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Brock scientist and student contribute to new Mars research – St. Catharines Standard

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For a few Brock University students taught by professor Mariek Schmidt, an opportunity to assist in her research has literally sent them “over the moon.”

Schmidt, a geologist who studies igneous and volcanic rocks on both Earth and Mars, is one of a team of world-renowned scientists collaborating on the Perseverance rover mission underway on Mars, searching the Jezero crater for signs of ancient life on the desolate world.

Thursday, about 18 months after the rover touched down on Mars, Schmidt’s team led by Yang Liu at NASA’s Jet Propulsion Laboratory published its first research paper on the science.org website, analysing a massive rock formation on the planet’s surface.

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Schmidt said Brock post-doctoral fellow Tanya Kizovski assisted with the research for that paper, while two other master’s students will be working with her on future research she’s conducting.

“They love it. They’re really enthusiastic about it,” she said.

Schmidt, an earth sciences professor at the university, said one of her students accompanied her on a visit to the Jet Propulsion Lab in California last week, “and he was over the moon.”

“He was just taking pictures of everything,” she said, adding the visit also gave them a look at future projects under development such as the Europa Clipper — a spacecraft being built to search for life under the ice of one of Jupiter’s frozen moons.

“He got to meet a lot of people. For students, they think of these people as sort of heroes, but for me they’re just my colleagues,” she said, laughing.

Schmidt’s research focused on the rover’s Planetary Instrument for X-Ray Lithochemistry (PIXL), which uses an X-ray fluorescence spectrometer to determine the composition of Martian regolith.

The research paper focused on the origins of a 70,000 square kilometre rock formation that contains high abundances of olivine, a mineral considered essential in the development of life. Schmidt said microbes on Earth have been known to eat olivine, which contains oxygen and iron.

“It’s huge. Its this wide-spread area,” she said, adding the formation extends from the planet’s norther lowlands through to the Jezero crater, located north of the Martian equator.

“This large olivine-bearing unit is something we’ve been able to identify from orbit and there has been a lot of studies that have been speculating about its origin,” she said, adding some of those studies suggested it could be associated with a meteor impact.

Schmidt said the new study, however, showed the formation is the result of slowly cooling magma, from volcanism or an impact.

“This study shows it’s an igneous rock — at least in the Jezero crater — that crystallized from magma and that’s really cool that we’re able to say what the origin is in this particular area.”

While the search for ancient life is a priority for the Perseverance rover, Schmidt said there are other goals associated with the mission such as learning more about the planet’s history.

But to determine when rock formations were formed, she said they will need to be returned to Earth.

“We can use radiometric isotopes to determine when that rock crystallized or formed. But we don’t have that ability with rovers right now or with landers to be able to find out how old a rock is,” Schmidt said.

Although previous Mars missions have estimated the age of rocks, she said those measurements are based on “a whole lot of assumptions” and there are “huge errors on those measurements.”

“If we can bring back a rock and can precisely date it, it’s going to be really important for understanding the history of the planet,” she said.

The rover is collecting core samples of Martian rocks — including samples taken from the olivine-rich rock formation — that will be collected and returned to Earth during a future mission, likely by 2034.

Schmidt said the latest research paper is one of several she has been working on that are being published in the near future.

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Marine plankton could act as alert in mass extinction event: UVic researcher – Langley Advance Times

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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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Scientists Say They Have Found New Evidence Of An Unknown Planet… – 2oceansvibe News

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In the new work, scientists looked at a set of trans-Neptunian objects, or TNOs, which is the technical term for those objects that sit out at the edge of the solar system, beyond Neptune

The new work looked at those objects that have their movement made unstable because they interact with the orbit of Neptune. That instability meant they were harder to understand, so typically astronomers looking at a possible Planet Nine have avoided using them in their analysis.

Researchers instead looked towards those objects and tried to understand their movements. And, Dr Bogytin claimed, the best explanation is that they result from another, undiscovered planet.

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The team carried out a host of simulations to understand how those objects’ orbits were affected by a variety of things, including the giant planets around them such as Neptune, the “Galactic tide” that comes from the Milky Way, and passing stars.

