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      The Mars 2020 Perseverance Rover Mast Camera Zoom (Mastcam-Z) Multispectral, Stereoscopic Imaging Investigation

      review-article
      1 , , 2 , 1 , 3 , 3 , 2 , 3 , 3 , 4 , 4 , 1 , 5 , 5 , 5 , 5 , 1 , 3 , 1 , 1 , 1 , 1 , 5 , 6 , 1 , 2 , 7 , 8 , 9 , 10 , 3 , 11 , 2 , 12 , 11 , 1 , 13 , 14 , 15 , 16 , 17 , 18 , 18 , 19 , 20 , 21 , 22 , 1 , 20 , 5 , 17
      Space Science Reviews
      Springer Netherlands
      Mars, Mars 2020 mission, Perseverance rover, Jezero crater, Space instrumentation, Space imaging

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          Abstract

          Mastcam-Z is a multispectral, stereoscopic imaging investigation on the Mars 2020 mission’s Perseverance rover. Mastcam-Z consists of a pair of focusable, 4:1 zoomable cameras that provide broadband red/green/blue and narrowband 400-1000 nm color imaging with fields of view from 25.6° × 19.2° (26 mm focal length at 283 μrad/pixel) to 6.2° × 4.6° (110 mm focal length at 67.4 μrad/pixel). The cameras can resolve (≥ 5 pixels) ∼0.7 mm features at 2 m and ∼3.3 cm features at 100 m distance. Mastcam-Z shares significant heritage with the Mastcam instruments on the Mars Science Laboratory Curiosity rover. Each Mastcam-Z camera consists of zoom, focus, and filter wheel mechanisms and a 1648 × 1214 pixel charge-coupled device detector and electronics. The two Mastcam-Z cameras are mounted with a 24.4 cm stereo baseline and 2.3° total toe-in on a camera plate ∼2 m above the surface on the rover’s Remote Sensing Mast, which provides azimuth and elevation actuation. A separate digital electronics assembly inside the rover provides power, data processing and storage, and the interface to the rover computer. Primary and secondary Mastcam-Z calibration targets mounted on the rover top deck enable tactical reflectance calibration. Mastcam-Z multispectral, stereo, and panoramic images will be used to provide detailed morphology, topography, and geologic context along the rover’s traverse; constrain mineralogic, photometric, and physical properties of surface materials; monitor and characterize atmospheric and astronomical phenomena; and document the rover’s sample extraction and caching locations. Mastcam-Z images will also provide key engineering information to support sample selection and other rover driving and tool/instrument operations decisions.

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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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            Mars Global Surveyor Mars Orbiter Camera: Interplanetary cruise through primary mission

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              Mars surface diversity as revealed by the OMEGA/Mars Express observations.

              The Observatoire pour la Minéralogie, l'Eau, les Glaces, et l'Activité (OMEGA) investigation, on board the European Space Agency Mars Express mission, is mapping the surface composition of Mars at a 0.3- to 5-kilometer resolution by means of visible-near-infrared hyperspectral reflectance imagery. The data acquired during the first 9 months of the mission already reveal a diverse and complex surface mineralogy, offering key insights into the evolution of Mars. OMEGA has identified and mapped mafic iron-bearing silicates of both the northern and southern crust, localized concentrations of hydrated phyllosilicates and sulfates but no carbonates, and ices and frosts with a water-ice composition of the north polar perennial cap, as for the south cap, covered by a thin carbon dioxide-ice veneer.
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                Author and article information

                Contributors
                Jim.Bell@asu.edu
                Journal
                Space Sci Rev
                Space Sci Rev
                Space Science Reviews
                Springer Netherlands (Dordrecht )
                0038-6308
                1572-9672
                15 February 2021
                15 February 2021
                2021
                : 217
                : 1
                : 24
                Affiliations
                [1 ]GRID grid.215654.1, ISNI 0000 0001 2151 2636, Arizona State Univ., ; Tempe, AZ USA
                [2 ]GRID grid.211367.0, JPL/Caltech, ; Pasadena, CA USA
                [3 ]GRID grid.486979.d, ISNI 0000 0004 6023 2081, Malin Space Science Systems, Inc., ; San Diego, CA USA
                [4 ]GRID grid.5254.6, ISNI 0000 0001 0674 042X, Univ. of Copenhagen, ; Copenhagen, Denmark
                [5 ]GRID grid.5386.8, ISNI 000000041936877X, Cornell Univ., ; Ithaca, NY USA
                [6 ]Opscode LLC, Healdsburg, CA USA
                [7 ]GRID grid.427160.6, ISNI 0000 0001 0719 6980, The Planetary Society, ; Pasadena, CA USA
                [8 ]GRID grid.267457.5, ISNI 0000 0001 1703 4731, Univ. of Winnipeg, ; Winnipeg, Canada
                [9 ]GRID grid.83440.3b, ISNI 0000000121901201, Mullard Space Science Laboratory, , Univ. College, ; London, UK
                [10 ]GRID grid.419075.e, ISNI 0000 0001 1955 7990, NASA/Ames Research Center, ; Moffett Field, CA USA
                [11 ]GRID grid.20861.3d, ISNI 0000000107068890, Caltech, ; Pasadena, CA USA
                [12 ]GRID grid.162346.4, ISNI 0000 0001 1482 1895, Univ. of Hawaii, ; Honolulu, HI USA
                [13 ]USGS Astrogeology Science Center, Flagstaff, AZ USA
                [14 ]GRID grid.169077.e, ISNI 0000 0004 1937 2197, Purdue Univ., ; South Bend, IN USA
                [15 ]GRID grid.14095.39, ISNI 0000 0000 9116 4836, Inst. of Geological Sciences, , Free University Berlin, ; Berlin, Germany
                [16 ]GRID grid.21107.35, ISNI 0000 0001 2171 9311, APL/Johns Hopkins Univ., ; Laurel, MD USA
                [17 ]GRID grid.296797.4, Space Science Inst., ; Boulder, CO USA
                [18 ]GRID grid.8684.2, ISNI 0000 0004 0644 9589, Joanneum Research, ; Graz, Austria
                [19 ]GRID grid.7445.2, ISNI 0000 0001 2113 8111, Imperial College, ; London, UK
                [20 ]VRVis Research Center, Vienna, Austria
                [21 ]GRID grid.7551.6, ISNI 0000 0000 8983 7915, DLR/German Aerospace Center, ; Berlin, Germany
                [22 ]GRID grid.281386.6, ISNI 0000 0001 2165 7413, Western Washington Univ., ; Bellingham, WA USA
                Author information
                http://orcid.org/0000-0002-2006-4074
                Article
                755
                10.1007/s11214-020-00755-x
                7883548
                33612866
                476b01f4-c697-424b-a209-474296319466
                © The Author(s) 2020

                Open Access This article is licensed under a Creative Commons Attribution 4.0 International License, which permits use, sharing, adaptation, distribution and reproduction in any medium or format, as long as you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons licence, and indicate if changes were made. The images or other third party material in this article are included in the article’s Creative Commons licence, unless indicated otherwise in a credit line to the material. If material is not included in the article’s Creative Commons licence and your intended use is not permitted by statutory regulation or exceeds the permitted use, you will need to obtain permission directly from the copyright holder. To view a copy of this licence, visit http://creativecommons.org/licenses/by/4.0/.

                History
                : 22 May 2020
                : 25 September 2020
                Funding
                Funded by: FundRef http://dx.doi.org/10.13039/100000104, National Aeronautics and Space Administration;
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                © Springer Nature B.V. 2021

                mars,mars 2020 mission,perseverance rover,jezero crater,space instrumentation,space imaging

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