Evaluation of the International Space Station Internal Environment (ISS Internal Environment) from air, water and surface samples of International Space Station (ISS) provided a baseline of the contaminant characterization onboard the ISS. All of the partner agencies recognize the importance of crew health to mission success and are dedicated to maintaining the health of all crewmembers throughout all phases of ISS missions. The data obtained from Environmental Monitoring provides insight into the environmental contamination during the stages of construction and habitation of ISS.Principal Investigator(s)
National Aeronautics and Space Administration (NASA)Sponsoring Organization
Human Exploration and Operations Mission Directorate (HEOMD)Research Benefits
Information PendingISS Expedition Duration:
Information PendingPrevious ISS Missions
To successfully live and work in the environment of space, the ISS environment must be monitored and kept within the guidelines set forth by the International Space Station Medical Operations Requirement Document to ensure the health of the crew living and working there. Astronauts can be more sensitive to air pollutants because of the closed environment. Pollutants in this environment are magnified in ISS because the exposure is continuous.
Sources of physical, chemical, and microbiological contaminants include humans and other organisms, food, cabin surface materials and experiment devices. One hazard is the off-gassing of vapors from plastics and other items on ISS; although this is a small hazard, the accumulation of these contaminants in the air can prove dangerous to crew health. The air sampling systems on ISS periodically checks the air for potential hazards. The U.S. segment utilizes advanced high efficiency particulate air (HEPA) filters and periodically participates in filter cleanings to keeping harmful vapors out of the air. The Russian segment uses pleated woven filters to maintain low microbial levels. Both the HEPA filter and the woven sheets have proven to reduce the number of dust particles and microorganisms aboard the ISS. Other significant contaminants that pose hazards to the crew are microbial growth, both bacterial and fungal; air, water and surface sampling by the crew in conjunction with periodic cleaning keep the microbial levels on ISS in check.
The volatile organic analyzer (VOA) is an atmospheric analysis device on ISS that uses a gas chromatograph and ion mobility spectrometer to detect, identify, and quantify a selected list of volatile organic compounds (i.e., ethanol, methanol and 2-propanol) that are harmful to humans at high levels in a closed environment, such as ISS. The ISS also utilizes the POTOK air filtration device employed by Roscosmos to disinfect and inactivate microorganisms by electrostatic pulses and charged ions.
To monitor microbial levels on ISS crewmembers use devices called grab sample containers, dual absorbent tubes and swabs to collect station air, water and surface samples and send them to Earth for detailed analysis and identification every 6 months. This data provides controllers on Earth detailed information about the type of microbial contaminants on board ISS. The controllers can then give direction to the crew on sanitation if increased microbial growth is identified. The crew keeps microbes under control on ISS through periodic scheduled sanitation of the ISS.
Missions to beyond low Earth orbit will increase the length of time that astronauts live and work in closed environments. To complete future long-duration missions the crews must remain healthy in closed environments, hence future spacecraft must provide sensors to monitor environmental health and accurately determine and control the physical, chemical and biological environment of the crew living areas and their environmental control systems.
Environmental Monitoring is vital to ensuring crew and spacecraft health during space flight. The results are being used to identify specific effects of a closed space environment on astronauts. This knowledge will allow scientists to develop systems to enable the crew to remain health on future long duration missions to the Moon and Mars.Earth Applications
Increased understanding of the affects of a closed space environment on humans will increase the knowledge of living in extreme conditions such as submarines or the artic. Due to widespread growth in the use of colloidal silver as a biocidal agent, develop of a simple and cost efficient method of silver testing is valuable.
Numerous air, water and surface samples are collected by ISS crews on a regular basis. Many of these samples are cultured on board ISS while others are preserved and returned to Earth for later analysis. These samples are analyzed using the following methods on board ISS:
The crew utilizes handheld equipment to monitor the air, water and surfaces of ISS on a daily, weekly and monthly basis. The samples can be returned to Earth for analysis by scientists. Other automated equipment, including the VOA and, the Major Constituent Analyzer monitor the atmosphere of ISS daily for potential harmful contaminants. The crew also performs weekly housekeeping duties on board ISS, which includes disinfecting surfaces and cleaning air filters which contributes to environmental monitoring.
During one study of the ISS atmosphere, 12 bacterial strains were isolated and fingerprinted from the ISS water system. These bacteria consisted of common strains and were encountered at levels below 10,000 colony-forming units/10 cm2, which is well below the minimum of bacteria needed to cause illness. These data represent the beginning of ISS habitation and indicate that the lessons learned from previous Mir and Skylab missions were implemented and have been effective in keeping station a safe place in which to live and work (Castro et al. 2004).
