  We report a new subdwarf B (sdB) pulsator, PG1142-037, discovered during the
first full-length campaign of K2, the two-gyro mission of the Kepler space
telescope. Fourteen periodicities have been detected between 0.9 and 2.5 hours
with amplitudes below 0.35 ppt. We have been able to associate all of the
pulsations with low-degree, ell<=2 modes. Follow-up spectroscopy of PG1142 has
revealed it to be in a binary with a period of 0.54 days. Phase-folding the K2
photometry reveals a two-component variation including both Doppler boosting
and ellipsoidal deformation. Perhaps the most surprising and interesting result
is the detection of an ellipsoidal, tidally distorted variable with no
indication of rotationally-induced pulsation multiplets. This indicates that
the rotation period is longer than 45 days, even though the binary period is
near 13 hours.
