Analysis of Exoplanet HD80606b in Primary-centric Framework
Sr No:
Page No:
17-23
Language:
English
Authors:
Bijay Kumar Sharma*
Received:
2025-07-02
Accepted:
2025-07-15
Published Date:
2025-07-19
Abstract:
The author in his quest for discovering the architectural layout of solar system and
exo-solar systems struck upon the design rules of architectural layout of planets and stars in star
pairs in the year 2011. In this paper the first section shows that a given stellar nebula falls in
outer Clarke’ configuration in the months/years. The first Clarke’s Orbit is untenable in case of
Star Pair HD80606A+HD80606B. The second Clarke’s orbit of the star pair is the present semimajor axis of the star pair. This paper goes further to show that HD80606A is hosting a highly
elliptical giant Jupiter exoplanet HD80606b which suffers from spin-orbital misalignment
problem.. In spite of this misalignment the observed and theoretical value of ω/Ω have
remarkable correspondence within the error bar of the Globe-orbit parameters of the exoplanet
system. This is the umpteenth example of Primary -centric formulation since 2011.
Keywords:
Sub-synchronous orbit; super-synchronous orbit, triple synchrony; Kinematic model.