Science

it’s-not-just-us:-other-animals-change-their-social-habits-in-old-age

It’s not just us: Other animals change their social habits in old age

out to pasture —

Long-term studies reveal what elderly deer, sheep, and macaques are up to in their later years.

A Rhesus macaque on a Buddhist stupa in the Swayambhunath temple complex in Kathmandu, Nepal

Enlarge / As female macaques age, the size of their social network shrinks.

Walnut was born on June 3, 1995, at the start of what would become an unusually hot summer, on an island called Rum (pronounced room), the largest of the Small Isles off the west coast of Scotland. We know this because since 1974, researchers have diligently recorded the births of red deer like her, and caught, weighed and marked every calf they could get their hands on—about 9 out of every 10.

Near the cottage in Kilmory on the northern side of the island where the researchers are based, there has been no hunting since the project began, which allowed the deer to relax and get used to human observers. Walnut was a regular there, grazing the invariably short-clipped grass in this popular spot. “She would always just be there in the group, with her sisters and their families,” says biologist Alison Morris, who has lived on Rum for more than 23 years and studies the deer year-round.

Walnut raised 14 offspring, the last one in 2013, when she was 18 years old. In her later years, Morris recalls, Walnut would spend most of her time away from the herd, usually with Vanity, another female (called a hind) of the same age who had never calved. “They were often seen affectionately grooming each other, and after Walnut died of old age in October 2016, at the age of 21—quite extraordinary for a hind—Vanity spent most of her time alone. She died two years later, at the grand age of 23.”

Are old hinds left behind?

Such a shift in social life is common in aging red deer females, says ecologist Gregory Albery, now at Georgetown University in Washington, DC, who spent months on the island studying the deer during his PhD training. (Males roam around more and associate less consistently with others, so they are harder to study.) “Older females tend to be observed in the company of fewer others. That was easy to establish,” he says. “The more difficult question to answer has been why we are seeing this pattern, and what it means.”

The first question one should ask, Albery says, is whether individual deer alter their behavior to associate with fewer others as they age, or whether individuals that associate with fewer others tend to live to an older age. This is the kind of question that many researchers are unable to answer when simply comparing individuals of different ages. But long-term studies like the one at Rum can do so through long-term tracking of populations. Forty times a year, the deer are censused by fieldworkers like Morris who recognize the deer on sight and meticulously note where they are and with whom.

When they accounted for the age and survival of the deer in their analysis, Albery and colleagues found that the link between age and number of associates remained solid: Social connections do, indeed, decrease as individuals age. Might this be because many of the older deer’s friends have died? On the contrary, Albery and colleagues found that older deer who had recently lost friends tended to hang out with others more often.

So why do old hinds have fewer contacts? Part of the explanation may be that they don’t range as widely as they grow older. Studying the deer for a couple of months would not have exposed this trend, says Albery: It was only revealed by tracking the same individuals through time. “Deer with a larger home range generally live longer,” he explains, so an analysis at any single point in time would show larger ranges for older deer and suggest that home ranges expand with age. Tracking individuals through time reveals the opposite is true. “Their home ranges decrease in size as they age,” Albery says.

It is unlikely that older deer move around less because they are concentrating on the core of their favorite habitat, says Albery. The center of their range shifts with age, and they are observed more often in taller and probably less nutritious vegetation, away from the most popular spots. This indicates there might be some kind of competitive exclusion going on: Perhaps more energetic, younger deer with offspring to feed are colonizing the best grazing patches.

On the other hand, older deer may also have different preferences. “Perhaps the longer grasses are easier to eat when your incisors are too worn to clip the short grass everyone else is after,” Albery says. Plus the deer don’t have to bend over as far to reach the longer grass.

A recent study by Albery and colleagues in Nature Ecology & Evolution  found that older deer reduce their contacts more than you’d expect if their shrinking range was the only cause. That suggests the behavior may have evolved for a reason—one that Albery prosaically summarizes as, “Deer shit where they eat.

Gastrointestinal worms are rampant on the island. And though the deer do not get infected through direct contact with others, being at the same place at the same time probably does increase their risk of ingesting eggs or larvae in the still-warm droppings of one of their associates.

“Younger animals need to put themselves out there to make friends, but perhaps when you’re older and you already have some, the risk of disease just isn’t worth it,” says study coauthor Josh Firth, a behavioral ecologist at the University of Oxford.

In addition, says ecologist Daniel Nussey of the University of Edinburgh, another coauthor, “there are indications that the immune system of aging deer is less effective in suppressing worm infections, so they might be more likely to die from them.”

It’s not just us: Other animals change their social habits in old age Read More »

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SpaceX roars back to orbit barely two weeks after in-flight anomaly

Look who’s back, back again —

“It was incredible to see how quickly the team was able to identify the cause of the mishap.”

The Starlink 10-9 mission lifts off early Saturday morning from Florida.

Enlarge / The Starlink 10-9 mission lifts off early Saturday morning from Florida.

SpaceX webcast

Early on Saturday morning, at 1: 45 am local time, a Falcon 9 rocket soared into orbit from its launch site at Kennedy Space Center in Florida.

By some measures this was an extremely routine mission—it was, after all, SpaceX’s 73rd launch of this calendar year. And like many other Falcon 9 launches this year, the “Starlink 10-9” mission carried 23 of the broadband internet satellites into orbit. However, after a rare failure earlier this month, this particular Falcon 9 rocket was making a return-to-flight for the company, and attempting to get the world’s most active booster back into service.

And by all measures, it performed. The first stage booster, B-1069, made its 17th flight into orbit before landing on the Just Read the Instructions drone ship in the Atlantic Ocean. Then, a little more than an hour after liftoff, the rocket’s second stage released its payload into a good orbit, from which the Starlink spacecraft will use their on-board thrusters to reach operational altitudes in the coming weeks.

A crack in the sense line

The Falcon 9 rocket only failed a little more than 15 days ago, during a Starlink launch from Vandenberg Space Force Base, California, at 7: 35 pm PDT (02: 35 UTC) on July 11. During that mission, just a few minutes after stage separation, an unusual buildup of ice was observed on the Merlin vacuum engine that powers the second stage of the vehicle.

