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Alien Life may be Hiding Beneath the Shield of Ice on Mars, According to a Study

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According to recent research, dusty ice in the Red Planet’s mid-latitudes may be covering the conditions necessary for photosynthesis to take place on Mars.

The process of photosynthesis is how cyanobacteria, algae, and plants produce chemical energy. In order to continue, it needs light and water, and it produces most of the oxygen in the atmosphere. According to the latest research, Mars may be able to create “radiative habitable zones”—zones where a thick enough covering of ice would block off the sun’s harmful radiation while still allowing enough light to support photosynthesis.

These findings need to be interpreted in the correct context, much as photosynthesis requires the ideal amount of light to occur. The findings do not imply that life has ever existed on Mars or exists now, but they do provide scientists conducting the ongoing search with a direction to search.

The “habitable zone” is the area surrounding a star where conditions are favorable for liquid water to exist on a planet’s surface, and this includes both Earth and Mars. Mars seems to be a largely dry landscape, despite the fact that 71% of Earth’s surface is covered in oceans with liquid water.

It has been revealed by observations made by Mars missions like the Curiosity and Perseverance rovers that this was not always the case. These robots’ explorations of geological features like dried lake basins and river tributaries suggest that liquid water once flowed across the Red Planet’s landscapes billions of years ago. Furthermore, water ice has been discovered on Mars by orbiting missions like NASA’s Mars Reconnaissance Orbiter (MRO), frequently in unexpected places.

Scientists believe that Mars’ atmosphere was mostly stripped away and its magnetic field burnt out billions of years ago, whence Earth’s magnetosphere still exists. This implied that not much could be done to stop water from evaporating and vanishing into space. Due to its thin atmosphere, modern Mars is also subjected to the sun’s intense UV radiation, which is lethal to life and breaks down the intricate molecules required for it.

“Unlike Earth, Mars lacks a protective ozone shield, so there is 30% more harmful ultraviolet radiation at the surface in comparison with our planet,” Khuller stated. “Thus, on Mars, the areas where photosynthesis could occur are more likely to be within dusty ice because the overlying dusty ice blocks the harmful ultraviolet radiation at Mars’ surface, and liquid water is highly unstable at the surface of Mars due to its dry atmosphere.”

The scientists discovered through computer simulations that the shallow liquid water beneath the surface of dusty Mars ice can melt from within, shielded from evaporating into the dry Martian atmosphere by the ice covering it.

“So, the two key ingredients for photosynthesis can be present within dusty Martian ice in the mid-latitudes,” Khuller stated. “For photosynthesis to take place, there must be sufficient sunlight and liquid water. Previous independent models of dense Martian snow have shown that if dust particles (less than 1 percent) are present in the snow, melting below the surface can still happen in the Martian mid-latitudes today.

“By discovering dusty ice exposed within buried dusty snowpacks associated with Martian gullies a few years ago, there is a mechanism for them to melt below the surface to form shallow subsurface liquid water.”

According to Khuller, the researchers discovered that the surrounding ice can shield the exposed dusty ice from the damaging UV rays that reach the surface of Mars. Additionally, enough sun energy can pass through this ice below the surface to support photosynthesis.

The concentration of dust in the ice determines the depths at which these radiative habitable zones are found. According to the team’s models, ice that is very dusty would obstruct too much light. On the other hand, a radiative zone might occur in ice containing 0.01% to 0.1% dust at a depth of 2 to 15 inches (5 to 38 centimeters). At a depth of seven to ten feet (2.2 to 3.1 meters), a wider and deeper radiative zone would be possible with less “polluted” ice.

The team believes that a lack of subsurface melting would make the polar regions of Mars, where most of the planet’s ice is found, too cold for these radiative habitable zones to exist. The Red Planet’s mid-latitude regions would be more prone to experience this kind of melting.

The observable evidence that the team has gathered comes from Earth rather than Mars, lending some credence to their theory.

