Stoker Carol R, Cannon Howard N, Dunagan Stephen E, Lemke Lawrence G, Glass Brian J, Miller David, Gomez-Elvira Javier, Davis Kiel, Zavaleta Jhony, Winterholler Alois, Roman Matt, Rodriguez-Manfredi Jose Antonio, Bonaccorsi Rosalba, Bell Mary Sue, Brown Adrian, Battler Melissa, Chen Bin, Cooper George, Davidson Mark, Fernández-Remolar David, Gonzales-Pastor Eduardo, Heldmann Jennifer L, Martínez-Frías Jesus, Parro Victor, Prieto-Ballesteros Olga, Sutter Brad, Schuerger Andrew C, Schutt John, Rull Fernando
NASA Ames Research Center, Moffett Field, California 94035, USA.
Astrobiology. 2008 Oct;8(5):921-45. doi: 10.1089/ast.2007.0217.
The Mars Astrobiology Research and Technology Experiment (MARTE) simulated a robotic drilling mission to search for subsurface life on Mars. The drill site was on Peña de Hierro near the headwaters of the Río Tinto river (southwest Spain), on a deposit that includes massive sulfides and their gossanized remains that resemble some iron and sulfur minerals found on Mars. The mission used a fluidless, 10-axis, autonomous coring drill mounted on a simulated lander. Cores were faced; then instruments collected color wide-angle context images, color microscopic images, visible-near infrared point spectra, and (lower resolution) visible-near infrared hyperspectral images. Cores were then stored for further processing or ejected. A borehole inspection system collected panoramic imaging and Raman spectra of borehole walls. Life detection was performed on full cores with an adenosine triphosphate luciferin-luciferase bioluminescence assay and on crushed core sections with SOLID2, an antibody array-based instrument. Two remotely located science teams analyzed the remote sensing data and chose subsample locations. In 30 days of operation, the drill penetrated to 6 m and collected 21 cores. Biosignatures were detected in 12 of 15 samples analyzed by SOLID2. Science teams correctly interpreted the nature of the deposits drilled as compared to the ground truth. This experiment shows that drilling to search for subsurface life on Mars is technically feasible and scientifically rewarding.
火星天体生物学研究与技术实验(MARTE)模拟了一次机器人钻探任务,以寻找火星地下的生命。钻探地点位于西班牙西南部力拓河源头附近的佩尼亚德耶罗,在一个包含块状硫化物及其铁帽化残骸的矿床,这些残骸类似于在火星上发现的一些铁和硫矿物。该任务使用了一台安装在模拟着陆器上的无流体、10轴自主取芯钻机。岩芯被切割;然后仪器收集彩色广角背景图像、彩色微观图像、可见-近红外点光谱以及(低分辨率)可见-近红外高光谱图像。然后将岩芯储存起来以供进一步处理或排出。一个钻孔检测系统收集钻孔壁的全景成像和拉曼光谱。使用三磷酸腺苷荧光素-荧光素酶生物发光测定法对完整岩芯进行生命检测,并使用基于抗体阵列的仪器SOLID2对粉碎的岩芯部分进行检测。两个位于远程的科学团队分析了遥感数据并选择了子样本位置。在30天的作业中,钻机钻进了6米并收集了21个岩芯。在SOLID2分析的15个样本中的12个中检测到了生物特征。与实际情况相比,科学团队正确地解释了所钻探矿床的性质。该实验表明,在火星上钻探以寻找地下生命在技术上是可行的,并且在科学上是有意义的。