Details

Autor(en) / Beteiligte

• Stern, Jennifer C
• Sutter, Brad
• Freissinet, Caroline
• Navarro-González, Rafael
• McKay, Christopher P
• Archer, Jr, P Douglas
• Buch, Arnaud
• Brunner, Anna E
• Coll, Patrice
• Eigenbrode, Jennifer L
• Fairen, Alberto G
• Franz, Heather B
• Glavin, Daniel P
• Kashyap, Srishti
• McAdam, Amy C
• Ming, Douglas W
• Steele, Andrew
• Szopa, Cyril
• Wray, James J
• Martín-Torres, F Javier
• Zorzano, Maria-Paz
• Conrad, Pamela G
• Mahaffy, Paul R

Titel

Evidence for indigenous nitrogen in sedimentary and aeolian deposits from the Curiosity rover investigations at Gale crater, Mars

Ist Teil von

• Proceedings of the National Academy of Sciences - PNAS, 2015-04, Vol.112 (14), p.4245-4250

Ort / Verlag

United States: National Academy of Sciences

Erscheinungsjahr

2015

Quelle

MEDLINE

Beschreibungen/Notizen

• Significance We present data supporting the presence of an indigenous source of fixed nitrogen on the surface of Mars in the form of nitrate. This fixed nitrogen may indicate the first stage in development of a primitive nitrogen cycle on the surface of ancient Mars and would have provided a biochemically accessible source of nitrogen. The Sample Analysis at Mars (SAM) investigation on the Mars Science Laboratory (MSL) Curiosity rover has detected oxidized nitrogen-bearing compounds during pyrolysis of scooped aeolian sediments and drilled sedimentary deposits within Gale crater. Total N concentrations ranged from 20 to 250 nmol N per sample. After subtraction of known N sources in SAM, our results support the equivalent of 110–300 ppm of nitrate in the Rocknest (RN) aeolian samples, and 70–260 and 330–1,100 ppm nitrate in John Klein (JK) and Cumberland (CB) mudstone deposits, respectively. Discovery of indigenous martian nitrogen in Mars surface materials has important implications for habitability and, specifically, for the potential evolution of a nitrogen cycle at some point in martian history. The detection of nitrate in both wind-drifted fines (RN) and in mudstone (JK, CB) is likely a result of N ₂ fixation to nitrate generated by thermal shock from impact or volcanic plume lightning on ancient Mars. Fixed nitrogen could have facilitated the development of a primitive nitrogen cycle on the surface of ancient Mars, potentially providing a biochemically accessible source of nitrogen.