The internal structure of the Moon, from surface to core, preserves a record of its evolution
from accretion to present-day. The structure of the Moon is unique in the Solar System by …

Volcanism is the most important endogenic geological process of the Moon, which is closely
related to its internal structure and thermal history. Lunar volcanism is one of the most …

Abstract Chang'e-5, China's first lunar sample return mission, is targeted to land in northern
Oceanus Procellarum, within a region selected on the basis of 1) its location away from the …

The lunar mascon basins are characterized by high gravity anomalies and thin crust. Study
of the density structure beneath the mascon basins can help to understand the origin of …

Abstract China's Chang'e‐5 (CE‐5) mission recently returned samples from a young
intermediate‐Ti mare unit (Em4/P58,∼ 1.5 Ga) in Northern Oceanus Procellarum. Rima …

Mons Gruithuisen is a rare example of nonmare silicic volcanoes on the Moon. We have
conducted analyses of the topography, chemical compositions, and subsurface structures of …

The Gardner region is a well‐known shield volcanic complex on the Moon. Its magma origin
and formation mechanism are of significant interest but still enigmatic. To reveal the …

Mare Crisium is a typical Mascon on the Moon, and a detailed 3-D structure of the lunar crust
and upper mantle is essential to explore the causes of the lunar Mascon. However, research …

Mare basalts on the lunar surface are tangible expressions of the complex thermal evolution
and geological processes that have occurred within the lunar interior. These basaltic …

Marius Hills, Rümker Hills, and Gardner are three prominent volcanic complexes on the
lunar nearside characterized by well‐preserved elevated topography, highly concentrated …