Category Archives: Science

Grand Conjunction of 5 planets and the moon coming: best viewing tips

A great sky event is coming up, and Michiganders have a really good chance at seeing this event. One astronomer is calling it a “Grand Conjunction.”

A conjunction is when two planets come very close together when viewing them in the sky. In this upcoming case, it won’t just be two planets, it will be five planets and the moon. Astronomer Todd Slisher, executive director of Flint’s Longway Planetarium and the Sloan Museum, says while this isn’t a typical conjunction of planets touching in a view, it is still considered a conjunction. For those tracking this sky event on social media, it’s also earned the “planet parade” nickname.

For the next several weeks, Michiganders will be able to look east and southeast just before sunrise and see the planets all in a row. Mercury, Venus, Mars, Jupiter and Saturn will stretch across the eastern to southern sky, according to Slisher.

Slisher says to start looking about one hour before sunrise at your location. You can check your sunrise time at any location here. The best viewing of the five planet conjunction will occur on June 24, June 25 and June 26. Start looking across the sky from just north of east to almost due south. Slisher says this is the expanse of the sky where you will see all of the planets.

A bonus is the moon will also be in this line of planets. Waiting until June 24 to June 26 to look for the planets allows you to see Mercury. Mercury will only be visible just above the horizon for about 15 minutes. As we get closer to sunrise, Mercury will disappear in the sunlight. Slisher also advises that binoculars will help you see the tiny Mercury.

The five planets are visible all at once only every 18 years. But this year’s Grand Conjunction is even more special, and something we haven’t seen since the 1950s, states Slisher. This year’s conjunction will have all of the planets lined up as they are in ordered distance from the sun. Mercury is about 35 million miles from the sun, and Saturn is around one billion miles from the sun.

So we are looking a long ways away when we see these planets lined up.

Fortunately for Michigan, we are in our sunny time of year. Friday and Saturday should have clear early mornings. Right now, Sunday morning looks stormy. I would definitely try viewing the Grand Conjunction Friday early morning or Saturday early morning.

If you want to know more about the summer sky and the Grand Conjunction, you can attend the Skies Over Michigan Show at 3 p.m. Tuesday through Saturday at the Longway Planetarium in Flint.

You can also learn more by listening to Delta College astronomer Mike Murray’s podcast about the Grand Conjunction.

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NASA weighs Artemis 1 moon rocket’s launch readiness after fueling success

Monday (June 20) was a big day for NASA’s Artemis 1 mission.

The agency’s huge new moon rocket, the Space Launch System (SLS), wrapped up a more than 50-hour launch simulation known as a “wet dress rehearsal” on Monday evening (June 20). Following several failed attempts in April, mission team members were able to fully fuel SLS for the first time on Monday, wrapping up a series of crucial prelaunch tests.

It was a big milestone for the Artemis 1 moon mission, but there were some snags along the way.

Related: NASA’s Artemis 1 moon mission explained in photos 

Ground teams at NASA’s Kennedy Space Center (KSC) in Florida spent the weekend reviewing procedures and checklists for Artemis 1’s SLS, Orion capsule and ground systems the same way they would if they were preparing for an actual launch. 

SLS is the backbone of NASA’s Artemis program, a new-age follow-on to Apollo that the space agency hopes will help establish a permanent human presence on the moon. And with a new moonshot comes a new moon rocket. SLS has never flown, and the recent wet dress rehearsal was supposed to be its last hurdle. But whether or not Artemis 1 is actually ready to fly now is not yet clear.

Monday’s activities primarily focused on filling the rocket’s cryogenic fuel tanks. The two-stage SLS uses liquid hydrogen (LH2) and liquid oxygen (LOX) as hypergolic propellants. Three attempts to fuel the rocket during a previous wet-dress try in April were cut short when operators encountered technical issues, including a hydrogen leak high in the Artemis 1 stack’s mobile launch platform (MLP). 

Those issues were addressed inside KSC’s Vehicle Assembly Building (VAB) over the past month, but controllers on Monday ran into another hydrogen leak while running the wet dress at the launch pad. This new leak, however, appeared in a “quick disconnect” — a point where the fueling cables connecting the SLS to the MLP are designed to separate during launch. 

This new leak affected the proceedings on Monday. Technicians’ efforts to troubleshoot the issue were unsuccessful, and their labors pushed the count back three hours. But, with the SLS fully tanked, NASA officials made the decision to route a software patch enabling them to continue the simulated countdown anyway. 

