Two types of sensitivities are proposed for statically stable sailcrafts. One type is the sensitivities of solar-radiation-pressure force with respect to position of the center of mass, and the other type is the sensitivities of solar-radiation-pressure force with respect to attitude. The two types of sensitivities represent how the solar-radiationpressure force changes with the position of mass center and the attitude. Sailcrafts with larger sensitivities undergo larger error of the solar-radiation-pressure force, leading to larger orbit error, as demonstrated by simulation. Then as a case study, detailed formulas are derived to calculate the sensitivities for sailcrafts with four triangular sails. According to these formulas, in order to reduce both types of sensitivities, the angle between opposed sails should not be too large, and the center of mass should be as close to the axis of symmetry of the four sails as possible and as far away from the center of pressure of the sailcraft as possible.Keywords Statically stable sailcraft · Sensitivity · Solarradiation-pressure force error · Mass center and pressure center errors · Attitude and orbit errorsDirection cosine matrix corresponding to rotation of φ rad about the λ-axis (λ = x, y, z)e 2 , e 3 [1 0 0] T , [0 1 0] T , [0 0 1] T F Resultant solar-radiation-pressure force represented in the body-fixed frame (N) F r , F ri Resultant solar-radiation-pressure force in the reference frame, the i-th component ofF r (N) n i Normal vector of S i O, O Apex of the cone formed by the four sails, center of the square A 1 A 2 B 2 B 1 O c , O i Center of mass of the whole sailcraft, pressure center of S i Ox b y b z b Body-fixed frame O r x r y r z r Reference frame P Pressure center of the sailcraft P 0 Nominal solar-radiation-pressure constant 1 AU from the Sun (N/m 2 ) R r Position vector of the sailcraft represented in the reference frame (AU) r, r c , r i Vector from P to O c , vector of mass center position, the i-th component of r (m)