Wednesday, December 13, 2023


Incredibly rare half-male, half-female bird spotted in South America

 Dec 13 2023
JOHN MURILLO

Extremely rare half female, half male Green Honeycreeper spotted by an Otago professor in rural Columbia.

It’s only the second such sighting in more than 100 years; a half-male, half-female bird.


Kiwi professor Hamish Spencer was holidaying in Colombia when his fellow bird watcher pointed to a distinct half green and half blue bird. He knew it was the most “unusual bird sighting in his life.”

Spencer, a Sesquicentennial Distinguished Professor in University of Otago’s Department of Zoology, was holidaying in rural Manizales of Colombia in January, when amateur ornithologist John Murillo pointed out wild Green Honeycreeper.

“It was a wow moment. It is a common bird in Columbia, but this 
phenomenon is incredibly rare. It has only been seen twice [in 100 years].”

The sighting was only the second recorded example of gynandromorphism [an organism that contains both male and female characteristics] in the species in more than 100 years.

Spencer said what made the bird unusual was that it exhibited typical male plumage on its right side and female plumage on the left.

A rare phenomenon called Bilateral Gynandromorphy is a condition in which one side of an animal/bird exhibits male characters and the other female.


JOHN MURRILO/SUPPLIED
The striking Green Honeycreeper has half green and half blue plumage – an extremely rare phenomenon in birds.

“Many birdwatchers could go their whole lives and not see a bilateral gynandromorph [an animal half him and half her] in any species of bird.

“The phenomenon is extremely rare in birds, I know of no examples from New Zealand ever.”

“I don’t expect to see one again in my life.”

Photographs of the bird make the discovery even more significant as they are “arguably the best of a wild bilateral gynandromorphic bird of any species ever”.

Professor Spencer explained gynandromorphs – animals with both male and female characteristics in a species that usually have separate sexes – were important for understanding of sex determination and sexual behaviour in birds.


JOHN MURRILO/SUPPLIED
Professor Hamish Spencer’s report on the find, only the second recorded example of gynandromorphism in the species in more than 100 years, has been published in the Journal of Field Ornithology.

He hoped the novel discovery would inspire people to “treasure exceptions” as they always revealed something interesting.

“Be always on the lookout for oddities – who will find the first New Zealand example of a bilateral gynandromorph in a bird?”

The finding was published in the Journal of Field Ornithology last Friday.


Extremely rare bird captured on film


Peer-Reviewed Publication

UNIVERSITY OF OTAGO

Bilaterally gynandromorphic Green Honeycreeper 

IMAGE: 

PHOTOS OF A BILATERALLY GYNANDROMORPHIC GREEN HONEYCREEPER NEAR MANIZALES, COLOMBIA, 20 MAY 2022. CREDIT: JOHN MURILLO

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CREDIT: CREDIT: JOHN MURILLO




A striking and extremely rare half female, half male bird has been spotted by a University of Otago zoologist.

 

Sesquicentennial Distinguished Professor Hamish Spencer was holidaying in Colombia when an amateur ornithologist John Murillo pointed out a wild Green Honeycreeper with distinct half green, or female, and half blue, male, plumage.

 

“Many birdwatchers could go their whole lives and not see a bilateral gynandromorph in any species of bird. The phenomenon is extremely rare in birds, I know of no examples from New Zealand ever.

 

“It is very striking, I was very privileged to see it,” Professor Spencer says.

 

Photographs of the bird make the discovery even more significant as they are “arguably the best of a wild bilateral gynandromorphic bird of any species ever”.

 

A report on the find, only the second recorded example of gynandromorphism in the species in more than 100 years, has just been published in the Journal of Field Ornithology.

 

Professor Spencer says gynandromorphs – animals with both male and female characteristics in a species that usually have separate sexes – are important for our understanding of sex determination and sexual behaviour in birds.

 

The main groups in which the phenomenon has been recorded include animal species which feature strong sexual dimorphism; most often insects, especially butterflies, crustaceans, spiders, even lizards and rodents.

 

“This particular example of bilateral gynandromorphy – male one side and female the other – shows that, as in several other species, either side of the bird can be male or female.

 

“The phenomenon arises from an error during female cell division to produce an egg, followed by double-fertilization by two sperm,” he explains.

 

He hopes the novel discovery will inspire people to “treasure exceptions” as they always reveal something interesting.

 

“Be always on the lookout for oddities – who will find the first New Zealand example of a bilateral gynandromorph in a bird?”

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Daily singing workout keeps songbird males attractive

Peer-Reviewed Publication

UNIVERSITY OF SOUTHERN DENMARK



Every year in the Christmas season it becomes clear again that some people are amazingly skilled singers, like Mariah Carey and George Michael. Their singing can stir strong emotions.

Singing involves probably the most complex, and mostly hidden, movements humans and animal can make. To become a good singer, you need to learn how to coordinate the movements of hundreds of muscles in your body with extreme precision. Therefore, you need a lot of talent, and practice.

We all know that athletes invest a lot of time exercising their limb and body muscles, but how about training the muscles in your voice box?

“Surprisingly we know very little about effects of exercise on these muscles and if they even react to training in humans,” says Professor Coen Elemans from the University of Southern Denmark, expert on sound production, “No singer will let you come even near their precious voice box”.

Now a new study in the prestigious journal Nature Communications reports that male songbirds need to sing daily to exercise their vocal muscles and produce pretty songs. And the females notice if they didn’t.

 “Singing is crucial for songbirds. They sing to impress future partners, to defend their territories and to maintain social bonds,” says Dr. Iris Adam, lead author of the study.

