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September 22, 2000"The Egg as Eye: Ultrananocrystalline Diamond in the Cosmos
and in the Laboratory" Synthesis of ultrananocrystalline diamond (UNCD) films has been accomplished in the laboratory making use of carbon dimer, C2, produced by fragmentation of C60. Interestingly, UNCD had been found in several primitive carbonaceous chondrites where it is the largest constituent of the presolar grain fraction in this class of meteorites. During the late stages of red giant stellar evolution, so-called planetary nebulae with lifetimes of ~ 104 years form. Although these objects have been known for over 200 years, their progenitors, called protoplanetary nebulae (PPNs) with lifetimes of ~ 103 years, were discovered only within the last 25 years. Many PPNs such as the Egg Nebula have intense C2 absorption bands. It is suggested that the synthesis of UNCD in the laboratory and in the cosmos proceeds on the basis of new growth and nucleation mechanisms involving the insertion of C2 into and carbon- hydrogen bonds. The carrier of the intense 21 µm emission is almost certainly a carbon containing material, and the possibility that UNCD is the carrier will be discussed. Carbon dimer, the small-est all-carbon molecule, is extremely reactive and can give rise to complex chemistries involving H, O, N, and other elements. The PPNs may, therefore, be viewed as cradles of chemistry providing insights into the earliest stages of cosmicchemical evolution. Addenda to the Sept. SMSI meeting: The meeting abstract is an excellent review of the talk. This time the recording secretary is only going to add notes to refresh the talk. Sources cited in the talk are:
Respectfully submitted, Stan Schmidt. | ||
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