Exact geodetic precession of the orbit of a two-body gyroscope in geodesic motion about a third mass

DOI10.1007/S11038-012-9402-2zbMath1259.83007OpenAlexW2031783106MaRDI QIDQ1936997

G. Renzetti

Publication date: 11 February 2013

Published in: Earth, Moon, and Planets (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1007/s11038-012-9402-2

zbMATH Keywords

celestial mechanicsclassical general relativityrelativity and gravitationexperimental studies of gravitytests of relativistic gravityartificial earth satellites

Mathematics Subject Classification ID

Three-body problems (70F07) Two-body problems (70F05) Observational and experimental questions in relativity and gravitational theory (83B05) Galactic and stellar dynamics (85A05) Equations of motion in general relativity and gravitational theory (83C10)

Related Items (5)

On the stability of the triangular points in the relativistic R3BP with a bigger triaxial primary ⋮ Triangular libration points in the CR3BP with radiation, triaxiality and potential from a belt ⋮ Collinear points in the photogravitational ER3BP with zonal harmonics of the secondary ⋮ Effect of oblateness of an artificial satellite on the orbits around the triangular points of the Earth-Moon system in the axisymmetric ER3BP ⋮ A possible new test of general relativity with Juno

Cites Work

• How accurate is the cancelation of the first even zonal harmonic of the geopotential in the present and future LAGEOS-based Lense-Thirring tests?
• Relativistic effects for near-Earth satellite orbit determination
• Phenomenology of the lense-thirring effect in the solar system
• Gauge Freedom in Orbital Mechanics

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