Methods are developed for estimating the rotation rate of a spacecraft using only measured magnetic e eld data. The goal is to provide rate information for use in applications such as detumbling, nutation damping, and momentum management without using gyroscopes. Two algorithms are developed, a deterministic algorithm and an extended Kalman e lter. Both algorithms employ the magnetic e eld direction kinematics equation and Euler’ s equation for attitude motion of a rigid body with momentum wheels. Neither algorithm requires a model of the Earth’ s magnetic e eld. The deterministic algorithm solves a nonlinear least-squares problem for the unknown angular momentum component along the magnetic e eld direction. The extended Kalman e lter estimates the attitude rate vector, corrections to e ve of the six inertia matrix elements, and two error states of the measured magnetic e eld direction. It uses an initial rate estimate from the deterministic algorithm to avoid divergence. The algorithms have been tested using data from a spinning sounding rocket. They achieve initial accuracies in the range 2‐7 deg/s when the rocket spins at about 80 deg/s, and their accuracies improve to 1 ‐2 deg/s after the spin rate decays to 20 deg/s. These results indicate a lower bound on the ratio of the error to the nominal spin rate, which suggests that dynamic modeling error is the dominant source of uncertainty. I. Introduction M ANY spacecraft need estimates of their rotation rates. The spin rate may be used to apply a control that stops tumbling, to manage the total system angular momentum, to aid a star tracker, or as part of an attitude determination system. The most common method of determining attitude rate is by direct rate-gyro measurement. This paper develops two attitude rate estimation methods that rely on Earth magnetic e eld measurements rather than on rate-gyro