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THE STRUCTURE AND EVOLUTION OF MEDIUM SIZED ICY BODIES
Uri Malamud Acknowledgment: Dina Prialnik Department of Geophysics, Atmospheric, and Planetary Sciences
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Water in the solar system
Asteroids Main Belt (disguised comets?) Trojans 500 km Comets Kuiper Belt Objects Centaurs Icy Satellites Long-period (Oort Cloud) Short-period (Kuiper Belt) Main Belt (?) Classical Plutinos Scattered
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Can life exist elsewhere?
Habitable Zone Sentient life evolving on planets Habitable Zone
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Why Modeling? Europa Enceladus Titan
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How does a Model work? MODEL Processes Properties Energy Sources
Heat Transport Composition Thermodynamics Structure Multiphase Flow Physical Traits MODEL Energy Sources Internal External
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Modeling of Structure&Evolution
IDEAL CASE REAL CASE (Icy bodies) Prototype object Individual object (affected by internal factors) (affected by environment) Equilibrium No equilibrium (hydrostatic, thermal…) (dependence on initial conditions) Multi – parameter family Few free parameters Known input physics/chemistry Uncertain input physics/chemistry (processes, properties) Testable by observations Untestable (ambiguous) Stars ! Exception: active comets !
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Water Migration Models
Structure Differentiated structure is postulated. Modeling Heating sources. Thermal Evolution. Water Migration Models
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Porosity is real
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Heat Sources in Larger Icy objects
Insolation Crystallization Tidal Heating Serpentinization Long & short lived Radionuclides
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Melting Point Water melting (pressure and solubles).
Rock melting (pressure and water saturation).
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Physical Description
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Output
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Significance of Water Migration
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Thank You
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Self Gravity? EOS for compressed porous material.
79 km – highly porous core depleted of ice 20 km – low porosity ice-enriched layer 125 km – porous layer 50% crystalline ice and 50% dust (rock) 7 km – gradual transition from “a” to “c” ice 19 km – “a” ice and dust pristine composition EOS for compressed porous material.
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Pore & Grain Distribution
Pore Size Distribution. Dust Transport.
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