Daily Archives: March 27, 2022

Large study challenges the theory that light alcohol consumption benefits heart health – EurekAlert

Posted: March 27, 2022 at 10:27 pm

BOSTON Observational research has suggested that light alcohol consumption may provide heart-related health benefits, but in a large study published in JAMA Network Open, alcohol intake at all levels was linked with higher risks of cardiovascular disease. The findings, which are published by a team led by researchers at Massachusetts General Hospital (MGH) and the Broad Institute of MIT and Harvard, suggest that the supposed benefits of alcohol consumption may actually be attributed to other lifestyle factors that are common among light to moderate drinkers.

The study included 371,463 adultswith an average age of 57 years and an average alcohol consumption of 9.2 drinks per weekwho were participants in the UK Biobank, a large-scale biomedical database and research resource containing in-depth genetic and health information. Consistent with earlier studies, investigators found that light to moderate drinkers had the lowest heart disease risk, followed by people who abstained from drinking. People who drank heavily had the highest risk. However, the team also found that light to moderate drinkers tended to have healthier lifestyles than abstainerssuch as more physical activity and vegetable intake, and less smoking. Taking just a few lifestyle factors into account significantly lowered any benefit associated with alcohol consumption.

The study also applied the latest techniques in a method called Mendelian randomization, which uses genetic variants to determine whether an observed link between an exposure and an outcome is consistent with a causal effectin this case, whether light alcohol consumption causes a person to be protected against cardiovascular disease. Newer and more advanced techniques in non-linear Mendelian randomization now permit the use of human genetic data to evaluate the direction and magnitude of disease risk associated with different levels of an exposure, says senior author Krishna G. Aragam, MD, MS, a cardiologist at MGH and an associate scientist at the Broad Institute. We therefore leveraged these new techniques and expansive genetic and phenotypic data from biobank populations to better understand the association between habitual alcohol intake and cardiovascular disease.

When the scientists conducted such genetic analyses of samples taken from participants, they found that individuals with genetic variants that predicted higher alcohol consumption were indeed more likely to consume greater amounts of alcohol, and more likely to have hypertension and coronary artery disease. The analyses also revealed substantial differences in cardiovascular risk across the spectrum of alcohol consumption among both men and women, with minimal increases in risk when going from zero to seven drinks per week, much higher risk increases when progressing from seven to 14 drinks per week, and especially high risk when consuming 21 or more drinks per week. Notably, the findings suggest a rise in cardiovascular risk even at levels deemed low risk by national guidelines from the U.S. Department of Agriculture (i.e. below two drinks per day for men and one drink per day for women).

The discovery that the relationship between alcohol intake and cardiovascular risk is not a linear one but rather an exponential one was supported by an additional analysis of data on 30,716 participants in the Mass General Brigham Biobank. Therefore, while cutting back on consumption can benefit even people who drink one alcoholic beverage per day, the health gains of cutting back may be more substantial and, perhaps, more clinically meaningful in those who consume more.

The findings affirm that alcohol intake should not be recommended to improve cardiovascular health; rather, that reducing alcohol intake will likely reduce cardiovascular risk in all individuals, albeit to different extents based on ones current level of consumption, says Aragam.

The studys lead author was Kiran J. Biddinger, and additional authors included Connor A. Emdin, MD, DPhil, Mary E. Haas, PhD, Minxian Wang, PhD, George Hindy, MD, Patrick T. Ellinor, MD, PhD, Sekar Kathiresan, MD, and Amit V. Khera, MD, MSc.

Funding was provided by the National Institutes of Health and the American Heart Association.

About the Massachusetts General HospitalMassachusetts General Hospital, founded in 1811, is the original and largest teaching hospital of Harvard Medical School. The Mass General Research Instituteconducts the largest hospital-based research program in the nation, with annual research operations of more than $1 billion and comprises more than 9,500 researchers working across more than 30 institutes, centers and departments. In August 2021, Mass General was named #5 in theU.S. News & World Reportlist of "Americas Best Hospitals."

