从陨石推断和经过电脑软件确认可行,行星的形成过程应该如此.首先,灰尘微粒聚集在一起形成宇宙尘球.早期太阳的热量爆发将这些尘球熔化,它们因此固化为陨石球粒.
First, dust particles clumped together to form cosmic dustballs. Bursts of heat from the primitive sun melted the dustballs, which solidified into chondrules.
一些人说，因为看起来该行星在它形成的早期已经迅速冷却，它的核心已经固化，磁场只是留在岩石中的剩余部分。
Some say because the planet appears to have cooled rapidly early in its history, its core has solidified and any magnetic field is a remnant captured in rocks.
该组合物在成型的早期阶段提供改善的和可重现的流动而不损害固化时间。
The composition provides improved and reproducible flow during the early stages of molding without compromising curing time.
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