Paleogeography and Shore Displacement of Eastern Gotland Between 9.5 and 2.8 Ka Cal BP
Total Page:16
File Type:pdf, Size:1020Kb

Load more
Recommended publications
-
Workshop on the Martiannorthern Plains: Sedimentological,Periglacial, and Paleoclimaticevolution
NASA-CR-194831 19940015909 WORKSHOP ON THE MARTIANNORTHERN PLAINS: SEDIMENTOLOGICAL,PERIGLACIAL, AND PALEOCLIMATICEVOLUTION MSATT ..V",,2' :o_ MarsSurfaceandAtmosphereThroughTime Lunar and PlanetaryInstitute 3600 Bay AreaBoulevard Houston TX 77058-1113 ' _ LPI/TR--93-04Technical, Part 1 Report Number 93-04, Part 1 L • DISPLAY06/6/2 94N20382"£ ISSUE5 PAGE2088 CATEGORY91 RPT£:NASA-CR-194831NAS 1.26:194831LPI-TR-93-O4-PT-ICNT£:NASW-4574 93/00/00 29 PAGES UNCLASSIFIEDDOCUMENT UTTL:Workshopon the MartianNorthernPlains:Sedimentological,Periglacial, and PaleoclimaticEvolution TLSP:AbstractsOnly AUTH:A/KARGEL,JEFFREYS.; B/MOORE,JEFFREY; C/PARKER,TIMOTHY PAA: A/(GeologicalSurvey,Flagstaff,AZ.); B/(NationalAeronauticsand Space Administration.GoddardSpaceFlightCenter,Greenbelt,MD.); C/(Jet PropulsionLab.,CaliforniaInst.of Tech.,Pasadena.) PAT:A/ed.; B/ed.; C/ed. CORP:Lunarand PlanetaryInst.,Houston,TX. SAP: Avail:CASIHC A03/MFAOI CIO: UNITEDSTATES Workshopheld in Fairbanks,AK, 12-14Aug.1993;sponsored by MSATTStudyGroupandAlaskaUniv. MAJS:/*GLACIERS/_MARSSURFACE/*PLAINS/*PLANETARYGEOLOGY/*SEDIMENTS MINS:/ HYDROLOGICALCYCLE/ICE/MARS CRATERS/MORPHOLOGY/STRATIGRAPHY ANN: Papersthathavebeen acceptedforpresentationat the Workshopon the MartianNorthernPlains:Sedimentological,Periglacial,and Paleoclimatic Evolution,on 12-14Aug. 1993in Fairbanks,Alaskaare included.Topics coveredinclude:hydrologicalconsequencesof pondedwateron Mars; morpho!ogical and morphometric studies of impact cratersin the Northern Plainsof Mars; a wet-geology and cold-climateMarsmodel:punctuation -
Pacing Early Mars Fluvial Activity at Aeolis Dorsa: Implications for Mars
1 Pacing Early Mars fluvial activity at Aeolis Dorsa: Implications for Mars 2 Science Laboratory observations at Gale Crater and Aeolis Mons 3 4 Edwin S. Kitea ([email protected]), Antoine Lucasa, Caleb I. Fassettb 5 a Caltech, Division of Geological and Planetary Sciences, Pasadena, CA 91125 6 b Mount Holyoke College, Department of Astronomy, South Hadley, MA 01075 7 8 Abstract: The impactor flux early in Mars history was much higher than today, so sedimentary 9 sequences include many buried craters. In combination with models for the impactor flux, 10 observations of the number of buried craters can constrain sedimentation rates. Using the 11 frequency of crater-river interactions, we find net sedimentation rate ≲20-300 μm/yr at Aeolis 12 Dorsa. This sets a lower bound of 1-15 Myr on the total interval spanned by fluvial activity 13 around the Noachian-Hesperian transition. We predict that Gale Crater’s mound (Aeolis Mons) 14 took at least 10-100 Myr to accumulate, which is testable by the Mars Science Laboratory. 15 16 1. Introduction. 17 On Mars, many craters are embedded within sedimentary sequences, leading to the 18 recognition that the planet’s geological history is recorded in “cratered volumes”, rather than 19 just cratered surfaces (Edgett and Malin, 2002). For a given impact flux, the density of craters 20 interbedded within a geologic unit is inversely proportional to the deposition rate of that 21 geologic unit (Smith et al. 2008). To use embedded-crater statistics to constrain deposition 22 rate, it is necessary to distinguish the population of interbedded craters from a (usually much 23 more numerous) population of craters formed during and after exhumation. -
Late Weichselian and Holocene Shore Displacement History of the Baltic Sea in Finland
Late Weichselian and Holocene shore displacement history of the Baltic Sea in Finland MATTI TIKKANEN AND JUHA OKSANEN Tikkanen, Matti & Juha Oksanen (2002). Late Weichselian and Holocene shore displacement history of the Baltic Sea in Finland. Fennia 180: 1–2, pp. 9–20. Helsinki. ISSN 0015-0010. About 62 percent of Finland’s current surface area has been covered by the waters of the Baltic basin at some stage. The highest shorelines are located at a present altitude of about 220 metres above sea level in the north and 100 metres above sea level in the south-east. The nature of the Baltic Sea has alter- nated in the course of its four main postglacial stages between a freshwater lake and a brackish water basin connected to