What if the secrets to discovering life on Mars lie hidden in our own environment? In the planet’s most extreme habitats, microbial life flourishes in unlikely places—from icy tundras to searing, acidic springs. These unique ecosystems not only support life but also preserve evidence of it. Among these, hot springs are particularly notable for generating distinctive silica-rich formations.Silica Center is capable of trapping remnants of ancient microbes.

Silica occurs when silica-laden water from hot springs rises, cools, and evaporates, leaving behind hardened silica that can encapsulate microorganisms, thus fossilizing them. NASA’s Spirit Rover discovered similar silica sinter in Gusev Crater on Mars, raising questions about whether these ancient Martian hot springs may also preserve signs of past life.

An international research team has revealed that fat-like molecules from cells, lipids, can endure alongside these silica sinters and might be detected using equipment akin to that on Martian rovers. These lipids can persist for millions of years and serve as chemical fossils, or biomarkers in the fossil record. They provide insights into the types of life that once existed in these environments, aiding scientists in reconstructing ancient ecosystems.

Researchers collected silica sintered samples from six hot springs in New Zealand’s Taupo volcanic region, where the waters range from 77°F to 203°F (25°C to 95°C) and vary in acidity. First, they extracted the lipids from the sintered material chemically. Next, they characterized these lipids using instruments that fragment the molecules into smaller components, identifying them by mass.Gas chromatography-mass spectrometry (GC-MS) was utilized.

The team employed GC-MS to identify a broad array of lipid molecules, including fatty acids, alcohols, sterols, and n-alkanes from the sinter. Most of these molecules likely originated from bacteria that either use sunlight or sulfate as an energy source, and such microorganisms are well-suited for extreme environments. Some lipids identified also stemmed from other sources, like algae and plants. The researchers interpreted this diversity of lipids as indicative of both ancient and contemporary microorganisms. They referred to the old fossilized communities preserved with newer ones in the silica, noting the mix of heat-altered and fresh compounds.

The shape and texture of sintered rocks were also found to influence the preservation of lipid biomarkers. A fine, pointed texture known as spicular sinter retained more lipids compared to knobbed or crusty types. These thorny textures form at the edges of hot spring pools where microorganisms interact with rapidly cooled silica-rich water, creating delicate silica structures that grow like small fingers. Researchers suggested that these fine textures offer protection to microorganisms against erosion and radiation. They believe these finger-like silica formations are particularly promising for detecting traces of past life on Mars, similar to those seen by the Spirit Rover.

To evaluate whether current Rover instruments could detect ancient lipids, researchers analyzed two silica sintered samples using techniques similar to those used by rovers.NASA’s Curiosity Rover employs a method called Pyrolysis-GC-MS, which does not require prior chemical extraction of lipids. The entire sample is heated until the molecules transform into gas, which is then analyzed.

In one sintered sample, the instrument successfully identified simple lipids commonly produced by organisms, such as n-alkanes, pristanes, and phytanes. In another sulfur-rich sample, it detected a sulfur-based compound known as thiophene, also found on Mars. However, the analysis did not reveal more complex biomarkers like hopane and sterols, likely because they were degraded by heat. Pyrolysis may result in quantities too small for GC-MS to detect.

Based on these findings, researchers concluded that current rover instruments can successfully detect simple and durable lipids but may overlook more delicate or complex ones. To enhance the likelihood of finding ancient biosignatures, the team recommended that future Mars missions adopt less destructive detection approaches. Despite these challenges, they suggested that silica-rich rocks, like those in the Gusev Crater, are prime targets for exploring evidence of ancient Martian life. By pinpointing the most suitable rock textures for lipid preservation that can be detected with existing rover technologies, scientists are one step closer to uncovering signs of life on Mars.

Post view: 557