Important discoveries in science are often made by accident. This was certainly the case in
the discovery of C
. Recall that Smalley and Kroto set out to simulate the atmospheric
conditions in carbon-rich red giant stars in order to address the question of whether linear cyanopolyynes
could form under these conditions. They were, in fact, able to answer their original question in the
affirmative. But more significantly, they refused to ignore the large unexpected peaks at m/e 720 and 840
in their mass spectra. Smalley and Kroto had the insight to recognize the significance of these peaks, and
that insight is what opened the field of fullerene science.
It is interesting that in the year prior to Kroto and Smalley's seminal paper in Nature, scientists at
Exxon (Rohlfing, 1984) had observed and published the time-of-flight mass spectrum of carbon clusters generated by laser vaporization of graphite. However, the Exxon group failed to appreciate
the significance of the enhanced peaks due to C
and C
and
failed to recognize that all of the high mass clusters were closed carbon cages.
Serendipity also played a role in Krätschmer and Huffman's breakthrough discovery of how to
synthesize macroscopic quantities of C
. Krätschmer and Huffman were originally interested
in generating graphite "soot" in the lab in order to compare its spectral properties with those of interstellar
carbon dust. They observed four unexpected (albeit weak) bands in the infrared spectrum of their "soot".
Again, their insight allowed them to recognize the significance of this observation, which in turn led to
their development of a large-scale isolation procedure.
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