Y Liu, M M Tice, M E Schmidt, A H Treiman, T V Kizovski, J A Hurowitz, A C Allwood, J Henneke, D A K Pedersen, S J VanBommel, M W M Jones, A L Knight, B J Orenstein, B C Clark, W T Elam, C M Heirwegh, T Barber, L W Beegle, K Benzerara, S Bernard, O Beyssac, T Bosak, A J Brown, E L Cardarelli, D C Catling, J R Christian, E A Cloutis, B A Cohen, S Davidoff, A G Fairén, K A Farley, D T Flannery, A Galvin, J P Grotzinger, S Gupta, J Hall, C D K Herd, K Hickman-Lewis, R P Hodyss, B H N Horgan, J R Johnson, J L Jørgensen, L C Kah, J N Maki, L Mandon, N Mangold, F M McCubbin, S M McLennan, K Moore, M Nachon, P Nemere, L D Nothdurft, J I Núñez, L O'Neil, C M Quantin-Nataf, V Sautter, D L Shuster, K L Siebach, J I Simon, K P Sinclair, K M Stack, A Steele, J D Tarnas, N J Tosca, K Uckert, A Udry, L A Wade, B P Weiss, R C Wiens, K H Williford, M-P Zorzano
The geological units on the floor of Jezero crater, Mars, are part of a wider regional stratigraphy of olivine-rich rocks, which extends well beyond the crater. We investigate the petrology of olivine and carbonate-bearing rocks of the Séítah formation in the floor of Jezero. Using multispectral images and x-ray fluorescence data, acquired by the Perseverance rover, we performed a petrographic analysis of the Bastide and Brac outcrops within this unit. We find that these outcrops are composed of igneous rock, moderately altered by aqueous fluid...
August 25, 2022: Science