The researchers show that training is necessary to keep songbird vocal muscles at top performance. And it is not just any training, it specifically is singing exercise that matters.

The study was conducted by an international team of researchers from the University of Southern Denmark, Leiden University, University of Umea and the University of Vermont and was led by Assistant Professor Iris Adam and Professor Coen Elemans at the Department of Biology University of Southern Denmark.

Vocal muscles need exercise, too

“It has long been known that songbird singing is controlled by fast vocal muscles, but until now we only had very little knowledge if and how these muscles might respond to exercise, like our leg muscles do”, says Iris Adam.

In their study, the researchers show that if songbirds don’t use their vocal muscles at all, they get much slower and weaker already within days. But even when the birds only skip singing, after 7 days the vocal muscles already lost 50% of their strength.

“This was very surprising”, says Dr. Adam, “First that these muscles reacted so strongly, but also how incredibly fast they lost performance. Indeed, it’s use it or lose it!”

Partners can hear the difference

When analyzing the songs sung, the team found that the birds sang differently before and after exercise.

“You and I could barely hear a difference between the songs, but we saw clear effects when we analyzed our song recordings”, says Dr. Adam.

As the ultimate test if this difference was important to the birds, the team next played songs to female zebra finches to ask them if they could hear a difference between before or after exercise, and which song they liked more.

"The female zebra finches in the playback experiment could directly hear the difference and 75 percent preferred the songs from the well exercised male", says Katharina Riebel, author on the study and expert in animal behaviour. 

The daily dawn chorus, an alternative explanation

“Interestingly, these results provide an alternative reason why birds sing so much and every day”, says Elemans.

Around the world, in spring and summer time, birds sing every morning in the daily dawn chorus. Why they do this is still puzzling to scientists.

“A lot of that singing seems out of context. They sing when they don’t need to,” says Adam.

“Our results now show that if they don’t exercise every day, their muscle performance decreases”, says Elemans, “On top of that, the lack of exercise is audible in their song and the females prefer song from exercised males”.

Thus, songbirds may need to invest lots of time and energy in singing every day to remain attractive.

And this may be true for all animals.

Vocal muscles need training programs different from leg muscles

When studying the zebra finch vocal muscles, the team made another very important discovery.

“When we humans go to the gym to exercise leg and arm muscles, they typically get slower with exercise,” says Per StÃ¥l, author on the study and expert in muscle exercise physiology in humans.

However, in songbirds vocal muscles don’t get stronger and slower with exercise, like limb muscles, but weaker and faster. This is opposite from normal limb and body muscles.

“This reversed training may be a unique feature for vocal muscles, that we think might be true for all vertebrates, including humans, because all vocal muscles are developmentally related”, says Iris Adam.

“Therefore, these findings can have major consequences for speech therapy and vocal training in humans”, says Coen Elemans.

Because it’s so challenging to study the physiology of human larynx muscles, therapeutic intervention is based on what we know from exercise physiology of leg muscles.

“However, training vocal muscle may thus work very differently”, says Elemans, adding that “Songbirds may be our best allies to study the physiology of vocal muscle to further improve voice training and rehabilitation in humans”. 

SPACE

CASSIOPEIA A: 
A FESTIVE SUPERNOVA REMNANT

BY: CAMILLE M. CARLISLE 
SKY &TELESCOPE
DECEMBER 12, 2023


New near-infrared observations from the Webb telescope reveal intricate strands of debris from the exploded star.
A new near-infrared image from NASA’s James Webb Space Telescope’s NIRCam of the supernova remnant Cassiopeia A. In the bottom right corner is a light echo , created by light from the star’s long-ago explosion off surrounding dust.
NASA / ESA / CSA / STScI / Danny Milisavljevic (Purdue University) / Ilse De Looze (UGent) / Tea Temim (Princeton University)

This new infrared image from the James Webb Space Telescope reveals the intricate knots of debris inside the supernova remnant Cassiopeia A. Cas A lies about 11,000 light-years from Earth and formed more than 300 years ago when a massive star went kablooey.

Spectroscopic study of the explosion’s light echo — the reflection of the flash off surrounding dust grains — has previously revealed that the event was a Type IIb supernova, the death of a big star stripped of most of its hydrogen shell.

JWST astronomers released a different image of Cas A earlier this year (see below). That one was assembled from mid-infrared data and highlighted in reddish orange where the expanding blast wave is ramming into material surrounding the dead star. In the new image, the outer regions have instead been colored white. This is not merely an aesthetic choice but one made to highlight that we’re looking at different kinds of emission: In mid-infrared, we were detecting glowing dust; in the near-infrared image, we’re seeing emission from electrons corkscrewing along magnetic field lines at breakneck speeds.
Cassiopeia A, as revealed by JWST's mid-infrared camera. This image combines various filters with the color red assigned to 25.5 microns, orange-red to 21 microns, orange to 18 microns, yellow to 12.8 microns, green to 11.3 microns, cyan to 10 microns, light blue to 7.7 microns, and blue to 5.6 microns.
NASA / ESA / CSA / Danny Milisavljevic (Purdue University) / Tea Temim (Princeton University) / Ilse De Looze (UGent); Image processing: Joseph DePasquale (STScI)

The most eye-catching part of the first, near-infrared image is the pinkish festoons. These strands are debris from the now-dead star and comprise sulfur, oxygen, argon, and neon. Dust sprinkles the mix. Cas A spans some 10 light-years, but some of these ejecta filaments are so small that they evade JWST’s resolution at this distance, meaning they’re at most 100 astronomical units across — roughly twice the size of the solar system, if you include the main part of the Kuiper Belt outside Neptune’s orbit.

