The high-resolution map of Oxia Planum, Mars; the landing site of the ExoMars Rosalind Franklin rover mission

Peter Fawdon* (Corresponding Author), Csilla Orgel, Solmaz Adeli, Matt Balme, Fred J. Calef, Joel M. Davis, Alessandro Frigeri, Peter Grindrod, Ernst Hauber, Laetitia Le Deit, Damien Loizeau, Andrea Nass, Cathy Quantin-Nataf, Elliot Sefton-Nash, Nick Thomas, Ines Torres, Jorge L. Vago, Matthieu Volat, Sander De Witte, Francesca AltieriAndrea Apuzzo, Julene Aramendia, Gorka Arana, Rickbir Singh Bahia, Steven G. Banham, Robert Barnes, Alexander M. Barrett, Wolf-Stefan Benedix, Anshuman Bhardwaj, Sarah Jane Boazman, Tomaso R. R. Bontognali, John Bridges, Benjamin Bultel, Valérie Ciarletti, Maria Cristina De Sanctis, Zach Dickeson, Elena A. Favaro, Marco Ferrari, Frédéric Foucher, Walter Goetz, Albert F. C. Haldemann, Elise Harrington, Angeliki Kapatza, Detlef Koschny, Agata M. Krzesinska, Alice Le Gall, Stephen R. Lewis, Tanya Lim, Juan Manuel Madariaga, Benjamin James Man, Lucia Mandon, Nicolas Mangold, Javier Martin-Torres, Joseph D. McNeil, Antonio Molina, Andoni G. Moral, Sara Motaghian, Sergei Nikiforov, Nicolas Oudart, Andrea Pacifici, Adam Parkes Bowen, Dirk Plettemeier, Pantelis Poulakis, Alfiah Rizky Diana Putri, Ottaviano Ruesch, Lydia Sam, Christian Schröder, Christoph Statz, Rebecca Thomas, Daniela Tirsch, Zsuzsanna Toth, Stuart Turner, Martin Voelker, Stephanie C. Werner, Frances Westall, Barry J. Whiteside, Adam Williams, Rebecca M. E. Williams, Jack Wright, Maria-Paz Zorzano

*Corresponding author for this work

Research output: Contribution to journalArticlepeer-review

Abstract

This 1:30,000 scale geological map describes Oxia Planum, Mars, the landing site for the ExoMars Rosalind Franklin rover mission. The map represents our current understanding of bedrock units and their relationships prior to Rosalind Franklin’s exploration of this location. The map details 15 bedrock units organised into 6 groups and 7 textural and surficial units. The bedrock units were identified using visible and near-infrared remote sensing datasets. The objectives of this map are (i) to identify where the most astrobiologically relevant rocks are likely to be found, (ii) to show where hypotheses about their geological context (within Oxia Planum and in the wider geological history of Mars) can be tested, (iii) to inform both the long-term (hundreds of metres to ∼1 km) and the short-term (tens of metres) activity planning for rover exploration, and (iv) to allow the samples analysed by the rover to be interpreted within their regional geological context.
Original languageEnglish
Article number 2302361
Number of pages24
JournalJournal of Maps
Volume20
Issue number1
Early online date22 Mar 2024
DOIs
Publication statusPublished - 2024

