In this chapter, we present and discuss in detail current and novel advances in our
understanding of the processes that drove primordial differentiation of the Moon. This …

Lunar meteorites are fragments of consolidated rock that were ejected from the Moon when
it was struck by an impacting asteroid or comet, entered an Earth-crossing orbit, and …

Objective To assess the association between cardiorespiratory fitness (CRF) and outcomes
in a cardiac rehabilitation (CR) cohort. Patients and Methods We conducted a retrospective …

Despite more than 40 years of studying Apollo samples, the age and early evolution of the
Moon remain contentious. Following the formation of the Moon in the aftermath of a giant …

Seven lunar crater sites of granular avalanches are studied utilizing high‐resolution images
(0.42–1.3 m/pixel) from the Lunar Reconnaissance Orbiter Camera; one, in Kepler crater, is …

Magma oceans are a common result of the high degree of heating that occurs during planet
formation. It is thought that almost all of the large rocky bodies in the Solar System went …

The Moon provides a unique window into the early evolution of terrestrial planets, which is
inaccessible on other planets due to the obliteration of their early surfaces by plate tectonics …

Miller Range (MIL) 13317 is a heterogeneous basalt‐bearing lunar regolith breccia that
provides insights into the early magmatic history of the Moon. MIL 13317 is formed from a …

Lunar granulitic meteorites provide new constraints on the composition and evolution of the
lunar crust as they are potentially derived from outside the Apollo and Luna landing sites …

Fourier transform infrared (FTIR) spectroscopy and cathodoluminescence (CL) imaging
techniques, combined with electron microprobe analyses, have been used to determine the …