Mathematical Foundations of Processing the Results of Astronomical Scientific Observation and a Program Used In PHOTOMETRY

Abstract

The Earth is a space of dust on the astronomical scale; astronomy contains the physics of several stellar objects. These objects are very far away from Earth; moreover, they are the most interested and attractive objects for human beings. Human beings are continuously developing and installing the observational facilities (telescopes) for solving the mystery of the Universe. The various photometric bands/filters are associated with these telescopes, and each band show different effective wavelength to detect the information about the interior physical phenomenon. The detected information can be used to constrain the dynamism and evolution model of interested stellar objects. Heavier atoms of matter are to be made in the interior part of stars and prescribed matter to pervade into space through the “Supernova burst”. Our earth is also made of such type materials. Thus, every molecule of our bodies is contained the matter that once was subjected to the tremendous temperatures and pressures at the center of a star.