A Field Guide to Finding Fossils on Mars
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202 Chapter 5 FUTURE WORK There is more work is planned for these projects. Some of the proposed future work fell out of the questions and problems that arise while first attempting to solve a problem. Some of it was originally intended to be encompassed in the thesis work, but work at an earlier stage grew to dominate the project as a result of the sheer volume of data available. Many questions were left unanswered in the work described in Chapter 4. It is not clear why the MM5 does not predict the secondary winds that clearly must exist in the current wind regime. These winds do not appear in GFDL GCM model runs, and they may not exist in any current atmospheric model. It is possible that they are produced by rare storms (i.e., storms that occur once a decade or century), and I would like to look into the possibility of observing or predicting these storms. The MM5 also does not predict winds strong enough to lift basaltic grains into saltation. This may simply be a problem of model resolution, and it is not a difficult prospect to run the model at a higher resolution and/or to output the strongest hourly winds at each grid point rather than the winds at the top of each hour. There is also the problem that the MM5 is meant to hold subgrids that are no more than three times smaller than their parent grids – and yet our model runs at a scale of 10 km were more than an order of magnitude higher resolution than the parent grid. -
Imaginative Geographies of Mars: the Science and Significance of the Red Planet, 1877 - 1910
Copyright by Kristina Maria Doyle Lane 2006 The Dissertation Committee for Kristina Maria Doyle Lane Certifies that this is the approved version of the following dissertation: IMAGINATIVE GEOGRAPHIES OF MARS: THE SCIENCE AND SIGNIFICANCE OF THE RED PLANET, 1877 - 1910 Committee: Ian R. Manners, Supervisor Kelley A. Crews-Meyer Diana K. Davis Roger Hart Steven D. Hoelscher Imaginative Geographies of Mars: The Science and Significance of the Red Planet, 1877 - 1910 by Kristina Maria Doyle Lane, B.A.; M.S.C.R.P. Dissertation Presented to the Faculty of the Graduate School of The University of Texas at Austin in Partial Fulfillment of the Requirements for the Degree of Doctor of Philosophy The University of Texas at Austin August 2006 Dedication This dissertation is dedicated to Magdalena Maria Kost, who probably never would have understood why it had to be written and certainly would not have wanted to read it, but who would have been very proud nonetheless. Acknowledgments This dissertation would have been impossible without the assistance of many extremely capable and accommodating professionals. For patiently guiding me in the early research phases and then responding to countless followup email messages, I would like to thank Antoinette Beiser and Marty Hecht of the Lowell Observatory Library and Archives at Flagstaff. For introducing me to the many treasures held deep underground in our nation’s capital, I would like to thank Pam VanEe and Ed Redmond of the Geography and Map Division of the Library of Congress in Washington, D.C. For welcoming me during two brief but productive visits to the most beautiful library I have seen, I thank Brenda Corbin and Gregory Shelton of the U.S. -
Geophagic Clay Around Uteh-Uzalla Near Benin: Mineral and Trace
Research Article Geophagic clay around Uteh‑Uzalla near Benin: mineral and trace elements compositions and possible health implications Iyobosa Timothy Asowata1 Received: 30 November 2020 / Accepted: 8 April 2021 © The Author(s) 2021 OPEN Abstract Geophagic clay consumption, which is an age-long cultural practice by humans and animals in many parts of the world, and particularly in Nigeria, may have long time health efects on the consumers. This is particularly so because of the relatively high concentration of harmful minerals and toxic elements. This study sought to determine the mineralogical and trace element compositions of geophagic clay in Uteh-Uzalla area, which is underlain by the Benin Formation of Oligocene to Miocene age, in order to evaluate the potential health risk associated with the consumption of the clay. Sixteen clay samples were collected from mine face profles of an open pit, analysed for mineral and trace element compositions, using x-ray difraction technique and ultra-trace inductively coupled plasma mass spectrometry (ICP- MS) methods, respectively. The mean mineral concentration in % includes kaolinite, quartz and smectite (64.88, 19.98, and 9.54), respectively, among other minerals. And the mean concentrations in mg/kg for Cu (15.0), Pb (14.4), Zn (30.9), Co (8.9), Mn (39.4) and Th (10.5) among other elements were found in the clay. From the trace elements results when compared with health risk indices by Agency for Toxic Substances and Diseases Registry (ATSDR): Minimum Risk Level, recommended daily intake and estimated daily intake, it was found that the elements are far above the daily oral intake requirement. -