The patch allowed the ground launch sequencer to basically skip over the automatic checks that would have detected the leak, but the onboard flight systems for SLS were unable to undergo the same failsafe bypass. As planned, the terminal count proceeded through the T-33 second mark, at which point the ground computers hand over flight control to SLS’s systems. 

The count was ultimately halted at T-29 seconds. NASA had hoped to run the clock all the way down to T-9 seconds, as originally planned, but are deeming the wet dress rehearsal to be largely a success regardless.

Photos: NASA’s new Space Launch System megarocket

“I would say we’re in the 90th percentile,” Mike Sarafin, Artemis mission manager at NASA, said during a call with reporters on Tuesday (June 21).

“Terminal count is a very dynamic time,” explained Charlie Blackwell-Thompson, Artemis launch director with the Exploration Ground Systems Program at KSC.

There are “lots of time-critical events that go on in the terminal count, that are checked both in the flight software and on the ground, and in the interaction between the two,” she added.

Citing the quick-disconnect leak as the only major hiccup during Monday’s tanking, Blackwell-Thompson and other NASA representatives on the call agreed the wet dress was “extremely smooth.”

Now, agency officials have to determine if this wet dress was good enough. The leak prevented the count from reaching the T-9 second target for wet dress launch abort, but that doesn’t mean NASA will have to do the wet dress rehearsal all over again before deciding to launch the Artemis 1 mission, which will send an uncrewed Orion on a roughly month-long journey around the moon. And by Tuesday’s call, nothing had been decided.

“There are a couple of things that we didn’t get in terminal count,” said Blackwell-Thompson. “We’ll go look at what those are. We’ll go look at what that means to us, if there are ways to go test those, and then we’ll come back and make a recommendation.”

“We need to really sit down and … look at what we’ve accomplished, see what additional work might be required, and take a look at the [quick disconnect],” Sarafin added during Tuesday’s call, pointing out that since NASA operators’ long day on Monday, not much work had been done yet to analyze any of the test data.  

NASA officials on the call were optimistic about the path ahead, even though they were noncommittal about what’s next for Artemis 1 in the immediate future. On the call, there was a shared confidence that a clearer path forward would emerge in a few days, after the team has had a chance to examine the Artemis 1 stack and data from the wet dress. 

“We’ll take all the data from yesterday and roll that into the next time we load this vehicle,” said Blackwell-Thompson. “I’m certain that it’ll be just as smooth as the core stage went yesterday.”

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‘No need to panic’ as sunspot with potential for solar flares doubles in size overnight, scientists say

Credit: Pixabay/CC0 Public Domain

A sunspot pointing toward Earth has the potential to cause solar flares, but experts told USA TODAY it’s far from unusual and eased concerns over how flares would affect the Blue Planet.

Active Region 3038, or AR3038, has been growing over the past week, said Rob Steenburgh, acting lead of the National Oceanic and Atmospheric Administration’s Space Weather Forecast Office.

“This is what sunspots do,” he said. “Over time, generally, they’ll grow. They go through stages, and then they decay.”

Sunspots appear darker because they are cooler than other parts of the sun’s surface, according to NASA. Sunspots are cooler because they form where strong magnetic fields prevent heat within the sun from reaching its surface.

“I guess the easiest way to put it is that sunspots are regions of magnetic activity,” Steenburgh said.

Solar flares, which typically rise from sunspots, are “a sudden explosion of energy caused by tangling, crossing or reorganizing of magnetic field lines near sunspots,” NASA said.

“You can think of it like the twisting of rubber bands,” Steenburgh said. “If you have a couple of rubber bands twisting around on your finger, they eventually get twisted too much, and they break. The difference with magnetic fields is that they reconnect. And when they reconnect, it’s in that process that a flare is generated.”

The larger and more complex a sunspot becomes, the higher the likelihood is for solar flares, Steenburgh said.

The sunspot has doubled in size each day for the past three days and is about 2.5 times the size of Earth, C. Alex Young, associate director for science in the Heliophysics Science Division at NASA’s Goddard Space Flight Center, said in an email.

Young said the sunspot is producing small solar flares but “does not have the complexity for the largest flares.” There is a 30% chance the sunspot will produce medium-sized flares and a 10% chance it will create large flares, he said.

W. Dean Pesnell, project scientist of the Solar Dynamics Observatory, said the sunspot is a “modest-sized active region” that “has not grown abnormally rapidly and is still somewhat small in area.”

“AR 3038 is exactly the kind of active region we expect at this point in the solar cycle,” he said.

Andrés Muñoz-Jaramillo, lead scientist at the SouthWest Research Institute in San Antonio, said the sunspot is nothing for people on Earth to worry about.

