EPISODE · Aug 15, 2022 · 15 MIN
Episode 496 - Dwarf Planets and Massive collisions forming Moons
from Lagrange Point · host Lagrange Point
Dwarf planets are strange objects in our solar systems, but Ceres is unusual amongst that group. Why is Ceres' surface so strange and how could it have formed without a hot core? Ceres is too small to really have a molten core or large molten surfaces. How did Ceres end up with odd plateaus and continent like features without an active core? How could radiation cause Ceres to form in such an odd way? The Moon's relative size is puzzling but how can we prove that it was caused by a colossal collision? Scott D. King, Michael T. Bland, Simone Marchi, Carol A. Raymond, Christopher T. Russell, Jennifer E. C. Scully, Hanna G. Sizemore. Ceres’ Broad‐Scale Surface Geomorphology Largely Due To Asymmetric Internal Convection. AGU Advances, 2022; 3 (3) DOI: 10.1029/2021AV000571 Patrizia Will, Henner Busemann, My E. I. Riebe, Colin Maden. Indigenous noble gases in the Moon’s interior. Science Advances, 2022; 8 (32) DOI: 10.1126/sciadv.abl4920
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Episode 496 - Dwarf Planets and Massive collisions forming Moons
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