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. -
Thermodynamics of DNA Binding by DNA Polymerase I and Reca
Louisiana State University LSU Digital Commons LSU Doctoral Dissertations Graduate School 2014 Thermodynamics of DNA Binding by DNA Polymerase I and RecA Recombinase from Deinococcus radiodurans Jaycob Dalton Warfel Louisiana State University and Agricultural and Mechanical College Follow this and additional works at: https://digitalcommons.lsu.edu/gradschool_dissertations Recommended Citation Warfel, Jaycob Dalton, "Thermodynamics of DNA Binding by DNA Polymerase I and RecA Recombinase from Deinococcus radiodurans" (2014). LSU Doctoral Dissertations. 2382. https://digitalcommons.lsu.edu/gradschool_dissertations/2382 This Dissertation is brought to you for free and open access by the Graduate School at LSU Digital Commons. It has been accepted for inclusion in LSU Doctoral Dissertations by an authorized graduate school editor of LSU Digital Commons. For more information, please [email protected]. THERMODYNAMICS OF DNA BINDING BY DNA POLYMERASE I AND RECA RECOMBINASE FROM DEINOCOCCUS RADIODURANS A Dissertation Submitted to the Graduate Faculty of the Louisiana State University and Agricultural and Mechanical College in partial fulfillment of the requirements for the degree of Doctor of Philosophy in The Department of Biological Sciences by Jaycob Dalton Warfel B.S. Louisiana State University, 2006 May 2015 ACKNOWLEDGEMENTS I would like to express my utmost gratitude to the myriad of individuals who have lent their support during the time it has taken to complete this dissertation. First and foremost is due glory to God, The Father, The Son and The Holy Spirit, through whom all is accomplished. It is with extreme thankfulness for the blessings bestowed upon me, and with vast appreciation for the beauty of God’s creation that I have pursued a scientific education. -
Warfare in a Fragile World: Military Impact on the Human Environment
Recent Slprt•• books World Armaments and Disarmament: SIPRI Yearbook 1979 World Armaments and Disarmament: SIPRI Yearbooks 1968-1979, Cumulative Index Nuclear Energy and Nuclear Weapon Proliferation Other related •• 8lprt books Ecological Consequences of the Second Ihdochina War Weapons of Mass Destruction and the Environment Publish~d on behalf of SIPRI by Taylor & Francis Ltd 10-14 Macklin Street London WC2B 5NF Distributed in the USA by Crane, Russak & Company Inc 3 East 44th Street New York NY 10017 USA and in Scandinavia by Almqvist & WikseH International PO Box 62 S-101 20 Stockholm Sweden For a complete list of SIPRI publications write to SIPRI Sveavagen 166 , S-113 46 Stockholm Sweden Stoekholol International Peace Research Institute Warfare in a Fragile World Military Impact onthe Human Environment Stockholm International Peace Research Institute SIPRI is an independent institute for research into problems of peace and conflict, especially those of disarmament and arms regulation. It was established in 1966 to commemorate Sweden's 150 years of unbroken peace. The Institute is financed by the Swedish Parliament. The staff, the Governing Board and the Scientific Council are international. As a consultative body, the Scientific Council is not responsible for the views expressed in the publications of the Institute. Governing Board Dr Rolf Bjornerstedt, Chairman (Sweden) Professor Robert Neild, Vice-Chairman (United Kingdom) Mr Tim Greve (Norway) Academician Ivan M£ilek (Czechoslovakia) Professor Leo Mates (Yugoslavia) Professor -
New Chryse and the Provinces
New Chryse and the Provinces The city of New Chryse is actually several connected cities. The Upper City is located on a break in the crater rim, looking down past a steep rock to the Lower City. Inside the da Vinci crater rim lies the Inner City, also known as the Old City – Red Era tunnels and cave shelters, as well as several nanocomposite towers and cupolas on Mona Lys Ridge looking down on the lower parts of the city. The Lower city lies in a valley sloping down to the Harbour City, which fills a crater 20 kilometres to the East. The Harbour City crater is connected to Camiling Bay and the sea through two canyons and is very well protected from both wind and ice. South of the Lower City and Harbour City lies The Slopes, a straight slope into the sea that is covered with sprawl and slums. Mona Lys Ridge is a mixture of palatial estates surrounded by gardens, imposing official imperial buildings and towering ancient structures used by the highest ranks of the Empire. The central imperial administration and especially the Council is housed in the Deimos Needle, a diamondoid tower that together with its sibling the Phobos Needle dominate the skyline. Escalators allow swift and discreet transport down to the lower levels of the city, and can easily be defended by the police force. North of Mona Lys lies a secluded garden city for higher administrators, guild officials and lesser nobility. The Inner City is to a large extent part of Mona Lys, although most of the inhabitants of Mona Lys do not care much for the dusty old tunnels and hidden vaults – that is left to the Guild of Antiquarians who maintain and protect it. -
