NASA Ames Research Center, Moffett Field, California, USA.
Astrobiology. 2012 Sep;12(9):841-53. doi: 10.1089/ast.2012.0861.
We report the first science results from the Space Environment Viability of Organics (SEVO) payload aboard the Organism/Organic Exposure to Orbital Stresses (O/OREOS) free-flying nanosatellite, which completed its nominal spaceflight mission in May 2011 but continues to acquire data biweekly. The SEVO payload integrates a compact UV-visible-NIR spectrometer, utilizing the Sun as its light source, with a 24-cell sample carousel that houses four classes of vacuum-deposited organic thin films: polycyclic aromatic hydrocarbon (PAH), amino acid, metalloporphyrin, and quinone. The organic films are enclosed in hermetically sealed sample cells that contain one of four astrobiologically relevant microenvironments. Results are reported in this paper for the first 309 days of the mission, during which the samples were exposed for ∼2210 h to direct solar illumination (∼1080 kJ/cm(2) of solar energy over the 124-2600 nm range). Transmission spectra (200-1000 nm) were recorded for each film, at first daily and subsequently every 15 days, along with a solar spectrum and the dark response of the detector array. Results presented here include eight preflight and 16 in-flight spectra of eight SEVO sample cells. Spectra from the PAH thin film in a water-vapor-containing microenvironment indicate measurable change due to solar irradiation in orbit, while three other nominally water-free microenvironments show no appreciable change. The quinone anthrarufin showed high photostability and no significant spectroscopically measurable change in any of the four microenvironments during the same period. The SEVO experiment provides the first in situ real-time analysis of the photostability of organic compounds and biomarkers in orbit.
我们报告了搭载在自由飞行的纳米卫星“生物体/有机暴露于轨道应力(O/OREOS)”上的“有机太空环境生存能力(SEVO)”有效载荷的第一批科学成果,该有效载荷于 2011 年 5 月完成了其标称的太空飞行任务,但仍在每两周获取一次数据。SEVO 有效载荷集成了一个紧凑的紫外-可见-近红外分光光度计,利用太阳作为光源,带有一个 24 单元样品旋转架,其中包含四类真空沉积的有机薄膜:多环芳烃(PAH)、氨基酸、金属卟啉和醌。有机薄膜被密封在样品室中,这些样品室包含四种与天体生物学相关的微环境之一。本文报告了任务的前 309 天的结果,在此期间,样品暴露在直接太阳光照下约 2210 小时(在 124-2600nm 范围内约 1080kJ/cm(2)的太阳能)。在每个薄膜上记录了透射光谱(200-1000nm),最初每天记录一次,随后每 15 天记录一次,同时记录太阳光谱和探测器阵列的暗响应。本文介绍的结果包括 8 个预飞行和 16 个飞行中的 8 个 SEVO 样品室的光谱。在含有水蒸气的微环境中的 PAH 薄膜的光谱表明,在轨道上的太阳照射下会发生可测量的变化,而其他三个名义上无水的微环境则没有明显的变化。在相同的四个微环境中,蒽醌蒽醌在任何一个微环境中都表现出很高的光稳定性,并且没有明显的光谱可测量的变化。SEVO 实验首次提供了在轨道上对有机化合物和生物标志物的光稳定性进行实时原位分析的方法。