  Analysis of the radio-metric tracking data from the Pioneer 10 and 11
spacecraft at distances between 20--70 astronomical units from the Sun has
consistently indicated the presence of an anomalous, small, and constant
Doppler frequency drift. The drift is a blue-shift, uniformly changing at the
rate of (5.99 +/- 0.01) x 10^{-9} Hz/s. The signal also can be interpreted as a
constant acceleration of each particular spacecraft of (8.74 +/- 1.33) x
10^{-8} cm/s^2 directed toward the Sun. This interpretation has become known as
the Pioneer anomaly. We provide a problem set based on the detailed
investigation of this anomaly, the nature of which remains unexplained.

Physics Education;Space Physics