Compiledin 1992by LUNAR AND PLANETARY INSTITUTE TheInstituteis operatedby theUniversitySpaceResearchAssociationunderContractNo. NASW- 4574with theNationalAeronauticsandSpaceAdministration. Materialin this volume may be copied without restraint for library, abstract service, education, or per- sonal research purposes; however, republication of any paper or portion thereof requires the written permission of the authors as well as the appropriate acknowledgment of this publication. This report may be cited as Ryder G., Schmitt H. H., and Spudis P. D., eds. (1992) Workshop on Geology of the Apollo 17 Landing Site. LPI Tech. Rpt. 92-09, Part 1, Lunar and Planetary Institute, Houston. 63 pp. This report is distributed by ORDER DEPARTMENT Lunar and Planetary Institute 3600 Bay Area Boulevard Houston TX 77058-1113 Mail order requestors will be invoiced for the cost of shipping and handling. Cover: Station 4 at Taurus-LiUrow, Apollo 17 landing site. -
Vm Goldschmidt
NORSK GEOLOGISK TIDSSKRIFT 27. 143 V. M. GOLD SCHMIDT Minnetale i Norsk geologisk forening 10. april 1947 Av IVAR OFTEDAL Med professor V. M. Goldschmidts død den 20. mars 1947 var det en av våre store, en vitenskapsmann av verdensformat, som gikk bort. Han døde av hjerneblødning i sitt hjem i Vestre Aker umid delbart etter at han var kommet hjem fra sykehus etter en mindre operasjon. I de siste årene var hans helbred meget dårlig, og en sterkt medvirkende årsak til dette var utvilsomt den voldsomme nerve påkjenning han var utsatt for i de første okkupasjonsårene her i Oslo. Da jødeforfølgelsen her antok åpenlyse former var hans stilling lite misunnelsesverdig. Han ble innkalt til forhør på Victoria Terrasse, senere arrestert og sendt til Berg med en av de beryktete jødetran sporter ennå før Berg-leiren hadde det nødtørftigste utstyr til å ta imot fanger. Her ble han alvorlig syk og kom heldigvis snart på Tønsberg sykehus, hvorfra han fikk reise hjem. Men trygg følte han seg ikke, og det hadde han heller ikke grunn til. Snart ble han, tross alle forsikringer, arrestert igjen, og denne gangen kom han helt til landgangen på vei ombord i et av jødetransportskipene til Tysk land, da han plutselig fikk beskjed om at han var fri. Etter disse opplevelser var Goldschmidts nervesystem, som rimelig kan være, temmelig nedbrutt, og det endte med at han straks før jul 1942 ble med en transport til Sverige. Etter et opphold her kom han over til Storbritannia, hvor han først var en tid i Skottland, siden ved Rothamsted Experimental Station i Harpenden nær London. -
Timeline of Natural History
Timeline of natural history Main articles: History of the Earth and Geological his- chondrules,[1] are a key signature of a supernova ex- tory of Earth plosion. See also: Geologic time scale and Timeline of evolution- ary history of life • 4,567±3 Ma: Rapid collapse of hydrogen molecular For earlier events, see Timeline of the formation of the cloud, forming a third-generation Population I star, Universe. the Sun, in a region of the Galactic Habitable Zone This timeline of natural history summarizes signifi- (GHZ), about 25,000 light years from the center of the Milky Way Galaxy.[2] • 4,566±2 Ma: A protoplanetary disc (from which Earth eventually forms) emerges around the young Sun, which is in its T Tauri stage. • 4,560–4,550 Ma: Proto-Earth forms at the outer (cooler) edge of the habitable zone of the Solar Sys- tem. At this stage the solar constant of the Sun was only about 73% of its current value, but liquid wa- ter may have existed on the surface of the Proto- Earth, probably due to the greenhouse warming of high levels of methane and carbon dioxide present in the atmosphere. Early bombardment phase begins: because the solar neighbourhood is rife with large planetoids and debris, Earth experiences a number of giant impacts that help to increase its overall size. Visual representation of the history of life on Earth as a spiral 2 Hadean Eon cant geological and biological events from the formation of the Earth to the rise of modern humans. Times are listed in millions of years, or megaanni (Ma). -
Field Trip B2: Triassic to Early Cretaceous Geodynamic History of the Central Northern Calcareous Alps (Northwestern Tethyan Realm)
ZOBODAT - www.zobodat.at Zoologisch-Botanische Datenbank/Zoological-Botanical Database Digitale Literatur/Digital Literature Zeitschrift/Journal: Berichte der Geologischen Bundesanstalt Jahr/Year: 2013 Band/Volume: 99 Autor(en)/Author(s): Gawlick Hans-Jürgen, Missoni Sigrid Artikel/Article: Field Trip B2: Triassic to Early Cretaceous geodynamic history of the central Northern Calcareous Alps (Northwestern Tethyan realm). 216-270 ©Geol. Bundesanstalt, Wien; download unter www.geologie.ac.at Berichte Geol. B.-A., 99 11th Workshop on Alpine Geological Studies & 7th IFAA Field Trip B2: Triassic to Early Cretaceous geodynamic history of the central Northern Calcareous Alps (Northwestern Tethyan realm) Hans-Jürgen Gawlick & Sigrid Missoni University of Leoben, Department of Applied Geosciences and Geophysics, Petroleum Geology, Peter-Tunner-Strasse 5, 8700 Leoben, Austria Content Abstract 1 Introduction 2 Overall geodynamic and sedimentary evolution 3 Palaeogeography, sedimentary successions and stratigraphy 3.1 Hauptdolomit facies zone 3.2 Dachstein Limestone facies zone 3.3 Hallstatt facies zone (preserved in the reworked Jurassic Hallstatt Mélange) 4 The Field Trip 4.1 The Late Triassic Dachstein/Hauptdolomit Carbonate Platform 4.1.1 Hauptdolomit (Mörtlbach road) 4.1.2 Lagoonal Dachstein Limestone: The classical Lofer cycle (Pass Lueg) 4.1.3 The Kössen Basin (Pass Lueg and Mörtlbach road) 4.2 Jurassic evolution 4.2.1 Hettangian to Aalenian 4.2.2 Bajocian to Tithonian 4.3 Early Cretaceous References Abstract The topic of this field trip is to get to know and understand the sedimentation of Austria’s Northern Calcareous Alps and its tectonic circumstances from Triassic rifting/drifting to Jurassic collision/accretion, and the Early Cretaceous “post-tectonic” sedimentary history. -
