Rationale for BepiColombo studies of Mercury's surface and composition

DA Rothery, M Massironi, G Alemanno, O Barraud… - Space science …, 2020 - Springer
BepiColombo has a larger and in many ways more capable suite of instruments relevant for
determination of the topographic, physical, chemical and mineralogical properties of …

Analysis of impact crater populations and the geochronology of planetary surfaces in the inner solar system

CI Fassett - Journal of Geophysical Research: Planets, 2016 - Wiley Online Library
Analyzing the density of impact craters on planetary surfaces is the only known technique for
learning their ages remotely. As a result, crater statistics have been widely analyzed on the …

Lunar impact basins revealed by Gravity Recovery and Interior Laboratory measurements

GA Neumann, MT Zuber, MA Wieczorek, JW Head… - Science …, 2015 - science.org
Observations from the Gravity Recovery and Interior Laboratory (GRAIL) mission indicate a
marked change in the gravitational signature of lunar impact structures at the morphological …

Evidence for geochemical terranes on Mercury: Global mapping of major elements with MESSENGER's X-Ray Spectrometer

SZ Weider, LR Nittler, RD Starr… - Earth and Planetary …, 2015 - Elsevier
We have mapped the major-element composition of Mercury's surface from orbital
MESSENGER X-Ray Spectrometer measurements. These maps constitute the first global …

Remote sensing evidence for an ancient carbon-bearing crust on Mercury

PN Peplowski, RL Klima, DJ Lawrence, CM Ernst… - Nature …, 2016 - nature.com
Mercury's global surface is markedly darker than predicted from its measured elemental
composition. The darkening agent, which has not been previously identified, is most …

Global resurfacing of Mercury 4.0–4.1 billion years ago by heavy bombardment and volcanism

S Marchi, CR Chapman, CI Fassett, JW Head… - Nature, 2013 - nature.com
The most heavily cratered terrains on Mercury have been estimated to be about 4 billion
years (Gyr) old,,,, but this was based on images of only about 45 per cent of the surface; …

Widespread effusive volcanism on Mercury likely ended by about 3.5 Ga

PK Byrne, LR Ostrach, CI Fassett… - Geophysical …, 2016 - Wiley Online Library
Crater size–frequency analyses have shown that the largest volcanic plains deposits on
Mercury were emplaced around 3.7 Ga, as determined with recent model production …

Orbital multispectral mapping of Mercury with the MESSENGER Mercury Dual Imaging System: Evidence for the origins of plains units and low-reflectance material

SL Murchie, RL Klima, BW Denevi, CM Ernst… - Icarus, 2015 - Elsevier
A principal data product from MESSENGER's primary orbital mission at Mercury is a global
multispectral map in eight visible to near-infrared colors, at an average pixel scale of 1 km …

Asymmetric distribution of lunar impact basins caused by variations in target properties

K Miljković, MA Wieczorek, GS Collins, M Laneuville… - Science, 2013 - science.org
Maps of crustal thickness derived from NASA's Gravity Recovery and Interior Laboratory
(GRAIL) mission revealed more large impact basins on the nearside hemisphere of the …

Calibration, projection, and final image products of MESSENGER's Mercury Dual Imaging System

BW Denevi, NL Chabot, SL Murchie, KJ Becker… - Space Science …, 2018 - Springer
We present an overview of the operations, calibration, geodetic control, photometric
standardization, and processing of images from the Mercury Dual Imaging System (MDIS) …