Test of Lense-Thirring orbital shift due to spin

被引:55
作者
Ciufolini, I
Chieppa, F
Lucchesi, D
Vespe, F
机构
[1] UNIV ROMA LA SAPIENZA,DIP AEROSPAZIALE,I-00184 ROME,ITALY
[2] UNIV ROMA LA SAPIENZA,SCUOLA ING AEROSPAZIALE,I-00184 ROME,ITALY
[3] UNIV PISA,DIPARTIMENTO MATEMAT,I-56127 PISA,ITALY
[4] ASI,CGS,I-75100 MATERA,ITALY
关键词
D O I
10.1088/0264-9381/14/10/003
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The Lense-Thirring effect is a very small shift of the orbit of a test particle due to the spin of a body. It may be described as al orbital drag due to the gravitomagnetic field generated by the spin of the central body. Gravitomagnetism, a fundamental weak-field prediction of Einstein's theory of general relativity, is generated by currents of mass and owes its name to its formal analogies with magnetism, generated by currents of electric charge. Then, according to general relativity, the Earth's spin should influence the motion of its orbiting satellites. Indeed, we have analysed the laser-ranging observations of the orbits of the satellites LAGEOS and LAGEOS II and have obtained the first direct measurement of the Lense-Thirring effect, or 'frame-dragging', due to the Earth's spin. We measured mu(Lense-Thirring) congruent to 1.1 and estimated the total error delta mu(Lense-Thirring) congruent to +/-0.3, whereas the general relativistic value is mu(Lense-Thirring) = 1.
引用
收藏
页码:2701 / 2726
页数:26
相关论文
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