IGNEOUS ROCKS BEGIN WHAT IS an IGNEOUS ROCK? an Igneous Rock Is a Rock That Has Formed from the Cooling and Solidification of Magma Or Lava

Total Page:16

File Type:pdf, Size:1020Kb

IGNEOUS ROCKS BEGIN WHAT IS an IGNEOUS ROCK? an Igneous Rock Is a Rock That Has Formed from the Cooling and Solidification of Magma Or Lava IGNEOUS ROCKS BEGIN WHAT IS AN IGNEOUS ROCK? An igneous rock is a rock that has formed from the cooling and solidification of magma or lava. LAST NEXT MAGMA LAVA Melted rock Melted rock that is beneath that is at or the surface of near the surface the Earth. of the Earth. LAST NEXT Lava Magma LAST NEXT LAST NEXT LAST NEXT TYPES OF IGNEOUS ROCKS Igneous rocks are classified according to where they cooled and solidified. LAST NEXT INTRUSIVE EXTRUSIVE IGNEOUS ROCKS IGNEOUS ROCKS Rocks that form Rocks that form from magma from lava cooling and cooling and solidifying while solidifying while still inside the at or near the Earth Earth LAST NEXT Rock Cycle in Earth’s Crust Relationship of Transported r Dep Particle Size to Water Velocity d/o osi an an tion 100.0 ion n d Bu ct atio ria Boulders pa nt l m e o em 25.6 C C 10.0 Cobbles SEDIMENTS 6.4 E (cm) SEDIMENTARY n r o o i 1.0 Pebbles ROCK s s o H ( i We Up o r e a lift n th ) E a e M rin 0.2 t g & & e E a ro M s l ion g 0.1 n t i ) n e n d i t f r t Pre g r s / d/o sur i a n e l o a at e Sand m e p r H ph h amor ism t P t e U o M a ( r r e 0.01 p e h s W 0.006 i s n s ) o u ft i m li s r p ro e (U IGNEOUS & E Silt g DIAMETER PARTICLE erin ROCK 0.001 ath We g eltin 0.0004 METAMORPHIC M n o Clay ROCK ti a 0.0001 c 1 100 1000 10 i 0.01 0.05 0.1 0.5 500 f 5 50 di M oli el S ting MAGMA STREAM VELOCITY (cm/s) This generalized graph shows the water velocity needed to maintain, but not start, movement. Variations occur due to differences in particle density and shape. CRYSTAL TEXTURE Scheme for Igneous Rock Identification SIZE Non- Obsidian Basaltic glass (usually appears black) Glassy vesicular non- Pumice Scoria crystalline Vesicular (gas Vesicular rhyolite Vesicular Vesicular basalt pockets) andesite (Volcanic) Fine EXTRUSIVE EXTRUSIVE Basalt Rhyolite Andesite 1 mm less than Diabase Peri- Non- Diorite to Coarse IGNEOUS ROCKS Granite Gabbro dotite vesicular 1 mm Dunite 10 mm Very ENVIRONMENT OF FORMATION ENVIRONMENT (Plutonic) Pegmatite or INTRUSIVE INTRUSIVE coarse larger 10 mm LIGHTER COLOR DARKER LOWER DENSITY HIGHER FELSIC COMPOSITION MAFIC (rich in Si, Al) (rich in Fe, Mg) 100% 100% Potassium CHARACTERISTICS feldspar (pink to white) 75% 75% Quartz (clear to white) Plagioclase feldspar (white to gray) 50% 50% Pyroxene (green) Biotite (black) (relative by volume) 25% Olivine 25% MINERAL COMPOSITION MINERAL (green) Amphibole (black) P. 6 of ESRT 0% 0% LAST 6 Physical Setting/Earth Science Reference TablesNEXT — 2010 Edition INTRUSIVE IGNEOUS ROCKS Because these rocks form inside the Earth, where it is very hot, it takes a long time for the magma to cool and solidify. This time allows mineral crystals to grow large. So all intrusive igneous rocks have inter-grown crystals that