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NASA’s Perseverance Rover Is Carrying First Spacesuit Materials to Mars – Here’s Why – SciTechDaily

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Advanced spacesuit designer Amy Ross of NASA’s Johnson Space Center stands with the Z-2, a prototype spacesuit. Credit: NASA

In a Q&A, spacesuit designer Amy Ross explains how five samples, including a piece of helmet visor, will be tested aboard the rover, which was launched on July 30.

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NASA is preparing to send the first woman and next man to the Moon, part of a larger strategy to send the first astronauts to the surface of Mars. But before they get there, they’ll be faced with a critical question: What should they wear on Mars, where the thin atmosphere allows more radiation from the Sun and cosmic rays to reach the ground?

Amy Ross is looking for answers. An advanced spacesuit designer at NASA’s Johnson Space Center in Houston, she’s developing new suits for the Moon and Mars. So Ross is eagerly awaiting this summer’s launch of the Perseverance Mars rover, which will carry the first samples of spacesuit material ever sent to the Red Planet.

While the rover explores Jezero Crater, collecting rock and soil samples for future return to Earth, five small pieces of spacesuit material will be studied by an instrument aboard Perseverance called SHERLOC (Scanning Habitable Environments with Raman & Luminescence for Organics & Chemicals). The materials, including a piece of helmet visor, are embedded alongside a fragment of a Martian meteorite in SHERLOC’s calibration target. That’s what scientists use to make sure an instrument’s settings are correct, comparing readings on Mars to base-level readings they got on Earth.

Read on as Ross shares insights into the materials chosen and the differences between suits designed for the Moon and those for Mars. More information about SHERLOC and the rover’s science can be found here.

Prototype Astronaut Suit Calibration Target

This graphic shows an illustration of a prototype astronaut suit, left, along with suit samples included in the calibration target, lower right, belonging to the SHERLOC instrument aboard the Perseverance rover. They’ll be observed to see how they hold up in the intense radiation of the Martian surface. Credit: NASA

Why were these particular materials on SHERLOC’s calibration target selected?

Ross: The materials we’re poking at the most are meant to be on the outer layer of a suit, since these will be exposed to the most radiation. There’s ortho-fabric, something we have a lot of experience using on the outside of spacesuits. That’s three materials in one: It includes Nomex, a flame-resistant material found in firefighter outfits; Gore-Tex, which is waterproof but breathable; and Kevlar, which has been used in bulletproof vests.

We are also testing a sample of Vectran on its own, which we currently use for the palms of spacesuit gloves. It’s cut-resistant, which is useful on the International Space Station: Micrometeoroids strike handrails outside the station, creating pits with sharp edges that can cut gloves.

We included a sample of Teflon, which we’ve used in spacesuits for a long time as part of astronaut glove gauntlets and the backs of gloves. Just like a nonstick pan, it’s slippery, and it’s harder to catch and tear a fabric if it’s slick. We also included a sample of Teflon with a dust-resistant coating.

Finally, there’s a piece of polycarbonate, which we use for helmet bubbles and visors because it helps reduce ultraviolet light. A nice thing about it is it doesn’t shatter. If impacted, it bends rather than breaks and still has good optical properties.

How will SHERLOC check the samples?

Ross: On Mars, radiation will break down the chemical composition of the materials, weakening their tensile strength. We want to figure out how long these materials will last. Do we need to develop new materials, or will these hang in there?

SHERLOC can get the spectra, or composition, of rocks the mission’s scientists want to study. It can do the same thing for these spacesuit materials. We’ve already tested them on Earth, bathing samples in radiation and then analyzing their spectra. The results of those tests, conducted in ultraviolet vacuum chambers at NASA’s Marshall Space Flight Center, will be compared to what we see on Mars.

Will Martian dust be a challenge?

Ross: Sure, it’s an engineering challenge, but there’s no reason we can’t design things to operate in dust. We’re already developing things like seals that keep dust out of our bearings. Spacesuits have bearings at the shoulders, wrists, hip, upper thighs, and ankles. They all give an astronaut mobility for walking, kneeling, and other movements you’d need to get up close to rocks or maintain a habitat.

