  The unprecedented imaging power of JWST provides new abilities to observe the
shapes of objects in the early Universe in a way that has not been possible
before. Recently, JWST acquired a deep field image inside the same field imaged
in the past as the HST Ultra Deep Field. Computer-based quantitative analysis
of spiral galaxies in that field shows that among 34 galaxies for which their
rotation of direction can be determined by the shapes of the arms, 24 rotate
clockwise, and just 10 rotate counterclockwise. The one-tailed binomial
distribution probability to have asymmetry equal or stronger than the observed
asymmetry by chance is $\sim$0.012. While the analysis is limited by the small
size of the data, the observed asymmetry is aligned with all relevant previous
large-scale analyses from all premier digital sky surveys, all show a higher
number of galaxies rotating clockwise in that part of the sky, and the
magnitude of the asymmetry increases as the redshift gets higher. This paper
also provides data and analysis to reproduce previous experiments suggesting
that the distribution of galaxy rotation in the Universe is random, to show
that the exact same data used in these studies in fact show non-random
distribution, and in excellent agreement with the results shown here. These
findings reinforce consideration of the possibility that the directions of
rotation of spiral galaxies as observed from Earth are not necessarily randomly
distributed. The explanation can be related to the large-scale structure of the
Universe, but can also be related to a possible anomaly in the physics of
galaxy rotation.