Mesozoic Basins and Associated Palaeogeographic Evolution in North China
Journal of Palaeogeography 2015, 4(2): 189-202 DOI: 10.3724/SP.J.1261.2015.00073 Tectonopalaeogeography andPalaeogeography palaeotectonics Mesozoic basins and associated palaeogeographic evolution in North China Yong-Qing Liu*, Hong-Wei Kuang, Nan Peng, Huan Xu, Peng Zhang, Neng-Sheng Wang, Wei An* Institute of Geology, Chinese Academy of Geological Sciences, Beijing 100037, China Abstract In North China, the Mesozoic terrestrial basins, sedimentary palaeogeography and tectonic settings involved five evolutionary stages: (1) the Early-Middle Triassic, (2) the Late Triassic to Early-Middle Jurassic, (3) the Late Jurassic to early Early Cretaceous, (4) the middle-late Early Cretaceous and (5) the Late Cretaceous. The regional punctuated tectonic events occurred during these evolutionary stages. During the Early-Middle Triassic (stage 1), the Xingmeng Orogenic Belt (XMOB, i.e., east- ern part of Central Asia Orogenic Belt, CAOB) of the northern North China was settled in the transition of tectonic environment from syn-orogenic compression to post-orogenic extension with intensive uplifting. It is a main provenance in the unified Ordos-North China Basin.The united continental plate of China and the Qinling-Dabie-Sulu Orogenic Belt formed due to convergence and collision between the North China Plate and the Yangtze Plate along two suture zones of the Mianlue and the Shangdan in the terminal Middle Triassic. During the Late Triassic to the Early-Middle Jurassic (stage 2), the Late Triassic mafic or alkaline rocks and intrusions occurred on the northern and southern margins of North China Craton (NCC) and XMOB, implying that intensified extension happened all over the North China (early phase of stage 2). -
WM White Geochemistry Chapter 7: Trace Elements
W. M. White Geochemistry Chapter 7: Trace Elements Chapter 7: Trace Elements in Igneous Processes 7.1 INTRODUCTION n this chapter we will consider the behavior of trace elements, particularly in magmas, and in- troduce methods to model this behavior. Though trace elements, by definition, constitute only a I small fraction of a system of interest, they provide geochemical and geological information out of proportion to their abundance. There are several reasons for this. First, variations in the concentrations of many trace elements are much larger than variations in the concentrations of major components, of- ten by many orders of magnitude. Second, in any system there are far more trace elements than major elements. In most geochemical systems, there are 10 or fewer major components that together account for 99% or more of the system. This leaves 80 trace elements. Each element has chemical properties that are to some degree unique, hence there is unique geochemical information contained in the varia- tion of concentration for each element. Thus the 80 trace elements always contain information not available from the variations in the concentrations of major elements. Third, the range in behavior of trace elements is large and collectively they are sensitive to processes to which major elements are in- sensitive. One example is the depth at which partial melting occurs in the mantle. When the mantle melts, it produces melts whose composition is only weakly dependent on pressure, i.e., it always pro- duces basalt. Certain trace elements, however, are highly sensitive to the depth of melting (because the phase assemblages are functions of pressure). -
Geological Survey of Denmark and Greenland Bulletin 26, 2012
GEOLOGICAL SURVEY OF DENMARK AND GREENLAND BULLETIN 26 • 2012 Review of Survey activities 2011 Edited by Ole Bennike, Adam A. Garde and W. Stuart Watt GEOLOGICAL SURVEY OF DENMARK AND GREENLAND MINISTRY OF CLIMATE, ENERGY AND BUILDING 1 Geological Survey of Denmark and Greenland Bulletin 26 Keywords Geological Survey of Denmark and Greenland, survey organisations, current research, Denmark, Greenland. Cover photographs from left to right 1. Retrieving a sediment core in Sermilik fjord, South-East Greenland. Photograph: Robert S. Fausto. 2. Field work in Vietnam. Photograph: Flemming Larsen. 3. This Danish beech forest on Fyn was farm land during the Iron Age. Photograph: Ole Bennike. 4. Small-scale miners in Nigeria. Worldwide, c. 100 million people depend on small-scale mining. Photograph: John Tychsen. Frontispiece: facing page In the summer of 2011, GEUS carried out extensive reconnaissance work in South-East Greenland. The aim is to assess the mineral potential of the region, which is one of the least known regions of Greenland. The geologist is panning stream sediments in order to separate heavy minerals, possibly including gold. Photograph: Jakob Lautrup. Chief editor of this series: Adam A. Garde Editorial board of this series: John A. Korstgård, Department of Geoscience, Aarhus University; Minik Rosing, Geological Museum, University of Copenhagen; Finn Surlyk, Department of Geography and Geology, University of Copenhagen Scientific editors: Ole Bennike, Adam A. Garde and W. Stuart Watt Editorial secretaries: Jane Holst and Esben