A NASA-led study has revealed that alien life could be hiding beneath the icy layers of Mars.

Scientists suggested that the Red Planet’s ancient ice packs may have long acted as a shield for microbial life, blocking out ᴅᴇᴀᴅly cosmic radiation.

But the key to their survival would be ice that likely formed from dusty snowfall, where sunlight absorbed by that darker dust would allow pockets of melt water to develop safely under its icy surface, lead author Dr Aditya Khuller told DailyMail.com.

Computer modeling showed that the amount of light piecing the water ice could trigger pH๏τosynthesis in these shallow pools of meltwater — similar to pools on Earth that are teeming with life.

‘These are called “cryoconite holes” and form when dust and sediment on top of the ice melt into the ice because it is darker than the ice,’ said Dr Khuller, who worked as a planetary scientist at NASA’s Jet Propulsion Laboratory.

A host of tiny, plant-like creatures have been documented in cryoconite holes on Earth — including algae, fungi, and cyanobacteria, all of which pull in energy from the sun via pH๏τosynthesis to live.

‘If we’re trying to find life anywhere in the universe today, Martian ice exposures are probably one of the most accessible places we should be looking,’ Dr Khuller said.

A 2016 image from NASA’s Mars Reconnaissance Orbiter documenting what scientists believe is dusty ice lining the edges of a set of Martian gullies. Planetary scientist Dr Aditya Khuller and his co-authors believe this ice (pictured) should be a prime candidate in the search for alien life

These cryoconite colonies have been uncovered and studied everywhere from Antarctica, to Greenland, to Norway’s Svalbard archipelago: an island chain midway between the Scandinavian country’s northern coast and the North Pole.

‘The microorganisms typically go dormant in the winter,’ Dr Khuller told Space.com, ‘when there is not enough sunlight to form liquid water within the dusty ice.’

‘So, the two key ingredients for pH๏τosynthesis can be present within dusty Martian ice in the mid-laтιтudes,’ he added. ‘PH๏τosynthesis requires adequate amounts of sunlight and also liquid water to occur.’

The new study builds off of Dr Khuller’s work as a PhD student, when he worked on a project to predict the dust content of ice deposits on Mars — based off of data collected by NASA’s Phoenix Mars Lander and its Mars Reconnaissance Orbiter.

The team poured this data into computer simulations that were originally built to predict the brightness of terrestrial snow and glacier ice on Earth.

These brightness models built off of Earth’s well-studied and better understood ice, they theorized, would help estimate the dust content mixed into distant Martian ice.

‘This small amount of dust has a very important effect,’ Dr Khuller told DailyMail.com.

‘The depth to which enough sunlight can reach for pH๏τosynthesis to occur within the ice changes depending on how dusty the ice is,’ he noted. ‘Similarly, the amount of dust within the ice also changes the depth [down] to which harmful ultraviolet radiation can penetrate.’

The Martian life that may one day be found in the Red Planet’s dusty ice might resemble life in ‘ ‘cryoconite holes’ here on Earth. Above, researchers sample a cryoconite hole on the Longyearbreen glacier, somewhere along Norway’s Svalbard archipelago in 2017

‘The microorganisms typically go dormant in the winter when there is not enough sunlight to form liquid water within the dusty ice,’ researchers said. Above, More cryoconite sampling performed during that same field work for a 2017 Arctic microbiology course on Svalbard

The team’s computer modelling efforts predicted that ice containing higher amounts of dust, 0.01 to 0.1 percent, will only be able to support life at a depth around five to 38 centimeter below the surface.

But, Dr Khuller noted: ‘There are zones where pH๏τosynthesis could occur at […] meter-depths for cleaner ice.’

The cleaner ice was found to be especially fertile territory for deeper pockets of microbial life along Mars’ mid-laтιтude ranges, in both its northern and southern hemispheres.

At 40° laтιтude in both hemispheres, these colonies of tiny alien life could exist as far down as 2.15 to 3.10 meters deep, based on Dr Khuller and his team’s estimates,  published Thursday in the journal Nature Communications Earth & Environment.

‘We are not stating we have found life on Mars,’ Dr Khuller emphasized to reporters, ‘but instead we believe that dusty Martian ice exposures in the mid-laтιтudes represent the most easily accessible places to search for Martian life today.’

But, complicating matters, Mars, unlike Earth, has two different kinds of naturally occurring ice: frozen water and frozen carbon dioxide, a la man-made ‘dry ice.’

Thanks to the thin and dry atmosphere on Mars, planetary and atmospheric scientists are still debating whether or not melting ‘water ice’ even becomes liquid water there at all — with many arguing it ‘sublimates’ immediately into water vapor.