JAMA Network Open

Data/statistical analysis

People

Association of Habitual Alcohol Intake With Risk of Cardiovascular Disease

25-Mar-2022

Dr Haas reported receiving personal fees and stock and stock options from Regeneron Pharmaceuticals outside the submitted work. Dr Ellinor reported receiving grants from Bayer AG and IBM Health and personal fees from Bayer AG, MyoKardia, Quest Diagnostics, and Novartis during the conduct of the study. Dr Kathiresan reported being an employee of Verve Therapeutics; owning equity in Verve Therapeutics, Maze Therapeutics, Color Health, and Medgenome; receiving personal fees from Medgenome and Color Health; serving on the advisory boards for Regeneron Genetics Center and Corvidia Therapeutics; and consulting for Acceleron, Eli Lilly and Co, Novartis, Merck, Novo Nordisk, Novo Ventures, Ionis, Alnylam, Aegerion, Haug Partners, Noble Insights, Leerink Partners, Bayer Healthcare, Illumina, Color Genomics, MedGenome, Quest Diagnostics, and Medscape outside the submitted work. Dr Khera reported receiving personal fees from Merck, Amarin Pharmaceuticals, Amgen, Maze Therapeutics, Navitor Pharmaceuticals, Sarepta Therapeutics, Verve Therapeutics, Silence Therapeutics, Veritas International, Color Health, and Third Rock Ventures and receiving grants from IBM Research outside the submitted work. Dr Aragam reported receiving speaking fees from the Novartis Institute for Biomedical Research. No other disclosures were reported.

Disclaimer: AAAS and EurekAlert! are not responsible for the accuracy of news releases posted to EurekAlert! by contributing institutions or for the use of any information through the EurekAlert system.

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Detailed Cell Atlas of the Fallopian Tube Created – Technology Networks

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The fallopian tube is the site of fertilization, where once a month for the duration of a females post-pubescent, pre-menopausal life, an egg is moved from the ovary, ready for fertilization by a sperm cell.

A new study from Michigan Medicine researchers creates a detailed "atlas" of the various cell types and their gene activities within the highly specialized fallopian tube, paving the way for new research into infertility and other diseases affecting this organ, including some cancers.

Using tissue samples from four premenopausal women,Saher Sue Hammoud, Ph.D., andJun Li, Ph.D.from the Department of Human Genetics led a team at U-M to analyze almost 60,000 cells by single-cell RNA sequencing. They used the data to characterize the diversity of cells that make up the fallopian tube, including both the lining of the tube (the epithelium) and the deeper stromal layer, consisting of immune, blood, muscle, and other cells.

Hammoud and Li are joined byAriella Shikanov, Ph.D.,of the Department of Biomedical Engineering,Erica Marsh, M.D.,of the Department of Obstetrics and Gynecology, and team membersNicole Ulrich, M.D.,Yu-chi Shen, Ph.D., andQianyi Ma, Ph.D.Their project is part of the Human Cell Atlas Seed Networks, an international effort supported by the Chan-Zuckerberg Initiative to map all cells in the human body as a resource for better understanding health and disease.

Prior to their work, it was known that there are about four epithelial cell types in the fallopian tube, said Hammoud. We were able to reveal a deeper level of heterogeneity within these cells.

Specifically, they identified 10 epithelial cell subtypes, including four of the finger-like ciliated cells responsible for moving the egg through the fallopian tubes three sections before and after fertilization.

The cells within the fallopian tube are ever changing, replenishing themselves over time and varying in number depending on a womans age, hormones, menstrual cycle, and in the presence of disease. By comparing cells from women with healthy fallopian tubes to two samples from women with a fallopian tube disease known as hydrosalpinx (conventionally known as a blocked fallopian tube), the researchers were able to pinpoint which cells increased in number, and which changed characteristics, such as a high degree of inflammation.

Some of the cells are the cause of the disease state, and some others are the consequence; and now we know the patterns for individual cell types to figure out the molecular reasons for that pathology, commented Li.

