Eco-Friendly Upcycling: Transforming Polystyrene with Sunlight and Sulfur – Sciworthy


Annually, over 20 million tons of polystyrene plastic is manufactured, yet only a fraction undergoes recycling globally. Traditional recycling processes demand substantial energy and often employ harsh, toxic chemicals to break down the robust molecular chains of polystyrene. An innovative solution lies in harnessing sulfur, a cost-effective byproduct from crude oil refining. Sulfur’s unique chemical properties enable it to cleave the strong bonds within long plastic molecules. Despite its plentiful availability, sulfur is underutilized, and converting it into a more practical form typically requires excessive heat, limiting its usability over time.


Researchers at the Dalian Institute of Chemical Physics proposed that sulfur could aid in breaking down polystyrene waste to generate more valuable chemicals. They harnessed sunlight through a process known as light heat conversion to facilitate this reaction. The team successfully used this thermal energy to transform polystyrene and sulfur into useful compounds such as 2,4-diphenylthiophene, also referred to as Chemical D, and 1,3,5-triphenylbenzene, or Chemical T, which are essential in the production of semiconductors and chemical sensors.


To verify their hypothesis, the research team combined ground polystyrene and sulfur in a 1:0.5 molar ratio within a sealed glass tube. They attached a balloon to the tube and secured it on a steel stand. Sunlight was focused onto the tube’s base using a curved mirror. Upon heating, the yellow-white solid melted and transitioned to a red-black liquid after just 2 minutes. Following heating, the mirror was removed, allowing the system to cool before collecting gaseous products from the balloon and dissolving the remaining solids for further analysis and purification.


The researchers fine-tuned the reaction conditions to identify factors affecting the results. They examined the reaction without sulfur, varying the sulfur ratio from 0.2 to 0.8 and substituted elemental sulfur with alternative sulfur-containing compounds. Additionally, they explored incorporating known photothermal agents, particularly metal oxide additives, into their mixture.


To draw comparisons between sunlight and artificial light, the team replicated the experiment indoors using 100-watt LED bulbs while monitoring temperature changes with a thermal camera. A control experiment with only polystyrene was conducted to observe sulfur’s impact on yield under LED light. The team varied exposure times in increments of 1 minute, ranging from 1 to 6 minutes, to determine optimal conditions for yield under LED light. These assessments were crucial in understanding the necessary conditions for the reaction and how various elements influenced outcomes.


The results indicated that, without sulfur or alternative sulfur compounds, the reaction failed to produce Chemicals D or T under sunlight. Conversely, when sulfur was included, the reaction yielded a maximum of 34% D and 16% T at a sulfur ratio of 0.5. The introduction of metal oxides diminished chemical yields to 22% and 12%, respectively, suggesting these additives hindered the desired reaction. Notably, switching from sunlight to LED reduced the reaction yield to 26% for D and 13% for T.


The investigation also revealed the impact of reaction time on product formation, with yields gradually increasing and peaking at 4 minutes before stabilizing. The sulfur-containing mixture heated from room temperature to 320°C (608°F), while the control exhibited minimal temperature change. These findings confirmed sulfur’s dual role as both a reactant and a photothermal converter, facilitating the transformation of polystyrene into valuable chemicals.


Taking their research further, the scientists tested their method using real-world polystyrene waste, including food packaging and plastic foam. They successfully synthesized Chemicals D and T from these materials, demonstrating the practicality of their approach beyond laboratory conditions.


The researchers concluded that their study presents a simple, rapid, and solvent-free methodology for converting two abundant waste products into valuable chemicals utilizing sunlight. By merging polystyrene waste with excess sulfur, they establish a sustainable polymer upcycling pathway that leverages clean energy, applicable to common plastics.


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Discovering a Mysterious Magma and Sulfur Planet Hidden in the Milky Way

Recent findings on L 98-59d, part of the five-planet system L 98-59, indicate that this intriguing exoplanet may host an extensive global magma ocean, effectively trapping sulfur deep within its interior. This discovery introduces a previously unidentified category of extraterrestrial worlds.

Artist’s impression of planetary system L 98-59. Image credit: Mark A. Garlick / markgarlick.com.

The distant L 98-59 system lies approximately 34.5 light-years away in the southern constellation Bootes.

