Never-before-seen microbes in Arctic could aid search for life on Mars
McGill researchers studied the extremely salty, very cold, and almost oxygen-free environment under the permafrost of Lost Hammer Spring in Canada’s High Arctic to search for life. Why? Because that environment is the closest to Mars' that exists on Earth, according to a press release published by the institution this week.
Microbes not only surviving but thriving
In this new study, the scientists found that microbes managed to survive—and even thrive—indicating that there may also be life on the Red Planet. The researchers even used state-of-the-art genomic techniques to gain insight into the microbe's metabolisms.
They found that the microorganisms can survive by eating and breathing simple inorganic compounds of a kind that have been detected on Mars, such as methane, sulfide, sulfate, carbon monoxide, and carbon dioxide.
“It took a couple of years of working with the sediment before we were able to successfully detect active microbial communities,” explained Elisse Magnuson, a Ph.D. student at McGill and the first author on the paper. “The saltiness of the environment interferes with both the extraction and the sequencing of the microbes, so when we were able to find evidence of active microbial communities, it was a very satisfying experience.”
DNA sequenced from 110 mostly new organisms
The researchers sequenced DNA from the spring community by reconstructing the genomes of approximately 110 microorganisms, most of which have never been seen before.
“The microbes we found and described at Lost Hammer Spring are surprising, because, unlike other microorganisms, they don’t depend on organic material or oxygen to live,” added study lead Lyle Whyte of the Department of Natural Resource Sciences.
“Instead, they survive by eating and breathing simple inorganic compounds such as methane, sulfides, sulfate, carbon monoxide and carbon dioxide, all of which are found on Mars. They can also fix carbon dioxide and nitrogen gasses from the atmosphere, all of which makes them highly adapted to both surviving and thriving in very extreme environments on Earth and beyond.”
Lost Hammer Spring, in Nunavut in Canada’s High Arctic, is one of the coldest and saltiest terrestrial springs ever discovered. The water is extremely salty (~24% salinity), perennially at sub-zero temperatures (~−5 °C), and contains almost no oxygen (<1ppm dissolved oxygen).
These types of conditions have also been found in certain areas on Mars, where widespread salt deposits and possible cold salt springs have been observed. Past studies have also found evidence of microbes in this kind of Mars-like environment. However, the McGill study is one of a very few to find microbes alive and active.
The research was published in Nature magazine.
Lost Hammer Spring, located in the High Arctic of Nunavut, Canada, is one of the coldest and saltiest terrestrial springs discovered to date. It perennially discharges anoxic (<1 ppm dissolved oxygen), sub-zero (~−5 °C), and hypersaline (~24% salinity) brines from the subsurface through up to 600 m of permafrost. The sediment is sulfate-rich (1 M) and continually emits gases composed primarily of methane (~50%), making Lost Hammer the coldest known terrestrial methane seep and an analog to extraterrestrial habits on Mars, Europa, and Enceladus. A multi-omics approach utilizing metagenome, metatranscriptome, and single-amplified genome sequencing revealed a rare surface terrestrial habitat supporting a predominantly lithoautotrophic active microbial community driven in part by sulfide-oxidizing Gammaproteobacteria scavenging trace oxygen. Genomes from active anaerobic methane-oxidizing archaea (ANME-1) showed evidence of putative metabolic flexibility and hypersaline and cold adaptations. Evidence of anaerobic heterotrophic and fermentative lifestyles were found in candidate phyla DPANN archaea and CG03 bacteria genomes. Our results demonstrate Mars-relevant metabolisms including sulfide oxidation, sulfate reduction, anaerobic oxidation of methane, and oxidation of trace gases (H2, CO2) detected under anoxic, hypersaline, and sub-zero ambient conditions, providing evidence that similar extant microbial life could potentially survive in similar habitats on Mars.