Determination of the molecular structure
of asphaltenes, especially
in their native environment, is a formidable challenge in petroleum
chemistry. Here we demonstrate that a combination of different spectroscopy
and imaging based experimental techniques can be utilized to determine
structures of asphaltenes, which have precipitated out of a crude
oil, in an environment similar to real field conditions. A high pressure–high
temperature quartz crystal microbalance (HPHT-QCM) setup can be used
to detect asphaltene onset at oil production conditions. HPHT-QCM
can also simulate CO2 injection conditions mimicking gas
injection methods used to enhance oil recovery from depleted oil reservoirs.
In this paper, we present the first compositional and structural research
study on the QCM asphaltene deposits under gas injection conditions
and compare it to n-C7 asphaltenes from
the same crude oil precipitated in the laboratory. This study combines
the use of Fourier transform infrared (FTIR) spectroscopy, nuclear
magnetic resonance (NMR), environmental scanning electron microscopy
(ESEM), and energy dispersive X-ray (EDX) analysis. Furthermore, deposits
collected from chemically treated fluids were also studied. The HPHT-QCM
asphaltene deposits from parent crude oil are richer in oxygen species,
such as the O
x
and R–OH polar groups,
relative to the n-C7 asphaltenes. The
results of this study provide high-pressure information that leads
to better understanding of asphaltene precipitation and deposition
phenomena and could be taken into account when designing prevention
strategies to avoid asphaltene problems throughout the oil production
process.