The Earth Has a Future
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Inferences on Potential Seamount Locations from Mid-Resolution
T. Morato and D. Pauly (eds.), Seamounts: Biodiversity and Fisheries, Page 7 INFERENCES ON POTENTIAL SEAMOUNT LOCATIONS FROM MID- RESOLUTION BATHYMETRIC DATA Adrian Kitchingman and Sherman Lai Fisheries Centre, The University of British Columbia. 2259 Lower Mall, Vancouver, B.C., V6T 1Z4, Canada [email protected]; [email protected] ABSTRACT Seamounts are underwater volcanoes that did not grow tall enough to break to the sea surface and turn into islands. Once formed, seamounts tend to gradually sink under their own weight and the subsidence of the lithosphere. The ocean floor is littered with these former seamounts, here called ‘seamounds’. Seamounts occur throughout the world's oceans, but their number (which may surpass 50,000) is difficult to estimate, even roughly, because it depends on the resolution of the bathymetric map used and the specific definition of a seamount used, i.e., the limits used to distinguish between seamounts and seamounds. Here, the locations of a subset of the seamounts of the world were identified using two algorithms relying on the depth differences between adjacent cells of a digital global elevation map distributed by the U.S. National Oceanographic and Atmospheric Agency (NOAA). The overlap of both algorithms resulted in a set of about 14,000 seamounts, but a different number would have been found had we used different thresholds. Known seamount locations supplied by NOAA and SeamountsOnline (http://seamounts.sdsc.edu) were compared against the corresponding seamounts located by the study, which led to some degree of ground-truthing. The coordinates of the seamounts identified in this study are available on the CD-ROM attached to this report, and on http://www.seaaroundus.org. -
Solar System Exploration
Theme: Solar System Exploration Cassini, a robotic spacecraft launched in 1997 by NASA, is close enough now to resolve many rings and moons of its destination planet: Saturn. The spacecraft has now closed to within a single Earth-Sun separation from the ringed giant. In November 2003, Cassini snapped the contrast-enhanced color composite pictured above. Many features of Saturn's rings and cloud-tops now show considerable detail. When arriving at Saturn in July 2004, the Cassini orbiter will begin to circle and study the Saturnian system. Several months later, a probe named Huygens will separate and attempt to land on the surface of Titan. Solar System Exploration MAJOR EVENTS IN FY 2005 Deep Impact will launch in December 2004. The spacecraft will release a small (820 lbs.) Impactor directly into the path of comet Tempel 1 in July 2005. The resulting collision is expected to produce a small impact crater on the surface of the comet's nucleus, enabling scientists to investigate the composition of the comet's interior. Onboard the Cassini orbiter is a 703-pound scientific probe called Huygens that will be released in December 2004, beginning a 22-day coast phase toward Titan, Saturn's largest moon; Huygens will reach Titan's surface in January 2005. ESA 2-1 Theme: Solar System Exploration OVERVIEW The exploration of the solar system is a major component of the President's vision of NASA's future. Our cosmic "neighborhood" will first be scouted by robotic trailblazers pursuing answers to key questions about the diverse environments of the planets, comets, asteroids, and other bodies in our solar system. -
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. -
National Weather Service High Wind Warning
