Department of Geosciences, State University of New York, Stony Brook, NY 11794, USA.
Science. 2014 Jan 24;343(6169):1244734. doi: 10.1126/science.1244734. Epub 2013 Dec 9.
Sedimentary rocks examined by the Curiosity rover at Yellowknife Bay, Mars, were derived from sources that evolved from an approximately average martian crustal composition to one influenced by alkaline basalts. No evidence of chemical weathering is preserved, indicating arid, possibly cold, paleoclimates and rapid erosion and deposition. The absence of predicted geochemical variations indicates that magnetite and phyllosilicates formed by diagenesis under low-temperature, circumneutral pH, rock-dominated aqueous conditions. Analyses of diagenetic features (including concretions, raised ridges, and fractures) at high spatial resolution indicate that they are composed of iron- and halogen-rich components, magnesium-iron-chlorine-rich components, and hydrated calcium sulfates, respectively. Composition of a cross-cutting dike-like feature is consistent with sedimentary intrusion. The geochemistry of these sedimentary rocks provides further evidence for diverse depositional and diagenetic sedimentary environments during the early history of Mars.
好奇号探测器在火星耶利哥湾(Yellowknife Bay)检查的沉积岩源自大约平均火星地壳成分演变成受碱性玄武岩影响的源区。没有保存下来化学风化的证据,表明存在干旱、可能寒冷的古气候以及快速的侵蚀和沉积。缺乏预测的地球化学变化表明,磁铁矿和层状硅酸盐是在低温、近中性 pH 值、以岩石为主的水相条件下成岩作用形成的。对高空间分辨率成岩特征(包括结核、隆起脊和裂缝)的分析表明,它们分别由富铁和卤素成分、富镁铁氯成分和水合硫酸钙组成。切穿的岩脉状特征的成分与沉积侵入一致。这些沉积岩的地球化学为火星早期多样化的沉积和成岩沉积环境提供了进一步的证据。