Final answer:
Nuclear fission reactions can naturally occur on Earth due to the lower energy required to initiate them, whereas nuclear fusion requires extremely high temperatures and pressures to overcome the electrostatic repulsion between light nuclei, conditions that are not naturally found on Earth but are present in stars.
Step-by-step explanation:
The difference in observation of nuclear fission and nuclear fusion under Earth's conditions can be explained by the inherent properties of these reactions. Fission can occur naturally when large, unstable nuclei, like uranium-235, capture a neutron and are split into smaller nuclei, releasing energy and more neutrons. This neutron-induced chain reaction can occur at lower energies compared to fusion. In contrast, fusion requires the combination of two light nuclei, such as those of hydrogen, to form a heavier nucleus, like helium. This process is hindered by the electrostatic repulsion between the positively charged nuclei, necessitating extremely high temperatures and pressures to overcome this barrier, akin to conditions found in stars.
Fusion is more efficient and can produce more energy per reactant mass, but the activation energy is very high due to the need to overcome the Coulomb barrier, which is the repulsion between nuclear particles. The gravitational pressure in stars provides the necessary environment for fusion, but achieving this on Earth requires sophisticated technology to replicate such extreme conditions.