Because of the power of remote sensing reflectance spectroscopy in determining mineralogy, it was used as the major method of identifying possible mineral analogs of the Martian surface. A summary of proposed Martian surface compositions from reflectance spectroscopy before 1979 was presented. Since that time, iron-rich montmorillonite clay, nanocrystalline or nanophase hematite, and palagonite were suggested as Mars soil analog materials
Relative reflectace point spectra (400–840 nm) were acquired by the Chemistry and Camera (ChemCam) i...
A number of questions concerning the surface mineralogy and the history of water on Mars remain unre...
A feasibility study assessing the utility of the adaptation of near infrared correlation spectroscop...
Mixtures of a Hawaiian palagonite and an iron-rich, montmorillonite clay (15.8 +/- 0.4 wt% Fe as Fe2...
The program of research outlined should advance significantly the understanding of the spectral sign...
The emissivity of a Mauna Kea palagonitic soil mixed with an Fe-substituted montmorillonite (FeM) wa...
Spectroscopic analyses have shown that Fe(3+)-doped smectites prepared in the laboratory exhibit imp...
A series of variably proportioned iron/calcium smectite clays and iron loaded smectite clays contain...
Visible and near infrared reflectance spectra of mixtures containing Hawaiian palagonitic soils, alu...
Visible and near-IR spectral data for some palagonitic soils from Mauna Kea, Hawaii, are similar to ...
Near-infrared remote sensing data of Mars have revealed thousands of ancient deposits of Fe/Mg-rich ...
During its exploration of the Columbia Hills, the Mars Exploration Rover ‘‘Spirit’...
Spectroscopic analyses have shown that smecthites enhanced in the laboratory with additionalferric s...
AbstractNear-infrared remote sensing data of Mars have revealed thousands of ancient deposits of Fe/...
The Al-clay-rich rock units at Mawrth Vallis, Mars, have been identified as mixtures of multiple com...
Relative reflectace point spectra (400–840 nm) were acquired by the Chemistry and Camera (ChemCam) i...
A number of questions concerning the surface mineralogy and the history of water on Mars remain unre...
A feasibility study assessing the utility of the adaptation of near infrared correlation spectroscop...
Mixtures of a Hawaiian palagonite and an iron-rich, montmorillonite clay (15.8 +/- 0.4 wt% Fe as Fe2...
The program of research outlined should advance significantly the understanding of the spectral sign...
The emissivity of a Mauna Kea palagonitic soil mixed with an Fe-substituted montmorillonite (FeM) wa...
Spectroscopic analyses have shown that Fe(3+)-doped smectites prepared in the laboratory exhibit imp...
A series of variably proportioned iron/calcium smectite clays and iron loaded smectite clays contain...
Visible and near infrared reflectance spectra of mixtures containing Hawaiian palagonitic soils, alu...
Visible and near-IR spectral data for some palagonitic soils from Mauna Kea, Hawaii, are similar to ...
Near-infrared remote sensing data of Mars have revealed thousands of ancient deposits of Fe/Mg-rich ...
During its exploration of the Columbia Hills, the Mars Exploration Rover ‘‘Spirit’...
Spectroscopic analyses have shown that smecthites enhanced in the laboratory with additionalferric s...
AbstractNear-infrared remote sensing data of Mars have revealed thousands of ancient deposits of Fe/...
The Al-clay-rich rock units at Mawrth Vallis, Mars, have been identified as mixtures of multiple com...
Relative reflectace point spectra (400–840 nm) were acquired by the Chemistry and Camera (ChemCam) i...
A number of questions concerning the surface mineralogy and the history of water on Mars remain unre...
A feasibility study assessing the utility of the adaptation of near infrared correlation spectroscop...