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Starspot Area Coverage: Correlation with Age and Spectral Type in FGK and M Stars

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Author(s):
Araujo, Alexandre ; Lima, Ciria ; Menezes, Fabian ; Valio, Adriana
Total Authors: 4
Document type: Journal article
Source: Astrophysical Journal Letters; v. 985, n. 2, p. 7-pg., 2025-06-01.
Abstract

Starspots, analogous to sunspots, are surface manifestations of stellar magnetic activity. Their study provides crucial insights into stellar dynamo processes and the evolution of magnetic phenomena. However, due to limited data on magnetic activity across stellar lifetimes, the relationship between starspot area coverage and stellar properties remains underexplored. This work investigates the correlation between starspot area coverage and stellar age, effective temperature, and rotation period in FGK and M stars using data from Kepler and CoRoT. We utilized the starspot transit mapping method to analyze 11 stars, calculating starspot area coverage by integrating spot areas on the stellar surface. The average starspot coverage ranged from 4% to 29%, consistent with theoretical models of stellar magnetic evolution. Our analysis revealed a strong anticorrelation with stellar age (Spearman rho = -0.80), confirming a significant decline in magnetic activity over time, but a weak anticorrelation between starspot coverage and rotation period. Regarding the relationship between absolute starspot area coverage and effective temperature, we found a moderate positive correlation (Spearman rho = 0.40), with the majority of stars with an absolute area coverage of (2-4 +/- 0.6) x 1010 km2. Incorporating starspot coverage into isochrone models could significantly improve stellar age estimates, especially for young stars. Moreover, these measurements are crucial for refining stellar dynamo models and advancing our understanding of magnetic field generation. (AU)

FAPESP's process: 22/12024-0 - Stellar activity from spot planetary transit modeling
Grantee:Fabian Marcel Menezes
Support Opportunities: Scholarships in Brazil - Post-Doctoral
FAPESP's process: 18/04055-8 - High precision spectroscopy: from the first stars to planets
Grantee:Jorge Luis Melendez Moreno
Support Opportunities: Research Projects - Thematic Grants
FAPESP's process: 21/02120-0 - Investigation of high energy and plasma astrophysics phenomena, installation of the ASTRI-Mini Array & construction of the Cherenkov Telescope Array Small Size Telescopes (CTA-SSTs)
Grantee:Elisabete Maria de Gouveia Dal Pino
Support Opportunities: Special Projects