the outside ocean by narrow straits. This article provides a general overview of the principal stages in the history of the Baltic Sea and examines the regional influence of the associated shore displacement phenomena within Finland. The maps depicting the vari- ous stages have been generated digitally by GIS techniques. Following deglaciation, the freshwater Baltic Ice Lake (12,600–10,300 BP) built up against the ice margin to reach a level 25 metres above that of the ocean, with an outflow through the straits of Öresund. At this stage the only substantial land areas in Finland were in the east and south-east. Around 10,300 BP this ice lake discharged through a number of channels that opened up in central Sweden until it reached the ocean level, marking the beginning of the mildly saline Yoldia Sea stage (10,300–9500 BP). -
Digital Cover
The Littorina transgression in southeastern Sweden and its relation to mid-Holocene climate variability Yu, Shiyong 2003 Link to publication Citation for published version (APA): Yu, S. (2003). The Littorina transgression in southeastern Sweden and its relation to mid-Holocene climate variability. Deaprtment of Geology. Total number of authors: 1 General rights Unless other specific re-use rights are stated the following general rights apply: Copyright and moral rights for the publications made accessible in the public portal are retained by the authors and/or other copyright owners and it is a condition of accessing publications that users recognise and abide by the legal requirements associated with these rights. • Users may download and print one copy of any publication from the public portal for the purpose of private study or research. • You may not further distribute the material or use it for any profit-making activity or commercial gain • You may freely distribute the URL identifying the publication in the public portal Read more about Creative commons licenses: https://creativecommons.org/licenses/ Take down policy If you believe that this document breaches copyright please contact us providing details, and we will remove access to the work immediately and investigate your claim. LUND UNIVERSITY PO Box 117 221 00 Lund +46 46-222 00 00 The Littorina transgression in L southeastern Sweden and its relation to mid-Holocene U climate variability N D Q Shi-Yong Yu U LUNDQUA Thesis 51 Quaternary Sciences A Department of Geology GeoBiosphere Science Centre Lund University T Lund 2003 H E S I S LUNDQUA Thesis 51 The Littorina transgression in southeastern Sweden and its relation to mid-Holocene climate variability Shi-Yong Yu Avhandling att med tillstånd från Naturvetenskapliga Fakulteten vid Lunds Universitet för avläggandet av filosofie doktorsexamen, offentligen försvaras i Geologiska institutionens föreläsningssal Pangea, Sölvegatan 12, Lund, fredagen den 14 november kl. -
Relative Sea Level Changes, Glacio-Isostatic Rebound and Shoreline Displacement in the Southern Baltic
SZYMON UŒCINOWICZ RELATIVE SEA LEVEL CHANGES, GLACIO-ISOSTATIC REBOUND AND SHORELINE DISPLACEMENT IN THE SOUTHERN BALTIC Polish Geological Institute Special Papers,10 WARSZAWA 2003 CONTENTS Introduction ..................................................................6 Area, objective and scope of study ......................................................7 Area of study ...............................................................7 Objective and scope of the work .....................................................8 Analysed materials ............................................................9 Geological setting of the Southern Baltic: an outline .............................................9 Pre-Quaternary ..............................................................9 Quaternary................................................................10 Relative sea level changes ..........................................................11 The problem and methods for its solution ...............................................11 Late Pleistocene and Early Holocene ..................................................18 The turn of Early and Middle Holocene, Middle Holocene ......................................31 Late Holocene ..............................................................35 Vertical crust movements ..........................................................37 Glacio-isostatic rebound: an outline of the problem ..........................................37 Glacio-isostatic movements in the Southern Baltic ...........................................38 -
