Turner G, Knott S F, Ash R D, Gilmour J D
Department of Earth Sciences, University of Manchester, UK.
Geochim Cosmochim Acta. 1997 Sep;61(18):3835-50. doi: 10.1016/s0016-7037(97)00285-8.
ALH84001, a cataclastic cumulate orthopyroxenite meteorite from Mars, has been dated by Ar-Ar stepped heating and laser probe methods. Both methods give ages close to 3,900 Ma. The age calculated is dependent on assumptions made about 39Ar recoil effects and on whether significant quantities of 40Ar from the Martian atmosphere are trapped in the meteorite. If, as suggested by xenon and nitrogen isotope studies, Martian atmospheric argon is present, then it must reside predominantly in the K-rich phase maskelynite. Independently determined 129Xe abundances in the maskelynite can be used to place limits on the concentration of the atmospheric 40Ar. These indicate a reduction of around 80 Ma to ages calculated on the assumption that no Martian atmosphere is present. After this correction, the nominal ages obtained are: 3940 +/- 50, 3870 +/- 80, and 3970 +/- 100 Ma. by stepped heating, and 3900 +/- 90 Ma by laser probe (1 sigma statistical errors), giving a weighted mean value of 3,920 Ma. Ambiguities in the interpretation of 39Ar recoil effects and in the contribution of Martian atmospheric 40Ar lead to uncertainties in the Ar-Ar age which are difficult to quantify, but we suggest that the true value lies somewhere between 4,050 and 3,800 Ma. This age probably dates a period of annealing of the meteorite subsequent to the shock event which gave it its cataclastic texture. The experiments provide the first evidence of an event occurring on Mars coincident with the time of the late heavy bombardment of the Moon and may reflect a similar period of bombardment in the Southern Highlands of Mars. Whether the age determined bears any relationship to the time of carbonate deposition in ALH84001 is not known. Such a link depends on whether the temperature associated with the metasomatic activity was sufficient to cause argon loss from the maskelynite and/or whether the metasomatism and metamorphism were linked in time through a common heat source.
ALH84001是一块来自火星的碎裂堆积斜方辉石岩陨石,已通过氩-氩阶段加热法和激光探针法进行了年代测定。两种方法得出的年龄都接近39亿年。计算出的年龄取决于对39Ar反冲效应所做的假设,以及火星大气中的大量40Ar是否被困在陨石中。如果正如氙和氮同位素研究表明的那样存在火星大气氩,那么它必定主要存在于富钾相的斜长石中。在斜长石中独立测定的129Xe丰度可用于确定大气40Ar的浓度范围。这些结果表明,与假设不存在火星大气时计算出的年龄相比,年龄减少了约8亿年。经过这种校正后,通过阶段加热法得到的标称年龄为:3940±50、3870±80和3970±100百万年,通过激光探针法得到的年龄为3900±90百万年(1σ统计误差),加权平均值为39.2亿年。对39Ar反冲效应的解释以及火星大气40Ar的贡献存在模糊性,导致氩-氩年龄存在难以量化的不确定性,但我们认为真实值介于40.5亿年和38亿年之间。这个年龄可能测定的是陨石在赋予其碎裂结构的冲击事件之后的退火时期。这些实验首次证明了火星上发生的一个事件与月球晚期重轰炸的时间一致,并且可能反映了火星南部高地类似的轰炸时期。所测定的年龄与ALH84001中碳酸盐沉积的时间是否存在任何关系尚不清楚。这样一种联系取决于与交代活动相关的温度是否足以导致斜长石中的氩损失,以及交代作用和变质作用是否通过共同的热源在时间上相互关联。