4800 Oak Grove Drive
M/S 169-506
Dr. Turner's research centers on the origins of the planets in the disks of gas and dust orbiting young stars. He uses computer calculations to model the gas flows in the disks, the heating and chemical evolution of the primordial materials, and the concentration of the dust particles leading to the growth of larger solid bodies. He calculates the models' appearance through radiative transfer methods and uses the results to understand the measurements of protostellar disks and planetary systems returned by space telescopes and by interplanetary probes sent to our own solar system's planets, moons, asteroids, and comets, as well as in creating proposals for future space missions.