are larger than 1mm. LAST NEXT INTRUSIVE IGNEOUS ROCKS PEGMATITE GRANITE *Notice the large mineral crystals LAST NEXT Rock Cycle in Earth’s Crust Relationship of Transported r Dep Particle Size to Water Velocity d/o osi an an tion 100.0 ion n d Bu ct atio ria Boulders pa nt l m e o em 25.6 C C 10.0 Cobbles SEDIMENTS 6.4 E (cm) SEDIMENTARY n r o o i 1.0 Pebbles ROCK s s o H ( i We Up o r e a lift n th ) E a e M rin 0.2 t g & & e E a ro M s l ion g 0.1 n t i ) n e n d i t f r t Pre g r s / d/o sur i a n e l o a at e Sand m e p r H ph h amor ism t P t e U o M a ( r r e 0.01 p e h s W 0.006 i s n s ) o u ft i m li s r p ro e (U IGNEOUS & E Silt g DIAMETER PARTICLE erin ROCK 0.001 ath We g eltin 0.0004 METAMORPHIC M n o Clay ROCK ti a 0.0001 c 1 100 1000 10 i 0.01 0.05 0.1 0.5 500 f 5 50 di M oli el S ting MAGMA STREAM VELOCITY (cm/s) This generalized graph shows the water velocity needed to maintain, but not start, movement. Variations occur due to differences in particle density and shape. CRYSTAL TEXTURE Scheme for Igneous Rock Identification SIZE Non- Obsidian Basaltic glass (usually appears black) Glassy vesicular non- Pumice Scoria crystalline Vesicular (gas Vesicular rhyolite Vesicular Vesicular basalt pockets) andesite (Volcanic) Fine EXTRUSIVE INTRUSIVE IGNEOUS ROCKS Basalt Rhyolite Andesite 1 mm less than Diabase Peri- Non- Diorite to Coarse IGNEOUS ROCKS Granite Gabbro dotite vesicular 1 mm Dunite 10 mm Very ENVIRONMENT OF FORMATION ENVIRONMENT (Plutonic) Pegmatite or INTRUSIVE coarse larger 10 mm LIGHTER COLOR DARKER LOWEREnvironment of Formation DENSITY Range of crystal sizesHIGHER (where the rock formed) FELSIC COMPOSITION MAFIC (rich in Si, Al) (richTexture in Fe, Mg) (description of crystal 100% Names of common 100% Potassium sizes) CHARACTERISTICS intrusive igneous rocks feldspar (pink to white) Non-vesicular means these rocks do 75% 75% Quartz not have any trapped air bubbles (clear to white) Plagioclase feldspar (white to gray) 50% 50% P. 6 of ESRT Pyroxene (green) Biotite LAST (black) NEXT (relative by volume) 25% Olivine 25% MINERAL COMPOSITION MINERAL (green) Amphibole (black) 0% 0% 6 Physical Setting/Earth Science Reference Tables — 2010 Edition EXTRUSIVE IGNEOUS ROCKS Because these rocks form on or near the surface of the Earth, where temperatures are lower, the lava cools and solidifies quickly. Without time, crystals cannot grow very large, or may not even form at all. So all extrusive igneous rocks have either no crystals, or crystals that are smaller than 1mm. LAST NEXT EXTRUSIVE IGNEOUS ROCKS BASALT RHYOLITE *Notice the mineral crystals are so small, you can barely see them LAST NEXT EXTRUSIVE IGNEOUS ROCKS BASALTIC GLASS OBSIDIAN *These extrusive igneous rocks formed so quickly, no crystals were able to form. They are called “glassy” or “non-crystalline.” LAST NEXT Rock Cycle in Earth’s Crust Relationship of Transported r Dep Particle Size to Water Velocity d/o osi an an tion 100.0 ion n d Bu ct atio ria Boulders pa nt l m e o em 25.6 C C 10.0 Cobbles SEDIMENTS 6.4 E (cm) SEDIMENTARY n r o o i 1.0 Pebbles ROCK