Petrology of the I Volcanic Rocks of Guam
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2009 Medals & Awards Mary C. Rabbitt History of Geology
2009 MEDALS & AWARDS MARY C. RABBITT emeritus since 2004. During his time at But there is more. As he is credited Calvin he was for a year a Fellow at the to be in several web sites, he is a noted HISTORY OF Calvin Center for Christian Scholarship. conservative evangelical Christian who is GEOLOGY AWARD He is a member of GSA, the Mineralogical also a geologist—and is a fine example of Society of America, the American Scientific both. As such, he has access to venues that Presented to Davis A. Young Affiliation, the Affiliation of Christian few of us can address, and is a spokesman Geologists, of which he has been president, for our science with a unique authority. His and the International Commission on the reviews of important books in the history of History of the Geological Sciences. geology speak to a wider audience than many In his long teaching career, I’m sure of us can reach. Dave will tell us more of his Dave has steered many a young person to journey. The Rabbitt Award is most fitting geology, and his department has just instituted recognition of Davis Young. a student Summer Research Fellowship in his name. He co-led a course on Hawaiian geology in the best of places, Hawaii itself. Response by Davis A. Young Reading the program for that, I envy the My profoundest gratitude to the History students who were able to take part in it. With of Geology Division for bestowing this student help, he has also assisted with the honor on me. -
History of Geology
FEBRUARY 2007 PRIMEFACT 563 (REPLACES MINFACT 60) History of geology Mineral Resources Early humans needed a knowledge of simple geology to enable them to select the most suitable rock types both for axe-heads and knives and for the ornamental stones they used in worship. In the Neolithic and Bronze Ages, about 5000 to 2500 BC, flint was mined in the areas which are now Belgium, Sweden, France, Portugal and Britain. While Stone Age cultures persisted in Britain until after 2000 BC, in the Middle East people began to mine useful minerals such as iron ore, tin, clay, gold and copper as early as 4000 BC. Smelting techniques were developed to make the manufacture of metal tools possible. Copper was probably the earliest metal to be smelted, that is, extracted from its ore by melting. Copper is obtained easily by reducing the green copper carbonate mineral malachite, itself regarded as a precious stone. From 4000 BC on, the use of clay for brick-making became widespread. The Reverend William Branwhite Clarke (1798-1878), smelting of iron ore for making of tools and the ‘father’ of geology in New South Wales weapons began in Asia Minor at about 1300 BC but did not become common in Western Europe until Aristotle believed volcanic eruptions and nearly 500 BC. earthquakes were caused by violent winds escaping from the interior of the earth. Since earlier writers had ascribed these phenomena to The classical period supernatural causes, Aristotle's belief was a By recognising important surface processes at marked step forward. Eratosthenes, a librarian at work, the Greek, Arabic and Roman civilisations Alexandria at about 200 BC, made surprisingly contributed to the growth of knowledge about the accurate measurements of the circumference of earth. -
Bedrock Geology Glossary from the Roadside Geology of Minnesota, Richard W
Minnesota Bedrock Geology Glossary From the Roadside Geology of Minnesota, Richard W. Ojakangas Sedimentary Rock Types in Minnesota Rocks that formed from the consolidation of loose sediment Conglomerate: A coarse-grained sedimentary rock composed of pebbles, cobbles, or boul- ders set in a fine-grained matrix of silt and sand. Dolostone: A sedimentary rock composed of the mineral dolomite, a calcium magnesium car- bonate. Graywacke: A sedimentary rock made primarily of mud and sand, often deposited by turbidi- ty currents. Iron-formation: A thinly bedded sedimentary rock containing more than 15 percent iron. Limestone: A sedimentary rock composed of calcium carbonate. Mudstone: A sedimentary rock composed of mud. Sandstone: A