P31A-2032
Seeking Signs of Life in Nili Patera with Icelandic Sinter Field Exploration.

Wednesday, 16 December 2015
Poster Hall (Moscone South)
John R Skok, SETI Institute Mountain View, Mountain View, CA, United States, Jack D Farmer, Arizona State Univ, Tempe, AZ, United States, Mario Parente, UMASS-Elect & Comp Engrg, Amherst, MA, United States, Jessica Gaskin, NASA Marshall Space Flight Center, Huntsville, AL, United States, Hanna Kaasalainen, University of Iceland, Reykjavik, Iceland, Dominique Tobler, University of Copenhagen, Copenhagen, Denmark and Gregory Jerman, Marshall Space Flight Center, Huntsville, AL, United States
Abstract:
The past decade of Martian orbital and surface exploration has made it clear that the planet could have supported life as we know it in many places throughout much of it’s history. The next step in exploration will be to find the evidence for and characterize any preserved Martian life. The jump from confirming habitability to finding life will be difficult and likely require a systemic surface exploration of multiple, specific sites. One site, the sinter mounds of the Nili Patera caldera, provides the ideal combination of hot, neutral to alkaline waters that can develop or support life and the sinter precipitation to preserve it. Nili Patera also provides deposits that are well mapped from orbit allowing a mission to pinpoint the target rocks.

With this target known, we can develop the mission, the payload and the science to fit the goals. Several sinter field sites in Iceland were selected for mission testing. They were selected to provide diversity in scale, chemistry and complexity. At each site, we asked the same questions that would drive a mission to Mars. Was there life? What are its preserved properties? What are the environmental history of the sinters and the volcanic history of the local terrain? These questions were investigated with spectral, compositional and morphological analysis. By investigating these questions in Iceland, we will determine which observations, in terms of terrain access and instrument selection are required for mission success on Mars.

We report the results from the August 2015 expedition, the first of two planned field seasons. This summer was focused on finalizing the field locations, acquiring mapping data and an initial sampling campaign to determine expected composition and calibrate instruments for year two. With this information, we will determine an investigation plan consistent with a range of mission types from robotic lander to sample return to human exploration. We will also determine the instruments required by the site diversity. By the end of the project we should know what mission types can provide the required results. Which instruments are required for basic mission success and the cost benefit of additional analysis and what basic science questions must be investigated before sending a focused mission to determine the past existence of life in the Nili Patera sinter mounds.