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      The PanCam Instrument for the ExoMars Rover

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          Abstract

          The scientific objectives of the ExoMars rover are designed to answer several key questions in the search for life on Mars. In particular, the unique subsurface drill will address some of these, such as the possible existence and stability of subsurface organics. PanCam will establish the surface geological and morphological context for the mission, working in collaboration with other context instruments. Here, we describe the PanCam scientific objectives in geology, atmospheric science, and 3-D vision. We discuss the design of PanCam, which includes a stereo pair of Wide Angle Cameras (WACs), each of which has an 11-position filter wheel and a High Resolution Camera (HRC) for high-resolution investigations of rock texture at a distance. The cameras and electronics are housed in an optical bench that provides the mechanical interface to the rover mast and a planetary protection barrier. The electronic interface is via the PanCam Interface Unit (PIU), and power conditioning is via a DC-DC converter. PanCam also includes a calibration target mounted on the rover deck for radiometric calibration, fiducial markers for geometric calibration, and a rover inspection mirror. Key Words: Mars—ExoMars—Instrumentation—Geology—Atmosphere—Exobiology—Context. Astrobiology 17, 511–541.

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          A versatile camera calibration technique for high-accuracy 3D machine vision metrology using off-the-shelf TV cameras and lenses

          R Tsai (1987)
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            A habitable fluvio-lacustrine environment at Yellowknife Bay, Gale crater, Mars.

            The Curiosity rover discovered fine-grained sedimentary rocks, which are inferred to represent an ancient lake and preserve evidence of an environment that would have been suited to support a martian biosphere founded on chemolithoautotrophy. This aqueous environment was characterized by neutral pH, low salinity, and variable redox states of both iron and sulfur species. Carbon, hydrogen, oxygen, sulfur, nitrogen, and phosphorus were measured directly as key biogenic elements; by inference, phosphorus is assumed to have been available. The environment probably had a minimum duration of hundreds to tens of thousands of years. These results highlight the biological viability of fluvial-lacustrine environments in the post-Noachian history of Mars.
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              Phyllosilicates on Mars and implications for early martian climate.

              The recent identification of large deposits of sulphates by remote sensing and in situ observations has been considered evidence of the past presence of liquid water on Mars. Here we report the unambiguous detection of diverse phyllosilicates, a family of aqueous alteration products, on the basis of observations by the OMEGA imaging spectrometer on board the Mars Express spacecraft. These minerals are mainly associated with Noachian outcrops, which is consistent with an early active hydrological system, sustaining the long-term contact of igneous minerals with liquid water. We infer that the two main families of hydrated alteration products detected-phyllosilicates and sulphates--result from different formation processes. These occurred during two distinct climatic episodes: an early Noachian Mars, resulting in the formation of hydrated silicates, followed by a more acidic environment, in which sulphates formed.
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                Author and article information

                Journal
                Astrobiology
                Astrobiology
                ast
                Astrobiology
                Mary Ann Liebert, Inc. (140 Huguenot Street, 3rd FloorNew Rochelle, NY 10801USA )
                1531-1074
                1557-8070
                01 July 2017
                01 July 2017
                01 July 2017
                : 17
                : 6-7
                : 511-541
                Affiliations
                [ 1 ]Mullard Space Science Laboratory, University College London , Dorking, UK.
                [ 2 ]Centre for Planetary Science at UCL/Birkbeck , London, UK.
                [ 3 ]Institute of Planetary Research , German Aerospace Centre (DLR), Berlin, Germany.
                [ 4 ]Space Exploration Institute , Neuchâtel, Switzerland.
                [ 5 ]Joanneum Research , Graz, Austria.
                [ 6 ]Department of Physics, Aberystwyth University , Aberystwyth, UK.
                [ 7 ]Department of Earth and Environmental Sciences, University of St Andrews , St Andrews, UK.
                [ 8 ]Department of Earth and Planetary Sciences, Birkbeck, University of London , London, UK.
                [ 9 ]Space Research Centre, University of Leicester , Leicester, UK.
                [ 10 ]Department of Earth Sciences, Open University , Milton Keynes, UK.
                [ 11 ]Department of Earth Science and Engineering, Imperial College London , London, UK.
                [ 12 ]Department of Physics, University of Oxford , Oxford, UK.
                [ 13 ]European Space Agency , Noordwijk, the Netherlands.
                [ 14 ]Centre for Planetary Science and Exploration, University of Western Ontario , London, Canada.
                Author notes
                Address correspondence to: Professor Andrew Coates, Mullard Space Science Laboratory, University College London Holmbury St Mary, Dorking RH5 6NT, UK

                E-mail: a.coates@ 123456ucl.ac.uk
                Article
                10.1089/ast.2016.1548
                10.1089/ast.2016.1548
                5568594
                34c48087-e6ea-414e-b1ef-b3b3fff950a2
                © A.J. Coates et al., and the PanCam Team, 2017; Published by Mary Ann Liebert, Inc.

                This Open Access article is distributed under the terms of the Creative Commons License ( http://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly credited.

                History
                : 14 June 2016
                : 01 November 2016
                Page count
                Figures: 15, Tables: 3, References: 162, Pages: 31
                Categories
                Special Collection of Papers: ExoMars Rover Mission

                Guest Editor: Jorge L. Vago

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