The team also found that some of the cell subtypes they defined in the fallopian tube may function as precursor cells, those that can regenerate multiple cell types in response to normal tissue turnover, or for repairing a damage.

One of the most surprising findings of the study, says Hammoud, was the discovery of cells with markers for epithelial-mesenchymal transition, also known as EMT, a process not previously associated with the fallopian tube, through which a cell can, under certain circumstances, become cancerous.

Ovarian cancer, it turns out, may be a misnomer. The new study adds to accumulating evidence that the root of ovarian cancerthe fifth leading cause of cancer death in womenmay originate within the adjacent fallopian tube.

The EMT process seems to be tightly regulated in the pre-menopausal woman, she said. One possible connection to cancer is that when there is misregulation in this population of cells in some unfortunate individuals, they may develop ovarian cancer. With EMT cells in the fallopian tube, you do have the predisposition right there.

Additional insights came from the fallopian tube cells from women with hydrosalpinx, specifically, that the disease may lead to a type of scarring called fibrosis. The implication is that for women who dont want to have their tubes removed, you could think about treating them with anti-fibrotic drugs such as the ones used to treat lung fibrosis as a way to save their tubes during reproductive age, noted Hammoud.

Compared to past efforts, the study provides much more detailed information about cell types and functions in the tube for researchers interested in a host of questions about the normal female reproductive system. This really is a basecamp to launch future studies, says Li, including ones that look at the effects of age, the menstrual cycle, hormone therapy, and ancestral background on cellular diversity and disease pathology.

Reference:Ulrich ND, Shen Y chi, Ma Q, et al. Cellular heterogeneity of human fallopian tubes in normal and hydrosalpinx disease states identified by scRNA-seq. Dev. Cell. 2021. doi: 10.1101/2021.09.16.460628

This article has been republished from the following materials. Note: material may have been edited for length and content. For further information, please contact the cited source.

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Antibodies From COVID Infection Shield Kids for Up to 7 Months – HealthDay News

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TUESDAY, March 22, 2022 (HealthDay News) -- Antibodies from a COVID-19 infection linger in most children for up to seven months, even if they had no symptoms, a new study finds.

To come to that reassuring conclusion, researchers analyzed data from 218 children in Texas, ages 5 to 19, who were enrolled in an ongoing survey launched in October 2020 to track COVID-19 antibody status in children and adults over time.

Blood samples were collected from participants before vaccines became available and during the surges of the Delta and Omicron variants.

While 96% of children who were infected with COVID-19 still had antibodies at least six months later, 58% did not have infection-triggered antibodies at their third and final blood test.

The report, published March 18 in the journal Pediatrics, did not assess the impact of vaccination.

"This is the first study from the Texas CARES survey that includes data from all three time points in the survey," said corresponding author Sarah Messiah. She is a professor of epidemiology, human genetics and environmental sciences at the University of Texas Health Science Center at Houston.

"These findings are important because the information we collected from children infected with COVID-19 didn't differ at all by whether a child was asymptomatic, severity of symptoms, when they had the virus, were at a healthy weight or had obesity, or by gender," she added in a university news release. "It was the same for everyone."

To date, 14 million children in the United States have tested positive for the virus, and these findings help improve understanding of how it affects children, according to Messiah.

"Adult literature shows us that natural infection, plus the vaccine-induced protection, gives you the best defense against COVID-19. There has been a misunderstanding from some parents who think just because their child has had COVID-19, they are now protected and don't need to get the vaccine," Messiah said.

"While our study is encouraging in that some amount [of] natural antibodies last at least six months in children, we still don't know the absolute protection threshold," she added. "We have a great tool available to give children additional protection by getting their vaccine, so if your child is eligible, take advantage of it."

More information

For more on children and COVID-19, go to the American Academy of Pediatrics.

SOURCE: University of Texas Health Science Center at Houston, news release, March 18, 2022

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The Save Women’s Sports Act The Edgefield Advertiser – Edgefieldadvertiser

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All writers in Op Ed are here to inform and acknowledge issues of importance to our communities, however these writings represent the views and opinions of the authors and not necessarily of The Advertiser.

