Context. In December 2020, China’s Chang’e-5 spacecraft successfully returned 1731 g of lunar samples to Earth. Rima Sharp, one of the longest sinuous rilles on the Moon, lies very near (<20 km) to the Chang’e-5 sampling site and is very likely to be the source of the returned samples. Constraining its formation age would provide key references for the ongoing sample analyses. Aims. Our intent is to obtain the accurate formation ages of Rima Sharp and related lunar rilles through crater population studies and to assess their implications for the Chang’e-5 sample analyses and interpretations. Methods. We utilized two separate techniques to measure and analyze craters that were formed after the formation of the studied sinuous rilles: the con...
As a semi-enclosed crater basin on the northwest rim of Imbrium basin, Sinus Iridum is a key site to...
International audienceWe have measured Sm–Nd systematics, including the short-lived 146Sm–142Nd chro...
Despite more than 40 years of studying Apollo samples, the age and early evolution of the Moon remai...
The Chang’e-4 (CE-4) lunar probe, the first soft landing spacecraft on the far side of the Moon, suc...
The Moon acts as a time capsule for events in our region of the Solar System. The combination of ret...
Cratering chronologies are used to derive the history of planetary bodies and assume an isotropic fl...
Impact cratering on the Moon and the derived size-frequency distribution functions of lunar impact c...
A sharp rise in the flux of asteroid-size bodies traversing the inner Solar System at 3.9 Ga has bec...
Radiometric dating and compositional clustering of lunar impact-melt rocks form the backbone of the ...
The determination of the timing of impact events and the ages of cratered planetary surfaces is a co...
A sharp rise in the flux of asteroid-size bodies traversing the inner Solar System at 3.9 Ga has bec...
Establishing the age of the Moon is critical to understanding solar system evolution and the formati...
Previous studies have estimated the ages of lunar lobate scarps, some of the youngest tectonic landf...
abstract: Lunar Reconnaissance Orbiter (LRO) and MErcury Surface, Space ENvironment, GEochemistry, a...
Miller Range (MIL) 13317 is a heterogeneous basalt‐bearing lunar regolith breccia that provides insi...
As a semi-enclosed crater basin on the northwest rim of Imbrium basin, Sinus Iridum is a key site to...
International audienceWe have measured Sm–Nd systematics, including the short-lived 146Sm–142Nd chro...
Despite more than 40 years of studying Apollo samples, the age and early evolution of the Moon remai...
The Chang’e-4 (CE-4) lunar probe, the first soft landing spacecraft on the far side of the Moon, suc...
The Moon acts as a time capsule for events in our region of the Solar System. The combination of ret...
Cratering chronologies are used to derive the history of planetary bodies and assume an isotropic fl...
Impact cratering on the Moon and the derived size-frequency distribution functions of lunar impact c...
A sharp rise in the flux of asteroid-size bodies traversing the inner Solar System at 3.9 Ga has bec...
Radiometric dating and compositional clustering of lunar impact-melt rocks form the backbone of the ...
The determination of the timing of impact events and the ages of cratered planetary surfaces is a co...
A sharp rise in the flux of asteroid-size bodies traversing the inner Solar System at 3.9 Ga has bec...
Establishing the age of the Moon is critical to understanding solar system evolution and the formati...
Previous studies have estimated the ages of lunar lobate scarps, some of the youngest tectonic landf...
abstract: Lunar Reconnaissance Orbiter (LRO) and MErcury Surface, Space ENvironment, GEochemistry, a...
Miller Range (MIL) 13317 is a heterogeneous basalt‐bearing lunar regolith breccia that provides insi...
As a semi-enclosed crater basin on the northwest rim of Imbrium basin, Sinus Iridum is a key site to...
International audienceWe have measured Sm–Nd systematics, including the short-lived 146Sm–142Nd chro...
Despite more than 40 years of studying Apollo samples, the age and early evolution of the Moon remai...