According to the company, the Merlin vacuum engine successfully completed its first burn after the second stage separated. However, during this time a liquid oxygen leak developed near the engine—which led to the buildup of ice observed during the webcast.

Engineers and technicians were quickly able to pinpoint the cause of the leak, a crack in a “sense line” for a pressure sensor attached to the vehicle’s liquid oxygen system. “This line cracked due to fatigue caused by high loading from engine vibration and looseness in the clamp that normally constrains the line,” the company said in an update published prior to Saturday morning’s launch.

This leak excessively cooled the engine, and caused a lower amount of igniter fluid to be available prior to re-lighting the Merlin for its second burn to circularize the rocket’s orbit before releasing the Starlink satellites. This caused a hard start of the Merlin engine. Ultimately the satellites were released into a lower orbit, where they burnt up in Earth’s atmosphere within days.

The sense line that failed is redundant, SpaceX said. It is not used by the flight safety system, and can be covered by alternate sensors already present on the engine. In the near term, the sense line will be removed from the second stage engine for Falcon 9 launches.

During a news briefing Thursday, SpaceX director Sarah Walker said this sense line was installed based on a customer requirement for another mission. The only difference between this component and other commonly flown sense lines is that it has two connections rather than one, she said. This may have made it a bit more susceptible to vibration, leading to a small crack.

Getting back fast

SpaceX identified the cause of the failure within hours of the anomaly, and worked the Federal Aviation Administration to come to a rapid resolution. On Thursday, the launch company received permission to return to flight.

“It was incredible to see how quickly the team was able to identify the cause of the mishap, and then the associated corrective actions to ensure success,” Walker said.

Before the failure on the night of July 11th, SpaceX had not experienced a mission failure in the previous 297 launches of the Falcon 9 rocket, dating back to the Amos-6 launch pad explosion in September 2016. The short interval between the failure earlier this month, and Saturday’s return to flight, appears to be unprecedented in spaceflight history.

The company now plans to launch two more Starlink missions on the Falcon 9 rocket this weekend, one from Cape Canaveral Space Force Station in Florida, as well as Vandenberg Space Force Base in California. It then has three additional missions before a critical astronaut flight for NASA, Crew-9, that could occur as soon as August 18.

For this reason, NASA was involved in the investigation of the second stage failure. Steve Stich, manager of NASA’s Commercial Crew Program, said SpaceX did an “extraordinary job” in identifying the root cause of the failure, and then rapidly looking at its Dragon spacecraft and first stage of the Falcon 9 rocket to ensure there were no other sensors that could cause similar problems.

SpaceX roars back to orbit barely two weeks after in-flight anomaly Read More »

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People are overdosing on off-brand weight-loss drugs, FDA warns

Dosage disarray —

Bad math and unclear directions are behind overdoses of up to 20 times the normal amount.

Wegovy is an injectable prescription weight-loss medicine that has helped people with obesity.

Enlarge / Wegovy is an injectable prescription weight-loss medicine that has helped people with obesity.

The US Food and Drug Administration has approved two injectable versions of the blockbuster weight-loss and diabetes drug, semaglutide (Wegovy and Ozempic). Both come in pre-filled pens with pre-set doses, clear instructions, and information about overdoses. But, given the drugs’ daunting prices and supply shortages, many patients are turning to imitations—and those don’t always come with the same safety guardrails.

In an alert Friday, the FDA warned that people are overdosing on off-brand injections of semaglutide, which are dispensed from compounding pharmacies in a variety of concentrations, labeled with various units of measurement, administered with improperly sized syringes, and prescribed with bad dosage math. The errors are leading some patients to take up to 20 times the amount of intended semaglutide, the FDA reports.

Though the agency doesn’t offer a tally of overdose cases that have been reported, it suggests it has received multiple reports of people sickened by dosing errors, with some requiring hospitalizations. Semaglutide overdoses cause nausea, vomiting, abdominal pain, fainting, headache, migraine, dehydration, acute pancreatitis, and gallstones, the agency reports.

Bad math

In typical situations, compounding pharmacies provide personalized formulations of FDA-approved drugs, for instance, if a patient is allergic to a specific ingredient, requires a special dosage, or needs a liquid version of a drug instead of a pill form. But, when commercially available drugs are in short supply—as semaglutide drugs currently are—then compound pharmacies can legally step in to make their own versions if certain conditions are met. However, these imitations are not FDA-approved and, as such, don’t come with the same safety, quality, and effectiveness assurances as approved drugs.

In the warning Friday, the FDA said that some patients received confusing instructions from compounding pharmacies, which indicated they inject themselves with a certain number of “units” of semaglutide—the volume of which may vary depending on the concentration—rather than milligrams or milliliters. In other instances, patients received U-100 (1-milliliter) syringes to administer 0.05-milliliter doses of the drug, or five units. The relatively large syringe size compared with the dose led some patients to administer 50 units instead of five.

The figure demonstrates how syringe size could lead some to an incorrect dosage.

Enlarge / The figure demonstrates how syringe size could lead some to an incorrect dosage.

FDA-approved semaglutide drugs, meanwhile, are dosed in milligrams and come in standardized concentrations. The agency received several reports of health care providers incorrectly converting from milligrams to units or milliliters, leading them to calculate the wrong dosages. With these math errors, some patients administered five to 10 times more semaglutide than intended.

“FDA recognizes the substantial consumer interest in using compounded semaglutide products for weight loss,” the agency wrote. “However, compounded drugs pose a higher risk to patients than FDA-approved drugs.” The agency urged patients and prescribers to only use compounded versions when absolutely necessary.

People are overdosing on off-brand weight-loss drugs, FDA warns Read More »

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Rocket Report: ABL loses its second booster; Falcon 9 cleared for return to flight

NASA's SLS rocket core stage for Artemis II is moved to the VAB.

Enlarge / NASA’s SLS rocket core stage for Artemis II is moved to the VAB.

NASA/Ben Smegelsky

Welcome to Edition 7.04 of the Rocket Report! Probably the most striking news this week came from ABL, which said in a terse social media statement that it had lost its second RS1 rocket during pre-flight testing. This is unfortunate, since the company had been so careful and meticulous in working toward this second launch attempt. It’s a reminder of how demanding this industry remains.

