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The Gamma Astrometric Measurement Experiment (GAME)

机译:伽玛占星术测量实验(GAME)

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The GAME mission concept is aimed at the very precise measurement of the gravitational deflection of light by the Sun, by means of an optimised telescope operating in the visible and launched in orbit on a small class satellite. The targeted precision on the 7 parameter of the Parametrized Post-Newtonian formulation of General Relativity is 10~(-6) or better, i.e. one to two orders of magnitude better than the best currently available results. Such precision is suitable to detect possible deviations from the unity value, associated to generalized Einstein models for gravitation, with potentially huge impacts on the cosmological distribution of dark matter and dark energy. The measurement principle is based on the differential astrometric signature on the stellar positions, i.e., based on the spatial component of the effect rather than the temporal component as in the most recent experiments using radio link delay timing. Exploiting the possibilities offered by the observation strategy, it is also possible to target other interesting scientific goals both in the realm of General Relativity and in the observations of extrasolar systems. The instrument concept is based on a dual field, multiple aperture Fizeau interferometer, observing simultaneously two regions close to the Solar limb. The diluted optics approach is selected for achieving an efficient rejection of the diffracted and scattered solar radiation, while retaining an acceptable angular resolution on the science targets. The baseline design approach aims at minimization of the development criticality, whereas performance optimization may benefit from state of the art technologies e.g. active and lightweight optics. An internal metrology option is considered. We describe the science motivation, the proposed mission profile, the payload concept and the expected performance from recent results.
机译:GAME任务概念旨在通过优化的望远镜在可见光中运行并在小型卫星上进行轨道发射,来非常精确地测量太阳的引力偏转。广义相对论的参数化后牛顿公式的7参数的目标精度为10〜(-6)或更高,即比目前可获得的最佳结果好一到两个数量级。这样的精度适合于检测与统一的爱因斯坦引力模型相关的单位值的可能偏差,这可能会对暗物质和暗能量的宇宙学分布产生巨大影响。测量原理基于恒星位置上的差分天文签名,即基于效果的空间成分,而不是像使用无线电链路延迟定时的最新实验中那样基于时间成分。利用观测策略提供的可能性,在广义相对论领域和太阳系外观测中也可以瞄准其他有趣的科学目标。该仪器的概念基于双场,多孔径Fizeau干涉仪,可同时观察到靠近太阳肢体的两个区域。选择稀释光学方法可有效抑制衍射和散射的太阳辐射,同时在科学目标上保持可接受的角分辨率。基线设计方法旨在最小化开发的关键性,而性能优化则可以受益于最新的技术,例如主动和轻巧的光学元件。考虑内部计量选项。我们描述了科学动机,拟议的任务概况,有效载荷概念以及最新成果的预期性能。

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