sedimentary rock made primarily of sand. Shale: A deposit of clay, silt, or mud solidified into more or less a solid rock. Siltstone: A sedimentary rock made primarily of sand. Igneous and Volcanic Rock Types in Minnesota Rocks that solidified from cooling of molten magma Basalt: A black or dark grey volcanic rock that consists mainly of microscopic crystals of pla- gioclase feldspar, pyroxene, and perhaps olivine. Diorite: A plutonic igneous rock intermediate in composition between granite and gabbro. Gabbro: A dark igneous rock consisting mainly of plagioclase and pyroxene in crystals large enough to see with a simple magnifier. Gabbro has the same composition as basalt but contains much larger mineral grains because it cooled at depth over a longer period of time. Granite: An igneous rock composed mostly of orthoclase feldspar and quartz in grains large enough to see without using a magnifier. Most granites also contain mica and amphibole Rhyolite: A felsic (light-colored) volcanic rock, the extrusive equivalent of granite. -
Ecology in Palau Chapter 1
ECOLOGY IN PALAU CHAPTER 1 CHAPTER 1 also has the largest tract of tropical lowland Ecology in Palau forest in the Pacific (Kitalong, 2014). In 1979, nearly 218 km2 or 52% of Palau’s land was The landscape of Palau is one of a medium to covered with lowland forests. Yet, slowly, forests low volcanic island chain with large fringing ECOLOGY IN PALAU are being cut for homesteads, development and/or barrier reefs. The Palauan island chain and roads. Forest trees and plants are valued as has all three-island types: volcanic, limestone Christopher Kitalong, David Mason sources of timber, food, medicine, habitat for and atolls. Palau’s proximity to the Asian other species, and for their cultural and aesthetic continent, Philippines, and Indonesia results Settings value (Kitalong, 2008). in increased radiation of plant taxa compared The archipelago of Palau was formed during to other islands in Micronesia. Despite being the Eocene epoch, 40 million years ago by the closest Micronesian island to larger land the subduction of the Pacific Plate beneath masses, Palau is still relatively isolated. Due the Philippine Plate along the Kyushu-Palau to these factors, Palau has the greatest number Ridge (PALARIS, 2009). Palau lies on the of endemics and highest species richness in east edge of the Andesite Line, which divides the Micronesian island chain (Canfield, 1981). the deeper basalts of the Central Pacific Basin However, the amount of arable soil is very from the partially submerged continental areas limited and very prone to erosion. As suggested of andesite. Volcanism ceased 20 million years by the USDA report deposited at Forestry ago and was succeeded by submergence of Service in Palau, islands and formation of the barrier reef began. -
Origin and Character of Loesslike Silt in the Southern Qinghai-Xizang (Tibet) Plateau, China
Origin and Character of Loesslike Silt in the Southern Qinghai-Xizang (Tibet) Plateau, China U.S. GEOLOGICAL SURVEY PROFESSIONAL PAPER 1549 Cover. View south-southeast across Lhasa He (Lhasa River) flood plain from roof of Potala Pal ace, Lhasa, Xizang Autonomous Region, China. The Potala (see frontispiece), characteristic sym bol of Tibet, nses 308 m above the valley floor on a bedrock hill and provides an excellent view of Mt. Guokalariju, 5,603 m elevation, and adjacent mountains 15 km to the southeast These mountains of flysch-like Triassic clastic and volcanic rocks and some Mesozoic granite character ize the southernmost part of Northern Xizang Structural Region (Gangdese-Nyainqentanglha Tec tonic Zone), which lies just north of the Yarlung Zangbo east-west tectonic suture 50 km to the south (see figs. 2, 3). Mountains are part of the Gangdese Island Arc at south margin of Lhasa continental block. Light-tan areas on flanks of mountains adjacent to almost vegetation-free flood plain are modern and ancient climbing sand dunes that exhibit evidence of strong winds. From flood plain of Lhasa He, and from flood plain of much larger Yarlung Zangbo to the south (see figs. 2, 3, 13), large dust storms and sand storms originate today and are common in capitol city of Lhasa. Blowing silt from larger braided flood plains in Pleistocene time was source of much loesslike silt described in this report. Photograph PK 23,763 by Troy L. P6w6, June 4, 1980. ORIGIN AND CHARACTER OF LOESSLIKE SILT IN THE SOUTHERN QINGHAI-XIZANG (TIBET) PLATEAU, CHINA Frontispiece. -
