Researchers from the School of Geographical & Earth Sciences have contributed to a new study of a Martian meteorite which could provide insights into the reactions that led to the building blocks of life on early Earth.
The study, led by the Carnegie Institution for Science and , demonstrates that organic molecules found in a meteorite that hurtled to Earth from Mars were synthesized during interactions between water and rocks that occurred on the Red Planet about 4 billion years ago.
The meteorite, called Allan Hills (ALH) 84001, was discovered in the Antarctic in 1984 and is considered one of the oldest known projectiles to reach Earth from Mars.
Organic molecules contain carbon and hydrogen, and sometimes include oxygen, nitrogen, sulfur, and other elements. Organic compounds are commonly associated with life, although they can be created by non-biological processes as well, which are referred to as abiotic organic chemistry.
For years, scientists have debated the origin story for the organic carbon found in the Allan Hills 84001 meteorite, with possibilities including various abiotic process related to volcanic activity, impact events on Mars, or hydrological exposure, as well as potentially the remnants of ancient life forms on Mars or contamination from its crash landing on Earth.
University of Glasgow planetary scientists Dr Lydia Hallis and Áine O’Brien and were part of the international research team which conducted the analysis on the meteorite.
The researchers used a variety of sophisticated sample preparation and analysis techniques-including co-located nanoscale imaging, isotopic analysis, and spectroscopy-to reveal the origin of organic molecules in the Allan Hills 84001 meteorite.
PhD candidate Áine’s involvement with the project began at the start of her postgraduate study, when she received frunding from the University to travel to Washington, DC to collaborate with principal investigator Prof Andrew Steele at the the Carnegie Institution for Science. Then, supported by funding from the Science and Technology Facilities Council (STFC), Áine, Dr Hallis and Prof Steele analysed samples at the STFC Diamond light source, a giant synchrotron in Oxfordshire.
Áine said: "This is a really significant paper, which uncovers vital new clues as to how these organic molecules were formed on the Allan Hills meteorite. I’m very proud to have been involved in the research, and grateful to the University and STFC for the support that made it possible for me to contribute. Being involved in a study like this as an early-career researcher is fantastic and I’m looking forward to building on this experience."
The research team found evidence of water-rock interactions similar to those that happen on Earth. The samples indicate that the Martian rocks experienced two important geochemical processes. One, called serpentinization, occurs when ironor magnesium-rich igneous rocks chemically interact with circulating water, changing their mineralogy and producing hydrogen in the process. The other, called carbonization, involves interaction between rocks and slightly acidic water containing dissolved carbon dioxide and results in the formation of carbonate minerals.
It is unclear whether these processes were induced by surrounding aqueous conditions simultaneously or sequentially, but the evidence indicates that the interactions between water and rocks did not occur over a prolonged period. What is evident, however, is that the reactions produced organic material from the reduction of carbon dioxide.
These mineralogical features are rare in Martian meteorites, and while carbonation and serpentinization have been shown in orbital surveys of Mars and carbonation has been found in other, less-ancient, Martian meteorites, this is the first instance of these processes occurring in samples from ancient Mars. Organic molecules have been detected by Steele in other Martian meteorites and from his work with the Sample Analysis at Mars (SAM) team on the Curiosity rover, indicating that abiotic synthesis of organic molecules has been a part of Martian geochemistry for much of the planet’s history.
Dr Andrew Steele, of the Carnegie Institution for Science, said: "These kinds of non-biological, geological reactions are responsible for a pool of organic carbon compounds from which life could have evolved and represent a background signal that must be taken into consideration when searching for evidence of past life on Mars.
"Furthermore, if these reactions happened on ancient Mars, they must have happened on ancient Earth, and could possibly explain the results we’ve from Saturn’s moon Enceladus as well. All that is required for this type of organic synthesis is for a brine that contains dissolved carbon dioxide to percolate through igneous rocks. The search for life on Mars is not just an attempt to answer the question ’are we alone’’ It also relates to early Earth environments and addresses the question of ’where did we come from’’"
The Steele-led team also included Carnegie’s Larry Nittler, Jianhua Wang, Pamela Conrad, Suzy Vitale, and Vincent Riggi as well as researchers from GFZ German Research Centre for Geosciences, Free University of Berlin, NASA Johnson Space Center, NASA Ames Research Center, and Rensselaer Polytechnic Institute.