Remember, our suits inflate to over 4 pounds per square inch of pressure. That’s not a crazy amount of pressure, but it’s pretty stiff. When you put a human inside a balloon and ask them to move, they’ll have trouble. It’s as tight as the head of a drum. So we need to seal off the bearings so dust doesn’t gunk them up.

We are looking for other ways to protect the suit from Martian dust over a long-duration mission. We know that a coated or film material will be better than a woven material that has space between the woven yarns. The two Teflon samples let us look at that as well as the performance of the dust-resistant coating.

How much would spacesuit design differ between the space station, the Moon, and Mars?

Ross: Spacesuit design depends on where you’re going and what you’re doing. The ISS suit is designed specifically for microgravity. If you go on a spacewalk, you’re not really walking; you use your hands everywhere. Your lower torso is just used as a stable platform for your upper body. The suit is also exposed to two environmental sources of degradation: solar radiation and atomic oxygen. Atomic oxygen is different from the oxygen we breathe. It’s very reactive and can degrade spacesuit materials.

The Moon doesn’t have the atomic oxygen problem but is worse than Mars in terms of radiation. You’re pretty close to the Sun and have no atmosphere to scatter the ultraviolet radiation like you do on Mars. The Moon is a big testbed for the Artemis program. The environments of the Moon and Mars aren’t exactly the same, but the durability challenges — materials exposed over long periods of time at low pressures in a dusty environment — are similar.

On Mars, you’re farther from the Sun, and you have at least a little atmosphere to scatter the UV. But that’s when the duration of exposure starts to get you. You have to plan on being exposed on the surface most of the time. Mars spacesuits will be more like ones we use for the Moon and less like those for the ISS. I’m trying to make the Moon suit as much like the Mars suit as possible.

More About the Mission

Perseverance is a robotic scientist that weighs just under 2,300 pounds (1,043 kilograms). The rover’s astrobiology mission will search for signs of past microbial life. It will characterize the planet’s climate and geology, collect samples for future return to Earth, and pave the way for human exploration of the Red Planet. Perseverance launched on July 30, 2020 and will land at Mars’ Jezero Crater on February 18, 2021.

A division of Caltech, NASA’s Jet Propulsion Laboratory manages the Mars 2020 Perseverance rover mission for the agency’s Science Mission Directorate. The mission is part of a larger program that includes missions to the Moon as a way to prepare for human exploration of the Red Planet. Charged with returning astronauts to the Moon by 2024, NASA will establish a sustained human presence on and around the Moon by 2028 through NASA’s Artemis lunar exploration plans.

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Marine plankton could act as alert in mass extinction event: UVic researcher – Saanich News

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A University of Victoria micropaleontologist found that marine plankton may act as an early alert system before a mass extinction occurs.

With help from collaborators at the University of Bristol and Harvard, Andy Fraass’ newest paper in the Nature journal shows that after an analysis of fossil records showed that plankton community structures change before a mass extinction event.

“One of the major findings of the paper was how communities respond to climate events in the past depends on the previous climate,” Fraass said in a news release. “That means that we need to spend a lot more effort understanding recent communities, prior to industrialization. We need to work out what community structure looked like before human-caused climate change, and what has happened since, to do a better job at predicting what will happen in the future.”

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According to the release, the fossil record is the most complete and extensive archive of biological changes available to science and by applying advanced computational analyses to the archive, researchers were able to detail the global community structure of the oceans dating back millions of years.

A key finding of the study was that during the “early eocene climatic optimum,” a geological era with sustained high global temperatures equivalent to today’s worst case global warming scenarios, marine plankton communities moved to higher latitudes and only the most specialized plankton remained near the equator, suggesting that the tropical temperatures prevented higher amounts of biodiversity.

“Considering that three billion people live in the tropics, the lack of biodiversity at higher temperatures is not great news,” paper co-leader Adam Woodhouse said in the release.

Next, the team plans to apply similar research methods to other marine plankton groups.

Read More: Global study, UVic researcher analyze how mammals responded during pandemic

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The largest marine reptile ever could match blue whales in size – Ars Technica

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Blue whales have been considered the largest creatures to ever live on Earth. With a maximum length of nearly 30 meters and weighing nearly 200 tons, they are the all-time undisputed heavyweight champions of the animal kingdom.

