A previously unidentified artifact has been found in Compact Reconnaissance Imaging Spectrometer for Mars targeted I/F data. It exists in a small fraction (<0.05%) of pixels within 90% of images investigated and occurs in regions of high spectral/spatial variance. This artifact mimics real mineral absorptions in width and depth and occurs most often at 1.9 and 2.1 μm, thus interfering in the search for some mineral phases, including alunite, kieserite, serpentine, and perchlorate. A filtering step in the data processing pipeline, between radiance and I/F versions of the data, convolves narrow artifacts (“spikes”) with real atmospheric absorptions in these wavelength regions to create spurious absorption-like features. The majority of previo...
The search for life on Mars targets the detection of organic matter from extant or extinct organisms...
The identification and classification of minerals on the Martian surface can provide important infor...
Orbital remote sensing data acquired from the Mars Express OMEGA and MRO CRISM instruments, in conju...
A previously unidentified artifact has been found in Compact Reconnaissance Imaging Spectrometer for...
Despite its current arid climate, Mars’ surface preserves a wide variety of morphologies and mineral...
NASA\u27s Phoenix mission, which landed on the northern plains of Mars in 2008, returned evidence of...
The validity of recent identification of various hydrated minerals (kieserite, gypsum, hexahydrite, ...
Three Mars missions have analyzed the composition of surface samples using thermal extraction techni...
Perchlorate (ClO₄⁻) was discovered in Martian soil by the Phoenix lander, with important implication...
Sites associated with serpentinization processes, both on Earth and throughout the Solar System, are...
Perchlorate was first detected on Mars by the Wet Chemistry Laboratory (WCL) instrument on the Phoen...
The 0.4 to 1.0 micron spectrum of Mars is dominated by a steep red, relatively featureless spectral ...
Hydrated minerals on the surface of Mars record past aqueous conditions and permit assessment of whe...
The Noachian terrain west of the Isidis basin hosts a diverse collection of alteration minerals in r...
Cross crater is a 65 km impact crater, located in the Noachian highlands of the Terra Sirenum region...
The search for life on Mars targets the detection of organic matter from extant or extinct organisms...
The identification and classification of minerals on the Martian surface can provide important infor...
Orbital remote sensing data acquired from the Mars Express OMEGA and MRO CRISM instruments, in conju...
A previously unidentified artifact has been found in Compact Reconnaissance Imaging Spectrometer for...
Despite its current arid climate, Mars’ surface preserves a wide variety of morphologies and mineral...
NASA\u27s Phoenix mission, which landed on the northern plains of Mars in 2008, returned evidence of...
The validity of recent identification of various hydrated minerals (kieserite, gypsum, hexahydrite, ...
Three Mars missions have analyzed the composition of surface samples using thermal extraction techni...
Perchlorate (ClO₄⁻) was discovered in Martian soil by the Phoenix lander, with important implication...
Sites associated with serpentinization processes, both on Earth and throughout the Solar System, are...
Perchlorate was first detected on Mars by the Wet Chemistry Laboratory (WCL) instrument on the Phoen...
The 0.4 to 1.0 micron spectrum of Mars is dominated by a steep red, relatively featureless spectral ...
Hydrated minerals on the surface of Mars record past aqueous conditions and permit assessment of whe...
The Noachian terrain west of the Isidis basin hosts a diverse collection of alteration minerals in r...
Cross crater is a 65 km impact crater, located in the Noachian highlands of the Terra Sirenum region...
The search for life on Mars targets the detection of organic matter from extant or extinct organisms...
The identification and classification of minerals on the Martian surface can provide important infor...
Orbital remote sensing data acquired from the Mars Express OMEGA and MRO CRISM instruments, in conju...