The shape of the Solar System has been a topic of fascination and debate among scientists. Recent studies on iron meteorites from the outer Solar System have shed light on its evolution. These meteorites are rich in refractory metals such as platinum and iridium, indicating a hot environment close to a forming star. This raises questions about their origin and movement within the Solar System.

According to researchers led by planetary scientist Bidong Zhang of the University of California Los Angeles, the composition of asteroids in the outer Solar System points towards a toroidal arrangement of the early Solar System. This challenges the traditional idea of a flat disk shaping the planets and other celestial bodies. The presence of metal-rich iron meteorites in the outer regions suggests a different mode of formation.

The formation of a planetary system involves the collapse of a molecular cloud of gas and dust under its own gravity. This leads to the birth of a protostar, surrounded by a spinning disk of material. Within this disk, smaller clumps form, eventually growing into planets or remaining as smaller objects like asteroids. Understanding the early stages of planetary system assembly can provide valuable insights into the evolution of our own Solar System.

The discovery of a toroidal shape in the early Solar System has significant implications for the study of other emerging planetary systems. By analyzing the composition of meteorites from different regions, scientists can gain a better understanding of how planets form and evolve around other stars. This information can help us piece together the puzzle of planetary system formation in the universe.

The study of iron meteorites from the outer Solar System has revealed a toroidal shape in the early stages of its evolution. This finding challenges previous theories and opens up new possibilities for understanding the formation of planets and other celestial bodies. By unraveling the mysteries of our own Solar System, scientists can unlock secrets about the vast universe beyond.

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