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Extrasolar space exploration by a solar sail accelerated via thermal desorption of coating

机译:通过涂层热解吸加速太阳帆进行太阳系外太空探索

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For extrasolar space exploration it might be very convenient to take advantage of space environmental effects such as solar radiation heating to accelerate a solar sail coated by materials that undergo thermal desorption at a particular temperature. Thermal desorption can provide additional thrust as heating liberates atoms, embedded on the surface of the solar sail. We are considering orbital dynamics of a solar sail coated with materials that undergo thermal desorption at a specific temperature, as a result of heating by solar radiation at a particular heliocentric distance, and focus on two scenarios that only differ in the way the sail approaches the Sun. For each scenario once the perihelion is reached, the sail coat undergoes thermal desorption. When the desorption process ends, the sail then escapes the Solar System having the conventional acceleration due to solar radiation pressure. We study the dependence of a cruise speed of a solar sail on perihelion of the orbit where the solar sail is deployed. The following scenarios are considered and analyzed: (1) Hohmann transfer plus thermal desorption. In this scenario the sail would be carried as a payload to the perihelion with a conventional propulsion system by a Hohmann transfer from Earth's orbit to an orbit very close to the Sun and then be deployed. Our calculations show that the cruise speed of the solar sail varies from 173 km/s to 325 km/s that corresponds to perihelion 0.3 AU and 0.1 AU, respectively. (2) Elliptical transfer plus Slingshot plus thermal desorption. In this scenario the transfer occurs from Earth's orbit to Jupiter's orbit; then a Jupiter's fly-by leads to the orbit close to the Sun, where the sail is deployed and thermal desorption comes active. In this case the cruise speed of the solar sail varies from 187 km/s to 331 km/s depending on the perihelion of the orbit. Our study analyses and compares the different scenarios in which thermal desorption comes beside traditional propulsion systems for extrasolar space exploration. (C) 2018 COSPAR. Published by Elsevier Ltd. All rights reserved.
机译:对于太阳系外太空探索,利用空间环境效应(例如太阳辐射加热)来加速由在特定温度下经历热解吸作用的材料覆盖的太阳帆可能会非常方便。当加热释放嵌入太阳帆表面的原子时,热解吸可以提供额外的推力。我们正在考虑涂有在特定温度下发生热解吸的材料的太阳帆的轨道动力学,这是由于太阳辐射在特定的日心中心距离上加热而导致的结果,因此我们着重研究了两种情况,它们仅在帆接近太阳的方式不同。太阳。对于每种情况,一旦到达近日点,帆罩都会经历热脱附。当解吸过程结束时,帆由于太阳辐射压力而逃逸出具有常规加速度的太阳系。我们研究了太阳帆的巡航速度对太阳帆所在轨道近日点的依赖。考虑并分析了以下情形:(1)霍曼转移加热解吸。在这种情况下,帆将通过霍曼从地球轨道转移到非常靠近太阳的轨道作为常规推进系统,作为有效载荷运送到近日点。我们的计算表明,太阳帆的巡航速度从173 km / s变为325 km / s,分别对应于近日点0.3 AU和0.1 AU。 (2)椭圆转移加弹弓加热脱附。在这种情况下,转移发生从地球轨道到木星轨道。然后木星飞越到靠近太阳的轨道,在那里展开帆并开始热解吸。在这种情况下,取决于轨道的近日点,太阳帆的巡航速度从187 km / s到331 km / s不等。我们的研究分析和比较了热解吸与传统推进系统一起用于太阳系外太空探索的不同情形。 (C)2018年COSPAR。由Elsevier Ltd.出版。保留所有权利。

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