The peculiar solar composition and its possible relation to planet formation
Jorge Melendez (CAUP), Martin Asplund (MPA), Bengt Gustafsson, (Upssala), David Yong (Stromlo)

TL;DR
This study reveals the Sun's unique elemental abundance pattern, with a depletion of refractory elements compared to solar twins and analogs, potentially linked to planetary system formation.
Contribution
It provides the first high-precision differential abundance analysis showing the Sun's peculiar composition relative to solar twins and analogs, suggesting a connection to planet formation.
Findings
The Sun is depleted in refractory elements by about 20% compared to solar twins.
The abundance pattern correlates strongly with element condensation temperatures.
Solar analogs with close-in giant planets do not show this depletion pattern.
Abstract
We have conducted a differential elemental abundance analysis of unprecedented accuracy (0.01 dex) of the Sun relative to 11 solar twins from the Hipparcos catalogue and 10 solar analogs from planet searches. We find that the Sun shows a characteristic signature with a ~20% depletion of refractory elements relative to the volatile elements in comparison with the solar twins. The abundance differences correlate strongly with the condensation temperatures of the elements. This peculiarity also holds in comparisons with solar analogs known to have close-in giant planets while the majority of solar analogs found not to have such giant planets in radial velocity monitoring show the solar abundance pattern. We discuss various explanations for this peculiarity, including the possibility that the differences in abundance patterns are related to the formation of planetary systems like our own,…
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