Using Transiting Planets to Model Starspot Evolution
James R. A. Davenport, Leslie Hebb, Suzanne L. Hawley

TL;DR
This paper models starspot evolution using Kepler light curves, combining in- and out-of-transit data to understand stellar dynamos, differential rotation, and spot lifetimes across different stars.
Contribution
It introduces a novel approach that models both in- and out-of-transit light curves to break degeneracies in starspot property measurements.
Findings
Measured slow differential rotation rates in stars without transiting planets.
Constrained key physical parameters like rotation period and diffusion timescales.
Revealed long-term changes in starspot sizes and positions over four years.
Abstract
Photometry from Kepler has revealed the presence of cool starspots on the surfaces of thousands of stars, presenting a wide range of spot morphologies and lifetimes. Understanding the lifetime and evolution of starspots across the main sequence reveals critical information about the strength and nature of stellar dynamos. We probe the dynamo by modeling the starspot properties over time using Kepler light curves. In particular, we use planetary systems like Kepler 17 that show in-transit starspot crossing features. Spot-occulting transits probe smaller-scale starspot features on the stellar surface along a fixed latitude region. Our approach is novel in modeling both the in- and out-of transit light curve features, allowing us to break fundamental degeneracies between spot size, latitude, and contrast. With continuous monitoring from Kepler we are able to observe small changes in the…
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Taxonomy
TopicsStellar, planetary, and galactic studies · Astro and Planetary Science · Astronomy and Astrophysical Research
