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Artykuły w czasopismach na temat "Precession; Mercury; planets"

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Kundu, Jayashree, Rakesh Kumar Mandal, and Tamal Sarkar. "Development of Computational Code to Estimate the Non-Relativistic Contribution to Mercury’s Perihelion Precession." Journal of Physics: Conference Series 2919, no. 1 (2024): 012043. https://doi.org/10.1088/1742-6596/2919/1/012043.

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Abstract The Sun’s gravitational field confines the solar system, our eight known planets, and dwarf planets. This gravitational pull of the Sun and other planets causes Mercury, the nearest planet to the Sun, having the highest orbital precession among all other planets in the Solar system, to follow a new path slightly preces than its normal one. This paper studies Mercury’s orbit by developing an algorithm to determine the nonrelativistic contribution to Mercury’s perihelion precession per century. To create this, we have considered Newton’s Law of Gravitation, Kepler’s Law of Planetary Mot
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Amel’kin, N. I. "The precession of Mercury’s orbit." Доклады Академии наук 489, no. 6 (2019): 570–75. http://dx.doi.org/10.31857/s0869-56524896570-575.

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Within the framework of classical mechanics the influence of the planets in the solar system to the precession of the orbit of Mercury is investigated. It is shown that the average offset of the perihelion of mercurys orbit computed within the flat limited tasks is 556,5 angular seconds per century and coincides with the observation data with relative accuracy of 2,5%. Incomplete overlap between the computed average offset and observations can be explained by the presence in observations offset oscillatory components with a total amplitude up to 20 angular seconds and periods from several year
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Iorio, Lorenzo. "Solar System Motions and the Cosmological Constant:cmd="newline"A New Approach." Advances in Astronomy 2008 (2008): 1–5. http://dx.doi.org/10.1155/2008/268647.

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We use the corrections to the Newton-Einstein secular precessions of the longitudes of perihelia of some planets (Mercury, Earth, Mars, Jupiter, Saturn) of the Solar System, phenomenologically estimated as solve-for parameters by the Russian astronomer E. V. Pitjeva in a global fit of almost one century of data with the EPM2004 ephemerides, in order to put on the test the expression for the perihelion precession induced by a uniform cosmological constant in the framework of the Schwarzschild-de Sitter (or Kottler) space-time. We compare such an extra rate to the estimated corrections to the pl
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Lixin, Yuan. "On the Unification of the Precession of the Foucault Pendulum, the Earth’s “Precession” and the Mercury Precession by Constructing the Vortex Gravitational Mechanism." Applied Science and Innovative Research 6, no. 4 (2022): p21. http://dx.doi.org/10.22158/asir.v6n4p21.

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Gravitation is generated between static objects, while vortex gravity is generated between moving objects. Forming the integrity and completeness of gravity theory, these complement each other. The vortex gravity mechanism of moving objects is established to solve the objective problem of vortex gravity. The precession of Foucault’s pendulum, the precession of the Earth and the precession of Mercury are objective phenomena, for which there are many different explanations. The author suggests, only by the mechanism of vortex gravity can reveal their operation law and unity of operation. Through
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IORIO, L., and M. L. RUGGIERO. "PHENOMENOLOGICAL CONSTRAINTS ON THE KEHAGIAS–SFETSOS SOLUTION IN THE HOŘAVA–LIFSHITZ GRAVITY FROM SOLAR SYSTEM ORBITAL MOTIONS." International Journal of Modern Physics A 25, no. 29 (2010): 5399–408. http://dx.doi.org/10.1142/s0217751x10050780.

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We focus on Hořava–Lifshitz (HL) theory of gravity, and, in particular, on the Kehagias and Sfetsos's solution that is the analog of Schwarzschild black hole of General Relativity. In the weak-field and slow-motion approximation, we analytically work out the secular precession of the longitude of the pericentre ϖ of a test particle induced by this solution. Its analytical form is different from that of the general relativistic Einstein's pericentre precession. Then, we compare it to the latest determinations of the corrections [Formula: see text] to the standard Newtonian/Einsteinian planetary
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Jordán, Andrés, and Gáspár Á. Bakos. "Observability of the General Relativistic Precession of Periastra in Exoplanets." Proceedings of the International Astronomical Union 4, S253 (2008): 492–95. http://dx.doi.org/10.1017/s1743921308027026.

