作者: A. W. Phelps
DOI:
关键词: Astrobiology 、 Condensation 、 Diamond 、 Nucleation 、 Formation and evolution of the Solar System 、 Xenon 、 Diamond dust 、 Materials science
摘要: Introduction: The formation mechanism(s) of meteoritic and interstellar diamond dust grains has been a subject debate for many years but few explanations have provided the predictive tools with which to further explore understand grain by direct astronomical observation. discovery that some these diamonds carry presolar isotopic xenon ratios means they survived intact since before solar system.