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The Spacecraft Atmosphere Monitor (S.A.M.) is a highly compact gas chromatograph mass spectrometer (GCMS) instrument built by JPL that is a technology demonstration on the International Space Station for monitoring the cabin atmosphere in human spacecraft. S.A.M. measures both the major constituents (e.g. nitrogen, oxygen, and carbon dioxide) and trace parts per billion volatile chemicals (e.g. benzene, ethanol, siloxanes)in the spacecraft cabin atmosphere to ensure the help safeguard the health of the astronauts. S.A.M. has a total mass of 9.5 kg and uses 40W (nominal) during operation.
![](http://upload.wikimedia.org/wikipedia/commons/thumb/1/16/Spacecraft_Atmosphere_Monitor.jpg/220px-Spacecraft_Atmosphere_Monitor.jpg)
S.A.M. is an advanced technology demonstration that can be employed on future crewed flight missions, like in the Artemis program and the Orion spacecraft. It was launched to ISS on a Dragon spacecraft on July 25, 2019, and began continuous operations on July 29, 2019.[1][2] S.A.M. was returned to earth aboard SpaceX-25 on Jan. 24, 2022 after almost two years of continuous operations aboard the ISS, exceeding its design lifetime goal of one year. The instrument was returned to JPL on Feb. 15, 2022.
This first S.A.M. instrument will be refurbished and be flown, along with a second S.A.M. unit, to ISS in late 2022. The two instruments operating at the same time will enable JPL scientists to continuously monitor the ISS cabin atmosphere for interesting or anomalous constituents and temporal or spatial variations in the cabin atmosphere.
See also
editReferences
edit- ^ Hill, Denise (2019-07-23). "S.A.M. Goes to Work Aboard ISS". NASA. Retrieved 2019-07-30.
- ^ "NASA's Spacecraft Atmosphere Monitor Goes to Work Aboard the International Space Station". Technology Org. 2019-07-30. Retrieved 2019-07-31.