Tag Archives: Unusual

An unusual object has been releasing pulses of radio waves in space for decades. Astronomers just discovered it – CNN

  1. An unusual object has been releasing pulses of radio waves in space for decades. Astronomers just discovered it CNN
  2. Astronomers find new type of stellar object that challenges understanding of neutron star physics Phys.org
  3. NRL’s VLITE confirmed magnetar GPM J1839–10 has been pulsing regularly every 22 minutes Interesting Engineering
  4. Are aliens trying to contact Earth? Scientists discover a mysterious stellar object that emits a five-minute p Daily Mail
  5. Scientists spot cosmic object that lights up every 20 minutes Metro.co.uk
  6. View Full Coverage on Google News

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Kevin Willard on West Virginia, message boards, an unusual tip time and more – 247Sports

  1. Kevin Willard on West Virginia, message boards, an unusual tip time and more 247Sports
  2. NCAA Tournament round of 64 preview: No. 8-seed Maryland vs. No. 9-seed West Virginia Testudo Times
  3. Arizona excited to head east to play West Virginia in 1st round of NCAA women’s bracket Arizona Daily Star
  4. Gary Williams previews Maryland-West Virginia, one performance he’d pray for, Willard’s strategy and more 247Sports
  5. West Virginia, Maryland to Renew Hoop Rivalry Thursday in NCAA Tournament – West Virginia University Athletics WVU Athletics
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Invasive strep A is on the rise and affecting kids in unusual ways

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The seven kids with oddball symptoms arrived at Children’s Mercy Kansas City Hospital in Missouri in quick succession this past month. One complained of an eye that was “stuck.” Another had a lump behind one ear. A third had trouble swallowing, and then began drooling.

There was no reason to think these and four other cases, all in children younger than 10, might be related, recalled Angela Myers, the director of infectious diseases. But when the lab tests came back, they all pointed to the same culprit.

It was a potentially lethal form of strep A.

“We were very surprised,” Myers said. “We just don’t see this many together in such a short time.”

Infection with Streptococcus pyogenes — or group A strep, for short — typically produces mild symptoms, such as rash, fever or swollen tonsils leading to the eponymous strep throat. But in recent months, cases related to a rare invasive form of the common bacteria have been popping up across the United States, as well as Europe, often in connection with sometimes confusing symptoms, including skin rashes, fever, a racing heart and unexplained swelling.

The first confirmed pediatric deaths in this country, in two young children in the Denver area, were reported last week. At least 16 children have died of it in the United Kingdom, seven in the Netherlands and two in France.

The rise of invasive strep A is one of a number of unusual ways pathogens have been interacting with us — and each other — amid the end of coronavirus-era social distancing and masking this year. Both the World Health Organization and the U.S. Centers for Disease Control and Prevention said they are investigating the cases, including whether the viral storm that has been keeping many people sick may be at least partially to blame.

Why a ‘tripledemic’ is keeping some people sick for weeks, even months

Viral infections tend to create disorder in a person’s immune system, making it easier for a secondary bacterial infection to take hold and intensify its effects in some cases.

Minnesota health officials said they had seen 46 cases of invasive strep A in all ages in November, more than double the average 20 cases in previous months. Colorado reported that it was investigating not only a rise in invasive strep A cases, but also a possible increase in other severe or invasive bacterial infections in children.

Texas Children’s Hospital said it has seen more than 60 patients with invasive strep A in October and November — a fourfold increase from the same period the previous year. James Versalovic, pathologist-in-chief for the medical center, said many of the affected children had current or recent viral infections. But, he said, it is still too early to rule out other factors that may be contributing to the seriousness of their illnesses.

“It could be we have altered patterns of immunity due to the pandemic that may have increased our vulnerability. But it could also be … different variants” of strep, he said. “It could be a combination of factors. No one knows.”

Unlike SARS-CoV-2, strep A is something humans have battled for centuries.

It has variously been described, incorrectly, throughout history as being associated with phenomena such as comets and eclipses, or the introduction of nonliving matter into humans. It wasn’t until 1874 that Austrian surgeon Theodor Billroth described an organism he saw under a microscope that appeared to be grouped in chains of four or more that would later be classified as bacteria. Bacteria can live in or out of a patient’s body, unlike viruses, which are a collection of molecules that can only replicate in a host. Both are transmitted in similar ways — through air, water, food and living things.

