dc.contributor.author |
Moroeng, Ofentse M.
|
|
dc.contributor.author |
Mhuka, Vimbai
|
|
dc.contributor.author |
Nindi, Mathew M.
|
|
dc.contributor.author |
Roberts, R.J. (James)
|
|
dc.contributor.author |
Wagner, Nicola J.
|
|
dc.date.accessioned |
2020-03-24T06:53:56Z |
|
dc.date.available |
2020-03-24T06:53:56Z |
|
dc.date.issued |
2019-12 |
|
dc.description.abstract |
This study aims to compare iso-rank vitrinite-rich and inertinite-rich coal samples to understand the impact of
coal-forming processes on pyrolysis chemistry. A medium rank C bituminous coal was density-fractionated to create a
vitrinite-rich and an inertinite-rich sub-sample. The vitrinite-rich sample has 83 vol% total vitrinite (mineral-matter-free
basis), whereas the inertinite-rich counterpart has 66 vol% total inertinite. The vitrinite-rich sample is dominated by
collotelinite and collodetrinite. Fusinite, semifusinite, and inertodetrinite are the main macerals of the inertinite-rich
sample. Molecular chemistry was assessed using a pyrolysis gas chromatograph (py-GC) equipped with a thermal desorption
unit coupled to a time of flight mass spectrometer (MS) (py-GC/MS) and solid-state nuclear magnetic resonance
(13C CP-MAS SS NMR). The pyrolysis products of the coal samples are generally similar, comprised of low and high
molecular weight alkanes, alkylbenzenes, alkylphenols, and alkyl-subtituted polycyclic aromatic hydrocarbons, although
the vitrinite-rich sample is chemically more diverse. The lack of diversity exhibited by the inertinite-rich sample upon
pyrolysis may be interpreted to suggest that major components were heated in their geologic history. Based on the 13C CPMAS
SS NMR analysis, the inertinite-rich sample has a greater fraction of phenolics, reflected in the py-GC/MS results as
substituted and unsubstituted derivatives. The greater abundance of phenolics for the inertinite-rich sample may suggest a
fire-related origin for the dominant macerals of this sample. The C2-alkylbenzene isomers (p-xylene and o-xylene) were
detected in the pyrolysis products for the vitrinite-rich and inertinite-rich samples, though more abundant in the former.
The presence of these in both samples likely reflects common source vegetation for the dominant vitrinite and inertinite
macerals. |
en_ZA |
dc.description.department |
Geology |
en_ZA |
dc.description.librarian |
am2020 |
en_ZA |
dc.description.sponsorship |
The Research, Education and Investment (REI)
Fund of the Geological Society of South Africa (GSSA), National
Research Foundation of South Africa (NRF), and the University of
Johannesburg’s (UJ) Centre of Excellence for Integrated Mineral and
Energy Resource Analysis (CIMERA). |
en_ZA |
dc.description.uri |
https://link.springer.com/journal/40789 |
en_ZA |
dc.identifier.citation |
Moroeng, O.M., Mhuka, V., Nindi, M.M. et al. Comparative study of a vitrinite-rich and an inertinite-rich Witbank coal (South Africa) using pyrolysis-gas chromatography. International Journal of Coal Science and Technology 6, 621–632 (2019). https://doi.org/10.1007/s40789-019-00274-3. |
en_ZA |
dc.identifier.issn |
2095-8293 (print) |
|
dc.identifier.issn |
2198-7823 (online) |
|
dc.identifier.other |
10.1007/s40789-019-00274-3 |
|
dc.identifier.uri |
http://hdl.handle.net/2263/73820 |
|
dc.language.iso |
en |
en_ZA |
dc.publisher |
SpringerOpen |
en_ZA |
dc.rights |
© The Author(s) 2019. Open Access. This article is distributed under the terms of the Creative Commons Attribution 4.0 International License (http://creativecommons.org/licenses/by/4.0/). |
en_ZA |
dc.subject |
y-TD-GC-TOFMS |
en_ZA |
dc.subject |
Main Karoo Basin |
en_ZA |
dc.subject |
Pyrolysis products |
en_ZA |
dc.subject |
13C CP-MAS SS NMR |
en_ZA |
dc.subject |
Molecular chemistry |
en_ZA |
dc.subject |
Phenolics |
en_ZA |
dc.subject |
Xylene (C2-alkylbenzene) isomers |
en_ZA |
dc.subject |
Pyrolysis gas chromatograph (py-GC) |
en_ZA |
dc.title |
Comparative study of a vitrinite-rich and an inertinite-rich Witbank coal (South Africa) using pyrolysis-gas chromatography |
en_ZA |
dc.type |
Article |
en_ZA |