The Li-age correlation: The Sun is unusually Li deficient for its age
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Carlos, Marília
Melendez, J
Spina, L.
dos Santos, L.
Bedell, M.
Ramirez, Ivan
Asplund, Martin
Bean, Jacob
Yong, David
Galarza, Jhon Yana
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Oxford University Press
Abstract
This work aims to examine in detail the depletion of lithium in solar twins to better constrain
stellar evolution models and investigate its possible connection with exoplanets. We employ
spectral synthesis in the region of the asymmetric 6707.75 Å Li I line for a sample of 77
stars plus the Sun. As in previous works based on a smaller sample of solar twins, we find
a strong correlation between Li depletion and stellar age. In addition, for the first time we
show that the Sun has the lowest Li abundance in comparison with solar twins at similar age
(4.6 ± 0.5 Gyr). We compare the lithium content with the condensation temperature slope for a
subsample of the best solar twins and determine that the most lithium-depleted stars also have
fewer refractory elements. We speculate whether the low lithium content in the Sun might be
related to the particular configuration of our Solar system.
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Monthly Notices of the Royal Astronomical Society
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