The best explanation was from the model that included Planet 9, however, Dr Bogytin said. They noted that there were other explanations for the behaviour of those objects – including the suggestion that other planets once influenced their orbit, but have since been removed – but claim that the theory of Planet 9 remains the best explanation.

A better understanding of the existence or not of Planet 9 will come when the Vera C Rubin Observatory is turned on, the authors note. The observatory is currently being built in Chile, and when it is turned on it will be able to scan the sky to understand the behaviour of those distant objects.

Planet Nine is theorised to have a mass about 10 times that of Earth and orbit about 20 times farther from the Sun on average than Neptune. It may take between 10,000 and 20,000 Earth years to make one full orbit around the Sun.

You may be tempted to ask how an entire planet could ‘hide’ in our solar system when we have zooming capabilities such as the new iPhone 15 has, but consider this: If Earth was the size of a marble, the edge of our solar system would be 11 kilometres away. That’s a lot of space to hide a planet.

[source:independent]

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Dragonfly: NASA Just Confirmed The Most Exciting Space Mission Of Your Lifetime – Forbes

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NASA has confirmed that its exciting Dragonfly mission, which will fly a drone-like craft around Saturn’s largest moon, Titan, will cost $3.35 billion and launch in July 2028.

Titan is the only other world in the solar system other than Earth that has weather and liquid on the surface. It has an atmosphere, rain, lakes, oceans, shorelines, valleys, mountain ridges, mesas and dunes—and possibly the building blocks of life itself. It’s been described as both a utopia and as deranged because of its weird chemistry.

Set to reach Titan in 2034, the Dragonfly mission will last for two years once its lander arrives on the surface. During the mission, a rotorcraft will fly to a new location every Titan day (16 Earth days) to take samples of the giant moon’s prebiotic chemistry. Here’s what else it will do:

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  • Search for chemical biosignatures, past or present, from water-based life to that which might use liquid hydrocarbons.
  • Investigate the moon’s active methane cycle.
  • Explore the prebiotic chemistry in the atmosphere and on the surface.

Spectacular Mission

“Dragonfly is a spectacular science mission with broad community interest, and we are excited to take the next steps on this mission,” said Nicky Fox, associate administrator of the Science Mission Directorate at NASA Headquarters in Washington. “Exploring Titan will push the boundaries of what we can do with rotorcraft outside of Earth.”

It comes in the wake of the Mars Helicopter, nicknamed Ingenuity, which flew 72 times between April 2021 and its final flight in January 2023 despite only being expected to make up to five experimental test flights over 30 days. It just made its final downlink of data this week.

Dense Atmosphere

However, Titan is a completely different environment to Mars. Titan has a dense atmosphere on Titan, which will make buoyancy simple. Gravity on Titan is just 14% of the Earth’s. It sees just 1% of the sunlight received by Earth.

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The atmosphere is 98% nitrogen and 2% methane. Its seas and lakes are not water but liquid ethane and methane. The latter is gas in Titan’s atmosphere, but on its surface, it exists as a liquid in rain, snow, lakes, and ice on its surface.

COVID-Affected

Dragonfly was a victim of the pandemic. Slated to cost $1 billion when it was selected in 2019, it was meant to launch in 2026 and arrive in 2034 after an eight-year cruise phase. However, after delays due to COVID, NASA decided to compensate for the inevitable delayed launch by funding a heavy-lift launch vehicle to massively shorten the mission’s cruise phase.

The end result is that Dragonfly will take off two years later but arrive on schedule.

Previous Visit

Dragonfly won’t be the first time a robotic probe has visited Titan. As part of NASA’s landmark Cassini mission to Saturn between 2004 and 2017, a small probe called Huygens was despatched into Titan’s clouds on January 14, 2005. The resulting timelapse movie of its 2.5 hours descent—which heralded humanity’s first-ever (and only) views of Titan’s surface—is a must-see for space fans. It landed in an area of rounded blocks of ice, but on the way down, it saw ancient dry shorelines reminiscent of Earth as well as rivers of methane.

The announcement by NASA makes July 2028 a month worth circling for space fans, with a long-duration total solar eclipse set for July 22, 2028, in Australia and New Zealand.

Wishing you clear skies and wide eyes.

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