  We analyse a set of moments of minima of eclipsing variable V0873 Per. V0873
Per is a short period low mass binary star. Data about moments of minima of
V0873 Per were taken from literature and our observations during 2013-2014. Our
aim is to test the system on existence of new bodies using timing of minima of
eclipses. We found the periodical variation of orbital period of V0873 Per.
This variation can be explained by the gravitational influence of a third
companion on the central binary star. The mass of third body candidate is
$\approx 0.2 M_{\odot}$, its orbital period is $\approx 300$ days. The paper
also includes a table with moments of minima calculated from our observations
which can be used in future investigations of V0873 Per.
