When humans get to Mars one day, they'll have some pressing needs. One of those is water.

Water is substantial and difficult to move through space, so preferably they'll have the option to discover what they need to make due on Mars itself.&nbsp;

A new study led by researchers at the Planetary Science Institute (PSI) points to a "large, previously unrecognized reservoir of water ice" in the Nereidum Montes region of Mars.&nbsp;

The paper - distributed in the diary Icarus - inspected Viscous Flow Features (VFFs), frosty developments found on the red planet.&nbsp;

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VFFs have been contrasted and chilly arrangements on Earth and could be a likely wellspring of water for space travelers.&nbsp;

"Our radar examination shows that in any event one of these highlights is around 500 meters thick and almost 100 per cent&nbsp;ice, with a flotsam and jetsam covering all things considered ten meters thick," said PSI Senior researcher Daniel Berman, lead creator of the paper, in articulation on Monday.&nbsp;

These water ice stores could speak to "conceivably the biggest groupings of any non-polar area in the southern half of the globe," as indicated by PSI. The specialists utilized information from NASA's Mars Reconnaissance Orbiter to find the VFFs, which date to inside the last hardly any million years of the planet's set of experiences.&nbsp;

The study ties in with other research on the history and current presence of water on Mars. NASA shared a "treasure map" of water ice deposits on Mars in 2019.

While it's enticing to pack a hairdryer and straw and head for Nereidum Montes, it won't be that straightforward for future red planet adventurers. "This area would be an intriguing landing site because of the lot of ice, which could be utilized as a hotspot for water," Berman said. "Shockingly, it is bumpy territory and it would almost certainly be extremely hard to land there."

When humans get to Mars one day, they'll have some pressing needs. One of those is water. Water is substantial and difficult to move through space, so preferably they'll have the option to discover what they need to make due on Mars itself.

When humans get to Mars one day, they'll have some pressing needs. One of those is water. Water is substantial and difficult to move through space, so preferably they'll have the option to discover what they need to make due on Mars itself. A new study led by researchers at the Planetary Science Institute (PSI) points to a "large, previously unrecognized reservoir of water ice" in the Nereidum Montes region of Mars. The paper - distributed in the diary Icarus - inspected Viscous Flow Features (VFFs), frosty developments found on the red planet. Also read: Aliens calling? Scientists receive radio signals from faraway planet VFFs have been contrasted and chilly arrangements on Earth and could be a likely wellspring of water for space travelers. "Our radar examination shows that in any event one of these highlights is around 500 meters thick and almost 100 per cent ice, with a flotsam and jetsam covering all things considered ten meters thick," said PSI Senior researcher Daniel Berman, lead creator of the paper, in articulation on Monday. These water ice stores could speak to "conceivably the biggest groupings of any non-polar area in the southern half of the globe," as indicated by PSI. The specialists utilized information from NASA's Mars Reconnaissance Orbiter to find the VFFs, which date to inside the last hardly any million years of the planet's set of experiences. The study ties in with other research on the history and current presence of water on Mars. NASA shared a "treasure map" of water ice deposits on Mars in 2019. While it's enticing to pack a hairdryer and straw and head for Nereidum Montes, it won't be that straightforward for future red planet adventurers. "This area would be an intriguing landing site because of the lot of ice, which could be utilized as a hotspot for water," Berman said. "Shockingly, it is bumpy territory and it would almost certainly be extremely hard to land there."

Scientists discover 'previously unrecognised' water ice reservoir on Mars

Mars&nbsp;has two&nbsp;''lumpy'' moons and their existence suggests that the red planet had rings&nbsp;around,&nbsp;like some of the larger planets in our solar system.

The findings were&nbsp;presented&nbsp;during the 236th Meeting of the American Astronomical Society, which is being held virtually this week during the pandemic.

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The two lumpy moons, Phobos and Deimos, were both discovered in 1877 and named after the sons of Ares from Greek mythology.

