Determining the relative cratering ages of regions of Psyche's surface

S Marchi, E Asphaug, JF Bell III, WF Bottke… - Space Science …, 2022 - Springer
The study of the cratering history of asteroid (16) Psyche is one of the investigations to be
performed by the NASA Psyche mission. A dedicated Relative Ages Working Group will …

Vesta's mineralogical composition as revealed by the visible and infrared spectrometer on Dawn

MC De Sanctis, E Ammannito… - … & Planetary Science, 2013 - Wiley Online Library
The Dawn spacecraft mission has provided extensive new and detailed data on Vesta that
confirm and strengthen the Vesta–howardite–eucrite–diogenite (HED) meteorite link and the …

Asteroid (4) Vesta II: Exploring a geologically and geochemically complex world with the Dawn Mission

TJ McCoy, AW Beck, TH Prettyman, DW Mittlefehldt - Geochemistry, 2015 - Elsevier
More than 200 years after its discovery, asteroid (4) Vesta is thought to be the parent body
for the howardite, eucrite and diogenite (HED) meteorites. The Dawn spacecraft spent∼ 14 …

Olivine in an unexpected location on Vesta's surface

E Ammannito, MC De Sanctis, E Palomba… - Nature, 2013 - nature.com
Olivine is a major component of the mantle of differentiated bodies, including Earth.
Howardite, eucrite and diogenite (HED) meteorites represent regolith, basaltic-crust, lower …

[HTML][HTML] Geochemistry and oxygen isotope composition of main-group pallasites and olivine-rich clasts in mesosiderites: Implications for the “Great Dunite Shortage” …

RC Greenwood, JA Barrat, ERD Scott, H Haack… - … et Cosmochimica Acta, 2015 - Elsevier
Evidence from iron meteorites indicates that a large number of differentiated planetesimals
formed early in Solar System history. These bodies should have had well-developed olivine …

Maskelynite in asteroidal, lunar and planetary basaltic meteorites: An indicator of shock pressure during impact ejection from their parent bodies

AE Rubin - Icarus, 2015 - Elsevier
Maskelynite is a diaplectic glass that forms from plagioclase at shock pressures of∼ 20–30
GPa, depending on the Ca concentration. The proportion of maskelynite-rich samples in a …

A deep crust–mantle boundary in the asteroid 4 Vesta

H Clenet, M Jutzi, JA Barrat, EI Asphaug, W Benz… - Nature, 2014 - nature.com
The asteroid 4 Vesta was recently found to have two large impact craters near its south pole,
exposing subsurface material. Modelling suggested that surface material in the northern …

Photometric behavior of spectral parameters in Vesta dark and bright regions as inferred by the Dawn VIR spectrometer

A Longobardo, E Palomba, F Capaccioni… - Icarus, 2014 - Elsevier
NASA's Dawn spacecraft orbited Vesta for approximately one year, collecting thousands of
hyperspectral images of its surface. The mission revealed that Vesta's surface shows the …

Asteroid photometry

JY Li, P Helfenstein, B Buratti, D Takir, BE Clark - Asteroids IV, 2015 - books.google.com
Asteroid photometry has three major applications: providing clues about asteroid surface
physical properties and compositions, facilitating photometric corrections, and helping …

Composition and mineralogy of dark material units on Vesta

E Palomba, A Longobardo, MC De Sanctis, F Zambon… - Icarus, 2014 - Elsevier
Vesta is the asteroid with the largest albedo variation among the known rocky Solar System
objects and shows a widespread occurrence of dark material (DM) and bright material (BM) …