Several million people in the United States are infected each year with strep A, and in our modern world, with its ample supply of antibiotics, it is mostly a nuisance. It usually translates into a sore throat, and maybe a missed day of school or work during the 24 hours it takes to stop being contagious after taking antibiotics such as penicillin and amoxicillin.

Strep A: What you need to know about the usually mild infection

“The good news is that we know how to treat it and how to test for it,” said Kristin Moffitt, an infectious-disease expert at Boston Children’s Hospital who studies bacterial infections. “Normally it’s not a source of serious concern that I would be hyper-anxious about.”

But in a small number of cases, strep A can turn dangerous when it invades parts of the body where bacteria don’t normally exist. When it goes into such areas, including the blood, cerebrospinal fluid, bone marrow and organs such as the brain and heart, it can spread quickly and kill.

The first reports of unusual activity as a result of invasive strep A, mostly involving children 5 and under, came from the Netherlands between March and July. It was not only the number of cases and their severity, doctors said in a preprint research paper posted Dec. 13, but also the fact that many of the patients had been co-infected with viruses such as the flu or chickenpox. (Unlike in the United States, vaccinations for varicella, which cause chickenpox, are not a part of the children’s immunization program in the Netherlands.)

In 2018 and 2019, most of the kids seen at Dutch hospitals with invasive strep A developed sepsis, a systemic infection or pneumonia. But this year, many were diagnosed as suffering from necrotizing fasciitis, a flesh-eating disease that involves bacteria that destroys tissue under the skin. Physicians Evelien B. van Kempen, Patricia C.J. Bruijning-Verhagen, and their co-authors urged the public to be aware that early recognition and prompt treatment may save lives.

“Clinicians and parents should be vigilant and aware of unusual pediatric presentations,” they wrote.

Serious illness in children has also been reported in the United Kingdom, Netherlands, France, Ireland and Sweden, but the patterns aren’t always the same. In the U.K., doctors reported a surge in scarlet fever — which is also caused by strep A bacteria — at around the same time as the invasive cases. But that wasn’t seen in the Netherlands.

Several hospitals in the United States said they are unaware of unusual scarlet fever activity in their areas.

Figuring out what’s going on in the United States is trickier than in some other countries because of the lack of a national heath-care system that facilitates tracking of cases. CDC spokeswoman Kate Grusich said in an email that it is too soon to say whether case numbers “are just returning to pre-pandemic levels, or if they are rising beyond what we would normally expect.”

The “CDC is watching these data closely, and talking with surveillance sites and hospitals in multiple states to learn more about any trends,” she said.

The email listservs for pediatricians and infectious-disease specialists in this country started blowing up in October with a question from a doctor in the Midwest: Was anyone else seeing an increase in invasive strep A?

The responses were mixed, as expected, given that such cases tend to cluster. Boston Children’s had not seen anything concerning. But physicians in Kansas City, Houston and Denver had.

At Texas Children’s, Versalovic said some children have come in with low blood pressure and septic shock, some with bacterial pneumonia, and still others with skin infections. Several were so ill that they required intensive care. He worries some of the cases are being missed. To diagnose invasive strep A, doctors must take samples of a patient’s blood, skin, or fluid in the lungs or other areas. But if a child needs emergency care, there may not be time to consider the cause of the illness.

Invasive strep A “does not follow a simple linear progression,” he said.

In Denver, Samuel Dominguez, an infectious-disease specialist at Children’s Hospital Colorado and a professor at the University of Colorado School of Medicine, said the cases he had seen were “across the age spectrum” in children, noting that they may be more susceptible because bacteria tend to colonize more aggressively in their throats and skin than in adults.

Dominguez sought to balance reassurances that this is a relatively rare infection with calls to be on the lookout for warning signs.

Versalovic agreed. “We don’t want to raise too many alarms, but these infections can progress very rapidly,” he said.

Myers said all the patients seen at Children’s Mercy in Missouri have recovered with treatment, but she urged parents to make sure their children’s vaccinations are up to date to prevent a viral infection that may open the doors to a more severe bacterial one. “I think there are a lot of things at play we don’t fully know yet,” she said.

