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A solar wind-derived water reservoir on the Moon hosted by impact glass beads
The past two decades of lunar exploration have seen the detection of substantial quantities
of water on the Moon's surface. It has been proposed that a hydrated layer exists at depth in …
of water on the Moon's surface. It has been proposed that a hydrated layer exists at depth in …
Planetary caves: A solar system view of processes and products
JJ Wynne, JE Mylroie, TN Titus… - Journal of …, 2022 - Wiley Online Library
We provide the first solar system wide compendium of speleogenic processes and products.
An examination of 15 solar system bodies revealed that six cave‐forming processes occur …
An examination of 15 solar system bodies revealed that six cave‐forming processes occur …
Lucy mission to the Trojan asteroids: science goals
Abstract The Lucy Mission is a NASA Discovery-class mission to send a highly capable and
robust spacecraft to investigate seven primitive bodies near both the L 4 and L 5 Lagrange …
robust spacecraft to investigate seven primitive bodies near both the L 4 and L 5 Lagrange …
Dawn at Vesta: Testing the protoplanetary paradigm
The Dawn spacecraft targeted 4 Vesta, believed to be a remnant intact protoplanet from the
earliest epoch of solar system formation, based on analyses of howardite-eucrite-diogenite …
earliest epoch of solar system formation, based on analyses of howardite-eucrite-diogenite …
Extensive water ice within Ceres' aqueously altered regolith: Evidence from nuclear spectroscopy
The surface elemental composition of dwarf planet Ceres constrains its regolith ice content,
aqueous alteration processes, and interior evolution. Using nuclear spectroscopy data …
aqueous alteration processes, and interior evolution. Using nuclear spectroscopy data …
Digital terrain map** by the OSIRIS-REx mission
Abstract The Origins, Spectral Interpretation, Resource Identification, Security–Regolith
Explorer mission will return a sample to Earth from asteroid (101955) Bennu. Digital terrain …
Explorer mission will return a sample to Earth from asteroid (101955) Bennu. Digital terrain …
Spectroscopic characterization of mineralogy and its diversity across Vesta
The mineralogy of Vesta, based on data obtained by the Dawn spacecraft's visible and
infrared spectrometer, is consistent with howardite-eucrite-diogenite meteorites. There are …
infrared spectrometer, is consistent with howardite-eucrite-diogenite meteorites. There are …
Constraints on Ceres' internal structure and evolution from its shape and gravity measured by the Dawn spacecraft
Ceres is the largest body in the asteroid belt with a radius of approximately 470 km. In part
due to its large mass, Ceres more closely approaches hydrostatic equilibrium than major …
due to its large mass, Ceres more closely approaches hydrostatic equilibrium than major …
Cratering on Ceres: Implications for its crust and evolution
INTRODUCTION Thermochemical models have predicted that the dwarf planet Ceres has,
to some extent, formed a mantle. Moreover, due to viscous relaxation, these models indicate …
to some extent, formed a mantle. Moreover, due to viscous relaxation, these models indicate …
Dawn; the Vesta–HED connection; and the geologic context for eucrites, diogenites, and howardites
The Dawn mission has provided new evidence strengthening the identification of asteroid
Vesta as the parent body of the howardite, eucrite, and diogenite (HED) meteorites. The …
Vesta as the parent body of the howardite, eucrite, and diogenite (HED) meteorites. The …