The incongruity in the cycle of galaxies has drawn a lot of attention, which led to the review of the connection between the rotational angular velocity of some spiral barred galaxies and radius. There is a need for an alternative method because the morphologies of galaxies that have been categorized so far do not match the rotational angular velocities of these spiral-barred galaxies. To reclassify spiral-barred galaxies and determine the relationship between the rotational angular velocities of eighty-four spiral-barred galaxies and their radius was substantiated here. Python, Visual Studio, and MATLAB are the software deployed to study eighty-four spiral-barred galaxies. Data for this computation of the rotational angular velocity were sourced from the Internet and the National Aeronautics and Space Administration (NASA). These parameter values were used in the equations of rotational angular velocity to calculate it. Rotational angular Velocity equations were used to write a Python calculation programme, and the results were tabulated alongside data sourced from the internet with their units. Some of the results for rotational angular velocity generated for eighty-four spiral barred galaxies are: Black eye =1.17E+03Km/s, Butterfly Nebula = 2Km/s. It was discovered that increased rotational angular velocity with radius of spiral barred galaxies behaved more aberrantly relative to their groups. Conclusively, there is no or little direct correlation between rotational angular velocity and radius.
Spiral Barred Galaxies, Radius, Rotational Angular Velocity, Angular Velocity, MATLAB.
IRE Journals:
Ekwubiri, E. C. "Analysis of The Sixth-Degree Polynomial Correlation Between Rotational Angular Velocity of Spiral Barred Galaxies with Radius" Iconic Research And Engineering Journals Volume 9 Issue 9 2026 Page 2598-2610
IEEE:
Ekwubiri, E. C.
"Analysis of The Sixth-Degree Polynomial Correlation Between Rotational Angular Velocity of Spiral Barred Galaxies with Radius" Iconic Research And Engineering Journals, 9(9)