  On the sighting of the constellations and their stars, they seem to be near
each other at first sight but some of thema are actually quite further from the
others. Froma the geocentric point view can the Zodiac Costellations be
perceived as referential marks divided into terrestrial ecliptic, which are
organized according to their shapes. In this paper are these star groups
simulated in order to compare the shapes of these groups and the diverse
coordinate system of the astronomy. Within the simulation is the distance
measure light-year remplaced with a so-called program's default "unity" that
uses a compilation in Python, where such distances are escalated to 1:10