Case Study of Aeolis Serpens in the Aeolis Dorsa, Mars, and Insight from the Mirackina Paleoriver, South Australia ⇑ Rebecca M.E
Icarus 225 (2013) 308–324 Contents lists available at SciVerse ScienceDirect Icarus journal homepage: www.elsevier.com/locate/icarus Variability in martian sinuous ridge form: Case study of Aeolis Serpens in the Aeolis Dorsa, Mars, and insight from the Mirackina paleoriver, South Australia ⇑ Rebecca M.E. Williams a, , Rossman P. Irwin III b, Devon M. Burr c, Tanya Harrison d,1, Phillip McClelland e a Planetary Science Institute, Tucson, AZ 85719-2395, United States b Center for Earth and Planetary Studies, Smithsonian Institution, Washington, DC 20013-7012, United States c Earth and Planetary Sciences, University of Tennessee, Knoxville, TN 37996-1410, United States d Malin Space Science Systems, San Diego, CA 92121, United States e Ultramag Geophysics, Mount Hutton, NSW 2280, Australia article info abstract Article history: In the largest known population of sinuous ridges on Mars, Aeolis Serpens stands out as the longest Received 3 August 2012 (500 km) feature in Aeolis Dorsa. The formation of this landform, whether from fluvial or glacio-fluvial Revised 6 March 2013 processes, has been debated in the literature. Here we examine higher-resolution data and use a terres- Accepted 10 March 2013 trial analog (the Mirackina paleoriver, South Australia) to show that both the morphology and contextual Available online 2 April 2013 evidence for Aeolis Serpens are consistent with development of an inverted fluvial landform from differ- ential erosion of variably cemented deposits. The results of this study demonstrate that the induration Keywords: mechanism can affect preservation of key characteristics of the paleoriver morphology. For groundwater Mars, Surface cemented inverted fluvial landforms, like the Mirackina example, isolated remnants of the paleoriver are Geological processes Earth preserved because of the temporal and spatial variability of cementation sites. -
Peter Weiss. Andrei Platonov. Ragnvald Blix. Georg Henrik Von Wright. Adam Michnik
A quarterly scholarly journal and news magazine. March 2011. Vol IV:1 From the Centre for Baltic and East European Studies (CBEES) Södertörn University, Stockholm FEATURE. Steklov – Russian BALTIC temple of pure thought W O Rbalticworlds.com L D S COPING WITH TRANSITIONS PETER WEISS. ANDREI PLATONOV. RAGNVALD BLIX. GEORG HENRIK VON WRIGHT. ADAM MICHNIK. SLAVENKA DRAKULIĆ. Sixty pages BETRAYED GDR REVOLUTION? / EVERYDAY BELARUS / WAVE OF RELIGION IN ALBANIA / RUSSIAN FINANCIAL MARKETS 2short takes Memory and manipulation. Transliteration. Is anyone’s suffering more important than anyone else’s? Art and science – and then some “IF YOU WANT TO START a war, call me. Transliteration is both art and science CH I know all about how it's done”, says – and, in many cases, politics. Whether MÄ author Slavenka Drakulić with a touch царь should be written as tsar, tzar, ANNA of gallows humor during “Memory and czar, or csar may not be a particu- : H Manipulation: Religion as Politics in the larly sensitive political matter today, HOTO Balkans”, a symposium held in Lund, but the question of the transliteration P Sweden, on December 2, 2010. of the name of the current president This issue of the journal includes a of Belarus is exceedingly delicate. contribution from Drakulić (pp. 55–57) First, and perhaps most important: in which she claims that top-down gov- which name? Both the Belarusian ernance, which started the war, is also Аляксандр Лукашэнка, and the Rus- the path to reconciliation in the region. sian Александр Лукашенко are in use. Balkan experts attending the sympo- (And, while we’re at it, should that be sium agree that the war was directed Belarusian, or Belarussian, or Belaru- from the top, and that “top-down” is san, or Byelorussian, or Belorussian?) the key to understanding how the war BW does not want to take a stand on began in the region. -
Analysis Ofcryokarstic Surfacepatterns on Debris
