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Laboratory Simulation of Sublimating Planetary Surface Ices: Experiment Design and Thermal Considerations

机译:升华行星表面夹具的实验室模拟:实验设计和热考虑因素

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We have developed a laboratory experiment to simulate ice surface environmental conditions on Europa and other icy worlds. The project studies the possible formation of ice penitentes in a vacuum environment, while controlling background pressure, ice and wall temperatures, ice chemical compositions, and incident photon flux. The experiment consists of two separate apparatus: a static testbed in which illumination conditions remain fixed, and a diurnal testbed in which a motorized linear stage sweeps a solar simulator source across the ice surface to simulate diurnal variations. The static testbed primarily serves as a platform for short-term tests at temperatures from 200K to 273K with moderate vacuum (10 Pa to atmospheric), while the diurnal testbed can achieve cryogenic temperatures down to 80K and a vacuum of 1x10-4 Pa. Preliminary results show the formation of sublimation- driven ice structures at Earth-like temperatures and moderate vacuum conditions close to the equilibrium vapor pressure curve for pure water.
机译:我们开发了一个实验室实验,以模拟欧罗巴和其他冰冷世界的冰面环境条件。该项目在真空环境中研究了冰畸形的可能形成,同时控制背景压力,冰和墙面温度,冰化学成分和事件光子通量。该实验由两个单独的装置组成:静态试验台,其中照明条件保持固定,并且在冰面上扫过太阳能模拟器源的昼夜试验台,以模拟落地变化。静态试验台主要用作从200k到273k的温度下的短期试验平台,中等真空(10Pa至大气),而日本试验台可以使低温温度降至80k和1x10-4 pa的真空。初步结果表明,在接地温度下升华驱动的冰结构的形成,靠近纯水的平衡蒸气压力曲线的适度真空条件。

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