Volcanoes and Igneous Activity Earth

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Transcript Volcanoes and Igneous Activity Earth

Chapter 3

Igneous Rocks

PowerPoint Presentation Stan Hatfield .

SW Illinois College

Ken Pinzke .

SW Illinois College

Charles Henderson .

University of Calgary

Tark Hamilton .

Camosun College

Copyright (c) 2005 Pearson Education Canada, Inc.

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Magma : The Parent Material of Igneous Rock Igneous rocks form as molten rock cools and solidifies General Characteristic of magma

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Parent material of igneous rocks

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Forms from partial melting inside the Earth

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Magma that reaches the surface is called lava

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Magma: The Parent Material of Igneous Rock General Characteristic of Magma

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Generally formed by partial melting in Upper Mantle (~1200° C) or Lower Crust (~850° C)

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Rocks formed from lava at the surface are classified as extrusive or volcanic rocks

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Rocks formed from magma that crystallizes at depth are termed intrusive or plutonic rocks

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Magmas are buoyant, gas laden & transport Heat

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Flow rates vary over many orders of magnitude from cm/yr to supersonic

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Magma : The Parent Material of Igneous Rock The Nature of Magma

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Consists of three components:

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A liquid portion, called melt , that is composed of mobile ions derived from the partial melting of minerals

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Solids , if any, are silicate minerals that have already crystallized from the melt:

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Phenocrysts are large, Microlites are small

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Volatiles , which are gases dissolved in the melt, including water vapour (H 2 O), carbon dioxide (CO 2 ), sulphur dioxide (SO 2 ) & minor HF, HCl, He

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Magma: The Parent Material of Igneous Rock From Magma to Crystalline Rock

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Cooling of magma results in the systematic arrangement of ions into orderly patterns, cations + anions = minerals

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The silicate minerals resulting from crystallization form in a predictable order

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Textures & inclusion relations tells order of crystallization (early small crystals get surrounded by later larger phenocrysts)

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Magma: The Parent Material of Igneous Rock From Magma to Crystalline Rock

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Texture the in igneous rocks is determined by size and arrangement of mineral crystals

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Igneous rocks are typically classified by

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Textures

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Mineral compositions & proportions

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Rocks with similar textures can have different compositions (glasses all appear similar)

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Rocks with similar compositions can have different textures (rhyolite and granite look different because of different cooling histories)

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Textures + Minerals = Igneous Rock

Texture is used to describe the overall appearance of a rock based on the size, shape, and arrangement of interlocking minerals Factors affecting crystal size :

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Cooling Rates

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Fast cooling forms glass or may tiny crystals (microlites) Slow cooling rates promote the growth of fewer larger phenocrysts

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Volatiles are Solvents

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Volatiles lower viscosity & increase diffusion leading to larger crystals

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Nucleation

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More crystal nuclei promote the growth of more, but smaller crystals which impinge on each other

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Igneous Textures

Factors affecting crystal size

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Cooling Rate for magma

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Slow cooling (°C/yr) allows crystals to chemically react with magma

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Fast rate (~few °C/hr) forms many small crystals Very fast rate (~hundreds of °C/sec) forms glass (disordered ions)

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Amount of

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Silica (SiO 2 ) present Mafic (Low silica) magmas like basalts (<50% SiO 2 ) flow easily

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Felsic (High silica) magmas are stiff and explosive

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Nucleation of crystals

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Contamination with crustal rocks promotes nucleation

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Amount of Dissolved Gases

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Affects viscosity, diffusion and explosivity

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<5% dissolved volatiles allows flows of km/day More than ~5% volatiles exsolve and form explosive foams

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Igneous Textures

Types of igneous textures

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Aphanitic (fine-grained) texture

 – – –

Rapid rate of cooling of lava or magma (in air, water) Microscopic crystals Volcanic!

May contain vesicles (holes from gas bubbles) and thus rocks that contain them have a vesicular texture

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Porphyritic = large phenocrysts & smaller groundmass

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Generally lava flows Phaneritic or sub-volcanic intrusions ( dykes/sills ) Phenocrysts grew slowly then eruption quenched the lava (coarse-grained) texture

Plutonic!

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Crystals can be identified without a microscope (>2mm) Generally caused by slow cooling (heat loss at depth) Pegmatitic (very coarse-grained) texture

Plutonic!