Now, digging on a beach in Somerset, UK, a team of British paleontologists found the remains of an ichthyosaur, a marine reptile that could give the whales some competition. “It is quite remarkable to think that gigantic, blue-whale-sized ichthyosaurs were swimming in the oceans around what was the UK during the Triassic Period,” said Dean Lomax, a paleontologist at the University of Manchester who led the study.

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Giant jawbones

Ichthyosaurs were found in the seas through much of the Mesozoic era, appearing as early as 250 million years ago. They had four limbs that looked like paddles, vertical tail fins that extended downward in most species, and generally looked like large, reptilian dolphins with elongated narrow jaws lined with teeth. And some of them were really huge. The largest ichthyosaur skeleton so far was found in British Columbia, Canada, measured 21 meters, and belonged to a particularly massive ichthyosaur called Shonisaurus sikanniensis. But it seems they could get even larger than that.

What Lomax’s team found in Somerset was a surangular, a long, curved bone that all reptiles have at the top of the lower jaw, behind the teeth. The bone measured 2.3 meters—compared to the surangular found in the Shonisaurus sikanniensis skeleton, it was 25 percent larger. Using simple scaling and assuming the same body proportions, Lomax’s team estimated the size of this newly found ichthyosaur at somewhere between 22 and 26 meters, which would make it the largest marine reptile ever. But there was one more thing.

Examining the surangular, the team did not find signs of the external fundamental system (EFS), which is a band of tissue present in the outermost cortex of the bone. Its formation marks a slowdown in bone growth, indicating skeletal maturity. In other words, the giant ichthyosaur was most likely young and still growing when it died.

Correcting the past

In 1846, five large bones were found at the Aust Cliff near Bristol in southwestern England. Dug out from the upper Triassic rock formation, they were dubbed “dinosaurian limb bone shafts” and were exhibited in the Bristol Museum, where one of them was destroyed by bombing during World War II.

But in 2005, Peter M. Galton, a British paleontologist then working at the University of Bridgeport, noticed something strange in one of the remaining Aust Cliff bones. He described it as an “unusual foramen” and suggested it was a nutrient passage. Later studies generally kept attributing those bones to dinosaurs but pointed out things like an unusual microstructure that was difficult to explain.

According to Lomax, all this confusion was because the Aust Cliff bones did not belong to dinosaurs and were not parts of limbs. He pointed out that the nutrient foramen morphology, shape, and microstructure matched with the ichthyosaur’s bone found in Somerset. The difference was that the EFS—the mark of mature bones—was present on the Aust Cliff bones. If Lomax is correct and they really were parts of ichthyosaurs’ surangular, they belonged to a grown individual.

And using the same scaling technique applied to the Somerset surangular, Lomax estimated this grown individual to be over 30 meters long—slightly larger than the biggest confirmed blue whale.

Looming extinction

“Late Triassic ichthyosaurs likely reached the known biological limits of vertebrates in terms of size. So much about these giants is still shrouded by mystery, but one fossil at a time, we will be able to unravel their secrets,” said Marcello Perillo, a member of the Lomax team responsible for examining the internal structure of the bones.

This mystery beast didn’t last long, though. The surangular bone found in Somerset was buried just beneath a layer full of seismite and tsunamite rocks that indicate the onset of the end-Triassic mass extinction event, one of the five mass extinctions in Earth’s history. The Ichthyotian severnensis, as Lomax and his team named the species, probably managed to reach an unbelievable size but was wiped out soon after.

The end-Triassic mass extinction was not the end of all ichthyosaurs, though. They survived but never reached similar sizes again. They faced competition from plesiosaurs and sharks that were more agile and swam much faster, and they likely competed for the same habitats and food sources. The last known ichthyosaurs went extinct roughly 90 million years ago.