Robert Scott

Back in January,I wrote an OpEd about gender prejudice, and howone office holder expressed suchprejudice against transgender women in general and, specifically, prejudice regarding thethen-current Jeopardy champion,Amy Schneider.A discussion following that OpEdindicated thisprejudicewasbased ona generaldisbelief thatbeingtransgenderwas a medical and physical condition rather than a hoax or a so-called woke perception of something that was in fact not real.

We live in a complex world, and as our knowledge of human genetics and psychology increases,that complexity manifests itself ina number ofways. The validity of the transgender condition among some of our fellow human beings is one such complexity that is widely misunderstood,and thereforeit isnot yet accepted by many Americans. Our country has expanded its initial announced basis of liberty and freedom from All men are created equal as stated in the Declaration of Independence to include not just white men (as it wasgenerallyunderstood to mean in 1776) butallmenregardless of race, creed, or national origin;then, after generations of discussion,all men and women. We are struggling now to expand this to include all people, as evolving Science brings us into the knowledge that genderdoes not entirely fall into the binary categories we once thought. All people, we should now acknowledge, are not only created equal but are entitled to equal treatment as part of their inherent right to the pursuit of happiness.

SomeAmericans, including unfortunately some who represent us not only in Congress but in our State Legislature, continue to reject that notion. The latest manifestation of the gender prejudice inherent in such a rejection is a bill currently before the South Carolina Legislature entitled the Save Womens Sports Act.It should be voted down again (itfailed to be enacted last session), and here is why.The announced premise sounds reasonable enough: to require student athletes between grades 6 and 12 to compete in team sports based on the sex they were assigned at birth. Gender prejudice hides in the word assigned. The vast majority ofthefellow members ofourspecies are, indeed, fully male or fully female. But science is learning that for some small number, this is not the case. Some of them are inherently transgender havingimportantphysical and/or psychological traits appropriate to the gender opposite to that initial assignment, which really means assignment by our society based on an initialexternalassessment of just their plumbing.

If we recognize transgender youth as being who theyreallyare, even when they areonlyin grades 6 through 12, would that not compromise team sports, in particular by allowing some girls who were initially (and wrongly) assigned as males to play?Wouldnt suchchildrenhave an unfair advantage? The short answer isadvantage perhaps yes,but unfair advantageno not anymore than allowing exceptionally tall girls (or boys) toplay basketball despite being taller than anybody else, particularly anybody else in their school grade. If their pursuit of happiness includes trying out for a team and, if they are good enough, making that team, then we need to recognize and honor that. To do otherwise does not Save anybodys sports. It sets up a fundamental fairness issue thatis even more important to teach our children: in the United States of America, we assure to all people the unalienable rights to life, to liberty, and to the pursuit of happiness.Even transgender people.

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India needs more world-class telescopes to do competitive research in Astronomy: Anupama – The Indian Express

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G C ANUPAMA, president, Astronomical Society of India (ASI), Saturday said India needs more observational facilities and telescopes in order to do competitive research at par with the global community.

She was delivering the presidential address at the 40th ASI meet hosted at IIT-Roorkee and jointly organised with Aryabhatta Research Institute of Observational Sciences (ARIES), Nainital.

India is lagging in observational facilities, thus making us dependent for data on other (global) facilities. This is not a happy situation. India needs to improve the observational facilities and have access to multi-wavelength and multi-messenger facilities, said Anupama. The Giant Metrewave Radio Telescope in Pune, she said, remains among the few world-class facilities available in India. Apart from some telescope facilities working between the 1 metre to 4 metre class, India otherwise does not have telescopes in the optical and infra-red spectra that function in ranges between the 8 metre to 10 metre class for doing competitive science, she said.

According to Anupama, Astronomy, over the recent decades, has grown with a lot of synergy present now in doing science. With Indias participation in the mega science projects like the Thirty Metre Telescope, Laser Interferometer Gravitational Wave Observatory and the Square Kilometre Array projects, a stronger astronomy community was required.