“I want to emphasize there is no need to panic,” he said. “They happen all the time, and we are prepared and doing everything we can to predict and mitigate their effects. For the majority of us, we don’t need to lose sleep over it.”

Solar flares have different levels, Muñoz-Jaramillo said. The smallest are A-class flares, followed by B, C, M and X at the highest strength. Within each letter class is a finer scale using numbers, and the higher numbers denote more intensity.

C flares are too weak to noticeably affect Earth, Muñoz-Jaramillo said. More intense M flares may disrupt radio communication at Earth’s poles. X flares can disrupt satellites, communication systems and power grids and, at their worst, cause electricity shortages and power outages.

Lower-intensity solar flares are pretty common; X flares are less so, Steenburgh said. In a single solar cycle, about 11 years, there are typically about 2,000 M1 flares, about 175 X1 flares and about eight X10 flares, he said. For the largest solar flares at X20 or above, there is less than one per cycle. This solar cycle began in December 2019.

The AR3038 sunspot has caused C flares, Steenburgh said. Although there have been no M or X flares from this area, he said there is a potential for more intense flares in the next week or so.


Sun releases moderate solar flare


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A huge comet will fly by Earth in July and you might see it

A comet first spotted in the distance in 2017 might finally be within view soon of amateur astronomers.

Comet C/2017 K2 (PANSTARRS), called K2 for short, was then the farthest active comet ever spotted, a title it recently surrendered to megacomet Comet Bernardinelli-Bernstein, detected last year. But even down one superlative, K2 is remarkable for activity. The comet began to spew gas and dust in the far outer solar system, whereas it’s more typical for comets to wake up around Jupiter’s orbit, much closer in.

Five years later, the icy body is finally drawing within reach of Earth and its amateur astronomers. K2’s closest approach to our planet will be on July 14, and it will get closest to the sun on Dec. 19. 

Related: Giant comet was active way farther from the sun than expected, scientists confirm

Assuming K2 survives the heated journey and continues to brighten, EarthSky (opens in new tab) predicts people with small telescopes will be able to spot the sojourner soon.

“It should brighten to magnitude 8 or even 7, still too dim for the unaided eye,” EarthSky wrote. 

Sharp-eyed viewers can usually spot stars of magnitude 6 in dark-sky conditions with no aid. In the case of this comet, you will also need areas away from light pollution to spot it with a telescope. 

“The darker the skies, the better the contrast will be,” EarthSky advised.

As the comet approaches us, professional observatories may be able to figure out how big its nucleus is. Early observations by the Canada–France–Hawaii Telescope (CFHT) suggested K2’s nucleus could be between 18 and 100 miles (30 to 160 kilometers) wide; Hubble Space Telescope observations suggested it might be only 11 miles (18 km) at most, EarthSky said.

In 2017, Hubble imagery determined that the comet’s coma (or fuzzy atmosphere) likely includes oxygen, nitrogen, carbon dioxide and carbon monoxide, all turning from solid to gas as the comet warmed.

An archival search of CFHT imagery suggested K2 was active at least as far back as 2013, when it was between the orbits of Uranus and Neptune, NASA said at the time.

All predictions for comet activity are subject to change, however. Comets are prone to falling apart or brightening unpredictably when the draw close to the intense heat and gravity of our sun. That characteristic, however, makes them all the more interesting to astronomers who want to understand how comets are put together.

Follow Elizabeth Howell on Twitter @howellspace (opens in new tab). Follow us on Twitter @Spacedotcom (opens in new tab) and on Facebook (opens in new tab).



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Can a Future Fleet of Robotic Fish Clean Up Microplastic Pollution in the Ocean?

Microplastics are a menace. They’ve been found everywhere from the top of Mount Everest to melted Antarctic snow. Microplastics have even been found circulating in human blood. But perhaps the place where they are having the worst impact is in Earth’s oceans. Plastic is the single most common debris in the sea—often breaking down over time into tiny bits that are consumed by fish and capable of wreaking havoc on marine ecosystems.

That’s why scientists have been working on a new method of getting rid of them for good: fish-shaped robots that can actually clean up the oceans while swimming.

In a study published Wednesday in the journal Nano Letters, researchers at Sichuan University in China created a fish-bot made of a light-activated material that can absorb microplastics as it swims in water. The team believes the new bot could be used to transport pollutants to another location where they can be collected and properly disposed of. It could also be used for detecting and monitoring microplastics in harsher environments that humans can’t explore easily like the frigid waters of the arctic.

