In February 1985 I decided that it is crazy not to be able to calculate such a simple thing. I decided not to use any approximations this time and I calculated, with high school calculus, Newtonian math, and a little of Einsteinian physics (limited to equation <math>E=mc^2</math>) how much of cosmological [[redshift]] in the universe is due to the expansion of space and how much is due to the Newtonian interaction between photons and the masses of universe that as I learned from Ned Wright <ref>Edward L. (Ned) Wright, Astronomy | In February 1985 I decided that it is crazy not to be able to calculate such a simple thing. I decided not to use any approximations this time and I calculated, with high school calculus, Newtonian math, and a little of Einsteinian physics (limited to equation <math>E=mc^2</math>) how much of cosmological [[redshift]] in the universe is due to the expansion of space and how much is due to the Newtonian interaction between photons and the masses of universe that as I learned from Ned Wright <ref>Edward L. (Ned) Wright, Astronomy |