India with a unique longitudinal positioning and places like Ladakh hold promising locations to set up suitable telescopes in future, proposals for which are under consideration, she said. We need to expand also to the submillimetre region the area of star formation. There is a need to upgrade and network the existing telescope facilities with the global ones, especially for studying transient objects, she said.Earlier in the day, the ASI 2022 was formally inaugurated by Professor K Vijay Raghavan, Principal Scientific Adviser to the Government of India. I urge the Indian astronomy community to plan forward-looking and futuristic research plans which will help India make significant contribution in global mega science projects, he said.

In his virtual address, he further elaborated on artificial intelligence (AI) and machine learning (ML) and their growing uses.

Anupama talked about the current areas of research and mentioned that Astronomy was among the top areas included in the Mega Science Vision Document 2035, an effort led by the office of Principal Scientific Advisor. This document will be a roadmap for deciding future course of research covering nuclear science, high energy physics, astronomy and astrophysics, accelerator-based science and technology and climate research, ecology and environment.

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April 8 Star Gaze with Oakland Astronomy Club in Oakland Twp. Oakland County Times – Oakland County Times

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April 8 Star Gaze with Oakland Astronomy Club in Oakland Twp.

April 8 Star Gaze with Oakland Astronomy Club in Oakland Twp.

Share safe telescopic views of the Winter night sky with the Oakland Astronomy Club. See details of lunar craters and the colorful gases of the star nursery in Orion. Find the Big Dipper and Leo the Lion and enjoy the colorful stars of the Winter sky before they disappear for the season!

April 8th, 8-9:30 for adults to teens, at Marsh View Park,3100 E Clarkston Rd, Oakland, MI 48363. Register online at: https://oaklandtownship.recdesk.com/Community/Program/Detail?programId=677

April 9th, 8-9:30 for star gazers of all ages, at Independence Oaks County Park, 501 Sashabaw Rd., Clarkston, MI 48348. Register via phone with Oakland County Parks during weekday business hours at248-858-0916.

More info: http://oaklandastronomy.net/event.html

For more things to do, visit the Oakland County Times Event Page! To submit event info email editor@oc115.com .

Thank you to Jim Shaffer & Associates Realtors for sponsoring this section!

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Parts of Milky Way are older than expected, astronomers say – FOX 6 Milwaukee

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Basic structure of our home galaxy, edge-on view. The new results from ESA's Gaia mission provide for a reconstruction of the history of the Milky Way, in particular of the evolution of the so-called thick disc. (Stefan Payne-Wardenaar / MPIA via ESA)

Scientists have discovered that parts of the Milky Way galaxy are actually older than previously thought at least by two billion years.

Data collected by the European Space Agencys (ESA) Gaia mission was analyzed by astronomers from the Max-Planck Institute for Astronomy in Heidelberg, Germany, and compared to earlier datasets from Gaias observation of the motion of stars in the outskirts of our galaxy, also known as the anticentre, in 2020.

In addition, astronomers received data from Chinas Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST) for roughly 250,000 stars to derive their ages, according to an agency news release.

Combining this information, astronomers were able to determine that stars within the "thick disc" part of our galaxy began forming 13 billion years ago, around 2 billion years earlier than expected, and just 0.8 billion years after the Big Bang, according to the ESA.

So, our beautiful galaxy is made up of billions of components, but to keep things simple, well narrow it down to the disc and the halo.

If one were to hypothetically look at our galaxy and it laid flat, you would be able to see a bulge in the center of the disc, which is essentially the center of our galaxy.

Surrounding that disc is the stellar halo, which is the outermost part of our galaxy and was originally believed to be the oldest part of the Milky Way, the ESA said.

The halo has a radius of about 100,000 light-years and contains isolated stars as well as many globular clusters, which are basically clusters of millions of stars packed into one area.