As always, we welcome reader submissions, and if you don’t want to miss an issue, please subscribe using the box below (the form will not appear on AMP-enabled versions of the site). Each report will include information on small-, medium-, and heavy-lift rockets as well as a quick look ahead at the next three launches on the calendar.

ABL loses rocket after static fire test. ABL Space Systems said Monday that its next rocket had suffered “irrecoverable” damage during preparations for launch. “After a pre-flight static fire test on Friday, a residual pad fire caused irrecoverable damage to RS1,” the company said on the social media site X. “The team is investigating root cause and will provide updates as the investigation progresses.” As of the writing of this report three days later, the company has not posted any additional information.

Not particularly promising … This is a serious setback for the launch company, which attempted the debut flight of its RS1 vehicle 18 months ago and had been preparing for this second attempt for a long time. The California-based company had been keeping a low profile and had not made a social media posting since May. The RS1 vehicle is advertised as having a lift capacity of 1.35 metric tons at a price of $12 million. During ABL’s initial launch attempt in January 2023, an anomaly in the rocket caused all nine of the RS1’s first-stage engines to shut down. (submitted by Ken the Bin)

Point-to-point company test-fires engine. A space transportation startup with visions of high-speed point-to-point travel has started tests of the engine that will power their vehicle, Space News reports. Frontier Aerospace test-fired its Mjölnir engine on July 18, its chairman, Alex Tai, said during a panel discussion at the Farnborough International Airshow. Mjölnir is a full-flow staged combustion engine. The firing lasted less than a second but demonstrated the startup of the turbopumps and successful ignition.

Starting with a smaller version … The company plans to do longer engine burns as part of the testing program. The version of Mjölnir currently being tested produces less than 3,000 pounds-force of thrust. New Frontier plans to use a much more powerful version of the engine on a vehicle called the Intercontinental Rocketliner, a suborbital vehicle intended to carry 100 people on high-speed flights around the planet at hypersonic speeds. (submitted by Ken the Bin and EllPeaTea)

The easiest way to keep up with Eric Berger’s space reporting is to sign up for his newsletter, we’ll collect his stories in your inbox.

Ursa Major invests in Ohio. Ursa Major will buy several industrial 3D printers and hire 15 new employees for a research and development center in Youngstown, Ohio, focused on additive manufacturing, Payload reports. The Colorado-based rocket engine maker will contribute $10.5 million in capital investment alongside a $4 million grant from JobsOhio, a privately funded economic development nonprofit. The expansion of a small existing facility will enable the company to step up its development of solid rocket motors—a top priority for the Department of Defense.

The war needs what it needs … In AprilUrsa won a contract of undisclosed value from the Navy to develop a lower-cost manufacturing approach for the standardized solid rocket motors used across a range of missiles. The US supply chains for those motors—mainly provided by Northrop Grumman and L3Harris—have been stressed by US support for Ukraine’s defense against Russian invaders. In November, Ursa raised $138 million to support its push into solid rocket motor manufacturing in a round that reportedly valued the company at $750 million.

Rocket Report: ABL loses its second booster; Falcon 9 cleared for return to flight Read More »

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Rocket delivered to launch site for first human flight to the Moon since 1972

Rocket delivered to launch site for first human flight to the Moon since 1972

The central piece of NASA’s second Space Launch System rocket arrived at Kennedy Space Center in Florida this week. Agency officials intend to start stacking the towering launcher in the next couple of months for a mission late next year carrying a team of four astronauts around the Moon.

The Artemis II mission, officially scheduled for September 2025, will be the first voyage by humans to the vicinity of the Moon since the last Apollo lunar landing mission in 1972. NASA astronauts Reid Wiseman, Victor Glover, Christina Koch, and Canadian mission specialist Jeremy Hansen will ride the SLS rocket away from Earth, then fly around the far side of the Moon and return home inside NASA’s Orion spacecraft.

“The core is the backbone of SLS, and it’s the backbone of the Artemis mission,” said Matthew Ramsey, NASA’s mission manager for Artemis II. “We’ve been waiting for the core to get here because all the integrated tests and checkouts that we do have to have the core stage. It has the flight avionics that drive the whole system. The boosters are also important, but the core is really the backbone for Artemis. So it’s a big day.”

The core stage rolled off of NASA’s Pegasus barge at Kennedy early Wednesday, following a weeklong ocean voyage from New Orleans, where Boeing builds the rocket under contract to NASA.

Ramsey told Ars that ground teams hope to begin stacking the rocket’s two powerful solid rocket boosters on NASA’s mobile launcher platform in September. Each booster, supplied by Northrop Grumman, is made of five segments with pre-packed solid propellant and a nose cone. All the pieces for the SLS boosters are at Kennedy and ready for stacking, Ramsey said.

The SLS upper stage, built by United Launch Alliance, is also at the Florida launch site. Now, the core stage is at Kennedy. In August or September, NASA plans to deliver the two remaining elements of the SLS rocket to Florida. These are the adapter structures that will connect the core stage to the upper stage, and the upper stage to the Orion spacecraft.

A heavy-duty crane inside the cavernous Vehicle Assembly Building (VAB) will hoist each segment of the SLS boosters into place on the launch platform. Once the boosters are fully stacked, ground teams will lift the 212-foot (65-meter) core stage vertical in the transfer aisle running through the center of the VAB. A crane will then lower the core stage between the boosters. That could happen as soon as December, according to Ramsey.

Then comes the launch vehicle stage adapter, the upper stage, the Orion stage adapter, and finally, the Orion spacecraft itself.

Moving toward operations

NASA’s inspector general reported in 2022 that NASA’s first four Artemis missions will each cost $4.1 billion. Subsequent documents, including a Government Accountability Office report last year, suggest the expendable SLS core stage is responsible for at least a quarter of the cost for each Artemis flight.

The core stage for Artemis II is powered by four hydrogen-fueled RS-25 engines produced by Aerojet Rocketdyne. Two of the reusable engines for Artemis II have flown on the space shuttle, and the other two RS-25s were built in the shuttle era but never flew. Each SLS launch will put the core stage and its engines in the Atlantic Ocean.

