Write a 2-3 pages report with illustrations to summarize the conditions needed for the fusion of Hydrogen to create Helium in the core of the SUN, which
necessary to produce the radiation energy we call sunshine. These steps are outlined in Fig 14.8, and the process is referred to as the Hydrogen Fusion by
the Proton-Proton Chain. To compliment these figures and connect this to the famous Figure 14.4 Figure 14.8 Einstein relation of mass and energy, you
should refer to the section labeled Mathematical Insight 14.1- Mas-energy Conversion in Hydrogen Fusion. Understand that only after Einstein made the
connection between mass and energy, via his now famous Formula, we really did not know how the SUN could produce so much energy for such a long time.