Small Business Innovation Research/Small Business Tech Transfer
Compact Sensor for Isotope and Trace Gas Analysis, Phase II
Project Introduction
We propose to develop and demonstrate a new sensor platform for isotope and trace-gas analysis that is appropriate for future planetary missions. Among other applications, the technology can enable the collection of isotope ratio data in support of the search for evidence of life within the solar system. Current limitations to in-situ isotope measurements will be overcome by utilizing a capillary absorption spectrometer (CAS). This concept enables high precision measurements within the ultra-small volume (~ 0.1 ml) of a hollow fiber optic capillary and has proven to be three orders of magnitude more sensitive than competing sensors. The proposed effort focuses on transitioning the current lab-based technique to a small size, weight, and power (SWaP) device that can be operated unattended. In Phase I, proposed concepts for improving the system performance, reducing the SWaP, and engineering a field-capable device were proven and specific options down selected. Under Phase II, we will fully develop a general prototype sensor platform, which is applicable to a wide range of isotope ratio and trace-gas analysis applications. Specific examples of the utility and versatility of the concept will be demonstrated by using the system as a stand-alone gas sensor, as well as in combination with both a laser ablation sampler and a gas chromatograph. In addition, a dual laser system will be developed to measure both Carbon (C) and Sulfur (S) isotope ratios. The sensitivity afforded by the proposed system would open up remote analysis of smaller samples than ever before measured, which could be a significant development in the search for biosignatures on other planets and near space objects, as well as in the early Earth rock record.
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Anticipated Benefits
The isotope and gas sensor resulting from this project will be developed to support efforts to search for evidence of life on future NASA missions. The research is specifically relevant to NASA Objective 2.3 which is to "Ascertain the content, origin, and evolution of the solar system and the potential for life elsewhere," as well as NASA Astrobiology Roadmap Goal 7: "Determine how to recognize signatures of life on other worlds and on Earth." In fact, NASA Astrobiology Roadmap Objective 7.1 is to "Learn how to recognize and interpret biosignatures which, if identified in samples from ancient rocks on Earth or from other planets, can help to detect and/or characterize ancient and/or present-day life." The anticipated technology would also be useful for the exploration of the Moon, asteroids, primitive meteorites, comets, and interplanetary dust particles. The relatively small size of the system will enable it to be inserted into a range of missions including landers and rovers. The capillary absorption spectrometer (CAS) at the heart of the system will also provide a new high precision, ultra-low-volume sensor relevant to a range of other NASA applications. These include water isotope ratio measurements, atmospheric sensing of Earth and other planets, environmental sensing from a small UAV, analysis of soil bacteria related to Carbon cycle, as well as full elemental analysis of various microscopic-sized samples and organisms. The CAS sensor to be developed under this project will provide an extremely attractive alternative to both isotope ratio mass spectrometers (IRMS) and cavity ring down spectrometers (CRDS). The CAS will be relatively inexpensive, require only picomoles of material, and be much smaller than competing systems. CAS sensors will fill niche markets in forensic analysis, environmental sensing, human breath analysis, and industrial process control. This STTR will lead to a new class of sensors, not just a modification of an existing concept. The resulting ultra-small volume sensors could compete with and complement current commercial sensors, and potentially open up new opportunities to perform real-time, in-situ analysis of trace molecules and stable isotopes in remote and/or sample-limited situations.
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Primary U.S. Work Locations and Key Partners
| Organizations Performing Work | Role | Type | Location |
|---|---|---|---|
| Opto-Knowledge Systems, Inc. (OKSI) | Lead Organization | Industry | Torrance, California |
Jet Propulsion Laboratory
(JPL)
|
Supporting Organization | NASA Center | Pasadena, California |
| Pacific Northwest National Laboratory (PNNL) | Supporting Organization | R&D Center | Richland, Washington |
Primary U.S. Work Locations
-
California
-
Washington
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Organizational Responsibility
Responsible Mission Directorate:
- Space Technology Mission Directorate (STMD)
Lead Organization:
- Opto-Knowledge Systems, Inc. (OKSI)
Responsible Program:
- Small Business Innovation Research/Small Business Tech Transfer
Project Management
Program Director:
Program Manager:
Principal Investigator:
Project Duration
Start: May 2015
End: Feb 2019
Technology Maturity (TRL)
| Start: | 4 |
| Current: | 6 |
| Estimated End: | 6 |
Applied Research
Development
Demo & Test
Technology Areas
Primary:
- TX08 Sensors and Instruments
- TX08.1 Remote Sensing Instruments/Sensors
- TX08.1.3 Optical Components
Target Destination
Others Inside the Solar System
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