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Exoplanets atmospheres: the impact of stellar activity on the transmission spectra

Grant number: 21/14897-9
Support Opportunities:Scholarships in Brazil - Doctorate
Effective date (Start): April 01, 2022
Effective date (End): January 31, 2026
Field of knowledge:Physical Sciences and Mathematics - Astronomy - Stellar Astrophysics
Principal Investigator:Adriana Benetti Marques Valio
Grantee:Viktor Yuri Doná Sumida
Host Institution: Escola de Engenharia (EE). Universidade Presbiteriana Mackenzie (UPM). Instituto Presbiteriano Mackenzie. São Paulo , SP, Brazil
Associated research grant:18/04055-8 - High precision spectroscopy: from the first stars to planets, AP.TEM
Associated scholarship(s):24/03652-3 - Impact parameter and stellar activity - implications for exoplanetary transmission spectroscopy: prospective analysis on future targets of ARIEL space telescope; and an in-depth investigation of the small planet radius gap, BE.EP.DR


Exoplanet atmospheres are our only window to study the physical and chemical processes that occur on distant worlds. Such processes are important tracers of the origins of evolution of planetary systems. These are also paramount to better understand how common or unique are the conditions that lead to the emergence of life, which can leave precise spectroscopic traces in exoplanetary atmospheres. Transmission spectroscopy is a very effective technique for probing and measuring the composition and properties of exoplanet atmospheres. This technique consists of taking a spectra during a planetary transit in front of its host star. During the transit, a small fraction of the stellar radiation is filtered through the planet's atmosphere, where it is only partially absorbed. The absorption will be wavelength dependent due to the scattering properties of atoms and molecules in the planetary atmosphere. At the wavelength of a strong atomic or molecular transition, the atmosphere is more opaque and the radius of the planet is larger. This raises the prospect of measuring the transmission spectrum of the planet's atmosphere and thus learning about its composition. One of the main limitations of this technique is the stellar activity that can lead to a significant underestimation or overestimation of the ratio between the radius of the planet and the stellar radius as a function of the wavelength. Therefore, we will quantitatively study the impact of stellar activity, such as the presence of spots, on the transmission spectrum of exoplanets.

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