Understanding of secular evolution of the Earth system is based largely on the rock and
mineral archive preserved in the continental lithosphere. Based on the frequency and range …

NASA's InSight (Interior exploration using Seismic Investigations, Geodesy and Heat
Transport) mission landed in Elysium Planitia on Mars on 26 November 2018. It aims to …

Clues to a planet's geologic history are contained in its interior structure, particularly its core.
We detected reflections of seismic waves from the core-mantle boundary of Mars using …

The detection of deep reflected S waves on Mars inferred a core size of 1,830±40 km (ref.),
requiring light-element contents that are incompatible with experimental petrological …

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 …

For 2 years, the InSight lander has been recording seismic data on Mars that are vital to
constrain the structure and thermochemical state of the planet. We used observations of …

Mars's seismic activity and noise have been monitored since January 2019 by the
seismometer of the InSight (Interior Exploration using Seismic Investigations, Geodesy and …

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 …

By the end of 2018, 42 years after the landing of the two Viking seismometers on Mars,
InSight will deploy onto Mars' surface the SEIS (S eismic E xperiment for I nternal S tructure) …

We detected surface waves from two meteorite impacts on Mars. By measuring group
velocity dispersion along the impact-lander path, we obtained a direct constraint on crustal …