Essor Mayer Humi, Advisor Project Number: MH-0140
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(Uth)He Age for the Shallowmarine Wetumpka Impact Structure
View metadata, citation and similar papers at core.ac.uk brought to you by CORE provided by OceanRep Meteoritics & Planetary Science 47, Nr 8, 1243–1255 (2012) doi: 10.1111/j.1945-5100.2012.01381.x An (U-Th)⁄He age for the shallow-marine Wetumpka impact structure, Alabama, USA Jo-Anne WARTHO1*, Matthijs C. van SOEST1, David T. KING, Jr.2, and Lucille W. PETRUNY2 1School of Earth and Space Exploration, Arizona State University, PO Box 876004, Tempe, Arizona 85287, USA 2Geology Office, Auburn University, Auburn, Alabama 36849, USA *Corresponding author. E-mail: [email protected] (Received 12 January 2012; revision accepted 27 May 2012) Abstract–Single crystal (U-Th) ⁄ He dating was applied to 24 apatite and 23 zircon grains from the Wetumpka impact structure, Alabama, USA. This small approximately 5–7.6 km impact crater was formed in a shallow marine environment, with no known preserved impact melt, thus offering a challenge to common geochronological techniques. A mean (U-Th) ⁄ He apatite and zircon age of 84.4 ± 1.4 Ma (2r) was obtained, which is within error of the previously estimated Late Cretaceous impact age of approximately 83.5 Ma. In addition, helium diffusion modeling of apatite and zircon grains during fireball ⁄ contact, shock metamorphism, and hydrothermal events was undertaken, to show the influence of these individual thermal processes on resetting (U-Th) ⁄ He ages in the Wetumpka samples. This study has shown that the (U-Th) ⁄ He geochronological technique has real potential for dating impact structures, especially smaller and eroded impact structures that lack impact melt lithologies. -
U.S. Postal Service Salutes Legendary Author Celebrating 100Th Anniversary of Edgar Rice Burroughs’ Creation of Tarzan
FOR IMMEDIATE RELEASE National Contact: Roy Betts August 16, 2012 [email protected] 202-268-3207 Local Contact: Richard Maher [email protected] 714-662-6350 usps.com/news Release No. 12-094 U.S. Postal Service Salutes Legendary Author Celebrating 100th anniversary of Edgar Rice Burroughs’ Creation of Tarzan To obtain a high-resolution image of the stamp for media use only, email [email protected]. TARZANA, CA — The U.S. Postal Service will honor tomorrow one of the most prolific authors of the early 20th century and inventor of the iconic character Tarzan with the issuance of the Edgar Rice Burroughs Forever Stamp. The stamp issuance coincides with the 100th anniversary of the publication of Burroughs’ first story, Under the Moons of Mars, and his first Tarzan story, Tarzan of the Apes, in 1912. The Edgar Rice Burroughs Forever Stamp will be dedicated tomorrow at 11:30 a.m. PT at the Tarzana Community and Cultural Center in Tarzana, CA, and will go on sale tomorrow at Post Offices nationwide, online at usps.com and by phone at 800-782-6724. Best known for inventing the legendary character Tarzan, Burroughs wrote more than 70 books, including historical fiction and several popular series of science fiction tales. “At the Postal Service, we’re proud to honor wonderful writers like Mr. Burroughs,” said Giselle Valera, vice president and managing director, Global Business. “These creative geniuses make lasting contributions to our cultural heritage, and we want more Americans to learn about them. Our stamp featuring Mr. -
General Vertical Files Anderson Reading Room Center for Southwest Research Zimmerman Library
“A” – biographical Abiquiu, NM GUIDE TO THE GENERAL VERTICAL FILES ANDERSON READING ROOM CENTER FOR SOUTHWEST RESEARCH ZIMMERMAN LIBRARY (See UNM Archives Vertical Files http://rmoa.unm.edu/docviewer.php?docId=nmuunmverticalfiles.xml) FOLDER HEADINGS “A” – biographical Alpha folders contain clippings about various misc. individuals, artists, writers, etc, whose names begin with “A.” Alpha folders exist for most letters of the alphabet. Abbey, Edward – author Abeita, Jim – artist – Navajo Abell, Bertha M. – first Anglo born near Albuquerque Abeyta / Abeita – biographical information of people with this surname Abeyta, Tony – painter - Navajo Abiquiu, NM – General – Catholic – Christ in the Desert Monastery – Dam and Reservoir Abo Pass - history. See also Salinas National Monument Abousleman – biographical information of people with this surname Afghanistan War – NM – See also Iraq War Abousleman – biographical information of people with this surname Abrams, Jonathan – art collector Abreu, Margaret Silva – author: Hispanic, folklore, foods Abruzzo, Ben – balloonist. See also Ballooning, Albuquerque Balloon Fiesta Acequias – ditches (canoas, ground wáter, surface wáter, puming, water rights (See also Land Grants; Rio Grande Valley; Water; and Santa Fe - Acequia Madre) Acequias – Albuquerque, map 2005-2006 – ditch system in city Acequias – Colorado (San Luis) Ackerman, Mae N. – Masonic leader Acoma Pueblo - Sky City. See also Indian gaming. See also Pueblos – General; and Onate, Juan de Acuff, Mark – newspaper editor – NM Independent and -
Martian Crater Morphology
