2026-07-072026-07-07http://salesiana.dossiersoluciones.com/handle/123456789/111170In this paper, we discuss the internal and external metric of the semi-realistic stars in relativistic MOND theory. We show the Oppenheimer-Volkoff equation in relativistic MOND theory and get the metric and pressure inside the stars to order of post-Newtonian corrections. We study the features of motion around the static, spherically symmetric stars by Hamilton-Jacobi mothod, and find there are only some small corrections in relativistic MOND theory.10 pages, no figureGeneral Relativity and Quantum Cosmologytext