Steve Wofford, who manages the stages office for the SLS program at NASA’s Marshall Space Flight Center, told Ars there are “no major configuration differences” between the core stages for Artemis I and Artemis II. The only minor differences involve instrumentation that NASA wanted on Artemis I to measure pressures, accelerations, vibrations, temperatures, and other parameters on the first flight of the Space Launch System.

“We are still working off some flight observations that we made on Artemis I, but no showstoppers,” Wofford said. “On the first article, the test flight, Artemis I, we really loaded it up. That’s a golden opportunity to learn as much as you can about the vehicle and the flight regime, and anchor all your models… As you progress, you need less and less of that. So Core Stage 2 will have less development flight instrumentation than Core Stage 1, and then Core Stage 3 will have less still.”

Rocket delivered to launch site for first human flight to the Moon since 1972 Read More »

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NASA nears decision on what to do with Boeing’s troubled Starliner spacecraft

Boeing's Strainer spacecraft is seen docked at the International Space Station in this picture taken July 3.

Enlarge / Boeing’s Strainer spacecraft is seen docked at the International Space Station in this picture taken July 3.

The astronauts who rode Boeing’s Starliner spacecraft to the International Space Station last month still don’t know when they will return to Earth.

Astronauts Butch Wilmore and Suni Williams have been in space for 51 days, six weeks longer than originally planned, as engineers on the groundwork through problems with Starliner’s propulsion system.

The problems are twofold. The spacecraft’s reaction control thrusters overheated, and some of them shut off as Starliner approached the space station June 6. A separate, although perhaps related, problem involves helium leaks in the craft’s propulsion system.

On Thursday, NASA and Boeing managers said they still plan to bring Wilmore and Williams home on the Starliner spacecraft. In the last few weeks, ground teams completed testing of a thruster on a test stand at White Sands, New Mexico. This weekend, Boeing and NASA plan to fire the spacecraft’s thrusters in orbit to check their performance while docked at the space station.

“I think we’re starting to close in on those final pieces of flight rationale to make sure that we can come home safely, and that’s our primary focus right now,” Stich said.

The problems have led to speculation that NASA might decide to return Wilmore and Williams to Earth in a SpaceX Crew Dragon spacecraft. There’s one Crew Dragon currently docked at the station, and another one is slated to launch with a fresh crew next month. Steve Stich, manager of NASA’s commercial crew program, said the agency has looked at backup plans to bring the Starliner crew home on a SpaceX capsule, but the main focus is still to have the astronauts fly home aboard Starliner.

“Our prime option is to complete the mission,” Stich said. “There are a lot of good reasons to complete this mission and bring Butch and Suni home on Starliner. Starliner was designed, as a spacecraft, to have the crew in the cockpit.”

Starliner launched from Cape Canaveral Space Force Station in Florida on June 5. Wilmore and Williams are the first astronauts to fly into space on Boeing’s commercial crew capsule, and this test flight is intended to pave the way for future operational flights to rotate crews of four to and from the International Space Station.

Once NASA fully certifies Starliner for operational missions, the agency will have two human-rated spaceships for flights to the station. SpaceX’s Crew Dragon has been flying astronauts since 2020.

Tests, tests, and more tests

NASA has extended the duration of the Starliner test flight to conduct tests and analyze data in an effort to gain confidence in the spacecraft’s ability to safely bring its crew home and to better understand the root causes of the overheating thrusters and helium leaks. These problems are inside Starliner’s service module, which is jettisoned to burn up in the atmosphere during reentry, while the reusable crew module, with the astronauts inside, parachutes to an airbag-cushioned landing.

The most important of these tests was a series of test-firings of a Starliner thruster on the ground. This thruster was taken from a set of hardware slated to fly on a future Starlink mission, and engineers put it through a stress test, firing it numerous times to replicate the sequence of pulses it would see in flight. The testing simulated two sequences of flying up to the space station, and five sequences the thruster would execute during undocking and a deorbit burn for return to Earth.

“This thruster has seen quite a bit of pulses, maybe even more than what we would anticipate we would see during a flight, and more aggressive in terms of two uphills and five downhills,” Stich said. “What we did see in the thruster is the same kind of thrust degradation that we’re seeing on orbit. In a number of the thrusters (on Starliner), we’re seeing reduced thrust, which is important.”

Starliner’s flight computer shut off five of the spacecraft’s 28 reaction control system thrusters, produced by Aerojet Rocketdyne, during the rendezvous with the space station last month. Four of the five thrusters were recovered after overheating and losing thrust, but officials have declared one of the thrusters unusable.

The thruster tested on the ground showed similar behavior. Inspections of the thruster at White Sands showed bulging in a Teflon seal in an oxidizer valve, which could restrict the flow of nitrogen tetroxide propellant. The thrusters, each generating about 85 pounds of thrust, consume the nitrogen tetroxide, or NTO, oxidizer and mix it with hydrazine fuel for combustion.

A poppet valve, similar to an inflation valve on a tire, is designed to open and close to allow nitrogen tetroxide to flow into the thruster.

“That poppet has a Teflon seal at the end of it,” Nappi said. “Through the heating and natural vacuum that occurs with the thruster firing, that poppet seal was deformed and actually bulged out a little bit.”

Stich said engineers are evaluating the integrity of the Teflon seal to determine if it could remain intact through the undocking and deorbit burn of the Starliner spacecraft. The thrusters aren’t needed while Starliner is attached to the space station.

“Could that particular seal survive the rest of the flight? That’s the important part,” Stich said.

NASA nears decision on what to do with Boeing’s troubled Starliner spacecraft Read More »

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Astronomers find first emission spectra in brightest GRB of all time

shine on, you beautiful BOAT —

Chance that first detected emission line is a noise fluctuation is one in half a billion.

A jet of particles moving at nearly light speed emerges from a massive star in this artist’s concept.

Enlarge / A jet of particles moving at nearly light-speed emerges from a massive star in this artist’s concept of the BOAT.

