Активность звезды TIC 88785435 и потеря массы атмосферы ее планеты

We investigate the activity of a young K7V star TIC 88785435 and estimate the mass loss from the atmosphere of its exoplanet. TIC 88785435 is a member of the  Lup subgroup with an age of 9.9-17.7 million years. The age of the star itself is 16.0±1.6 million years. According to the analysis of the observations of the TESS mission we estimate the spottedness of the star's surface, which is equal to 6.3 and 10.5% of the surface area of the star, or in absolute values 43000 and 71300 MSH for TESS observations in sectors 38 and 65 respectively. For the most reliable flare, the energy emitted in the flare was measured as 1.031033 erg. calculations performed using the energy-limited atmospheric loss model for TIC 88785435 b, it was found that depending on the star's activity level the amount of atmospheric mass loss from the exoplanet can be in the range of 2.7 108 g/s - 1.7 109 g/s.

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Publication Details

Journal
Astrophysics
Published
2025-07-21
DOI
https://doi.org/10.54503/0571-7132-2025.68.2-169
Primary Topic
Stellar, planetary, and galactic studies
Type
article
Field-Weighted Citation Impact
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article

Активность звезды TIC 88785435 и потеря массы атмосферы ее планеты

И. С. Саванов
Astrophysics
Stellar, planetary, and galactic studies
article

Активность звезды TIC 88785435 и потеря массы атмосферы ее планеты

И. С. Саванов
article en

Abstract

We investigate the activity of a young K7V star TIC 88785435 and estimate the mass loss from the atmosphere of its exoplanet. TIC 88785435 is a member of the  Lup subgroup with an age of 9.9-17.7 million years. The age of the star itself is 16.0±1.6 million years. According to the analysis of the observations of the TESS mission we estimate the spottedness of the star's surface, which is equal to 6.3 and 10.5% of the surface area of the star, or in absolute values 43000 and 71300 MSH for TESS observations in sectors 38 and 65 respectively. For the most reliable flare, the energy emitted in the flare was measured as 1.031033 erg. calculations performed using the energy-limited atmospheric loss model for TIC 88785435 b, it was found that depending on the star's activity level the amount of atmospheric mass loss from the exoplanet can be in the range of 2.7 108 g/s - 1.7 109 g/s.

Astrophysics
Openalex Percentile: Top 87%
Stellar, planetary, and galactic studies
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