Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, USA.
Electrophoresis. 2018 Nov;39(22):2854-2863. doi: 10.1002/elps.201700459. Epub 2018 Feb 9.
For decades, the Martian regolith has stymied robotic mission efforts to catalog the organic molecules present. Perchlorate salts, found widely throughout Mars, are the main culprit as they breakdown and react with organics liberated from the regolith during pyrolysis, the primary extraction technique attempted to date on Mars. This work further develops subcritical water extraction (SCWE) as a technique for extraction of amino acids on future missions. The effect of SCWE temperature (185, 200, and 215°C) and duration of extraction (10-120 min) on the total amount and distribution of amino acids recovered was explored for three Mars analog soils (JSC Mars-1A simulant, an Atacama desert soil, and an Antarctic Dry Valleys soil) and bovine serum albumin (as a control solution of known amino acid content). Total amounts of amino acids extracted increased with both time and temperature; however, the distribution shifted notably due to the destruction of the amino acids with charged or polar side chains at the higher temperatures. The pure bovine serum albumin solution and JSC Mars 1A also showed lower yields than the Atacama and Antarctic extractions suggesting that SCWE may be less effective at hydrolyzing large or aggregated proteins. Changing solvent from water to a dilute (10 mM) HCl solution allowed total extraction efficiencies comparable to the higher temperature/time combinations while using the lowest temperature/time (185°C/20 min). The dilute HCl extractions also did not lead to the shift in amino acid distribution observed at the higher temperatures. Additionally, adding sodium perchlorate salt to the extraction did not interfere with recoveries. Native magnetite in the JSC Mars-1A may have been responsible for destruction of glycine, as evidenced by its uncharacteristic decrease as the temperature/time of extraction increased. This work shows that SCWE can extract high yields of native amino acids out of Mars analog soils with minimal disruption of the distribution of those amino acids, even in the presence of a perchlorate salt.
几十年来,火星风化层一直阻碍着机器人任务对存在的有机分子进行编目。在火星上广泛发现的高氯酸盐盐是主要罪魁祸首,因为它们在热解过程中分解并与从风化层中释放的有机物反应,这是迄今为止在火星上尝试的主要提取技术。这项工作进一步将亚临界水提取 (SCWE) 发展为未来任务中提取氨基酸的技术。探索了 SCWE 温度(185、200 和 215°C)和提取时间(10-120 分钟)对从三种火星模拟土壤(JSC Mars-1A 模拟物、阿塔卡马沙漠土壤和南极干谷土壤)和牛血清白蛋白(作为已知氨基酸含量的对照溶液)中回收的氨基酸总量和分布的影响。氨基酸提取总量随时间和温度的增加而增加;然而,由于在较高温度下带电荷或极性侧链的氨基酸被破坏,分布明显发生了变化。纯牛血清白蛋白溶液和 JSC Mars 1A 的产率也低于阿塔卡马和南极提取液,这表明 SCWE 可能在水解大或聚集的蛋白质方面效果较差。将溶剂从水改为稀(10 mM)HCl 溶液可实现与较高温度/时间组合相当的总提取效率,同时使用最低的温度/时间(185°C/20 分钟)。在较高温度下观察到的氨基酸分布变化也不会导致稀 HCl 提取物。此外,向提取液中添加高氯酸钠盐不会干扰回收。JSC Mars-1A 中的天然磁铁矿可能是破坏甘氨酸的原因,因为随着提取温度/时间的增加,其含量异常下降。这项工作表明,SCWE 可以从火星模拟土壤中提取出高产量的天然氨基酸,而对这些氨基酸的分布几乎没有干扰,即使存在高氯酸盐盐也是如此。