The galactic disc is made up of both thick and thin discs. The thin disc, which is about 700 light-years high in comparison to the galactic disc, contains most of the stars we humans can see. Its often photographed as a misty streak across the night sky and dotted with stars.

The thick disc, which is about 3,000 light-years high, contains fewer stars but this is the area where astronomers were able to find their surprising discovery, thanks to Gaia, according to the ESA.

An artists impression of our Milky Way galaxy, a roughly 13 billon-year-old barred spiral galaxy that is home to a few hundred billion stars. (NASA/JPL-Caltech; right: ESA; layout: ESA/ATG medialab)

Determining a stars age is one of the most difficult things to decipher, according to the ESA.

"It cannot be measured directly but must be inferred by comparing a stars characteristics with computer models of stellar evolution. The compositional data helps with this," according to the ESA.

Astronomers must take into account the matter of which a star is made in its early stages which includes hydrogen and helium. Once a star is born, it will continue to develop and create metals within itself. These metals are expelled out into space as a star grows older, according to the ESA.

So, to make a very complicated method easy to understand: The fewer metals a star has, the older it is.

"Together, the brightness and metallicity allow astronomers to extract the stars age from the computer models," the ESA said.

The Milky Way was formed in two phases, according to the ESA.

The first phase was the Big Bang which happened around 0.8 billion years ago, scientists believe.

The aforementioned "thick disk" began to form at this time. Astronomers also believe other parts of the galaxy, such as the inner parts of the stellar halo which basically encircles the entirety of the Milky Way galaxy, began to form as well.

Then, the Gaia-Sausage-Enceladus, which was a dwarf galaxy hurtling through space, collided with the Milky Way and rapidly accelerated the formation of our galaxy, according to Carnegie Mellon University.

This collision gave birth to millions of stars, according to the ESA.

During the second phase of the galaxys formation, a thinner disc developed as all of the space matter began to form together and thats when Earths sun and subsequent planets were formed.

This story was reported out of Los Angeles.

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A new all-abilities accessible observatory in Heathcote is opening up new worlds for Victorians – ABC News

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Growing up, Jesse Stout remembers learning about astronomy from his dad.

"When I was younger my father used to take us out camping and that was probably the first time I was introduced to astronomy," he said.

"We used to look up at the stars and my father used to point out things I'm not too sure how accurate he was."

But a life-changing workplace accident in 2018 saw him rethink how he saw himself, and rediscover an old interest.

"A lot of my hobbies before my accident were very, very active, so camping, going to the beach or surfing," he said.

"The ASV has allowed me to explore my new hobby and be positive about a new element in my life I think that's a very, very hard thing to express when you've got a disability."

Late last year, as he recovered from a second surgery on his back, Jesse's partner and family decided to pool their money to buy him a telescope.

Excited to try it out, Jesse soon discovered having to manoeuvre himself around the equipment came with a very painful drawback, that could leave him in pain for days afterwards.

Looking around for groups to join, he found the Astronomical Society of Victoria's (ASV) Pathways to the Planets project, trying to raise funds to make their sites and equipment more accessible for people with varying levels of mobility.

With around 12 per cent of its members having some sort of disability, ASV Vice president Mark Iscaro said it was stories like Jesse's that inspired them.

"The sky belongs to everyone," he said.

"If there are people who've got sight issues, they should still be able to feel the night sky, whether that's through 3D-printed star maps, and those with mobility issues shouldn't be prevented from coming up and seeing the stars."

Now, in the year of their 100th anniversary, the society has opened an all-abilities accessible observatory at the Leon Mow dark sky site near Heathcote, north of Melbourne, with features such as better-lit and widened pathways, a motorised entry gate and accommodation for those staying overnight.

There are also plans to build remote-controlled astrophotography observatories for people who can't physically travel to the site, or use an eyepiece.

The main attraction is a specially designed telescope, altered to make the eyepiece the axis so it stays at the perfect height for a viewer sitting down.

ASV President Chris Rudge said traditional astronomical equipment wasn't always easy for everyone to use.

