Jean-Baptiste P, Petit J R, Lipenkov V Y, Raynaud D, Barkov N I
Laboratoire des Sciences du Climat et de l'Environnement, CEA/CNRS, Centre d'études de Saclay, 91191 Gif sur Yvette, France.
Nature. 2001 May 24;411(6836):460-2. doi: 10.1038/35078045.
Lake Vostok, the largest subglacial lake in Antarctica, is covered by the East Antarctic ice sheet, which varies in thickness between 3,750 and 4,100 m (ref. 1). At a depth of 3,539 m in the drill hole at Vostok station, sharp changes in stable isotopes and the gas content of the ice delineate the boundary between glacier ice and ice accreted through re-freezing of lake water. Unlike most gases, helium can be incorporated into the crystal structure of ice during freezing, making helium isotopes in the accreted ice a valuable source of information on lake environment. Here we present helium isotope measurements from the deep section of the Vostok ice core that encompasses the boundary between the glacier ice and accreted ice, showing that the accreted ice is enriched by a helium source with a radiogenic isotope signature typical of an old continental province. This result rules out any significant hydrothermal energy input into the lake from high-enthalpy mantle processes, which would be expected to produce a much higher 3He/4He ratio. Based on the average helium flux for continental areas, the helium budget of the lake leads to a renewal time of the lake of the order of 5,000 years.
沃斯托克湖是南极洲最大的冰下湖,被东南极冰盖覆盖,该冰盖厚度在3750米至4100米之间(参考文献1)。在沃斯托克站钻孔深度3539米处,冰的稳定同位素和气体含量的急剧变化划定了冰川冰与通过湖水再冻结而积聚的冰之间的边界。与大多数气体不同,氦在冻结过程中可以融入冰的晶体结构,使得积聚冰中的氦同位素成为湖泊环境信息的宝贵来源。在此,我们展示了来自沃斯托克冰芯深部的氦同位素测量结果,该深部涵盖了冰川冰与积聚冰之间的边界,结果表明积聚冰因一个具有古老大陆省份典型放射性同位素特征的氦源而富集。这一结果排除了高焓地幔过程向湖泊输入任何大量热液能量的可能性,因为这种过程预计会产生高得多的3He/4He比值。根据大陆地区的平均氦通量,该湖的氦收支情况得出该湖的更新时间约为5000年。