The main focus
behind my research has been the development of scientific and measurement
criteria for the unambiguous detection of life in early earth and Mars samples
and future robotic and sample return missions to Mars as well as missions to
Europa and Enceladus. This has evolved into a three-pronged approach of
laboratory investigations using a diverse range of techniques and samples
coupled with development and testing of instrumentation for future Mars
missions and the characterisation of data from space flight missions to Earth
orbit, Mars and Comets. The scientific underpinning of this work has
revolved around the establishment of a “null hypothesis” to life detection that
relies on accurately cataloguing non-biological morphological and organic
chemical input to a particular sample. My laboratory work has concentrated on
samples as diverse as Apex chert, Strelley pool chert, Isua, Akilia, Gunflint
samples as well as mantle xenoliths, fossil lagerstatten
(Enspel, Messel) Martian meteorites, Apollo return samples, ordinary and
carbonaceous chondrites, Stardust, ureilites and inclusions in diamonds. Principally
I use a combination of light microscopy with high resolution scanning confocal
Raman spectroscopy to initially survey samples of interest. The search for life
cannot be accomplished with confidence in one particular measurement and as
such multiple analysis techniques must be used on the same sample to give a
convincing answer. Due to this I have developed the capability to use and
interpret data from a wide range of instrumental techniques including; Atomic
Force Microscopy, Scanning and Transmission Electron Microscopy, FTIR
spectroscopy, Isotope Ratio Mass Spectroscopy, Time of Flight Secondary Ion
Mass Spectrometry, Gas Chromatography Mass Spectrometry, Electron and Ion Microprobes,
X-ray elemental and Diffraction analysis (EDX and XRD), microbial culturing and
aseptic technique, biomolecule extraction, DNA amplification, Lab-on-a-chip
microfluidic capillary electrophoresis and metabolism and endotoxin analysis. I
have been instrumental in developing several of the latter techniques for
robust use in field conditions and was a part of a team using non-culture based
methods on the International Space Station. My laboratory work with a range of
co-investigators has led to some significant discoveries including; lunar
graphite, new carbon allotropes in meteorites, the detection of 4 abiogenic
organic carbon synthesis mechanism on Mars, as well as water in lunar and
Martian rocks. This year I have also been part of the COSAC instrument team
onboard the Philae lander on the ESA Rosetta mission. By following the trail of
abiotic carbon I have also become very interested in the terrestrial and
Martian deep carbon cycles. My current work is focussing on what appears to be
an explanation for reduced carbon species within the terrestrial and Martian
mantles, following the unambiguous discovery of organic carbon in Martian
meteorites. Currently I am also a co-investigator on
the Sample Analysis at Mars (SAM) instrument onboard the Curiosity. My duties have
been to rapidly assess data products and help in the development of science
plans to undertake the search for organic material on Mars. These studies will
continue and extend my current mission involvement in the Curiosity and Rosetta
missions to the Mars 2020 mission as a co-investigator on the SHELOC instrument
and hopefully after samples return from Mars. My future goals
are to continue to address the problems of early and extraterrestrial life
detection using all the tools at my disposal. I will to continue to augment the
techniques I have with new cutting edge technologies, including instrument
concepts that I have been developing. I would in the near future like to integrate
high resolution electron imaging, Confocal Raman spectroscopy and augment that with
Time of Flight SIMS instrument capable of in-situ organic compound
characterisation and preparation. This instrument initially funded for a short
feasibility study by the DCO has become a commercial reality and this kind of
cutting edge technology would address many of my own and my colleagues science
problems. Furthermore, in an
effort to continue setting an abiotic baseline for the detection of life myself
and collaborators have been undertaking high pressure and temperature
experiments into organic carbon production during the cooling of silicate
melts. I am currently funded to undertake these experiments through a NASA
grant and we will continue to vary temperature, composition and oxygen fugacity
parameters to characterise possible organic synthesis reactions in these
systems. Finally, I am also exploring a further line of research that I have recently begun, to probe the reactions that could lead to the transition of abiotic chemistry to prebiotic chemistry and then life. At this time this work has involved bioinformatics research into the nature of protein nucleic acid interactions that could have led to the first proto-life molecular constructs that led to information exchange and storage under the conditions that formed life on earth. It is my goal to transport this in-silico work into a number of laboratory experiments that would shed light on the origin of protein / nucleic acid interactions. |