THE PECULIAR SOLAR COMPOSITION AND ITS POSSIBLE RELATION TO PLANET FORMATION

被引:304
作者
Melendez, J. [1 ]
Asplund, M. [2 ]
Gustafsson, B. [3 ]
Yong, D. [4 ]
机构
[1] Univ Porto, Ctr Astrofis, P-4150762 Oporto, Portugal
[2] Max Planck Inst Astrophys, D-85741 Garching, Germany
[3] Uppsala Univ, Inst Fys Astron, SE-75120 Uppsala, Sweden
[4] Australian Natl Univ, Res Sch Astron & Astrophys, Mt Stromlo Observ, Weston, ACT 2611, Australia
基金
瑞典研究理事会; 澳大利亚研究理事会;
关键词
planetary systems; solar system: formation; stars: abundances; Sun: abundances; PRE-MAIN-SEQUENCE; EARLY EVOLUTION; GAS ACCRETION; NEARBY STARS; SUN; ABUNDANCE; SYSTEM; GRADIENTS; DISK; NUCLEOSYNTHESIS;
D O I
10.1088/0004-637X/704/1/L66
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We have conducted a differential elemental abundance analysis of unprecedented accuracy (similar to 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 approximate to 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.
引用
收藏
页码:L66 / L70
页数:5
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