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Crystals (>2cm) Generally caused by very slow cooling Also caused by abundant volatiles (increases diffusion rates) Rare metals (Au, B, Be, Sn) & unusual minerals can occur

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Hand Specimen

Igneous Textures: Volcanic

Fe Staining: Weathering Andesite with twinned Plagioclase laths, birefringent Augite, Magnetite & Glass Copyright (c) 2005 Pearson Education Canada Inc.

Thin Section 3-10

Igneous Textures: Plutonic

Granite with: Pink K-Feldspar, White Plagioclase, Phaneritic Grey Quartz & Black Biotite Biotite-birefringent, Qtz-grey/white Feldspars-Twinned Black/white Copyright (c) 2005 Pearson Education Canada Inc.

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Igneous Textures: Volcanic

Types of igneous textures

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Porphyritic texture : 2 different crystal sizes

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Minerals form at different temperatures as well as crystallizing at differing rates

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Large crystals, called phenocrysts , are embedded in a matrix of smaller crystals, called the groundmass

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Sudden loss of volatiles can arrest crystallization

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Glassy texture (Vitreous & Conchoidal fracture)

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Very rapid cooling to volcanic rock in air or water

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This is common in very viscous, Hi-Silica magmas

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Resulting rock is called obsidian

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Volcanic Textures

Flattened & fused Glassy shards Indicate flow & Horizontal directions Black Magnetite as dust sized particles darkens the glass Pale green patches are altered to chlorite.

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Igneous Textures

Types of igneous textures

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Pyroclastic texture (volcanic)

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Various fragments ejected during a violent volcanic eruption (rocks, crystals, glass shards, foams)

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Textures often appear more similar to sedimentary rocks, but usually angular & partly glassy

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Pegmatitic texture (plutonic)

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Exceptionally coarse-grained Form in late stages of crystallization of magmas

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Xenolithic / Xenocrystic texture (plutonic)

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Accidental rock fragments from mantle or crust

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Included crystals from other rocks or magmas

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Igneous Textures: Plutonic

Large K-Feldspars, White Plagioclase, Grey Quartz, Brown-Green Hornblende, Black Magnetite Phaneritic Porphyritic

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Igneous Compositions Igneous rocks are composed primarily of silicate minerals

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Dark (or ferro magnesian ) silicates,

∑

= Colour Index

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Depends on Mg + Fe content of magma

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Crystallize in order of falling Temperature

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May react with magma to form a lower T°C phase

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Spinel or Magnetite (oxides not silicates) Fe 3 O 4

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Olivine (Mg,Fe)SiO 4 , lone tetrahedra

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Pyroxene Ca(Mg,Fe)Si 2 O 6 , single chains

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Amphibole Ca 2 (Mg,Fe) 5 Si 8 O 22 (OH) 2 , double chains

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Biotite mica K(Mg,Fe) 3 (Al,Si) 3 O 10 (OH,F) 2 , sheets

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Igneous Compositions

Igneous rocks are composed primarily of silicate minerals

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Light (or nonferromagnesian) silicates (with falling Temperature)

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Plagioclase Feldspar: framework silicate

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Anorthite CaAl 2

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K-Feldspar KAlSi 3 O 8 , framework silicate

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Quartz SiO 2 Si 2 O 8 to Albite NaAlSi 3 O 8 , framework silicate

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Muscovite mica K(Mg,Fe) 3 (Al,Si) 3 O 10 (OH,F) (this mineral is only found in plutonic rocks) 2 , sheets,

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Igneous Compositions Felsic versus Mafic Compositions

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Rhyolitic composition

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Common in explosive strato-volcanoes (arcs)

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Granitic composition

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Composed of light-coloured silicates

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Designated as being felsic (feldspar and silica) in composition

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Contains high amounts of silica (SiO 2 ), >68%

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Low temperature melts but high viscosity

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Major rock type in continental crust

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Common in batholiths of continental margin arcs

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Igneous Compositions Mafic versus Felsic Compositions

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Basaltic (or Gabbroic) composition

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Composed of dark silicates and calcium-rich feldspar

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Designated as being mafic (magnesium and ferrum, for iron) in composition

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High Temperature magmas but low viscosity

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More dense than granitic rocks

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Comprise the ocean crust as well as many volcanic islands

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Igneous Compositions

Other compositional groups

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Intermediate (or andesitic ) composition

