Two 56Fe atoms can theoretically fuse if they collide with sufficient energy, potentially forming Tellurium-112, though this process would likely result in the emission of neutrons and the creation of various isotopes. Under extreme heat and pressure, the stability of 56Fe changes, leading to different nuclear reactions; while high temperatures favor smaller nuclei, high pressures can stabilize larger nuclei. The collapse of an iron star into a neutron star may occur when the pressure exceeds a critical point, destabilizing 56Fe. The discussion also touches on the concept of equilibrium among elements, suggesting that at low pressure, 56Fe is the most stable form, but other isotopes like Ni-64 and Kr-86 have higher binding energies. Ultimately, the conversation highlights the complexities of nuclear fusion and the conditions required for stability and transformation in stellar environments.