Dust is a major player in stellar evolution. It helps cool gas, enabling it to collapse and form stars. Astronomers still question what the universe’s primary source of dust is. Some dust comes from aging, puffy giants that are sloughing off their outer layers as winds, but these don’t form rapidly enough to explain the high quantities of dust found in the early universe.

Supernovae also create dust, which forms in the cooling ejecta. The problem is, supernovae destroy the same dust they create: The shock wave created when the ejecta slam into surrounding material rebounds back into the remnant’s interior, heating and destroying dust as it goes.

The highly clumpy nature of ejecta that JWST is revealing could explain how dust survive this process: Grains may shelter deep inside the clumps, away from the shock wave’s destructive effects.

NASA’s Webb stuns with new high-definition look at exploded star

Reports and Proceedings

NASA/GODDARD SPACE FLIGHT CENTER

NASA’s Webb Stuns With New High-Definition Look at Exploded Star 

IMAGE: 

NASA’S JAMES WEBB SPACE TELESCOPE’S NEW VIEW OF CASSIOPEIA A (CAS A) IN NEAR-INFRARED LIGHT IS GIVING ASTRONOMERS HINTS AT THE DYNAMICAL PROCESSES OCCURRING WITHIN THE SUPERNOVA REMNANT. TINY CLUMPS REPRESENTED IN BRIGHT PINK AND ORANGE MAKE UP THE SUPERNOVA’S INNER SHELL, AND ARE COMPRISED OF SULFUR, OXYGEN, ARGON, AND NEON FROM THE STAR ITSELF. A LARGE, STRIATED BLOB AT THE BOTTOM RIGHT CORNER OF THE IMAGE, NICKNAMED BABY CAS A, IS ONE OF THE FEW LIGHT ECHOES VISIBLE NIRCAM’S FIELD OF VIEW. IN THIS IMAGE, RED, GREEN, AND BLUE WERE ASSIGNED TO WEBB’S NIRCAM DATA AT 4.4, 3.56, AND 1.62 MICRONS (F444W, F356W, AND F162M, RESPECTIVELY).

 

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CREDIT: NASA, ESA, CSA, STSCI, D. MILISAVLJEVIC (PURDUE UNIVERSITY), T. TEMIM (PRINCETON UNIVERSITY), I. DE LOOZE (UNIVERSITY OF GENT)




Like a shiny, round ornament ready to be placed in the perfect spot on a holiday tree, supernova remnant Cassiopeia A (Cas A) gleams in a new image from NASA’s James Webb Space Telescope. As part of the 2023 Holidays at the White House, First Lady of the United States Dr. Jill Biden debuted the first-ever White House Advent Calendar. To showcase the “Magic, Wonder, and Joy” of the holiday season, Dr. Biden and NASA are celebrating with this new image from Webb.

While all is bright, this scene is no proverbial silent night. Webb’s NIRCam (Near-Infrared Camera) view of Cas A displays this stellar explosion at a resolution previously unreachable at these wavelengths. This high-resolution look unveils intricate details of the expanding shell of material slamming into the gas shed by the star before it exploded.

Cas A is one of the most well-studied supernova remnants in all of the cosmos. Over the years, ground-based and space-based observatories, including NASA’s Chandra X-Ray ObservatoryHubble Space Telescope, and retired Spitzer Space Telescope have assembled a multiwavelength picture of the object’s remnant.

However, astronomers have now entered a new era in the study of Cas A. In April 2023, Webb’s MIRI (Mid-Infrared Instrument) started this chapter, revealing new and unexpected features within the inner shell of the supernova remnant. Many of those features are invisible in the new NIRCam image, and astronomers are investigating why.

‘Like Shards of Glass’

Infrared light is invisible to our eyes, so image processors and scientists translate these wavelengths of light to visible colors. In this newest image of Cas A, colors were assigned to different filters from NIRCam, and each of those colors hints at different activity occurring within the object.

At first glance, the NIRCam image may appear less colorful than the MIRI image. However, this simply comes down to the wavelengths in which the material from the object is emitting its light.

The most noticeable colors in Webb’s newest image are clumps represented in bright orange and light pink that make up the inner shell of the supernova remnant. Webb’s razor-sharp view can detect the tiniest knots of gas, comprised of sulfur, oxygen, argon, and neon from the star itself. Embedded in this gas is a mixture of dust and molecules, which will eventually become components of new stars and planetary systems. Some filaments of debris are too tiny to be resolved by even Webb, meaning they are comparable to or less than 10 billion miles across (around 100 astronomical units). In comparison, the entirety of Cas A spans 10 light-years across, or 60 trillion miles.

“With NIRCam’s resolution, we can now see how the dying star absolutely shattered when it exploded, leaving filaments akin to tiny shards of glass behind,” said Danny Milisavljevic of Purdue University, who leads the research team. “It’s really unbelievable after all these years studying Cas A to now resolve those details, which are providing us with transformational insight into how this star exploded.”

 

Hidden Green Monster

When comparing Webb’s new near-infrared view of Cas A with the mid-infrared view, its inner cavity and outermost shell are curiously devoid of color.

The outskirts of the main inner shell, which appeared as a deep orange and red in the MIRI image, now look like smoke from a campfire. This marks where the supernova blast wave is ramming into surrounding circumstellar material. The dust in the circumstellar material is too cool to be detected directly at near-infrared wavelengths, but lights up in the mid-infrared.