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Contain at least 25 percent dark silicate minerals

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Associated with explosive volcanic activity

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Present in arc volcanoes and plutons

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Ultramafic composition

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Composition that is high in MgO and FeO > 55%

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Dense, high Temperature, Low viscosity melts

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Composed entirely of >90% ferromagnesian silicates

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Common in mantle (plutonic) but rare in crust

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More common in lower crust and in Precambrian rocks

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Igneous Compositions

Silica Content as an Indicator of Composition

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Silica content in crustal rocks exhibits a considerable range

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A lower than 45% in ultramafic rocks

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Over 75% percent in some felsic rocks

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Tends to increase during fractional crystallization

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Igneous Rock Classification

Rock Names Depend on Mineral %’s & Textures Plutonic/Volcanic

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Igneous Compositions

Silica content influences a magma’s behaviour

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Granitic magma

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High silica content > 68%

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Extremely viscous, flows slowly, explosive

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Liquid exists at temperatures as low as 700 o C

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Forms by differentiation from more Mafic magmas

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Can also form by partial melting of Lower Crust in collisional orogens

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Often high volatile contents: H 2 O, CO 2 etc.

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Igneous Compositions

Silica content influences a magma’s behaviour

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Basaltic magma

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Much lower silica content <54%

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Fluid-like behaviour

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Low volatile content < a few %, usually not explosive

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Crystallizes at higher temperatures

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Most common Magma on Earth (or Moon!)

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Partial melt of Peridotite (5% to 25%)

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Igneous Compositions

Naming Igneous Rocks – Felsic (Granitic) Rocks

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Granite

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Phaneritic

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Over 25 percent quartz, about 65 percent or more feldspar

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May exhibit a porphyritic texture

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Very abundant as it is often associated with mountain building

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The term granite covers a wide range of mineral compositions but mostly alkali feldspar & quartz

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Plutonic Igneous Compositions

Granite:

K-spar > Plagioclase CI < 15 Collisional varieties have 2 micas Copyright (c) 2005 Pearson Education Canada Inc.

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Igneous Compositions

Naming Igneous Rocks – Felsic (Granitic) Rocks

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Rhyolite

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Extrusive equivalent of granite

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Found in stratovolcanoes & calderas

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May contain glass fragments and vesicles

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Aphanitic texture

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Less common and less voluminous than granite

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Volcanic Igneous Compositions

Rhyolite

Aphanitic may be any colour Vesicles & glass are common May contain Quartz phenocrysts Copyright (c) 2005 Pearson Education Canada Inc.

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Felsic Volcanic Compositions

Naming Igneous Rocks – Felsic (Granitic) Rocks

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Obsidian

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Dark-coloured, often flow banded

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Glassy texture, conchoidal fracture

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Gas bubbles (vesicles) are common but flattened

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Pumice

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Low density & Light Coloured Vesicular Volcanic

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Glassy texture with few if any crystals

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Frothy appearance with numerous voids

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Felsic Volcanic Compositions

Obsidian

with palagonite (Fe-clays) in fractures Copyright (c) 2005 Pearson Education Canada Inc.

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Felsic Volcanic Compositions

Pumice

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Intermediate Volcanic Compositions

Naming Igneous Rocks – Intermediate (Andesitic) Rocks

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Andesite

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Volcanic origin usually in arc stratovolcanoes

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Aphanitic or aphanitic-porphyritic texture

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Often crystal rich with 25% to 40% phenocrysts

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Essential Plagioclase with Pyroxene or Hornblende

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Often resembles rhyolite when pyroclastic (tuffaceous)

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Andesite

From Black to White!

Abundant Plagioclase phenocrysts with small hornblende micro phenocrysts.

Magnetite is opaque.

Groundmass is smaller by 50X.

High phenocryst content makes these viscous & explosive.

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Intermediate Plutonic Compositions

Naming Igneous Rocks – Intermediate (Andesitic) Rocks

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Diorite

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Plutonic equivalent of andesite

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Coarse-grained

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Intrusive (like in the roots of the Andes!)