NASA’s Goddard Space Flight Center Conceptual Image Lab

Scientists have been all aflutter since several space-based detectors picked up a powerful gamma-ray burst (GRB) in October 2022—a burst so energetic that astronomers nicknamed it the BOAT (Brightest Of All Time). Now an international team of astronomers has analyzed an unusual energy peak detected by NASA’s Fermi Gamma-ray Space Telescope and concluded that it was an emission spectra, according to a new paper published in the journal Science. Per the authors, it’s the first high-confidence emission line ever seen in 50 years of studying GRBs.

As reported previously, gamma-ray bursts are extremely high-energy explosions in distant galaxies lasting between mere milliseconds to several hours. There are two classes of gamma-ray bursts. Most (70 percent) are long bursts lasting more than two seconds, often with a bright afterglow. These are usually linked to galaxies with rapid star formation. Astronomers think that long bursts are tied to the deaths of massive stars collapsing to form a neutron star or black hole (or, alternatively, a newly formed magnetar). The baby black hole would produce jets of highly energetic particles moving near the speed of light, powerful enough to pierce through the remains of the progenitor star, emitting X-rays and gamma rays.

Those gamma-ray bursts lasting less than two seconds (about 30 percent) are deemed short bursts, usually emitting from regions with very little star formation. Astronomers think these gamma-ray bursts are the result of mergers between two neutron stars, or a neutron star merging with a black hole, comprising a “kilonova.” That hypothesis was confirmed in 2017 when the LIGO collaboration picked up the gravitational wave signal of two neutron stars merging, accompanied by the powerful gamma-ray bursts associated with a kilonova.

Several papers were published last year reporting on the analytical results of all the observational data. Those findings confirmed that GRB 221009A was indeed the BOAT, appearing especially bright because its narrow jet was pointing directly at Earth. But the various analyses also yielded several surprising results that puzzled astronomers. Most notably, a supernova should have occurred a few weeks after the initial burst, but astronomers didn’t detect one, perhaps because it was very faint, and thick dust clouds in that part of the sky were dimming any incoming light.

Earlier this year, astronomers confirmed that the BOAT came from a supernova, thanks to the telltale signatures of key elements like calcium and oxygen that one would expect to find with a supernova. However, they did not find evidence of the expected heavy elements like platinum and gold, which bears on the longstanding question of the origin of such elements in the universe. The BOAT might just be special in that regard; further data will tell us more.

“It gave me goosebumps”

A few minutes after the BOAT erupted, Fermi’s Gamma-ray Burst Monitor recorded an unusual energy peak. Scientists now say this feature is the first high-confidence emission line ever seen in 50 years of studying GRBs.

The newly detected spectral emission line was likely caused by the collision of matter and anti-matter, according to the authors, producing a pair of gamma rays that are blue-shifted toward higher energies because we are looking into the jet. Having a spectral emission associated with a GRB is important because it can shed light on the specific chemicals involved in the interactions. There have been prior studies reporting possible evidence for absorption or emission lines in other GRBs, but they have usually turned out likely to be statistical noise.

That’s not the case with this latest detection, according to co-author Om Sharan Salafia at INAF-Brera Observatory in Milan, Italy, who added that the odds of this turning out to be a statistical fluctuation “are less than one chance in half a billion.” His INAF colleague and co-author, Maria Edvige Ravasio, said that when she first saw the signal, “it gave me goosebumps.”

Why did astronomers take so long to detect it? When the BOAT first erupted in 2022, it saturated most of the space-based gamma-ray detectors, including the Fermi Space Telescope, making them unable to measure the most intense part of that blast. The emission line didn’t appear until a good five minutes after the burst when it had sufficiently dimmed for Fermi to make a measurement. The spectral emission lasted for about 40 seconds and reached a peak energy of about 12 MeV, compared to 2 or 3 MeB for visible light, per the authors.

Science, 2024. DOI: 10.1126/science.adj3638  (About DOIs).

Astronomers find first emission spectra in brightest GRB of all time Read More »

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Astronauts find their tastes dulled, and a VR ISS hints at why

Pass the sriracha —

The visual environment of the ISS seems to influence people’s experience of food.

Image of astronauts aboard the ISS showing off pizzas they've made.

Enlarge / The environment you’re eating in can influence what you taste, and space is no exception.

Astronauts on the ISS tend to favor spicy foods and top other foods with things like tabasco or shrimp cocktail sauce with horseradish. “Based on anecdotal reports, they have expressed that food in space tastes less flavorful. This is the way to compensate for this,” said Grace Loke, a food scientist at the RMIT University in Melbourne, Australia.

Loke’s team did a study to take a closer look at those anecdotal reports and test if our perception of flavor really changes in an ISS-like environment. It likely does, but only some flavors are affected.

Tasting with all senses

“There are many environmental factors that could contribute to how we perceive taste, from the size of the area to the color and intensity of the lighting, the volume and type of sounds present, the way our surroundings smell, down to even the size and shape of our cutlery. Many other studies covered each of these factors in some way or another,” said Loke.

That’s why her team started to unravel the bland ISS food mystery by recreating the ISS environment in VR. “Certain environments are difficult to be duplicated, such as the ISS, which led us to look at digital solutions to mimic how it felt [to be] living and working in these areas,” said Julia Low, a nutrition and food technologist at the RMIT University and co-author of the study.

Once the VR version of the ISS was ready, the team had 54 participants smell flavors of vanilla, almonds, and lemon. The first round of tests was done in a pretty normal room, and the second with the VR goggles on, running the simulated ISS environment complete with sterile, cluttered spaces, sounds present at the real ISS, and objects floating around in microgravity.

The participants said the lemon flavor seemed the same in both rounds. Almonds and vanilla, on the other hand, seemed more intense when participants were in the VR environment. While that’s the opposite of what might be expected from astronauts’ dining habits, it is informative. “The bottom line is we may smell aromas differently in a space-like environment, but it is selective as to what kind of aromas. We’re not entirely sure why this happens, but knowing that a difference exists is the first step to find out more,” Loke said.

Loke and her colleagues then pulled out a mass spectrometer and took a closer look at the composition of the flavors they used in the tests.

