The aim of this work is to investigate and characterize the multiple planetary system HD-28109, combining both photometric and spectroscopic data. The main focus is to exploit the transit time variation technique in order to determine the mass of the three orbiting planets and the dynamics of the planetary system, allowing a stability simulation through numerical integration which gives further insights on the evolution of the latter.
The aim of this work is to investigate and characterize the multiple planetary system HD-28109, combining both photometric and spectroscopic data. The main focus is to exploit the transit time variation technique in order to determine the mass of the three orbiting planets and the dynamics of the planetary system, allowing a stability simulation through numerical integration which gives further insights on the evolution of the latter.
Characterization of the multiple planetary system HD-28109 using Transit Time Variations
CECCA, LUCA
2024/2025
Abstract
The aim of this work is to investigate and characterize the multiple planetary system HD-28109, combining both photometric and spectroscopic data. The main focus is to exploit the transit time variation technique in order to determine the mass of the three orbiting planets and the dynamics of the planetary system, allowing a stability simulation through numerical integration which gives further insights on the evolution of the latter.| File | Dimensione | Formato | |
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Cecca_Luca.pdf
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https://hdl.handle.net/20.500.12608/92337