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LETSGO: A spacecraft-based mission to accurately measure the solar angular momentum with frame-dragging

机译:LETSGO:一项基于航天器的任务,可通过拖动框架来精确测量太阳角动量

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摘要

LETSGO (LEnse-Thirring Sun-Geo Orbiter) is a proposed space-based mission involving the use of a spacecraft moving along a highly eccentric heliocentric orbit perpendicular to the ecliptic. It aims to accurately measure some important physical properties of the Sun and to test some post-Newtonian features of its gravitational field by continuously monitoring the Earth-probe range. Preliminary sensitivity analyses show that, by assuming a cm-level accuracy in ranging to the spacecraft, it would be possible to test, in principle, the Lense-Thirring effect at a ~ 10~(-2) level over a timescale of 2 years, while the larger Schwarzschild component of the solar gravitational field may be sensed with a relative accuracy of about 10~(-8)-10~(-9) during the same temporal interval. The competing range perturbation due to the non-sphericity of the Sun would be a source of systematic error, but it turns out that all the three dynamical features of motion examined affect the Earth-probe range in different ways, allowing for separating them in real data analyses. The high eccentricity would help in reducing the impact of the non-gravitational perturbations whose disturb would certainly be severe when LETSGO would approach the Sun at just a few solar radii. It can be preliminarily argued that a drag-free apparatus should perform at a 10~(-8)-10~(-9) ms~(-2) Hz~(-1/2)2 level for frequencies of about 10~(-7) Hz. Further studies should be devoted to investigate both the consequences of the non-conservative forces and the actual measurability of the effects of interest by means of extensive numerical data simulations, parameter estimations and covariance analyses. Also an alternative, fly-by configuration is worth of consideration.
机译:LETSGO(低空引力太阳-地球轨道飞行器)是一项拟议的太空任务,涉及使用航天器沿着垂直于黄道的高度偏心日心轨道运动。它旨在通过连续监测地球探测范围,来精确测量太阳的一些重要物理性质,并测试其牛顿后引力场的某些特征。初步的灵敏度分析表明,通过假设在厘米范围内的航天器精度,原则上可以在2年的时间范围内以〜10〜(-2)的水平测试Lense-Thirring效应。 ,而在相同的时间间隔内,可以以大约10〜(-8)-10〜(-9)的相对精度感测太阳重力场的较大Schwarzschild分量。由于太阳的非球形性引起的竞争范围摄动是系统误差的来源,但事实证明,所检查运动的所有三个动力学特征均以不同方式影响地球探测范围,从而可以将它们实际分离。数据分析。高偏心率将有助于减少非引力扰动的影响,当LETSGO仅以几个太阳半径接近太阳时,其干扰肯定会很严重。可以初步认为,无拖曳装置应在10〜(-8)-10〜(-9)ms〜(-2)Hz〜(-1/2)2的频率下工作,频率约为10〜 (-7)赫兹。应通过大量的数值数据模拟,参数估计和协方差分析,进一步研究非保守力的结果和感兴趣效应的实际可测量性。另外一种替代的飞越配置也值得考虑。

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