Retrograde planetary perihelion precession refers to the phenomenon where the perihelion, or the closest point of an orbiting body to the Sun, shifts direction during its orbit. Typically, perihelion precession occurs in a prograde motion, aligning with the orbit's direction. However, in retrograde perihelion precession, the perihelion moves opposite to the orbit's direction. This concept highlights the complexities of orbital mechanics and gravitational influences. Understanding these motions is essential for comprehending planetary dynamics.