Citation

BibTex format

@article{Farley:2022:10.1126/science.abo2196,
author = {Farley, KA and Stack, KM and Shuster, DL and Horgan, BHN and Hurowitz, JA and Tarnas, JD and Simon, JI and Sun, VZ and Scheller, EL and Moore, KR and McLennan, SM and Vasconcelos, PM and Wiens, RC and Treiman, AH and Mayhew, LE and Beyssac, O and Kizovski, TV and Tosca, NJ and Williford, KH and Crumpler, LS and Beegle, LW and Bell, JF and Ehlmann, BL and Liu, Y and Maki, JN and Schmidt, ME and Allwood, AC and Amundsen, HEF and Bhartia, R and Bosak, T and Brown, AJ and Clark, BC and Cousin, A and Forni, O and Gabriel, TSJ and Goreva, Y and Gupta, S and Hamran, S-E and Herd, CDK and Hickman-Lewis, K and Johnson, JR and Kah, LC and Kelemen, PB and Kinch, KB and Mandon, L and Mangold, N and Quantin-Nataf, C and Rice, MS and Russell, PS and Sharma, S and Siljeström, S and Steele, A and Sullivan, R and Wadhwa, M and Weiss, BP and Williams, AJ and Wogsland, BV and Willis, PA and Acosta-Maeda, TA and Beck, P and Benzerara, K and Bernard, S and Burton, AS and Cardarelli, EL and Chide, B and Cla},
doi = {10.1126/science.abo2196},
journal = {Science},
title = {Aqueously altered igneous rocks sampled on the floor of Jezero crater, Mars},
url = {http://dx.doi.org/10.1126/science.abo2196},
volume = {0},
year = {2022}
}

RIS format (EndNote, RefMan)

TY  - JOUR
AB - The Perseverance rover landed in Jezero crater, Mars, to investigate ancient lake and river deposits. We report observations of the crater floor, below the crater?s sedimentary delta, finding the floor consists of igneous rocks altered by water. The lowest exposed unit, informally named Séítah, is a coarsely crystalline olivine-rich rock, which accumulated at the base of a magma body. Fe-Mg carbonates along grain boundaries indicate reactions with CO2-rich water, under water-poor conditions. Overlying Séítah is a unit informally named Máaz, which we interpret as lava flows or the chemical complement to Séítah in a layered igneous body. Voids in these rocks contain sulfates and perchlorates, likely introduced by later near-surface brine evaporation. Core samples of these rocks were stored aboard Perseverance for potential return to Earth.
AU - Farley,KA
AU - Stack,KM
AU - Shuster,DL
AU - Horgan,BHN
AU - Hurowitz,JA
AU - Tarnas,JD
AU - Simon,JI
AU - Sun,VZ
AU - Scheller,EL
AU - Moore,KR
AU - McLennan,SM
AU - Vasconcelos,PM
AU - Wiens,RC
AU - Treiman,AH
AU - Mayhew,LE
AU - Beyssac,O
AU - Kizovski,TV
AU - Tosca,NJ
AU - Williford,KH
AU - Crumpler,LS
AU - Beegle,LW
AU - Bell,JF
AU - Ehlmann,BL
AU - Liu,Y
AU - Maki,JN
AU - Schmidt,ME
AU - Allwood,AC
AU - Amundsen,HEF
AU - Bhartia,R
AU - Bosak,T
AU - Brown,AJ
AU - Clark,BC
AU - Cousin,A
AU - Forni,O
AU - Gabriel,TSJ
AU - Goreva,Y
AU - Gupta,S
AU - Hamran,S-E
AU - Herd,CDK
AU - Hickman-Lewis,K
AU - Johnson,JR
AU - Kah,LC
AU - Kelemen,PB
AU - Kinch,KB
AU - Mandon,L
AU - Mangold,N
AU - Quantin-Nataf,C
AU - Rice,MS
AU - Russell,PS
AU - Sharma,S
AU - Siljeström,S
AU - Steele,A
AU - Sullivan,R
AU - Wadhwa,M
AU - Weiss,BP
AU - Williams,AJ
AU - Wogsland,BV
AU - Willis,PA
AU - Acosta-Maeda,TA
AU - Beck,P
AU - Benzerara,K
AU - Bernard,S
AU - Burton,AS
AU - Cardarelli,EL
AU - Chide,B
AU - Clavé,E
AU - Cloutis,EA
AU - Cohen,BA
AU - Czaja,AD
AU - Debaille,V
AU - Dehouck,E
AU - Fairén,AG
AU - Flannery,DT
AU - Fleron,SZ
AU - Fouchet,T
AU - Frydenvang,J
AU - Garczynski,BJ
AU - Gibbons,EF
AU - Hausrath,EM
AU - Hayes,AG
AU - Henneke,J
AU - Jørgensen,JL
AU - Kelly,EM
AU - Lasue,J
AU - Le,Mouélic S
AU - Madariaga,JM
AU - Maurice,S
AU - Merusi,M
AU - Meslin,P-Y
AU - Milkovich,SM
AU - Million,CC
AU - Moeller,RC
AU - Núñez,JI
AU - Ollila,AM
AU - Paar,G
AU - Paige,DA
AU - Pedersen,DAK
AU - Pilleri,P
AU - Pilorget,C
AU - Pinet,PC
AU - Rice,JW
AU - Royer,C
AU - Sautter,V
AU - Schulte,M
AU - Sephton,MA
AU - Sharma,SK
AU - Sholes,SF
AU - Spanovich,N
AU - St,Clair M
AU - Tate,CD
AU - Uckert,K
AU - VanBommel,SJ
AU - Yanchilina,AG
AU - Zorzano,M-P
DO - 10.1126/science.abo2196
PY - 2022///
TI - Aqueously altered igneous rocks sampled on the floor of Jezero crater, Mars
T2 - Science
UR - http://dx.doi.org/10.1126/science.abo2196
UR - https://doi.org/10.1126/science.abo2196
VL - 0
ER -