Initial Tests Show Green Sand Carbon Dioxide Removal Poses No Threat to Marine Life

Beach in Southampton, New York Treated with Olivine Sand

Cheyenne Morrow

Initial studies of adding crushed olivine to ocean waters for atmospheric carbon dioxide absorption showed no adverse effects on the seafloor ecosystem during the first year.

While the New York State trial offers promising findings for this innovative carbon removal technology, researchers advise caution, as it may not encapsulate all potential negative impacts.

Emilia Jankowska from Hourglass Climate, the nonprofit organization conducting the study, stated that while the addition of olivine to the ocean should be regulated, “there are methods to minimize effects while maintaining effectiveness.”

The UN climate change agency highlights the necessity for carbon removal strategies, including reforestation and advanced carbon filtration methods, to achieve net-zero greenhouse gas emissions. With rising emissions, the aspiration to limit global warming to 1.5 degrees Celsius remains a challenge.

Olivine, a magnesium iron silicate mineral, is often found within the Earth’s mantle and reacts with CO2 when reaching the surface, forming stable compounds that can sequester carbon in the ocean for millennia.

A recent study indicated that spreading crushed olivine and similar silicates on crops could enhance this process, potentially removing up to 1.1 billion tons of CO2 annually. U.S. startup Vesta aims to introduce olivine directly into ocean waters, facilitating increased carbon absorption through bicarbonate formation.

However, olivine may contain trace amounts of heavy metals. Research has detected elevated nickel and chromium levels in crustaceans and mollusks exposed to olivine. There are concerns about sand potentially suffocating benthic organisms, such as crustaceans and worms.

In 2022, Vesta distributed 650 tons of olivine sand along Long Island’s coast, overlaying it with 13,500 tons of regular sand for shore reinforcement. However, as storms intensified, tides washed away much of the olivine.

Researchers collected sediment samples from shallow waters up to 160 meters offshore before and after adding olivine, and a year later. They compared these to samples from areas where only regular sand or no sand was added.

Among numerous species, only a minor decline was observed in the fringe bloodworm within the olivine-treated area, with overall benthic species’ abundance and diversity rebounding within two months. Species composition shifted similarly in regions where only regular sand was used, indicating common beach aquaculture practices.

Crucially, nickel, chromium, cobalt, and manganese concentrations in organisms remained low. “Natural systems are highly dynamic, causing dissolved elements to dilute rapidly,” Jankowska remarked.

While Vesta oversaw environmental monitoring for these trials, the analyses conducted by Hourglass were independently funded by the Grantham Foundation.

Olivine’s dissolution in ocean waters may lead to calcium carbonate precipitating from seawater, potentially trapping trace metals, as noted by Christopher Pierce at the UK National Marine Centre. Nevertheless, this might limit the additional CO2 absorption capacity of seawater.

This significant research transitions understanding from laboratory settings to real-world applications. Further investigation remains essential to comprehend varying biological responses and infection rates associated with CO2 ingestion.

Nonetheless, the study’s assertion of no negative effects may overstate the findings, according to James Kelly of Ocean Care. He notes that fluctuations in olivine concentrations could imply limited exposure, questioning the notion that olivine is inherently safe.

Hourglass Climate is currently tracking the results from a large-scale trial with Vesta. In 2024, 8,200 tons of olivine were identified 450 meters offshore from Duck, North Carolina. Preliminary insights suggest recovery in species richness and diversity, although metal accumulation analysis is ongoing.

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Source: www.newscientist.com

Ancient Human Footprints in White Sand Estimated to Be Up to 22,400 Years Old: New Research

The identification of human footprints in White Sands, New Mexico, estimated to be between 21,000 and 23,000 years old, was a significant advancement in our comprehension of the earliest inhabitants of the Americas. However, this research faced scrutiny concerning the dependability of radiocarbon dating materials, such as common aquatic plant seeds Rupiah Silhosa and coniferous pollen grains. A recent study, spearheaded by University of Arizona researcher Vance Holiday, indicates that the ancient mud from Perelora ceotero, the third material utilized for dating the footprints, dates back to approximately 20,700 to 22,400 years ago.

Ancient human footprints found in White Sands National Park, New Mexico, USA. Image credit: Bennett et al. , doi: 10.1126/science.abg7586.

Historically, scientists believed that humans entered North America roughly 16,000 to 13,000 years ago.

However, the footprints found at White Sands indicate that human presence in the area dates back to between 23,000 and 21,000 years ago. This timeline offers insights into the development of culture in North America.

The remnants of 10,000-year-old prints, uncovered nearly a century ago at a site near Clovis, New Mexico, led to a classification of artifacts long considered to represent the earliest known cultures in North America.

Critics have challenged two prior studies over the last four years, asserting that ancient species and pollen in the soil used for dating the footprints are unreliable indicators.

“The record is consistently strong, and it’s challenging to explain it all,” Dr. Holiday stated.

“As I mention in my publication, it would be an extraordinary coincidence for all these dates to be inaccurate.”

Thousands of years prior, the white sands formed from a series of lakes that eventually dried up.

Wind erosion created layers of plaster on the sand dunes that now characterize the region.

The footprints were excavated from stream beds that once fed into this ancient lake.

“Wind erosion has erased part of the narrative, leaving that segment lost. The remainder is buried beneath the world’s largest accumulation of plaster sand,” Dr. Holiday remarked.

For their latest research, Dr. Holiday and his team returned to White Sands in 2022 and 2023, excavating new trenches to gain deeper insights into the lakebed’s geology.

“We’ve put in considerable effort to explore this area,” stated Jason Windingstad, a doctoral candidate at the University of Arizona.

“You essentially find yourself questioning everything taught about North American populations.”

