We report detection of differential rotation on the F5 dwarf psi Cap using
line profile analysis. The Fourier transform of both Fe I lambda 5775 and S
i I lambda 5772 are used to obtain a projected rotational velocity of v sin
i = 42 +/- 1 km s(-1). Modelling of the Fourier transformed profiles shows
that the combined effects of equatorial velocity, inclination and differen
tial rotation dominate the line profile while limb darkening and turbulence
velocities have only minor effects. Rigid rotation is shown to be inconsis
tent with the measured profiles. Modelling the line profiles analogous to s
olar differential rotation we find a differential rotation parameter of alp
ha = 0.15 +/- 0.1 (15 +/- 10%) comparable to the solar case. To our knowled
ge this is the first successful measurement of differential rotation throug
h line profile analysis.