“The proof-of-concept robot is demonstrated to emphasize its maximum swimming speed of 2.67 body length per second, whose speed is comparable to that of plankton,” the study authors wrote, adding that the speed outperforms similar soft robots.

The fish-bot is made of a composite material that’s safe for marine environments and physically reacts when a near-infrared light laser is pointed at it. Blinking the laser on and off can cause the robot’s “tail” to flap back and forth, allowing it to mimic a real fish and swim. As it moves, microplastic material sticks to its body, much like suckerfish do to whales and sharks. On top of that, the material the Sichuan University researchers used can repair itself when cut—which means it’s effectively self-healing.

While we’re still a long ways away from schools of fish-bots roaming the seas, this is still an innovative solution to the persistent problem of microplastics in our polluted oceans. It could one day provide a novel way of ridding some areas of the pollutant—just don’t eat one if you catch it on your line.

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NASA to Power Down Voyager Probes: Here Are Their Best Space Photos

The Voyager Space Probes — the most distant cameras in the universe — are being powered down after 44 years of interstellar travel.

Voyager 1 and Voyager 2 have made it deeper into space than any manmade object in history. Both were launched in 1977 to photograph a fortuitous alignment of the planets in our solar system.

A Voyager probe took this false-color image of Saturn’s rings on August 23, 1981.
Neptune, as seen by Voyager 2 in 1989.

The Voyager program was able to take advantage of a moment of cosmic coordination when Jupiter, Saturn, Uranus, and Neptune were all lined up in such a way that the probes could visit each of these planets on their one-way journey away from Earth.

The probes snapped images of Jupiter’s clouds, discovered new phenomena like volcanic activity on Jupiter’s moon Io, and investigated Saturn’s rings.

NASA used three Voyager 2 images — taken through ultraviolet, violet and green filters — to make this photograph of Saturn.
The Voyager probes’ pictures of Miranda, Uranus’ moon, revealed its complicated geological past.
Neptune’s moon Triton, as seen by Voyager 2 in 1989.

NASA has previously said that the Voyagers “were destined—perhaps eternally—to wander the Milky Way.” But the radioactive plutonium-powered probes are losing energy by about four watts a year.

Launched 45 years ago, NASA has made the decision to reduce power on the probes which could extend their life span a few more years until about 2030. Initial projections had expected the Voyager mission to last just four years.

“We’ve done 10 times the warranty on the darn things,” Ralph McNutt, a physicist at the Johns Hopkins University Applied Physics Laboratory, tells Scientific American.

Jupiter and two of its moons.
A false-color image of Jupiter’s ring, discovered by the Voyager probes.
Profile of Voyager

The probes’ primary purpose was to fly by Jupiter and Saturn, which they did in two years. After successfully completing their initial mission, they just kept going deeper into space and sending back images of our solar system from afar.

In 1990, the Voyager 1 sent back the iconic “Pale Blue Dot” picture, showing the Earth against the massive expanse of space taken 3.7 billion miles away from our sun.

Pale Blue Dot

In 1998, Voyager 1 became the farthest human-made object in space — 6.5 billion miles from Earth. The probes are now 12 billion and 14.5 billion miles away from Earth and counting, according to NASA’s live tracker.

Volcanic activity on the surface of Io, one of Jupiter’s moons.
Neptune’s Rings
Neptune, seen in false color by Voyager 2 in 1989. Here, the red or white coloring means that sunlight is passing through a methane-rich atmosphere.

After 2030, Voyager will likely lose contact with Earth but both probes carry a 12-inch, gold-plated record that carries information from Earth. This includes 115 images, greetings in 55 different languages, sounds of the wind, rain, the human heartbeat, and 90 minutes of music.

Neptune, as seen by Voyager 2 in 1989.
Enceladus, one of Saturn’s moons, as seen by Voyager.
Voyager 2 captured these images, in true color (left) and false-color (right) of Neptune in 1986.
Saturn, November 16, 1980.
Neptune in 1989.

In another 20,000 years, the probes will pass the nearest star, Proxima Centauri, with this time capsule of human life.


Image credits: All photos by NASA/JPL.

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Swarm of rainbow-colored starfish devour sea lion corpse on seafloor

This stunning photo of a dead California sea lion covered in colorful bat stars recently announced as the winner of a major wildlife photography award. (Image credit: David Slater)

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An award-winning photographer has captured the somber moment when dozens of colorful starfish set about devouring a lifeless sea lion on the seafloor in California. 

