Seasonal Dynamics and Phylogenetic Diversity of Free-Living and Particle-Associated Bacterial Communities in Four Lakes in Northeastern Germany
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Isolation and Characterization of Culturable Thermophilic Bacteria from Hot Springs in Benguet, Philippines Socorro Martha Meg-Ay V
International Journal of Philippine Science and Technology, Vol. 08, No. 2, 2015 14 ARTICLE Isolation and characterization of culturable thermophilic bacteria from hot springs in Benguet, Philippines Socorro Martha Meg-ay V. Daupan1 and Windell L. Rivera*1,2 1Institute of Biology, College of Science, University of the Philippines, Diliman, Quezon City, 1101, Philippines 2Natural Sciences Research Institute, University of the Philippines, Diliman, Quezon City, 1101, Philippines Abstract—Despite the numerous geothermal environments in the Philippines, there is limited information on the composition of thermophilic bacteria within the country. This study is the first to carry out both culture and molecular-based methods to characterize thermophilic bacteria from hot springs in the province of Benguet in the Philippines. The xylan-degrading ability of each isolate was also investigated using the Congo red method. A total of 14 phenotypically-different isolates (7 from Badekbek mud spring and 7 from Dalupirip hot spring) were characterized. Phylogenetic analysis based on the nearly complete 16S rDNA sequences revealed that all the isolates obtained from Badekbek were affiliated with Geobacillus, whereas the isolates from Dalupirip clustered into 3 major linkages of bacterial phyla, Firmicutes (72%) consisting of the genera Geobacillus and Anoxybacillus; Deinococcus-Thermus (14%) consisting of the genus Meiothermus; and Bacteroidetes consisting of the genus Thermonema (14%). In addition, xylan-degrading ability was observed in all isolates from Badekbek and in 2 isolates from Dalupirip which showed high sequence similarity with Geobacillus spp. The results are also essential in understanding the roles of the physico-chemical properties of hot spring water as a driver of thermophilic bacterial compositions. -
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. -
Workshop on Mars Telescopic Observations
WORKSHCPON MARS TELESCOPIC OBSERVATIONS 90' 180'-;~~~~~~------------------..~~------------~~----..~o~,· 270' LPI Technical Report Number 95-04 Lunar and Planetary Institute 3600 Bay Area Boulevard Houston TX 77058-1113 LPIITR--95-04 WORKSHOP ON MARS TELESCOPIC OBSERVATIONS Edited by J. F. Bell III and J. E. Moersch Held at Cornell University, Ithaca, New York August 14-15, 1995 Sponsored by Lunar and Planetary Institute Lunar and Planetary Institute 3600 Bay Area Boulevard Houston TX 77058-1113 LPI Technical Report Number 95-04 LPIITR--95-04 Compiled in 1995 by LUNAR AND PLANETARY INSTITUTE The Institute is operated by the Universities Space Research Association under Contract No. NASW-4574 with the National Aeronautics and Space Administration. Material in this volume may be copied without restraint for library, abstract service, education, or personal 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 Bell J. F.III and Moersch J. E., eds. (1995) Workshop on Mars Telescopic Observations. LPI Tech. Rpt. 95-04, Lunar and Planetary Institute, Houston. 33 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 ofshipping and handling. Cover: Orbits of Mars (outer ellipse) and Earth (inner ellipse) showing oppositions of the planet from 1954to 1999. From C. Aammarion (1954) The Flammarion Book ofAstronomy, Simon and Schuster, New York. LPl Technical Report 95-04 iii Introduction The Mars Telescopic Observations Workshop, held August 14-15, 1995, at Cornell University in Ithaca, New York, was organized and planned with two primary goals in mind: The first goal was to facilitate discussions among and between amateur and professional observers and to create a workshop environment fostering collaborations and comparisons within the Mars ob serving community. -