Solid-waste treatment in space must be safely processed and stored in a confined environment. Most of the solid-waste is wet and therefore poses a high risk of culturing the growth of undesirable microorganisms. Analysis was performed in order to assess potential crew risks resulting from microbial decay. Results show certain levels of volatile organic compounds, ethylene, methane and carbon dioxide. These gases are being contained within the trash compartments, therefore minimalizing potential risk for crewmembers (Peterson et al 2004).
In comparison to previous identification techniques, scientist decided to test additional sampling and detection methods on station. Previously, samples were limited to conventional culture-dependent methods. Now, scientist looked at specific biomarkers, such as ATP and DNA, to help identify non-culturable species. Samples were collected from several different surfaces along with drinking water reservoirs. Culture-dependent samples identified different species of Bacillus, while culture-independent techniques revealed a whole array of different microbes, previously not identified. Once samples were returned to Earth, further DNA analysis confirmed the findings including certain opportunistic pathogens with all levels within the accepted range. This study supports the idea of utilizing multiple detection techniques to completely identify all microbes present on the ISS (La Duc 2004).
Another study performed an in-depth microbial examination of the drinking water in various stages (from the NASA Kennedy Space Center, Cape Canaveral, FL to the ISS ports). These studies have revealed that NASA policy for biocide treatment has effectively removed pathogenic microbes prior to ingestions by crew members (La Duc 2004). Further analysis of samples collected from station noted the reoccurring presence of Ralstonia eutropha, Methylobacterium fujisawaense, and Psuedomonas aeruginosa in the potable water system. Certain counts were above the acceptable limit, calling for supplementary antimicrobial attention. Additional in-flight monitoring for the specific detection of coliforms (bacteria typically indicative of food contamination) was also introduced (Bruce et al 2005).
The following year, additional water samples were returned for ground examination. Analysis revealed the presence of nucleic acids belonging to various pathogens, but no viable pathogens were recovered. Air and surface samples were also analyzed for microbial characterization. Concentrations of airborne bacteria and fungi were within the accepted range, with a predominant concentration of Staphylococcus, Aspergillus and Penicillium. Surface samples rarely exceeded the acceptable limit, with increased concentrations of Staphylococcus, Aspergillus and Caldosporium (Novikova et al 2006).
After a population of microorganisms of 500,000 to 1 million CFU/100 ml was identified in a flex hose assembly, it was brought back to Earth for further analysis. Studies focused on determining if a biofilm formed on certain parts of the assembly. Analysis revealed that the nickel hydroxide and nickel phosphates acted as a barrier to additional biofilms in the flex hose assembly and the SPCU heat exchanger. There are other parts that do not come in contact with these additional protectants, and are potentially the culprit of such high microbial concentrations. Continued studies must be performed to ensure zero biolfilm formation to maintain the integrity of the water system aboard the ISS (Roman et al 2006).
On station, silver is used as a biocidal agent based on its antimicrobial properties in the potable water system. Recent studies have shown the possible toxicity of colloidal silver to humans, including crew members aboard the ISS. Researchers are currently developing and testing a simple technique that will enable crew members to test silver levels in the water system in less than two minutes (Hill et al 2010).
Continued monitoring has marked the ISS a microbiologically safe working and living habitat. Microbial contamination levels are generally below the required standards with occasional escalations in contamination levels. These increases could be minimized with further developed technologies, specifically with online detection tools that offered simultaneous quantification and identification (Van Houdt et al 2011).
Another area of particular interest deals with the growth of microbial organisms on space-generated solid waste. Once trash was returned to Earth, it was weighed and categorized into personal hygiene waste (56%), drink (11%) and food (18%) waste, plastic waste (12%) or office waste (3%). Station trash has an abundant amount of biodegradable compounds that can aid the growth and proliferation of microorganisms. After ground analysis, several microbes typical of human’s normal flora were identified along with certain pathogenic microbes including Staphylococcus aureus and Escherichia coli. These results can be further utilized to create new criteria for NASA Waste Management Systems (Strayer et al "Characterization" 2012).
Microorganisms recovered from space generated solid waste were processed through a Heat Melt Compactor to determine how efficiently this process eliminated potential threats. Prior to melting trash, specific markers indicative of spore forming bacteria marked the trash to indicate the survival rate of the microbes after the melting process. Post melting, the samples were run though microbial character analysis. Results indicate that this sanitization technique greatly reduced the number of viable microbes, but did not eliminate entirely. Interior samples were also analyzed, resulting in similar results, indicating this technique efficient in eradicating active microbial growth (Strayer et al "Microbial" 2012).
Continual efforts to ensure crew safety will accompany the lifetime of the ISS. A new type of air testing was performed in 2010, evaluating threshold (T) values for sixteen adverse health effect groups. All T levels were within the safe limit. The highest values were found in mucosal limits, headaches, central nervous system depression, and cardiac sensitization. This evaluation is an integral tool of NASA’s Lifetime Surveillance of Astronaut Health (James et al 2012).
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