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Composed mainly of intermediate plagioclase feldspar and amphibole

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K-feldspar is minor if present, < 1/3 of total feldspar

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16 < CI < 45 is intermediate

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Intermediate Plutonic Compositions

Diorite Phaneritic Grey Rocks ½ Plagioclase & ½ Pyroxene or Hornblende

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Igneous Compositions

Naming Igneous Rocks – Mafic (Basaltic) Rocks

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Basalt

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Volcanic origin

– – –

Dark green to black in colour Aphanitic texture Composed mainly of pyroxene and calcium rich plagioclase feldspar

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Most common extrusive igneous rock

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Igneous Compositions

Basalt Copyright (c) 2005 Pearson Education Canada Inc.

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Igneous Compositions

Naming Igneous Rocks – Mafic (Basaltic) Rocks

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Gabbro

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Intrusive equivalent of basalt

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Phaneritic texture consisting of pyroxene and calcium-rich plagioclase

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Makes up a significant percentage of the oceanic crust

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Igneous Compositions

Naming Igneous Rocks – Pyroclastic Rocks

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Composed of fragments ejected during a volcanic eruption

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Varieties

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Tuff – ash-sized fragments

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Volcanic breccia – particles larger than ash

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Origin of Magma

Highly debated topic Generating magma from solid rock

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Produced from partial melting of rocks in the crust and upper mantle

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Role of Temperature

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Temperature increases within Earth’s upper crust (called the geothermal gradient ) average between 20 o C to 30 o C per kilometre

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Origin of Magma

Estimated temperatures in the crust and mantle.

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Origin of Magma

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Role of Temperature

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Rocks in the lower crust and upper mantle are near their melting points

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Any additional heat (from rocks descending into the mantle or rising heat from the mantle) may induce melting

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Origin of Magma

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Role of Pressure

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An increase in confining pressure causes an increase in a rock’s melting temperature or conversely, reducing the pressure lowers the melting temperature

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When confining pressures drop, decompression melting occurs

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Origin of Magma

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Decompression melting 3-44

Origin of Magma

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Role of volatiles

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Volatiles (primarily water) cause rocks to melt at lower temperatures

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This is particularly important where oceanic lithosphere descends into the mantle

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How Magmas Evolve

A single volcano may extrude lavas exhibiting very different compositions Bowen’s reaction series and the composition of igneous rocks

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N.L. Bowen demonstrated that as a magma cools, minerals crystallize in a systematic fashion based on their melting points

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How Magmas Evolve

Bowen’s Reaction Series shows the sequence in which minerals crystallize from a magma.

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How Magmas Evolve

Bowen’s reaction series

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During crystallization, the composition of the liquid portion of the magma continually changes

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Composition changes due to removal of elements by earlier-forming minerals

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The silica component of the melt becomes enriched as crystallization proceeds

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Minerals in the melt can chemically react and change

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How Magmas Evolve

Processes responsible for changing a magma’s composition

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Magmatic differentiation

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Separation of a melt from earlier formed crystals to form a different composition of magma

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Assimilation

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Changing a magma’s composition by the incorporation of foreign matter (surrounding rock bodies) into a magma

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Processes responsible for changing a magma’s composition

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Magma mixing

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Involves two bodies of magma intruding one another

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Two chemically distinct magmas may produce a composition quite different from either original magma

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How Magmas Evolve

Magma mixing, assimilation and magmatic differentiation.

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How Magmas Evolve

Partial Melting and Magma Formation

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Incomplete melting of rocks is known as partial melting

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Formation of a Mafic Magma (basaltic)

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Most originate from partial melting of ultramafic rock in the mantle

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Basaltic magmas form at mid-ocean ridges by decompression melting or at subduction zones

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How Magmas Evolve

Partial Melting and Magma Formation

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Formation of Basaltic Magmas

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As basaltic magmas migrate upward, confining pressure decreases which reduces the melting temperature

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Large outpourings of basaltic magma are common at Earth’s surface

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How Magmas Evolve

Partial Melting and Magma Formation

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Formation of Andesitic Magmas

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Interactions between mantle-derived basaltic magmas and more silica-rich rocks in the crust generate magma of andesitic composition

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Andesitic magma may also evolve by magmatic differentiation

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How Magmas Evolve

Partial Melting and Magma Formation

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Formation of Felsic (granitic) Magmas

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Most likely form as the end product of crystallization of andesitic magma

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Granitic magmas are higher in silica and therefore more viscous than other magmas

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Because of their viscosity, they lose their mobility before reaching the surface

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Tend to produce large plutonic structures

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End of Chapter 3

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