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Cited by 451

The DOI matches its Crossref record; 41 of the 41 references it cites were found in a registry or an index.

THE PECULIAR SOLAR COMPOSITION AND ITS POSSIBLE RELATION TO PLANET FORMATION

Open access
Meléndez, J., Asplund, M., Gustafsson, B., Yong, D.·2009·The Astrophysical Journal

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 catalog 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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Metadata

Authors
Meléndez, J., Asplund, M., Gustafsson, B., & Yong, D.
Venue
The Astrophysical Journal
Published
2009-09-25
Volume
704
Issue
1
Pages
L66-L70
ISSN
  • 0004-637X (ISSN-L)
  • 1538-4357
OpenAlex
W2066293328
Cited by
451
References
41
FWCI
13.36
Type
journal article
Language
en
Open access
bronze

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CoChat. (2026). Citation check: THE PECULIAR SOLAR COMPOSITION AND ITS POSSIBLE RELATION TO PLANET FORMATION. https://app.cochat.ai/papers/10.1088/0004-637x/704/1/l66
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Meléndez, J., Asplund, M., Gustafsson, B., & Yong, D. (2009). THE PECULIAR SOLAR COMPOSITION AND ITS POSSIBLE RELATION TO PLANET FORMATION. The Astrophysical Journal. https://doi.org/10.1088/0004-637x/704/1/l66

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