Garai, Jozsef; Haggerty, Stephen E.; Rekhi, Sandeep; Chance, Mark. Infrared Absorption Investigations Confirm the Extraterrestrial Origin of Carbonado-Diamonds. The Astrophysical Journal. 2006-12-20, 653 (2): L153–L156. Bibcode:2006ApJ...653L.153G. ISSN 0004-637X. arXiv:physics/0608014. doi:10.1086/510451. (原始内容存档于2007-08-09) (英语). 引文格式1维护:日期与年 (link)。
研究顯示這些黑鑽石的紅外線吸收頻譜與地外來源的鑽石的吸收頻譜近似;
selected significant peaks are due to trace abundances of the elements 氮 and 氢.
The researchers concluded with the assumption that the mineral necessarily formed in an interstellar environment. In this sense, carbonado are theorized to be akin to carbon-rich cosmic dust, likely having formed in an environment near carbon stars. The diamonds were suggested to have been fragments of a body of asteroid size that subsequently fell to Earth as meteorites.
doi.org
Heaney, P. J.; Vicenzi, E. P.; De, S. Strange Diamonds: the Mysterious Origins of Carbonado and Framesite. Elements. 2005, 1 (2): 85. doi:10.2113/gselements.1.2.85.
Garai, Jozsef; Haggerty, Stephen E.; Rekhi, Sandeep; Chance, Mark. Infrared Absorption Investigations Confirm the Extraterrestrial Origin of Carbonado-Diamonds. The Astrophysical Journal. 2006-12-20, 653 (2): L153–L156. Bibcode:2006ApJ...653L.153G. ISSN 0004-637X. arXiv:physics/0608014. doi:10.1086/510451. (原始内容存档于2007-08-09) (英语). 引文格式1维护:日期与年 (link)。
研究顯示這些黑鑽石的紅外線吸收頻譜與地外來源的鑽石的吸收頻譜近似;
selected significant peaks are due to trace abundances of the elements 氮 and 氢.
The researchers concluded with the assumption that the mineral necessarily formed in an interstellar environment. In this sense, carbonado are theorized to be akin to carbon-rich cosmic dust, likely having formed in an environment near carbon stars. The diamonds were suggested to have been fragments of a body of asteroid size that subsequently fell to Earth as meteorites.
Garai, Jozsef; Haggerty, Stephen E.; Rekhi, Sandeep; Chance, Mark. Infrared Absorption Investigations Confirm the Extraterrestrial Origin of Carbonado-Diamonds. The Astrophysical Journal. 2006-12-20, 653 (2): L153–L156. Bibcode:2006ApJ...653L.153G. ISSN 0004-637X. arXiv:physics/0608014. doi:10.1086/510451. (原始内容存档于2007-08-09) (英语). 引文格式1维护:日期与年 (link)。
研究顯示這些黑鑽石的紅外線吸收頻譜與地外來源的鑽石的吸收頻譜近似;
selected significant peaks are due to trace abundances of the elements 氮 and 氢.
The researchers concluded with the assumption that the mineral necessarily formed in an interstellar environment. In this sense, carbonado are theorized to be akin to carbon-rich cosmic dust, likely having formed in an environment near carbon stars. The diamonds were suggested to have been fragments of a body of asteroid size that subsequently fell to Earth as meteorites.
Garai, Jozsef; Haggerty, Stephen E.; Rekhi, Sandeep; Chance, Mark. Infrared Absorption Investigations Confirm the Extraterrestrial Origin of Carbonado-Diamonds. The Astrophysical Journal. 2006-12-20, 653 (2): L153–L156. Bibcode:2006ApJ...653L.153G. ISSN 0004-637X. arXiv:physics/0608014. doi:10.1086/510451. (原始内容存档于2007-08-09) (英语). 引文格式1维护:日期与年 (link)。
研究顯示這些黑鑽石的紅外線吸收頻譜與地外來源的鑽石的吸收頻譜近似;
selected significant peaks are due to trace abundances of the elements 氮 and 氢.
The researchers concluded with the assumption that the mineral necessarily formed in an interstellar environment. In this sense, carbonado are theorized to be akin to carbon-rich cosmic dust, likely having formed in an environment near carbon stars. The diamonds were suggested to have been fragments of a body of asteroid size that subsequently fell to Earth as meteorites.
Garai, Jozsef; Haggerty, Stephen E.; Rekhi, Sandeep; Chance, Mark. Infrared Absorption Investigations Confirm the Extraterrestrial Origin of Carbonado-Diamonds. The Astrophysical Journal. 2006-12-20, 653 (2): L153–L156. Bibcode:2006ApJ...653L.153G. ISSN 0004-637X. arXiv:physics/0608014. doi:10.1086/510451. (原始内容存档于2007-08-09) (英语). 引文格式1维护:日期与年 (link)。
研究顯示這些黑鑽石的紅外線吸收頻譜與地外來源的鑽石的吸收頻譜近似;
selected significant peaks are due to trace abundances of the elements 氮 and 氢.
The researchers concluded with the assumption that the mineral necessarily formed in an interstellar environment. In this sense, carbonado are theorized to be akin to carbon-rich cosmic dust, likely having formed in an environment near carbon stars. The diamonds were suggested to have been fragments of a body of asteroid size that subsequently fell to Earth as meteorites.
Garai, Jozsef; Haggerty, Stephen E.; Rekhi, Sandeep; Chance, Mark. Infrared Absorption Investigations Confirm the Extraterrestrial Origin of Carbonado-Diamonds. The Astrophysical Journal. 2006-12-20, 653 (2): L153–L156. Bibcode:2006ApJ...653L.153G. ISSN 0004-637X. arXiv:physics/0608014. doi:10.1086/510451. (原始内容存档于2007-08-09) (英语). 引文格式1维护:日期与年 (link)。
研究顯示這些黑鑽石的紅外線吸收頻譜與地外來源的鑽石的吸收頻譜近似;
selected significant peaks are due to trace abundances of the elements 氮 and 氢.
The researchers concluded with the assumption that the mineral necessarily formed in an interstellar environment. In this sense, carbonado are theorized to be akin to carbon-rich cosmic dust, likely having formed in an environment near carbon stars. The diamonds were suggested to have been fragments of a body of asteroid size that subsequently fell to Earth as meteorites.