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Global Modeling of Nebulae With Particle Growth, Drift, and Evaporation Fronts. III. Redistribution of Refractories and Volatiles
Paul R. Estrada, Jeffrey N. Cuzzi
Formation of the first planetesimals remains an unsolved problem. Growth by sticking must initiate the process, but multiple studies have revealed a series of barriers that can slo…
Global Modeling of Nebulae With Particle Growth, Drift, and Evaporation Fronts. II. The Influence of Porosity on Solids Evolution
Paul R. Estrada, Jeffrey N. Cuzzi, Orkan M. Umurhan
Incremental particle growth in turbulent protoplanetary nebulae is limited by a combination of barriers that can slow or stall growth. Moreover, particles that grow massive enough…
Depletion of Moderately Volatile Elements by Open-System loss in the Early Solar Nebula
Debanjan Sengupta, Paul R. Estrada, Jeffrey N. Cuzzi +1
Rocky bodies of the inner solar system display a systematic depletion of the "Moderately Volatile Elements" (MVEs) that correlates with the expected condensation temperature of the…