Passive Detection of Biological Aerosols in the Atmosphere with a Fourier Transform Instrument (FTIR)—the Results of the Measurements in the Laboratory and in the Field
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Fourier Transform Infrared Radiation (FTIR) spectroscopy is one of the most powerful methods for the detection of gaseous constituents, aerosols, and dust in planetary atmospheres. Infrared spectroscopy plays an important role in searching for biomarkers, organics and biological substances in the Universe. The possibility of detection and identifications with FTIR spectrometer of bio-aerosol spores (Bacillus atrophaeus var. globigii=BG) in the atmosphere is discussed in this paper. We describe the results of initial spectral measurements performed in the laboratory and in the field. The purpose of these experiments was to detect and to identify bio-aerosol spores in two conditions: 1) In a closed chamber where the thermal contrast between the background and aerosols was large, and 2) In open air where the thermal contrast between the background and aerosols was small. The extinction spectrum of BG spores was deduced by comparing our measurements with models, and other measurements known from the literature. Our theoretical and experimental studies indicate that, during passive remote sensing measurements, it is difficult—but possible to detect and to identify bio-aerosol clouds by their spectral signatures. The simple spectral analysis described in the paper can be useful for the detection of various kinds of trace aerosols—not only in the Earth’s atmosphere, but also during planetary missions in the environments of other astronomical objects such as planets, comets etc. We expect that the interpretation of data from spectrometric sounding of Venus and Mars during the current missions Mars and Venus Express, and later during the Rosetta mission will benefit from our experimental work and numerical modelling.
KeywordsBio-aerosols Spectroscopy Remote sensing of the atmosphere Astrobiology
Infrared spectrometric technique of the detection of main gaseous constituents, trace gases, various aerosols and dusts in the atmospheres of planets and environments of other objects (e.g. comets) in the Solar System is a well known research method. The spectrometers orbiting the Earth, Mars and Venus continuously give us new and interesting measurements to be interpreted. Envisat’s MIPAS, Sciamachy and GOMOS sensors are able to see holes in the ozone layer and the plumes of pollutants over industrial cities. Methane (CH4) (possibly of biological origin) in the atmosphere of Mars and molecular oxygen (O2) in the atmosphere of Venus have been detected using infrared spectroscopy.
There are over 120 molecular species discovered spectroscopicaly in the interstellar clouds. The most interesting one to astrobiologists is glycine, the simplest of life’s amino acids. About 10 to 30 % of the carbon in the interstellar medium is thought to be in the form of complex organic material PAH (polycyclic aromatic hydrocarbon) that matches the 3.4 μm infrared spectral feature attributed to CH bonds (Brownlee and Kress 2007). It is worth mentioning that PAHs are also present in the Martian meteorite ALH84001 (McKay et al. 1996) where microscopic forms that could be fossils of microbial life also exist.
Spectroscopy emerges as the most powerful tool available for the characterization of the composition and structure of atmospheres of exoplanets. Detection of molecules in the atmosphere of exoplanet has been demonstrated with the Hubble and Spitzer Space Telescopes for a transiting hot-Jupiter exoplanet. Water (H2O), methane (CH4), carbon dioxide (CO2), and carbon monoxide (CO) have been detected via infrared spectroscopy in emission spectrum of HD 189733b (Swain et al. 2008; Grillmair et al. 2007, 2008; Harrington et al. 2006). H2O, CH4, and CO2 may have potential biological significance, and thus their detection in a hot-Jupiter atmosphere is an important step in search for biomarkers and maybe for a simplest forms of life (Swain et al. 2009)
For most of Earth’s history, life was microscopic, and even now microorganisms dominate our planet in diverse and extreme environments (Shapiro 2007). For these reasons it is thought that if life exists in another place of the Universe, it might still be in the stage of microbial life.
FTIR spectroscopy has also been successfully applied in the laboratories for the detection, discrimination, identification, and classification of bacteria such as Listeria, Escherichia coli, Salmonella, Staphylococcus, and many others (Helm et al. 1991). FTIR spectroscopy is not only used as a method for bacterial identification, but it also provides information about bacterial metabolism, its growth phase, and it allows distinguishing between different serotypes (Davis and Mauer 2010).
