Mars Rovers Will Need to Dig Deeper If They Want to Find Evidence of Life

The search for life—even ancient life—on Mars is trickier than we thought. In a recent study published in the journal Astrobiology, researchers have determined that NASA’s Mars Perseverance (Percy) Rover will have to dig two meters (6.6 feet) beneath the Martian surface in order to find traces of ancient life. This is because the surface of Mars is constantly bombarded with extreme levels of solar radiation that scientists hypothesize would quickly degrade small molecules such as amino acids. The reason for this extreme level of radiation is due to the absence of a magnetic field, which scientists believe was stripped away billions of years ago when the planet’s liquid outer core ceased to produce the dynamo that created the field.

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We've Seen a Helicopter on Mars. Next, Sailplanes?

The team conducted a tethered launch of an early version of the sailplane, in which it descended slowly to Earth attached to a balloon. Credit: University of Arizona.

The success of the Mars Ingenuity helicopter has encouraged engineers to consider and reconsider all options for remote aerial observations of the Red Planet.  Additional methods for birds-eye views of Mars would not only provide higher resolution data on the landscapes where rovers can’t go — such as canyons and volcanoes — but also could include studying atmospheric and climate processes that current orbiters and rovers aren’t outfitted to observe.  

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A New Map of Mars, Made From 51,000 Orbital Images

Seen are six views of the Nili Fossae region of Mars captured by the Compact Reconnaissance Imaging Spectrometer for Mars, or CRISM, one of the instruments aboard NASA’s Mars Reconnaissance Orbiter. The varying colors represent minerals on the Martian surface seen in different wavelengths of light. Credits: NASA/JPL-Caltech/JHU-APL

When NASA sent the Mars Reconnaissance Orbiter (MRO) to the red planet in 2006, the spacecraft took an instrument with it called CRISM—Compact Reconnaissance Imaging Spectrometer for Mars. CRISM’s job is to produce maps of Mars’ surface mineralogy. It’s been an enormous success, but unfortunately, the loss of its last cryocooler in 2017 means the spectrometer can only undertake limited observations.

But CRISM is going out with a bang, creating one final image of the surface of Mars that NASA will release in batches over the next six months.

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Curiosity Finds Life-Crucial Carbon in Mars Rocks

Curiosity at Mt. Sharp, Gale Crater, Mars. To the left of the rover are two drill holes into the rocks "Aberlady" and "Kilmarie." Curiosity found high concentrations of clay in both rocks. Image Credit: NASA/JPL-Caltech/MSSS

We are carbon-based life forms. That means the basis for the chemical compounds that forms our life is the element carbon. It’s crucial because it bonds with other elements such as hydrogen and oxygen to create the complex molecules that are part of life. So, when we look for evidence of life elsewhere in the solar system, we look for carbon. That includes Mars.

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Dust Devils and Strong Winds Produce the Constant Haze on Mars

Dust is an everyday feature on Mars and wreaks havoc on various pieces of equipment humans decide to send to it, such as Insight’s continual loss of power or the losses of Opportunity and Spirit. But we’ve never really understood what causes the dust to get up into the air in the first place. That equipment that is so affected by it usually isn’t set up to monitor it, or if it is, it has been sent to a place where there isn’t much dust, to begin with. Now, that has changed with new readings from Perseverance in Jerezo crater, and the answer shouldn’t be much of a surprise – dust devils seem to cause some of the dust in the atmosphere on Mars. But strong winds contribute a significant amount too.

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Amazing Flaky Martian Rocks Were Formed in a Stream or a Small Pond

Since 2012, NASA’s Curiosity rover has been exploring the Gale Crater for clues about Mars’ past and possible evidence that it once supported life. For the past year, this search has centered on the lower levels of Mount Sharp, a transitional zone between a clay-rich region and one filled with sulfates (a type of mineral salt). These regions can offer insight into Mars’ warm, watery past, but the transition zone between them is also of scientific value. In short, the study of this region may provide a record of the major climatic shift that took place billions of years ago on Mars.

For example, this region has unique geological features that include clay minerals that appear as flaky layers of sedimentary rock. One in particular, “The Prow,” was recently imaged by Curiosity and had the mission science teams buzzing. These features formed when water still flowed into the Gale Crater, depositing sediment at the base of Mount Sharp. Higher on the mountain, the hill was likely covered in wind-swept dunes that hardened into rock over time. In between them is where the flaky layers formed, possibly as a result of small ponds or streams that wove them among the dunes.

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Could We Use Mars as a Base for Asteroid Mining?

A composite image of Mars and its two moons, Phobos (foreground) and Deimos (background). Credit: NASA/JPL/University of Arizona

The earliest mention of asteroid mining might be in a story from 1898 titled “Edison’s Conquest of Mars,” by Garrett Serviss. In that story, Martians attack Earth, killing tens of thousands and destroying New York City. Earth retaliates and sends an armada to Mars. While travelling, the armada comes across an asteroid that the Martians are mining. The asteroid is a rubble pile of gold nuggets.

A conversation breaks out among the crew.

“Phew! Won’t we be rich?” exclaimed a voice.

“How are we going to dig it and get it back to earth?” asked another.

“Carry it in your pockets,” said one.

“No need of staking claims here,” remarked another. “There is enough for everybody.”

Their conversation was a prescient hint of things to come.

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This Bizarre Terrain on Mars is Caused by Water Ice and Carbon Dioxide

Spring fans and polygons on Mars, as seen by the HiRISE camera on the Mars Reconnaissance Orbiter. Credit: NASA/JPL-Caltech/UArizona.

From orbit, this landscape on Mars looks like a lacy honeycomb or a spider web. But the unusual polygon-shaped features aren’t created by Martian bees or spiders; they are actually formed from a ongoing process of seasonal change from created from water ice and carbon dioxide.

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A Perfectly Balanced Rock Seen by Perseverance

NASA's Mars Perseverance rover acquired this image using its Right Mastcam-Z camera. Mastcam-Z is a pair of cameras located high on the rover's mast. This image was acquired on June 12, 2022 (Sol 466) at the local mean solar time of 12:20:39. Image Credit: NASA/JPL-Caltech/ASU

The Perseverance rover has begun exploring a region that looks a little like Monument Valley in Arizona and Utah in the US, or perhaps like a set on an old sci-fi movie. The rover’s science team has nicknamed the area “Hogwallow Flats,” and the rock formations in this area on Mars are stunning in their varied and sometimes absurd shapes and structures. One wonders what took place here eons ago to create the weird variety of formations.

While small, one feature catches the eye:  a smaller rock that appears to be perfectly perched and balanced on top of a larger rock formation.

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Japan’s Upcoming Mission Will Use a Vacuum to Get its Sample From Phobos

The Martian Moons eXploration (MMX) mission (courtesy: JAXA/NASA).

JAXA, the Japanese Aerospace Exploration Agency, is carving out a niche for itself in sample-return missions. Their Hayabusa mission was the first mission to sample an asteroid when it brought dust from the asteroid Itokawa to Earth in 2010. Then its successor, Hayabusa 2, brought back a sample from asteroid Ryugu in 2020.

Now JAXA has the Martian moon Phobos in its sights and will send a spacecraft to sample it as soon as 2024. The mission is called Martian Moons eXploration (MMX), and it’ll use a pneumatic vacuum device to collect its samples.

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