The Heat Flow and Physical Properties Package (HP3) for the InSight Mission

T Spohn, M Grott, SE Smrekar, J Knollenberg… - Space Science …, 2018 - Springer
Abstract The Heat Flow and Physical Properties Package HP 3 for the InSight mission will
attempt the first measurement of the planetary heat flow of Mars. The data will be taken at the …

The bulk composition of Mars

GJ Taylor - Geochemistry, 2013 - Elsevier
An accurate assessment of the bulk chemical composition of Mars is fundamental to
understanding planetary accretion, differentiation, mantle evolution, the nature of the …

Thickness and structure of the Martian crust from InSight seismic data

B Knapmeyer-Endrun, MP Panning, F Bissig, R Joshi… - Science, 2021 - science.org
A planet's crust bears witness to the history of planetary formation and evolution, but for
Mars, no absolute measurement of crustal thickness has been available. Here, we …

The seismicity of Mars

D Giardini, P Lognonné, WB Banerdt, WT Pike… - Nature …, 2020 - nature.com
Abstract The InSight (Interior Exploration using Seismic Investigations, Geodesy and Heat
Transport) mission landed in Elysium Planitia on Mars on 26 November 2018 and fully …

The composition of Mars

T Yoshizaki, WF McDonough - Geochimica et Cosmochimica Acta, 2020 - Elsevier
Comparing compositional models of the terrestrial planets provides insights into
physicochemical processes that produced planet-scale similarities and differences. The …

Updated global map of Martian valley networks and implications for climate and hydrologic processes

BM Hynek, M Beach, MRT Hoke - Journal of Geophysical …, 2010 - Wiley Online Library
Martian valley networks have long been viewed as some of the best evidence of prolonged
surface water on Mars. Analysis from Viking data showed that valleys were primarily …

Geophysical and cosmochemical evidence for a volatile-rich Mars

A Khan, PA Sossi, C Liebske, A Rivoldini… - Earth and Planetary …, 2022 - Elsevier
Constraints on the composition of Mars principally derive from chemical analyses of a set of
Martian meteorites that rely either on determinations of their refractory element abundances …

Origin and age of the earliest Martian crust from meteorite NWA 7533

M Humayun, A Nemchin, B Zanda, RH Hewins… - Nature, 2013 - nature.com
The ancient cratered terrain of the southern highlands of Mars is thought to hold clues to the
planet's early differentiation,, but until now no meteoritic regolith breccias have been …

Geologic constraints on early Mars climate

ES Kite - Space Science Reviews, 2019 - Springer
Early Mars climate research has well-defined goals (MEPAG 2018). Achieving these goals
requires geologists and climate modelers to coordinate. Coordination is easier if results are …

Concentration of H, Si, Cl, K, Fe, and Th in the low‐and mid‐latitude regions of Mars

WV Boynton, GJ Taylor, LG Evans… - Journal of …, 2007 - Wiley Online Library
We report maps of the concentrations of H, Si, Cl, K, Fe, and Th as determined by the
Gamma Ray Spectrometer (GRS) on board the 2001 Mars Odyssey Mission for±∼ 45° …