Bibliographical note

Acknowledgements
The ExoMars Rosalind Franklin Mission is a partnership between ESA and NASA. The Rosalind Franklin Rover has eight instruments in its ‘Pasteur’ Payload, with Principal Investigators from seven countries all of whom we would like to thank for there support of this project. We would like to acknowledge the following funding bodies, people and institutions supporting the lead authors of this work. We thank the UK Space Agency (UK SA) for funding P. Fawdon, on grants; ST/W002736/1, ST/L00643X/1 and ST/R001413/1, MRB on grants; ST/T002913/1, ST/V001965/1, ST/R001383/1, ST/R001413/1, P. Grindrod on grants; ST/L006456/1, ST/R002355/1, ST/V002678/1 and J. Davis on grants ST/K502388/1, ST/R002355/1, ST/V002678/1 through the ongoing Aurora space exploration programme. C. Orgel was supported by the ESA Research Fellowship Program. Alessandro Frigeri: was funded by the Italian Space Agency (ASI) grant ASI-INAF number 2017-412-H.0 (ExoMars/Ma_MISS) and D. Loizeau was funded by the H2020-COMPET-2015 programme (grant 687302), C. Quantin-Nataf was supported by the French space agency CNES, I. Torres was supported by an ESA Young Graduate Traineeship, A. Nass was supported by Helmholtz Metadata Projects (#ZT-I-PF-3-008). We thank NASA and the HiRISE camera team for data collection support throughout the ExoMars landing site selection and charectorisation process. The USGS for the HiRISE DTM data and maintaining the ISIS and SOCET SET DEM workflows. The authors wish to thank the CaSSIS spacecraft and instrument engineering teams. CaSSIS is a project of the University of Bern and funded through the Swiss Space Office via ESA's PRODEX programme. The instrument hardware development was also supported by the Italian Space Agency (ASI) (ASI-INAF agreement no. I/2020-17-HH.0), INAF/Astronomical Observatory of Padova, and the Space Research Center (CBK) in Warsaw. Support from SGF (Budapest), the University of Arizona (Lunar and Planetary Lab.) and NASA are also gratefully acknowledged. Operations support from the UK Space Agency under grant ST/R003025/1 is also acknowledged. This research has made use of the USGS Integrated Software for Imagers and Spectrometers (ISIS) Technical support for setup of the Multi-Mission Geographic Information System for concurrent team mapping was provided by F. Calef (III) and T. Soliman at NASA JPL and S. de Witte at ESA-ESTEC.
Funding
This work was supported by Agencia Estatal de Investigación [grant number ID2019-107442RB-C32, MDM-2017-0737]; Agenzia Spaziale Italiana [grant number 2017-412-H.0]; Bundesministerium für Wirtschaft und Technologie [grant number 50 QX 2002]; Centre National de la Recherche Scientifique; Centre National d’Etudes Spatiales; Euskal Herriko Unibertsitatea [grant number PES21/88]; Istituto Nazionale di Astrofisica [grant number I/ 060/10/0]; Ministerio de Economía y Competitividad [grant number PID2019-104205GB-C21]; Ministry of Science and Higher Education of the Russian Federation [grant number AAAA-A18-118012290370-6]; National Aeronautics and Space Administration [grant number NNX15AH46G]; Norges Forskningsråd [grant number 223272]; European Union's Horizon 2020 (H2020-COMPET-2015) [grant number 687302 (PTAL)]; Sofja Kovalevskaja Award of the Alexander von Humboldt Foundation; MINECO [grant number PID2019-107442RB-C32]; The Open University [grant number Space Strategic Research Area]; European Union's Horizon 2020 research and innovation programme [grant number 776276]; H2020-COMPET-2015 [grant number 687302]; The Research Council of Norway, Centres of Excellence funding scheme [grant number 223272]; Helmholtz Metadata Projects [grant number ZT-I-PF-3-008]; The Research Council of Norway [grant number 223272]; Swiss Space Office via ESA's PRODEX programme; Ines Torres was supported by an ESA Young Graduate Traineeship; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung [grant number 200021_197293]; Science and Technology Facilities Council [grant number 1967420]; UK Space Agency [grant number ST/K502388/1, ST/R002355/1, ST/V002678/1].

Data Availability Statement

The data used in the map, the informal geographic areas, the rover operations quad grid, and the multiband CaSSIS cubes being used for the scientific evaluation of Oxia Planum are freely available through the ESA Guest Storage Facility (https://www.cosmos.esa.int/web/psa/exomars2022-rsowg_oxia-planum_geography-cassis-ctx_v1.0) and as the supplementary data set to (Fawdon et al., Citation2021). The map geodatabase is available through The Open University (Fawdon et al., Citation2023) The HiRISE orthomosaic and DEM (Quantin-Nataf et al., Citation2018; Volat & Quantan-Nataf, Citation2020) basemap was produced using the MarsSI infrastructure, is published on the Planetary SUrface Portal (PSUP), and is co-registered with the datasets presented here. Individual HiRISE DTM are being released publicly through the University of Arizona (Table 1). NOAH-H data and HiRISE basemap information is available through Barrett et al. (Citation2023). A package of the map layers including georeferenced HiRISE RGB data is publicly available through the ArcOnline living atlas https://arcg.is/0y4bSa.

Keywords

  • ExoMars
  • Oxia Planum
  • Mars
  • Geological map
  • Astrobiology
  • Rosalind Franklin Rover

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