National Weather Service Text Product Display https://forecast.weather.gov/product.php?site=HFO&issuedby=HFO&pr... National Weather Service Weather Forecast Office Honolulu, HI Non-Precipitation Warnings / Watches / Advisories Issued by NWS Honolulu, HI Home | Current Version | Previous Version | Text Only | Print | Product List | Glossary On Versions: 1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 000 WWHW70 PHFO 071330 NPWHFO URGENT - WEATHER MESSAGE National Weather Service Honolulu HI 330 AM HST Sat Mar 7 2020 ...HIGH WIND WARNING FOR LEEWARD WEST MAUI LANAI KAHOOLAWE AND THE LEEWARD KOHALA DISTRICT UNTIL 6 PM HST THIS EVENING... ...WIND ADVISORY FOR ALL HAWAIIAN ISLANDS UNTIL 6 PM HST THIS EVENING... .High pressure far north of the islands will support strong to locally damaging trade winds today, with winds gradually weakening tonight and Sunday. HIZ014>016-018-026-080400- /O.CON.PHFO.HW.W.0003.000000T0000Z-200308T0400Z/ Lanai Makai-Lanai Mauka-Kahoolawe-Maui Leeward West-Kohala- Including the cities of Manele, Lanai City, Lahaina, Kaanapali, and Waikoloa 330 AM HST Sat Mar 7 2020 ...HIGH WIND WARNING REMAINS IN EFFECT UNTIL 6 PM HST THIS EVENING... * WHAT...Northeast winds 30 to 40 mph with localized gusts over 60 mph. * WHERE...Leeward West Maui, Lanai, Kahoolawe and the Leeward Kohala District on the Big Island. * WHEN...Until 6 PM HST this evening. * IMPACTS...Damaging winds will blow down trees and power lines. Sporadic power outages can be expected. Travel will be difficult, especially for high profile vehicles. PRECAUTIONARY/PREPAREDNESS ACTIONS... Motorists, especially those in high profile vehicles, are urged to drive with extreme caution. -
The Kingdom of Tonga Devastated by a Megatsunami in the Mid-15Th Century
EGU21-5317, updated on 25 Sep 2021 https://doi.org/10.5194/egusphere-egu21-5317 EGU General Assembly 2021 © Author(s) 2021. This work is distributed under the Creative Commons Attribution 4.0 License. The kingdom of Tonga devastated by a megatsunami in the mid-15th century Franck Lavigne1,2,3, Julie Morin4, Wassmer Patrick2, Weller Olivier5, Kula Taaniela6, Ana V. Maea6, Karim Kelfoun7, Fatima Mokadem2, Raphael Paris7, Mukhamad N. Malawani1,2,8, Faral Audrey1,2, Mhammed Benbakkar7, Ségolène Saulnier-Copard2, Céline M. Vidal4, Tu’I’ahai Tu’I’afitu6, Gomez Christopher9, and Fuka Kitekei’aho10 1Paris 1 Pantheon-Sorbonne University, ([email protected]) 2Laboratory of Physical Geography, UMR 8591 CNRS, Meudon, France 3Institut Universitaire de France, Paris, France 4Department of Geography, University of Cambridge, Cambridge, UK 5Trajectoires, UMR 8215 CNRS, Paris, France 6Ministry of Land and Natural Resources, Natural Resources Division, Nuku'alofa, Kingdom of Tonga 7Laboratoire Magmas et Volcans, Université Clermont Auvergne, CNRS, IRD, OPGC, France 8Faculty of Geography, Universitas Gadjah Mada, Yogyakarta, Indonesia 9Laboratory of Sediment Hazards and Disaster Risk, Kobe University, Japan 10Geocare & Petroleum Consult Ltd, Nuku'alofa, Kingdom of Tonga The pre-colonial history of Tonga and West Polynesia still suffers from major gaps because its reconstruction is essentially based on legends left by oral tradition, and by archaeological evidence somehow difficult to interpret. By the fourteenth century, the powerful Tu'i Tonga kingdom united the islands of the Tongan archipelago under a centralised authority and, according to tradition, extended its influence to neighbouring island groups in the Central Pacific. However, some periods of deep crisis were identified, e.g. -
Literature Review of Tsunami Sources Affecting Tsunami Hazard Along the US East Coast
Literature review of tsunami sources affecting tsunami hazard along the US East Coast Department of Ocean Engineering, University of Rhode Island Narragansett, USA Feb. 21, 2011 1 TABLE OF CONTENTS 1. BACKGROUND ...................................................................................................................... 3 2. LITERATURE REVIEW OF RELEVANT TSUNAMI SOURCES .................................... 5 2.1 Submarine Mass Failures ........................................................................................................ 5 2.2 Co-seismic tsunamis .................................................................................................................. 8 2.2.1 Review of literature on Caribbean subduction zone ............................................................. 8 2.2.2 NOAA Forecast Source Database for Caribbean subduction zone ............................... 16 2.2.3 Azores-Gibraltar convergence zone .......................................................................................... 17 2.3 Cumbre Vieja Volcano flanK collapse ............................................................................... 21 3. INITIAL SOURCE DEFINITIONS AND TSUNAMI SIMULATIONS .......................... 24 3.1 Modeling methodology .......................................................................................................... 24 3.1.1 Initial conditions for model .......................................................................................................... 24 3.1.2 Co-seismic sources -