Known as TOI-175 or TIC 307210830, this bright M dwarf star has a mass roughly one-third that of the Sun.

This intriguing planetary system features at least three transiting planets and two non-transiting planets: L 98-59b, L 98-59c, L 98-59d, L 98-59e, and L 98-59f.

L 98-59d completes an orbit around its parent star every 7.5 days and is about 1.6 times larger than Earth, receiving approximately four times the radiant energy of our planet.

A recent study led by astronomer Harrison Nichols from the University of Oxford aimed to reconstruct the planetary history of this super-Earth, tracing its evolution from its formation nearly 5 billion years ago.

By correlating telescope observations with comprehensive physical models of the planet’s interior and atmosphere, the research team gained insights into the planet’s deep geological processes.

The findings suggest that L 98-59d possesses a mantle of molten silicate similar to Earth’s lava, underpinned by a vast global magma ocean that extends for thousands of kilometers.

This massive molten reservoir enables L 98-59d to store significant amounts of sulfur within its interior over geological timescales.

Moreover, the magma ocean assists in retaining a hydrogen-rich atmosphere laden with sulfur compounds like hydrogen sulfide, which is typically lost to space due to X-ray radiation emitted by the host star.

Over billions of years, the interplay between its molten interior and atmosphere has sculpted L 98-59d into the striking world observed today.

Researchers propose that L 98-59d may represent the inaugural example of a newly identified category of gas-rich sulfur exoplanets that sustain long-lived magma oceans. If validated, this could greatly expand our understanding of planetary diversity in the galaxy.

“This discovery highlights that the current classifications of small planets may be overly simplistic,” remarked Dr. Nichols.

“While this molten world is unlikely to support life, it showcases the vast array of planets beyond our solar system. What other types of celestial bodies remain undiscovered?”

For more details, refer to the study published in today’s edition of Nature Astronomy.

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H. Nichols et al. Evolution of a volatile-rich molten super-Earth L 98-59d. Nat Astron, published online March 16, 2026. doi: 10.1038/s41550-026-02815-8

Source: www.sci.news

Apollo 17 Moon Samples Reveal Uncommon Sulfur, New Analysis Indicates

The prevailing theory regarding the origin of the Moon suggests it formed from a colossal impact event involving Earth and a body known as Theia. The degree to which materials from these two celestial objects mixed during this event is still debated. Poor mixing may leave traces of the original atomic and/or Theia composition. The sulfur isotopic makeup of the primordial materials that survived the impact can help establish parameters concerning the chemistry of the early solar nebula, the sulfur distribution in the early solar system, and the efficiency of mixing during this significant lunar impact event. In a recent study, researchers from Brown University and other institutions present intriguing sulfur isotope data derived from lunar rocks collected from the Taurus Littrow region during Apollo 17. Their analysis reveals that the volcanic material in the samples is significantly depleted in sulfur-33. This depletion sharply contrasts with sulfur isotope ratios found on Earth, suggesting the likelihood of:



Commander Eugene Cernan retrieves a drive tube from a lunar roving vehicle during Apollo 17 EVA. Image credit: NASA.

Some elements possess distinct “fingerprints” through specific isotopic ratios, revealing slight variations in atomic weights.

If two rocks share the same isotopic fingerprint, it strongly indicates a common origin.

In terms of the Moon and Earth, researchers have identified general similarities in the oxygen isotopes of both bodies.

Dr. James Dottin, a researcher from Brown University, stated:

“Previously, it was assumed that the Moon’s mantle shared the same sulfur isotope composition as Earth.”

“This was the anticipated outcome when we examined these samples, yet we observed values markedly different from those found on Earth.”

The sample under investigation was sourced from a double-drive tube—a hollow metal cylinder driven approximately 60 cm into the lunar soil by Apollo 17 astronauts Gene Cernan and Harrison Schmidt.

Upon returning to Earth, NASA secured the tube in a helium chamber to preserve the sample for future studies under the Apollo Next Generation Sample Analysis (ANGSA) program.

In recent years, NASA has begun to make ANGSA samples accessible to academic researchers via a competitive application process.

Dr. Dottin and his team chose secondary ion mass spectrometry for sulfur isotopic analysis. This precise analytical method did not exist in 1972 when the samples were initially returned to Earth.