"Unfortunately, to use those large telescopes you have to go up a ladder, but this new telescope we've specially built so that you can sit down and look at the night sky," he said.

"We have many older members these days, including myself, who may be mobility-limited, they can just sit down and enjoy the night sky at their leisure."

The telescope is the second in Victoria, with the first being in the regional town of Ballarat.

But the ASV is hoping their larger member base and more widely accessible facilities will attract more keen astronomers in the future.

Jesse was just looking forward to enjoying his hobby pain-free.

"I'll be able to use the telescope and I'll be able to look at the stars and not have to worry about the next day that I'm going to be bedridden because of the pain from bending down or moving around or adjusting my body slightly," he said.

And it has reminded him of what he loves about looking up at the skies.

"There's a huge element of mystery behind astronomy," he said.

"Being able to look up into the sky and realising you're finding something new each time you look and the fact that a telescope can bring you even closer to finding something."

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Bad Astronomy | Spicules on the Sun may be due to Faraday waves | SYFY WIRE – Syfy

Posted: at 10:26 pm

The Sun is literally the closest star to us in the entire Universe, but theres a lot about it thats still pretty mysterious.

For example, nearly 150 years ago, the astronomer Angelo Secchi first observed narrow, towering fingers of material stretching vertically away from the Sun. Called spicules, these can grow to a height of 12,000 kilometers nearly the diameter of the Earth but tend to be only 1/10th that wide. They grow in a matter of minutes, shooting upwards at tens of thousands of kilometers per hour, then collapse back down.

There are millions of spicules on the Sun at any given moment, and they look like grass or shag carpeting. Time-lapse video of them is entrancing and eerie:

And while theyre known to be associated with strong magnetic fields typical of phenomena on the Sun even after all this time its not clear what causes them. Paper after paper has been published over the years, with varying degrees of success in explaining these weird features.

A few years ago, a study showed that they may be due to the way the magnetic field interacts with both electrically neutral and charged particles on the Suns surface. However, a different team of solar astronomers wondered if there might be a more fundamental piece of physics going on with them. They noticed how fluids can dance when vibrated by the sound waves from a speaker heres a good video of that and thought there might be a connection. When the surface of a fluid is vibrated you can get neat patterns in it as waves get pumped up by them, but as the frequency gets higher theres a critical frequency when the surface starts to create jets of water shooting up. This type of motion is called Faraday excitation or Faraday waves. Usually in water or other liquids the top of the jet breaks off into a droplet that then falls back to the surface.

This type of event is common in nature; in fact alligators use a low-frequency mating call that can cause it to happen in the water around them, shown in this video about 20 seconds in.

The Suns surface is a plasma, mostly hydrogen thats so hot the atoms have lost an electron, and is dense enough to act like a fluid. Also, there are plenty of sources of vibrations in the solar surface. Deep inside the Sun theres a layer where extremely hot material rises buoyantly, and when it gets to the surface it cools and falls back down. This is called convection, and there are many towering convective conveyor belts transporting material up and down in the Sun. This causes a continuous rumble on the surface at a frequency that could excite Faraday waves.

The new research [link to paper] first shows that the physics of Faraday waves in the Sun and in a fluid dancing on a speaker are similar. They then experimented in the lab with various fluids to see if they could mimic spicules. They found that a diluted mixture of a polymer (specifically polyethylene oxide) when placed over a speaker can create jets very similar to spicules, and when diluted at the right amount the droplet creation is suppressed as well. Spicules dont make droplets, so given that the math is similar to describe both effects, there could be some physical similarities.

They then turned to software that simulates the behavior of the solar plasma. Using the known physics of how it behaves, the code can be tweaked to see if certain behaviors can be reproduced. Without any real detailed inputs just using the vibrations of the solar surface created from sound waves of certain harmonic frequencies their code reproduced spicule-like structures. Thats encouraging! They also found the driving frequency doesnt need to be harmonic (that is, sound waves of evenly divisible frequencies, like say 440 and 220 and 110 Hertz), but can be quasi-periodic; mostly periodic but with some randomness thrown in. Thats good too, as the Suns surface is a cacophony of different frequencies that dont always create harmonic chords.