“I was surprised to find out that there are potentially similar analogs for life within ice on Earth that contains dust and sediment,” Khuller said. “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.”

The study went on to say that every summer, even though the ice above is frozen, liquid water forms surrounding the black dust within the ice as a result of heating from sunshine. This occurs as a result of the ice’s transparency, which lets light through below the surface.

“People have found microorganisms that live in these shallow subsurface habitats on Earth,” Khuller stated. “The microorganisms typically go dormant in the winter when there is not enough sunlight to form liquid water within the dusty ice.”

Naturally, none of this suggests that there is or ever was photosynthetic life on Mars. However, it’s exciting and might encourage more research into the possibility that the Red Planet has subterranean radiative livable zones.

“I am working with a team of scientists to develop improved simulations of if, where, and when dusty ice could be melting on Mars today,” Khuller said. “Additionally, we are recreating some of these dusty ice scenarios in a lab setting to examine them in more detail.”

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Chinese Rover Discovers Signs of Mars’s Ancient Ocean: Study

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Researchers claim that recently analyzed data from a Chinese investigator on Mars supports the body of evidence showing the planet originally had a massive ocean.

Zhurong is the name of the rover, or exploring vehicle. In 2021, it made its surface landing on Mars. Utopia Planitia is the region where the rover has been functioning. The American space organization NASA says that this region is a sizable plain in the northern hemisphere of Mars.

The scientists integrated information from Zhurong’s equipment with observations from spacecraft and satellites circling Mars. Geological elements that suggested an ancient ocean coastline were found in Utopia Planitia, according to the team’s studies.

Several characteristics, according to the experts, suggested that there was a sizable ocean on Mars billions of years ago. The troughs and channels found on the surface could have been created by water flowing across Mars.

Mud volcanoes, which most likely erupted in regions where there had been water or ice, may have produced them, according to earlier studies that looked at data on comparable surface features.

According to the researchers, the data indicates that both shallow and deep ocean conditions were probably present in the region. The results of a recent study were published in the journal Scientific Reports.

The study was primarily written by Bo Wu. At Hong Kong Polytechnic University, he works as a planetary scientist. According to Wu, “We estimate the flooding of the Utopia Planitia on Mars was approximately 3.68 billion years ago. The ocean surface was likely frozen in a geologically short period.”

On Mars, the hunt for water is closely related to the hunt for potential life. The planet might have once hosted microbial life if there is evidence of a former ocean.

Previous research indicates that Mars formerly had a sizable northern ocean. In 2022, one such study was published. Satellite photos of the Martian surface served as the basis for that study. Detailed maps of the planet’s northern hemisphere were created by combining the pictures. Analyzing the maps revealed indications of coastlines that were previously part of a vast ocean.

Evidence from a different study that was published in August suggested that Mars might have a sizable ocean located far below the surface. NASA’s InSight Lander served as the basis for that proof.

In May 2021, the Zhurong rover from China started gathering data. It ceased operations almost a year later, with mission planners stating that dust and sand probably had an impact on the power system. The rover nevertheless outlived its three-month mission.

According to the researchers, the data indicates that the ocean appears to have vanished approximately 3.42 billion years ago.

According to research co-writer Sergey Krasilnikov, the water that most likely filled the Martian ocean was “heavily silted.” At Hong Kong Polytechnic University, he works as a planetary scientist. Water-borne silt is a mixture of clay and sand that eventually settles on land.

Krasilnikov went on to say that the planet “…probably had a thick, warm atmosphere” when the Martian ocean would have been active.” “Microbial life was much more likely at that time,” he stated.

The latest discoveries do “provide further evidence to support the theory of a Martian ocean,” according to Wu of Hong Kong Polytechnic.

The study does “not claim that our findings definitively prove” that there was an ocean on Mars, he told the French news agency AFP. According to him, such evidence would probably necessitate a further trip to return items from Mars to Earth for additional analysis.

