Q: Add these two equations together, then solve for the radius RA. 4 RA = [ (t4 - t1) + (t3 - t2) ] * (v1 + v2) RA = 0.25 * [ (t4 - t1) + (t3 - t2) ] * (v1 + v2) Then plug in values to compute the radius of star A in meters. RA = 0.25 * [ (17300 s) + (6050 s) ] * (150 km/s) = 8.76 x 10^(8) m = 1.26 solar radii