Precontact Vegetation and Soil Nutrient Status in the Shadow of Kohala Volcano, Hawaii ⁎ Oliver A
Geomorphology 89 (2007) 70–83 www.elsevier.com/locate/geomorph Precontact vegetation and soil nutrient status in the shadow of Kohala Volcano, Hawaii ⁎ Oliver A. Chadwick a, , Eugene F. Kelly b, Sara C. Hotchkiss c, Peter M. Vitousek d a Department of Geography, University of California, Santa Barbara, CA 93106, USA b Department of Crop and Soil Science, Colorado State University, Fort Collins, CO 80523, USA c Department of Botany, University of Wisconsin, Madison, WI 53706, USA d Department of Biological Sciences, Stanford University, Stanford, CA 94305, USA Received 13 January 2005; received in revised form 25 July 2006; accepted 25 July 2006 Available online 2 October 2006 Abstract Humans colonized Hawaii about 1200 years ago and have progressively modified vegetation, particularly in mesic to dry 13 tropical forests. We use δ C to evaluate the contribution of C3 and C4 plants to deep soil organic matter to reconstruct pre-human contact vegetation patterns along a wet to dry climate transect on Kohala Mountain, Hawaii Island. Precontact vegetation assemblages fall into three distinct zones: a wet C3 dominated closed canopy forest where annual rainfall is N2000 mm, a dry C4 dominated grassland with annual rainfall b500 mm, and a broad transition zone between these communities characterized by either C3 trees with higher water-use efficiency than the rainforest trees or C3 trees with a small amount of C4 grasses intermixed. The likelihood of C4 grass understory decreases with increasing rainfall. We show that the total concentration of rock-derived nutrients in the b2-mm soil fraction differs in each of these vegetation zones. -
Importance of Seamount-Like Features for Conserving Mediterranean Marine Habitats and Threatened Species
Nº. 1105 IMPORTANCE OF SEAMOUNT-LIKE FEATURES FOR CONSERVING MEDITERRANEAN MARINE HABITATS AND THREATENED SPECIES Ricardo Aguilar, Xavier Pastor, Silvia García & Pilar Marín Oceana. Leganitos, 47 - 28013 Madrid. Spain - *[email protected] INTRODUCTION HABITAT LOCATION MAIN SPECIES 16 of the more than 200 seamount‑like peaks in the Mediterranean1 have been observed using ROV. Coral reefs 4, 5, 6, 7 Lophelia pertusa, Madrepora oculata Desmophyllum dianthus, Stenocyathus vermiformis, The findings, which include carnivorous sponges, elasmobranches, coral gardens, sponge aggregations, Cold water corals All sites Caryophyllia spp. Pourtalosmilia anthophyllites, Javania caileti, coralligenous beds, as well as species new to science like the giant foraminifera Spiculosiphon oceana, Anomocora fecunda, Dendrophyllia spp. Paramuricea spp., Eunicella spp., Viminella flagellum, or new to the Mediterranean, like the scleractinian Anomocora fecunda, underscore the importance of 1, 2, 3, 4, 5, Callogorgia verticillata, Acanthogorgia spp., Placogorgia these geological features as hotspots and shelters/refuges species and habitats that are threatened, in Gorgonian/coral gardens: 6, 7, 8, 9, 11, coronata, Swiftia pallida, Muriceides lepida, Villogorgia regression, or rare in other Mediterranean areas. 12, 13, 14 bebrycoides, Bebryce mollis, Nicella granifera 1, 4, 5, 6, 7, Leiopathes glaberrima, Antipathes dichotoma, Antipathella METHODOLOGY Black corals Since 2006, Oceana has carried out six expeditions in the Mediterranean performing 129 ROV’s dives 9, 11, 15, 16 subpinnata, Parantipathes larix Isidella elongata, Pennatula spp., Pteroeides griseum, 2, 3, 4, 7, 8, over 16 seamounts, between ‑37 and ‑638 meters deep. Soft bottoms’ octocorals Virgularia mirabilis, Veretillun cynomorium, Kophobelemnon 9, 11, 14, 16 RESULTS stelliferum, Funiculina quadrangularis 2 3, 4, 5, 6, 7, Asconema setubalense, Phakellia spp., Axinella spp. -
What Is the Future of Earth's Climate?
