s3 Flashcards

1
Q

the thermal energy that was generated during the formation and early evolution of the Earth.

A

Primordial Heat from Planetary Formation

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2
Q

The process of planet formation involves the collision and aggregation of smaller bodies (planetesimals). The kinetic energy from these collisions was converted into heat.

A

Accretion

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3
Q

As the Earth formed, gravitational forces caused it to compress. The conversion of gravitational potential energy into thermal energy generated significant heat.

A

Gravitational Compression

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4
Q

The decay of short-lived radioactive isotopes (such as aluminum-26) during the early stages of Earth’s formation contributed to the initial heat.

A

Radioactive Decay

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5
Q

also known as gravitational contraction or self-compression, is the process by which a celestial body generates heat due to the conversion of gravitational potential energy into thermal energy.

Process converting gravitational potential energy into thermal energy during celestial body formation.

A

Gravitational Compression

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6
Q

Accretion of smaller bodies into a larger body increases mass and gravitational force.

A

Formation Process

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7
Q

The potential energy of particles transforms into thermal energy through friction and collisions.

A

Conversion of Energy

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8
Q

Generated by the movement of tectonic plates.

A

Heat from Friction Due to Plate Movements

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9
Q

Significant heat produced in the planet’s interior during early formation stages.

A

Heat Generation

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10
Q

Plates of the Earth’s crust move over the semi-fluid asthenosphere.

A

Tectonic Activity

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11
Q

Plates grinding against each other at boundaries (convergent, divergent, and transform) generate frictional heat

A

Frictional Heat

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12
Q

Heat generated within the Earth’s interior is transferred to the surface through three main mechanisms: conduction, convection, and radiation.

A

Heat Transfer Mechanisms within Earth

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12
Q

One plate being forced under another generates significant friction and heat.

A

Subduction Zones

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13
Q

Direct Heat Transfer: Heat moves through solid materials like rocks.

A

Conduction

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14
Q

Fluid Movement: Heat transfer through the movement of semi-fluid rock in the mantle.

A

Convection

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15
Q

Localized Heat Sources: Areas of volcanic activity not directly associated with plate boundaries
.

A

Hotspots

16
Q
  1. Heat
  2. Pressure
  3. Volatiles
A

Conditions Required for Magma Formation

17
Q

For rocks to melt and form magma, temperatures must be high enough to overcome the bonds holding the minerals together.

A

Heat

18
Q

Residual heat from the planet’s formation.

A

Primordial Heat

19
Q

Continuous heat production from the decay of radioactive isotopes.

A

Radioactive Decay

20
Q

Generated by the movement and deformation of tectonic plates.

A

Frictional Heating

21
Q
  1. Decompression Melting
  2. Flux Melting
  3. Heat-Induced Melting
A

Processes Leading to Magma Formation

22
Q

Heat-induced melting occurs when the temperature of the mantle or crust increases due to tectonic processes such as mantle plumes or hotspots.

A

Heat-Induced Melting

22
Q

Occurs when there is a decrease in pressure as mantle rocks ascend. This process is common at divergent plate boundaries, such as mid-ocean ridges, where tectonic plates move apart. As the pressure decreases, the mantle material rises and partially melts, forming basaltic magma.

A

Decompression Melting

23
Q

Happens when volatiles like water and carbon dioxide are added to the mantle, reducing the melting temperature of the rocks.

A

Flux Melting

24
Q

these chambers act as storage areas where magma can evolve before potentially leading to volcanic eruptions.

A

Magma Chambers

25
Q

When magma cools and solidifies below the Earth’s surface, it forms intrusive igneous rocks.

A

Intrusive Pathways

26
Q

Low in silica (about 45-55%) and high in iron and magnesium, basaltic magma is the most fluid type. It commonly forms shield volcanoes and basalt plateaus

A

Basaltic Magma

26
Q

When magma reaches the surface, it erupts through volcanic vents, forming extrusive igneous rocks like basalt, andesite, and rhyolite.

A

Extrusive Pathways

27
Q

Intermediate in silica content (about 55-65%), andesitic magma is more viscous than basaltic magma. It is often associated with stratovolcanoes and volcanic arcs

A

Andesitic Magma

28
Q

Low-viscosity magma (typically basaltic) flows out of the volcano, forming lava flows. These eruptions are generally less explosive and create broad gently sloping shield volcanoes.

A

Effusive Eruptions

29
Q

High-viscosity magma (such as andesitic or rhyolitic) traps gases, leading to pressure build-up and explosive eruptions. These eruptions can produce pyroclastic flows, ash falls, and significant volcanic debris, forming steep-sided stratovolcanoes or calderas

A

Explosive Eruptions:

30
Q

Formed by low-viscosity basaltic lava that flows easily and spreads widely

A

Shield Volcanoes

31
Q

Characterized by alternating layers of lava and pyroclastic material, resulting from explosive and effusive eruptions.

A

Stratovolcanoes/composite:

32
Q

Large, basin-shaped depressions formed when a volcano collapses following a massive eruption.

A

Calderas

33
Q

As magma cools, early-forming minerals crystallize and settle out of the melt, removing specific elements and altering the composition of the remaining liquid. This process can create layered intrusions with distinct mineral bands

A

Fractional Crystallization

34
Q

Magma can incorporate surrounding rock material as it ascends, altering its composition. This process is called assimilation, and it can lead to the formation of hybrid magmas with mixed characteristics.

A

Assimilation

35
Q

When magmas from different sources or depths come into contact, they can mix, forming a new magma with intermediate properties. This process can produce complex igneous rock formations with varied textures and compositions.

A

Magma Mixing

36
Q

Caused by mechanical deformation along fault zones, leading to changes primarily due to pressure. This can create rocks like mylonite.

A

Dynamic Metamorphism