s s o H ( i We Up o r e a lift n th ) E a e M rin 0.2 t g & & e E a ro M s l ion g 0.1 n t i ) n e n d i t f r t Pre g r s / d/o sur i a n e l o a at e Sand m e p r H ph h amor ism t P t e U o M a ( r r e 0.01 p e h s W 0.006 i s n s ) o u ft i m li s r p ro e (U IGNEOUS & E Silt g DIAMETER PARTICLE erin ROCK 0.001 ath We g eltin 0.0004 METAMORPHIC M n o Clay ROCK ti a 0.0001 c 1 100 1000 10 i 0.01 0.05 0.1 0.5 500 f 5 50 di M oli el S ting MAGMA STREAM VELOCITY (cm/s) This generalized graph shows the water velocity needed to maintain, but not start, movement. Variations EXTRUSIVE IGNEOUSoccur due toROCKS differences in particle density and shape. CRYSTAL TEXTURE Scheme for Igneous Rock Identification SIZE Non- Obsidian Basaltic glass (usually appears black) Glassy vesicular non- Pumice Scoria crystalline Vesicular (gas Vesicular rhyolite Vesicular Vesicular basalt pockets) andesite (Volcanic) Fine EXTRUSIVE Basalt Rhyolite Andesite 1 mm less than Diabase Peri- Non- Diorite to Coarse IGNEOUS ROCKS Granite Gabbro dotite vesicular 1 mm Dunite 10 mm Environment of Formation Very ENVIRONMENT OF FORMATION ENVIRONMENT (Plutonic) Pegmatite Range of crystal sizes or (whereINTRUSIVE the rock formed) coarse larger 10 mm Texture Names of common (description of crystal LIGHTER intrusive igneous rocks COLOR DARKERsizes) LOWER DENSITY HIGHER FELSIC COMPOSITION Some of theseMAFIC rocks have trapped gas (rich in Si, Al) bubbles,(rich in Fe, some Mg) do not 100% 100% Potassium CHARACTERISTICS P. 6 of ESRT feldspar LAST (pink to white) NEXT 75% 75% Quartz (clear to white) Plagioclase feldspar (white to gray) 50% 50% Pyroxene (green) Biotite (black) (relative by volume) 25% Olivine 25% MINERAL COMPOSITION MINERAL (green) Amphibole (black) 0% 0% 6 Physical Setting/Earth Science Reference Tables — 2010 Edition A quick review... ✓ Igneous rocks form from cooled and solidified magma or lava. ✓ When magma cools slowly inside Earth, we get intrusive (plutonic) igneous rocks with large crystals. ✓ When lava cools quickly at or near Earth’s surface, we get extrusive (volcanic) igneous rocks with small or no crystals. These may be vesicular, meaning there are trapped gas bubbles. ✓ Page 6 of the ESRT shows common igneous rocks and their characteristics. LAST NEXT Rock Cycle in Earth’s Crust Relationship of Transported r Dep Particle Size to Water Velocity d/o osi an an tion 100.0 ion n d Bu ct atio ria Boulders pa nt l m e o em 25.6 C C 10.0 Cobbles SEDIMENTS 6.4 E (cm) SEDIMENTARY n r o o i 1.0 Pebbles ROCK s s o H ( i We Up o r e a lift n th ) E a e M rin 0.2 t g & & e E a ro M s l ion g 0.1 n t i ) n e n d i t f r t Pre g r s / d/o sur i a n e l o a at e Sand m e p r H ph h amor ism t P t e U o M a ( r r e 0.01 p e h s W 0.006 i s n s ) o u ft i m li s r p ro e (U IGNEOUS & E Silt g DIAMETER PARTICLE erin ROCK 0.001 ath We g eltin 0.0004 METAMORPHIC M n o Clay ROCK ti a 0.0001 c 1 100 1000 10 i 0.01 0.05 0.1 0.5 500 f 5 50 di M oli el S ting MAGMA STREAM VELOCITY (cm/s) This generalized graph shows the water velocity needed to maintain, but not start, movement.
