- PII
- S30345170S0004629925090063-1
- DOI
- 10.7868/S3034517025090063
- Publication type
- Article
- Status
- Published
- Authors
- Volume/ Edition
- Volume 102 / Issue number 9
- Pages
- 810-820
- Abstract
- The paper presents an analysis of high-precision satellite light curves of exoplanets HD 189733 b and HD 209458 b. The dependence of the exoplanet radius on the wavelength caused by scattering in the planetary atmosphere is determined using a four-parameter limb darkening law based on a three-dimensional model of the stellar atmosphere. It is shown that when using the same exoplanet system characteristics for all wavelengths, primarily the orbital inclination, as well as when using a four-parameter law with a refined radius of the star, the change in the radius of the exoplanet HD 189733 b with increasing corresponds to the model of an exponential Rayleigh atmosphere with a characteristic height of 380–400 km. At the same time, the characteristics of the atmosphere of HD 209458 b largely depend on the adopted eccentricity of the system.
- Keywords
- экзопланеты экзопланетные атмосферы HD 189733 b HD 209458 b
- Date of publication
- 01.09.2025
- Year of publication
- 2025
- Number of purchasers
- 0
- Views
- 50
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