Appendix I Lunar and Martian Nomenclature
APPENDIX I LUNAR AND MARTIAN NOMENCLATURE LUNAR AND MARTIAN NOMENCLATURE A large number of names of craters and other features on the Moon and Mars, were accepted by the IAU General Assemblies X (Moscow, 1958), XI (Berkeley, 1961), XII (Hamburg, 1964), XIV (Brighton, 1970), and XV (Sydney, 1973). The names were suggested by the appropriate IAU Commissions (16 and 17). In particular the Lunar names accepted at the XIVth and XVth General Assemblies were recommended by the 'Working Group on Lunar Nomenclature' under the Chairmanship of Dr D. H. Menzel. The Martian names were suggested by the 'Working Group on Martian Nomenclature' under the Chairmanship of Dr G. de Vaucouleurs. At the XVth General Assembly a new 'Working Group on Planetary System Nomenclature' was formed (Chairman: Dr P. M. Millman) comprising various Task Groups, one for each particular subject. For further references see: [AU Trans. X, 259-263, 1960; XIB, 236-238, 1962; Xlffi, 203-204, 1966; xnffi, 99-105, 1968; XIVB, 63, 129, 139, 1971; Space Sci. Rev. 12, 136-186, 1971. Because at the recent General Assemblies some small changes, or corrections, were made, the complete list of Lunar and Martian Topographic Features is published here. Table 1 Lunar Craters Abbe 58S,174E Balboa 19N,83W Abbot 6N,55E Baldet 54S, 151W Abel 34S,85E Balmer 20S,70E Abul Wafa 2N,ll7E Banachiewicz 5N,80E Adams 32S,69E Banting 26N,16E Aitken 17S,173E Barbier 248, 158E AI-Biruni 18N,93E Barnard 30S,86E Alden 24S, lllE Barringer 29S,151W Aldrin I.4N,22.1E Bartels 24N,90W Alekhin 68S,131W Becquerei -
The Role of External Factors in the Variability of the Structure of the Zooplankton Community of Small Lakes (South-East Kazakhstan)
water Article The Role of External Factors in the Variability of the Structure of the Zooplankton Community of Small Lakes (South-East Kazakhstan) Moldir Aubakirova 1,2,*, Elena Krupa 3 , Zhanara Mazhibayeva 2, Kuanysh Isbekov 2 and Saule Assylbekova 2 1 Faculty of Biology and Biotechnology, Al-Farabi Kazakh National University, Almaty 050040, Kazakhstan 2 Fisheries Research and Production Center, Almaty 050016, Kazakhstan; mazhibayeva@fishrpc.kz (Z.M.); isbekov@fishrpc.kz (K.I.); assylbekova@fishrpc.kz (S.A.) 3 Institute of Zoology, Almaty 050060, Kazakhstan; [email protected] * Correspondence: [email protected]; Tel.: +7-27-3831715 Abstract: The variability of hydrochemical parameters, the heterogeneity of the habitat, and a low level of anthropogenic impact, create the premises for conserving the high biodiversity of aquatic communities of small water bodies. The study of small water bodies contributes to understanding aquatic organisms’ adaptation to sharp fluctuations in external factors. Studies of biological com- munities’ response to fluctuations in external factors can be used for bioindication of the ecological state of small water bodies. In this regard, the purpose of the research is to study the structure of zooplankton of small lakes in South-East Kazakhstan in connection with various physicochemical parameters to understand the role of biological variables in assessing the ecological state of aquatic Citation: Aubakirova, M.; Krupa, E.; ecosystems. According to hydrochemical data in summer 2019, the nutrient content was relatively Mazhibayeva, Z.; Isbekov, K.; high in all studied lakes. A total of 74 species were recorded in phytoplankton. The phytoplankton Assylbekova, S. The Role of External abundance varied significantly, from 8.5 × 107 to 2.71667 × 109 cells/m3, with a biomass from 0.4 Factors in the Variability of the to 15.81 g/m3. -
Liquid Water on Mars
