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dc.contributor.authorCoates, Andrew
dc.contributor.authorJaumann, Ralf
dc.contributor.authorGriffiths, Andrew
dc.contributor.authorLeff, Craig
dc.contributor.authorSchmitz, Nicole
dc.contributor.authorJosset, Jean-Luc
dc.contributor.authorPaar, Gerhard
dc.contributor.authorGunn, Matthew
dc.contributor.authorHauber, Ernst
dc.contributor.authorCousins, Claire Rachel
dc.contributor.authorCross, Rachel
dc.contributor.authorGrindrod, Peter
dc.contributor.authorBridges, John
dc.contributor.authorBalme, Matthew
dc.contributor.authorGupta, Sanjeev
dc.contributor.authorCrawford, Ian
dc.contributor.authorIrwin, P
dc.contributor.authorStabbins, Roger
dc.contributor.authorTirsch, D
dc.contributor.authorVago, Jorge
dc.contributor.authorTheodorou, T
dc.contributor.authorCaballo-Perucha, M
dc.contributor.authorOsinski, Gordon
dc.contributor.authorThe PanCam team
dc.date.accessioned2017-05-29T15:30:09Z
dc.date.available2017-05-29T15:30:09Z
dc.date.issued2017-07-01
dc.identifier.citationCoates , A , Jaumann , R , Griffiths , A , Leff , C , Schmitz , N , Josset , J-L , Paar , G , Gunn , M , Hauber , E , Cousins , C R , Cross , R , Grindrod , P , Bridges , J , Balme , M , Gupta , S , Crawford , I , Irwin , P , Stabbins , R , Tirsch , D , Vago , J , Theodorou , T , Caballo-Perucha , M , Osinski , G & The PanCam team 2017 , ' The PanCam instrument for the ExoMars rover ' , Astrobiology , vol. 17 , no. 6/7 . https://doi.org/10.1089/ast.2016.1548en
dc.identifier.issn1531-1074
dc.identifier.otherPURE: 250036849
dc.identifier.otherPURE UUID: e08f6057-f551-46b3-b94d-44af5604faca
dc.identifier.otherScopus: 85025466556
dc.identifier.otherORCID: /0000-0002-3954-8079/work/60196592
dc.identifier.otherWOS: 000406038400002
dc.identifier.urihttps://hdl.handle.net/10023/10873
dc.descriptionThe authors acknowledge support from the UK Space Agency (lead funding agency for PanCam) and STFC, DLR agency, Swiss Space Office (via PRODEX), Austrian agency.en
dc.description.abstractThe 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.
dc.language.isoeng
dc.relation.ispartofAstrobiologyen
dc.rights© 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.en
dc.subjectMarsen
dc.subjectExoMarsen
dc.subjectInstrumentationen
dc.subjectGeologyen
dc.subjectAtmosphereen
dc.subjectExobiologyen
dc.subjectContexten
dc.subjectQB Astronomyen
dc.subjectGE Environmental Sciencesen
dc.subjectT-NDASen
dc.subject.lccQBen
dc.subject.lccGEen
dc.titleThe PanCam instrument for the ExoMars roveren
dc.typeJournal articleen
dc.contributor.sponsorUK Space Agencyen
dc.contributor.sponsorScience & Technology Facilities Councilen
dc.contributor.sponsorThe Royal Society of Edinburghen
dc.description.versionPublisher PDFen
dc.contributor.institutionUniversity of St Andrews. St Andrews Centre for Exoplanet Scienceen
dc.contributor.institutionUniversity of St Andrews. Earth and Environmental Sciencesen
dc.identifier.doihttps://doi.org/10.1089/ast.2016.1548
dc.description.statusPeer revieweden
dc.identifier.grantnumberen
dc.identifier.grantnumberST/P001297/1en
dc.identifier.grantnumberen


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