An important conclusion of these briefly described results is that among various instruments selected to search for life spectrometers are well placed. No wonder therefore that in the recent years there has been significant interest in using passive infrared spectrometers to possibly detect biological substances in various environments.
We have decided to begin these new and promising studies in Poland as well. Our long-term experience (Błęcka et al. 2009, 2010) in the construction and use of FTIR spectrometers and in the interpretation of the spectrometric data from planetary missions (Mars-Express, Venus-Express, Herschel) allows us to be convinced that we can achieve interesting results for the benefit of the astrobiological community.
In this paper we concentrate on the passive detection of biological aerosols in the Earth’s atmosphere using our newly constructed FTIR spectrometer (this instrument will be described in detail in another paper). The results of our first set of measurements and a preliminary interpretation of the spectra are briefly outlined here.
In this first chapter we provide information about the preparation of endospores of Bacillus atrophaeus (BG) in the laboratory. In the next chapter we present information about our newly constructed FTIR spectrometer. The third chapter provides analysis of measurements performed in the laboratory testing cube. The results described in the fourth part of the paper are based on our initial spectral measurements performed in the field between 14th and 19th of April 2011. The final, fifth, chapter of this paper presents our initial conclusions, and describes our plans for the future.
Laboratory Work on BG Spores
Endospores of Bacillus atrophaeus var. globigii ATCC 9372 (BG), a well-known simulant of Bacillus anthracis endospores, were used in this study. The endospores were obtained from seven days-old BG and purified of cell debris and the medium. Purity of the endospores was >98 %, verified by microscopic examination. Finally, BG endospores were suspended in ethanol, or in purified sterile water, and used for bio-aerosol generation. The densities of the endospore suspensions used for bio-aerosol generation inside the aerosol chamber were in the range of 106–109 colony forming units (CFU) per ml.
The transmittance of BG spores described above was measured at Military University of Technology and was used in the interpretation of the measured infrared spectra.
The FTIR Spectrometer Constructed for Remote Detection of Bio-aerosols in the Laboratory and in the Field
The newly built FTIR spectrometer is a prototype of a portable field instrument intended to monitor the atmosphere. The instrument works in two spectral channels, namely: 3–5 μm and 8–12 μm atmospheric windows, with spectral resolution of about 1 cm−1. The spectral resolution and other measurement parameters were chosen to take into account dynamic behaviours of biological agents. Adequate high speed of both, optical path changes and data collection, is necessary. The system enables us to measure between 4 and 8 interferograms per second. Reduction of the spectral resolution allows optimizing the speed of the measurements. The spectrometer can work as an autonomous system collecting data in its mass memory. Moreover, the measurements can be controlled by software from a portable computer.
Passive Remote Detection of Biological Aerosols in the Laboratory
The examples of radiance spectra measured in the laboratory.
the average radiances measured when the aerosol “cloud” was present in the cell, and
the averaged radiances when there was no cloud in the sensor field of view
To test our methods, and to identify BG spores from the sets of spectra, we compared values ΔL with the spectral shape of the absorption coefficient of BG spores known from the literature (see Fig. 7).
Figure 10 shows the ΔL spectra from the field tube that were numerically simulated with MODTRAN – code (Berk et al. 1989); US Standard Model of the Atmosphere was used for calculations. The influence of atmospheric gases is visible e.g. ozone around 1000 cm−1. A maximal influence of BG spores appears at ~1000–1100 cm−1. The smoothed shape (the brown upper curve) can be interpreted as BG absorption coefficient.
We analysed the spectra obtained in the laboratory and from the field chamber using the same methods. The spectral shapes of ΔL of the averaged spectra were similar in both cases, and the main maxima were around 1000 cm−1. The existing differences were probably caused by variable conditions during the measurements. Laboratory spectra are less noisy, and the influence of gases that were present in the laboratory is visible near the maximum of ΔL.
