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Design, construction and testing of a Cavity-Ring Down Spectrometer for determination of the concentration and isotopic composition of methane
Project Investigators: John Kessler, Tullis Onstott
Other Project Members
Barbara Sherwood Lollar (Collaborator)Summary
The recent detection of CH4 in the Martian atmosphere and observations suggesting that it varies both temporally and spatially argues for dynamic sources and sinks. CH4 is a gaseous biomarker on Earth that is readily associated with methanogens when its H and C isotopic composition falls within a certain range. It is imperative that a portable instrument be developed that is capable of measuring the C and H isotopic composition of CH4 at levels comparable to that on Mars with a precision similar to that of an isotope ratio mass spectrometer and that such an instrument be space flight capable. Such an instrument could guide a rover to a site on Mars where emission of biogenic gases is occurring and samples could be collected for Mars sample return.
Astrobiology Roadmap Objectives:
- Objective 2.1: Mars exploration
- Objective 2.2: Outer Solar System exploration
- Objective 3.3: Origins of energy transduction
- Objective 4.1: Earth's early biosphere
- Objective 5.1: Environment-dependent, molecular evolution in microorganisms
- Objective 5.2: Co-evolution of microbial communities
- Objective 5.3: Biochemical adaptation to extreme environments
- Objective 6.1: Environmental changes and the cycling of elements by the biota, communities, and ecosystems
- Objective 6.2: Adaptation and evolution of life beyond Earth
- Objective 7.1: Biosignatures to be sought in Solar System materials
- Objective 7.2: Biosignatures to be sought in nearby planetary systems
Project Progress
Design, construction and testing of a Cavity-Ring Down Spectrometer (CRDS) for determination of the concentration and isotopic composition of methane
During the past 12 months, we have measured in detail the absorption spectra for 12CH4, 13CH4, CH3D and CO2. We’ve designed a peak fitting routine to integrate the 12CH4 and 13CH4 peaks in the wavelength region of our CRDS. We’ve tested this software on a CH4 gas standard of known isotopic composition and were able to reproduce the δ13C of the 2 ppm standard with an accuracy of ±5o/oo. Although this accuracy is twice that of the multipass instrument on MSL, it is 10 times less than the accuracy of the individual ring-down events. The inaccuracy is due to imprecision in the wavelength of the laser, which will be rectified by upgrading the instrument with a wavelength monitor. A manuscript describing the methodology, instrument and first measurement is being prepared for Optics Express. A proposal to take the current instrument to Technology Readiness Level 6 was submitted to the Mars Instrument Development Program in June ’07 with collaboration from Paul Mahaffy of Goddard Space Flight Center and has recently been awarded.
We also tested a Los Gatos CRDS at the McGill University arctic research station (MARS) on Axel Heiberg Island for two weeks in April ’08 where we measured CH4 fluxes from the permafrost soil and hot springs. These results indicate that the CH4 fluxes are sufficiently high that our current CRDS should be able to measure their isotopic composition and our current plan is to return to MARS next spring with the upgraded instrument. We are presently preparing the instrument for CH4 activity measurements on permafrost methanogens while they are being exposed to simulated Martian conditions at the Techshot facility in Greenfield, Indiana.
Mission Involvement
MFLA Cavity Ringdown Spectrometer is the instrument most likely to be ready for the next landed instrument package on Mars after the Mars Science Laboratory. Onstott and Mahaffy (Goddard) will collaborate on development of an improved Cavity Ringdown Spectrometer with funding from a recent NASA MDIP award.Cross-Team Collaborations
Paul Mahaffy at Goddard has been collaborating with Onstott and Kessler on calibration of a Cavity Ringdown Spectrometer. Mahaffy and Onstott will now design and build an improved spectrometer with funding from a NASA MDIP.
Publications
Kessler, J.D. (2008). Isotopic Characterization of Martian Methane by CRDS. AbSciCon. Santa Clara CA.
- Amino Acid Preservation in Saline-Lake Sediments and Mars-Simulant Regolith
- Application of U-tube and fiber-optic distributed temperature sensor to characterize the chemical and physical properties of a deep permafrost and sub-permafrost environment at High Lake, Nunavut, Canada.
- Challenges for Coring Deep Permafrost on Earth and Mars: Drilling Project at High Lake, Nunavut, Canada
- Design, construction and testing of a Cavity-Ring Down Spectrometer for determination of the concentration and isotopic composition of methane
- Environmental genomics reveals a single species ecosystem deep within the Earth.
- High Lake Gossan deposit: An Arctic analogue for ancient Martian surficial processes?
- Isotopic Signatures of Methane and Higher Hydrocarbon Gases from Precambrian Shield Sites: A Model for Abiogenic Polymerization of Hydrocarbons
- Mars Forward Contamination Studies Utilizing a Mars Environmental Simulation Chamber
- Microbial Communities in Subpermafrost saline fracture water at the Lupin Au Mine, Nunavut, Canada
- Radiolytic oxidation of sulfide minerals as a source of sulfate and hydrogen to sustain microbial metabolism
- Saline Lakes and Gypsum Dunes in the Rio Grande Rift System as Analogues for Sulfate Deposits on Mars
- Stability of methane hydrates in the presence of high salinity brines on Mars
- The Diversity of the Original Prebiotic Soup: Re-Analyzing the Original Miller-Urey Spark Discharge Experiments
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