Chile’s arid desert is said to be the closest thing to Mars that we have on Earth and a new discovery in the hellish landscape could help scientists find life on the Red Planet.

A team from Cornell University uncovered diverse microbes lurking in wet clay just 11 inches below the surface of the Atacama Desert, suggesting there could be biosignatures in similar clay deposits on the Martian planet.

The Gale crater on Mars is littered with similar clay-rich rocks and may have been habitable to microorganisms similar to those found in subsurface soils in the Earth-based desert.

Researches note that if NASA‘s 2020 rover spots the same fractures around Gale Crater, the region ‘should be high-priority targets for sample’ in order to find life. 

The study reinforces the notion that early Mars could have had a similar subsurface, particularly during the first billion years of its history. 

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A team from Cornell University uncovered diverse microbes lurking in wet clay just 11 inches below the surface of the Atacama Desert, suggesting there could be biosignatures in similar clay deposits on the Martian planet

Scientists worked in the Yungay region of the Atacama desert and found the layer of clay that was a previously unreported habitat for at least 30 salt-loving microbial species of single-celled, metabolically active bacteria and archaea.

Corresponding author Alberto G. Fairén said: ‘Our discovery suggests that something similar may have occurred billions of years ago—or it still may be occurring—on Mars.’

‘That’s why clays are important.’

‘They preserve organic compounds and biomarkers extremely well and they are abundant on Mars.’ 

The Gale crater (pictured) on Mars is littered with similar clay-rich rocks and may have been habitable to microorganisms similar to those found in subsurface soils in the Earth-based desert.

The Gale crater (pictured) on Mars is littered with similar clay-rich rocks and may have been habitable to microorganisms similar to those found in subsurface soils in the Earth-based desert.

The Gale crater (pictured) on Mars is littered with similar clay-rich rocks and may have been habitable to microorganisms similar to those found in subsurface soils in the Earth-based desert.

Scientists worked in the Yungay region of the Atacama desert and found the layer of clay that was a previously unreported habitat for at least 30 salt-loving microbial species (pictured) of single-celled, metabolically active bacteria and archaea

Scientists worked in the Yungay region of the Atacama desert and found the layer of clay that was a previously unreported habitat for at least 30 salt-loving microbial species (pictured) of single-celled, metabolically active bacteria and archaea

Scientists worked in the Yungay region of the Atacama desert and found the layer of clay that was a previously unreported habitat for at least 30 salt-loving microbial species (pictured) of single-celled, metabolically active bacteria and archaea

Fairén and his team dug a pit in the middle of Yungay to gather samples from the soil.

At 11 inches deep, they identified a number of minerals, including quartz and albite, along with a layer of wet clay mineral-rich soil.

Researchers dug four more ditches in the area and found the same wet layer ‘confirming the existence of a widespread and sustained phenomenon of sub-surface water availability at Yungay, reads the study published in Nature.

‘To the best of our knowledge, this represents the first detection of wet subsurface clay-rich layers (or any other type of subsurface wet minerals) at Yungay or other sites of the hyperarid core of the Atacama.’

The  team dug pits in the middle of Yungay to gather samples from the soil. At 11 inches deep, they identified a number of minerals, including quartz and albite, along with a layer of wet clay mineral-rich soil

The  team dug pits in the middle of Yungay to gather samples from the soil. At 11 inches deep, they identified a number of minerals, including quartz and albite, along with a layer of wet clay mineral-rich soil

The  team dug pits in the middle of Yungay to gather samples from the soil. At 11 inches deep, they identified a number of minerals, including quartz and albite, along with a layer of wet clay mineral-rich soil

The team links the wet clay to unusually intense rain that hit the area over the past decades, but in 2017, Yungay received so much participation that lagoons had formed – a phenomenon never observed before in this region in the past 500 years.

‘Although the exact environmental conditions on early Mars are largely unknown, similarities in mineralogy between soils at Yungay and Noachian- and Hesperian-aged Martian terrains indicate similar conditions to those in Yungay soils may have existed on early Mars,’ according to the study.

NASA has previously detected sulfates and chlorides in the Martian planet’s orbit, are commonly found in arid and evaporative environments on Earth, and have been identified in depressions and impact craters on Mars –providing more similarities between the Atacama desert’s and the Red plant’s environments.

‘The results presented here, showing that wet subsurface clay minerals are inhabited by a number of metabolically active microorganisms in the midst of the driest place on earth, isolated and protected just centimeters bellow the extremely harsh surface environmental conditions typical of the Atacama, reinforce the notion that early Mars could have been a planet with similar subsurface protected habitable niches, particularly during the first billion years of its history,’ researchers shared in the study.

WHAT EVIDENCE DO SCIENTISTS HAVE FOR LIFE ON MARS?

The search for life on other planets has captivated mankind for decades.

But the reality could be a little less like the Hollywood blockbusters, scientists have revealed.

They say if there was life on the red planet, it probably will present itself as fossilized bacteria – and have proposed a new way to look for it.

Here are the most promising signs of life so far –

Water 

When looking for life on Mars, experts agree that water is key.

Although the planet is now rocky and barren with water locked up in polar ice caps there could have been water in the past.

In 2000, scientists first spotted evidence for the existence of water on Mars.

The Nasa Mars Global Surveyor found gullies that could have been created by flowing water.

The debate is ongoing as to whether these recurring slope lineae (RSL) could have been formed from water flow.

Meteorites 

Earth has been hit by 34 meteorites from Mars, three of which are believed to have the potential to carry evidence of past life on the planet, writes Space.com.

In 1996, experts found a meteorite in Antarctica known as ALH 84001 that contained fossilised bacteria-like formations.

However, in 2012, experts concluded that this organic material had been formed by volcanic activity without the involvement of life.

Signs of Life 

The first close-ups of the planet were taken by the 1964 Mariner 4 mission.

These initial images showed that Mars has landforms that could have been formed when the climate was much wetter and therefore home to life.

In 1975, the first Viking orbiter was launched and although inconclusive it paved the way for other landers.

Many rovers, orbiters and landers have now revealed evidence of water beneath the crust and even occasional precipitation.

Earlier this year, Nasa’s Curiosity rover found potential building blocks of life in an ancient Martian lakebed.

The organic molecules preserved in 3.5 billion-year-old bedrock in Gale Crater — believed to have once contained a shallow lake the size of Florida’s Lake Okeechobee — suggest conditions back then may have been conducive to life.

Future missions to Mars plan on bringing samples back to Earth to test them more thoroughly.

Methane 

In 2018, Curiosity also confirmed sharp seasonal increases of methane in the Martian atmosphere.

Experts said the methane observations provide ‘one of the most compelling’ cases for present-day life.

Curiosity’s methane measurements occurred over four-and-a-half Earth years, covering parts of three Martian years.

Seasonal peaks were detected in late summer in the northern hemisphere and late winter in the southern hemisphere. 

The magnitude of these seasonal peaks – by a factor of three – was far more than scientists expected.

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