The future of the Sun: an evolved solar twin revealed by CoRoT
J.-D. do Nascimento Jr., Y. Takeda, J. Melendez, J.S. da Costa, G.F., Porto de Mello, M. Castro

TL;DR
This study identifies and characterizes an evolved solar twin star using space-based photometry and high-resolution spectroscopy, revealing its age, rotation period, and chemical composition, and compares it to the Sun.
Contribution
First solar twin identified by CoRoT with a measured rotation period and detailed chemical analysis, extending knowledge of solar analogs to older ages.
Findings
Star CoRoT ID 102684698 is an evolved solar twin with a 29-day rotation period.
It has a low lithium abundance and is approximately 6.7 billion years old.
The star shows enhanced refractory element abundances compared to the Sun.
Abstract
The question of whether the Sun is peculiar within the class of solar-type stars has been the subject of active investigation over the past three decades. Although several solar twins have been found with stellar parameters similar to those of the Sun (albeit in a range of Li abundances and with somewhat different compositions), their rotation periods are unknown, except for 18 Sco, which is younger than the Sun and with a rotation period shorter than solar. It is difficult to obtain rotation periods for stars of solar age from ground-based observations, as a low activity level imply a shallow rotational modulation of their light curves. CoRoT has provided space-based long time series from which the rotation periods of solar twins as old as the Sun could be estimated. Based on high S/N high resolution spectroscopic observations gathered at the Subaru Telescope, we show that the star…
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