论文标题
重力理论的测试，包括与Bepicolombo无线电科学实验的扭转
A test of gravitational theories including torsion with the BepiColombo radio science experiment
论文作者
论文摘要
The Mercury Orbiter radio Science Experiment (MORE) is one of the experiments on-board the ESA/JAXA BepiColombo mission to Mercury, to be launched in October 2018. Thanks to full on-board and on-ground instrumentation performing very precise tracking from the Earth, MORE will have the chance to determine with very high accuracy the Mercury-centric orbit of the spacecraft and the heliocentric orbit of Mercury.这将允许对引力的相对论理论（相对论实验）进行准确的检验，该理论包括提高一些牛顿后和相关参数的知识，其价值是通过一般相对性预测的。本文重点介绍了Bepicolombo相对性实验的两个关键方面。首先，我们以实验目的确定汞和泥土男气味的轨道的精致问题，并讨论了一种解决问题中出现的等级缺陷的策略。其次，我们介绍并讨论了太阳能透射效应在汞轨道确定问题以及相对论参数估计中的作用。
The Mercury Orbiter radio Science Experiment (MORE) is one of the experiments on-board the ESA/JAXA BepiColombo mission to Mercury, to be launched in October 2018. Thanks to full on-board and on-ground instrumentation performing very precise tracking from the Earth, MORE will have the chance to determine with very high accuracy the Mercury-centric orbit of the spacecraft and the heliocentric orbit of Mercury. This will allow to undertake an accurate test of relativistic theories of gravitation (relativity experiment), which consists in improving the knowledge of some post-Newtonian and related parameters, whose value is predicted by General Relativity. This paper focuses on two critical aspects of the BepiColombo relativity experiment. First of all, we address the delicate issue of determining the orbits of Mercury and the Earth-Moon barycenter at the level of accuracy required by the purposes of the experiment and we discuss a strategy to cure the rank deficiencies that appear in the problem. Secondly, we introduce and discuss the role of the solar Lense-Thirring effect in the Mercury orbit determination problem and in the relativistic parameters estimation.