Space-ready ingredients

The lemon flavor in Loke’s team tests was lemon essential oil applied to a cotton ball, which was then placed in a closed container that was kept sealed until it was given to the participants to smell. The vapors released from the container contained several volatile chemicals such as limonene, camphene, 3-carene, and monoterpene alcohols like linalool, carveol, and others.

Almond flavors contained similar chemicals, but there was one notable difference: the almond and vanilla flavors contained benzaldehyde, while the lemon did not. “Benzaldehyde naturally gives off a sweet aroma, while the lemon aroma, which did not have it, has a more fruity and citrusy aroma profile. We believe that it may be the sweet characteristics of aromas that leads to a more intense perception in [simulated] space,” said Loke.

Astronauts find their tastes dulled, and a VR ISS hints at why Read More »

barbie-movie-“may-have-spurred-interest-in-gynecology,”-study-finds

Barbie movie “may have spurred interest in gynecology,” study finds

Do you need a gynecologist? —

The movie apparently sparked some questions.

A digital advertisement board displaying a Barbie movie poster is seen in New York on July 24, 2023.

Enlarge / A digital advertisement board displaying a Barbie movie poster is seen in New York on July 24, 2023.

This post contains spoilers—for the movie and women’s health care.

There’s nothing like stirrups and a speculum to welcome one to womanhood, but for some, the recent Barbie movie apparently offered its own kind of eye-opening introduction.

The smash-hit film ends with the titular character making the brave decision to exit Barbieland and enter the real world as a bona fide woman. The film’s final scene follows her as she fully unfurls her new reality, attending her first woman’s health appointment. “I’m here to see my gynecologist,” she enthusiastically states to a medical receptionist. For many, the line prompted a wry chuckle, given her unsuspecting eagerness and enigmatic anatomy. But for others, it apparently raised some fundamental questions.

Online searches in the US for “gynecologist”—or alternate spellings, such as “gynaecologist”—rose an estimated 51 percent over baseline in the week following Barbie‘s July 21, 2023 release, according to a study published Thursday in JAMA Network Open. Moreover, searches related to the definition of gynecology spiked 154 percent. Those search terms included “gynecologist meaning,” “what is a gynecologist,” “what does a gynecologist do,” “why see a gynecologist,” and the weightiest of questions: “do I need a gynecologist.”

The “Barbie effect”

The study’s authors, led by researchers at Harvard Medical School, assessed 34 query terms that fit into six categories of searches, including “gynecologist,” “gynecologist definition,” “gynecologist appointment,” “doctors,” “doctor’s appointment,” and “women’s health.” The last three served as controls for more general interest in medical information. As the authors put it, the three control searches helped establish “whether unobserved contemporaneous factors influencing health-seeking behavior more generally may have contributed to gynecologic-related search volume.”

While the researchers noted clear spikes in “gynecologist” and “gynecologist definition” searches, they saw no changes in search trends for the three control search categories during the week after the movie’s release: “doctors,” “doctor’s appointment,” and “women’s health.” This suggested that the increase in gynecology-related searches may, in fact, be linked to the movie rather than some increased interest in health care generally.

The researchers also did not see a corresponding increase in searches related to gynecology appointments, suggesting that the transient online interest in gynecology didn’t translate to online searches for actual gynecological care, with queries such as “gynecologist near me.” The researchers speculate that two factors might explain this. For one, there’s the possibility that the data couldn’t capture care-seeking decisions. It may be that there’s a longer, variable time gap between newfound awareness of gynecology and the decision to seek care. The second possibility is that the people searching for basic information about gynecology may not need gynecological care themselves.

Overall, the authors conclude that “Barbie’s closing line may have spurred interest in gynecology.” The finding is supported by earlier work that also suggests popular culture can have measurable influences on health literacy and awareness among the general public, the authors conclude. For instance, when journalist Katie Couric live streamed her colonoscopy, there was a transient 21 percent increase in colonoscopies, and when actress Angelina Jolie penned an editorial about her experience with breast cancer, there was a transient 64 percent increase in genetic testing for breast cancer risk (BRCA testing). But while the “Barbie effect” seems to have raised some awareness of gynecology, it remains unclear if it will lead to a measurable improvement in health outcomes.

Barbie movie “may have spurred interest in gynecology,” study finds Read More »

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US solar production soars by 25 percent in just one year

Solar sailing —

2024 is seeing the inevitable outcome of the building boom in solar farms.

A single construction person set in the midst of a sea of solar panels.

With the plunging price of photovoltaics, the construction of solar plants has boomed in the US. Last year, for example, the US’s Energy Information Agency expected that over half of the new generating capacity would be solar, with a lot of it coming online at the very end of the year for tax reasons. Yesterday, the EIA released electricity generation numbers for the first five months of 2024, and that construction boom has seemingly made itself felt: generation by solar power has shot up by 25 percent compared to just one year earlier.

The EIA breaks down solar production according to the size of the plant. Large grid-scale facilities have their production tracked, giving the EIA hard numbers. For smaller installations, like rooftop solar on residential and commercial buildings, the agency has to estimate the amount produced, since the hardware often resides behind the metering equipment, so only shows up via lower-than-expected consumption.

In terms of utility-scale production, the first five months of 2024 saw it rise by 29 percent compared to the same period in the year prior. Small-scale solar was “only” up by 18 percent, with the combined number rising by 25.3 percent.

Most other generating sources were largely flat, year over year. This includes coal, nuclear, and hydroelectric, all of which changed by 2 percent or less. Wind was up by 4 percent, while natural gas rose by 5 percent. Because natural gas is the largest single source of energy on the grid, however, its 5 percent rise represents a lot of electrons—slightly more than the total increase in wind and solar.

US electricity sources for January through May of 2024. Note that the numbers do not add up to 100 percent due to the omission of minor contributors like geothermal and biomass.

Enlarge / US electricity sources for January through May of 2024. Note that the numbers do not add up to 100 percent due to the omission of minor contributors like geothermal and biomass.