The laboratory conditions were stable during the measurements: the temperature (20 °C), pressure, and humidity around 38 %. The weather in the field was unfortunately rather bad: the temperature varied between 10 °C and 14 °C, with very high humidity. In both cases, the concentration of BG spores in the field of view of the instrument changed between successive measurements due to sedimentation by gravity and atmospheric turbulences.
Conclusion and discussion
Preliminary results on the detection of bio-aerosols in the atmosphere performed in the laboratory and in the field are presented here. The spectral shapes of differential radiance ΔL of averaged spectra were similar in both cases, and the main maxima caused by the presence of BG spores were around 1000 cm−1. Our observations indicate that it is difficult, but possible to detect bio-aerosol clouds through the use of passive remote sensing by FTIR measurements. At this stage of our work, however, it is difficult to discern any type of biological substance. But we dare to believe that in the nearest future, through the use of refined spectrometric methods, we will be able not only to detect but also to distinguish between various kinds of biological particles and to identify them from their spectra (Ben-David and Ren 2003 and references therein, D’Amico 2005).
We continue our theoretical and laboratory work, and will continue it into the future. The radiometric calibration of the measurements will be repeated. But a larger collection of datasets is needed. During the next two years we will perform new tests, in the laboratory as well as in an open-air environment during various seasons, under differing weather conditions, and varying geometries of the measurements (the sensors will be positioned to view the releases at longer ranges), also with natural aerosols, kaolin dust and new biological materials. A new advanced method of spectral analysis will be also elaborated.
We consider the work presented here as the first step of our preparation for remote search of bio-substances in the atmospheres of planets during future planetary missions to Mars and Venus. The Earth’s environment is a good proving ground in this case.
The work was supported by the grants: 123/N-ESA/2008/0; PBZ-MNiSW-DBO-03/1/200 and 181/1/N-HSO/08/2010/0. The authors would like to thank Military University of Technology, Military Institute of Hygiene and Epidemiology and Military Institute of Chemistry and Radiometry for their cooperation, especially for giving us opportunity to test in the laboratory and in the field the newly constructed FTIR spectrometer. We are grateful also to the referees for their suggestions of changes of the paper.
This article is distributed under the terms of the Creative Commons Attribution License which permits any use, distribution, and reproduction in any medium, provided the original author(s) and the source are credited.
- Berk A, Bernstein LS, Robertson DC (1989) Modtran: a moderate resolution model for Lowtran 7, Report GL-TR-89-0122; Prepared for Geoph. Laboratory, Air Force Systems Command, United States Air Force, Hanscom Air Force Base, MA 01731-5000Google Scholar
- Błęcka MI, Rataj M, Mularczyk-Oliwa M (2009) The spectroscopic search for the biological aerosols in the planetary atmospheres: numerical simulations and laboratory measurements. Orig Life Evol Biosph 40:575 Special issue of abstracts from the 9th European Workshop on Astrobiology, Brussels, October 12–14, 2009.Google Scholar
- Błęcka MI, Rataj M, Palijczuk D, Szymanski G, Trafny E (2010) Examination the spectral signatures of biological aerosols in the Earth atmosphere using FTIR technique. Abstract presented at the 10th European Workshop on Astrobiology, Pushchino, September 6–9, 2010.Google Scholar
- Brownlee DE, Kress E (2007) Formation of Earth-like habitable planets. In: Sullivan WT III, Baross JA (eds) Planets and life. Cambridge University Press, Cambridge, pp 69–90Google Scholar
- D’Amico FM (2005) Passive standoff detection of biological aerosols. Research and Technology Directorate US Army, Edgewood chemical Biological Center: 1–13Google Scholar
- Davis R, Mauer LJ (2010) Fourier transform infrared (FT-IR) spectroscopy: a rapid tool for detection and analysis of foodborne pathogenic bacteria. In: Méndez-Vilas A (ed) Current research, technology and education topics in applied microbiology and microbial biotechnology. Formatex Research Center, Spain, pp 1582–1594Google Scholar
- Shapiro R (2007) Origin of life: the crucial issues. In: Sullivan WT III, Baross JA (eds) Planets and life. Cambridge University Press, Cambridge, pp 132–153Google Scholar