Newswise — ITHACA, N.Y. – Current state-of-the-art instrumentation being sent to Mars to collect and analyze evidence of life might not be sensitive enough to make accurate assessments, according to a research team co-led by a Cornell University astronomer.
In a paper published in Nature Communications, visiting planetary scientist Alberto Fairén, and an international team of researchers, claim that ancient organic material in Martian rocks could be difficult, if not impossible, to detect with current instruments and techniques.
Fairén – also a research professor at the Center of Astrobiology (CAB) in Madrid – and colleagues conducted tests on sedimentary rocks found in the Red Stone Jurassic fossil delta of the Atacama Desert in northwestern Chile, the oldest and driest desert on Earth and a popular geological analog to Mars.
This revealed to the researchers that the instrumentation sent to Mars might not be sensitive enough, depending on the instrument used and the organic compound being sought. “Specifically, the chance of obtaining false negatives in the search for life on Mars highlights the need for more powerful tools,” said lead author Armando Azua-Bustos, a research scientist on Fairén’s team at CAB.
Either putting complex instrumentation on Mars, approximately 53 million miles away, or bringing Martian samples to Earth is necessary in order “to conclusively address whether life ever existed on Mars,” the researchers wrote. In this case, both options are extremely difficult, Fairén said.
“You need to decide whether is more advantageous having limited capability for analysis on the surface of Mars to interrogate a wide variety of samples,” he said, “or having limited samples to be analyzed with the wide variety of state-of-the-art instrumentation on Earth.”
NASA is currently partnering with the European Space Agency and others in an effort to safely transport Martian geological samples gathered by the Perseverance rover to Earth. And Fairén said the first European Mars rover, named Rosalind Franklin, is also expected to launch as early as 2028.
“This European rover will carry a drill with the unprecedented capability of reaching down to a depth of 2 meters (6 ½ feet) to analyze sediments better protected against the harsh conditions on the Martian surface,” he said. “If biosignatures are better preserved at depth, which we expect, there will be more abundance and diversity, and better preservation of biosignatures, in those deep samples. Our instruments in the rover will therefore have more chances to detect them.”
For additional information, see this Cornell Chronicle story.
Cornell University has dedicated television and audio studios available for media interviews.
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