Mineralogy of Basaltic Material on the Minor Bodies of Our Solar System
作者： Ren Duffard
DOI: 10.5772/35808
关键词:
摘要: Our modern understanding of the formation solar system is that it began in a cold cloud gas and dust under conditions similar to other nebulae. After dissipation dust, nebula continues evolve as planetesimals form larger bodies. In process, these bodies are heated by collisions radioactive decay. Asteroids remnants could not bigger planet. The materials currently present asteroids most primitive, less evolved one, that’s why important understand.
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