"It might seem like we're looking for a needle in a haystack," remarked Carnegie researcher Marilyn Fogel.1 "But it's much better than that. One of our studies showed that we can detect even the most minute amounts of the element nitrogen, which can be evidence of life. Interestingly, rocks might be particularly promising places to find traces left by the tiniest microbes. Svalbard is brittle cold, very dry, and rocky, much like the Martian environment, making it an excellent test bed."
Nitrogen is essential to DNA, RNA, and protein. All life depends on it. The scientists looked at how a certain type, or isotope, of nitrogen was distributed in soils, water, rocks, plants, and in microbes. They found that nitrogen quantities varied depending on how the element interacted with the environment and living organisms. "We found that organisms leave tell-tale nitrogen fingerprints on rocks, " stated Fogel. "The technology is well suited for finding remains of life on the rocky terrain of Mars."
In another study, the group found that they could adapt techniques used in genetic laboratories to the field.2 They found that DNA sampling and the polymerase chain reaction (PCR) method--which makes many copies of a specific segment of DNA for analysis--can detect genetic differences in rock-dwelling communities of blue-green algae (cyanobacteria) and fungi. Further, they identified over 90 different compounds that can be correlated to biosignatures of those life forms. These fingerprints will be part of an enormous library of signatures to which Martian samples can be compared in the search for life.
Talk and poster schedule subject to change. See http://abscicon2006.arc.nasa.gov/agenda.php for the latest information.
1 Fogel and AMASE team, "Nitrogen cycling in cold analogue environments"
Monday, March 27th, 10:35
Reagan Center, Horizon A & B conference room, Session 3: Cold Mars Analogue Environments
2 Jennifer Eigenbrode, et al., "Biosignatures of arctic organisms from different rock types"
Poster displayed throughout the conference. Poster session Monday night, March 27, 2006, 6-8pm
Reagan Center, Atrium Hall.
Rebecca Martin, et al., "Antibody microarrays for real-time monitoring of microbial environment and astronaut health"
Poster displayed throughout the conference. Poster session Monday night, March 27, 2006, 6-8pm
Reagan Center, Atrium Hall
*The Arctic Mars Analog Svalbard Expedition (AMASE) team comes from the following institutions: lead institution, Physics of Geological Processes, University of Oslo; The Carnegie Institution of Washington, Geophysical Laboratory and Department of Terrestrial Magnetism; NASA Jet Propulsion Laboratory; University of Leeds; University of Oxford; Universidad de Burgos, Spain; The Smithsonian Institution; Penn State University; Geological Institute, University of Oslo and Idaho National Laboratory.
The Carnegie Institution of Washington (www.CarnegieInstitution.org) has been a pioneering force in basic scientific research since 1902. It is a private, nonprofit organization with six research departments throughout the U.S. Carnegie scientists are leaders in plant biology, developmental biology, astronomy, materials science, global ecology, and Earth and planetary science.
This work is supported by the NASA Astrobiology Institute (NAI). The NAI, founded in 1998, is a partnership between NASA, 16 major U.S. teams and six international consortia. NAI's goal is to promote, conduct, and lead integrated multidisciplinary astrobiology research and to train a new generation of astrobiology researchers. For more information about the NAI on the Internet, visit: http://nai.nasa.gov/