Detection and Quantification of Nitrogen Compounds in the First Drilled Martian Solid Samples by the Sample Analysis at Mars (SAM) Instrument Suite on the Mars Science Laboratory (MSL)

• Main Authors: Buch, A., Szopa, C., McAdam, A. C., Glavin, D. P., Franz, H. B., Sutter, B., Steele, A., Mahaffy, P. R., Coll, P., Ming, D., Archer, P. D., Jr., Conrad, P., McKay, C. P., Navarro-Gonzales, R., Wray, J. J., Freissinet, C., Brunner, A. E., Stern, J. C., Eigenbrode, J. L.
• Format: Other/Unknown Material
• Language: unknown
• Published: 2014
• Subjects: Lunar and Planetary Science and Exploration; Yellowknife; Yellowknife Bay
• Online Access: http://hdl.handle.net/2060/20140017075

The Sample Analysis at Mars (SAM) instrument suite on the Mars Science Laboratory (MSL) Curiosity Rover detected both reduced and oxidized nitrogen-bearing compounds during the pyrolysis of surface materials at Yellowknife Bay in Gale Crater. Preliminary detections of nitrogen species include NO, HCN, ClCN, CH3CN, and TFMA (trifluoro-N-methyl-acetamide). Confirmation of indigenous Martian N-bearing compounds requires quantifying N contribution from the terrestrial derivatization reagents (e.g. N-methyl-N-tertbutyldimethylsilyltrifluoroacetamide, MTBSTFA and dimethylformamide, DMF) carried for SAM's wet chemistry experiment that contribute to the SAM background. Nitrogen species detected in the SAM solid sample analyses can also be produced during laboratory pyrolysis experiments where these reagents are heated in the presence of perchlorate, a compound that has also been identified by SAM in Mars solid samples.