42nd Lunar and Planetary Science Conference (2011) 1305.pdf ANALYSIS OF CRYOKARSTIC SURFACE PATTERNS ON DEBRIS APRONS AT THE MID–LATITUDES OF MARS. Cs. Orgel, Department of Physical and Applied Geology, Eötvös Loránd University, H-1117, Pázmány Péter sétány 1/C, Budapest, Hungary ([email protected]). Introduction: The presence of ice-related glacier-like Perpendicular (Fig.1./J) and parallel (Fig.1./K) furrows landforms on the Martian mid-latitudes have been have been observed in Deuteronilus-A on inner crater studying on the basis of Viking imagery. These features walls, parallel ones are possible the result of melting are evidences of colder climatic conditions in the Mar- flows or gully processes near the faults-like features. tian geologic history, which have three proposed origin Verges of furrows in Hourglass region are rounded, [1][2][3]. Three types of landforms are distinguished on causing of viscous material. (3) The craters of the debris Mars: Lobate Debris Aprons (LDA), Lineated Valley apron surfaces are classificated in different types: 1. Fills (LVF), and Concentric Crater Fills (CCF) [4][5][6]. Pitted ring-mold craters (Fig.1./G). 2. Bowl-shaped cra- This work focuses on the morphological analysis and ters (Fig.1./H). 3. Inverted-relief craters (Fig.1./I). 4. interpretation of the surface patterns like mounds, fur- Softened craters. Deuteronilus-A has small, high num- rows, ridges, pits, craters, and different surface types ber of bowl-shaped craters, which can indicate low- like „smooth surface”, „corn-like surface”, polygonal percent of ice in the near-surface layers. Hourglass has mantling material and „brain-like texture” based on larger and lesser number of craters than Deuteronilus-A MRO HiRISE’s images [6][7][8]. -
The Late Quaternary Development of the Baltic Sea
The late Quaternary development of the Baltic Sea Svante Björck, GeoBiosphere Science Centre, Department of Geology, Quaternary Sciences, Lund University, Sölveg. 12, SE-223 62 Lund, Sweden INTRODUCTION Since the last deglaciation of the Baltic basin, which began 15 000-17 000 cal yr BP (calibrated years Before Present) and ended 11 000-10 000 cal yr BP, the Baltic has undergone many very different phases. The nature of these phases were determined by a set of forcing factors: a gradually melting Scandinavian Ice Sheet ending up into an interglacial environment, the highly differential glacio-isostatic uplift within the basin (from 9 mm/yr to -1mm/yr; Ekman 1996), changing geographic position of the controlling sills (Fig. 1), varying depths and widths of the thresholds between the sea and the Baltic basin, and climate change. These factors have caused large variations in salinity and water exchange with the outer ocean, rapid to gradual paleographic alterations with considerable changes of the north-south depth profile with time. For example, the area north of southern Finland-Stockholm has never experienced transgressions, or land submergence, while the developmen south of that latitude has been very complex. The different controlling factors are also responsible for highly variable sedimentation rates, both in time and space, and variations of the aquatic productivity as well as faunal and floral changes. The basic ideas in this article follow the lengthy, but less up-dated version of the Baltic Sea history (Björck, 1995), a more complete reference list and, e.g., the calendar year chronology of the different Baltic phases can be found on: http://www.geol.lu.se/personal/seb/Maps%20of%20the%20Baltic.htm. -
Extensive Noachian Fluvial Systems in Arabia Terra: Implications for Early Martian Climate
Extensive Noachian fluvial systems in Arabia Terra: Implications for early Martian climate J.M. Davis1*, M. Balme2, P.M. Grindrod3, R.M.E. Williams4, and S. Gupta5 1Department of Earth Sciences, University College London, London WC1E 6BT, UK 2Department of Physical Sciences, Open University, Walton Hall, Milton Keynes MK7 6AA, UK 3Department of Earth and Planetary Sciences, Birkbeck, University of London, Malet Street, London WC1E 7HU, UK 4Planetary Science Institute, 1700 E. Fort Lowell, Suite 106, Tucson, Arizona 85719, USA 5Department of Earth Sciences and Engineering, Imperial College London, London SW7 2AZ, UK ABSTRACT strata, as much as hundreds of meters thick, that mantle the topography Valley networks are some of the strongest lines of evidence for (e.g., Moore, 1990; Fassett and Head, 2007). They are more eroded in the extensive fluvial activity on early (Noachian; >3.7 Ga) Mars. How- north, where they become discontinuous and then absent (e.g., Zabrusky ever, their purported absence on certain ancient terrains, such as et al., 2012). In the south, the Meridiani Planum region is covered by the Arabia Terra, is at variance with patterns of precipitation as predicted youngest etched unit, interpreted to be early Hesperian (ca. 3.6–3.7 Ga; by “warm and wet” climate models. This disagreement has contrib- Hynek and Di Achille, 2016). uted to the development of an alternative “icy highlands” scenario, These observations suggest that valley networks in Arabia Terra might whereby valley networks were formed by the melting of highland ice have been buried by the etched units and/or removed by later erosion. -