Researchers say the white color is light from synchrotron radiation, which is emitted across the electromagnetic spectrum, including the near-infrared. It’s generated by charged particles traveling at extremely high speeds spiraling around magnetic field lines. Synchrotron radiation is also visible in the bubble-like shells in the lower half of the inner cavity.

Also not seen in the near-infrared view is the loop of green light in the central cavity of Cas A that glowed in mid-infrared, nicknamed the Green Monster by the research team. This feature was described as “challenging to understand” by researchers at the time of their first look.

While the ‘green’ of the Green Monster is not visible in NIRCam, what’s left over in the near-infrared in that region can provide insight into the mysterious feature. The circular holes visible in the MIRI image are faintly outlined in white and purple emission in the NIRCam image – this represents ionized gas. Researchers believe this is due to the supernova debris pushing through and sculpting gas left behind by the star before it exploded.

Cassiopeia A NIRCam/MIRI (IMAGE)

NASA/GODDARD SPACE FLIGHT CENTER

Baby Cas A

Researchers were also absolutely stunned by one fascinating feature at the bottom right corner of NIRCam’s field of view. They’re calling that large, striated blob Baby Cas A – because it appears like an offspring of the main supernova.

This is a light echo, where light from the star’s long-ago explosion has reached and is warming distant dust, which is glowing as it cools down. The intricacy of the dust pattern, and Baby Cas A’s apparent proximity to Cas A itself, are particularly intriguing to researchers. In actuality, Baby Cas A is located about 170 light-years behind the supernova remnant.

There are also several other, smaller light echoes scattered throughout Webb’s new portrait.

The Cas A supernova remnant is located 11,000 light-years away in the constellation Cassiopeia. It’s estimated to have exploded about 340 years ago from our point of view.

The James Webb Space Telescope is the world’s premier space science observatory. Webb is solving mysteries in our solar system, looking beyond to distant worlds around other stars, and probing the mysterious structures and origins of our universe and our place in it. Webb is an international program led by NASA with its partners, ESA (European Space Agency) and the Canadian Space Agency.


14-inch spacecraft delivers new details 

about ‘hot Jupiters'


Reports and Proceedings

UNIVERSITY OF COLORADO AT BOULDER



A spacecraft the size of a cereal box has collected precise measurements of the atmospheres of large and puffy planets called “hot Jupiters.” The findings, led by a team from the University of Colorado Boulder, could help reveal how the atmospheres around these and a host of other worlds are escaping into space.

The observations are the first results to come from a hard-working NASA spacecraft known as the Colorado Ultraviolet Transit Experiment (CUTE). 

Kevin France, principal investigator for the mission, will present the group’s results at a media availability Monday, Dec. 11 at 4:30 p.m. at the 2023 meeting of the American Geophysical Union in San Francisco.

The diminutive spacecraft, which measures just 14 inches in length, may be cute, but its scientific findings are anything but. Since its launch in September 2021, CUTE has trained its single ultraviolet telescope at a series of hot Jupiters, some hundreds of light-years from Earth.

Hot Jupiters are among the hottest and angriest planets in the galaxy. As their name suggests, they are gas giants like our own Jupiter. These planets, however, hug much closer to their home stars, completing an orbit roughly once every several Earth days. In the process, stellar radiation cooks hot Jupiters to thousands of degrees Fahrenheit, and their atmospheres swell to enormous sizes, a bit like bread rising in an oven. 

Researchers have long suspected that this constant pummeling from stellar radiation could strip away the atmospheres from around some exoplanets over millions-to-billions of years. Data from CUTE suggest that the process might not be so simple. 

The CUTE team, which includes several undergraduate and graduate students, has observed seven hot Jupiters so far, with more on the way. Some of them seem to be losing their atmospheres, but others aren’t.

“The planets seem to be coming in all of the flavors,” said France, associate professor in the Laboratory for Atmospheric and Space Physics (LASP) and Department of Astrophysical and Planetary Sciences.

He added that CUTE is helping scientists to build out their field guide to the many kinds of planets that exist in the Milky Way Galaxy—including those that look nothing like Earth’s close neighbors.

“We want to understand how our solar system fits into the family of solar systems in the universe,” France said. “That means understanding the big planets, the small planets, the ones that have life and the ones that definitely don’t—and all of the important physical processes that are operating on these planets.”

Getting hot in here

CUTE’s road to scientific success wasn’t easy.

When the spacecraft first entered into orbit around Earth, France and his colleagues quickly noticed that it seemed to be experiencing a few glitches—a normal problem for many small satellites, or CubeSats, which often test out technology that’s never before flown into space. In one case, the shutter that protected CUTE’s telescope kept snapping shut when it wasn’t supposed to. 

The team, which included several undergraduate and graduate students, didn’t give up. The researchers commanded the spacecraft to open its shutter, then drained the battery that fed it, preventing the apparatus from shutting again. 

“CUTE is still working and collecting data today,” France said. “When we got our first real science results, it was really exciting.”

CUTE observes distant planets as they pass in front of their home stars, causing ultraviolet light from those stars to dim in the process. In some cases, the spacecraft is so precise that it can detect when starlight dims by just 1%. 

In a paper published in September, the researchers described their observations of a world called WASP-189b. This planet orbits a star in the constellation Libra more than 300 light-years, or thousands of trillions of miles, from Earth. It’s also incredibly toasty, with its atmosphere reaching temperatures of roughly 15,000 degrees Fahrenheit, according to the team’s results. That’s thousands of degrees hotter than the surface of the sun.