One of the tricky things about the illness is that it can look so different in different children, she said. The child having trouble moving their eyeball had an infection of the soft tissues of the eye socket; the one with the lump behind the ear, an infection of the bone in that area; and the third patient, a collection of pus in the back of the throat.

Myers urged parents to err on the side of caution.

“If a child looks sicker than they should be after they develop a fever, it’s always a good idea to bring them to a doctor if they have trouble breathing, or you notice something else — even a swollen eye,” she said.

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Earth has been hit by an ‘unusual, intense blast of energy’ from nearby galaxy that could change our understanding of the universe




© Aaron M. Geller/Northwestern/CIERA and IT Research Computing Services
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Earth has been hit by an intense, unusual blast of light that could change our understanding of the universe, scientists have said.

Late last year, scientists spotted a 50-second-long blast of energy coming towards Earth, known as a gamma-ray burst or GRB, which are the most powerful explosions in the universe. Immediately, researchers started looking for the afterglow that such blasts leave behind, with that visible light being useful to find where the blast has come from.

But those researchers instead found something else entirely: that the blast appeared to have come from a kilonova. Those rare events only happen when a neutron star merges with another very compact object – either another neutron star or a black hole.

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The study challenges our understanding of where such long-lasting GRBs come from. But it could also provide an exciting way to answer other questions about the universe, such as where its heaviest elements come from, which still remains a mystery.

And the galaxy from which the GRB came from is also strange. It is young and still forming stars – the opposite of the only other known nearby galaxy that has played host to such an event.

“This event looks unlike anything else we have seen before from a long gamma-ray burst,” said Jillian Rastinejad, from Northwestern University, who led the study. “Its gamma rays resemble those of bursts produced by the collapse of massive stars.

Given that all other confirmed neutron star mergers we have observed have been accompanied by bursts lasting less than two seconds, we had every reason to expect this 50-second GRB was created by the collapse of a massive star. This event represents an exciting paradigm shift for gamma-ray burst astronomy.”

A paper describing the findings, ‘A kilonova following a long-duration gamma-ray burst at 350 Mpc’, is published in the journal Nature today.

The blast was first spotted in December 2021, by Nasa’s Neil Gehrels Swift Observatory and the Fermi Gamma-ray Space Telescope. Since then, researchers have been looking to categorise the explosion, and understand where it might have come from.

Among other findings, they showed that the one event produced heavy elements that amounted to roughly 1,000 times the mass of our Earth. That suggests that kilonovae are the main place that gold is produced in the universe.

And because the galaxy from which the GRB came from is relatively nearby, scientists were able to get an unusually good look at it. What’s more, that could help explain other gamma-ray bursts that do not seem to fit with our understanding of where they come from.

“This was a remarkable GRB,” said Benjamin Gompertz. “We don’t expect mergers to last more than about two seconds. Somehow, this one powered a jet for almost a full minute. It’s possible the behaviour could be explained by a long-lasting neutron star, but we can’t rule out that what we saw was a neutron star being ripped apart by a black hole.

“Studying more of these events will help us determine which is the right answer and the detailed information we gained from GRB 211211A will be invaluable for this interpretation.”

And scientists hope that the switch-on of the James Webb Space Telescope will get an even better view of kilonovae. That telescope is able to capture images of distant astronomical objects, and “sniff” their atmosphere, allowing it to see exactly what elements are present through a process known as spectroscopy.

“Unfortunately, even the best ground-based telescopes are not sensitive enough to perform spectroscopy,” Rastinejad said. “With the JWST, we could have obtained a spectrum of the kilonova. Those spectral lines provide direct evidence that you have detected the heaviest elements.”

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Earth has been hit by an ‘unusual, intense blast of energy’ from nearby galaxy that could change our understanding of the universe

Earth has been hit by an intense, unusual blast of light that could change our understanding of the universe, scientists have said.

Late last year, scientists spotted a 50-second-long blast of energy coming towards Earth, known as a gamma-ray burst or GRB, which are the most powerful explosions in the universe. Immediately, researchers started looking for the afterglow that such blasts leave behind, with that visible light being useful to find where the blast has come from.

But those researchers instead found something else entirely: that the blast appeared to have come from a kilonova. Those rare events only happen when a neutron star merges with another very compact object – either another neutron star or a black hole.

