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hello everyone and welcome to Skye scholar our prior video explained how the Sun produces the solar spectrum through liquid metallic hydrogen a structure similar to graphite this flexible structure easily explains other aspects of solar emission including limb darkening sunspots faculae and granules theoretical studies on dense atomic hydrogen suggest that its metallic character is dependent on internuclear distance the shorter the distance the greater the metallic character at longer distance the material becomes a semi metal like graphite in my papers linked below I refer to the less metallic hydrogen as type 1 and the more metallic form as type 2 it is believed that metallic hydrogen is made by high temperatures and pressures in the solar interior and remain stable once formed this is the same situation in diamonds which are formed at high pressures but remain stable at atmospheric pressures to understand the emissive behavior of the Sun we should learn a little about direct