CUTE’s observations also suggest that gas is escaping from around WASP-189b at a similarly staggering rate of about 400 million kilograms (nearly 900 million pounds) per second.

Planets evolving

Not all of the planets CUTE has studied in its first two years were so exciting. In unpublished results, the team observed a second planet called MASCARA-4b that didn’t seem to be losing much gas at all. Others, like KELT-9b, fell somewhere in the middle.

France and his colleagues hope that their results could help uncover why some planets lose big chunks of their atmosphere, while others remain mostly unchanged. He suspects that it has to do with a combination of the planets themselves (larger planets generate a stronger gravitational pull) and the dynamics of their stars (more active stars likely wreak more havoc on planets than sedate stars).

Those same processes potentially sculpt planets, both in and out of Earth’s solar system, over time. Scientists, for example, theorize that Mars once hosted a much thicker atmosphere, but the sun eroded it away over billions of years. 

Atmospheric escape may also explain the origin of a class of planets known as “super Earths,” which are slightly larger than our own world. 

“There’s a lot of evidence that suggests that super Earths begin as planets the size of Neptune with large, puffy atmospheres, which then lose so much mass that all that is left is the rocky core and possibly a thin atmosphere,” France said.  

CUTE’s greatest legacy may be its impact on students, he said. The mission’s small team of about 20 people were involved in almost every aspect of the spacecraft’s life—from building the satellite to launching it, sending it commands, then downloading and analyzing scientific data. CUTE is currently orbiting about 326 miles (525 kilometers) above Earth’s surface, and is expected to reenter the atmosphere by 2027. 

“All of these things are what happens on big NASA missions, just on a much larger scale,” France said. “Our students and early career scientists are getting the full experience from the proposal stage all the way to getting out the science product.”

NASA: some icy exoplanets may have habitable oceans and geysers

Peer-Reviewed Publication

NASA/GODDARD SPACE FLIGHT CENTER

Enceladus plumes 

IMAGE: 

NASA’S CASSINI SPACECRAFT CAPTURED THIS IMAGE OF ENCELADUS ON NOV. 30, 2010. THE SHADOW OF THE BODY OF ENCELADUS ON THE LOWER PORTIONS OF THE JETS IS CLEARLY VISIBLE.

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CREDIT: NASA/JPL-CALTECH/SPACE SCIENCE INSTITUTE




A NASA study expands the search for life beyond our solar system by indicating that 17 exoplanets (worlds outside our solar system) could have oceans of liquid water, an essential ingredient for life, beneath icy shells. Water from these oceans could occasionally erupt through the ice crust as geysers. The science team calculated the amount of geyser activity on these exoplanets, the first time these estimates have been made. They identified two exoplanets sufficiently close where signs of these eruptions could be observed with telescopes.

The search for life elsewhere in the Universe typically focuses on exoplanets that are in a star’s “habitable zone,” a distance where temperatures allow liquid water to persist on their surfaces. However, it’s possible for an exoplanet that’s too distant and cold to still have an ocean underneath an ice crust if it has enough internal heating. Such is the case in our solar system where Europa, a moon of Jupiter, and Enceladus, a moon of Saturn, have subsurface oceans because they are heated by tides from the gravitational pull of the host planet and neighboring moons.

These subsurface oceans could harbor life if they have other necessities, such as an energy supply as well as elements and compounds used in biological molecules. On Earth, entire ecosystems thrive in complete darkness at the bottom of oceans near hydrothermal vents, which provide energy and nutrients.

“Our analyses predict that these 17 worlds may have ice-covered surfaces but receive enough internal heating from the decay of radioactive elements and tidal forces from their host stars to maintain internal oceans,” said Dr. Lynnae Quick of NASA’s Goddard Space Flight Center in Greenbelt, Maryland. “Thanks to the amount of internal heating they experience, all planets in our study could also exhibit cryovolcanic eruptions in the form of geyser-like plumes.” Quick is lead author of a paper on the research published on October 4 in the Astrophysical Journal.

The team considered conditions on 17 confirmed exoplanets that are roughly Earth-sized but less dense, suggesting that they could have substantial amounts of ice and water instead of denser rock. Although the planets’ exact compositions remain unknown, initial estimates of their surface temperatures from previous studies all indicate that they are much colder than Earth, suggesting that their surfaces could be covered in ice.

The study improved estimates of each exoplanet’s surface temperature by recalculating using the known surface brightness and other properties of Europa and Enceladus as models. The team also estimated the total internal heating in these exoplanets by using the shape of each exoplanet’s orbit to get the heat generated from tides and adding it to the heat expected from radioactive activity. Surface temperature and total heating estimates gave the ice layer thickness for each exoplanet since the oceans cool and freeze at the surface while being heated from the interior. Finally, they compared these figures to Europa’s and used estimated levels of geyser activity on Europa as a conservative baseline to estimate geyser activity on the exoplanets.

They predict that surface temperatures are colder than previous estimates by up to 60 degrees Fahrenheit (16 degrees Celsius). Estimated ice shell thickness ranged from about 190 feet (58 meters) for Proxima Centauri b and one mile (1.6 kilometers) for LHS 1140 b to 24 miles (38.6 kilometers) for MOA 2007 BLG 192Lb, compared to Europa’s estimated average of 18 miles (almost 29 kilometers). Estimated geyser activity went from just 17.6 pounds per second (about 8 kilograms/second) for Kepler 441b to 639,640 pounds/second (290,000 kilograms/second) for LHS 1140b and 13.2 million pounds/second (six million kilograms/second) for Proxima Centauri b, compared to Europa at 4,400 pounds/second (2,000 kilograms/second).

