Little is known about seismic activity of Venus and location of seismic sources. There are no seismic instruments that would be able to survive over extended periods under Venus conditions. Nevertheless, a seismic experiment is planned on the surface of Venus. It is also proposed to register disturbances in the atmosphere and ionosphere of the planet caused by seismic events. For forthcoming seismic experiments on Venus, it is important to know in which areas the stresses are large enough and capable of producing venusquakes. Here we study stress field of Venus starting from a simple model: a liquid core and an elastic mantle and crust with the help of a static method.