Catalytic Origins of Organic Compounds in Extraterrestrial Space
Lead Research Organisation:
University of Sheffield
Department Name: Chemical & Biological Engineering
Abstract
It has been proposed that organic compounds are formed in protostellar nebulae through heterogeneous catalytic reactions, analogous to Fischer-Tropsch synthesis. These reactions occur on mineral grain surfaces that are coated in carbonaceous deposits. The production of these organic compounds could be the necessary first step towards organic complexity and hence the evolution of life. This project will investigate the feasibility of such catalytic reactions by applying catalytic engineering methods to model systems of protostellar environments. This will provide reaction mechanism data with which to test the evolutionary hypothesis.
While carbon deposits ("coke") are more typically associated with catalyst deactivation, recent work from our laboratory and others have shown that they can also play an important beneficial role in a wide range of heterogeneously catalysed transformations. CO or CO2 hydrogenation (Fischer-Tropsch type catalysis) or nitrogen hydrogenation (analogous to the Haber-Bosch process) are two such processes. Metal-containing mineral grains e.g. iron-silicates, covered by carbonaceous deposits are hypothesised to catalyse these reactions in protstellar nebulae - extraterrestrial regions rich in organic matter and subject to 'high' temperatures (500-1000 K).
In order to develop structure-performance relationships model carbonaceous compounds, e.g. graphene oxide will also be investigated; while reaction studies will be extended to consider other processes where carbon laydown plays a beneficial role such as the non-oxidative and oxidative dehydrogenation of alkanes.
These results will shed light on the origin of complex organic species observed in extraterrestrial environments, but will also directly assist in the development of novel catalysts and processes for major industrial processes in the chemicals and fuels sectors. The department is currently developing a large-scale (1 l) Fischer-Tropsch reactor and this work will align closely with the development of that facility.
While carbon deposits ("coke") are more typically associated with catalyst deactivation, recent work from our laboratory and others have shown that they can also play an important beneficial role in a wide range of heterogeneously catalysed transformations. CO or CO2 hydrogenation (Fischer-Tropsch type catalysis) or nitrogen hydrogenation (analogous to the Haber-Bosch process) are two such processes. Metal-containing mineral grains e.g. iron-silicates, covered by carbonaceous deposits are hypothesised to catalyse these reactions in protstellar nebulae - extraterrestrial regions rich in organic matter and subject to 'high' temperatures (500-1000 K).
In order to develop structure-performance relationships model carbonaceous compounds, e.g. graphene oxide will also be investigated; while reaction studies will be extended to consider other processes where carbon laydown plays a beneficial role such as the non-oxidative and oxidative dehydrogenation of alkanes.
These results will shed light on the origin of complex organic species observed in extraterrestrial environments, but will also directly assist in the development of novel catalysts and processes for major industrial processes in the chemicals and fuels sectors. The department is currently developing a large-scale (1 l) Fischer-Tropsch reactor and this work will align closely with the development of that facility.
Organisations
People |
ORCID iD |
| James McGregor (Primary Supervisor) | |
| Hannah Woodward (Student) |