In neutron stars, traditional atomic structures do not exist due to extreme gravitational forces that unbind electrons from nuclei, resulting in a composition of free neutrons, protons, and electrons. The outer crust may contain a dense arrangement of bare nuclei, which can be considered as being in close proximity, akin to "touching." As one moves deeper into the star, the matter becomes increasingly dense, potentially forming a quark-gluon plasma where nucleons are decomposed into quarks and gluons. The concept of "touching" is complex in this context, as atomic interactions differ significantly from those in normal matter. Overall, the extreme conditions in neutron stars lead to unique states of matter that challenge conventional definitions of atomic contact.