@article{ffe1c8be8a8743589383b62bb11473a6,
title = "The Tsenkher structure in the Gobi-Altai, Mongolia: Geomorphological hints of an impact origin",
abstract = "The Tsenkher structure, in the Gobi-Altai region of Mongolia, was studied using a wide array of remote sensing data and field observations. The structure has a shallow, 3.6 km wide, central depression bordered by a near-circular ridge (putative crater rim) with breaches to the northwest. The central depression is obliterated partially by fluvial infill through these breaches. Outside the ridge, the western side is a rugged terrain, but the eastern half is characterized by a concentric outer ridge that occurs at about one radius distance from the inner ridge. Although intrusion, salt tectonics and maar crater hypotheses cannot be completely ruled out, its morphology strongly implies an impact origin for the Tsenkher structure. If of impact origin, it has a well-preserved morphology and its position in the basin fills indicates that the formation may have occurred relatively recently, sometime during the late Tertiary or Quaternary. The outer ridge morphology is similar to rampart craters on Mars, whose formation has been attributed to fluidization of a water-rich target layer and ejecta materials, or to atmospheric entrainment and deposition of ejected materials. However, other hypotheses including erosional remnant of ejecta blanket, erosional scarp of structural rim uplift, multi-ring or deeply eroded crater rim of a peak-ring crater are also possible at this stage. A complex fluvial and probable lacustrine history is envisaged within the Tsenkher structure. The structure is also associated with archaeology, including Paleolithic and Bronze Age remains.",
keywords = "Ejecta, Fluidization, Impact craters, Mongolia",
author = "Goro Komatsu and Olsen, \{John W.\} and Jens Orm{\"o} and \{Di Achille\}, Gaetano and Kring, \{David A.\} and Takafumi Matsui",
note = "Funding Information: We appreciate helpful reviews by N.G. Barlow and V.R. Baker. T. Oguchi, editor of Geomorphology, provided suggestions that improved our manuscript. We thank Academician A.P. Derevianko, Director of the Institute of Archaeology and Ethnography, Russian Academy of Science, Siberian Branch and Professor D. Tseveendorj, Director of the Mongolian Academy of Sciences' Institute of Archaeology for granting permission for the use of vehicles and other logistical support provided by the Russian and Mongolian teams. D. Dorjnamjaa of the Center of Palaeontology, Mongolian Academy of Sciences and J. Namjiliin of the Institute of Geology and Mineral resources, Mongolian Academy of Sciences, kindly assisted us in obtaining precious topographic and geologic maps and permits for samples. Y. Shiokawa of the Earth Remote Sensing Data Analysis Center, Tokyo, Japan provided JERS-1 SAR and optical images. The ASTER images were provided by the ASTER project through A.P. Rossi of the International Research School of Planetary Sciences. The Radarsat data were acquired by the Radarsat project through V.R. Baker of the University of Arizona. The field expedition was financed by grants to J. Olsen and A.P. Derevianko from the National Geographic Society, L.S.B. Leakey Foundation, University of Arizona, and other private donors. The work by J. Orm{\"o} was partially supported by the Spanish Ministry for Science and Technology (References AYA2003-01203 and CGL2004-03215/BTE) and the Spanish Ram{\'o}n y Cajal Program. This project was partially supported by funding from the Italian Space Agency. Funding Information: Our research was conducted using satellite remote sensing data, field observation and sample analysis. The remote sensing data used include ASTER (Advanced Spaceborne Thermal Emission and Reflection Radiometer), Canadian Radarsat, Landsat and JERS-1 (Japanese Earth Resources Satellite-1) SAR/optical images. The digital elevation models used were the SRTM (Shuttle Radar Topography Mission) DEMs and we utilized ASTER stereo-derived DEMs to confirm their accuracy. Data processing was partially supported by the MEGIS (Mars Express Geographic Information System) program, which was developed at IRSPS (International Research School of Planetary Sciences) in Pescara, Italy. Geomorphic mapping was conducted on the GIS-registered multi-layer data set with the help of unsupervised spectral classification of the ASTER data in order to distinguish units. The spectral classification was based on ASTER SWIR (Shortwave Infrared) and TIR (Thermal Infrared) bands. Color composite images produced from JERS-1 optical data were also used in the mapping. The field observation was based on the expedition to the Tsenkher structure in 1998 and focused mostly on geomorphology. Collected rock samples were analyzed by optical microscope. ",
year = "2006",
month = mar,
doi = "10.1016/j.geomorph.2005.07.031",
language = "English (US)",
volume = "74",
pages = "164--180",
journal = "Geomorphology",
issn = "0169-555X",
publisher = "Elsevier B.V.",
number = "1-4",
}