The heliogyro is an ultra-lightweight, high performance, helicopter-like, spinning solar sail architecture. One principal concern for the feasibility of heliogyro solar sails is the ability to adequately control the dynamic response of their long, unsupported blades, and, in particular, to damp disturbances caused by maneuvering transients at the blade tips. In this study, the authors investigated the use of reflectivity control devices (RCDs) at the blade tips for damping pitch disturbances for a conceptual, small-scale, heliogyro technology, flight demonstrator. The simple RCD controller enforces pitch rate tracking but requires pitch rate knowledge at multiple stations to ensure stability. Sensitivity analyses explored the design space for future RCDs. Results showed that RCDs similar to those flown on Japan Aerospace Exploration Agency's IKAROS (Interplanetary Kite-craft Accelerated by Radiation of the Sun) and covering 10% of the blade's reflective area were sufficient to control blade torsional disturbances, albeit not quickly enough for short-period orbit applications. Using advanced RCDs that are thinner and have a larger reflectivity difference between on and off states reduced maneuver settling time by 67%. Doubling the on/off reflectivity difference cut settling time in half, allowed for a smaller RCD, and boosted total solar sail acceleration 63%. Reducing RCD thickness by half decreased settling time only 35% but did enhance acceleration by 127%. Such gains should be feasible with moderate improvements in current RCD materials technology and make RCD-based heliogyro blade control a viable solid-state alternative to mechanical, torsional damping systems at the blade root. Nomenclature a 0 = characteristic acceleration (mm/s 2 ) A = cross-sectional area (m 2 ), system dynamics matrix B = control matrix B f = Lambertian coefficient of diffuse reflectivity C d = coefficient of diffuse reflectivity C s = coefficient of specular reflectivity c = blade chord (m) c s = solar cell chord (m) f RCD = reflectivity control device blade area fraction F = force (N) 2 h = blade thickness (m) iRs = index of transition from inboard to outboard I = area moment of inertia (m 4 ) J = mass moment of inertia (kg-m 2 ) K = stiffness (N-m/rad) or control gain m = mass (kg) M = moment (N-m) � = moment per length span (N-m/m) n = finite element index n = blade normal unit vector N = total number of finite elements P 0 = solar radiation pressure at 1AU (4.56e-6 Pa) P n = pressure normal to blade surface (Pa) R = total blade span or heliogyro radius (m) R s = span inboard of RCDs (m) s = solar radiation unit vector t = time (s) u = system control input w = vertical displacement (m) x = spanwise position (m) y = in-plane, chordwise position from centerline (m) α= vector describing steady-state blade shape (rad/N-m) β = blade sun angle (rad) δθ n = difference in blade pitch from one element to the next (rad) Δx = element span (m) γ = local angle of incident solar radiation (rad) ϕ = vertical membrane deflection (rad) θ = blade pit...