The study challenges our understanding of where such long-lasting GRBs come from. But it could also provide an exciting way to answer other questions about the universe, such as where its heaviest elements come from, which still remains a mystery.

And the galaxy from which the GRB came from is also strange. It is young and still forming stars – the opposite of the only other known nearby galaxy that has played host to such an event.

“This event looks unlike anything else we have seen before from a long gamma-ray burst,” said Jillian Rastinejad, from Northwestern University, who led the study. “Its gamma rays resemble those of bursts produced by the collapse of massive stars.

Given that all other confirmed neutron star mergers we have observed have been accompanied by bursts lasting less than two seconds, we had every reason to expect this 50-second GRB was created by the collapse of a massive star. This event represents an exciting paradigm shift for gamma-ray burst astronomy.”

A paper describing the findings, ‘A kilonova following a long-duration gamma-ray burst at 350 Mpc’, is published in the journal Nature today.

The blast was first spotted in December 2021, by Nasa’s Neil Gehrels Swift Observatory and the Fermi Gamma-ray Space Telescope. Since then, researchers have been looking to categorise the explosion, and understand where it might have come from.

Among other findings, they showed that the one event produced heavy elements that amounted to roughly 1,000 times the mass of our Earth. That suggests that kilonovae are the main place that gold is produced in the universe.

And because the galaxy from which the GRB came from is relatively nearby, scientists were able to get an unusually good look at it. What’s more, that could help explain other gamma-ray bursts that do not seem to fit with our understanding of where they come from.

“This was a remarkable GRB,” said Benjamin Gompertz. “We don’t expect mergers to last more than about two seconds. Somehow, this one powered a jet for almost a full minute. It’s possible the behaviour could be explained by a long-lasting neutron star, but we can’t rule out that what we saw was a neutron star being ripped apart by a black hole.

“Studying more of these events will help us determine which is the right answer and the detailed information we gained from GRB 211211A will be invaluable for this interpretation.”

And scientists hope that the switch-on of the James Webb Space Telescope will get an even better view of kilonovae. That telescope is able to capture images of distant astronomical objects, and “sniff” their atmosphere, allowing it to see exactly what elements are present through a process known as spectroscopy.

“Unfortunately, even the best ground-based telescopes are not sensitive enough to perform spectroscopy,” Rastinejad said. “With the JWST, we could have obtained a spectrum of the kilonova. Those spectral lines provide direct evidence that you have detected the heaviest elements.”

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4000-year-old hair from the Middle Nile highlights unusual ancient DNA degradation pattern and a potential source of early eastern Africa pastoralists

Archaeological context of Kadruka 1 SK68

Archaeological fieldwork in the Kadruka district of northern Sudan has revealed widespread past occupation of the alluvial plain and paleochannel systems to the east of the current Nile River channel9. In accordance with broader archaeological sequences for this region of the Middle Nile Valley10,11,12, cultural deposits were primarily linked to the Neolithic (spanning the 7th millennium BP), as well as the more recent Kerma period (3450–4450 BP). Excavation programs in the Kadruka district focused on several cemeteries from these cultural periods, including Kadruka 1 and Kadruka 21. Reflecting local environmental fluctuations between dry and wet conditions associated with more intensive Nile floods during the Middle Holocene, Neolithic skeletal remains at these cemeteries are typically highly degraded13,14. In contrast, progressive local aridification and floodplain contraction15, has facilitated enhanced preservation of organics, including hair and leather items, in the more recent Kerma period burials at Kadruka 116.

A recent study exploring the diet of individuals from Kadruka 21 and Kadruka 1 detected milk proteins attributable to domesticated cow (Bovinae) or sheep (Ovis) in the dental calculus of individual SK129 from Kadruka 21 and to goat (Carpa) in the dental calculus of individual SK68 from Kadruka 117. Furthermore, isotopic analyses of hair from individual SK68 (named “Sudan_Kadruka1_4000BP” in this study) broadly indicate a diet primarily composed of C3-based resources (C3 plants or animals consuming C3 plants, δ13C -17.0‰, δ15N 12.0‰).