ANALYSIS OF THE DEPTH-DIAMETER RELATIONSHIP OF MARTIAN CRATERS A Capstone Experience Thesis Presented by Jared Howenstine Completion Date: May 2006 Approved By: Professor M. Darby Dyar, Astronomy Professor Christopher Condit, Geology Professor Judith Young, Astronomy Abstract Title: Analysis of the Depth-Diameter Relationship of Martian Craters Author: Jared Howenstine, Astronomy Approved By: Judith Young, Astronomy Approved By: M. Darby Dyar, Astronomy Approved By: Christopher Condit, Geology CE Type: Departmental Honors Project Using a gridded version of maritan topography with the computer program Gridview, this project studied the depth-diameter relationship of martian impact craters. The work encompasses 361 profiles of impacts with diameters larger than 15 kilometers and is a continuation of work that was started at the Lunar and Planetary Institute in Houston, Texas under the guidance of Dr. Walter S. Keifer. Using the most ‘pristine,’ or deepest craters in the data a depth-diameter relationship was determined: d = 0.610D 0.327 , where d is the depth of the crater and D is the diameter of the crater, both in kilometers. This relationship can then be used to estimate the theoretical depth of any impact radius, and therefore can be used to estimate the pristine shape of the crater. With a depth-diameter ratio for a particular crater, the measured depth can then be compared to this theoretical value and an estimate of the amount of material within the crater, or fill, can then be calculated. The data includes 140 named impact craters, 3 basins, and 218 other impacts. The named data encompasses all named impact structures of greater than 100 kilometers in diameter. -
Acadia Geology Alumni/Ae Newsletter
Acadia Geology Alumni/ae Newsletter Issue 21 December, 2009 Department of Earth and Environmental Science, Acadia University, Wolfville, Nova Scotia, B4P 2R6 [email protected] VIEW FROM ACADIA As I write this message, my term as the “acting head” course, it costs less to deliver. Another aspect of of Earth and Environmental Science is rapidly budgetary constraints is a lack of replacements for drawing to a close. Rob Raeside returns as head faculty on sabbatical. In the “good old days” such beginning Jan. 1, 2010, and it is probably a “toss-up” absences were typically covered by a full-time faculty as to which one of us is happier about that! To be replacement, but now we are lucky to receive one honest, however, I found many aspects of being “per-course replacement”. Such replacements have department head to be rewarding, and if we did not been great but they are paid specifically to teach the have a capable and willing incumbent returning to the single course assigned to them, and hence do not job, continuing in the role would have been OK. provide any coverage for other activities integral to running a department, such as counselling students, The past year at Acadia has more than lived up to the supervising honours and special project students, supposed ancient Chinese curse “may you live in serving on committees, and so on. This ripple-down interesting times”. The main topic occupying effect hits especially hard in a small department such everyone’s mind on campus has been the university as ours. Fortunately, faculty in E&ES have been budget. -
Australian Aborigines and Meteorites
Records of the Western Australian Museum 18: 93-101 (1996). Australian Aborigines and meteorites A.W.R. Bevan! and P. Bindon2 1Department of Earth and Planetary Sciences, 2 Department of Anthropology, Western Australian Museum, Francis Street, Perth, Western Australia 6000 Abstract - Numerous mythological references to meteoritic events by Aboriginal people in Australia contrast with the scant physical evidence of their interaction with meteoritic materials. Possible reasons for this are the unsuitability of some meteorites for tool making and the apparent inability of early Aborigines to work metallic materials. However, there is a strong possibility that Aborigines witnessed one or more of the several recent « 5000 yrs BP) meteorite impact events in Australia. Evidence for Aboriginal use of meteorites and the recognition of meteoritic events is critically evaluated. INTRODUCTION Australia, although for climatic and physiographic The ceremonial and practical significance of reasons they are rarely found in tropical Australia. Australian tektites (australites) in Aboriginal life is The history of the recovery of meteorites in extensively documented (Baker 1957 and Australia has been reviewed by Bevan (1992). references therein; Edwards 1966). However, Within the continent there are two significant areas despite abundant evidence throughout the world for the recovery of meteorites: the Nullarbor that many other ancient civilizations recognised, Region, and the area around the Menindee Lakes utilized and even revered meteorites (particularly of western New South Wales. These accumulations meteoritic iron) (e.g., see Buchwald 1975 and have resulted from prolonged aridity that has references therein), there is very little physical or allowed the preservation of meteorites for documentary evidence of Aboriginal acknowledge thousands of years after their fall, and the large ment or use of meteoritic materials. -
Raman Spectroscopy of Shocked Gypsum from a Meteorite Impact Crater