Mars is named after the Roman god of war, which is Ares in Greek. Phobos means fear or panic and Deimos means dread.

Scientists believed that they were asteroids captured by the planet's gravity for a very long time.&nbsp;Both appear to be&nbsp;similar in composition to blackish carbonaceous chondrite asteroids.&nbsp;

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However,&nbsp;the recent research revealed that the moons are nearly in the same plane as the Martian equator. This suggests that they formed around the same time Mars did around 4.5 billion years ago.

Over time, Phobos&nbsp;will lose&nbsp;height as it interacts with Martian gravity and eventually, its orbit will be too low and Mars will essentially rip it into pieces that form a ring around the planet. It's estimated that this will happen within 50 million years.

Phobos, slightly larger than Deimos, is only about 3,700 miles above the Martian surface, no known moon in our solar system is closer to its planet.&nbsp;

Being so close, Phobos completes three orbits around Mars in one Earth day, while Deimos, which is more distant, takes about 30 Earth hours to complete an orbit.

The researchers believe that Phobos once had a grandparent 3 billion years ago that they called proto-Phobos — likely 20 times more massive as the small moon is now. Over the course of a few moon-ring cycles, it became Phobos — which would explain why some researchers believe it only formed about 200 million years ago.

A prominent ring around Mars would have pushed proto-Phobos outward, away from the planet. This would have also affected proto-Phobos' orbital resonance with Deimos and pushed it further from Mars as well.

The Japanese space agency, JAXA, plans to send a spacecraft to Phobos in 2024 to collect samples from the surface and return them to Earth. This may reveal more about the moon's past.

Mars has two ''lumpy'' moons and their existence suggests that the red planet had rings around, like some of the larger planets in our solar system. The findings were presented during the 236th Meeting of the American Astronomical Society, which is being held virtually this week during the pandemic.

Mars has two ''lumpy'' moons and their existence suggests that the red planet had rings around, like some of the larger planets in our solar system. The findings were presented during the 236th Meeting of the American Astronomical Society, which is being held virtually this week during the pandemic. Also read: NASA seeking volunteers for paid isolation during 'fake' Mars mission The two lumpy moons, Phobos and Deimos, were both discovered in 1877 and named after the sons of Ares from Greek mythology. Mars is named after the Roman god of war, which is Ares in Greek. Phobos means fear or panic and Deimos means dread. Scientists believed that they were asteroids captured by the planet's gravity for a very long time. Both appear to be similar in composition to blackish carbonaceous chondrite asteroids. Also read: Indian-origin teenager names NASA’s first Mars helicopter However, the recent research revealed that the moons are nearly in the same plane as the Martian equator. This suggests that they formed around the same time Mars did around 4.5 billion years ago. Over time, Phobos will lose height as it interacts with Martian gravity and eventually, its orbit will be too low and Mars will essentially rip it into pieces that form a ring around the planet. It's estimated that this will happen within 50 million years. Phobos, slightly larger than Deimos, is only about 3,700 miles above the Martian surface, no known moon in our solar system is closer to its planet. Being so close, Phobos completes three orbits around Mars in one Earth day, while Deimos, which is more distant, takes about 30 Earth hours to complete an orbit. The researchers believe that Phobos once had a grandparent 3 billion years ago that they called proto-Phobos — likely 20 times more massive as the small moon is now. Over the course of a few moon-ring cycles, it became Phobos — which would explain why some researchers believe it only formed about 200 million years ago. A prominent ring around Mars would have pushed proto-Phobos outward, away from the planet. This would have also affected proto-Phobos' orbital resonance with Deimos and pushed it further from Mars as well. The Japanese space agency, JAXA, plans to send a spacecraft to Phobos in 2024 to collect samples from the surface and return them to Earth. This may reveal more about the moon's past.

Mars' 'lumpy' moons suggests existence of ring around it

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Scientists discover 'previously unrecognised' water ice reservoir on Mars

Mars' 'lumpy' moons suggests existence of ring around it