Gravitomagnetism and Lense-Thirring Effect of the Sun and Planets in the Solar System

Jin Wen-jin
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Abstract

The general situation of gravitational experiments in the fundamental physics,especially the progress of measuring the Lense-Thirring effect induced by a test particle orbiting around a central rotating body, such as the Earth, is outlined. The Schiff formula which is a fundamental formula to describe the motion of a particle in the Gravitoelectromagnetic(GEM) field of a central rotating body, is given. Various methods, such as Satellite Laser Ranging(SLR), GP-B, Lunar Laser Ranging(LLR) and Ring Laser Gyroscope(RLG), to measure the Lense-Thirring effect are introduced. Especially, the application in Geophysics with RLG, such as earthquake, tide, earth rotation, polar motion, is presented. The present and future planes to measure the Lense-Thirring effect in high accuracy, such as LARES,OPTIS etc. are introduced. The situation of measuring Lense-Thirring effect of Martian gravitational field with MGS Doppler and range data or observing data of Martian natural satellites, Phobos and Deimos is indicated. The suggestion to lunch Martian mission in the future is also given. The measurement of the Lense-Thirring in Solar Gravitomagnetic field is described with the presently available planetary ranging to Mercury, Venus and Mars.The future plan LATOR to test the general theory of relativity is introduced with the International Space Station(ISS). Finally, The general relativity effect of gravitational field in binary pulsar, X-ray binary and the system of S-stars in infrared band near the Galactic center Sgr A* is briefly introduced. The situation about the experiments to confirm the relativistic theory in China with the tracking and ranging data in the planetary space and some suggestions to develop this work are mentioned.
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太阳和太阳系行星的引力磁力和透镜效应
概述了基础物理学中引力实验的概况,特别是测量由绕中心旋转物体(如地球)运行的测试粒子引起的透镜-蒂林效应的进展。给出了描述粒子在中心旋转体引力电磁场中运动的基本公式——席夫公式。介绍了卫星激光测距(SLR)、GP-B、月球激光测距(LLR)和环形激光陀螺仪(RLG)等测量透镜-三环效应的方法。重点介绍了RLG在地震、潮汐、地球自转、极移等地球物理研究中的应用。介绍了目前和将来用于高精度测量透镜-三环效应的飞机,如LARES、OPTIS等。指出了利用MGS多普勒和火星天然卫星、火卫一和火卫二的距离数据或观测数据测量火星引力场透镜- thirring效应的情况。并对未来的火星任务提出了建议。用目前可用的水星、金星和火星等行星,描述了对太阳引力磁场透镜效应的测量。介绍了用于检验广义相对论的未来计划LATOR与国际空间站(ISS)。最后,简要介绍了银河系中心Sgr A*附近红外波段脉冲星、x射线双星和s星系统引力场的广义相对论效应。介绍了国内利用行星空间跟踪和测距数据验证相对论理论的实验情况,并提出了进一步开展这一工作的建议。
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