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Determining the amplitude of Mercury's long period librations with the BepiColombo radio science experiment

机译:用Bepicolombo无线电科学实验确定水星长期守恒的幅度

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The Mercury Orbiter Radio science Experiment (MORE) is one of the experiments on-board the ESA/JAXA BepiColombo mission to Mercury. A crucial goal of MORE is to determine the gravity field and rotational state of Mercury in order to enable a better understanding of the planet's geophysics. The authors have recently reported on the results of a set of simulations of the MORE gravimetry and rotation experiments, carried out with the dedicated ORBIT14 software. Since that time, the launch date has been postponed twice, leading to a shift of more than one year in the orbital phase of the mission. Actually, the updated schedule results in a more suitable planetary configuration to determine the amplitude of the forced librations in longitude induced by Jupiter. In fact, the amplitude can be considerably enhanced due to a near-resonance with the free librations period, a key parameter to constrain the interior structure of Mercury. We show that the newest launch date allows the measurement of the long period librations amplitude forced by Jupiter with an accuracy of some tenth of arcseconds, a significant improvement with respect to the results with the previous mission schedule.
机译:汞轨道机器无线电科学实验(更多)是欧安全盟/雅加贝斯科罗博士的实验之一。最重要的目标是确定汞的重力场和旋转状态,以便更好地了解地球的地球物理。最近提交的作者报告了通过专用轨道14软件进行的更多重量和旋转实验的模拟的结果。从那时起,发布日期已经推迟了两次,导致任务轨道阶段超过一年的转变。实际上,更新的时间表导致更合适的行星结构,以确定Jupiter引起的经度的迫使缩放的幅度。事实上,由于与自由衰减期近共振,可以显着提高幅度,以限制汞的内部结构的关键参数。我们表明最新的发布日期允许测量Jupiter迫使Jupiter的长期幅度,精度为第十附庸的十分之一,对于使用以前的任务时间表的结果有显着改进。

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