  Light curves of the eclipsing binary FL Lyr acquired by the Kepler space
telescope are analyzed. Eclipse timing measurements for FL Lyr testify to the
presence of a third body in the system. Preliminary estimates of its mass and
orbital period are > 4M_Jupiter and > 7 yrs. The times of primary minimum in
the light curve of FL Lyr during the operation of the Kepler mission are
presented.
