The Theory of Magnitudes
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Abstract
This is a way to look at a photos of stars and make sense to get a value that shows the closest star: in the vicinity: It uses star’s apparent magnitudes to get theses inverse magnitudes and to get a nearby star of the largest ratio ; of the inverse apparent magnitude divided by the distance. Now the beginning reference star obeys this ratio . For the greater the distance the lower the value. And we want the highest value . The greater the brightness enlarges and the greater the distance makes the value lessons. After trying to use aspects of General Relativity’s Tensor Calculus, l found l could not find my formulas to fit the data . In an original way l used the inverse Apparent Magnitudes in Astronomical to get a consistant formula that is data proven with general ideas from Global analysis. It works with Star charts/photos. Before l even tried using the inverse of the determinates of linear algebra. But my attempts were to no avail. Therefore l became inspired by basic formulas in General Relativity but that did not work. Using Global Analysis in an new l succeeded. Keywords Using my new formula l can obtain the distance between a reference star, using its inverse apparent magnitude, l obtain the distance to from another star using certain restrictions which the measurement in centimeters to this other star from its reference star nearby.

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References
Martin Ince ; (1997); Dictionary of Astronomy ; page 128 ; Peter Collin Publishing Ltd
Charles Liu ; (2008) ; The Handy Astronomy Book ; page 94,95 : Visible Ink Press.
John W. Moffat ; (2008) ; Reinventing Gravity ; page 55 ; Harper Collins Books