What is the Future of Earth’s Climate? Introduction The question of whether the Earth is warming is one of the most intriguing questions that scientists are dealing with today. Climate has a significant influence on all of Earth’s ecosystems today. What will future climates be like? Scientists have begun to examine ice cores dating back over 100 years to study the changes in the concentrations of carbon dioxide gas from carbon emissions to see if a true correlation exists between human impact and increasing temperatures on Earth. CO2 from Carbon Emissions This has led many scientists to ask the question: What will future climates be like? Today, you will interact, ask questions, and analyze data from the NASA Goddard Institute for Space Studies to generate some predictions about global climate change in the future. Review the data of global climate change on the slide below. Complete the questions on the following slide. This link works! Graphics Courtesy: NASA Goodard Space Institute-- https://data.giss.nasa.gov/gistemp/animations/5year_2y.mp4 Looking at the data... 1. Between what years was the greatest change in overall climate observed? 2. Using what you know, what happened in this time period that may have attributed to these changes in global climate? 3. How might human activities contribute to these changes? What more information would you need to determine how humans may have impacted global climate change? Is there a connection between fossil fuel consumption and global climate change? Temperature Change 1880-2020 CO2 Levels (ppm) from 2006-2018 Examine the graphs above. -
Bildnachweis
Bildnachweis Im Bildnachweis verwendete Abkürzungen: With permission from the Geological Society of Ame- rica l – links; m – Mitte; o – oben; r – rechts; u – unten 4.65; 6.52; 6.183; 8.7 Bilder ohne Nachweisangaben stammen vom Autor. Die Autoren der Bildquellen werden in den Bildunterschriften With permission from the Society for Sedimentary genannt; die bibliographischen Angaben sind in der Literaturlis- Geology (SEPM) te aufgeführt. Viele Autoren/Autorinnen und Verlage/Institutio- 6.2ul; 6.14; 6.16 nen haben ihre Einwilligung zur Reproduktion von Abbildungen gegeben. Dafür sei hier herzlich gedankt. Für die nachfolgend With permission from the American Association for aufgeführten Abbildungen haben ihre Zustimmung gegeben: the Advancement of Science (AAAS) Box Eisbohrkerne Dr; 2.8l; 2.8r; 2.13u; 2.29; 2.38l; Box Die With permission from Elsevier Hockey-Stick-Diskussion B; 4.65l; 4.53; 4.88mr; Box Tuning 2.64; 3.5; 4.6; 4.9; 4.16l; 4.22ol; 4.23; 4.40o; 4.40u; 4.50; E; 5.21l; 5.49; 5.57; 5.58u; 5.61; 5.64l; 5.64r; 5.68; 5.86; 4.70ul; 4.70ur; 4.86; 4.88ul; Box Tuning A; 4.95; 4.96; 4.97; 5.99; 5.100l; 5.100r; 5.118; 5.119; 5.123; 5.125; 5.141; 5.158r; 4.98; 5.12; 5.14r; 5.23ol; 5.24l; 5.24r; 5.25; 5.54r; 5.55; 5.56; 5.167l; 5.167r; 5.177m; 5.177u; 5.180; 6.43r; 6.86; 6.99l; 6.99r; 5.65; 5.67; 5.70; 5.71o; 5.71ul; 5.71um; 5.72; 5.73; 5.77l; 5.79o; 6.144; 6.145; 6.148; 6.149; 6.160; 6.162; 7.18; 7.19u; 7.38; 5.80; 5.82; 5.88; 5.94; 5.94ul; 5.95; 5.108l; 5.111l; 5.116; 5.117; 7.40ur; 8.19; 9.9; 9.16; 9.17; 10.8 5.126; 5.128u; 5.147o; 5.147u; -
Geology, Geochemistry and Earthquake History of Lō`Ihi Seamount, Hawai`I
