Abstract The evolution of the solar system and the origin of life remain some of the most intriguing questions for humankind. Addressing these questions experimentally is challenging due to the difficulty of mimicking environmental conditions representative for Early Earth and/or space conditions in general in ground-based laboratories. Performing experiments directly in space offers the great chance to overcome some of these obstacles and to possibly find answers to these questions. Exposure platforms in Low Earth Orbit (LEO) with the possibility for long-duration solar exposure are ideal for investigating the effects of solar and cosmic radiation on various biological and non-biological samples. Up to now, the Exobiology and space science research community has successfully made use of the International Space Station (ISS) via the EXPOSE facility to expose samples to the space environment with subsequent analyses after return to Earth. The emerging small and nanosatellite market represents another opportunity for astrobiology research as proven by the robotic O/OREOS mission, where samples were monitored in-situ, i.e. in Earth orbit. In this framework, the European Space Agency is developing a novel Exobiology facility outside the ISS. The new platform, which can host up to four different experiments, will combine the advantages of the ISS (long-term exposure, sample return capability) with near-real-time in-situ monitoring of the chemical/biological evolution in space. In particular, ultraviolet–visible (UV–Vis) and infrared (IR) spectroscopy were considered as key non-invasive methods to analyse the samples in situ. Changes in the absorption spectra of the samples developing over time will reveal the chemical consequences of exposure to solar radiation. Simultaneously, spectroscopy provides information on the growth rate or metabolic activities of biological cultures. The first quartet of experiments to be performed on-board consists of IceCold, OREOcube and Exocube (dual payload consisting of ExocubeChem and ExocubeBio). To prepare for the development of the Exobiology facility, ground units of the UV–Vis and IR spectrometers were studied, manufactured and tested as precursors of the flight units. The activity led to a modular in-situ spectroscopy platform able to perform different measurements (e.g. absorbance, optical density, fluorescence measurements) at the same time on different samples. We describe here the main features of the ground model platform, the verification steps, results and approach followed in the customization of commercial–off-the-shelf (COTS) modules to make them suitable for the space environment. The environmental tests included random and shock vibration, thermal vacuum cycles in the range −20 °C to +40 °C and irradiation of the components with a total dose of 1800 rad (18 Gy). The results of the test campaign consolidated the selection of the optical devices for the Exobiology Facility. The spectroscopic performance of the optical layout was tested and benchmarked in comparison with state-of-the-art laboratory equipment and calibration standards showing good correlation. This includes spectra of samples sets relevant for the flight experiments and a performance comparison between the SPECTROModule ground model and state-of-the-art laboratory spectrometers. Considering the large number of samples and different types of optical measurements planned on-board the ISS, the main outcome was the implementation of an LED-photodiode layout for the optical density and fluorescence measurements of IceCold (42 samples) and ExocubeBio (111 samples); while the UV–Vis spectrometer will be mainly focused on the change of the absorption spectra of the 48 samples of OREOcube.The ExocubeChem samples (in total 48) will be analysed by infrared spectroscopy. The ground platform supports the establishment of analogue research capabilities able to address the long-term objectives beyond the current application.
Highlights Biological samples shall be exposed to solar and cosmic radiation. UV/VIS and IR spectroscopy are used for in-situ measurements in space. Commercial off-the shelf (COTS) spectrometers were tested and verified for use in space. A scientific test campaign proved the predicted results. SPECTROmodule is the precursor mission of the Exobiology facility accommodated outside the International Space Station.
SPECTROModule: A modular in-situ spectroscopy platform for exobiology and space sciences
Acta Astronautica ; 166 ; 377-390
2019-10-06
14 pages
Aufsatz (Zeitschrift)
Elektronische Ressource
Englisch
Exobiology , Astrobiology , Spectroscopy , <italic>In-situ</italic> monitoring , Low earth orbit , International space station , UV/VIS , IR , ISS , International Space Station , COTS , commercial off-the- shelf , CRS , Commercial Resupply Service , UV–Vis , ultraviolet–visible , infrared , LEO , low Earth Orbit , FTIR , Fourier-transform infrared spectroscopy , ELIPS , European Programme for Life and Physical Sciences in Space , ILSRA , International Life Sciences Research Announcement , GM , Ground Model , GSE , Ground Support Equipment , ESA , European Space Agency , PSI , Planetary and Space SImulation , OD , Optical Density , LED , Light-Emitting Diode , SM , Scientific Module , Fourier Transform InfraRed Spectrometer , MAIT , Manufacturing, Assembly, Integration and Testing , CTB , Cargo Transportation Bag , TID , Total Ionizing Dose , MLI , Multi-Layer Insulation , DLR , German Aerospace Centre , HZM , Helmholtz Zentrum München
Elsevier | 1987
|Exobiology research on Space Station Freedom
NTRS | 1995
|NTRS | 1990
|British Library Conference Proceedings | 1998
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