For their research, they targeted specific samples from drive tubes believed to originate from mantle-derived volcanic rocks.

“There are two possible explanations for the anomalous sulfur,” Dr. Dottin explained.

They may represent remnants of chemical processes that took place during the Moon’s early history.

When sulfur interacts with ultraviolet light in a thin atmosphere, a diminished sulfur-33 ratio can be observed.

It is theorized that the Moon had a transient atmosphere in its early history, which could have facilitated such photochemical reactions.

If this is indeed the case, it would have interesting implications for the Moon’s evolutionary history.

“This offers evidence of ancient material transfer from the lunar surface into the mantle,” Dr. Dottin said.

“On Earth, we rely on plate tectonics for this process, but the Moon lacks such tectonic activity.”

“Thus, the idea of some form of exchange mechanism on the early Moon is thrilling.”

Alternatively, the unusual sulfur signatures could be remnants from the Moon’s formation itself.

The prevailing theory states that a Mars-sized object named Theia collided with Earth early on, with debris from that impact eventually forming the Moon.

The sulfur signatures from Theia differ significantly from those of Earth, and these differences may be reflected in the Moon’s mantle.

This study does not definitively resolve which explanation is accurate.

“Investigating sulfur isotopes from Mars and other celestial bodies may someday provide insights,” Dr. Dottin remarked.

“Ultimately, a better understanding of isotopic distributions will enhance our comprehension of solar system formation.”

study Published in Journal of Geophysics: Planets.

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JW Dottin III et al. 2025. Endogenous yet exotic sulfur in the lunar mantle. JGR: Planet 130(9):e2024je008834; doi:10.1029/2024je008834

Source: www.sci.news

Pure sulfur discovered on Mars by Curiosity

Yellow crystals Elemental Sulfur According to the Curiosity team, the discoveries were made when NASA's Curiosity rover accidentally drove over a rock on May 30, 2024, breaking it apart.

Yellow crystals of elemental sulfur on Mars. Image courtesy of NASA.

Although sulfur may remind you of the smell of rotten eggs, elemental sulfur is odorless.

It forms only under a narrow range of conditions that scientists have not linked to the history of the place.

Curiosity then discovered lots of bright chunks of rock that looked similar to the rock the rover had crushed.

“Finding a rock block made of pure sulfur is like finding an oasis in the desert,” said Dr. Ashwin Vasavada, Curiosity project scientist and a research scientist at NASA's Jet Propulsion Laboratory.

“It can't be there, so now we have to explain it. Discovering strange and unexpected things is what makes planetary exploration so exciting.”

It was one of several Curiosity discovered while driving off-road through a channel in Gediz Canyon, a 5-kilometer (3-mile) groove that runs gently down part of Mount Sharp, where Curiosity has been climbing the base of the mountain since 2014.

The channel was discovered from space years before the rover launched and is one of the main reasons the science team wanted to visit this part of Mars.

Researchers believe the channel was carved out by flows of liquid water and debris, leaving a ridge of rock and sediment stretching for 3.2 kilometers (2 miles) on the mountainside below the channel.

The goal is to better understand how this landscape changed billions of years ago, and while recent clues are helping, there is still much to learn from this dramatic formation.

Since Curiosity arrived in the strait earlier this year, scientists have been studying whether a large pile of rubble that rose from the bottom of the strait was formed by an ancient flood or landslide.

The latest clues from the spacecraft suggest that both played a role: some mountains appear to have been left by powerful flows of water and debris, while others appear to be the result of more localized landslides.

These conclusions are based on the rocks found in the debris middens: while stones carried by water are rounded like river stones, some of the debris middens are littered with more angular rocks that appear to have been deposited by dry avalanches.

Eventually, water seeped into all the material that had settled here.

Chemical reactions caused by water have caused white “halo” shapes to appear on some of the rocks.

Erosion by wind and sand has revealed the shapes of these halos over the years.

“This has not been a quiet period for Mars,” said Dr. Becky Williams, a scientist at the Planetary Science Institute in Tucson, Arizona, and deputy principal investigator for Curiosity's Mast Camera.

“There has been a lot of activity here. We're seeing multiple flows through the channel, including heavy flooding and rocky flows.”

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This article is a version of a press release provided by NASA.

Source: www.sci.news