Visits to Mars by unmanned probes from NASA and the European Space Agency have found evidence that a prime condition for life once may have existed: water.
"There has been a tremendous amount of very exciting findings this year that Mars once contained actively flowing, low-saline, near-neutral-pH water - pretty much the type of water where you find life on Earth today," said Alison Olcott Marshall, assistant professor of geology at the University of Kansas.
Marshall is working with her colleague, Craig Marshall, associate professor of geology at KU, to improve the way scientists detect condensed aromatic carbon, thought to be a chemical signature of astrobiology.
"If we're going to identify life on Mars, it will likely be the fossil remnants of the chemicals once synthesised by life, and we hope our research helps strengthen the ability to evaluate the evidence collected on Mars," Craig said.
According to a recent paper in the journal Philosophical Transactions of the Royal Society, by itself Raman spectroscopy is able to screen for carbonaceous material, but it can't determine its source - thus the technology needs to be supplemented in order to determine if life exists on Mars.
"Raman spectroscopy works by impinging a laser on a sample so the molecules within that sample vibrate at diagnostic frequencies," Craig said.
"Measuring those frequencies allows the identification of inorganic and organic materials. It's insufficient because however the carbonaceous material is made, it will be the same chemically and structurally, and thus Raman spectroscopy cannot determine the origin," said Craig.
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