John Timmer

Overall, energy use was up by about 4 percent compared to the same period in 2023. This could simply be a matter of changing weather conditions that require more heating or cooling. But there have been several trends that should increase electricity usage: the rise of bitcoin mining, the growth of data centers, and the electrification of appliances and transport. So far, that hasn’t shown up in the actual electricity usage in the US, which has stayed largely flat for decades. It could be possible that 2024 is the year when usage starts going up again.

More to come

It’s worth noting that this data all comes from before some of the most productive months of the year for solar power; overall, the EIA is predicting that solar production could rise by as much as 42 percent in 2024.

So, where does this leave the US’s efforts to decarbonize? If we combine nuclear, hydro, wind, and solar under the umbrella of carbon-free power sources, then these account for about 45 percent of US electricity production so far this year. Within that category, wind and solar now produce more than three times hydroelectric, and roughly the same amount as nuclear.

Wind and solar have also produced 1.3 times as much electricity as coal so far in 2024, with solar alone now producing about half as much as coal. That said, natural gas still produces twice as much electricity as wind and solar combined, indicating we still have a long way to go to decarbonize our grid.

When you look at the generating facilities that will be built over the next 12 months, it's difficult not to see a pattern.

Enlarge / When you look at the generating facilities that will be built over the next 12 months, it’s difficult not to see a pattern.

Still, we can expect solar’s productivity to climb even before the year is out. That’s in part because we don’t yet have numbers for June, the month that contains the longest day of the year. But it’s also because the construction boom shows no sign of stopping. As noted here, solar and wind deployments are expected to dwarf everything else over the coming year. The items in gray on the map primarily represent battery storage, which will allow us to make better use of those renewables, as well.

By contrast, facilities that are scheduled for retirement over the next year largely consist of coal and natural gas plants.

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Scientists unlock more secrets of Rembrandt’s pigments in The Night Watch

More from operation night watch —

Use of arsenic sulfides for yellow, orange/red hues adds to artist’s known pigment palette.

The Nightwatch, or Militia Company of District II under the Command of Captain Frans Banninck Cocq (1642)

Enlarge / Rembrandt’s The Night Watch underwent many chemical and mechanical alterations over the last 400 years.

Public domain

Since 2019, researchers have been analyzing the chemical composition of the materials used to create Rembrandt’s masterpiece, The Night Watch, as part of the Rijksmuseum’s ongoing Operation Night Watch, devoted to its long-term preservation. Chemists at the Rijksmuseum and the University of Amsterdam have now detected unusual arsenic-based yellow and orange/red pigments used to paint the duff coat of one of the central figures in the painting, according to a recent paper in the journal Heritage Science. It’s a new addition to Rembrandt’s known pigment palette that further adds to our growing body of knowledge about the materials he used.

As previously reported, past analyses of Rembrandt’s paintings identified many pigments the Dutch master used in his work, including lead white, multiple ochres, bone black, vermilion, madder lake, azurite, ultramarine, yellow lake, and lead-tin yellow, among others. The artist rarely used pure blue or green pigments, with Belshazzar’s Feast being a notable exception. (The Rembrandt Database is the best resource for a comprehensive chronicling of the many different investigative reports.)

Early last year, the researchers at Operation Night Watch found rare traces of a compound called lead formate in the painting—surprising in itself, but the team also identified those formates in areas where there was no lead pigment, white or yellow. It’s possible that lead formates disappear fairly quickly, which could explain why they have not been detected in paintings by the Dutch Masters until now. But if that is the case, why didn’t the lead formate disappear in The Night Watch? And where did it come from in the first place?

Hoping to answer these questions, the team whipped up a model of “cooked oils” from a 17th-century recipe and analyzed those model oils with synchrotron radiation. The results supported their hypothesis that the oil used for light parts of the painting was treated with an alkaline lead drier. The fact that The Night Watch was revarnished with an oil-based varnish in the 18th century complicates matters, as this may have provided a fresh source of formic acid, such that different regions of the painting rich in lead formates may have formed at different times in the painting’s history.

Last December, the team turned its attention to the preparatory layers applied to the canvas. It’s known that Rembrandt used a quartz-clay ground for The Night Watch—the first time he had done so, perhaps because the colossal size of the painting “motivated him to look for a cheaper, less heavy and more flexible alternative for the ground layer” than the red earth, lead white, and cerussite he was known to use on earlier paintings.

The Night Watch. (b) Detail of figure’s embroidered gold buff coat. (c) X-ray diffraction image of coat detail showing arsenic. (d) Stereomicroscope image showing arsenic hot spot.” height=”531″ src=”https://cdn.arstechnica.net/wp-content/uploads/2024/07/rembrandt1-640×531.jpg” width=”640″>

Enlarge / (a) Rembrandt’s The Night Watch. (b) Detail of figure’s embroidered gold buff coat. (c) X-ray diffraction image of coat detail showing arsenic. (d) Stereomicroscope image showing arsenic hot spot.

N. De Keyser et al., 2024

They used 3D X-ray methods to capture more detail, revealing the presence of an unknown (and unexpected) lead-containing layer located just underneath the ground layer. This could be due to using a lead compound added to the oil used to prepare the canvas as a drying additive—perhaps to protect the painting from the damaging effects of humidity. (Usually a glue sizing was used before applying the ground layer.) The lead layer discovered last year could be the reason for the unusual lead protrusions in areas of The Night Watch, since there are no other lead-containing compounds in the paint. It’s possible that lead migrated into the painting’s ground layer from the lead-oil preparatory layer below.

An intentional combination

The presence of arsenic sulfides in The Night Watch appears to be an intentional pigment combination by Rembrandt, according to the authors of this latest paper. Artists throughout history have used naturally occurring orpiment and realgar, as well as artificial arsenic sulfide pigments, to get yellow, orange, and red hues in their paints. Orpiment was also used for medicinal purposes, in hair removal creams and oils, in wax seals, yellow ink, bookbinder green (mixed with indigo), and for the treatment or coating of metals like silver.

However, the use of artificial arsenic sulfides has rarely been reported in artworks, although they are mentioned in multiple artists’ treatises dating back to the 15th century. Earlier work using advanced analytical techniques such as Raman spectroscopy and X-ray powder diffraction revealed that Rembrandt used arsenic sulfide pigments (artificial orpiment) in two late paintings: The Jewish Bride (c 1665) and The Man in a Red Cap (c 1665).