Inverted Relief Landforms in the Kumtagh Desert of Northwestern China: a Mechanism to Estimate Wind Erosion Rates
GEOLOGICAL JOURNAL Geol. J. 52: 131–140 (2017) Published online 13 November 2015 in Wiley Online Library (wileyonlinelibrary.com). DOI: 10.1002/gj.2739 Inverted relief landforms in the Kumtagh Desert of northwestern China: a mechanism to estimate wind erosion rates ZHEN-TING WANG1,2*, ZHONG-PING LAI3 and JIAN-JUN QU2 1State Key Laboratory of Earth Surface Processes and Resource Ecology, Beijing Normal University, Beijing, China 2Dunhuang Gobi Desert Research Station, Cold and Arid Regions Environmental and Engineering Research Institute, CAS, Dunhuang, China 3State Key Laboratory of Biogeology and Environmental Geology, China University of Geosciences, Wuhan, China Although commonly found in deserts, our knowledge about inverted relief landforms is very limited. The so-called ‘Gravel Body’ in the northern Kumtagh Desert is an example of an inverted relief landform created by the exhumation of a former fluvial gravel channel. The common occurrence of these landforms indicates that fluvial processes played an important role in shaping the Kumtagh Desert in the past 151 ka. A physical model is presented to reconstruct the palaeohydrology of these fluvial channels in terms of several measurable parameters including terrain slope, boulder size, and channel width. Combining the calculated palaeoflood depth, the maximal depth of channel bed eroded by wind, and the current height of inverted channels with the age of the aeolian sediments covered by gravels, the local wind erosion rate is estimated to be 0.21–0.28 mm/year. It is shown that wind erosion occurring in the Kumtagh Desert is no more severe than in adjacent regions. Since the modern Martian environment is very similar to that of hyperarid deserts on Earth, and Mars was once subjected to fluvial processes, this study will be helpful for understanding the origin of analogous Martian surface landforms and their causative processes. -
•1I1ii11i11 Se0000219
•1I1II11I11 SE0000219 Technical Report TR-99-38 Salinity change in the Baltic Sea during the last 8,500 years: evidence, causes and models Per Westman, Stefan Wastegard, Kristian Schoning Department of Quaternary Research, Stockholm University Bo Gustafsson Oceanus Havsundersokningar, Goteborg Anders Omstedt, SMHl, Norrkoping December 1999 Svensk Karnbranslehantering AB Swedish Nuclear Fuel and Waste Management Co Box 5864 102 40 Stockholm Tel 08-459 84 00 Fax 08-661 57 19 3 1/ 21 Salinity change in the Baltic Sea during the last 8,500 years: evidence, causes and models Per Westman, Stefan Wastegard, Kristian Scheming Department of Quaternary Research, Stockholm University Bo Gustafsson Oceanus Havsundersokningar, Goteborg Anders Omstedt, SMHI, Norrkoping December 1999 Keywords: biosphere, salinity, landrise, surface ecosystem, palaeo salinity This report concerns a study which was conducted for SKB. The conclusions and viewpoints presented in the report are those of the author(s) and do not necessarily coincide with those of the client. NEXT PAGE(S) left BLANK Abstract The salinity influences which ecosystems will dominate in the coastal area and what property radionuclides have. Salinity is also an important boundary condition for the transport models in the geosphere. Knowledge about the past salinity is important background to evaluate the hydrology and geochemistry in the rock and further to assess the radiological consequences of possible releases from a radioactive repository. This report concerns the salinity in the Baltic Sea during the last 8500 calendar years BP. Shore-level data for the inlet areas and proxy (indirect) data for the palaeosalinity and the climate are reviewed. These data is furthered used in a steady-state model for the salt exchange between the Baltic Sea and Kattegat.