Mantle-Derived Magmas II Skaergaard Intrusion, Greenland.

Slides:



Advertisements
Similar presentations
Radiogenic isotopic evolution of the mantle and crust Matt Jackson and Bill McDonot.
Advertisements

Ocean Floor Basalts (MORB) Igneous Petrology 423, Francis 2013 The eruption of MORB basalts is the dominant form of active volcanism on the Earth today:
Igneous Rocks and Classifying Igneous Rocks
CH. 5 – Igneous Rocks   What are igneous rocks?   Formed by the hardening of magma.   “Ignis” means fire   What is the difference between magma.
Silicate Earth Primitive mantle Present-day mantle Crust Oceanic crust Continental crust Reservoir Volume Mass Mass % (10 27 cm 3 )(10 27 g) Earth
Creation of Magma Unlike snow, rock doesn’t all melt at once, because rocks are made up of several minerals, each with its own melting point. This reflects.
The Earth II: The Core; Mantle Reservoirs Lecture 46.
Compositional Model for the Mantle beneath the Pacific Plate Rhea Workman Outline: 1. Concepts of trace element and isotope geochemistry for the Earth’s.
Tim Horner, CSUS Geology Department Igneous Rocks, Intrusive Activity, and the Origin of Igneous Rocks Physical Geology 13/e, Chapter 3.
Trace Element in Behavior in Crystallization Lecture 28.
Igneous Rocks Igneous Rocks “Ignis” means fire
Rb-Sr and Sm-Nd Dating 8/30/12
Igneous Rocks. Summary 1. The Rock Cycle 2. Formation of Igneous Rocks 3. Classification of Igneous Rocks.
III. Igneous Rocks Minerals Crystallized from Melts 1. The Rock Cycle 2. Formation of Igneous Rocks 3. Classification of Igneous Rocks 4. Igneous Rocks.
Outline 1.Properties of silicate liquids 2.Adiabatic decompression melting Melting temperature(s) of lherzolite Model for mid-ocean ridges 3.Melting in.
Chapter 13: Mid-Ocean Rifts The Mid-Ocean Ridge System Figure After Minster et al. (1974) Geophys. J. Roy. Astr. Soc., 36,
Igneous Rocks Basic Principles. Igneous Rocks Igneous means “fire formed” Igneous rocks originate at high temperatures Temperatures are hot enough to.
Chapter 5-Igneous Rocks
Chemistry of the mantle. Physical processes (subduction, convection) affect the chemistry of the mantle. Chemical processes occur mainly through melting.
Igneous Rocks
Earth Science Notes Igneous Rocks. Objectives I can… Define and describe Igneous Rocks Explain how different Igneous Rocks are formed – Explain the process.
EARTH MATERIALS V The Rock Cycle: Igneous Rocks Professor Peter Doyle
Chapter 5.1 – Igneous Rocks Magma – molten rock below Earth’s surface Lava – magma that flows out onto the surface Igneous rocks – rocks that form when.
Bowen’s Reaction Series
IGNEOUS ROCKS rock = mixture of minerals, mineraloids, glass, or organic matter bound together in some way 1. magma is parent material for all rocks 2.
Classification of Igneous Rocks
Guided Notes for Igneous Rocks
Igneous Rocks Textures. The Rock Cycle A rock is a naturally formed, consolidated material usually composed of grains of one or more minerals The rock.
Classroom presentations to accompany Understanding Earth, 3rd edition prepared by Peter Copeland and William Dupré University of Houston Chapter 4 Igneous.
The Rock Cycle: Igneous Rocks
IGNEOUS ROCKS.
Chapter 4 ~ Intrusives ~.
Chapter 5: Igneous rocks
Volcanic Suites Francis 2014 Agua Pacaya Acatenango.
(Earth Science Teachers’ Association)
