Initial SAM calibration gas experiments on Mars: Quadrupole mass spectrometer results and implications. (April 2017)

• Record Type: Journal Article
• Authors: Franz, Heather B.; Trainer, Melissa G.; Malespin, Charles A.; Mahaffy, Paul R.; Atreya, Sushil K.; Becker, Richard H.; Benna, Mehdi; Conrad, Pamela G.; Eigenbrode, Jennifer L.; Freissinet, Caroline; Manning, Heidi L.K.; Prats, Benito D.; Raaen, Eric; Wong, Michael H.
• Is Part Of: Planetary and space science. Volume 138(2017)
• Page Start: 44
• Page End: 54
• Publication Date: 2017-04
• Subjects: Mars -- Atmosphere -- Isotopes -- Mars Science Laboratory -- Sample Analysis at Mars Investigation -- Calibration; Space sciences -- Periodicals; Atmosphere, Upper -- Periodicals; Sciences spatiales -- Périodiques; Haute atmosphère -- Périodiques; 523
• DOI: 10.1016/j.pss.2017.01.014
• Languages: English
• ISSNs: 0032-0633

Abstract

Abstract: The Sample Analysis at Mars (SAM) instrument suite of the Mars Science Laboratory (MSL) Curiosity rover is equipped to analyze both martian atmospheric gases and volatiles released by pyrolysis of solid surface materials, with target measurements including chemical and isotopic composition (Mahaffy et al., 2012). To facilitate assessment of instrument performance and validation of results obtained on Mars, SAM houses a calibration cell containing CO2, Ar, N2, Xe, and several fluorinated hydrocarbon compounds (Franz et al., 2014; Mahaffy et al., 2012). This report describes the first two experiments utilizing this calibration cell on Mars and gives results from analysis of data acquired with the SAM Quadrupole Mass Spectrometer (QMS). These data support the accuracy of isotope ratios obtained with the QMS (Conrad et al., 2016; Mahaffy et al., 2013) and provide ground-truth for reassessment of analytical constants required for atmospheric measurements, which were reported in previous contributions (Franz et al., 2015, 2014). The most significant implication of the QMS data involves reinterpretation of pre-launch contamination previously believed to affect only CO abundance measurements (Franz et al., 2015) to affect N2 abundances, as well. The corresponding adjustment to the N2 calibration constant presented here brings the atmospheric volume mixing ratios for Ar and N2 retrieved by SAM into closer agreement with those reported by the Viking mission (Owen et al., 1977; Oyama and Berdahl, 1977). Highlights: The SAM instrument measures the composition of the martian atmosphere. SAM's calibration gas cell was exercised in July and December 2015. Calibration constants for atmospheric composition have been adjusted. Revised SAM nitrogen abundance is similar to that measured by Viking. SAM accurately retrieved isotope ratios of CO2 and Xe in the calibration cell.