For this latest work, Nouchka De Keyser of the Rijksmuseum and co-authors used macroscopic X-ray fluorescence imaging to map The Night Watch, which revealed the presence of arsenic and sulfur in the doublet sleeves and embroidered buff coat worn by Lt. Willem Van Ruytenburch, i.e., the central figure to the right of Captain Frans Bannick Cocq in the painting. The researchers initially assumed that this was due to Rembrandt’s use of orpiment for yellow hues and realgar for red hues.

Ars Vitraria Experimentalis, 1679. (c) Page from the Weimar taxa of 1674 including prices for white, yellow, and red arsenic.” height=”300″ src=”https://cdn.arstechnica.net/wp-content/uploads/2024/07/rembrandt2-640×300.jpg” width=”640″>

Enlarge / (a, b) Pages from Johann Kunckel’s Ars Vitraria Experimentalis, 1679. (c) Page from the Weimar taxa of 1674 including prices for white, yellow, and red arsenic.

N. De Keyser et al., 2024

To learn more, they took tiny samples and analyzed them with light microscopy, micro-Raman spectroscopy, electron microscopy, and X-ray powder diffraction. They found the yellow particles were actually pararealgar while the orange to red particles were semi-amorphous pararealgar. These are more unusual arsenic sulfide components, typically associated with degradation products from either the natural minerals or their artificial equivalents as they age.

But De Keyser et al. concluded that the presence of these components was actually an intentional mixture, based on their perusal of multiple historical sources and catalogs of collection cabinets with long lists of various arsenic sulfides. There was clearly contemporary knowledge of manipulating both natural and artificial arsenic sulfides to get different shades of yellow, orange, and red.

They also found vermilion and lead-tin yellow in the paint mixture; Rembrandt was known to use these to add brightness and intensity to his paintings. In the case of The Night Watch, “Rembrandt clearly aimed for a bright orange tone with a high color strength that allowed him to create an illusion of the gold thread embroidery in Van Ruytenburch’s costume,” the authors wrote. “The artificial orange to red arsenic sulfide might have offered different optical and rheological paint properties as compared to the mineral form of orpiment and realgar.”

In addition, the team examined paint samples from different artists known to use arsenic sulfides—whose works are also part of the Rijksmuseum collection—and found a similar mixture of pigments in a painting by Rembrandt’s contemporary, Willem Kalf. “It is evidence that a variety of natural and artificial arsenic sulfides were manufactured and traded during Rembrandt’s time and were available in Amsterdam,” the authors wrote—most likely imported, since the Dutch Republic did not have considerable mining resources.

Heritage Science, 2024. DOI: 10.1186/s40494-024-01350-x  (About DOIs).

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no,-nasa-hasn’t-found-life-on-mars-yet,-but-the-latest-discovery-is-intriguing

No, NASA hasn’t found life on Mars yet, but the latest discovery is intriguing

Look at the big brain on percy —

“These spots are a big surprise.”

NASA’s Perseverance rover discovered “leopard spots” on a reddish rock nicknamed “Cheyava Falls” in Mars’ Jezero Crater in July 2024.

Enlarge / NASA’s Perseverance rover discovered “leopard spots” on a reddish rock nicknamed “Cheyava Falls” in Mars’ Jezero Crater in July 2024.

NASA/JPL-Caltech/MSSS

NASA’s Perseverance rover has found a very intriguing rock on the surface of Mars.

An arrowhead-shaped rock observed by the rover has chemical signatures and structures that could have been formed by ancient microbial life. To be absolutely clear, this is not irrefutable evidence of past life on Mars, when the red planet was more amenable to water-based life billions of years ago. But discovering these colored spots on this rock is darn intriguing and has Mars scientists bubbling with excitement.

“These spots are a big surprise,” said David Flannery, an astrobiologist and member of the Perseverance science team from the Queensland University of Technology in Australia, in a NASA news release. “On Earth, these types of features in rocks are often associated with the fossilized record of microbes living in the subsurface.”

What the rover found

This is a very recent discovery, and the science has not yet been peer-reviewed. The sample was collected on July 21—a mere four days ago—as the rover explored the Neretva Vallis riverbed. This valley was formed long ago when water rushed into Jezero Crater.

The science team operating Perseverance has nicknamed the rock Chevaya Falls and subjected it to multiple scans by the rover’s SHERLOC (Scanning Habitable Environments with Raman & Luminescence for Organics & Chemicals) instrument. The distinctive colorful spots, containing both iron and phosphate, are a smoking gun for certain chemical reactions—rather than microbial life itself.

On Earth, microbial life can derive energy from these kinds of chemical reactions. So, what we have here is a plausible source of energy for microbes on Mars. In addition, there are organic chemicals present on the same rock, which is consistent with something living there. From this, it is tempting to jump to the idea of microbes living on a rock, eons ago, in a Martian river. But this is not direct evidence of life.

NASA has a seven-step process for determining whether something can be confirmed as extraterrestrial life. This is known as the CoLD scale, for Confidence of Life Detection. In this case, the detection of these spots on a Martian rock represents just the first of seven steps—for example, scientists must still rule out non-biological possibility and identify other signals to have confidence in off-world life.

Bring them home

According to NASA, Perseverance has used all of its available instrumentation to study Chevaya Falls. “We have zapped that rock with lasers and X-rays and imaged it literally day and night from just about every angle imaginable,” said Ken Farley, Perseverance project scientist. “Scientifically, Perseverance has nothing more to give.”

The discovery provides some wind in the sails for NASA’s flagging efforts to devise and fly a Mars Sample Return mission. The agency’s most recent plan, costing $11 billion, was determined to be too expensive. Now, the space agency is asking the industry for help. In June it commissioned 10 studies on alternative means of returning rocks from Mars sooner, and presumably for a lower cost.

Now, scientists can point to rocks like Chevaya Falls and say this is precisely why they must be studied in ultra-capable labs back on Earth.

No, NASA hasn’t found life on Mars yet, but the latest discovery is intriguing Read More »