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 …

The tectonic character of Mercury

PK Byrne, C Klimczak… - Mercury: The view after …, 2018 - books.google.com
From its three flybys in 1974–1975, Mariner 10 told us that Mercury is a tectonic world. That
is, the planet has experienced a long and complicated history of tectonic deformation …

Evaluating an impact origin for Mercury's high‐magnesium region

EA Frank, RWK Potter, O Abramov… - Journal of …, 2017 - Wiley Online Library
During its four years in orbit around Mercury, the MErcury Surface, Space ENvironment,
GEochemistry, and Ranging (MESSENGER) spacecraft's X‐ray Spectrometer revealed a …

[KNIHA][B] Geological Processes on Mercury and the Map** of the Derain (H-10) Quadrangle

CC Malliband - 2020 - search.proquest.com
Open Research Online oro.open.ac.uk Page 1 Open Research Online The Open University’s
repository of research publications and other research outputs Geological Processes on …

PAUL K. BYRNE, JENNIFER L. WHITTEN, CHRISTIAN KLIMCZAK, FRANCIS M. MCCUBBIN

LR OSTRACH - Mercury: The View after MESSENGER, 2018 - books.google.com
From its three flybys in 1974–1975, Mariner 10 raised the tantalizing prospect that Mercury is
a volcanic world. That is, the planet has experienced a geological history that included …