Resolving Sub-Surface Ice Pebbles in Cometary Simulants using THz Time-Domain Spectroscopy
Planetary formation theories aim to explain how planets form from the proto-planetary disk through processes such as classical hierarchical growth or pebble accretion. Comets are considered primitive remnants of this early phase, bodies that never coalesced into planets and now reside in the Oort Cloud and Kuiper Belt....
Linus Leo Stöckli, H. Girard, Rafael Ottersberg et al.
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