Magnetized Impact Craters
Icarus xxx (2011) xxx–xxx Contents lists available at ScienceDirect Icarus journal homepage: www.elsevier.com/locate/icarus Predicted and observed magnetic signatures of martian (de)magnetized impact craters ⇑ Benoit Langlais a, , Erwan Thébault b a CNRS UMR 6112, Université de Nantes, Laboratoire de Planétologie et Géodynamique, 2 Rue de la Houssinière, F-44000 Nantes, France b CNRS UMR 7154, Institut de Physique du Globe de Paris, Équipe de Géomagnétisme, 1 Rue Cuvier, F-75005 Paris, France article info abstract Article history: The current morphology of the martian lithospheric magnetic field results from magnetization and Received 3 May 2010 demagnetization processes, both of which shaped the planet. The largest martian impact craters, Hellas, Revised 6 January 2011 Argyre, Isidis and Utopia, are not associated with intense magnetic fields at spacecraft altitude. This is Accepted 6 January 2011 usually interpreted as locally non- or de-magnetized areas, as large impactors may have reset the mag- Available online xxxx netization of the pre-impact material. We study the effects of impacts on the magnetic field. First, a care- ful analysis is performed to compute the impact demagnetization effects. We assume that the pre-impact Keywords: lithosphere acquired its magnetization while cooling in the presence of a global, centered and mainly Mars, Surface dipolar magnetic field, and that the subsequent demagnetization is restricted to the excavation area cre- Mars, Interior Impact processes ated by large craters, between 50- and 500-km diameter. Depth-to-diameter ratio of the transient craters Magnetic fields is set to 0.1, consistent with observed telluric bodies. Associated magnetic field is computed between 100- and 500-km altitude. -
DMAAC – February 1973
LUNAR TOPOGRAPHIC ORTHOPHOTOMAP (LTO) AND LUNAR ORTHOPHOTMAP (LO) SERIES (Published by DMATC) Lunar Topographic Orthophotmaps and Lunar Orthophotomaps Scale: 1:250,000 Projection: Transverse Mercator Sheet Size: 25.5”x 26.5” The Lunar Topographic Orthophotmaps and Lunar Orthophotomaps Series are the first comprehensive and continuous mapping to be accomplished from Apollo Mission 15-17 mapping photographs. This series is also the first major effort to apply recent advances in orthophotography to lunar mapping. Presently developed maps of this series were designed to support initial lunar scientific investigations primarily employing results of Apollo Mission 15-17 data. Individual maps of this series cover 4 degrees of lunar latitude and 5 degrees of lunar longitude consisting of 1/16 of the area of a 1:1,000,000 scale Lunar Astronautical Chart (LAC) (Section 4.2.1). Their apha-numeric identification (example – LTO38B1) consists of the designator LTO for topographic orthophoto editions or LO for orthophoto editions followed by the LAC number in which they fall, followed by an A, B, C or D designator defining the pertinent LAC quadrant and a 1, 2, 3, or 4 designator defining the specific sub-quadrant actually covered. The following designation (250) identifies the sheets as being at 1:250,000 scale. The LTO editions display 100-meter contours, 50-meter supplemental contours and spot elevations in a red overprint to the base, which is lithographed in black and white. LO editions are identical except that all relief information is omitted and selenographic graticule is restricted to border ticks, presenting an umencumbered view of lunar features imaged by the photographic base. -
Access to Electronic Thesis
Access to Electronic Thesis Author: Khalid Salim Al-Abri Thesis title: USE OF MOLECULAR APPROACHES TO STUDY THE OCCURRENCE OF EXTREMOPHILES AND EXTREMODURES IN NON-EXTREME ENVIRONMENTS Qualification: PhD This electronic thesis is protected by the Copyright, Designs and Patents Act 1988. No reproduction is permitted without consent of the author. It is also protected by the Creative Commons Licence allowing Attributions-Non-commercial-No derivatives. If this electronic thesis has been edited by the author it will be indicated as such on the title page and in the text. USE OF MOLECULAR APPROACHES TO STUDY THE OCCURRENCE OF EXTREMOPHILES AND EXTREMODURES IN NON-EXTREME ENVIRONMENTS By Khalid Salim Al-Abri Msc., University of Sultan Qaboos, Muscat, Oman Mphil, University of Sheffield, England Thesis