  We have observed evidence for $p$-mode oscillations in the G0 IV star etaBoo
(V = 2.68). This represents the first clear evidence of solar-like oscillations
in a star other than the Sun. We used a new technique which measures
fluctuations in the temperature of the star via their effect on the equivalent
widths of the Balmer lines. The observations were obtained over six nights with
the 2.5 m Nordic Optical Telescope on La Palma and consist of 12684
low-dispersion spectra. In the power spectrum of the equivalent-width
measurements, we find an excess of power at frequencies around 850 microHz
(period 20 minutes) which consists of a regular series of peaks with a spacing
of $\Delta\nu=40.3$ microHz. We identify thirteen oscillation modes, with
frequency separations in agreement with theoretical expectations. Similar
observations of the daytime sky show the five-minute solar oscillations at the
expected frequencies.
