Abstract
Despite recent insight regarding the history and current state of
the Moon from satellite sensing and analyses of limited Apollo-era
seismic data, deficiencies remain in our understanding of the deep
lunar interior. We reanalyzed Apollo lunar seismograms using array-processing
methods to search for the presence of reflected and converted seismic
energy from the core. Our results suggest the presence of a solid
inner and fluid outer core, overlain by a partially molten boundary
layer. The relative sizes of the inner and outer core suggest that
the core is \~60\% liquid by volume. Based on phase diagrams of
iron alloys and the presence of partial melt, the core probably contains
less than 6 weight \% of lighter alloying components, which is consistent
with a volatile-depleted interior.
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