45th Lunar and Planetary Science Conference (2014) 1228.pdf BRINE EVOLUTION IN QAIDAM BASIN, NORTHERN TIBETAN PLATEAU, AND THE FORMATION OF PLAYAS AS MARS ANALOGUE SITE. W. G. Kong1 M. P. Zheng1 and F. J. Kong1, 1 MLR Key Laboratory of Saline Lake Resources and Environments, Institute of Mineral Resources, CAGS, Beijing 100037, China. (
[email protected]) Introduction: Terrestrial analogue studies have part of the basin (Kunteyi depression). The Pliocene is served much critical information for understanding the first major salt forming period for Qaidam Basin, Mars [1]. Playa sediments in Qaidam Basin have a and the salt bearing sediments formed at the southwest complete set of salt minerals, i.e. carbonates, sulfates, part are dominated by sulfates, and those formed at the and chlorides,which have been identified on Mars northwest part of basin are partially sulfates dominate [e.g. 2-4]. The geographical conditions and high eleva- and partially chlorides dominate. After Pliocene, the tion of these playas induces Mars-like environmental deposition center started to move towards southeast conditions, such as low precipitation, low relative hu- until reaching the east part of the basin at Pleistocene, midity, low temperature, large seasonal and diurnal T reaching the second major salt forming stage, and the variation, high UV radiation, etc. [5,6]. Thus the salt bearing sediments formed at this stage are mainly playas in the Qaidam Basin servers a good terrestrial chlorides dominate. The distinct change in salt mineral reference for studying the depositional and secondary assemblages among deposition centers indicates the processes of martian salts. migration and geochemical differentiation of brines From 2008, a set of analogue studies have been inside the basin.