The Theorem I=W102 Highlights an Accurate Method of Rapid Measurements of Abnormal Areas on the Moon’s Surface

Asis Ghosh and Syama P. Bhattacharya

Published on: 2024-06-19

Abstract

In the new wave of lunar exploration, polar water has become one of the main task of NASA, ISRO, ESA, and RKA. It is expected that most important task after landing on the moon surface would be to find out of the source of water. Up-to-date the astronomers are convinced that water-ice can be found at the moon’s poles inside the shadowed craters. Most landed areas of astronomical interest on the moon’s surface are expected to be blended with many bends and deflections. In case the moon explorers decide to record accurate measurements of these spot areas it will be difficult for them to do so using any of the existing methods. In order to solve the problem an alternative method has been proposed along with a newly developed formula I=W10². The authors are also interested to mention that now-a-days radar is used for the measurements of areas. But the authors believe that the use of radar has limitation in the measurement of different area types as well as the sizes. Such as in case of measurements of very big size of areas or microscopical size of areas the use of radar is never been reported. In our case of experiment I=W10² is considered to be the best method.