The Theory of Magnitudes

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Daniel Weinstock

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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Article Details

How to Cite
Weinstock, D. (2022). The Theory of Magnitudes. Technium: Romanian Journal of Applied Sciences and Technology, 4(10), 11–14. https://doi.org/10.47577/technium.v4i10.7606
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Articles

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