Recommended publications
  • Source to Surface Model of Monogenetic Volcanism: a Critical Review
    Downloaded from http://sp.lyellcollection.org/ by guest on September 28, 2021 Source to surface model of monogenetic volcanism: a critical review I. E. M. SMITH1 &K.NE´ METH2* 1School of Environment, University of Auckland, Auckland, New Zealand 2Volcanic Risk Solutions, Massey University, Palmerston North 4442, New Zealand *Correspondence: [email protected] Abstract: Small-scale volcanic systems are the most widespread type of volcanism on Earth and occur in all of the main tectonic settings. Most commonly, these systems erupt basaltic magmas within a wide compositional range from strongly silica undersaturated to saturated and oversatu- rated; less commonly, the spectrum includes more siliceous compositions. Small-scale volcanic systems are commonly monogenetic in the sense that they are represented at the Earth’s surface by fields of small volcanoes, each the product of a temporally restricted eruption of a composition- ally distinct batch of magma, and this is in contrast to polygenetic systems characterized by rela- tively large edifices built by multiple eruptions over longer periods of time involving magmas with diverse origins. Eruption styles of small-scale volcanoes range from pyroclastic to effusive, and are strongly controlled by the relative influence of the characteristics of the magmatic system and the surface environment. Gold Open Access: This article is published under the terms of the CC-BY 3.0 license. Small-scale basaltic magmatic systems characteris- hazards associated with eruptions, and this is tically occur at the Earth’s surface as fields of small particularly true where volcanic fields are in close monogenetic volcanoes. These volcanoes are the proximity to population centres.
    [Show full text]
  • 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.
    [Show full text]
  • 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)
    [Show full text]
  • Geological Mapping, Structural Setting and Petrographic Description of the Archean Volcanic Rocks of Mnanka Area, North Mara
    PROCEEDINGS, 43rd Workshop on Geothermal Reservoir Engineering Stanford University, Stanford, California, February 12-14, 2018 SGP-TR-213 Geological Mapping, Structural Setting and Petrographic Description of the Archean Volcanic Rocks of Mnanka Area, North Mara Ezra Kavana Acacia Mining PLc, North Mara Gold Mine, Department of Geology, P. O. Box 75864, Dar es Salaam, Tanzania Email: [email protected] Keywords: Musoma Mara Greenstone Belt, Mnanka volcanics, Archaean rocks and lithology ABSTRACT The Mnanka area is situated within the Musoma Mara Greenstone Belt, the area is near to Nyabigena, Gokona and Nyabirama gold mines. Mnanka area comprises of the sequence of predominant rhyolitic volcanic rocks, chert and metasediments. Gold mineralizations in Mnanka area is structure controlled and occur mainly as hydrothermal disseminated intrusion related deposits. Hence the predominant observed structures are joints and flow banding. Measurements from flow banding plotted on stereonets using win-TENSOR software has provided an estimate for the general strike of the area lying 070° to 100° dipping at an average range angle of 70° to 85° while data from joints plotted on stereonets suggest multiple deformation events one of which conforms to the East Africa Rift System (striking WSW-ENE, NNE-SSW and N-S). 1. INTRODUCTION This paper focuses on performing a systematic geological mapping and description of structures and rocks of the Mnanka area. The Mnanka area is located in the Mara region, Tarime district within the Musoma Mara Greenstone Belt. The gold at Mnanka is host ed by volcanic rocks that belong to the Musoma Mara Greenstone Belt (Figure 1). The Mnanka volcanics are found within the Kemambo group that comprises of the sequence of predominant rhyolitic volcanic rocks, chert and metasediments south of the Nyarwana fault.
    [Show full text]
  • LAYERED PEGMATITE-APLITE Division of Earth Sciences, The
    MINERALOGICAL SOCIETY OF AMERICA, SPECIAL PAPER 1, 1963 INTERNATIONALMINERALOGICALASSOCIATION,PAPERS, THIRD GENERAL MEETING LAYERED PEGMATITE-APLITE INTRUSIVES 1 RICHARD H. JAHNS AND O. FRANK TUTTLE Division of Earth Sciences, The Pennsylvania State University, University Park, Pennsylvania ABSTRACT Intrusive bodies of granitic pegmatite and aplite with simple or complex layering include those representing multiple injections of magma from external sources and those representing single injections of magma followed by segregation dur- ing crystallization. Those of the latter category can be subdivided into four classes, intergradations among which are not uncommon: 1. Bodies of aplite or fine-grained pegmatite with very large phenocrysts, or megacrysts. 2. Aplite bodies with mar- ginal or interior pegmatite masses generally formed in situ. 3. Pegmatite bodies with marginal or interior aplite masses formed in situ or by autoinjection. 4. Highly asymmetric bodies whose upper parts consist mainly or wholly of pegmatite and whose lower parts consist mainly or wholly of aplite. Zonal structure defines a gross layering within many pegmatite bodies, and a layer-like distribution of pegmatite and aplite also is common over a wide range of scales. Some of the aplites are faintly to distinctly flow layered, and others are featured by rhythmic layering in which adjacent thin and regular units differ from each other in composition. None of the observed types of layering is regarded as a result of crystal accumulation. The bulk composition of the layered intrusive bodies falls in the thermal valley of petrogeny's residua system at an average composition corresponding to a parent magma saturated with water at high pressures (e.g.