Report, Planetary Sciences Unit (AST80015), Swinburne Astronomy Online Preprint typeset using LATEX style emulateapj v. 12/16/11 LIQUID WATER ON MARS M. Usatov1 Report, Planetary Sciences Unit (AST80015), Swinburne Astronomy Online ABSTRACT Geomorphological, mineralogical and other evidence of the conditions favoring the existence of water on Mars in liquid phase is reviewed. This includes signatures of past and, possibly, present aqueous environments, such as the northern ocean, lacustrine environments, sedimentary and thermokarst landforms, glacial activity and water erosion features. Reviewed also are hydrous weathering processes, observed on surface remotely and also via analysis of Martian meteorites. Chemistry of Martian water is discussed: the triple point, salts and brines, as well as undercooled liquid interfacial and solid-state greenhouse effect melted waters that may still be present on Mars. Current understanding of the evolution of Martian hydrosphere over geological timescales is presented from early period to the present time, along with the discussion of alternative interpretations and possibilities of dry and wet Mars extremes. 1. INTRODUCTION morphological and mineralogical evidence of aqueous en- The presence of water on Earth, as seen from space, vironments available in the past and, possibly, present can be implied from the observations of low-albedo fea- time is presented in x3 which will be correlated with the tures, like seas and oceans, fluvial features on its sur- current understanding of the evolution of Martian hy- face, atmospheric phenomena, polar ice caps, and the drosphere at x4. Alternative (dry) interpretations of the snow cover exhibiting seasonal variations, not to mention evidence are discussed in x5. spectroscopy. -
Exploring the Lipidomes of Shallow-Water and Deep-Sea Hydrothermal Systems
Exploring the lipidomes of shallow-water and deep-sea hydrothermal systems Dissertation zur Erlangung des Doktorgrades der Naturwissenschaften - Dr. rer. nat. - Am Fachbereich Geowissenschaften der Universität Bremen vorgelegt von Miriam Sollich Bremen Mai 2018 1. Gutachter: Dr. Solveig I. Bühring 2. Gutachter: Associate Prof. Dr. Eoghan P. Reeves Tag des Promotionskolloquiums:16. Februar 2018 Den Wissenschaftlern geht es wie den Chaoten. Es ist alles da, man muss es nur suchen. - Franz Kern - CONTENTS Abstract Zusammenfassung Acknowledgements List of Abbreviations Chapter I 1 Introduction and Methods Chapter II 37 Scope and Outline Chapter III 43 Heat stress dictates the microbial lipid composition along a thermal gradient in marine sediments Chapter IV 91 Shallow-water hydrothermal systems offer ideal conditions to study archaeal lipid membrane adaptations to environmental extremes Chapter V 113 Transfer of chemosynthetic fixed carbon and its ecological significance revealed by lipid analysis of fluids at diffuse flow deep-sea vents (East Pacific Rise 9°50’N) Chapter VI 143 Concluding Remarks and Future Perspectives ABSTRACT Shallow-water and deep-sea hydrothermal systems are environments where seawater percolates downward through fractures in the oceanic crust, and becomes progressively heated and chemically altered. Finally, the entrained water is expelled into the overlying water column as a hydrothermal fluid. Hydrothermal circulation occurs at all active plate boundaries like mid-ocean ridges, submarine volcanic arcs and backarc basins. They represent one of the most extreme and dynamic ecosystems on the planet with steep physico-chemical gradients. Nevertheless, these environments are characterized by exceptional high biomass representing hotspots of life in the mostly hostile and desolated deep sea. -
VV D C-A- R 78-03 National Space Science Data Center/ World Data Center a for Rockets and Satellites
VV D C-A- R 78-03 National Space Science Data Center/ World Data Center A For Rockets and Satellites {NASA-TM-79399) LHNAS TRANSI]_INT PHENOMENA N78-301 _7 CATAI_CG (NASA) 109 p HC AO6/MF A01 CSCl 22_ Unc.las G3 5 29842 NSSDC/WDC-A-R&S 78-03 Lunar Transient Phenomena Catalog Winifred Sawtell Cameron July 1978 National Space Science Data Center (NSSDC)/ World Data Center A for Rockets and Satellites (WDC-A-R&S) National Aeronautics and Space Administration Goddard Space Flight Center Greenbelt) Maryland 20771 CONTENTS Page INTRODUCTION ................................................... 