The early proliferation of herding economies in northeastern Africa, particularly apparent in the Kerma civilisation of Upper Nubia11,12, has been proposed as a potential link to the dispersal of pastoral populations into eastern Africa5,6,7, though there is as yet no published genetic evidence to support this migration model. Direct palaeoproteomic evidence for milk consumption17, together with the remains of cattle, sheep and goat found in grave assemblages18, identify individuals from Kadruka 1 and Kadruka 21 as belonging to early populations practicing pastoralism, making the sites ideal for archaeogenetic research seeking to examine early pastoralist dispersals in northeastern Africa.

Ancient DNA authentification and sequencing strategy

We screened five specimens deriving from four individuals from the Kadruka district of northern Sudan (Fig. 1a) for aDNA preservation, drawing on tooth (KDR001.A), hair (KDR001.B), petrous bone (KDR002, KDR004) and cranial (KDR003) samples. All specimens were excavated from archaeological contexts dating to the Neolithic and Kerma periods. The only sample that yielded detectable authentic aDNA was a lock of dark hair (127 mg) (Fig. 1b) from a Kerma period individual. We used a total of 27.5 cm of hair for aDNA extraction and 78.5 mg for radiocarbon dating. The hair sample from Kadruka 1 SK68 is directly dated to 3928–4139 calBP (Fig. 1c), contemporaneous to the Pastoral Neolithic period in eastern Africa.

Figure 1

Sample details of the 4,000-year-old hair from Sudan. (a) Geographic location of Kadruka and modern African populations used for subsequent analyses. (b) Picture of the Kadruka hair sample. (c) C14 calibrated age (cal BC) of the Kadruka hair, plotted using IntCal13 calibration curve19.

To maximize the possibility of aDNA retrieval from shotgun sequencing, we applied double-stranded and single-stranded library protocols to the four extracts deriving from the Kadruka skeletal remains, but only applied the single-stranded library protocol to the hair sample, since this protocol typically results in higher yields than the double-stranded library approach for highly fragmented DNA. None of the aDNA libraries extracted from the skeletal elements showed authentic aDNA damage patterns, i.e., substitutions from cytosine to thymine (C- > T) (Table S1). The hair sample (KDR001.B0101), however, provided an observed 17.5% C- > T substitution rate at the first 5-prime base in sequencing reads (Table S1). Accordingly, we selected this library from the hair sample for deeper sequencing.

We found that the average read length was relatively short (33 base pair/bp, Table S1). This poses a challenge, since short DNA fragments can result in spurious alignments to the human reference genome, even if they do not originate from humans, but from, for example, microbes present in the burial environment. On the other hand, while long DNA fragments have high mapping certainty, they are more likely to originate from modern human DNA contamination (which typically consists of long DNA fragments). We therefore explored various read length cut-offs to yield as much authentic human aDNA as possible, while maintaining a low proportion of reads from presumed modern human contamination. For this purpose, we used two tools to assess both the rate of spurious alignments and the rate of modern human contaminants. First, we used SpAl20 which uses simulations to estimate fractions of spurious and authentic alignments given certain read length cut-offs. For a cut-off length of 25 bp, SpAI estimated a spurious alignment fraction of 10% (Table S2). As the read length cut-off increases, the estimation for spurious alignments drops respectively (Table S2). Second, we used AuthentiCT21 to estimate the overall contamination level in the aligned fragments using base substitution patterns. We explored length cut-offs at 10, 25, 30 (custom setting) and 34 bp in the raw data processing steps, and summarised EAGER statistics and respective contamination estimates in Table S2.

We find that at a length cut-off of 30 bp, 47.3 ± 2.4% of retrieved aDNA is likely of modern-human contaminant origin (Table 1). In comparison, a length cut-off of 25 bp yielded 4,680,356 mapped reads with 0.1 ± 0.3% contamination (Table 1). Together with the results from SpAL, we consider 25 bp a safe cut-off length for this library. Thus, we continued our downstream analyses with a 25 bp read length filter, ending up with 231,040 sequencing reads after mapping, from which we derived 3,336 pseudo-haploid allele calls on 1240 k SNP positions (Table 1).

Table 1 Eager statistics of deeper shotgun sequenced data from the hair sample KDR001.B0101.SG1.2 with different length filter cut-off.

