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Fluid-evaporation records preserved in salt assemblages in Meridiani rocks

机译:Meridiani岩石中盐组合中保存的流体蒸发记录

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We studied the inter-relationships between the major anions (SO3, Cl, and Br) and cations (FeO, CaO and MgO) using elemental abundances determined by APXS in salt assemblages of RATted (abraded) rocks at Meridiani to characterize the behavior of fluids that infiltrated into this region on Mars. A Plot Of SO3 versus Cl for the abraded rocks yielded an unusual pattern, whereas the SO3/Cl ratios versus Cl for the same rocks showed a monotonically decreasing trend represented by a hyperbola. The systematic behavior of the SO3 and Cl data in the documented rocks at Meridiani suggests that these anions behaved conservatively during fluid-rock interactions. These results further indicate that two kinds of fluids, referred to as SOL-I and SOL-II, infiltrated into Endurance/Eagle/Fram craters, where they underwent progressive evaporative concentration. SOL-I is a low pH fluid consisting of high SO3 and low Cl and high Br, (this fluid infiltrated all the way to the crater-top region), whereas SOL-II fluid of high pH with low SO3 and high Cl and low Br reached only an intermediary level known as the Whatanga contact at Endurance. Based on the FeO/MgO as well as CaO/MgO versus SO3/Cl diagram for rocks above the Whatanga contact, the cation and anion relationships in this system suggest that the Fe2+/SO4 and Ca2+/SO4 ratios in SOL-I fluids at Meridiani were > 1 before the onset of evaporation based on the "chemical divide" considerations. Below the Whatanga contact, relatively dilute SOL-II fluids seem to have infiltrated and dissolved/flushed away the easily soluble Mg-sulfate/chloride phases (along with Br) without significantly altering the SO3/Cl ratios in the residual salt assemblages. Further, Cl/Br versus Br in rocks above the Whatanga contact show a hyperbolic trend suggesting that Cl and Br behaved conservatively similar to SO3 and Cl in the SOL-I fluids at Meridiani. Our results are consistent with a scenario involving two episodes (SOL-I and SOL-II) of groundwater recharge at Meridiani Planum.
机译:我们使用APXS在Meridiani RATRAT(磨合)岩石的盐组合中确定的元素丰度,研究了主要阴离子(SO3,Cl和Br)与阳离子(FeO,CaO和MgO)之间的相互关系,以表征流体的行为渗透到火星的这个区域。磨蚀岩石的SO3与Cl的关系图显示出不同寻常的模式,而相同岩石的SO3 / Cl比与Cl的关系则以双曲线表示单调下降的趋势。 Meridiani记录的岩石中SO3和Cl数据的系统行为表明,这些阴离子在流体-岩石相互作用过程中表现为保守。这些结果进一步表明,两种流体,分别称为SOL-I和SOL-II,渗入了Endurance / Eagle / Fram火山口,并在那里进行了逐步蒸发浓缩。 SOL-I是一种低pH值的流体,由高SO3,低Cl和高Br组成(该流体一直渗透到火山口顶部区域),而SOL-II的高pH值流体则具有低SO3,高Cl和低含量Br仅在Endurance达到了称为Whatanga contact的中间级别。根据Whatanga接触上方岩石的FeO / MgO以及CaO / MgO与SO3 / Cl的关系图,该系统中的阳离子和阴离子关系表明,Meriidiani SOL-1流体中Fe2 + / SO4和Ca2 + / SO4的比率根据“化学分度”的考虑,在蒸发开始之前,≥1。在Whattana接触之下,相对稀薄的SOL-II流体似乎已经渗透并溶解/倒掉了易溶的硫酸镁/氯化物相(以及Br),而没有显着改变残留盐组合中的SO3 / Cl比。此外,Whatanga接触上方岩石中的Cl / Br与Br呈双曲线趋势,表明在Meridiani的SOL-1流体中,Cl和Br的行为与SO3和Cl保守地相似。我们的结果与Meridiani Planum涉及两次地下水补给(SOL-I和SOL-II)的情景是一致的。

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