PLOS ONE, 2024.  DOI: 10.1371/journal.pone.0300289

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Jeremy Hansen – The Canadian Encyclopedia

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Early Life and Education

Jeremy Hansen grew up on a farm near the community of Ailsa Craig, Ontario, where he attended elementary school. His family moved to Ingersoll,
Ontario, where he attended Ingersoll District Collegiate Institute. At age 12 he joined the 614 Royal Canadian Air Cadet Squadron in London, Ontario. At 16 he earned his Air Cadet
glider pilot wings and at 17 he earned his private pilot licence and wings. After graduating from high school and Air Cadets, Hansen was accepted for officer training in the Canadian Armed Forces (CAF). He was trained at Chilliwack, British Columbia, and the Royal Military College at Saint-Jean-sur-Richelieu,
Quebec. Hansen then enrolled in the Royal Military College of Canada in Kingston,
Ontario. In 1999, he completed a Bachelor of Science in space science with First Class Honours and was a Top Air Force Graduate from the Royal Military College. In 2000, he completed his Master of Science in physics with a focus on wide field of view satellite tracking.   

CAF Pilot

In 2003, Jeremy Hansen completed training as a CF-18 fighter pilot with the 410 Tactical Fighter Operational Training Squadron at Cold Lake, Alberta.
From 2004 to 2009, he served by flying CF-18s with the 441 Tactical Fighter Squadron and the 409 Tactical Fighter Squadron. He also flew as Combat Operations Officer at 4 Wing Cold Lake. Hansen’s responsibilities included NORAD operations effectiveness,
Arctic flying operations and deployed exercises. He was promoted to the rank of colonel in 2017. (See also Royal Canadian Air Force.)

Career as an Astronaut

In May 2009, Jeremy Hansen and David Saint-Jacques were chosen out of 5,351 applicants in the Canadian Space Agency’s
(CSA) third Canadian Astronaut Recruitment Campaign. He graduated from Astronaut Candidate Training in 2011 and began working at the Mission Control Center in Houston, Texas, as capsule communicator (capcom, the person in Mission Control who speaks directly
to the astronauts in space.

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David Saint-Jacques (left) and Jeremy Hansen (right) during a robotics familiarization session, 25 July 2009.

As a CSA astronaut, Hansen continues to develop his skills. In 2013, he underwent training in the High Arctic and learned how to conduct geological fieldwork (see Arctic Archipelago;
Geology). That same year, he participated in the European Space Agency’s CAVES program in Sardinia, Italy. In that human performance experiment Hansen lived underground for six days.
In 2014, Hansen was a member of the crew of NASA Extreme Environment Mission Operations (NEEMO) 19. He spent seven days off Key Largo, Florida, living in the Aquarius habitat on the ocean floor, which is used to simulate conditions of the International
Space Station and different gravity fields. In 2017, Hansen became the first Canadian to lead a NASA astronaut class, in which he trained astronaut candidates from Canada and the United States.  

Did you know?

Hansen has been instrumental in encouraging young people to become part of the STEM (Science, Technology,
Engineering, Mathematics) workforce with the aim of encouraging future generations of space explorers.
His inspirational work in Canada includes flying a historical “Hawk One” F-86 Sabre jet.

Artemis II

In April 2023, Hansen was chosen along with Americans Christina Koch, Victor Glover and Reid Wiseman to crew NASA’s Artemis II mission to the moon. The mission, scheduled for no earlier
than September 2025 after a delay due to technical problems, marks NASA’s first manned moon voyage since Apollo 17 in 1972. The Artemis II astronauts will not land on the lunar
surface, but will orbit the moon in an Orion spacecraft. They will conduct tests in preparation for future manned moon landings, the establishment of an orbiting space station called Lunar Gateway, or Gateway, and a base on the moon’s surface where astronauts
can live and work for extended periods. The path taken by Orion will carry the astronauts farther from Earth than any humans have previously travelled. Hansen’s participation in Artemis II is a direct result of Canada’s contribution of Canadarm3
to Lunar Gateway. (See also Canadarm; Canadian Space Agency.)

“Being part of the Artemis II crew is both exciting and humbling. I’m excited to leverage my experience, training and knowledge to take on this challenging mission on behalf of Canada. I’m humbled by the incredible contributions and hard work of so many
Canadians that have made this opportunity a reality. I am proud and honoured to represent my country on this historic mission.” – Jeremy Hansen (Canadian Space Agency, 2023)

Did you know?

On his Artemis II trip, Hansen will wear an Indigenous-designed mission patch created for him by Anishinaabe artist Henry Guimond.

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Honours and Awards

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