Molten rock generated by the partial melting of the mantle and crust
Magma
Contains liquids, crystals, gases, and rock fragments in varying proportions depending on temperature, pressure, and chemistry
Only contains liquid and gases at temperatures of 1200°C and above
Exsolution
When gases separate from the magma due to decompression; gas bubble develop, expand, and rise towards the surface as a separate phase
Pluton
Magma chambers of various sizes, shapes, and depths that can store magma within the Earth
Intrusive/Plutonic rocks
Form when magma cools within the surface
Commonly composed of coarse crystals (large ones) which grew large due to prolonged cooling
Lava
Magma that has erupted out the surface
Extrusive/Volcanic rocks
Form from magma that rises and erupts from within due to dissolved gases acting as a fuel blaster
Produce rocks with small crystals; did not grow large enough due to fast cooling
Igneous rock classification
Based on composition and texture
Igneous rock groups
Ultrabasic/Ultramafic
Basic/Mafic
Intermediate
Acidic/Felsic
Ultrabasic/Ultramafic rocks
Komatiite
Peridotite
Peridotite
Very dark-colored ultramafic rock depleted with silica and enriched with minerals like olivine, amphibole, and plagioclase
Rare and occur in the Earth's mantle
Basic/Mafic rocks
Basalt
Gabbro
Basalt
Very common volcanic rock (most common); encompassing the upper few kilometers of the oceanic crust
Gabbro
Crystallizes more slowly at depth at the lower portions of the ocean basin
Intermediate rocks
Andesite
Diorite
Andesite
Most common volcanic rock in the Pacific Ring of Fire
Diorite
Dioritic plutons underlies most andesitic volcanoes
Acidic/Felsic rocks
Dacite
Granodiorite
Rhyolite
Granite
Dacite
Also occurs along the Pacific Ring of Fire
Granodiorite
Underlies most andesitic-dacitic volcanoes
Rhyolite
Commonly erupts on thick continental crusts
Granite
Crystallizes also occur at thick continental crusts
Holocrystalline
Wholly crystalline
Hypocrystalline
Partially crystalline / partially glass
Holohyaline
Wholly glass
Euhedral minerals
Contain complete crystal faces that are not impinged by other crystals
Develop as early mineral phases in the crystallization of magma wherein crystals have abundant free space for growth, enhancing the likelihood to form perfectly formed crystal faces
Subhedral minerals
Contain partially complete crystal forms in which at least one of the crystal faces is impinged by adjacent rock material
Nucleation on pre-existing surfaces such as early formed crystals on the margins of the magma chamber
Resorption in which pre-existing euhedral crystals are partially remelted
Growth can be aborted due to other secondary alteration processes that destroy pre-existing euhedral faces
Anhedral minerals
Lack any observable crystal faces
The space available for the development of euhedral and subhedral crystals diminishes as crystallization progresses
Shape determined by the available space left (interstitial spaces)
Pegmatitic texture
Characterized by large crystals averaging more than 30mm in diameter
Display large, early formed euhedral crystals surrounded by later formed subhedral grains
Commonly develops on granitic plutons with high volatile components
Source of many gemstones and valuable ore deposits of metals such as Sn, Ag, and Au
Phaneritic texture
Crystal diameters between 1-30mm
Mineral crystals are visible to the naked eye
Early formed are euhedral, later formed are subhedral to anhedral
Can be subdivided into three: fine (1-3mm), medium (3-10mm), and coarse (10-30mm)
Fine-grained varieties are common o shallow intrusions like dikes and sills
Coarse-grained varieties are associated with larger and deeper intrusions
Aphanitic texture
Small crystals less than 1mm; not visible to the naked eye
Associated with volcanic rocks that cool quickly on Earth's surface
Microcrystalline if minerals can be identified under the microscope
Cryptocrystalline if minerals cannot be identified individually under the microscope
Porphyritic texture
Consists of two distinct size of crystals; large ones called phenocrysts while the finer-grained material is called the groundmass
Porphyritic-phaneritic texture = all crystals are visible but the phenocrysts are larger than groundmass crystals
Porphyritic-aphanitic texture = phenocrysts are embedded in an aphanitic groundmass composed of microcrystalline, cryptocrystalline, or glassy material
Shows a two-stage cooling process where larger phenocrysts form slowly at depth, while the finer grained groundmass crystals cool rapidly as magma approaches the surface
Crystal nucleation
Involves the formation of new crystals through nuclei, or seed crystals which are large enough to persist and grow to even larger crystals
Crystal nucleation rate is the number of new seed crystals that develop per volume per unit time (commonly expressed as nuclei/cm3/s)
Nucleation peaks at regions below the liquidus line
Nucleation needs undercooling because crystal formation requires the development of bonds between ions which produces the heat of formation
Crystal growth rate
Measure of the increase in crystal radius over time (commonly expressed as cm/s)
Governed by the rate of undercooling as well as the availability of elements and magma viscosity
Low nucleation rate = high growth rate (when magma experiences small levels of undercooling)
Prolonged undercooling results to phaneritic, porphyritic, and pegmatitic textures with euhedral-subhedral grains
Ion availability
Refers to the availability of ions that can fill specific ionic site in a crystal lattice structure
Enhanced crystal growth = appropriate ions readily available and migrate immediately
Explains why minerals that require rare trace elements tend to be very small (apatite and zirconium)
Viscosity
Resistance of a fluid to shear stress
Determined by silica content (higher silica content, more viscous), temperature (cooler, more viscous), and amount of dissolved gases (more volatiles, less viscous)
Higher viscosity = lower strain rate
Chemical diffusion rate
Diffusion is the rate at which elements migrate through magma; depends on viscosity
Low magma viscosity increases the rate of diffusion and increases crystal growth rate
High magma viscosity decreases the rate of diffusion and decreases crystal growth rate
Viscosity and chemical composition
Increased molecular linkages results in higher magma viscosity
Network formers are elements that tend to increase the molecular linkage thereby increasing viscosity (Si, Al, and O)
Network modifiers are elements that decrease molecular linkage thereby reducing viscosity
Silica-rich = more viscous; silica-poor but rich in Fe and Mg = less viscous
Viscosity, molecular bonding, and heat
Temperature inversely proportional to viscosity and molecular bonding (that's why hotter magma is more fluid and cooler magmas are more viscous)
Role of gases
Magma contain 7 weight percent volatile gases (water, carbon dioxide, and sulfur dioxide) and minor gases (N, H, S, F, Ar, CO, and Cl)
Gases reduce molecular bonding; important network modifiers
More gases = less viscous because dissolved volatiles partially bonds with the corners of the silica tetrahedra