The Geological Newsletter
JAN 90 THE GEOLOGICAL NEWSLETTER ·• GEOLOGICAL SOCIETY OF THE OREGON COUNTRY GEOLOGICAL SOCIETY Non-Profit Org. U.S. POSTAGE OF THE OREGON COUNTRY PAID P.O. BOX ?a 7- Portland, Oregon PORTLAND, OR 97207- -:· ·--~··, Permit No. 999 - -- '~ Dr. Frank Boersma 120 W. 33~d Street Vancouver, WA 98660 GEOLOGICAL SOCIETY OF THE OREGOt\ COllNTRY 1989-1990 ADMINISTRATION BOARD OF DIRECTORS President Directors Rosemary Kenney 221-0757 Peter E. Baer (3 years) 661-7995 4211 S\-1 Condor Charlene Holzwarth (2 years) 284-3444 Portland, OR 97201 Esther Kennedy (1 year) 287-3091 Vice President Margaret L. Steere 246-1670 Immediate Past Presidents Joline Robustelli 223-2852 6929 SW 34 Ave. ~ Portland, OR 97219 R.E. (Andy) Corcoran 244-5605 Secretary Alta B. Fosback 641-6323 THE GEOLOGICAL NEWSLETTER 8942 SW Fairview Place Tigard, OR 97223 Editor: Sandra Anderson 775-5538 Treasurer Calendar: Margaret Steere 246-1670 Braden Pillow 659-6318 Business Manager: Carol Cole 220-0078 19562 SE Cottonwood St. Assist: Cecelia Crater 235-5158 Milwaukie, OR 97267 ACTIVITIES CHAIRS Calligrapher Properties and PA System Wallace R.· McClung 637-3834 (Luncheon) Donald Botteron 245-6251 Field Trips (Evening) Walter A. Sunderland 625-6840 Charlene Holzwarth 284-3444 Publications Alta B. Fosback 641-6323 Geneva E. Reddekopp 654-9818 Geology Seminars Publicity Donald D. Barr 246-2785 Roberta L. Walter 235-3579 Historian Refreshments Phyllis G. Bonebrake 289-8597 (Friday Evening) Hospitality David and Marvel Gillespie 246-2368 254-0135 (Luncheon) Margaret Fink 289-0188 Harold and Patricia Gay Moore (Evening) Maxine Harrington 297-ll86 (Geology Seminars) Catherine Evenson 654-2636 Library: Esther Kennedy 287-3091 ' ' Betty Turner 246-3192 Telephone n Past Presidents Panel Jean L. -
A POST IMPACT VOLCANISM SCENARIO for the FORMATION of the OLIVINE-RICH UNIT in the REGION of NILI FOSSAE, MARS. L. Mandon1, C. Q
49th Lunar and Planetary Science Conference 2018 (LPI Contrib. No. 2083) 1473.pdf A POST IMPACT VOLCANISM SCENARIO FOR THE FORMATION OF THE OLIVINE - RICH UNIT IN THE REGION OF NILI FOSSAE, MARS. L. Mandon 1 , C. Quantin 1 , P. Thollot 1 , L. Lozac’h 1 , N. Mangold 2 , G. Dromart 1 , P. Beck 3 , E. Dehouck 1 , S. Breton 1 , C. Millot 1 . 1 Laboratoire de Géologie de Lyon Terre, Planètes, Environnement , Université de Lyon, France. 2 Laboratoire de Planétologie et Géodynamique , Université de Nantes, France. 3 Institut de Planétologie et d'Astrophysique de Gre- noble , Université Grenoble Alpes, France. lucia.ma ndon@univ - lyon1.fr. Introduction: The Nili Fossae region exhibits the gets using MarsSI. We used HRSC DTMs computed largest Martian exposures of olivine - rich materials, as by the Fr eie Universitaet Berlin and DLR Berlin . deduced from orbital near - infrared and thermal spec- Strikes and dips measurements were performed using troscopy [1, 2] . Several hypotheses have been pro- the ArcGIS extension LayerTools [7]. Finally, we posed to explain the origin of a widespread olivine - rich performed crater size analyses on both small (~1 km²) formati on in the region: (1) these materials might be and wide (~900 km²) olivine - rich areas. Using the crustal rocks excavated by the giant impact leading to Craterstats software [8], we compared size distribu- the formation of Isidis Planitia [2], a 1200 km wide tions to isochrons generated by the Ivanov production impact basin east of Nili Fossae. (2) They could result function to estimate a surface age [9]. from mafic effusive lava flows occurring befo re [3] or Results: At HiRISE resolution, the unit appears after [4] the giant impact. -
Lafayette - 800 Grams Nakhlite
