Everybody understands what is meant by an eclipse: a body that covers another one. However, the general audience and the students in particular do not know exactly “What the relative positions of the Earth, the Sun and the Moon have to be in order for an eclipse to take place?”

You can read a newspaper or watch TV and observe that the information about an eclipse is not correct. In my country, it was stated, in a very important newspaper, that “the solar eclipse will take place tomorrow because there will be a Full Moon”.

Teaching this topic in schools or in educational sessions in observatories, it is a good idea to introduce a simple model that maintains the proportion between the diameters and distances of these three bodies. This contribution will introduce this model, showing their applications in the playgrounds of the school, for sunny days or in the classroom for cloudy days.