“Since our models predict that oceans could be found relatively close to the surfaces of Proxima Centauri b and LHS 1140 b, and their rate of geyser activity could exceed Europa's by hundreds to thousands of times, telescopes are most likely to detect geological activity on these planets,” said Quick, who is presenting this research December 12 at the American Geophysical Union meeting in San Francisco, California.

This activity could be seen when the exoplanet passes in front of its star. Certain colors of starlight could be dimmed or blocked by water vapor from the geysers. “Sporadic detections of water vapor in which the amount of water vapor detected varies with time, would suggest the presence of cryovolcanic eruptions,” said Quick. The water might contain other elements and compounds that could reveal if it can support life. Since elements and compounds absorb light at specific “signature” colors, analysis of the starlight would let scientists determine the geyser’s composition and evaluate the exoplanet’s habitability potential.

For planets like Proxima Centauri b that don’t cross their stars from our vantage point, geyser activity could be detected by powerful telescopes that are able to measure light that the exoplanet reflects while orbiting its star. Geysers would expel icy particles at the exoplanet’s surface which would cause the exoplanet to appear very bright and reflective.

The research was funded by NASA’s Habitable Worlds Program, the University of Washington's Astrobiology Program, and the Virtual Planetary Laboratory, a member of the NASA Nexus for Exoplanet System Science coordination group.


 

“Energy droughts” in wind and solar can last nearly a week, research shows


Understanding the risk of compound energy droughts—times when the sun doesn’t shine and the wind doesn’t blow—will help grid planners understand where energy storage is needed most


Peer-Reviewed Publication

DOE/PACIFIC NORTHWEST NATIONAL LABORATORY

Solar panels 

IMAGE: 

SOLAR PANELS UNDER A CLOUDY SKY.

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CREDIT: MARK STEBNICKI




Solar and wind power may be free, renewable fuels, but they also depend on natural processes that humans cannot control. It’s one thing to acknowledge the risks that come with renewable energy: the sun doesn’t always shine and the wind doesn’t always blow, but what happens when the grid loses both of these energy sources at the same time?

This phenomenon is known as a compound energy drought. In a new paper, researchers at Pacific Northwest National Laboratory (PNNL) found that in some parts of the country, these energy droughts can last nearly a week.

“When we have a completely decarbonized grid and depend heavily on solar and wind, energy droughts could have huge amounts of impact on the grid,” said Cameron Bracken, an Earth scientist at PNNL and lead author on the paper. Grid operators need to know when energy droughts will occur so they can prepare to pull energy from different sources. On top of that, understanding where, when, and for how long energy droughts occur will help experts manage grid-level battery systems that can store enough electricity to deploy during times when energy is needed most.

The team published the findings October 31 in the journal Renewable Energy and will be presenting at this week’s annual meeting of the American Geophysical Union.

Hunting for cloudy, windless days

In the past, researchers studied compound energy droughts on a state or regional scale. But not much has been studied on a nationwide scale. To find out more about the risk of energy droughts over the entire continental U.S., the researchers dug into weather data and then used historical energy demand data to understand how often an energy drought occurs when that energy is needed the most.

The team examined 4 decades of hourly weather data for the continental U.S. and homed in on geographical areas where actual solar and wind energy plants operate today. Weather data included wind speeds at the height of wind turbines as well as the intensity of solar energy falling on solar panels. Times when the weather data showed stagnant air and cloudy skies translated into lower energy generation from the wind and solar plants—a compound energy drought.

“We essentially took a snapshot of the infrastructure as of 2020 and ran it through the 40 years of weather data, starting in 1980,” Bracken said. “We are basically saying ‘here is how the current infrastructure would have performed under historical weather conditions.’”

The researchers found that energy droughts can occur in any season across the continental U.S., though they vary widely in frequency and duration. In California, for instance, cloudy and windless conditions might last several days, whereas the same conditions might last for only a few hours in Texas. Utah, Colorado, and Kansas experience frequent energy droughts both over several-hour timescales as well as several-day timescales. The Pacific Northwest and Northeast, meanwhile, seem to experience energy droughts that last several hours more frequently than several days. The different timescales (hourly versus daily) will help inform the energy drought’s impact on the grid—will it last just a few hours, or several days?

Overall, researchers found that the longest potential compound energy drought on an hourly timescale was 37 hours (in Texas), while the longest energy drought on a daily timescale was six days (in California).

Energy drought at peak demand

Simply knowing the where and how of energy droughts is just one piece of the puzzle, Bracken said. He also stressed that a drought of solar and wind power won’t necessarily cause an energy shortage. Grid operators can turn to other sources of energy like hydropower, fossil fuels, or energy transmitted from other regions in the U.S.

But as the nation aims to move away from fossil fuels and rely more on solar and wind power, grid operators must understand whether energy droughts will occur during times when the demand for electricity might exceed supply. Climate change brings hotter summers and more intense winter storms, and these are times when not only people use more energy to stay safe (for cooling or heating), but access to electricity might mean life or death.

To understand the possible connection between energy droughts and energy demand, the team mapped their historical, hypothetical generation data onto 40 years of historical energy demand data that also covered real power plants across the continent.

The data showed that “wind and solar droughts happen during peak demand events more than you would expect due to chance,” Bracken said, meaning that more often than not, windless and cloudless periods occurred during times when demand for power was high. For now, Bracken isn’t certain that the correlation means causation.

“This could be due to well-understood meteorological phenomenon such as inversions suppressing wind and increasing temperatures, but further study is needed,” Bracken said.

