Search

The immune system belongs to the most affected systems during spaceflight, and sensitivity of cells of the human immune system to reduced gravity has been confirmed in numerous studies in real and simulated microgravity. Immune system dysfunction during spaceflight represents a substantial risk for exploration class mission knowledge about the clinical, cellular, and genetic basis of immune system response, and adaptation to altered gravity will provide key information for appropriate risk management, efficient monitoring, and countermeasures against existing limiting factors for human health and performance during manned exploration of the solar system. In spite of the immune system dysregulation, studies indicate an adaptation reaction of the immune system to the new microgravity environment, at least for the T-cell system, starting after 2 weeks and continuing until 6 months or longer, reflected by cytokine concentrations in blood plasma or in stimulation assays. At the cellular level, rapid adaptation responses could be detected as early as after seconds until minutes in T cells and macrophages. Therefore, adaptive responses of cells and the whole organism could be expected under microgravity and altered gravity in general. Preventive countermeasures should therefore consider support and stabilization of the endogenous adaptation programs. Potential countermeasures for risk mitigation are summarized in this chapter. We assume that the immune systems not only have a significant adaptation potential when challenged with low gravitational environments but also provide interesting preventive and therapeutic options for long-term space missions.

Sensitivity of the human immune system to microgravity has been supposed since the first Apollo missions and was demonstrated during several space missions in the past. In vitro experiments demonstrated that cells of the immune system are exceptionally sensitive to microgravity. Therefore, serious concerns arose whether spaceflight-associated immune system weakening ultimately precludes the expansion of human presence beyond Earth’s orbit. In human cells, gravitational forces may be sensed by an individual cell in the context of altered extracellular matrix mechanics, cell shape, cytoskeletal organization, or internal prestress in the cell–tissue matrix. The development of cellular mechanosensitivity and signal transduction was probably an evolutionary requirement to enable our cells to sense their individual microenvironment. Therefore it is possible that the same mechanisms, which enable human cells to sense and to cope with mechanical stress, are potentially dangerous in microgravity.

The search for evidence of past or present life on Mars will require the detection of markers that indicate the presence of life. Because deoxyribonucleic acid (DNA) is found in all known living organisms, it is considered to be a ‘biosignature’ of life. The main function of DNA is the long-term storage of genetic information, which is passed on from generation to generation as hereditary material. The Polymerase Chain Reaction (PCR) is a revolutionary technique which allows a single fragment or a small number of fragments of a DNA molecule to be amplified millions of times, making it possible to detect minimal traces of DNA. The compactness of the contemporary PCR instruments makes routine sample analysis possible with a minimum amount of laboratory space. Furthermore the technique is effective, robust and straightforward. Our goal was to establish a routine for the detection of DNA from micro-organisms using the PCR technique during the EuroGeoMars simulation campaign. This took place at the Mars Society's Mars Desert Research Station (MDRS) in Utah in February 2009 (organized with the support of the International Lunar Exploration Working Group (ILEWG), NASA Ames and the European Space Research and Technology Centre (ESTEC)). During the MDRS simulation, we showed that it is possible to establish a minimal molecular biology lab in the habitat for the immediate on-site analysis of samples by PCR after sample collection. Soil and water samples were taken at different locations and soil depths. The sample analysis was started immediately after the crew returned to the habitat laboratory. DNA was isolated from micro-organisms and used as a template for PCR analysis of the highly conserved ribosomal DNA to identify representatives of the different groups of micro-organisms (bacteria, archaea and eukarya). The PCR products were visualized by agarose gel electrophoresis and documented by transillumination and digital imaging. The microbial diversity in the collected samp