1 SOURCES AND REFERENCES ......................................... 7 APPENDIX REFERENCES ............................................ 9 LUNAR TRANSIENT PHENOMENA .. .................................... 21 iii INTRODUCTION This catalog, which has been in preparation for publishing for many years is being offered as a preliminary one. It was intended to be automated and printed out but this form was going to be delayed for a year or more so the catalog part has been typed instead. Lunar transient phenomena have been observed for almost 1 1/2 millenia, both by the naked eye and telescopic aid. The author has been collecting these reports from the literature and personal communications for the past 17 years. It has resulted in a listing of 1468 reports representing only slight searching of the literature and probably only a fraction of the number of anomalies actually seen. The phenomena are unusual instances of temporary changes seen by observers that they reported in journals, books, and other literature. Therefore, although it seems we may be able to suggest possible aberrations as the causes of some or many of the phenomena it is presumptuous of us to think that these observers, long time students of the moon, were not aware of most of them. -
Raineya Orbicola Gen. Nov., Sp. Nov. a Slightly Thermophilic Bacterium of the Phylum Bacteroidetes and the Description of Raineyaceae Fam
TAXONOMIC DESCRIPTION Albuquerque et al., Int J Syst Evol Microbiol 2018;68:982–989 DOI 10.1099/ijsem.0.002556 Raineya orbicola gen. nov., sp. nov. a slightly thermophilic bacterium of the phylum Bacteroidetes and the description of Raineyaceae fam. nov. Luciana Albuquerque,1 Ana Rita M. Polónia,1 Cristina Barroso,1,2 Hugo J. C. Froufe,2 Olga Lage,3,4 Alexandre Lobo-da-Cunha,4,5 Conceiçao~ Egas1,2 and Milton S. da Costa1,* Abstract An isolate, designated SPSPC-11T, with an optimum growth temperature of about 50 C and an optimum pH for growth between 7.5 and 8.0, was recovered from a hot spring in central Portugal. Based on phylogenetic analysis of its 16S rRNA sequence, the new organism is most closely related to the species of the genus Thermonema but with a pairwise sequence similarity of <85 %. The isolate was orange-pigmented, formed non-motile long filaments and rod-shaped cells that stain Gram-negative. The organism was strictly aerobic, oxidase-positive and catalase-positive. The major fatty acids were iso- C15:0, iso-C15 : 0 2-OH and iso-C17 : 0 3-OH. The major polar lipids were one aminophospholipid, two aminolipids and three unidentified lipids. Menaquinone 7 was the major respiratory quinone. The DNA G+C content of strain SPSPC-11T was 37.6 mol% (draft genome sequence). The high quality draft genome sequence corroborated many of the phenotypic characteristics of strain SPSPC-11T. Based on genotypic, phylogenetic, physiological and biochemical characterization we describe a new species of a novel genus represented by strain SPSPC-11T (=CECT 9012T=LMG 29233T) for which we propose the name Raineya orbicola gen. -
Bilan /Report: 2006 2010 Projet / Project: (2011) 2012 2015
Laboratoired’Astrophysiquede Marseille,UMR6110 Bilan /Report:2006R2010 Projet/Project:(2011)20122015 BILANdel’activitéderecherche20062010/ QuadrennialReport20062010 et/and ProjetQuadriennal(2011)20122015 QuadrennialProject(2011)20122015 LABORATOIRED’ASTROPHYSIQUEDE MARSEILLE«LAM»(UMR6110) Septembre / September 2010 Laboratoire d’Astrophysique de Marseille (UMR 6110) Technopôle de Château-Gombert, 38, rue F. Joliot-Curie - 13388 - MARSEILLE Cedex 13 Tel. 04 91 05 59 00 - Fax 04 91 66 18 55 SOMMAIRE Pages Introduction 6 Chap. I - PRESENTATION GENERALE du LAM / GENERAL LAM PRESENTATION 13 - Stratégie du laboratoire / Strategy - Organigramme et fonctionnement général / General organization Chap. II - BILAN SCIENTIFIQUE / SCIENTIFIC REPORT 35 1 – Introduction 36 2 – Equipes scientifiques / Science teams a) Cosmology, Galaxies, Interstellar medium : - Cosmology 40 - PDG : Physique des Galaxies 55 - PSEG : Populations Stellaires et Evolution des Galaxies 67 - Dynamique des Galaxies 76 - MIS : Milieu Interstellaire 84 b) Exoplanets and Solar System - PASI : Planètes, Atmosphères Stellaires & Interactions 92 - Exoplanet Genesis 101 - Système Solaire 105 c) R&D Optics and Instrumentation - LOOM 113 Chap. III - BILAN TECHNIQUE / TECHNICAL REPORT 125 a) - Département instrumentation et projets / Instrumentation and Projects Department 126 1) Présentation : structure ; compétences ; équipements 2) Projets instrumentaux 3) Plan de charge des Services Techniques 4) Les Services : Optique Mécanique Essais Electronique Soutien aux Projets b) – -