Energy storage for energy droughts

Studying patterns in the frequency and duration of energy droughts will also help inform the deployment of long-duration energy storage projects, said Nathalie Voisin, an Earth scientist at PNNL and coauthor on the paper. The paper is the first to provide a uniform standard of what a compound energy drought is and how long it can last in different parts of the country.

“We’re providing insight on how to adequately design and manage multi-day storage. So when you know an energy drought is going to last for five hours or five days, you can incentivize storage to be managed accordingly,” Voisin said.

Next, Bracken and the team will extrapolate weather and demand data into the future to see how climate change will affect the frequency and duration of energy droughts. The team plans to model energy droughts all the way to the end of the century combined with evolving infrastructure.

This research was funded by PNNL through its internal GODEEEP initiative.

  

Workplace gossip can benefit employees and employers


Binghamton University School of Management doctoral student's research explores how workplace gossip can help employees, improve an organization's effectiveness

Peer-Reviewed Publication

BINGHAMTON UNIVERSITY

Illustration of office workers 

IMAGE: 

SME WORKPLACE GOSSIP COULD REDUCE THE LIKELIHOOD OF EMPLOYEE TURNOVER AND, AS A RESULT, POTENTIALLY BOOST AN ORGANIZATION’S EFFECTIVENESS, ACCORDING TO NEW RESEARCH FROM BINGHAMTON UNIVERSITY.

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CREDIT: BINGHAMTON UNIVERSITY, STATE UNIVERSITY OF NEW YORK




BINGHAMTON, N.Y. -- New research from Binghamton University, State University of New York shows how some workplace gossip could reduce the likelihood of employee turnover and, as a result, potentially boost an organization’s effectiveness.

“Organizations should be aware of the impact of positive gossip because turnover can be a very important factor in dictating an organization’s success,” said Jinhee Moon, a doctoral student at the Binghamton University School of Management who conducted the study with a team of other researchers. “To make employees participate in positive gossip, the organization should do the right things by treating their employees well, and being aware their behaviors can show they care about their employees.”

While studies linked to workplace gossip aren’t new, Moon’s work builds upon previous research by exploring how employees who gossip might experience social gains. Moon previously worked on a study that dealt with why people participate in gossipy behavior at their workplace, and the recent publication is connected to her own leadership research focus at SOM, which centers on interpersonal relationships and social networks.

For the recent study, Moon and fellow researchers surveyed 338 health workers in South Korea on positive and negative forms of workplace gossip related to their organizations and management. Some of the topics included:

  • “At work, I sometimes complain about my organization when management is absent.”
  • “If I feel treated badly by management, I talk about this to my colleagues.”
  • “I sometimes praise my organization’s capability when the management is absent.”

Moon said the research showed gossip is viewed as more valuable when people positively talk about their management or organization. Health workers who participated in the survey expressed more interest in information they could use to enhance or maintain their organizational status.

The study also indicated no relationship between negative gossip and coercive power in the workplace, which Moon said proved contrary to what researchers had expected.

“We expected that if you participate in negative gossip, maybe you’re trying to appear powerful or controlling or want to ‘beat someone up,’ but we couldn’t find any supportive results,” Moon said. “If anything, we found that people didn’t value that type of gossip as information and just saw it as someone who wants to complain. So, if you’re thinking about negative workplace gossip, you might want to save your time because there’s no positive impact for you.”

But one of the most helpful aspects of the research, as Moon saw it, was how it highlighted that participating in positive gossip among one’s coworkers could reduce the chances of voluntary employee turnover.

“It can be very hard just to quit your job, and if you’re experiencing difficulty where you work, maybe you want to participate in positive gossip with your colleagues and talk about some of the more bearable aspects of the organization,” Moon said. “Eventually, that can help you gain some personal power. It’s a very convenient way to reduce negative feelings toward your own workplace, which can help you more in the long run.”


  


Scientists and space agencies are shooting for the Moon – 5 essential reads on modern luna

The Conversation
December 12, 2023 

Full Moon (Shutterstock)

The year 2023 proved a big one for lunar science. India’s Chandrayaan-3 spacecraft landed near the south pole of the Moon, a huge accomplishment for a country relatively new to the space scene, especially after its Chandrayaan-2 craft crashed in 2019.

At the same time, NASA’s been gearing up for a host of Moon-related missions, including its Artemis program. In 2023, the agency gained nine signatories to the Artemis Accords, an international agreement for peaceful space exploration, for a total of 32 countries that have signed so far.

As Georgia Tech’s Mariel Borowitz explains, the U.S. now has widespread bipartisan political support for spacefaring – for the first time since the 1970s – and returning missions to the Moon is the first natural target.

Here are five stories that The Conversation U.S. has published over the past year about lunar exploration, including why people want to go back to the Moon, what Chandrayaan-3 found during its initial foray across the lunar surface and the ever-growing problem of lunar space junk.

1. Why shoot for the Moon?


Missions to the Moon hold potential benefits for a variety of sectors, including commercial, military and geopolitical.

“Ever since humans last left the Moon in 1972, many have dreamed about the days when people would return. But for decades, these efforts have hit political roadblocks,” wrote Borowitz. “This time, the United States’ plans to return to the Moon are likely to succeed – it has the cross-sector support and the strategic importance to ensure continuity, even during politically challenging times.”

NASA is planning to return to the Moon with Artemis missions. This video describes where on the Moon it may land and how it will decide.

