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During the last years extensive work has been done to design and develop the Closed Loop Air Revitalization System ARES. The potential of ARES for future space exploration missions is to significantly reduce the water upload demand, increase the safety of the crew by reducing dependency on re-supply flights and due to the launch mass restraints - make future exploration missions to other planets possible. Past years’ activities concentrated on the development of a full-scale demonstrator which was in form, fit, and function comparable to an ‘engineering model’ (EM). Most equipment was off-the-shelf and has been mechanically upgraded to EM standard. The demonstrator includes the functions of CO2 concentration, CO2 reduction and oxygen generation. All components fit into one ISPR. The design minimizes the number of external interfaces in order to achieve a high degree of independence and flexibility. Design baseline for the development was the accommodation in NODE 3 of the ISS.

At the 2002 ICES, FAVORITE, the orbital flight experiment for a fixed alkaline electrolyte (FAE) electrolyser stack was presented. The planning at that time was to fly the experiment in September 2003 on board the Space-Hab mission STS-118 with the space shuttle COLUMBIA flight ISS-13A.1. Due to the tragic accident of COLUMBIA on Feb. 1st, 2003, these plans became obsolete and alternative launch opportunities were looked for. They were finally found with the unmanned Russian FOTON-M2, which is built by TsSKB-PROGRESS in Samara, Russia and scheduled for launch from the Baikonur cosmodrome in April 2005. Because of the switch from a manned to an unmanned mission and other operational constraints, FAVORITE had to be redesigned in several parts. This paper summarizes the objectives of the flight experiment and describes the required design changes. It also presents an overview of the actual development status as well as of the work ahead.

Since 1985 in a step by step approach an advanced air revitalisation system has been developed for a crewed spacecraft. The metabolically produced carbon dioxide is concentrated through a solid amine water steam desorp-tion system and reduced to water and methane in a so-called Sabatier reactor. The water is currently fed into a fixed alkaline electrolyser to reclaim the oxygen for the crew. However, also water from other sources may be used. The hydrogen is recycled into the Sabatier reactor. The present system handles methane as a waste product closing so far the oxygen loop only. The system has been already successfully demonstrated in a laboratory scale configuration for a crew of three persons in 1996/1997. This paper discusses the results of the current development phase in which the system is reconfigured to fit into an International Space Station payload rack (ISPR). For this purpose the complete system design has been reviewed and upgraded where necessary.

In this paper, an advanced trace gas monitoring system for manned space cabins is presented. The principle of functioning of the measurement system is based on the detection of gas-specific absorption features in the Infrared area of the spectrum. The core element in the monitoring system is a Fourier-Transform Infrared (FTIR) Spectrometer. When calibration is carried out applying sophisticated, novel analysis methods, the system can simultaneously detect and quantify all the interesting gases in manned space cabins. In a previous Trace Gas Monitoring multi-phase program (TGM 2) [1],[2], the FTIR technology has demonstrated its ability to handle multi-component, quasi on-line gas measurements, including identification and quantification of 23 important trace gases in a mixture. In the ongoing phase 3 (TGM 3), initiated end of 1997 [3], a fully operational FTIR technology demonstration model is tested being able to detect simultaneously 30 different trace gases in a mixture.

The longer human beings in closed habitats need to be supplied with life support functions, the more the closure of the ECLSS loops becomes a must. This is certainly valid for habitats in space, where a steady resupply of consumables from Earth is impossible due to excessive distances or prohibitive high cost, but it may apply in general to earthbound habitats as well, if for instance large submarines want to extend their diving time. In two harmonised programs for the two customers European and German Space Agency (ESA/ESTEC, DARA), Dornier is now in charge with the development of the technologies for the closure of the oxygen loop.

In support of the Columbus ECLSS, a technology development program has been performed on four items: Regenerative CO2 removal Trace Gas Contamination Control Trace Gas Contamination Monitoring Low Noise Variable Speed Fan This paper describes the contents and results of the concluding Subsystem Level Tests and consecutive programme extensions which concentrated on: performance of the Contamination Monitoring Unit noise generation of the Variable Speed Fan lifetime tests of the CO2 removal solid amine closed water loop operation of a solid amine CO2 removal unit