A solar wind-derived water reservoir on the Moon hosted by impact glass beads

H He, J Ji, Y Zhang, S Hu, Y Lin, H Hui, J Hao, R Li… - Nature …, 2023 - nature.com
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 …

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 …

Lucy mission to the Trojan asteroids: science goals

HF Levison, CB Olkin, KS Noll, S Marchi… - The Planetary …, 2021 - iopscience.iop.org
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 …

Dawn at Vesta: Testing the protoplanetary paradigm

CT Russell, CA Raymond, A Coradini, HY McSween… - Science, 2012 - science.org
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 …

Extensive water ice within Ceres' aqueously altered regolith: Evidence from nuclear spectroscopy

TH Prettyman, N Yamashita, MJ Toplis, HY McSween… - Science, 2017 - science.org
The surface elemental composition of dwarf planet Ceres constrains its regolith ice content,
aqueous alteration processes, and interior evolution. Using nuclear spectroscopy data …

Digital terrain map** by the OSIRIS-REx mission

OS Barnouin, MG Daly, EE Palmer, CL Johnson… - Planetary and Space …, 2020 - Elsevier
Abstract The Origins, Spectral Interpretation, Resource Identification, Security–Regolith
Explorer mission will return a sample to Earth from asteroid (101955) Bennu. Digital terrain …

Spectroscopic characterization of mineralogy and its diversity across Vesta

MC De Sanctis, E Ammannito, MT Capria, F Tosi… - Science, 2012 - science.org
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 …

Constraints on Ceres' internal structure and evolution from its shape and gravity measured by the Dawn spacecraft

AI Ermakov, RR Fu, JC Castillo‐Rogez… - Journal of …, 2017 - Wiley Online Library
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 …

Cratering on Ceres: Implications for its crust and evolution

H Hiesinger, S Marchi, N Schmedemann, P Schenk… - Science, 2016 - science.org
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 …

Dawn; the Vesta–HED connection; and the geologic context for eucrites, diogenites, and howardites

HY McSween Jr, RP Binzel… - … & Planetary Science, 2013 - Wiley Online Library
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 …