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Cometary activity model for near nucleus space flight dynamics analysis

机译:用于近核空间飞行动力学分析的彗星活动模型

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To analyze the spacecraft motion near a comet nucleus surface,an approximated model of the cometary activity has been developed.Short-periodic comet,heliocentric distance up to 5 AU,cometary nucleus radius ranging between 0.5km and 10km and cometocentric distances up to 100 Km are considered.There are determinde the mass gas and dust production rates as well as the gas and dust velocities.The comparison with astronomical observations and laboratory experiment data as well as some more sophisticated models is performed and has given a satisfactory agreement.This model has been implemented into the ROSETTA Near Comet Operation Simulator has been developed by GMV under ESA contract for analysis of orbit planning and navigation of all the near comet phases for the future ROSETTA mission results on the effect of gas,dust and jets activity on the spacecraft flight dynamics,orbit detemination and cometary parameters estimation in the vicinity of the comet nucleus.
机译:为了分析航天器在彗核表面附近的运动,开发了一个近似的彗星活动模型。短周期彗星,其中心距离最大为5 AU,彗核半径范围为0.5km至10km,彗中心距离最大为100 Km确定了气体和粉尘的生产率以及气体和粉尘的速度。与天文观测和实验室实验数据以及一些更复杂的模型进行了比较,并给出了令人满意的协议。已由GMV根据欧洲航天局(ESA)合同开发了ROSETTA近彗星运行模拟器,用于分析轨道规划和所有近彗星阶段的导航,以用于未来ROSETTA任务结果对气体,粉尘和喷气流活动对航天器飞行的影响彗核附近的动力学,轨道确定和彗星参数估计。

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