The CM chondrites are samples of primitive water-rich asteroids formed during the early
solar system. They record significant interaction between liquid water and silicate rock …

Carbonaceous asteroids, such as (101955) Bennu, preserve material from the early Solar
System, including volatile compounds and organic molecules. We report spacecraft imaging …

Thermal inertia and surface roughness are proxies for the physical characteristics of
planetary surfaces. Global maps of these two properties distinguish the boulder population …

The CM carbonaceous chondrite meteorites provide a record of low temperature (< 150° C)
aqueous reactions in the early solar system. A number of CM chondrites also experienced …

Context. Asteroid (101955) Bennu is the target of NASA's Origins, Spectral Interpretation,
Resource Identification, and Security–Regolith Explorer (OSIRIS-REx) mission. The …

On the microscale, the Winchcombe CM carbonaceous chondrite contains a number of
lithological units with a variety of degrees of aqueous alteration. However, an understanding …

Ryugu is a second-generation C-type asteroid formed by the reassembly of fragments of a
previous larger body in the main asteroid belt. While the majority of Ryugu samples returned …

Like most primitive carbonaceous chondrites, the CM chondrites experienced varying
degrees of asteroidal aqueous alteration, which may have overprinted pre-accretionary …

We report a comprehensive study of the ungrouped type 2 carbonaceous chondrite, Tarda,
which fell in Morocco in 2020. This meteorite exhibits substantial similarities to Tagish Lake …

Abstract On April 23rd, 2019, the Aguas Zarcas meteorite fall occurred in Costa Rica.
Because the meteorite was quickly recovered, it contains valuable extraterrestrial materials …