Determining whether liquid water exists on the Martian surface is central to understanding
the hydrologic cycle and potential for extant life on Mars. Recurring slope lineae, narrow …

Hyperspectral data (Table 1) is acquired as continuous narrowbands (eg, each band with 1
to 10 nanometer or nm bandwidths) over a range of electromagnetic spectrum (eg, 400 …

The investigation of hyperspectral data from the Mars Reconnaissance Orbiter Compact
Reconnaissance Imaging Spectrometer for Mars (CRISM) and the Observatoire pour la …

The surface of Mars has preserved the record of early environments in which its basaltic
crust was altered by liquid water. These aqueous environments have survived in the form of …

We present results from geomorphic map** and visible to near‐infrared spectral analyses
of the Jezero crater paleolake basin and its associated watershed. The goal of this study is …

Precipitated minerals, including salts, are primary tracers of atmospheric conditions and
water chemistry in lake basins. Ongoing in situ exploration by the Curiosity rover of …

We have developed a refined geologic map and stratigraphy for lower Mount Sharp using
coordinated analyses of new spectral, thermophysical, and morphologic orbital data …

Carbonates are key minerals for understanding ancient Martian environments because they
are indicators of potentially habitable, neutral‐to‐alkaline water and may be an important …

We examine the stratigraphic architecture and mineralogy of the western fan deposit in the
Jezero crater paleolake on Mars to reassess whether this fan formed as a delta in a standing …

China's first Mars mission Tianwen-1 successfully touched down the surface of the southern
Utopia Planitia on 15th May 2021. In this study we investigate the geological characteristics …