Journal of the Association of Lunar & Planetary Observers
ISSN-0039-2502 Journal of the Association of Lunar & Planetary Observers The Strolling Astronomer Volume 45, Number 1, Winter 2003 Now in Portable Document Format (PDF) for MacIntosh and PC-Compatible Computers Inside...Inside...Inside... More on lunar domes While not the subject of this month’s dome study, we present here a view of lunar dome Mons Gruithuisen Delta (named for Franz von Paul Gruithuisen, a German physician-turned- astronomer) taken from an orbiting Apollo spacecraft. See page 12 for details. • Also . * An ALPO project team to study Saturn’s rings * Isophotes of the Sun * Getting ready for the upcoming Mercury/Venus transits * Getting ready for the Mars apparition * Jupiter and Saturn apparition reports Cover Graphic: John Sanford . plus reports about your ALPO section activities and much, much more. THE ASSOCIATION OF LUNAR AND PLANETARY OBSERVERS (ALPO) P.O. Box 13456, Springfield, Illinois 62791-3456 U.S.A. Thank you for your interest in our organization. The Association of Lunar and Planetary Observers (ALPO) was founded by Walter H. Haas in 1947, and incorporated in 1990, as a medium for advancing and conducting astronomical work by both profes- sional and amateur astronomers who share an interest in Solar System observations. We welcome and provide services for all indi- viduals interested in lunar and planetary astronomy. For the novice observer, the ALPO is a place to learn and to enhance observational techniques. For the advanced amateur astronomer, it is a place where one's work will count. For the professional astronomer, it is a resource where group studies or systematic observing patrols add to the advancement of astronomy. -
Long-Term Trends in Lake-Wide Phytoplankton Productivity in the Upper Great Lakes: 1998-2013
Michigan Technological University Digital Commons @ Michigan Tech Michigan Tech Research Institute Publications Michigan Tech Research Institute 2015 Long-term trends in lake-wide phytoplankton productivity in the Upper Great Lakes: 1998-2013 Gary L. Fahnenstiel Michigan Technological University Michael J. Sayers Michigan Technological University Robert A. Shuchman Michigan Technological University S. A. Pothoven NOAA GLERL Foad Yousef Michigan Technological University Follow this and additional works at: https://digitalcommons.mtu.edu/mtri_p Part of the Physical Sciences and Mathematics Commons Recommended Citation Fahnenstiel, G. L., Sayers, M. J., Shuchman, R. A., Pothoven, S. A., & Yousef, F. (2015). Long-term trends in lake-wide phytoplankton productivity in the Upper Great Lakes: 1998-2013. IAGLR 58th Annual Conference on Great Lakes Research. Retrieved from: https://digitalcommons.mtu.edu/mtri_p/72 Follow this and additional works at: https://digitalcommons.mtu.edu/mtri_p Part of the Physical Sciences and Mathematics Commons ABSTRACTS International Association for Great Lakes Research ABSTRACTS 58th Annual Conference on Great Lakes Research May 25–29, 2015 University of Vermont © 2015 International Association for Great Lakes Research 4890 South State Road Ann Arbor, Michigan 48108 Cover design and conference logo by Jenifer Thomas CONTENTS ABSTRACTS .......................................................................................................... 1 A .......................................................................................................................