Earth's Separate Layers Flashcards

1
Q

What does the segregation of planets from the solar nebula explain?

A

Various features like bulk density and elemental abundances, and the differentiation of planets into distinct layers.

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2
Q

How do meteorites contribute to our understanding of planetary formation?

A

They provide samples from disrupted parent bodies, revealing Fe-rich metals, rock-metal mixtures, and volcanic rocks.

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3
Q

What challenges exist in studying Earth’s interior?

A

Limited direct sampling, with deepest drill holes penetrating only a small fraction of Earth’s radius, and reliance on indirect evidence.

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4
Q

How is Earth’s density estimated?

A

Density is calculated as Mass / Volume, with volume easily measured and mass calculated using Newton’s laws and Cavendish’s experiment.

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5
Q

What does Earth’s ellipsoidal shape indicate?

A

The equatorial bulge due to Earth’s rotation suggests mass concentration towards the center, with a lower moment of inertia indicating a dense core.

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6
Q

What do seismic waves reveal about Earth’s interior?

A

Seismic velocities show density variations, with compressional, shear, and surface waves revealing a liquid layer in the shadow zone

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7
Q

What are the main layers of Earth’s interior?

A

Crust (continental and oceanic), mantle, outer core, inner core, defined by seismic velocities and density variations.

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8
Q

What is the composition of Earth’s core?

A

The core consists of iron (Fe) and nickel (Ni) with lighter elements, with the outer core being liquid and the inner core solid due to high pressure.

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9
Q

What are lithophile, siderophile, and chalcophile elements?

A

Lithophile elements prefer silicate rocks (mantle and crust), siderophile elements favor metallic state (core), and chalcophile elements occur in sulfur-bearing minerals.

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10
Q

How are magmaphile elements distributed?

A

Magmaphile elements concentrate in silicate liquid during melting, predominantly found in Earth’s crust.

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11
Q

What evidence supports Earth’s formation from meteoritic materials?

A

Earth’s composition compared to chondritic proportions, suggesting formation from meteoritic materials, though with some uncertainties.

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12
Q

What do radiogenic isotopes suggest about core formation?

A

Core formation likely occurred rapidly within the first 30 million years due to substantial heat sources.

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13
Q

How does Earth’s crust form?

A

Through partial melting of Earth’s interior, producing magma that erupts as lava or cools to form plutons, with ocean crust being basaltic and continental crust granitic.

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14
Q

What processes contribute to the formation of continents?

A

A multistage process involving basaltic layers followed by granite formation, possibly involving recycling of basaltic material or weathering.

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15
Q

How did Earth’s atmosphere and oceans form?

A

Volatiles like H2O and CO2 released through degassing from rocks, with evidence from xenon isotopes suggesting early formation.

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