
Teresa Fornaro
Main scientific activity pertains to Astrobiology, focusing on experimental and theoretical studies for detection of biomarkers on Mars. These studies primarily support the scientific investigations and technology development of Mars Organics Molecule Analyser (MOMA) instrument on board the European Space Agency (ESA) ExoMars 2020 space mission, devoted to detection of a wide range of organic molecules, operating in two modes, i.e. laser desorption ionization- and gas chromatography- mass spectrometry.
Specifically, new protocols are developed in laboratory to adsorb biomarkers onto mineral matrices, in order to study the physico-chemical interactions characterizing such molecule-mineral complexes, and prepare Mars soil analogues for payload tests.
The thermodynamics of the adsorption process is examined both experimentally, determining equilibrium adsorption isotherms, and computationally through quantum mechanical and surface complexation modelling, by using CRYSTAL and GEOSURF software, respectively.
Sample characterization is carried out experimentally by means of several analytical techniques, such as Infrared and Raman vibrational spectroscopies, UV-vis spectrophotometry, High Performance Liquid Chromatography - Mass Spectrometry (HPLC-MS), Ion Chromatography (IC), Scanning Electron Microscopy (SEM), Transmission Electron Microscopy (TEM), X-Ray Diffraction (XRD).
The experimental measurements are integrated by computational quantum mechanical spectroscopy studies in order to assess the various contributions to the overall spectroscopic signals due to different molecule-mineral interactions and correctly assign the experimental spectroscopic features. This is achieved by using a virtual multi-frequency spectrometer covering rotational, vibrational, electronic, as well as magnetic resonance spectral ranges, implemented in the GAUSSIAN suite of programs.
Moreover, photochemistry of molecules adsorbed on minerals is investigated under Martian-like conditions through UV irradiation processing. The degradation kinetics under Martian-like conditions is inspected taking into account possible catalytic and/or protective effects of minerals.
After preparation, UV processing and characterization of Martian analogues, high-sensitivity tests of MOMA instrument are performed at NASA - Goddard Space Flight Centre (USA), to evaluate the detection limits of MOMA instrument for organic molecules that are considered biomarkers of extant or extinct life, and optimize the instrument parameters in order to improve detection efficiency.
In addition, experience is gained in the development of liquid extraction protocols of biomarkers adsorbed on minerals for in situ biosensor-based life detection technologies, specifically the Life Marker Chip (LMC) instrument on board ExoMars space mission, which is an antibody microarray biosensor instrument with optical readout that uses fluorescently labelled antibodies to detect and quantify the presence of polar and non-polar biomolecules extracted from the Martian soil.
Further activity concerns the study of properties of surface materials of primitive carbon-rich asteroids to support NASA OSIRIS-REX sample return space mission. In particular, criteria and procedures for selection of representative analogue material to be present on primitive carbon-rich asteroids are identified. Characterization of surface properties of primitive carbon-rich asteroids is performed to allow a direct comparison with ground-based observations and laboratory spectroscopic studies. Planetary protection activities are carried out in order to study chemical contamination of samples.
Supervisors: John Robert Brucato
Specifically, new protocols are developed in laboratory to adsorb biomarkers onto mineral matrices, in order to study the physico-chemical interactions characterizing such molecule-mineral complexes, and prepare Mars soil analogues for payload tests.
The thermodynamics of the adsorption process is examined both experimentally, determining equilibrium adsorption isotherms, and computationally through quantum mechanical and surface complexation modelling, by using CRYSTAL and GEOSURF software, respectively.
Sample characterization is carried out experimentally by means of several analytical techniques, such as Infrared and Raman vibrational spectroscopies, UV-vis spectrophotometry, High Performance Liquid Chromatography - Mass Spectrometry (HPLC-MS), Ion Chromatography (IC), Scanning Electron Microscopy (SEM), Transmission Electron Microscopy (TEM), X-Ray Diffraction (XRD).
The experimental measurements are integrated by computational quantum mechanical spectroscopy studies in order to assess the various contributions to the overall spectroscopic signals due to different molecule-mineral interactions and correctly assign the experimental spectroscopic features. This is achieved by using a virtual multi-frequency spectrometer covering rotational, vibrational, electronic, as well as magnetic resonance spectral ranges, implemented in the GAUSSIAN suite of programs.
Moreover, photochemistry of molecules adsorbed on minerals is investigated under Martian-like conditions through UV irradiation processing. The degradation kinetics under Martian-like conditions is inspected taking into account possible catalytic and/or protective effects of minerals.
After preparation, UV processing and characterization of Martian analogues, high-sensitivity tests of MOMA instrument are performed at NASA - Goddard Space Flight Centre (USA), to evaluate the detection limits of MOMA instrument for organic molecules that are considered biomarkers of extant or extinct life, and optimize the instrument parameters in order to improve detection efficiency.
In addition, experience is gained in the development of liquid extraction protocols of biomarkers adsorbed on minerals for in situ biosensor-based life detection technologies, specifically the Life Marker Chip (LMC) instrument on board ExoMars space mission, which is an antibody microarray biosensor instrument with optical readout that uses fluorescently labelled antibodies to detect and quantify the presence of polar and non-polar biomolecules extracted from the Martian soil.
Further activity concerns the study of properties of surface materials of primitive carbon-rich asteroids to support NASA OSIRIS-REX sample return space mission. In particular, criteria and procedures for selection of representative analogue material to be present on primitive carbon-rich asteroids are identified. Characterization of surface properties of primitive carbon-rich asteroids is performed to allow a direct comparison with ground-based observations and laboratory spectroscopic studies. Planetary protection activities are carried out in order to study chemical contamination of samples.
Supervisors: John Robert Brucato
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