- Research Article
- 10.1088/1674-4527/ae4e81
Complex Analysis of Close Visual Stellar Systems in the Context of Gaia Observations. I. HIP 16348
- May 18, 2026
- Research in Astronomy and Astrophysics
- Mashhoor A Al-Wardat + 8 more +8
Abstract We present the habitability and stability of the proposed planets around the young stellar system HD 21841 based on the estimated astrophysical parameters of its components. Our study utilizes an orbital analysis of the system, employing Tokovinin's Method and incorporating 12 new speckle interferometric measurements that collectively span approximately 90 degrees of the orbit. Additionally, we use Al-Wardat's method for analyzing binary and multiple stellar systems in conjunction with Gaia DR3 astrometry and spectral data for a comprehensive spectrophotometric assessment of the components. This approach utilizes Kurucz’s model stellar atmospheres and available photometric data to develop synthetic spectral energy distributions (SEDs) for each component and subsequently the entire system. We can identify the physical parameters and the optimal solution by comparing the synthetic SED of the entire system with the observational data from Gaia. The analysis successfully determined the stellar parameters of the system for the first time, revealing the following: $ T_{\rm eff.}=5945\pm80\,K$, $R=1.018\pm0.05\, R_\odot$ , $\mathcal{M}=1.12\pm0.10\, \mathcal{M_\odot}$ for the primary component and $T_{\rm eff.}=5700\pm80\,K$, $R=0.975\pm0.06\, R_\odot$ , $\mathcal{M}=1.05\pm0.09\, \mathcal{M_\odot}$ for the secondary component. Both components are found to have solar metallicity and are approximately 1 billion years old. The combined spectrophotometric and dynamical analysis resulted in precise stellar masses and a new dynamical parallax of $23.756\pm0.001$ mas, consistent with the Hipparcos 1997 measurement ($23.76\pm1.07$) and intermediate between that of Gaia DR2 ($23.51\pm0.28$) and Gaia DR3 ($24.31\pm0.19$). In addition to studying the habitability and stability of the exoplanets within the system, we explored the processes of its formation and evolution.
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