The authors recognize that their research hasn’t addressed lingering questions posed by critics since 2021: Why are there no artifacts or settlements left by the individuals who made the footprints?

“This is a valid inquiry. Some footprints discovered during the 2021 survey belong to a trackway that was created in mere seconds,” they explained.

“It is entirely plausible that hunter-gatherers would act with caution to avoid leaving resources in such a brief timeframe.”

“These individuals were aware of their resources and were distanced from their replacements.”

“They wouldn’t abandon artifacts casually. It doesn’t make sense for you to be viewing a debris field.”

The team’s recent findings will be published in the journal Advances in Science.

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Vance T. Holliday et al. 2025. Perelorace Geochronology supports the last Glacier Max (LGM) age of human tracks in White Sands, New Mexico. Advances in Science 11 (25); doi:10.1126/sciadv.adv4951

Source: www.sci.news

Transforming Mars into a world of sand dunes: A step-by-step guide

Dune is the nickname for the planet Arrakis, a harsh desert world in the Canopus system where much of the story unfolds. The primary residents are the resilient Fremen people and their native species, the Shai Huld, enormous sandworms that can live for thousands of years and grow over two kilometers long.

The Shai Huld’s main diet consists of sand, with tiny organisms called sand plankton as a supplement. Their digestion of this bland food releases oxygen, which makes the planet’s atmosphere breathable for humans. This process is similar to Earth’s photosynthesis, where plants and bacteria produce oxygen through sunlight, water, and carbon dioxide.

Professor Gary King of Louisiana State University is studying the use of photosynthetic bacteria to introduce oxygen into Mars’ atmosphere, a concept known as terraforming. By creating greenhouse gases to warm the planet and melt ice into a liquid form, automated factories could potentially make Mars habitable for humans.

Korolev Crater is one of the best preserved examples of craters on Mars. Korolev is filled with ice all year round © ESA/DLR/FU Berlin

Without a protective magnetic field like Earth’s, Mars lost its original atmosphere due to high-energy radiation from the sun. Establishing a biosphere on Mars could lead to oxygen production, replenishing what is lost due to radiation exposure.

Can we live without water?

Arrakis, despite being a harsh desert, is home to the Fremen people who rely on innovative technologies like the Stillsuit to recycle all the water they excrete. These suits filter sweat, urine, and feces to recover water for the wearer to drink, powered by the user’s movements.

In Dune, humans wear stillsuits that filter and purify the water their bodies produce so they can drink it © Warner Brothers

Similar water recycling systems are used on the International Space Station to reuse up to 93% of water on board. Mars, with limited liquid water, may adopt similar technologies to sustain human life on the planet.

Research shows promise in extracting water from the atmosphere using moisture-absorbing technology, offering solutions for clean water production in arid regions.

Source: www.sciencefocus.com

Sand dunes and ice formations found in Mars’s north pole by Mars Express

new images from high resolution stereo camera (HRSC) On ESA's Mars Express spacecraft It shows the terrain surrounding Mars's permanent ice cap at its north pole.



This image from ESA's Mars Express shows an area close to Mars' north pole. This image consists of data collected by Mars Express' High Resolution Stereo Camera (HRSC) on April 14, 2023. Image credit: ESA / DLR / FU Berlin.

Mars' permanent north polar ice cap is a stack of water ice and dust layers up to 3 km thick and approximately 1,000 km in diameter.

These are divided into four stacked “packets” of different thicknesses, which are further composed of finer layers.

These layers contain information about the climate going back millions of years in Mars' history.

The deposits were formed by precipitation of dust and water ice in the atmosphere and by direct frost formation.

These consist primarily of water ice, with fine dust deposits accounting for 10-15% of the total.

These likely reflect changes in Mars' orbit and the tilt of Mars' axis of rotation, which is much more unstable than Earth's orientation.

It changes in several cycles with periods ranging from thousands of years to millions of years.

Changes in solar radiation cause significant changes in climate, especially in the polar regions. The Arctic ice sheet is currently thought to be growing.

“The landforms surrounding Mars' north pole, known as pranum boriumfascinating,” said a member of the Mars Express team.

“The poles themselves are covered with a layer of fine dust and water ice. These stack up several kilometers thick and extend for about 1,000 kilometers.”

“Most of this material is not visible here, but you can see the beginning of the planum boreum on the right side of the frame. There are some subtle wrinkles that indicate where layers of material are starting to accumulate.”

“The ground has also become more distinctly stepped, as most clearly seen in the topographical map of the area below.”

“The lowest elevation areas are blue/green, and the highest elevation areas are red/white/brown.”

“These layers formed as a mixture of dust, water ice, and frost that accumulated on the Martian ground over a long period of time.”

“Each layer contains valuable information about Mars' history, telling us how the planet's climate has changed over the past millions of years.”

“During the Martian winter, a thin cap of carbon dioxide ice several meters thick rests on top of that layer. This cap completely disappears into the atmosphere each year during the Martian summer.”

The left side of the image is dominated by a vast strip of undulating sand dunes, extending over 150 km within this frame alone.

This wrinkled, turbulent appearance is very different from the smoother, more primitive terrain seen on the right.

This smooth area shows no obvious signs of erosion and has been spared from being hit by rocks from space. This indicates that the surface is very young and is probably getting younger every year.

“Between these two extremes are two semicircular cliffs, the larger of which is approximately 20 km wide,” the researchers said.

“Within the curves of these cliffs are frost-covered dunes.”

“The sheer scale of the cliffs is evident from the dark shadow they cast on the ground below. Sheer walls of ice can reach up to a kilometer in height.”

“These two cliffs are located in what's called a polar trough, a landform formed when wind pushes and wears down the earth's surface.”

“These appear as wavy ridges in the landscape and are common in this region, creating the characteristic spiral pattern of the polar plateau.”

Source: www.sci.news