  At least $70\%$ of massive OBA-type stars reside in binary or higher-order
systems. The dynamical evolution of these systems can lend insight into the
origins of extreme phenomena such as X-ray binaries and gravitational wave
sources. In one such dynamical process, the Eccentric Kozai-Lidov (EKL)
Mechanism, a third companion star alters the secular evolution of a binary
system. For dynamical stability, these triple systems must have a hierarchical
configuration. We explore the effects of a distant third companion's
gravitational perturbations on a massive binary's orbital configuration before
significant stellar evolution has taken place ($\leq 10$ Myr). We include tidal
dissipation and general relativistic precession. With large ($38,000$ total)
Monte-Carlo realizations of massive hierarchical triples, we characterize
imprints of the birth conditions on the final orbital distributions.
Specifically, we find that the final eccentricity distribution over the range
$0.1-0.7$ is an excellent indicator of its birth distribution. Furthermore, we
find that the period distributions have a similar mapping for wide orbits.
Finally, we demonstrate that the observed period distribution for approximately
$10$ Myr-old massive stars is consistent with EKL evolution.