Lecture Outlines Physical Geology, 12/e Plummer & Carlson Copyright © The McGraw-Hill Companies, Inc. Permission required for reproduction or display.
Igneous Rocks Magma is the molten rock material below the surface. Lower density causes magma to rise toward the surface (compared to the surrounding.
Igneous rocks are further classified according to; Describes the appearance of an igneous rock, based on the size, shape and arrangement of interlocking.
Ultramafic Rock Bodies
Igneous Rocks and Their Origin Chapter 5. Igneous rocks - Formed from volcanic eruptions - either external or internal Sedimentary rocks - Formed from.
Radioactive Isotope Geochemistry. FIGURE 01: Simple Bohr-type model of a lithium atom.
Layered Igneous Intrusions
Isotopes. Update: Midterm graded Today: What are isotopes Radioactive decay Age dating Isotopes as fingerprint Today’s lecture.
Mantle-Derived Magmas: The Ocean Basins Pahoehoe flowing into ocean, Hawaii.
1 Petrology Lecture 6 Generation of Basaltic Magma GLY Spring, 2012.
Igneous Rocks and Their Origin Chapter 3. The Rock Cycle A rock is composed of grains of one or more minerals The rock cycle shows how one type of rocky.
Igneous Rocks Text ref. Ch5 (pg. 98).
Magmas Best, Ch. 8. Constitution of Magmas Hot molten rock T = degrees C Composed of ions or complexes Phase –Homogeneous – Separable part.
Importance of tighter constraints on U and Th abundances of the whole Earth by Geo-neutrino determinations Shun’ichi Nakai ERI, The University of Tokyo.
Trace Elements Ni Zr ppm wt. % SiO
Igneous Rocks. Igneous: “Ignis” Latin for Fire Magma – molten rock inside the earth Intrusive rocks Cool slowly below ground Generally course- grained.
Igneous Rocks Intrusive and extrusive rocks formed from the cooling and crystallization of magma.
Objectives Compare and contrast intrusive and extrusive igneous rocks. What are igneous rocks? Describe the composition of magma. Discuss the factors.
Crater Lake Jena Hershkowitz and Ethan Farina-Henry.
G EOL 2312 I GNEOUS AND M ETAMORPHIC P ETROLOGY Lecture 9a Diversification of Magmas February 17, 2016.
CHAPTER 5 – IGNEOUS ROCKS. WHAT ARE IGNEOUS ROCKS? Igneous Rock Formation  Igneous rocks form when lava or magma cools and minerals crystallize.  Most.
Rocks and Rock Cycle Intro. Rocks are not what they seem. They are constantly changing. The Rock Cycle or happen very quickly. Changes can take millions.
Jeff Taylor Ages of Highland Rocks1 Ages of Pristine Highlands Rocks Ages of lunar rocks informative about: –Timing of magma ocean crystallization –Timescales.
Ocean basins: OIBs and MORBs
Rocks and Rock Cycle Intro. The Rock Cycle Illustrates relationships between 3 rock types & their methods of formation Illustrates relationships between.
The formation of MORB vs Ophiolites Anneen Burger Anhydrous Melting of Peridotite at 0-15 Kb Pressure and the Genesis of Tholeiitic Basalts A.L. Jaques.
Igneous Rocks December 7-8,   Melted rock that cools & crystallizes at or below the surface Igneous Rocks.
The Mantle Lherzolite xenolith.
Lecture 5: Partial melting of the mantle
Using rock compositions to understand their origin and evolution
Geol 2312 Igneous and Metamorphic Petrology
Chapter 5 Igneous Rocks Section 5.1.
5.1 Lecture Igneous Rocks.
Trace elements.
Igneous Rocks Chapter 5.
Presentation transcript:

Mantle-Derived Magmas II Skaergaard Intrusion, Greenland

Enrichment of OIB and E-MORB Mantle

Depleted N-MORBS 20-40% 1% 10% 5% Incompatible elements are more enriched in a magma generated by smaller amounts of partial melting

Incompatibles versus Compatibles O% melting Rock: red/blue = 1 15% melting Rock: red/blue = 0.6 Melt: red/blue = 7 50% melting Rock: red/blue = 0.31 Melt: red/blue = 1.6

Enrichment of OIB and E-MORB Mantle Partial melting alone cannot explain the enrichment of E-MORB and N-MORB. Need metasomatism of source.

Isotopes Isotope systems are used to investigate the contribution of different geochemical reservoirs Two nuclides of the same heavy element have the same charge, size and electronic structure and behave in the same way during melting and crystallisation. They cannot be separated (i.e. fractionated). Daughter nuclides produced by decay are usually different elements and are fractionated by igneous processes.

Rb-Sr Isotopes 87 Rb decays to 87 Sr in 4.88x10 10 yrs. 86 Sr is a stable isotope and its abundance doesn’t change. 87 Rb 86 Sr 87 Sr Time 87 Sr 86 Sr= Sr 86 Sr= 2.5

Rb-Sr Isotopes: Change with Time The abundance of 87 Sr increases with time. The abundance of 86 Sr stays the same. Therefore, the 87 Sr/ 86 Sr ratio increases with time. Larger initial Rb/Sr = larger slope

Changes with Melting 87 Rb 86 Sr 87 Sr Melting increases Rb but doesn’t change Sr Crystallisation + time Rb is more incompatible than Sr

Changes with Melting

Rb-Sr of MORB

Rb-Sr of OIB Need to add significant amounts of Rb to generate OIB

Rb-Sr Isochrons Depleted rocks Enriched rocks

Nd-Sm Isotopes 147 Sm decays to 143 Nd with a half life of 1.06x10 11 yr 144 Nd is the stable isotope Nd is more incompatible than Sm (this is the opposite of Rb-Sr). 143 Nd/ 144 Nd are higher in depleted sources and lower in enriched sources.

Nd-Sm and Rb-Sr Values measured today!

Nd-Sm and Rb-Sr Enriched melts

Mantle Plumes

Diversification of Basaltic Magmas How Do We Make All Those Different Rocks? AFM diagram

Liquid Line of Descent Compositions of Lavas Crystal Fractionation (removal of crystals from a magma).

Layered Intrusions - Fossil Magma Chambers Lopolith (funnel shaped intrusions). (Some layered intrusions are sills) Skaergaard Intrusion, Greenland (500 km 3 )

Layered Series Rhythmic layering mafics plag

Layered Series Cross-bedding

Layered Series Imbrication of Gneiss Xenoliths (flow direction towards centre).

Layered Series Chilled Margins around Gneiss Xenoliths.

Cryptic Layering Cryptic layering is the change in compositions of the cumulate Minerals through the intrusion

Cryptic Layering Mg-rich olivine and pyroxene Ca-rich plag

Cryptic Layering More Fe-rich px and ol More Na-rich plag

Cryptic Layering Very iron-rich ol and px (ferrodiorite) Na-rich plag

Dunite & Peridotite as Cumulates Dunite overlain by Gabbro In some intrusions olivine crystallises first and settles to produce a dunite cumulate.

Cryptic Layering

LZ and MZ increase in Fe, Na, Si

Cryptic Layering UZ Fe-oxides crystallise rapid increases in Si, Na

Acid Granophyres (Pegmatites)

Cryptic Layering Tholeiitic fractionation trend

Phase Layering No olivine! Olivine disappears in the middle zone!

Phase Layering No olivine! Olivine disappears in the middle zone! Olivine reacts with the liquid to generate low-Ca px!

Rhythmic Layering

Densest crystals sink faster!

Rhythmic Layering But plag floats!

Rhythmic Layering Rafts of plag + mafics will sink

Rhythmic Layering Nuclei form More nuclei form Due to supercooling Sudden pulse of crystallisation Nuclei depleted Crystal melt slush sinks

Rhythmic Layering Turbidity currents of melt+crystals in magma chamber Normal grading + cross-bedding

Cumulates

Cumulates: Lamination

Cumulates: Filtration Intercumulus liquid can be squeezed out. On a larger scale, liquid squeezed from the lunar mantle may explain KREEP basic magmas erupted in the lunar highlands.