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ORBITAL DYNAMICS OF A SOLAR SAIL ACCELERATED BY THERMAL DESORPTION OF COATINGS

机译:涂层热脱附加速了太阳帆的轨道动力学

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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 [1]. Thermal desorption is a physical process of mass loss which dominates all other similar processes and it can provide additional thrust as heating liberates atoms, embedded on the surface of a solar sail [2]. In this study we considered 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. Three different scenarios, that only differ in the way the sail approaches the Sun, were analyzed and compared. In every case 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. Thermal desorption here comes as an additional source of solar sail acceleration beside traditional propulsion systems for extrasolar space exploration. The compared scenarios are the following: i. 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 an Hohmann transfer from Earth's orbit to an orbit very close to the Sun (almost at 0.1 AU) and then be deployed there, ii. Elliptical transfer plus Slingshot plus thermal desorption. In this scenario the transfer occurs from Earth's orbit to Jupiter's orbit. A Jupiter's fly-by leads to the orbit close to the Sun, where the sail is deployed, iii. Two stage acceleration of the solar sail through thermal desorption. The proposed sail has two coats of the materials that undergo thermal desorption at different temperatures depending on the heliocentric distance. The first desorption occurs at the Earth orbit and provides the thrust needed to propel the solar sail toward the Sun. The second desorption is equivalent to that of the other scenarios.
机译:对于太阳外太空探索,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进行热解吸的材料所覆盖的太阳帆可能是非常方便的[1]。热脱附是质量损失的物理过程,在所有其他类似过程中占主导地位,并且当加热释放嵌入太阳帆表面的原子时,它可以提供额外的推力[2]。在这项研究中,我们考虑了一种太阳帆,该太阳帆上涂有在特定温度下会发生热脱附的材料,这是由于太阳辐射在特定的日心距上进行加热而导致的。分析和比较了三种不同的情况,仅在帆接近太阳的方式不同。在每种情况下,一旦到达近日点,帆罩都会发生热脱附。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。除了传统的推进系统用于太阳系外太空探索外,这里的热脱附是太阳帆加速的另一种来源。比较的方案如下:霍曼转移加热脱附。在这种情况下,帆将通过霍曼从地球轨道转移到非常接近太阳(几乎为0.1 AU)的轨道,作为常规推进系统的载荷,被运送到近日点,然后ii。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。木星的飞越通向靠近太阳的轨道,帆在此展开。iii。太阳帆通过热解吸的两阶段加速。所提出的帆具有两层材料,这些涂层根据日心距而在不同温度下进行热脱附。第一次解吸发生在地球轨道上,并提供了将太阳帆推向太阳所需的推力。第二次解吸等效于其他方案。

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