In 1772, astronomer Joseph-Louis Lagrange discovered the namesake “Lagrangian” or libration points, which are points where a small body could orbit in a constant pattern with two larger masses (specifically, a satellite in respect to the Earth and Moon). Of these points, the Trojan points, L4 on the eastern horizon, and L5 on the western, are of special significance to future space endeavors. In the Trojan points, the contending gravitational tugs of the Earth and the moon offer exactly the right amount of centripetal force in these locations for an object to essentially “park” there and stay in place within the Earth-moon system. Artificial objects, or even habitats, could be inserted into these locations where they would be locked into place by gravity and become a permanent part of the Earth-moon system. These would offer locations closer than the Moon, and act as possible bases for future space exploration; they are potential stepping stones across the cosmic pond.