A method for determining the inertia tensor of a spacecraft in flight, including the inertial orientation and turns of the spacecraft, characterized in that the spacecraft is oriented by stabilizing its construction axis in the inertial coordinate system, which is closest to the axis corresponding to the maximum moment of inertia, and spin the spacecraft around this building axis with an angular velocity Ω of at least 2%, they measure in the construction coordinate system of the spacecraft the directions to the recorded stars and the angle the speed of the spacecraft up to the time T = T + Δt, where, where T is the time of the spin of the spacecraft; Δt is the time interval of the weakly perturbed motion of the spacecraft; Ω is the angular velocity of the spin around the construction axis nearest the axis of the maximum moment of inertia; R - radius of the orbit; µ is the Earth’s gravitational parameter; K is the reliability coefficient, the registered stars are recognized, the directions to the identified stars are determined in the inertial coordinate system and the inertia tensor of the spacecraft is determined from measured and determined on the time interval Δt directions to recognized stars and measurements of the angular velocity of the spacecraft.
展开▼
机译:一种用于确定飞行器在飞行中的惯性张量的方法,包括飞行器的惯性定向和转弯,其特征在于,通过在惯性坐标系中稳定其构造轴线来使航天器定向,该惯性坐标系最接近于与飞行器相对应的轴线。最大惯性矩,并以至少2%的角速度Ω围绕该建筑轴旋转航天器,它们在航天器的构造坐标系中测量记录星的方向以及航天器的速度,直至时间T = T +Δt,其中,T是航天器旋转的时间; Δt是航天器微扰运动的时间间隔; Ω是围绕构造轴的自旋角速度,最接近最大惯性矩的轴; R-轨道半径; µ是地球的引力参数; K是可靠性系数,识别出已登记的恒星,在惯性坐标系中确定了指向已识别恒星的方向,并根据测量值确定了航天器的惯性张量,并在时间间隔Δt方向上确定了至识别恒星的方向,并确定了航天器的角速度。
展开▼