Lafayette - 800 grams Nakhlite Figure 1. Photograph showing fine ablation features Figure 2. Photograph of bottom surface of Lafayette of fusion crust on Lafayette meteorite. Sample is meteorite. Photograph from Field Museum Natural shaped like a truncated cone. This is a view of the top History, Chicago, number 62918. of the cone. Sample is 4-5 centimeters across. Photo- graph from Field Museum Natural History, Chicago, number 62913. Introduction According to Graham et al. (1985), “a mass of about 800 grams was noticed by Farrington in 1931 in the geological collections in Purdue University in Lafayette Indiana.” It was first described by Nininger (1935) and Mason (1962). Lafayette is very similar to the Nakhla and Governador Valadares meteorites, but apparently distinct from them (Berkley et al. 1980). Lafayette is a single stone with a fusion crust showing Figure 3. Side view of Lafayette. Photograph from well-developed flow features from ablation in the Field Museum Natural History, Chicago, number Earth’s atmosphere (figures 1,2,3). The specimen is 62917. shaped like a rounded cone with a blunt bottom end. It was apparently oriented during entry into the Earth’s that the water released during stepwise heating of atmosphere. Note that the fine ablation features seen Lafayette was enriched in deuterium. The alteration on Lafayette have not been reported on any of the assemblages in Lafayette continue to be an active field Nakhla specimens. of research, because it has been shown that the alteration in Lafayette occurred on Mars. Karlsson et al. (1992) found that Lafayette contained the most extra-terrestrial water of any Martian Lafayette is 1.32 b.y. -
Chapter 2 Alaska’S Igneous Rocks
Chapter 2 Alaska’s Igneous Rocks Resources • Alaska Department of Natural Resources, 2010, Division of Geological and Geophysical Surveys, Alaska Geologic Materials Center website, accessed May 27, 2010, at http://www.dggs.dnr.state.ak.us/?link=gmc_overview&menu_link=gmc. • Alaska Resource Education: Alaska Resource Education website, accessed February 22, 2011, at http://www.akresource.org/. • Barton, K.E., Howell, D.G., and Vigil, J.F., 2003, The North America tapestry of time and terrain: U.S. Geological Survey Geologic Investigations Series I-2781, 1 sheet. (Also available at http://pubs.usgs.gov/imap/i2781/.) • Danaher, Hugh, 2006, Mineral identification project website, accessed May 27, 2010, at http://www.fremontica.com/minerals/. • Digital Library for Earth System Education, [n.d.], Find a resource—Bowens reaction series: Digital Library for Earth System Education website, accessed June 10, 2010, at http://www.dlese.org/library/query.do?q=Bowens%20reaction%20series&s=0. • Edwards, L.E., and Pojeta, J., Jr., 1997, Fossils, rocks, and time: U.S. Geological Survey website. (Available at http://pubs.usgs.gov/gip/fossils/contents.html.) • Garden Buildings Direct, 2010, Rocks and minerals: Garden Buildings Direct website, accessed June 4, 2010, at http://www.gardenbuildingsdirect.co.uk/Article/rocks-and- minerals. • Illinois State Museum, 2003, Geology online–GeoGallery: Illinois State Museum Society database, accessed May 27, 2010 at http://geologyonline.museum.state.il.us/geogallery/. • Knecht, Elizebeth, designer, Pearson, R.W., and Hermans, Majorie, eds., 1998, Alaska in maps—A thematic atlas: Alaska Geographic Society, 100 p. Lillie, R.J., 2005, Parks and plates—The geology of our National parks, monuments, and seashores: New York, W.W. -
Module 7 Igneous Rocks IGNEOUS ROCKS
Module 7 Igneous Rocks IGNEOUS ROCKS ▪ Igneous Rocks form by crystallization of molten rock material IGNEOUS ROCKS ▪ Igneous Rocks form by crystallization of molten rock material ▪ Molten rock material below Earth’s surface is called magma ▪ Molten rock material erupted above Earth’s surface is called lava ▪ The name changes because the composition of the molten material changes as it is erupted due to escape of volatile gases Rocks Cycle Consolidation Crystallization Rock Forming Minerals 1200ºC Olivine High Ca-rich Pyroxene Ca-Na-rich Amphibole Intermediate Na-Ca-rich Continuous branch Continuous Discontinuous branch Discontinuous Biotite Na-rich Plagioclase feldspar of liquid increases liquid of 2 Temperature decreases Temperature SiO Low K-feldspar Muscovite Quartz 700ºC BOWEN’S REACTION SERIES Rock Forming Minerals Olivine Ca-rich Pyroxene Ca-Na-rich Amphibole Na-Ca-rich Continuous branch Continuous Discontinuous branch Discontinuous Biotite Na-rich Plagioclase feldspar K-feldspar Muscovite Quartz BOWEN’S REACTION SERIES Rock Forming Minerals High Temperature Mineral Suite Olivine • Isolated Tetrahedra Structure • Iron, magnesium, silicon, oxygen • Bowen’s Discontinuous Series Augite • Single Chain Structure (Pyroxene) • Iron, magnesium, calcium, silicon, aluminium, oxygen • Bowen’s Discontinuos Series Calcium Feldspar • Framework Silicate Structure (Plagioclase) • Calcium, silicon, aluminium, oxygen • Bowen’s Continuous Series Rock Forming Minerals Intermediate Temperature Mineral Suite Hornblende • Double Chain Structure (Amphibole) -
