HD 166620: Portrait of a Star Entering a Grand Magnetic Minimum
Jacob K. Luhn, Jason T. Wright, Gregory W. Henry, Steven H. Saar, Anna, C. Baum

TL;DR
This study provides conclusive evidence that HD 166620 is entering a grand magnetic minimum, similar to the Maunder Minimum, based on extended activity data, and discusses implications for identifying such states.
Contribution
The paper presents new long-term activity and photometry data confirming HD 166620's transition into a Maunder Minimum-like state, the first definitive case of such a star.
Findings
HD 166620 is entering a grand magnetic minimum.
Brightness and activity levels are not significantly lower during the minimum.
Reduced intraseasonal variability in activity may indicate a grand minimum.
Abstract
HD 166620 was recently identified as a Maunder Minimum candidate based on nearly 50 years of Ca II H & K activity data from Mount Wilson and Keck-HIRES (Baum et al. 2022). These data showed clear cyclic behavior on a 17-year timescale during the Mount Wilson survey that became flat when picked up later with Keck-HIRES planet-search observations. Unfortunately, the transition between these two data sets -- and therefore the transition into the candidate Maunder Minimum phase -- contained little to no data. Here we present additional Mount Wilson data not present in Baum et al. (2022) along with photometry over a nearly 30-year baseline that definitively trace the transition from cyclic activity to a prolonged phase of flat activity. We present this as conclusive evidence of the star entering a grand magnetic minimum and therefore the first true Maunder Minimum analog. We further show…
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