Wildlife photographer David Slater captured the haunting photo in the shallow waters of Monterey Bay. The dead sea lion and its compatriots swimming in the background are most likely California sea lions (Zalophus californianus), but they could also be Steller sea lions (Eumetopias jubatus), based on the two species’ geographical ranges. The sea stars are all bat stars (Patiria miniata), scavenging starfish that come in a wide range of colors. The bat stars play a key role in recycling the sea lion into energy and nutrients, returning its remains to the marine food web.

The eerie image recently won first place in the “Aquatic Life” category at the California Academy of Science’s Big Picture Competition (opens in new tab). “I knew this image was special when I first published it but words cannot even describe how I feel taking first place in such a prestigious contest,” Slater wrote on Instagram (opens in new tab). The image shows that “beauty and adventure can be found in unexpected places,” he added.

Related: No one knows why decapitated sea lions keep turning up in Vancouver Island 

It is unclear how the sea lion in the image died. It may have died from natural causes or been killed by anthropogenic factors, such as a vessel strike, plastic ingestion or entanglement in fishing gear. However, California sea lion populations are actually sharply increasing in size and are listed as “least concern” on the International Union for Conservation Nature (IUCN) Red List of Threatened Species (opens in new tab).

Bat stars get their name from the webbing that grows between their arms, which resembles a bat’s wings. The starfish typically have five arms but can have as many as nine, and the animals grow to be up to 8 inches (20 centimeters) across, according to Monterey Bay Aquarium (opens in new tab). They have been documented in a range of colors but are most commonly red, orange, yellow, brown, green or purple. 

Bat stars have light-sensing “eye-spots” at the end of each arm, and olfactory cells on the bottom of their arms enable them to “taste” chemicals left by small invertebrates or corpses in the water. When bat stars find food they push out one of their two stomachs through their mouths and release digestive enzymes to break down their meal before ingesting it, according to Monterey Bay Aquarium.

An orange bat star off the coast of the Santa Cruz Island in southern California. (Image credit: Shutterstock)

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These starfish also have tiny, symbiotic worms that live in the grooves on the underside of the stars’ bodies and feed on scraps left behind by their hosts. A single bat star can support up to 20 of these worms, so there may be more than 100 worms in the new image that are busily digesting bits of sea lion.

As scavengers, the bat stars and their hitchhiking worms play an important role in this ocean ecosystem by recycling nutrients and energy from the top of the food chain back to the bottom. 

“While this scene appears melancholic, rest assured the sea lion is giving back to the community with which it once swam,” competition organizers wrote on the Big Picture website. “When the bat stars have had their fill, any number of creatures big and small will [also] be able to derive energy and shelter from what’s left behind for years to come.”

However, bat stars may be under threat due to climate change. Rising ocean temperatures have helped to spread a new disease known as sea star wasting syndrome, which first emerged in Alaska in 2013. The disease is believed to be caused by a bacterium and leads to abnormally twisted arms, white lesions, deflation of arms and body, arm loss and body disintegration, which is almost always fatal, according to the National Park Service (opens in new tab). Bat stars are one of the species known to be at risk from this disease, according to Monterey Bay Aquarium.

Originally published on Live Science.



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Scientists Identify a Possible Source for Red Cap on Pluto’s Largest Moon Charon

Southwest Research Institute scientists combined data from NASA’s New Horizons mission with novel laboratory experiments and exospheric modeling to reveal the likely composition of the red cap on Pluto’s moon Charon and how it may have formed. New findings suggest drastic seasonal surges in Charon’s thin atmosphere combined with light breaking down the condensing methane frost may be key to understanding the origins of Charon’s red polar zones. Credit: Courtesy NASA / Johns Hopkins APL / SwRI

Research combined spacecraft data with new lab experiments, models of

Charon is the largest of Pluto’s moons. At half the size of Pluto, it is the largest known satellite relative to its parent body. Charon orbits Pluto every 6.4 Earth days. James Christy and Robert Harrington discovered Charon in 1978 at the U.S. Naval Observatory in Flagstaff, Arizona.

“Prior to New Horizons, the best Hubble images of Pluto revealed only a fuzzy blob of reflected light,” said SwRI’s Randy Gladstone, a member of the New Horizons science team. “In addition to all the fascinating features discovered on Pluto’s surface, the flyby revealed an unusual feature on Charon, a surprising red cap centered on its north pole.”

Soon after the 2015 encounter, New Horizons scientists proposed that a reddish “tholin-like” material at Charon’s pole could be synthesized by ultraviolet light breaking down methane molecules. These are captured after escaping from Pluto and then frozen onto the moon’s polar regions during their long winter nights. Tholins are sticky organic residues formed by chemical reactions powered by light, in this case the Lyman-alpha ultraviolet glow scattered by interplanetary hydrogen atoms.