International Journal of Astrobiology 16 (3): 286–292 (2017) doi:10.1017/S1473550416000367 © Cambridge University Press 2016 This is an Open Access article, distributed under the terms of the Creative Commons Attribution licence (http://creativecommons.org/licenses/by/4.0/), which permits unrestricted re-use, distribution, and reproduction in any medium, provided the original work is properly cited. Raman spectroscopy of shocked gypsum from a meteorite impact crater Connor Brolly, John Parnell and Stephen Bowden Department of Geology & Petroleum Geology, University of Aberdeen, Meston Building, Aberdeen, UK e-mail: c.brolly@ abdn.ac.uk Abstract: Impact craters and associated hydrothermal systems are regarded as sites within which life could originate onEarth,and onMars.The Haughtonimpactcrater,one ofthemost well preservedcratersonEarth,is abundant in Ca-sulphates. Selenite, a transparent form of gypsum, has been colonized by viable cyanobacteria. Basementrocks, which havebeenshocked,aremoreabundantinendolithicorganisms,whencomparedwithun- shocked basement. We infer that selenitic and shocked gypsum are more suitable for microbial colonization and have enhanced habitability. This is analogous to many Martian craters, such as Gale Crater, which has sulphate deposits in a central layered mound, thought to be formed by post-impact hydrothermal springs. In preparation for the 2020 ExoMars mission, experiments were conducted to determine whether Raman spectroscopy can distinguish between gypsum with different degrees of habitability. Ca-sulphates were analysed using Raman spectroscopyand resultsshow nosignificant statistical difference between gypsumthat has experienced shock by meteorite impact and gypsum, which has been dissolved and re-precipitated as an evaporitic crust. Raman spectroscopy is able to distinguish between selenite and unaltered gypsum. This showsthat Raman spectroscopy can identify more habitable forms of gypsum, and demonstrates the current capabilities of Raman spectroscopy for the interpretation of gypsum habitability. -
Mars Exploration Rovers: 4 Years on Mars
https://ntrs.nasa.gov/search.jsp?R=20080047431 2019-10-28T16:17:34+00:00Z Mars Exploration Rovers: 4 Years on Mars Geoffrey A. Landis This January, the Mars Exploration Rovers "Spirit" and "Opportunity" are starting their fifth year of exploring the surface of Mars, well over ten times their nominal 90-day design lifetime. This lecture discusses the Mars Exploration Rovers, presents the current mission status for the extended mission, some of the most results from the mission and how it is affecting our current view of Mars, and briefly presents the plans for the coming NASA missions to the surface of Mars and concepts for exploration with robots and humans into the next decade, and beyond. Four Years on Mars: the Mars Exploration Rovers Geoffrey A. Landis NASA John Glenn Research Center http://www.sff.net/people/geoffrey.landis Presentation at MIT Department of Aeronautics and Astronautics, January 18, 2008 Exploration - Landis Mars viewed from the Hubble Space Telescope Exploration - Landis Views of Mars in the early 20th century Lowell 1908 Sciaparelli 1888 Burroughs 1912 (cover painting by Frazetta) Tales of Outer Space ed. Donald A. Wollheim, Ace D-73, 1954 (From Winchell Chung's web page projectrho.com) Exploration - Landis Past Missions to Mars: first close up images of Mars from Mariner 4 Mariner 4 discovered Mars was a barren, moon-like desert Exploration - Landis Viking 1976 Signs of past water on Mars? orbiter Photo from orbit by the 1976 Viking orbiter Exploration - Landis Pathfinder and Sojourner Rover: a solar-powered mission -
A Novel Geomatics Method for Assessing the Haughton Impact Structure
Meteoritics & Planetary Science 1–13 (2020) doi: 10.1111/maps.13573-3267 Electronic-Only Article A novel geomatics method for assessing the Haughton impact structure Calder W. PATTERSON * and Richard E. ERNST Department of Earth Sciences, Ottawa Carleton Geoscience Center, Carleton University, 1125 Colonel By Drive, Ottawa, Ontario K1S 5B6, Canada *Corresponding author. E-mail: [email protected] (Received 22 July 2019; revision accepted 22 August 2020) Abstract–Terrestrial impact structures are typically modified by erosion, burial, and tectonic deformation. Their systematic morphologies are typically reconstructed through a combination of geological and topographic mapping, satellite imagery, and geophysical surveys. This study applies a novel geomatics approach to assessment of the morphology of the extensively studied Haughton impact structure (HIS), Devon Island, Nunavut, in order to test its potential to improve the accuracy and quality of future impact structure reconstruction. This new methodology integrates HIS lithological data, in the form of digitized geologic mapping, with a digital elevation model, within diametrically opposed, wedge-shaped couplets, and plots these data as pseudo cross sections that capitalize on the radial symmetry of the impact structure. The pseudo cross sections provide an accurate reconstruction of the near- surface stratigraphic sequences and terraces in the faulted annulus of the modified crater rim. The resultant pseudo cross sections support current interpretations regarding the 10–12 km diameter of the transient cavity, and successfully reproduce the visible outer ring and intermediate uplifted zone within the central basin. Observed positions of vertical offsets suggest that the extent of impact deformation extends beyond the current estimates of the apparent crater rim to radial distances of between 14 and 15 km. -