  We report the detection of the first extrasolar planet, ET-1 (HD 102195b),
using the Exoplanet Tracker (ET), a new generation Doppler instrument. The
planet orbits HD 102195, a young star with solar metallicity that may be part
of the local association. The planet imparts radial velocity variability to the
star with a semiamplitude of $63.4\pm2.0$ m s$^{-1}$ and a period of 4.11 days.
The planetary minimum mass ($m \sin i$) is $0.488\pm0.015$ $M_J$.
