Influence of Cu:Fe ratio in synthesis of higher alcohols from syngas over CuFeCoK/attapulgite catalysts

Abstract
Synthesis of higher alcohols from syngas (H2:CO ratio 2 and 1) was performed at 225–300 °C and 30 bar over copper, iron and cobalt containing catalysts supported on attapulgite and promoted with potassium. The Cu:Fe ratio was varied to study its influence on the syngas conversion and product distribution. It was found that while the copper rich catalyst 17Cu3FeCoK/attapulgite resulted in higher selectivity to the undesired alkanes with methane as the major one, the iron rich 3Cu17FeCoK/attapulgite was more selective towards alkenes. Selectivity to CO2 was independent on the Cu:Fe ratio tested in this work. With the higher H2:CO ratio (i.e. 2) selectivity to the liquid products increased with the increasing iron content. Moreover, a higher iron content in the catalyst improved formation of higher alcohols while the α-value reflecting the chain growth probability was more or less independent on the catalyst type.
Main Authors
Format
Articles Research article
Published
2024
Series
Subjects
Publication in research information system
Publisher
Elsevier
The permanent address of the publication
https://urn.fi/URN:NBN:fi:jyu-202408155519Use this for linking
Review status
Peer reviewed
ISSN
2950-6492
DOI
https://doi.org/10.1016/j.apcato.2024.206972
Language
English
Published in
Applied Catalysis O: Open
Citation
  • Aho, A., Lind, N., Virtanen, P., Mäki-Arvela, P., Eränen, K., Granroth, S., Korpelin, V., Honkala, K., Russo, V., Simakova, I., & Murzin, D. Y. (2024). Influence of Cu:Fe ratio in synthesis of higher alcohols from syngas over CuFeCoK/attapulgite catalysts. Applied Catalysis O: Open, 193, Article 206972. https://doi.org/10.1016/j.apcato.2024.206972
License
CC BY 4.0Open Access
Additional information about funding
This work is part of the activities of the Johan Gadolin Process Chemistry Centre at Åbo Akademi University. Funding from Business Finland through the SynJet project is greatly acknowledged. Materials research infrastructure/Department of Physics and Astronomy, University of Turku is gratefully acknowledged for a possibility to use their XPS.
Copyright© 2024 the Authors

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