submitted in partial fulfillment for the requirements of the Degree of Doctor of Philosophy in the Department of Molecular Biology and Biotechnology, University of Sheffield, England 2011 Introductory Pages I DEDICATION To the memory of my father, loving mother, wife “Muneera” and son “Anas”, brothers and sisters. Introductory Pages II ACKNOWLEDGEMENTS Above all, I thank Allah for helping me in completing this project. I wish to express my thanks to my supervisor Professor Milton Wainwright, for his guidance, supervision, support, understanding and help in this project. In addition, he also stood beside me in all difficulties that faced me during study. My thanks are due to Dr. D. J. Gilmour for his co-supervision, technical assistance, his time and understanding that made some of my laboratory work easier. In the Ministry of Regional Municipalities and Water Resources, I am particularly grateful to Engineer Said Al Alawi, Director General of Health Control, for allowing me to carry out my PhD study at the University of Sheffield. -
Representatives of a Novel Archaeal Phylum Or a Fast-Evolving
Open Access Research2005BrochieretVolume al. 6, Issue 5, Article R42 Nanoarchaea: representatives of a novel archaeal phylum or a comment fast-evolving euryarchaeal lineage related to Thermococcales? Celine Brochier*, Simonetta Gribaldo†, Yvan Zivanovic‡, Fabrice Confalonieri‡ and Patrick Forterre†‡ Addresses: *EA EGEE (Evolution, Génomique, Environnement) Université Aix-Marseille I, Centre Saint-Charles, 3 Place Victor Hugo, 13331 Marseille, Cedex 3, France. †Unite Biologie Moléculaire du Gène chez les Extremophiles, Institut Pasteur, 25 rue du Dr Roux, 75724 Paris Cedex ‡ 15, France. Institut de Génétique et Microbiologie, UMR CNRS 8621, Université Paris-Sud, 91405 Orsay, France. reviews Correspondence: Celine Brochier. E-mail: [email protected]. Simonetta Gribaldo. E-mail: [email protected] Published: 14 April 2005 Received: 3 December 2004 Revised: 10 February 2005 Genome Biology 2005, 6:R42 (doi:10.1186/gb-2005-6-5-r42) Accepted: 9 March 2005 The electronic version of this article is the complete one and can be found online at http://genomebiology.com/2005/6/5/R42 reports © 2005 Brochier et al.; licensee BioMed Central Ltd. This is an Open Access article distributed under the terms of the Creative Commons Attribution License (http://creativecommons.org/licenses/by/2.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited. Placement<p>Anteins from analysis 25of Nanoarcheumarchaeal of the positiongenomes equitans of suggests Nanoarcheum in the that archaeal N. equitans phylogeny inis likethe lyarchaeal to be the phylogeny representative using aof large a fast-evolving dataset of concatenatedeuryarchaeal ribosomalineage.</p>l pro- deposited research Abstract Background: Cultivable archaeal species are assigned to two phyla - the Crenarchaeota and the Euryarchaeota - by a number of important genetic differences, and this ancient split is strongly supported by phylogenetic analysis. -
In Vivo Interactions of Archaeal Cdc6 Orc1 and Minichromosome
In vivo interactions of archaeal Cdc6͞Orc1 and minichromosome maintenance proteins with the replication origin Fujihiko Matsunaga*, Patrick Forterre*, Yoshizumi Ishino†, and Hannu Myllykallio*§ *Institut de Ge´ne´ tique et Microbiologie, Universite´de Paris-Sud, 91405 Orsay, France; and †Department of Molecular Biology, Biomolecular Engineering Research Institute, 6-2-3 Furuedai, Suita, Osaka 565-0874, Japan Communicated by Bruce W. Stillman, Cold Spring Harbor Laboratory, Cold Spring Harbor, NY, July 25, 2001 (received for review May 25, 2001) Although genome analyses have suggested parallels between basis of asymmetry in base composition between leading and archaeal and eukaryotic replication systems, little is known about lagging strands (10, 11). In Pyrococcus abyssi, the location of the the DNA replication mechanism in Archaea. By two-dimensional predicted origin coincides with an early replicating chromosomal gel electrophoreses we positioned a replication origin (oriC) within segment of 80 kb identified by radioactive labeling of chromo- 1 kb in the chromosomal DNA of Pyrococcus abyssi, an anaerobic somal DNA in cultures released from a replication block (12). hyperthermophile, and demonstrated that the oriC is physically Our in silico and labeling data also allowed us to conclude that linked to the cdc6 gene. Our chromatin immunoprecipitation as- the hyperthermophilic archaeon P. abyssi uses a single bidirec- says indicated that P. abyssi Cdc6 and minichromosome mainte- tional origin to replicate its genome. We proposed that this origin nance (MCM) proteins bind preferentially to the oriC region in the would correspond to the long intergenic region conserved in all exponentially growing cells. Whereas the oriC association of MCM three known Pyrococcus sp.