“Our findings indicate that drastic seasonal surges in Charon’s thin atmosphere as well as light breaking down the condensing methane frost are key to understanding the origins of Charon’s red polar zone,” said SwRI’s Dr. Ujjwal Raut, lead author of a paper titled “Charon’s Refractory Factory” in the journal Science Advances. “This is one of the most illustrative and stark examples of surface-atmospheric interactions so far observed at a planetary body.”

The team realistically replicated Charon surface conditions at SwRI’s new Center for Laboratory Astrophysics and Space Science Experiments (CLASSE) to measure the composition and color of hydrocarbons produced on Charon’s winter hemisphere as methane freezes beneath the Lyman-alpha glow. The team fed the measurements into a new atmospheric model of Charon to show methane breaking down into residue on Charon’s north polar spot.

“Our team’s novel ‘dynamic photolysis’ experiments provided new limits on the contribution of interplanetary Lyman-alpha to the synthesis of Charon’s red material,” Raut said. “Our experiment condensed methane in an ultra-high vacuum chamber under exposure to Lyman-alpha photons to replicate with high fidelity the conditions at Charon’s poles.”

SwRI scientists also developed a new computer simulation to model Charon’s thin methane atmosphere. 

“The model points to ‘explosive’ seasonal pulsations in Charon’s atmosphere due to extreme shifts in conditions over Pluto’s long journey around the Sun,” said Dr. Ben Teolis, lead author of a related paper titled “Extreme Exospheric Dynamics at Charon: Implications for the Red Spot” in Geophysical Research Letters.

The team input the results from SwRI’s ultra-realistic experiments into the atmospheric model to estimate the distribution of complex hydrocarbons emerging from methane decomposition under the influence of ultraviolet light. The model has polar zones primarily generating ethane, a colorless material that does not contribute to a reddish color.

“We think ionizing radiation from the solar wind decomposes the Lyman-alpha-cooked polar frost to synthesize increasingly complex, redder materials responsible for the unique albedo on this enigmatic moon,” Raut said. “Ethane is less volatile than methane and stays frozen to Charon’s surface long after spring sunrise. Exposure to the solar wind may convert ethane into persistent reddish surface deposits contributing to Charon’s red cap.” 

“The team is set to investigate the role of solar wind in the formation of the red pole,” said SwRI’s Dr. Josh Kammer, who secured continued support from



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What’s Inside The Squid Cube?

In a containment lab in Wellington, New Zealand, Kat Bolstad considered the squid cube. It was the size of a keg and had been frozen solid since January, when it was hauled up during a research trawl in fishing grounds to the east of the country. The squid cube was not a cube of squids but rather one single cube-shaped squid, whose flaccid body had been folded into a rectangular fish bin and subsequently stored in a freezer. It chilled there until June, when Bolstad, a deep-sea squid biologist at Auckland University of Technology, was ready to unbox it.

“It’s not the first squid cube,” said Bolstad, who has seen many cubes of varying sizes and species in her line of work. But it certainly was a very special squid cube, comprising the carefully pleated body of an entire giant squid, meaning a species of deep-sea squid in the family Architeuthidae. When giant giant squids are caught in research trawls, their bodies are too big to be cubed, i.e. stored whole in a standard 50-liter fish bin. Those true giants are often frozen in pieces or “whole, in a gigantic sort of sausage-shaped, very large package that has to be moved by a forklift,” Bolstad said. But this giant squid, a young female, was just small enough to fit inside the fish bin and become a cube of her own. As Bolstad described the arrangement of the squid’s body: “It was like a cat curled up for a nap inside the fish bin.”

About twice a year, Bolstad’s lab sojourns to Wellington to thaw squid cubes and other squidsicles (frozen squids that bear somewhat less resemblance to regular geometric shapes). The city is home to the marine collection facilities of the National Institute of Water and Atmospheric Research, or NIWA, which slowly accumulates and freezes creatures collected on the institute’s research cruises. Some of the squids are frozen for months before their dead flesh experiences warmth again. And the quality of the carcasses can vary a lot depending on the squid’s journey from the deep to the surface. “Sometimes you get a really beautiful one,” Bolstad said. “Sometimes it looks like somebody sneezed in a tray.”

Credit: Kat Bolstad
This large Chiroteuthis, which has exceptionally long arms, is what would be considered a “beautiful” specimen.

