August 1978
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52 Reads
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1,508 Citations
Physics Today
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... In the framework of relativistic planetary motion, especially in highly eccentric orbits or near relativistic regimes, density gradients or perturbations in the interstellar or circumstellar medium may induce additional drag forces that vary nonlinearly with velocity and spatial position [5,10]. These nonlinear dissipative forces could alter orbital parameters and impact phenomena like the precession of planetary orbits, with corrections beyond classical relativistic predictions [11]. ...
- Citing Article
August 1978
Physics Today