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The peculiar solar composition and its possible relation to planet formation
Solar and Stellar Astrophysics · Submitted 12 Sep 2009
abstract compiled · 2026-09-23 · no language-model review
The authors' main claim 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, in particular to the existence of terrestrial planets.
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The abstract, sentence by sentence
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, in particular to the existence of terrestrial planets.
background contribution method result interpretation main claim
| # | sentence | role | the authors' own work | states the main conclusion | strength |
|---|---|---|---|---|---|
| s0 | 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. | method 0.62 | 0.97 | 0.03 | asserted 1.00 |
| s1 | 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. | result 1.00 | 0.97 | 0.68 | asserted 1.00 |
| s2 | The abundance differences correlate strongly with the condensation temperatures of the elements. | result 1.00 | 0.90 | 0.13 | asserted 1.00 |
| s3 | 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. | result 0.99 | 0.83 | 0.32 | asserted 1.00 |
| s4 | 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, in particular to the existence of terrestrial planets. | interpretation 1.00 | 0.32 | 0.22 | hedged possibility 0.88 |
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The paper
Original 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, in particular to the existence of terrestrial planets.
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References
How later papers used it
64 later papers cite it
1 later paper by other authors is listed below: 1 used its data or values. 2 more papers by the same authors are listed: 2 used its method or tool.
Uses its method or tool 2 of 6 papers with this label · 2 by the same authors
By the same authors
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Followed this paper to calculate the abundances of a typical solar twin and compare this abundance pattern to that of the Sun.
The Chemical Homogeneity of Sun-like Stars in the Solar Neighborhood (2018) (same authors) · 0.86 · paraphrased: the licence does not allow quoting
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Used the differential analysis techniques pioneered by this paper to obtain high precision relative chemical abundance measurements of a large sample of co-moving pairs of stars.
C3PO: Towards a complete census of co-moving pairs of stars. I. High precision stellar parameters for 250 stars (2023) (same authors) · 1.00 · paraphrased: the licence does not allow quoting
Uses its data or values 1 of 4 papers with this label
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Used this paper's average of the solar twins of 0.04 dex, or 10 per cent, to compare the photospheric composition of models with a planet to a reference model without planets.
Fingerprints of giant planets in the composition of solar twins (2020) · 0.84 · paraphrased: the licence does not allow quoting
How the literature uses it
4 arXiv papers cite this in 8 sentences
Papers whose main result relates to this one's
States the same result 1 paper
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The peculiarities in the solar chemical composition can be explained as signatures of the formation of terrestrial planets like our own Earth.
Unprecedented accurate abundances: signatures of other Earths? · 0.93
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