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AbstractThe general relativistic precession rate of periastra in close-in exoplanets can be orders of magnitude larger than the magnitude of the same effect for Mercury. The realization that some of the close-in exoplanets have significant eccentricities raises the possibility that this precession might be detectable. We explore here the observability of the periastra precession using radial velocity and transit light curve observations. Our analysis is independent of the source of precession, which can also have significant contributions due to additional planets and tidal deformations. We fi
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Iorio, Lorenzo. "Frame-Dragging in Extrasolar Circumbinary Planetary Systems." Universe 8, no. 10 (2022): 546. http://dx.doi.org/10.3390/universe8100546.

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Extrasolar circumbinary planets are so called because they orbit two stars instead of just one; to date, an increasing number of such planets have been discovered with a variety of techniques. If the orbital frequency of the hosting stellar pair is much higher than the planetary one, the tight stellar binary can be considered as a matter ring current generating its own post-Newtonian stationary gravitomagnetic field through its orbital angular momentum. It affects the orbital motion of a relatively distant planet with Lense-Thirring-type precessional effects which, under certain circumstances,
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Pashkevich, Vladimir V., and Andrey N. Vershkov. "Geodetic Precession of the Sun, Solar System Planets, and their Satellites." Artificial Satellites 57, no. 1 (2022): 77–109. http://dx.doi.org/10.2478/arsa-2022-0005.

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Abstract The effect of the geodetic precession is the most significant relativistic effect in the rotation of celestial bodies. In this article, the new geodetic precession values for the Sun, the Moon, and the Solar System planets have been improved over the previous version by using more accurate rotational element values. For the first time, the relativistic effect of the geodetic precession for some planetary satellites (J1–J4, S1–S6, S8–S18, U1–U15, N1, and N3–N8) with known quantities of the rotational elements was studied in this research. The calculations of the values of this relativi
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Pashkevich, Vladimir V., and Andrey N. Vershkov. "Geodetic Precession of the Sun, Solar System Planets, and their Satellites." Artificial Satellites 57, no. 1 (2022): 77–109. http://dx.doi.org/10.2478/arsa-2022-0005.

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Abstract The effect of the geodetic precession is the most significant relativistic effect in the rotation of celestial bodies. In this article, the new geodetic precession values for the Sun, the Moon, and the Solar System planets have been improved over the previous version by using more accurate rotational element values. For the first time, the relativistic effect of the geodetic precession for some planetary satellites (J1–J4, S1–S6, S8–S18, U1–U15, N1, and N3–N8) with known quantities of the rotational elements was studied in this research. The calculations of the values of this relativi
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Mozaffari, S. Mohammad. "Holding or Breaking with Ptolemy's Generalization: Considerations about the Motion of the Planetary Apsidal Lines in Medieval Islamic Astronomy." Science in Context 30, no. 1 (2017): 1–32. http://dx.doi.org/10.1017/s0269889717000011.

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ArgumentIn the Almagest, Ptolemy finds that the apogee of Mercury moves progressively at a speed equal to his value for the rate of precession, namely one degree per century, in the tropical reference system of the ecliptic coordinates. He generalizes this to the other planets, so that the motions of the apogees of all five planets are assumed to be equal, while the solar apsidal line is taken to be fixed. In medieval Islamic astronomy, one change in this general proposition took place because of the discovery of the motion of the solar apogee in the ninth century, which gave rise to lengthy d
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Części książek na temat "Precession; Mercury; planets"

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Kundu, Jayashree, Dr Rakesh Kumar Mandal, and Dr Tamal Sarkar. "STUDYING THE PLANETARY MOTION USING PYTHON." In Futuristic Trends in Computing Technologies and Data Sciences Volume 3 Book 9. Iterative International Publisher, Selfypage Developers Pvt Ltd, 2024. http://dx.doi.org/10.58532/v3bgct9p4ch2.

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In the present work, we have studied the motion of planet and the dwarf planet and estimated the value of Mass of the Sun and value of Gravitational Constant (in case of dwarf planet). We also have studied the non-relativistic contribution of Mercury’s perihelion precession. For the purpose of the same, we have considered the paper by Price and Rush, the freely available NASA data from NASA website as well as freely available data in Wikipedia website. For computational modeling purpose, we have used the Python programming language.
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"3: Slower than Light: The Precession of the Perihelion of the Planet Mercury." In Mathematical Models and Their Analysis. Society for Industrial and Applied Mathematics, 2018. http://dx.doi.org/10.1137/1.9781611975277.ch3.

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DUBOIS, DANIEL M. "Deduction of the Relativistic Newton Law of Gravitation Based on Anticipation and Retardation and Simulation of the Precession of Mercury Planet with Incursive Algorithm." In Fundamental Physics at the Vigier Centenary. WORLD SCIENTIFIC, 2021. http://dx.doi.org/10.1142/9789811246463_0004.

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