When they added a simple vertical magnetic field to their code they found they got even more spicule-like behavior, with about the right heights and widths. The speed of growth was similar, too. The magnetic field introduces an anisotropy, a non-symmetric nature to the surface that helps squeeze the plasma into narrow towers. This is similar for the need of the polymeric fluid to be diluted; that also is an anisotropy that helps the jets form.

The overall conclusion is that they found a more fundamental reason spicules might be produced on the Sun without the need for lots of special circumstances. This doesnt mean earlier research was wrong, necessarily, but it can be nice to reach for more basic physics sometimes to see what it contributes, and then add layers to it.

And, like the earlier attempts to explain spicules, its hard to know if this is the right answer. Just because the experiments and code make something that looks like spicules doesnt mean thats whats going on.

As I like to point out, this is the nature of science. We usually wind up with lots of ideas to explain a phenomenon, and it can take a while to weed out which ones are actually involved and which arent. The Sun is a nightmare of complexity, and a lot of its behavior is incredibly difficult to understand. But we now have observatories like Hinode and Solar Dynamics Observatory and the Inouye Solar Telescope that can see the Sun in high resolution and at wavelengths of light our eyes cant see, and all these observations help the theorists figure out whats what.

As time goes on, well understand the Sun better and better. That too is how science works.

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Bad Astronomy | Spicules on the Sun may be due to Faraday waves | SYFY WIRE - Syfy

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Whoa! Another asteroid whizzes past Earth hours after discovery – EarthSky

Posted: at 10:26 pm

There are thousands of near-Earth asteroids in the inner solar system, as depicted in this graphic. Some known and some unknown. Another asteroid discovered by the same astronomer to discover 2022 EB5 in early March made a close pass with Earth in the early hours of March 25, 2022. Image via NASA/ JPL-Caltech/ Wikimedia Commons.Another asteroid whizzes past Earth overnight

Overnight on March 24-25, 2022, another small asteroid raced toward Earth, unseen until hours before its closest approach. Hungarian astronomer Krisztin Srneczky, same astronomer who first spotted asteroid 2022 EB5 earlier this month hours before it hit Earth near Iceland, found this new asteroid, too. He caught it just hours before it sped by Earth. This asteroid is labeled Sar2594. Its close encounter with Earth came at 8:10 UTC or 3:10 a.m. CDT.

This time, instead of a collision, the space rock slipped through Earths shadow.

It passed at a distance of about 5,400 miles (8,700 km). Thats in contrast to the moons distance of 238,900 miles (384,000 km).

Sar2594 is categorized as a Near-Earth Object, or NEO. It raced by at about 40,265 miles an hour (18 km/s).

Sar2594 now has an official designation: 2022 FD1. Srneczky says the asteroid is about 2-4 meters in size. This could put it in the running for the smallest asteroid known. The current record holder is 2015 TC25, which is approximately 6 feet or 2 meters in diameter.

The asteroids flyby of Earth changed its course. Srneczky and Tony Dunn share charts and simulations of 2022 FD1s inclination:

Bottom line: Another asteroid whizzes past Earth hours after discovery. The asteroid, Sar2594, was discovered by the same astronomer, Krisztin Srneczky, who discovered 2022 EB5, which impacted near Iceland earlier this month.

Kelly Kizer Whitt has been a science writer specializing in astronomy for more than two decades. She began her career at Astronomy Magazine, and she has made regular contributions to AstronomyToday and the Sierra Club, among other outlets. Her childrens picture book, Solar System Forecast, was published in 2012. She has also written a young adult dystopian novel titled A Different Sky. When she is not reading or writing about astronomy and staring up at the stars, she enjoys traveling to the national parks, creating crossword puzzles, running, tennis, and paddleboarding. Kelly lives with her family in Wisconsin.

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Whoa! Another asteroid whizzes past Earth hours after discovery - EarthSky

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