Successfully unboxing frozen squids can be a race against time: Bolstad’s lab and NIWA staff members have to complete their work before the flesh starts to rot. Although a single, finger-sized squid might defrost in a half-hour, larger squids can take an entire day. And a squid compacted into a cube also does not defrost evenly, running the risk that the outside of the cube could rot while the inside is still frozen solid. A few years ago, Bolstad had to thaw a squid cube of a colossal squid—a different species altogether, and the largest invertebrate on the planet—weighing more than a thousand pounds. Colossal squid tissue is more delicate than giant squid tissue, so Bolstad’s team defrosted that colossal cube in a bath of sea ice to keep the dead squid in relatively pristine condition.

This June’s squid cube was less fussy, defrosting in air overnight until the researchers returned to unfold the half-thawed cube and run water over its body to help it along. “We did have visions of it, like, unfolding and then slithering to the floor and just having a horrible disaster in the morning,” Bolstad said. But the squid cube cooperated, and the next day could be fully unrolled and restored to its tentacled, 21-foot-long glory.

The formerly cube-shaped giant squid, fully unboxed.

Scientists do not often have the chance to examine giant squids. The animals are very large and live in waters thousands of feet deep, making it fairly unpredictable when one might turn up. For a long time, scientists could only study Architeuthis from squids that were discovered dead on the shore, dead in the water, or were digested or regurgitated by sperm whales, according to a 2013 paper in the American Malacological Bulletin. Recent advances in deep-sea trawling and underwater camera systems have given scientists a little more access to the elusive giants.

Still, it’s rare to come across a giant squid that has yet to reach full size, Bolstad said. Scientists are still sleuthing out the life cycle of giant squids, a cephalopod whose babyhood is somewhat of a black box. “There’s a size below which specimens are basically unknown,” Bolstad said, adding that there are records of “fairly small” mature males. But female giant squids get much larger: Whereas a mature male might top out at around 32 feet, a mature female can grow as long as 42 feet. Mature male giant squids produce packages of sperm called spermatophores and implant them into the skin of a female giant squid. But the researchers found only tiny hints of eggs in this particular cubed squid, meaning she was an immature female who had not mated.

Curious to learn what she ate, Bolstad’s team gently slid out the squid’s nearly gallon-sized innards. This week, the researchers plan to defrost the squid’s guts—which are sadly not cube-shaped but roughly oblong—and examine what half-digested creatures and undigested microplastics might lurk inside. With any luck, they’ll find a few parasites. Many parasites in the ocean have to move through different unique hosts throughout their life cycle: After being pooped out by a fish, they might have to penetrate a snail and then perhaps a clam before being eaten by another fish. Finding a parasitic worm in a giant squid could help scientists more fully understand where the worm journeys in its weird little life.

Credit: Kat Bolstad
Another mysterious squidsicle thawed into the head and tentacles of a giant squid.

Bolstad also wanted to retrieve a tiny calcium carbonate bone called a statolith from within the squid’s head that could hold a clue to the giant squid’s lifespan—one of the many creature’s many mysteries. “The squid has this little crystal floating around inside a fluid filled chamber,” Bolstad said. “The motion of the crystals in there tells the squid about its motion and momentum and position.” Squid statoliths function like our ear canals, helping the squid balance in the water. They also have growth rings, which could theoretically help estimate the age of the squid. But even though scientists can count the growth rings, they don’t yet know how often they accumulate, Bolstad said.

But a giant squid statolith is about the third of a size of a grain of rice, making removal from a larger squid rather tricky. “It’s very difficult to cut into a frozen giant squid head,” Bolstad said. “You need it to be like in this sweet spot of partially defrosted but not too defrosted.” The crystals always occur in a fluid-filled chamber in the same general region of the squid’s head, so scientists have to take a scalpel to the area without crushing or breaking the fragile crystals. “It’s a little bit of a lottery,” she said, adding that she successfully scooped out one of the squid’s two statoliths.

Although the squid cube was perhaps the grandest squid of the frozen bunch, Bolstad’s lab thawed another significantly-sized squidsicle that turned out to be the head and arms of a truly big giant squid. Even though the partial specimen was missing the bulk of its body, the head and arms alone weighed more than the small giant squid.

While Bolstad was in the lab, NIWA asked if she could identify a tiny specimen that was collected separately. The squid, which resembled an itty-bitty burrito, was the elusive and iconic ram’s horn squid, Spirula spirula. The species gets its common name from a delicately whorled shell inside its body, which could be seen poking out from the mantle.

Credit: Kat Bolstad
The ram’s horn squid, Spirula spirula, looking quite regal in death.

This year’s squid unboxing unearthed at least 30 species that have yet to be described and named, Bolstad said. “It’s the chance to potentially open a box and really make a discovery,” she said. “To experience taking something out of a box that one or two people have seen before,” she added.

