Giant Impact Scenarios: Earth-Moon System Formation

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These flashcards cover key vocabulary related to giant impact scenarios in Earth's history, specifically focusing on the Earth-Moon system formation and its implications.

Last updated 4:58 AM on 2/10/26
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14 Terms

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GIANT IMPACT SCENARIOS

Impact origin studies aiming to identify collisional events that explain the Earth-Moon system's properties.

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Angular Momentum (LEM)

Current angular momentum of the Earth-Moon system, approximately 3.5 x 10^41 g cm² s^-1.

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Roche Limit

The distance within which a given astronomical body will disintegrate due to a tidal force exceeding the body's own gravitational self-attraction.

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Ejecta

Material ejected during a collision, which can form disks around planets after impacts.

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Smoothing Particle Hydrodynamics (SPH)

A computational method used for simulating the dynamics of fluids and gaseous processes, often applied to impacts.

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Canonical Impact

A type of impact involving a roughly Mars-mass impactor colliding with Earth at low velocity, producing an iron-depleted Moon.

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Hit-and-Run Impact

Impact scenarios that involve higher velocities and less oblique angles, resulting in disks with more target material.

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Fast-Spinning Earth Impact

Impacts into a rapidly rotating Earth that result in substantial angular momentum and must create a corresponding disk.

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Half-Earth Impact

A scenario where two objects, each about half the mass of Earth, collide to produce a disk with equal silicate compositions.

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Equilibration

The process that may erasure distinctive compositional signatures of the impactor in the post-impact disk.

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Post-Impact Evolution

The complex evolution of the planet and its orbiting material following a significant impact event.

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Hf-W System

A geochemical system relevant to the early Earth, characterized by isotopic anomalies indicating mantle heterogeneity.

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Mantle Heterogeneity

Variations and differences in the composition of Earth's mantle, which may persist due to impact events.

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Multiple Impacts

Model suggesting that Earth's Moon may have formed from a sequence of medium to large collisions.