Orbit averaging techniques are used to develop analytical approximations of circle-to-circle low-thrust trajectory transfers with plane-change about the Sun. Separate expressions are developed for constant acceleration, or thrust, electric propulsion, solar sail propulsion and combined, or hybrid electric (constant acceleration or thrust) / solar sail propulsion. The analytical expressions uniquely allow the structure of circle-to-circle low-thrust trajectory transfers with plane-change about the Sun to be understood, and the optimal trajectory structure is analytically derived for each propulsion system considered. It is found that the optimal fixed thrust electric propulsion transfer reduces the orbit radius with no plane change and then performs the plane-change, while the optimal solar sail and hybrid transfers combine the reduction of orbit radius with some plane change, before then completing the plane change. The optimal level of plane change during the reduction of orbit radius is derived and it is found the analytically-derived minimum time solar sail transfer is within 1% of the numerically-derived optimal transfer. It is also found that, under the conditions considered, a sail characteristic acceleration of less than 0.5 mm/s2 can, in 5-years, attain a solar orbit that maintains the observer-to-solar pole zenith angle below 40 degrees for 25 days; the approximate sidereal rotation period of the Sun. However, a sail characteristic acceleration of more than 0.5 mm/s2 is required to attain an observer-to-solar pole zenith angle below 30 degrees for 25 days within 5-years of launch. Finally, it was found that the hybridization of electric propulsion and solar sail propulsion was, typically, of more benefit when the system was thrust constrained than when it was mass constrained.
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机译:轨道平均技术被用来发展围绕太阳的平面变化的圆到圆低推力轨迹转移的解析近似。分别为恒定加速度或推力,电力推进,太阳帆推进和组合或混合电动(恒定加速度或推力)/太阳帆推进建立了单独的表达式。解析表达式独特地允许理解围绕太阳的平面变化的圆到圆低推力轨迹转移的结构,并且针对所考虑的每个推进系统通过解析得出最佳轨迹结构。发现最佳的固定推力电推进传递在没有平面变化的情况下减小了轨道半径,然后进行了平面改变,而最佳的太阳帆和混合动力传递结合了在一定平面变化下的轨道半径的减小,然后完成了换飞机。推导了减小轨道半径过程中平面变化的最佳水平,发现解析得出的最小时间太阳帆转移量在数值衍生的最佳转移量的1%以内。还发现,在所考虑的条件下,帆特征加速度小于0.5 mm / s2可以在5年内获得一个太阳轨道,该轨道将观察者与太阳的极顶角保持在40度以下25天;太阳的近似恒星自转周期。但是,要在发射后的5年内达到25天的观察者与太阳的极顶角在30度以下,就需要大于0.5 mm / s2的风帆特性加速度。最后,人们发现,当系统受到推力约束时,电动推进与太阳帆推进的混合通常比受质量约束时更有利。
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