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SpaceX launches the enigmatic “Optus-X” from the Kennedy Space Center aboard a Falcon 9 rocket

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At sundown, SpaceX launched a Falcon 9 rocket carrying a payload so secret that no details of the mission have been revealed, and the original designation has been changed.

While SpaceX refers to the mission as “TD7,” all regulatory documents and U.S. government organizations, including the Federal Aviation Administration and the Space Force, refer to the payload as “Optus-X.” During SpaceX’s broadcast, the commentator pointed out that it was a communications satellite.

On Sunday, November 17, at 5:28 p.m. EST (2228 UTC), the spacecraft lifted out from Launch Complex 39A at NASA’s Kennedy Space Center.

At sundown, SpaceX launched a Falcon 9 rocket carrying a payload so secret that no details of the mission have been revealed, and the original designation has been changed.

While SpaceX refers to the mission as “TD7,” all regulatory documents and U.S. government organizations, including the Federal Aviation Administration and the Space Force, refer to the payload as “Optus-X.” During SpaceX’s broadcast, the commentator pointed out that it was a communications satellite.

On Sunday, November 17, at 5:28 p.m. EST (2228 UTC), the spacecraft lifted out from Launch Complex 39A at NASA’s Kennedy Space Center.

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Researchers find that laser light has the ability to cast shadows

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A blue laser was used to illuminate the ruby cube from the side while a high-power green laser was focused through it for the experiment. In order to produce a matched region in the illuminating light and a darker area that looks as a shadow of the green laser beam, the green laser increases the optical absorption of the blue illuminating laser beam.

Is it possible for light to cast a shadow? Researchers have discovered that, in some circumstances, a laser beam can behave like an opaque object and cast a shadow, which may sound like a philosophical conundrum. The finding casts doubt on the conventional wisdom regarding shadows and creates new opportunities for devices that could manipulate another laser beam with a laser beam.

“Laser light casting a shadow was previously thought impossible since light usually passes through other light without interacting,” said Raphael A. Abrahao, the leader of the study team from Brookhaven National Laboratory, formerly at the University of Ottawa. “Our demonstration of a very counter-intuitive optical effect invites us to reconsider our notion of shadow.”

In Optica, scientists explain how they demonstrated that a laser beam could block light and produce a visible shadow because of a nonlinear optical process using a ruby crystal and particular laser wavelengths. Light can affect another optical field when it interacts with a material in an intensity-dependent manner.

“Our understanding of shadows has developed hand-in-hand with our understanding of light and optics,” Abrahao stated. “This new finding could prove useful in various applications such as optical switching, devices in which light controls the presence of another light, or technologies that require precise control of light transmission, like high-power lasers.”

The new study is a part of a broader investigation of nonlinear optical processes and the interaction of two light beams under specific conditions.

Some experimental drawings created with 3D visualization software portray the shadow of a laser beam because they interpret it as a cylinder without taking into account the physics of a laser beam. This idea was first raised during a lunch chat. Could this be done in a lab? asked some of the scientists.

“What started as a funny discussion over lunch led to a conversation on the physics of lasers and the nonlinear optical response of materials,” Abrahao remarked. “From there, we decided to conduct an experiment to demonstrate the shadow of a laser beam.”

The researchers accomplished this by shining a blue laser sideways on a cube of regular ruby crystal and passing a high-power green laser through it. The material’s reaction to the blue wavelength is locally altered when the green laser enters the ruby. Whereas the blue laser behaves like illumination, the green laser behaves like a regular object.

On a screen, the interaction of the two light sources produced a shadow that could be seen as a dark spot where the blue light was blocked by the green laser. Because it was visible to the unaided eye, followed the outlines of the surface it fell on, and followed the location and form of the laser beam, which functioned as an object, it satisfied all the requirements for a shadow.

The ruby’s optical nonlinear absorption is what causes the laser shadow effect. The green laser produces a corresponding region in the illuminating light with reduced optical intensity by increasing the blue illuminating laser beam’s optical absorption. As a result, the green laser beam appears as a shadow in a darker area.

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