darkdestruction420
Well-Known Member
......?
Anyway, I have been researching the universe and physics/astrophysics for a long time now and ive come across something that it seems half the scientific community of astrophysicists havent been taking into consideration, when you try to measure dark energy you use la supernova, a type of supernova that is always of the same energy and fades at a predictable rate, they result when a white dwarf star becomes too large from sucking in gas from a binary companion to support its own pressure and collapses, which is a universal constant, but now it seems nickel 56 level is what determines the brightness of a supernova explosion, the energy released is always the same, but the brightness we measure to tell how quickly they are receding is not......so, what do you guys think?
Anyway, I have been researching the universe and physics/astrophysics for a long time now and ive come across something that it seems half the scientific community of astrophysicists havent been taking into consideration, when you try to measure dark energy you use la supernova, a type of supernova that is always of the same energy and fades at a predictable rate, they result when a white dwarf star becomes too large from sucking in gas from a binary companion to support its own pressure and collapses, which is a universal constant, but now it seems nickel 56 level is what determines the brightness of a supernova explosion, the energy released is always the same, but the brightness we measure to tell how quickly they are receding is not......so, what do you guys think?