The NRC Astrophysics Decadal Survey identified Cosmic Dawn (i.e., first stars and first light in the Universe) as one of the top science priorities for this decade. The NLSI LUNAR team has shown that such observations are best conducted from the radio-quiet lunar farside using an array of low radio frequency telescopes to measure redshifted 21-cm signals from neutral hydrogen that surround the first stars and galaxies. We have developed a concept for a deployable low-mass radio antenna array on the Moon using polyimide film as a backbone. Our team has proposed that such an array could be deployed with a modest rover on the lunar farside teleoperated by astronauts in the Orion crew vehicle stationed in orbit about the EM L-2 libration point. To demonstrate the feasibility for such a mission, we have recently conducted the first surface telerobotics engineering tests using the K-10 rover at the NASA Ames Roverscape under the command of an astronaut aboard the ISS. During the 3.5-hr ISS crew session, two “arms” of polyimide film were successfully unrolled from the back of the K-10 rover. This test session achieved a number of “firsts” including the first real-time teleoperation of a planetary rover from the ISS, the first astronaut to interactively control a high fidelity planetary rover in an outdoor analog testbest, and the first realistic simulation of a human-robot “Waypoint” mission concept.