Volume XL-8
Int. Arch. Photogramm. Remote Sens. Spatial Inf. Sci., XL-8, 477-479, 2014
https://doi.org/10.5194/isprsarchives-XL-8-477-2014
© Author(s) 2014. This work is distributed under
the Creative Commons Attribution 3.0 License.
Int. Arch. Photogramm. Remote Sens. Spatial Inf. Sci., XL-8, 477-479, 2014
https://doi.org/10.5194/isprsarchives-XL-8-477-2014
© Author(s) 2014. This work is distributed under
the Creative Commons Attribution 3.0 License.

  28 Nov 2014

28 Nov 2014

Mineralogical characterization of Juventae Chasma, Mars: evidences from MRO-CRISM

M. Singh and V. J. Rajesh M. Singh and V. J. Rajesh
  • Department of Earth and Space Sciences, Indian Institute of Space Science and Technology, Trivandrum, India

Keywords: Juventae Chasma, Hydrous Sulphates, Mafic minerals, Carbonates, Light Toned Layered Deposits, CRISM

Abstract. Juventae Chasma is a long depression associated with Valles Marineris and this study discusses the spectral observation made after analysing the Mars Reconnaissance Orbiter (MRO) Compact Reconnaissance Imaging Spectrometer for Mars (CRISM) Full Resolution targeted (FRT) Images in the wavelength region of 1000–2600 nm. Observations reveal the presence of hydrous sulphates, pyroxenes (mafic minerals) and silica rich minerals, more likely opaline silica or glass. Hydrous mineral identified shows the absorption bands, which are more consistent with gypsum. Absorption bands at 2300–2350 nm, and 2500–2550 nm, which are characteristics of carbonates, have been also identified in the region. Presence of this mineral assemblage, confirmed by the observed spectral signatures ranging from volcanic to sedimentary origin, implies a relatively geologically active area, and a significant region in terms of aqueous activity.