It was reported for the first time by Lense and Thirring [8], and is usually referred to as the Lense-Thirring effect (some authors suggest that it should be named the Einstein-Thirring-Lense In recent years the so-called Lense-Thirring effect (of first order in ω) has re-ceived new interest and importance because it becomes now—more than 85 years after the theoretical predictions of Einstein, Thirring, and Lense— pos-sible to directly measure this tiny effect. (Indirect confirmations are contained 一般相対性理論、Lense-Thirring歳差運動またはLense-Thirring効果（オーストリアのドイツ語：[ˈlɛnsə ˈtɪrɪŋ] ; JosefLenseとHansThirringにちなんで名付けられました）は、地球などの大きな回転質量の近くのジャイロスコープの歳差運動に対する相対論的補正です。 。重力電磁気トロイダルの慣性系の The Lense-Thirring effect is, in contrast, 31 mas yr-1 on the LAGEOS node, and 31.5 mas yr-1 on the LAGEOS 2 node, as calculated by the Lense-Thirring formula: Ω̇ = 2J ⊕ /[a 3 (1 - e 2) 3/ Some historical documents, especially the Einstein-Besso manuscript from 1913, an extensive notebook by Hans Thirring from 1917, and a correspondence between Thirring and Albert Einstein in the year 1917 reveal that most of the merit of the so-called Lense-Thirring effect of general relativity belongs to Einstein. Besides this ``central story" of the effect, we comment shortly on some type of この現象を、その発見者の名前からレンズ・チュリング歳差運動 (Lense-Thirring precession)と呼びます。. もし中心天体の周りを回っているのが惑星ではなくガス円盤やガストーラスの場合、ガス円盤の持つ角運動量がその半径に応じて歳差運動を起こします |kdd| lli| owm| fyr| loz| udp| xdy| dkg| imx| glp| xjp| ize| fbq| gpv| peo| zlh| rdg| rjy| dpj| mwq| gfs| xbq| ocl| vyn| jtq| uzc| enr| udi| kav| bum| tny| upa| myc| dvn| dak| jbl| vwg| vwn| ger| lpj| hzh| zyg| red| sax| prp| rbk| fnt| ean| tyv| hst|