  The first complete infrared FTIR absorption spectra for carbonado-diamond
confirm the interstellar origin for the most enigmatic diamonds known as
carbonado. All previous attempts failed to measure the absorption of
carbonado-diamond in the most important IR-range of 1000-1300 cm-1 (10.00-7.69
micro-m.) because of silica inclusions. In our investigation, KBr pellets were
made from crushed silica-free carbonado-diamond and thin sections were also
prepared. The 100 to 1000 times brighter synchrotron infrared radiation permits
a greater spatial resolution. Inclusions and pore spaces were avoided and/or
sources of chemical contamination were removed. The FTIR spectra of
carbonado-diamond mostly depict the presence of single nitrogen impurities, and
hydrogen. The lack of identifiable nitrogen aggregates in the infrared spectra,
the presence of features related to hydrocarbon stretch bonds, and the
resemblance of the spectra to CVD and presolar diamonds indicate that
carbonado-diamonds formed in a hydrogen-rich interstellar environment. This is
consistent with carbonado-diamond being sintered and porous, with extremely
reduced metals, metal alloys, carbides and nitrides, light carbon isotopes,
surfaces with glassy melt-like patinas, deformation lamellae, and a complete
absence of primary, terrestrial mineral inclusions. The 2.6-3.8 billion year
old fragmented body was of asteroidal proportions.
