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相关论文: A new general relativistic contribution to Mercury…

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The effect of general relativistic prediction of the dependence of mass on gravitational potential on the dynamics of a planet moving around the sun is shown to have a negative contribution of 14.326 arcsec/century towards the overall…

天体物理学 · 物理学 2007-05-23 Harihar Behera

C. M. Will in a recent Letter [arXiv:1802.05304] predicts a new Mercury's precession rate which is $100$ times larger than the second-post-Newtonian contribution, our calculation is about $30$ times larger. Thus the new Mercury's precession…

广义相对论与量子宇宙学 · 物理学 2018-05-28 J. Y. Zhou , Z. Li , Q. Li , X. Wang , Q. H. Liu

We numerically and analytically work out the first-order post-Newtonian (1pN) orbital effects induced on the semimajor axis $a$, the eccentricity $e$, the inclination $I$, the longitude of the ascending node $\Omega$, the longitude of…

广义相对论与量子宇宙学 · 物理学 2020-04-27 Lorenzo Iorio

The work is devoted to the critical analysis of theoretical prediction and astronomical observation of GR effects, first of all, the Mercury's perihelion advance. In the first part, the methodological issues of observations are discussed…

综合物理 · 物理学 2010-08-12 Anatoli A. Vankov

A very famous ``test'' of the General Theory of Relativity (GTR) is the advance of Mercury's perihelion (and of other planets too). To be more precise, this is not a prediction of General Relativity, since the anomaly was known in the XIXth…

广义相对论与量子宇宙学 · 物理学 2024-02-08 Bertrand Berche , Ernesto Medina

The perihelion advance of the orbit of Mercury has long been one of the observational cornerstones for testing General Relativity (G.R.). The main goal of this paper is to discuss how, presently, observational and theoretical constraints…

天体物理学 · 物理学 2009-11-07 S. Pireaux , J. P. Rozelot , S. Godier

The Hermean average perihelion rate $\dot\omega^\mathrm{2PN}$, calculated to the second post-Newtonian (2PN) order with the Gauss perturbing equations and the osculating Keplerian orbital elements, ranges from $-18$ to $-4$ microarcseconds…

广义相对论与量子宇宙学 · 物理学 2023-01-05 Lorenzo Iorio

In this paper we represent a different approach to the calculation of the perihelion shift than the one presented in common text books. We do not rely on the Schwarzschild metric and the Hamilton Jacobi technique to obtain our results.…

综合物理 · 物理学 2022-05-09 Asher Yahalom

The motion of Mercury using numerical methods in the framework of a model including only the non-relativistic Newtonian gravitational interactions of the solar system, 9 planets in translation (including Pluto) around the sun has been…

地球与行星天体物理 · 物理学 2022-09-26 Souren P. Pogossian

The theory of General Relativity explaines the advance of Mercury perihelion using space curvature and the Schwartzschild metric. We demonstrate that this phenomena can also be interpreted due to the cogravitational field produced by the…

广义相对论与量子宇宙学 · 物理学 2007-05-23 Clovis Jacinto de Matos , Martin Tajmar

The theory of General Relativity explaines the advance of Mercury perihelion using space curvature and the Schwartzschild metric. We demonstrate that this phenomena can also be interpreted due to the cogravitational field produced by the…

广义相对论与量子宇宙学 · 物理学 2017-08-23 C. J. de Matos , M. Tajmar

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…

空间物理 · 物理学 2018-11-07 Giulia Schettino , Daniele Serra , Giacomo Tommei , Andrea Milani

Recently, Will calculated an additional contribution to the Mercury's precession of the longitude of perihelion $\varpi$ of the order of $\dot\varpi_\textrm{W}\simeq 0.22$ $\textrm{milliarcseconds per century}$ ($\textrm{mas cty}^{-1}$). It…

广义相对论与量子宇宙学 · 物理学 2022-12-15 Lorenzo Iorio

We present a new simple relativistic model for planetary motion describing accurately the anomalous precession of the perihelion of Mercury and its origin. The model is based on transforming Newton's classical equation for planetary motion…

综合物理 · 物理学 2016-03-09 Y. Friedman , J. M. Steiner

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…

广义相对论与量子宇宙学 · 物理学 2020-07-08 Giulia Schettino , Daniele Serra , Giacomo Tommei , Vincenzo di Pierri

We investigate the relativistic modeling of spacecraft motion in Mercury's post-Newtonian local coordinates. This investigation is motivated by the fact that Mercury's post-Newtonian gravitational field (as well as that of any other planet)…

广义相对论与量子宇宙学 · 物理学 2026-02-10 Miriam Falletta , Gabriel Rodríguez-Moris , Sergei A. Klioner

The radioscience experiment is one of the on board experiment of the Mercury ESA mission BepiColombo that will be launched in 2014. The goals of the experiment are to determine the gravity field of Mercury and its rotation state, to…

广义相对论与量子宇宙学 · 物理学 2015-05-14 G. Tommei , A. Milani , D. Vokrouhlicky

Let $r(\varphi)$ denote the orbit of Mercury. We compare the formulae obtained via general relativity for $r(\varphi)$ and for the corresponding perihelion precession angle $\Delta \varphi$, with the formulae obtained via the relativistic…

综合物理 · 物理学 2016-08-15 Athanassios S. Fokas , Constantinos G. Vayenas , D. Grigoriou

Gravitational Thomas Precession (GTP) is the name given to Thomas Precession when the acceleration is caused by a gravitational force field. The GTP gives a negative contribution of 7.163 arcsec/century for the anomalous perihelion advance…

天体物理学 · 物理学 2007-05-23 Harihar Behera

The predicted Lense-Thirring perihelion precession of Mercury induced by the Sun's angular momentum through its general relativistic gravitomagnetic field amounts to 2 milliarcseconds per century. It turned out to be compatible with the…

广义相对论与量子宇宙学 · 物理学 2017-11-28 Lorenzo Iorio
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