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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
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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.

Journal: IRASS Journal of Multidisciplinary Studies
ISSN(Online): 3049-0073
Publisher: IRASS Publisher
Frequency: Monthly
Language: English

Analysis of Exoplanet HD80606b in Primary-centric Framework