JAMB - Physics (2001 - No. 31)
The process of energy production in the sun is
nuclear fission
nuclear fussion
electron collision
radioactive decay
解释
The sun produces energy primarily through the nuclear fusion of hydrogen nuclei, a reaction that occurs at extremely high temperatures, around 10\(^7\) K.
H\(_1\) + H\(_1\) → \(_2\)H
H\(_1\) + H\(_1\) → \(_2\)H