While some of these potential uses are incredibly far off – from mining the Moon for resources to sending out military satellites to orbit around the Moon – missions to the Moon in the near term will help inform scientists and stakeholders of future possibilities.

2. Searching for sulfur

India’s Chandrayaan-3 lander touched down on the Moon’s surface, just a few miles away from the lunar south pole, in late August 2023.

Its rover, called Pragyan, took measurements of the lunar surface and found the soil near the south pole contains a surprise – sulfur.



India’s lunar rover Pragyan rolls out of the lander and onto the surface.

As Jeffrey Gillis-Davis, a physicist at Washington University in St. Louis, wrote, future Moon missions or a future Moon base could use lunar sulfur as an ingredient in everything from fuel and fertilizer to concrete.

3. Water in ice

But sulfur’s not the only resource the lunar south pole could have to offer. For several years, scientists have predicted that the lunar south pole might have water in the form of ice. And Chandrayaan-3’s sulfur discovery gives scientists more insight into how and how recently ice might have formed on the surface.

Comets or volcanic activity could have brought water to the Moon years ago. If volcanic activity is the culprit for water’s appearance, scientists would also expect to see sulfur in higher levels, wrote Paul Hayne, an assistant professor of astrophysical and planetary sciences at the University of Colorado Boulder.

A host of future missions to the Moon, including NASA’s VIPER mission planned for 2024, will continue to investigate where ice could be hiding on the Moon.

4. Moon debris

With all the Moon missions, both current and upcoming, some experts have raised concerns about the increased space junk in the “cislunar space” – or the space between Earth and the Moon and around the Moon.

NASA doesn’t currently track the space junk left behind from its missions, and this lack of oversight has many people worried.


A team of students and professors at the University of Arizona built a telescope to track objects near the Moon.
 Vishnu Reddy/University of Arizona, CC BY-ND

One team at the University of Arizona has started building a catalog of debris left in this space. Team members started off by identifying a few large objects, and as their methods got better, they were able to see objects as small as a cereal box. The team hopes this work will one day improve the sustainability of future lunar missions.

“While there is still a long way to go, these efforts are designed to ultimately form the basis for a catalog that will help lead to safer, more sustainable use of cislunar orbital space as humanity begins its expansion off of the Earth,” writes Vishnu Reddy, a professor of planetary science at the University of Arizona.


5. Future flyers

Early this year, NASA announced who will make up the crew of their Artemis II mission. Set for late 2024, Artemis II will fly by the Moon and test the technology and equipment planned for use in future missions. It will also mark the first time people are close to the lunar surface in over 50 years.


Crew members of the Artemis II mission are NASA astronauts Christina Hammock Koch, Reid Wiseman and Victor Glover and Canadian Space Agency astronaut Jeremy Hansen. NASA


Three of the four crew members have spent time in space, with the fourth having spent lots of time in spaceflight simulations. Each started their careers as a military pilot, just like all the astronauts of the Apollo missions. But this crew represents more racial and gender diversity than the astronauts of the Apollo era.

“Unlike the Apollo program of the 1960s and 1970s, with Artemis, NASA has placed a heavy emphasis on building a politically sustainable lunar program by fostering the participation of a diverse group of people and countries,” wrote Wendy Whitman Cobb, a professor of strategy and security studies at Air University.

This story is a roundup of articles from The Conversation’s archives.

Mary Magnuson, Assistant Science Editor, The Conversation

This article is republished from The Conversation under a Creative Commons license. Read the original article.
Blue Origin announces space launch next week, first since 2022 crash

Agence France-Presse
December 13, 2023 

The VTVL (vertical-takeoff, vertical-landing) booster New Shepard from the Blue Origin company during landing. 
Blue Origin/dpa

Blue Origin said on Tuesday it was aiming to launch its New Shepard suborbital rocket next week, the first mission since an uncrewed crash in September 2022 set back the space company owned by billionaire Jeff Bezos.

"We're targeting a launch window that opens on Dec. 18 for our next New Shepard payload mission," the company tweeted on X, adding the flight would contain 33 science and research payloads, as well as 38,000 postcards.

But the launch first needs to be cleared by the Federal Aviation Administration (FAA), which said in a statement to AFP it is "continuing to work on outstanding items related to the license modification application." A Blue Origin spokesperson said "we expect to receive approval."

In September the FAA announced it had closed its probe into last year's crash, ordering the company to carry out 21 corrective actions before it could resume launches.

The report said failure of an engine nozzle caused by higher-than-expected engine operating temperatures caused the New Shepard rocket to fall back to the ground shortly after liftoff, even as the capsule carrying research experiments escaped and floated safely back to Earth.

"During the mishap the onboard launch vehicle systems detected the anomaly, triggered an abort and separation of the capsule from the propulsion module as intended and shut down the engine," said the FAA.

The fact the capsule ejected right away was viewed positively, suggesting that any crew would have been safe if they had been aboard.

In all, Blue Origin has flown six crewed flights -- some passengers were paying customers and others flew as guests -- since July 2021, when Bezos himself took part in the first flight.

While Blue Origin has been grounded, rival Virgin Galactic, the company founded by British billionaire Richard Branson, has pressed on, flying five commercial flights this year.

The two companies compete in the emerging space tourism sector, offering a few minutes of weightlessness in "suborbital" space.

While Blue Origin launches a small rocket vertically, Virgin Galactic uses a large carrier plane to gain altitude and then drop off a smaller rocket-powered spaceplane that completes the journey to space.

Virgin Galactic tickets were sold for between $200,000-$450,000, while Blue Origin doesn't disclose its ticket prices publicly.