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Fawdon, Peter; Orgel, Csilla; Adeli, Solmaz; Balme, Matt; Calef, Fred J.; Davis, Joel M.; Frigeri, Alessandro; Grindrod, Peter; Hauber, Ernst; Le Deit, Laetitia; Loizeau, Damien; Nass, Andrea; Quantin-Nataf, Cathy; Sefton-Nash, Elliot; Thomas, Nick; Torres, Ines; Vago, Jorge L.; Volat, Matthieu; De Witte, Sander; Altieri, Francesca; Apuzzo, Andrea; Aramendia, Julene; Arana, Gorka; Bahia, Rickbir Singh; Banham, Steven G.; Barnes, Robert; Barrett, Alexander M.; Benedix, Wolf-Stefan; Bhardwaj, Anshuman; Boazman, Sarah Jane; Bontognali, Tomaso R. R.; Bridges, John; Bultel, Benjamin; Ciarletti, Valérie; De Sanctis, Maria Cristina; Dickeson, Zach; Favaro, Elena A.; Ferrari, Marco; Foucher, Frédéric; Goetz, Walter; Haldemann, Albert F. C.; Harrington, Elise; Kapatza, Angeliki; Koschny, Detlef; Krzesinska, Agata M.; Le Gall, Alice; Lewis, Stephen R.; Lim, Tanya; Madariaga, Juan Manuel; Man, Benjamin James; Mandon, Lucia; Mangold, Nicolas; Martin-Torres, Javier; McNeil, Joseph D.; Molina, Antonio; Moral, Andoni G.; Motaghian, Sara; Nikiforov, Sergei; Oudart, Nicolas; Pacifici, Andrea; Parkes Bowen, Adam; Plettemeier, Dirk; Poulakis, Pantelis; Putri, Alfiah Rizky Diana; Ruesch, Ottaviano; Sam, Lydia; Schröder, Christian; Statz, Christoph; Thomas, Rebecca; Tirsch, Daniela; Toth, Zsuzsanna; Turner, Stuart; Voelker, Martin; Werner, Stephanie C.; Westall, Frances; Whiteside, Barry J.; Williams, Adam; Williams, Rebecca M. E.; Wright, Jack and Zorzano, Maria-Paz
(2024).
DOI: https://doi.org/10.1080/17445647.2024.2302361
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.