    [Show full text]
  • (FP)-Rich Aplite-Pegmatites in the Central Iberian Zone Geologic
    Ore Geology Reviews 95 (2018) 408–430 Contents lists available at ScienceDirect Ore Geology Reviews journal homepage: www.elsevier.com/locate/oregeorev Petrogenetic relationships between Variscan granitoids and Li-(F-P)-rich T aplite-pegmatites in the Central Iberian Zone: Geological and geochemical constraints and implications for other regions from the European Variscides ⁎ E. Roda-Roblesa, , C. Villasecab, A. Pesqueraa, P.P. Gil-Crespoa, R. Vieirac, A. Limac, I. Garate-Olavea a Dpto. Mineralogía y Petrología, Universidad del País Vasco UPV/EHU, Barrio Sarriena s/n, 48940 Leioa, Spain b Dpto. Petrología y Geoquímica, Universidad Complutense, IGEO (UCM, CSIC), 28040 Madrid, Spain c Instituto de Ciências da Terra, Universidade do Porto/DGAOT, Rua do Campo Alegre 687, 4169-007 Porto, Portugal ARTICLE INFO ABSTRACT Keywords: The Central Iberian Zone (CIZ) is characterised by a large volume of Variscan granitic intrusions, which can be Li-rich aplite-pegmatites grouped into five types: (1) two-mica peraluminous leucogranites (S1); (2) P-rich highly peraluminous granites Granite batholiths (S2); (3) P-poor moderately peraluminous granites (S3); (4) moderately to low peraluminous granites (S4); and Geochemistry (5) I-type low peraluminous granites (I). Though not as abundant as granites, aplite-pegmatite rocks are Central Iberian Zone nonetheless widespread in this region, occurring either as fields of aplite-pegmatite dykes or as leucogranitic European Variscan Belt cupolas. They are commonly enriched in Li-(F-P) minerals such as spodumene, petalite, micas, and phosphates of the amblygonite-montebrasite and triphylite-lithiophilite series. Many of the Li-rich bodies show an aplitic texture, frequently with the development of layered units.
    [Show full text]
  • Relationships Between Pre-Eruptive Conditions and Eruptive Styles of Phonolite-Trachyte Magmas Joan Andújar, Bruno Scaillet
    Relationships between pre-eruptive conditions and eruptive styles of phonolite-trachyte magmas Joan Andújar, Bruno Scaillet To cite this version: Joan Andújar, Bruno Scaillet. Relationships between pre-eruptive conditions and eruptive styles of phonolite-trachyte magmas. Lithos, Elsevier, 2012, 152 (1), pp.122-131. 10.1016/j.lithos.2012.05.009. insu-00705854 HAL Id: insu-00705854 https://hal-insu.archives-ouvertes.fr/insu-00705854 Submitted on 10 Jul 2012 HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. 1 Relationships between pre-eruptive conditions and eruptive styles of phonolite-trachyte magmas JOAN ANDÚJAR*,a AND BRUNO SCAILLETa a. CNRS/INSU-UNIVERSITÉ D’ORLÉANS-BRGM ; INSTITUT DES SCIENCES DE LA TERRE D’ORLEANS, UMR 6113 - 1A, RUE DE LA FÉRROLLERIE-45071 ORLEANS CEDEX 2 (FRANCE) * Corresponding author : Joan Andújar phone number : (+33) 2 38 25 53 87 Fax: (+33) 02 38 63 64 88 e-mail address: [email protected] Bruno Scaillet e-mail address: [email protected] KEY WORDS: Phase equilibria, phonolite, trachyte, experimental petrology, eruptive dynamic, explosive, effusive, andesite, rhyolite, melt viscosity, magma viscosity. 2 Abstract Phonolitic eruptions can erupt either effusively or explosively, and in some cases develop highly energetic events such as caldera-forming eruptions.
