Neutron stars are incredibly dense, primarily composed of neutrons, with a mix of protons and electrons, especially near the core due to extreme pressure. The term "neutron star" reflects this composition, as the high density causes protons and electrons to combine into neutrons. The discussion clarifies misconceptions about atomic structure, emphasizing that while fundamental particles are often considered point-like, they interact over measurable distances, contributing to the perceived size of atoms. The debate also touches on the nature of empty space within atoms, suggesting that atomic systems can be viewed as either mostly empty or filled with fields, depending on the perspective. Overall, neutron stars exemplify the complexities of matter and density in astrophysical contexts.