Pyroclastic Flow Hazards
Pyroclastic Flow Hazards Lecture Objectives -definition and characteristics -generation of pyroclastic flows -impacts and hazards What are pyroclastic flows? Pyroclastic flows are high- density mixtures of hot, dry rock fragments and hot gases that move away from the vent that erupted them at high speeds. Generation Mechanisms: -explosive eruption of molten or solid rock fragments, or both. -non-explosive eruption of lava when parts of dome or a thick lava flow collapses down a steep slope. Most pyroclastic flows consist of two parts: a basal flow of coarse fragments that moves along the ground, and a turbulent cloud of ash that rises above the basal flow. Ash may fall from this cloud over a wide area downwind from the pyroclastic flow. Mt. St. Helens Effects of pyroclastic flows A pyroclastic flow will destroy nearly everything in its path. With rock fragments ranging in size from ash to boulders traveling across the ground at speeds typically greater than 80 km per hour, pyroclastic flows knock down, shatter, bury or carry away nearly all objects and structures in their way. The extreme temperatures of rocks and gas inside pyroclastic flows, generally between 200°C and 700°C, can cause combustible material to burn, especially petroleum products, wood, vegetation, and houses. Pyroclastic flows vary considerably in size and speed, but even relatively small flows that move <5 km from a volcano can destroy buildings, forests, and farmland. On the margins of pyroclastic flows, death and serious injury to people and animals may result from burns and inhalation of hot ash and gases. Pyroclastic flows generally follow valleys or other low-lying areas and, depending on the volume of rock debris carried by the flow, they can deposit layers of loose rock fragments to depths ranging from less than one meter to more than 200 m. -
Lab 2: Silicate Minerals
GEOLOGY 640: Geology through Global Arts and Artifacts LAB 2: SILICATE MINERALS FRAMEWORK SILICATES The framework silicates quartz and feldspar are the most common minerals in Earth’s crust. Quartz (SiO 2) is one of the few common minerals that is harder than a streak plate. It may display numerous colors (purple= amethyst ; pink= rose quartz ; brown= smoky quartz ; yellow-orange= citrine ). It may form long hexagonal crystals but lacks cleavage, and instead breaks along irregular, curving surfaces (conchoidal fracture). In many cases quartz forms masses of microscopic crystals (e.g., chert, flint, chalcedony ) that still maintain the hardness and conchoidal fracture of quartz. Banded chalcedony is called agate , whereas reddish chalcedony is called carnelian (bloodstone). Plagioclase is a group of feldspar minerals that have complete solid solution from NaAlSi 3O8 ( albite ) to CaAl 2Si 2O8 ( anorthite ). Na-rich plagioclase tends to white in hands sample, whereas Ca-rich plagioclase tends to be dark grey. Twinning is the intergrowth of two or more crystals in a symmetrical fashion by the sharing of lattice points in adjacent crystals. In plagioclase, the most common twins are planar and repeated (polysynthetic twinning), resulting in the striations that are characteristic of plagioclase in hand-sample. Twinning tends to be better developed in Ca-plagioclase minerals. Ca-rich plagioclase (labradorite and anorthite) may also display iridescent colors (mostly blue). Iridescent albite is rare and is known as the semi-precious gem moonstone . Microcline (KAlSi 3O8) is the most common alkali feldspar. It is similar to plagioclase in most of its optical properties (hard, blocky, 2 cleavages at 90°).