Bolstad’s lab preserved around 20 specimens to be held in the collections at the Museum of New Zealand Te Papa Tongarewa. Her lab will return to Wellington next year or even sooner to do it all over again, unwrapping bags and unboxing cubes of small giant squids, giant giant squids, and many more squids of all sizes, observing all they can before the rot sets in.

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Scientists unveil bionic robo-fish to remove microplastics from seas | Plastics

Scientists have designed a tiny robot-fish that is programmed to remove microplastics from seas and oceans by swimming around and adsorbing them on its soft, flexible, self-healing body.

Microplastics are the billions of tiny plastic particles which fragment from the bigger plastic things used every day such as water bottles, car tyres and synthetic T-shirts. They are one of the 21st century’s biggest environmental problems because once they are dispersed into the environment through the breakdown of larger plastics they are very hard to get rid of, making their way into drinking water, produce, and food, harming the environment and animal and human health.

“It is of great significance to develop a robot to accurately collect and sample detrimental microplastic pollutants from the aquatic environment,” said Yuyan Wang, a researcher at the Polymer Research Institute of Sichuan University and one of the lead authors on the study. Her team’s novel invention is described in a research paper in the journal Nano Letters. “To the best of our knowledge, this is the first example of such soft robots.”

Researchers at Sichuan University have revealed an innovative solution to track down these pollutants when it comes to water contamination: designing a tiny self-propelled robo-fish that can swim around, latch on to free-floating microplastics, and fix itself if it gets cut or damaged while on its expedition.

The robo-fish is just 13mm long, and thanks to a light laser system in its tail, swims and flaps around at almost 30mm a second, similar to the speed at which plankton drift around in moving water.

The researchers created the robot from materials inspired by elements that thrive in the sea: mother-of-pearl, also known as nacre, which is the interior covering of clam shells. The team created a material similar to nacre by layering various microscopic sheets of molecules according to nacre’s specific chemical gradient.

This made them a robo-fish that is stretchy, flexible to twist, and even able to pull up to 5kg in weight, according to the study. Most importantly, the bionic fish can adsorb nearby free-floating bits of microplastics because the organic dyes, antibiotics, and heavy metals in the microplastics have strong chemical bonds and electrostatic interactions with the fish’s materials. That makes them cling on to its surface, so the fish can collect and remove microplastics from the water. “After the robot collects the microplastics in the water, the researchers can further analyse the composition and physiological toxicity of the microplastics,” said Wang.

Plus, the newly created material also seems to have regenerative abilities, said Wang, who specialises in the development of self-healing materials. So the robot fish can heal itself to 89% of its ability and continue adsorbing even in the case it experiences some damage or cutting – which could happen often if it goes hunting for pollutants in rough waters.

This is just a proof of concept, Wang notes, and much more research is needed – especially into how this could be deployed in the real world. For example, the soft robot currently only works on water surfaces, so Wang’s team will soon be working on more functionally complex robo-fish that can go deeper under the water. Still, this bionic design could offer a launchpad for other similar projects, Wang said. “I think nanotechnology holds great promise for trace adsorption, collection, and detection of pollutants, improving intervention efficiency while reducing operating costs.”

Indeed, nanotechnology will be one of the most important players in the fight against microplastics, according to Philip Demokritou, the director of the Nanoscience and Advanced Materials Research Center at Rutgers University, who was not involved in this study.

Demokritou’s lab also focuses on using nanotechnology to get rid of microplastics from the planet – but instead of cleaning them up, they are working on substituting them. This week, in the journal Nature Food, he announced the invention of a new plant-based spray coating which can serve as an environmentally friendly alternative to plastic food wraps. Their case study showed that this starch-based fibre spray can fend off pathogens and guard against transportation damage just as well, if not better, than current plastic packaging options.

“The motto for the last 40 to 50 years for the chemical industry is: let’s make chemicals, let’s make materials, put them out there and then clean the mess 20, or 30 years later,” said Demokritou. “That’s not a sustainable model. So can we synthesise safer design materials? Can we derive materials from food waste as part of the circular economy and turn them into useful materials that we can use to address this problem?”

This is low-hanging fruit for the field of nanotechnology, Demokritou said, and as research into materials gets better so will the multi-pronged approach of substituting plastic in our daily lives and filtering out its microplastic residue from the environment.

“But there’s a big distinction between an invention and an innovation,” Demokritou said. “Invention is something that nobody has thought about yet. Right? But innovation is something that will change people’s lives, because it makes it to commercialisation, and it can be scaled.”

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