    [Show full text]
  • Part 629 – Glossary of Landform and Geologic Terms
    Title 430 – National Soil Survey Handbook Part 629 – Glossary of Landform and Geologic Terms Subpart A – General Information 629.0 Definition and Purpose This glossary provides the NCSS soil survey program, soil scientists, and natural resource specialists with landform, geologic, and related terms and their definitions to— (1) Improve soil landscape description with a standard, single source landform and geologic glossary. (2) Enhance geomorphic content and clarity of soil map unit descriptions by use of accurate, defined terms. (3) Establish consistent geomorphic term usage in soil science and the National Cooperative Soil Survey (NCSS). (4) Provide standard geomorphic definitions for databases and soil survey technical publications. (5) Train soil scientists and related professionals in soils as landscape and geomorphic entities. 629.1 Responsibilities This glossary serves as the official NCSS reference for landform, geologic, and related terms. The staff of the National Soil Survey Center, located in Lincoln, NE, is responsible for maintaining and updating this glossary. Soil Science Division staff and NCSS participants are encouraged to propose additions and changes to the glossary for use in pedon descriptions, soil map unit descriptions, and soil survey publications. The Glossary of Geology (GG, 2005) serves as a major source for many glossary terms. The American Geologic Institute (AGI) granted the USDA Natural Resources Conservation Service (formerly the Soil Conservation Service) permission (in letters dated September 11, 1985, and September 22, 1993) to use existing definitions. Sources of, and modifications to, original definitions are explained immediately below. 629.2 Definitions A. Reference Codes Sources from which definitions were taken, whole or in part, are identified by a code (e.g., GG) following each definition.
    [Show full text]
  • Rocks and Geology: General Information
    Rocks and Geology: General Information Rocks are the foundation of the earth. Rock provides the firmament beneath our oceans and seas and it covers 28% of the earth's surface that we all call home. When we travel any distance in any given direction, it is impossible not to see the tremendous variety in color, texture, and shape of the rocks around us. Rocks are composed of one or more minerals. Limestone, for example, is composed primarily of the mineral calcite. Granite can be made up of the minerals quartz, orthoclase and plagioclase feldspars, hornblende, and biotite mica. Rocks are classified by their mineral composition as well as the environment in which they were formed. There are three major classifications of rocks: igneous, sedimentary and metamorphic. A question: Which kind of rock came first? Think about it....... The following sections describe the conditions and processes that create the landscape we admire and live on here on "terra firma." IGNEOUS ROCKS The millions of tons of molten rock that poured out of the volcano Paracutin in Mexico, and from the eruption of Mount St. Helens in Washington State illustrate one of the methods of igneous rock formation. Igneous (from fire) rocks are formed when bodies of hot liquid rock called magma located beneath the earth's crust, find their way upward through the crust by way of fissures or faults. If the magma reaches the earth's surface, it forms extrusive igneous rocks or volcanic rocks. If the magma cools before it reaches the surface, it forms bodies of rock called intrusive igneous rocks or plutonic rocks.
    [Show full text]
  • A) Diorite B) Gabbro C) Andesite D) Pumice 1. the Photograph Below
    1. The photograph below shows an igneous rock with 4. The photograph below shows the intergrown crystals mineral crystals ranging in size from 2 to 6 of a pegmatite rock. millimeters. The rock is composed of 58% plagioclase feldspar, 26% amphibole, and 16% biotite. What is the name of this rock? A) diorite B) gabbro Which characteristic provides the best evidence that this pegmatite solidified deep underground? C) andesite D) pumice 2. Which igneous rock is dark colored, cooled rapidly on A) low density Earth's surface, and is composed mainly of B) light color plagioclase feldspar, olivine, and pyroxene? C) felsic composition D) very coarse texture A) obsidian B) rhyolite C) gabbro D) scoria 3. Which intrusive igneous rock could be composed of approximately 60% pyroxene, 25% plagioclase feldspar, 10% olivine, and 5% amphibole? A) granite B) rhyolite C) gabbro D) basalt 5. The graph below shows the relationship between the cooling time of magma and the size of the crystals produced. Which graph correctly shows the relative positions of the igneous rocks granite, rhyolite, and pumice? A) B) C) D) 6. The diagrams below show the crystals of four different rocks viewed through the same hand lens. Which crystals most likely formed from molten material that cooled and solidified most rapidly? A) B) C) D) 7. "Which granite sample most likely formed from magma that cooled and solidified at the slowest rate?" A) " " B) " " C) " " D) " " Base your answers to questions 8 and 9 on the diagram below and on your knowledge of Earth science. The diagram represents a portion of the scheme for igneous rock identification.
