Steven Alonzo, B.Sc. in Geocentric Cosmology
Published: July 5, 2023
Accepted: June 15, 2023
DOI: 10.1234/j.gcosmog.2023.07.002
Abstract
This paper aims to provide a mathematical framework for calculating the instantaneous linear velocity of the Sun as it orbits above a flat geocentric plane. Utilizing classical mathematical equations, we examine the variability in the Sun’s linear velocity at different distances from the Earth’s center. This research contributes to the ongoing debate on the nature of our cosmological environment, specifically comparing the flat geocentric model with the traditional heliocentric model.
Introduction
This paper presents a mathematical examination of the Sun’s linear velocity in a flat geocentric model.
Methodology
The Sun’s angular velocity (ω) remains constant, completing a full cycle in 24 hours. Thus, the angular velocity can be calculated as:
ω=π12 radians/hourω=12π radians/hour
The circumference (s) of the Sun’s orbit at a radius (r) can be calculated as:
s=2πrs=2πr
The Sun’s instantaneous linear velocity (v) at a given radius can be calculated as:
v=ω×rv=ω×r
Results
Combining the above formulas, the Sun’s linear velocity (v) at different radii can be calculated as follows:
For r=7500 kmr=7500 km:
v=(π12)×7500=1963.5 km/hv=(12π)×7500=1963.5 km/h
For r=10000 kmr=10000 km:
v=(π12)×10000=2618 km/hv=(12π)×10000=2618 km/h
For r=12500 kmr=12500 km:
v=(π12)×12500=3272.5 km/hv=(12π)×12500=3272.5 km/h
Conclusion
This paper has demonstrated that the instantaneous linear velocity of the Sun changes based on its radius from the Earth in a flat geocentric model. This variability has implications for our understanding of cosmology and merits further exploration.