Global S&T Development Trend Analysis Platform of Resources and Environment
DOI | 10.1126/science.abb3091 |
Bifurcation of planetary building blocks during Solar System formation | |
Tim Lichtenberg; Joanna Dra̧żkowska; Maria Schönbächler; Gregor J. Golabek; Thomas O. Hands | |
2021-01-22 | |
发表期刊 | Science |
出版年 | 2021 |
英文摘要 | Measurements of meteorites have shown that the inner and outer Solar System formed from two distinct reservoirs of material. Existing models have proposed that these were split by Jupiter forming first, which would open a gap in the protoplanetary disc. Lichtenberg et al. instead argue that the snow line, the boundary between regions containing water vapor and solid ice, migrated first outward and then inward, forming two separate populations of planetesimals. Those planetesimals then grew through collisions to form the planets. Their simulation of this model explains the meteorite data and is consistent with astronomical observations of protoplanetary disks around other stars. Science , this issue p. [365][1] Geochemical and astronomical evidence demonstrates that planet formation occurred in two spatially and temporally separated reservoirs. The origin of this dichotomy is unknown. We use numerical models to investigate how the evolution of the solar protoplanetary disk influenced the timing of protoplanet formation and their internal evolution. Migration of the water snow line can generate two distinct bursts of planetesimal formation that sample different source regions. These reservoirs evolve in divergent geophysical modes and develop distinct volatile contents, consistent with constraints from accretion chronology, thermochemistry, and the mass divergence of inner and outer Solar System. Our simulations suggest that the compositional fractionation and isotopic dichotomy of the Solar System was initiated by the interplay between disk dynamics, heterogeneous accretion, and internal evolution of forming protoplanets. [1]: /lookup/doi/10.1126/science.abb3091 |
领域 | 气候变化 ; 资源环境 |
URL | 查看原文 |
引用统计 | |
文献类型 | 期刊论文 |
条目标识符 | http://119.78.100.173/C666/handle/2XK7JSWQ/312360 |
专题 | 气候变化 资源环境科学 |
推荐引用方式 GB/T 7714 | Tim Lichtenberg,Joanna Dra̧żkowska,Maria Schönbächler,et al. Bifurcation of planetary building blocks during Solar System formation[J]. Science,2021. |
APA | Tim Lichtenberg,Joanna Dra̧żkowska,Maria Schönbächler,Gregor J. Golabek,&Thomas O. Hands.(2021).Bifurcation of planetary building blocks during Solar System formation.Science. |
MLA | Tim Lichtenberg,et al."Bifurcation of planetary building blocks during Solar System formation".Science (2021). |
条目包含的文件 | 条目无相关文件。 |
除非特别说明,本系统中所有内容都受版权保护,并保留所有权利。
修改评论