Experiment
Vis-IR reflectance spectra (i=0°, e=30°, az=0°) of bulk (powders or raw pieces) Martian meteorites
Sub-Experiment
Basaltic shergottites
Spectrum
Vis-NIR reflectance spectrum (i=0°, e=30°, az=0°) of powdered Los Angeles Martian meteorite under ambient conditions
Spectrum
Vis-NIR reflectance spectrum (i=0°, e=30°, az=0°) of a raw piece of NWA480 Martian meteorite under ambient conditions
Spectrum
Vis-NIR reflectance spectrum (i=0°, e=30°, az=0°) of powdered Zagami Martian meteorite under ambient conditions
Spectrum
Vis-NIR reflectance spectrum (i=0°, e=30°, az=0°) of powdered NWA12633 Martian meteorite under ambient conditions
Spectrum
Vis-NIR reflectance spectrum (i=0°, e=30°, az=0°) of powdered NWA12960 Martian meteorite under ambient conditions
Spectrum
Vis-NIR reflectance spectrum (i=0°, e=30°, az=0°) of powdered NWA12965 Martian meteorite under ambient conditions
Sub-Experiment
Ol-phyric shergottites
Spectrum
Vis-NIR reflectance spectrum (i=0°, e=30°, az=0°) of powdered EETA79001 Martian meteorite under ambient conditions
Spectrum
Vis-NIR reflectance spectrum (i=0°, e=30°, az=0°) of a raw piece of NWA1068 Martian meteorite under ambient conditions
Spectrum
Vis-NIR reflectance spectrum (i=0°, e=30°, az=0°) of a raw piece of NWA1068 Martian meteorite under ambient conditions
Spectrum
Vis-NIR reflectance spectrum (i=0°, e=30°, az=0°) of a raw piece of SAU008 Martian meteorite under ambient conditions
Spectrum
Vis-NIR reflectance spectrum (i=0°, e=30°, az=0°) of a raw piece of Tissint Martian meteorite under ambient conditions
Sub-Experiment
Poikilitic shergottites
Spectrum
Vis-NIR reflectance spectrum (i=0°, e=30°, az=0°) of powdered ALHA77005 Martian meteorite under ambient conditions
Spectrum
Vis-NIR reflectance spectrum (i=0°, e=30°, az=0°) of a raw piece of NWA1950 Martian meteorite under ambient conditions
Spectrum
Vis-NIR reflectance spectrum (i=0°, e=30°, az=0°) of a raw piece of NWA1950 Martian meteorite under ambient conditions
Spectrum
Vis-NIR reflectance spectrum (i=0°, e=30°, az=0°) of a raw piece of NWA4468 Martian meteorite under ambient conditions
Spectrum
Vis-NIR reflectance spectrum (i=0°, e=30°, az=0°) of a raw piece of NWA7397 Martian meteorite under ambient conditions
Sub-Experiment
Ol/Opx-phyric shergottites
Spectrum
Vis-NIR reflectance spectrum (i=0°, e=30°, az=0°) of a raw piece of DAG476 Martian meteorite under ambient conditions
Spectrum
Vis-NIR reflectance spectrum (i=0°, e=30°, az=0°) of a raw piece of DAG489 Martian meteorite under ambient conditions
Spectrum
Vis-NIR reflectance spectrum (i=0°, e=30°, az=0°) of a raw piece of NWA1195 Martian meteorite under ambient conditions
Sub-Experiment
Nakhlites
Spectrum
Vis-NIR reflectance spectrum (i=0°, e=30°, az=0°) of a raw piece of CeC022 Martian meteorite under ambient conditions
Spectrum
Vis-NIR reflectance spectrum (i=0°, e=30°, az=0°) of powdered Lafayette Martian meteorite under ambient conditions
Spectrum
Vis-NIR reflectance spectrum (i=0°, e=30°, az=0°) of powdered MIL03346 Martian meteorite under ambient conditions
Spectrum
Vis-NIR reflectance spectrum (i=0°, e=30°, az=0°) of a raw piece of NWA817 Martian meteorite under ambient conditions
Spectrum
Vis-NIR reflectance spectrum (i=0°, e=30°, az=0°) of powdered Nakhla Martian meteorite under ambient conditions
Sub-Experiment
other
Spectrum
Vis-NIR reflectance spectrum (i=0°, e=30°, az=0°) of a raw piece of NWA2737 Martian meteorite under ambient conditions
Spectrum
Vis-NIR reflectance spectrum (i=0°, e=30°, az=0°) of powdered ALH84001 Martian meteorite under ambient conditions
Spectrum
Vis-NIR reflectance spectrum (i=0°, e=30°, az=0°) of a raw piece of NWA8159 Martian meteorite under ambient conditions
Spectrum
Vis-NIR reflectance spectrum (i=0°, e=30°, az=0°) of a raw piece of NWA7034 Martian meteorite under ambient conditions
Layer
- Name
- Nakhla Martian meteorite
- Type of layer
- granular
- Thickness
- 2.0 $\pm$ 0.5 $mm$
- Texture
- loose granular
- Type of porosity
- particulate
- Formation mode
- deposition by hand
- Temperature
- 297.0 $\pm$ 1.0 $K$
- Pressure
- 1000.0 $None$