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The SCITEAS experiment: Optical characterizations of sublimating icy planetary analogues

机译:SCITEAS实验:升华的冰冷行星类似物的光学表征

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We have designed and built a laboratory facility to investigate the spectro-photometric and morphologic properties of different types of ice-bearing planetary surface analogs and follow their evolution upon exposure to a low pressure and low temperature environment. The results obtained with this experiment are used to verify and improve our interpretations of current optical remote-sensing datasets. They also provide valuable information for the development and operation of future optical instruments. The Simulation Chamber for Imaging the Temporal Evolution of Analogue Samples (SCITEAS) is a small thermal vacuum chamber equipped with a variety of ports and feedthroughs that permit both in-situ and remote characterizations as well as interacting with the sample. A large quartz window located directly above the sample is used to observe its surface from outside with a set of visible and near-infrared cameras. The sample holder can be easily and quickly inserted and removed from the chamber and is compatible with the other measurement facilities of the Laboratory for Outflow Studies of Sublimating Materials (LOSSy) at the University of Bern. We report here on the results of two of the first experiments performed in the SCITEAS chamber. In the first experiment, fine-grained water ice mixed with dark organic and mineral matter was left to sublime in vacuum and at low temperature, simulating the evolution of the surface of a comet nucleus approaching the Sun. We observed and characterized the formation and evolution of a crust of refractory organic and mineral matter at the surface of the sample and linked the evolution of its structure and texture to its spectro-photometric properties. In the second experiment, a frozen soil was prepared by freezing a mixture of smectite mineral and water. The sample was then left to sublime for 6 h to simulate the loss of volatiles from icy soil at high latitudes on Mars. Colour images were produced using the definitions of the filters foreseen for the CaSSIS imager of the Exomars/TGO mission in order to prepare future science operations. (C) 2015 Elsevier Ltd. All rights reserved.
机译:我们已经设计并建造了一个实验室设施,以研究不同类型的含冰行星表面类似物的分光光度和形态学特性,并在暴露于低压和低温环境时跟踪其演变。通过本实验获得的结果用于验证和改进我们对当前光学遥感数据集的解释。它们还为未来光学仪器的开发和操作提供了有价值的信息。用于对模拟样品的时间演变进行成像的模拟腔室(SCITEAS)是一个小型热真空腔室,配备了多种端口和馈通孔,可进行原位和远程表征以及与样品的相互作用。位于样品正上方的大石英窗用于通过一组可见和近红外摄像机从外部观察其表面。样品架可以轻松,快速地从反应室中插入和取出,并且与伯尔尼大学升华材料流出研究实验室(LOSSy)的其他测量设备兼容。我们在这里报告在SCITEAS室内进行的两个首次实验的结果。在第一个实验中,将掺有深色有机物和矿物质的细粒水冰在真空和低温下升华,以模拟接近太阳的彗核表面的演化。我们观察并表征了样品表面难熔有机物和矿物物质结皮的形成和演化,并将其结构和织构的演化与其分光光度特性联系起来。在第二个实验中,通过冷冻蒙脱石矿物和水的混合物来制备冷冻土壤。然后将样品升华6小时,以模拟在火星上高纬度的冰冷土壤中挥发物的损失。使用为Exomars / TGO任务的CaSSIS成像仪预见的滤镜定义,可以生成彩色图像,以准备将来的科学操作。 (C)2015 Elsevier Ltd.保留所有权利。

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