INVITED REVIEW Geology, Geochemistry and Earthquake History of Lō`ihi Seamount, Hawai`i Michael O. Garcia1*, Jackie Caplan-Auerbach2, Eric H. De Carlo3, M.D. Kurz4 and N. Becker1 1Department of Geology and Geophysics, University of Hawai`i, Honolulu, HI, USA 2U.S.G.S., Alaska Volcano Observatory, Anchorage, AK, USA 3Department of Oceanography, University of Hawai`i, Honolulu, HI, USA 4Department of Chemistry, Woods Hole Oceanographic Institution, Woods Hole, MA, USA *Corresponding author: Tel.: 001-808-956-6641, FAX: 001-808-956-5521; email: [email protected] Key words: Loihi, seamount, Hawaii, petrology, geochemistry, earthquakes Abstract A half century of investigations are summarized here on the youngest Hawaiian volcano, Lō`ihi Seamount. It was discovered in 1952 following an earthquake swarm. Surveying in 1954 determined it has an elongate shape, which is the meaning of its Hawaiian name. Lō`ihi was mostly forgotten until two earthquake swarms in the 1970’s led to a dredging expedition in 1978, which recovered young lavas. This led to numerous expeditions to investigate the geology, geophysics, and geochemistry of this active volcano. Geophysical monitoring, including a real- time submarine observatory that continuously monitored Lō`ihi’s seismic activity for three months, captured some of the volcano’s earthquake swarms. The 1996 swarm, the largest recorded in Hawai`i, was preceded by at least one eruption and accompanied by the formation of a ~300-m deep pit crater, renewing interest in this submarine volcano. Seismic and petrologic data indicate that magma was stored in a ~8-9 km deep reservoir prior to the 1996 eruption. -
Chapter 51. Biological Communities on Seamounts and Other Submarine Features Potentially Threatened by Disturbance
Chapter 51. Biological Communities on Seamounts and Other Submarine Features Potentially Threatened by Disturbance Contributors: J. Anthony Koslow, Peter Auster, Odd Aksel Bergstad, J. Murray Roberts, Alex Rogers, Michael Vecchione, Peter Harris, Jake Rice, Patricio Bernal (Co-Lead members) 1. Physical, chemical, and ecological characteristics 1.1 Seamounts Seamounts are predominantly submerged volcanoes, mostly extinct, rising hundreds to thousands of metres above the surrounding seafloor. Some also arise through tectonic uplift. The conventional geological definition includes only features greater than 1000 m in height, with the term “knoll” often used to refer to features 100 – 1000 m in height (Yesson et al., 2011). However, seamounts and knolls do not appear to differ much ecologically, and human activity, such as fishing, focuses on both. We therefore include here all such features with heights > 100 m. Only 6.5 per cent of the deep seafloor has been mapped, so the global number of seamounts must be estimated, usually from a combination of satellite altimetry and multibeam data as well as extrapolation based on size-frequency relationships of seamounts for smaller features. Estimates have varied widely as a result of differences in methodologies as well as changes in the resolution of data. Yesson et al. (2011) identified 33,452 seamount and guyot features > 1000 m in height and 138,412 knolls (100 – 1000 m), whereas Harris et al. (2014) identified 10,234 seamount and guyot features, based on a stricter definition that restricted seamounts to conical forms. Estimates of total abundance range to >100,000 seamounts and to 25 million for features > 100 m in height (Smith 1991; Wessel et al., 2010).