On the occasion of the inaugural observations of the James Webb space telescope we will briefly analyze the "Stephan's Quintet". The group is known for the gigantic shock waves to which astronomers claim it is exposed.The calculation is crude: we cannot have observations at different times nor measure any transverse velocity to us. The use of computational code for the N-body system is beyond the scope of this simple processing. Anyhow, I am not sure there would be enough data to set up the simulation (Eccentricity is missing). This short study is being carried out in the context of the cosmological model named "4-Sphere" and described in [viXra:2209.0098] (it works in the Special Relativity context). Excluding the more distant NGC 7320 and NGC 7318B, to look for a cause of the observed strong interactions, we must hypothesize that NGC 7317, NGC 7318A and NGC 7319 are close to each other and that their relative recession speeds are instead radial components of their peculiar velocity.We assume in the vicinity of NGC 7319 and its supermassive Active Galactic Nuclei, the center of gravity of the three remaining galaxies. The equivalent of a triple star, with NGC 7317 and NGC 7318A that form a binary system of galaxies, is the setup we will confirm. The system is dynamically unstable, also leading to a galaxy being ejected: this context could involve the big shockwaves, that astronomers speak of.