    [Show full text]
  • The Boring Volcanic Field of the Portland-Vancouver Area, Oregon and Washington: Tectonically Anomalous Forearc Volcanism in an Urban Setting
    Downloaded from fieldguides.gsapubs.org on April 29, 2010 The Geological Society of America Field Guide 15 2009 The Boring Volcanic Field of the Portland-Vancouver area, Oregon and Washington: Tectonically anomalous forearc volcanism in an urban setting Russell C. Evarts U.S. Geological Survey, 345 Middlefi eld Road, Menlo Park, California 94025, USA Richard M. Conrey GeoAnalytical Laboratory, School of Earth and Environmental Sciences, Washington State University, Pullman, Washington 99164, USA Robert J. Fleck Jonathan T. Hagstrum U.S. Geological Survey, 345 Middlefi eld Road, Menlo Park, California 94025, USA ABSTRACT More than 80 small volcanoes are scattered throughout the Portland-Vancouver metropolitan area of northwestern Oregon and southwestern Washington. These vol- canoes constitute the Boring Volcanic Field, which is centered in the Neogene Port- land Basin and merges to the east with coeval volcanic centers of the High Cascade volcanic arc. Although the character of volcanic activity is typical of many mono- genetic volcanic fi elds, its tectonic setting is not, being located in the forearc of the Cascadia subduction system well trenchward of the volcanic-arc axis. The history and petrology of this anomalous volcanic fi eld have been elucidated by a comprehensive program of geologic mapping, geochemistry, 40Ar/39Ar geochronology, and paleomag- netic studies. Volcanism began at 2.6 Ma with eruption of low-K tholeiite and related lavas in the southern part of the Portland Basin. At 1.6 Ma, following a hiatus of ~0.8 m.y., similar lavas erupted a few kilometers to the north, after which volcanism became widely dispersed, compositionally variable, and more or less continuous, with an average recurrence interval of 15,000 yr.
    [Show full text]
  • General Geology of the Franklin Mountains, El Paso County, Texas
    THE GENERAL GEOLOGY OF THE FRANKLIN MOUNTAINS, EL PASO COUNTY, TEXAS EL PASO GEOLOGICAL SOCIETY AND PERMIAN BASIN SOCIETY OF ECONOMIC PALEONTOLOGISTS AND MINERALOGISTS FEBRUARY 24, 1968 Society Members Permian Basin Section El Paso Geological Society Society of Economic Paleontologists and Mineralogists Robert Habbit, President W.F. Anderson, President David V. LeMone, Vice President Richard C. Todd, First Vice President Karl W. Klement, Second Vice President Charles Crowley, Secretary Kenneth O. Sewald, Secretary William S. Strain Gerald L. Scott, Treasurer Editor and Coordinator: David V. LeMone ii TABLE OF CONTENTS Page Introduction ............................................................................. ii Robert Habbit General Geology of the Franklin Mountains: Road Log .......................................... 1 David V. LeMone Precambrian Rocks of the Fusselman Canyon Area ............................................. 12 W.N. McAnulty, Jr. Paleoecology of a Canadian (Lower Ordovician) Algal Complex .................................. 15 David V. LeMone Late Paleozoic in the El Paso Border Region .................................................. 16 Frank E. Kottlowski Late Cenozoic Strata of the El Paso Area ..................................................... 17 William S.Strain A Preliminary Note on the Geology of the Campus “Andesite .................................... 18 Jerry M. Hoffer Conjectural Dating by Means of Gravity Slide Masses of Cenozoic Tectonics of the Southern Franklin Mountains, El Paso County, Texas ..........................................
    [Show full text]