Characteristics of the aDNA fragments from hair

Employing our final read length filter at 25 bp and additionally filtering for alignment mapping quality (Methods), we further explored alignment statistics. We find two unusual characteristics in the aDNA library generated from the Kadruka hair sample. The first is that the sample is enriched in unusually short DNA molecules, giving a median read length of 25 bp, compared to 44 bp for typical bone-derived shotgun aDNA in a previous African aDNA study using the same laboratory pipeline4. The second is that unusually high damage rates were observed in the interior of the DNA molecules from hair, while unusually low damage rates were seen in the exterior of the molecules. For instance, at the interior 10th bp from the 5’ end, damage rates were 10% compared to 1% from typical bone-derived aDNA. While at the exterior, the 1st bp from the 5’ end showed damage rates of 15%, compared to on average of 27%22 from typical bone-derived aDNA. These patterns are consistent with high degradation of DNA fragments in hair through intense sun exposure, already during the lifetime of the individual, which may result in hair containing largely denatured single-stranded DNA fragments, as opposed to the more typically intact double-stranded fragments preserved in bone samples.

We find the ratio of mitochondrial to nuclear DNA in the hair-derived DNA library to be relatively high (with a ratio at 224 at length cut-off 25 bp, Table S1), compared to typical rates with other tissues; for example the ratio is at 110 on average for petrous bones in a previous study using the same laboratory pipeline4. We investigated whether there is a notable difference in terms of aDNA preservation in nuclear DNA and mitochondria from the hair material. Specifically, we examined if the two idiosyncratic features of hair aDNA we describe above apply to both nuclear and mitochondrial DNA from hair. In Fig. 2 and Fig S2, we compared the read length distribution and average base substitution rates of reads mapped to the complete genome (i.e., nuclear and mitochondrial), the nuclear genome, and the mitochondrial genome. We find that both nuclear and mitochondrial DNA have high base substitution rates in the interior of sequence reads (Fig S2a, c), but reads mapped to mitochondria are relatively longer than reads mapped to autosomes (Fig S2b, d).

Figure 2

Characteristics of aDNA fragments from the hair sample. (a) Length distribution of shotgun sequencing reads mapped to the whole genome using read length filter cut-off at 25 bp in the step of adaptor removal. (b) High C-to-T substitution rates in the interior of aDNA fragments.

Given the tenfold reduction of mapped reads after applying a mapping quality filter (Table 1), we examined if the two features of hair aDNA observed here resulted from the mapping quality filter. We find that our mapping quality filter did not have a notable effect on the two features of ultra-short DNA fragment enrichment and high interior aDNA damage pattern (Fig S3).

Given the success of SNP capture techniques for poorly preserved human DNA23, we also performed SNP capture for our hair-derived aDNA library. However, SNP capture did not provide an improvement over shotgun sequencing. Instead, we found the base substitution rates in the exterior and interior of reads are substantially lower in capture data, in comparison to the rate distribution in shotgun data (Fig. S1, Table S1), corroborating the fact of high contamination rate in the capture data (42 ± 3% as estimated by AuthentiCT), likely due to capture preferentially targeting molecules without damage (due to more effective hybridization) than with damage. In addition, longer molecules are preferentially captured over short molecules.

Genetic affinity to early eastern African pastoralists

We performed Principal Components Analysis (PCA) and Outgroup-f3 (Figs. 2, 3) to investigate the genetic ancestry of the individual (Sudan_Kadruka1_4000BP) from whom our hair sample derived, utilizing 3336 mapped reads overlapping with SNP positions from the Shotgun data, after read length filter at 25 bp of Sudan_Kadruka1_4000BP (Table S2). To maximise the resolution given the extremely low coverage and low number of called alleles, we used high-coverage modern African genomic data from the SGDP24 and the HGDP25, which includes all SNPs in 1240 k panel, instead of the commonly used Human Origin array data26, for calculating Principal Components (PCs). We projected ancient Africans and ancient Near Easterners on the background of modern African groups25. Although the number of available populations in SGDP and HGDP is limited, we observe clear separations of African populations from different regions, with eastern/northern, southern and western African populations falling into the right, left and top corner of PC1/PC2 space, respectively.

Figure 3

Genetic ancestry of Sudan_Kadruka1_4000BP. Principal Component Analysis (PCA) of African populations. We project Sudan_Kadruka1_4000BP into an African PCA (Table S3) with PCs calculated from modern Africans in SGDP24. We use block jackknife strategy (taking-one-chromosome-out)26 for error bar calculation of Sudan_Kadruka1_4000BP ‘s location on the PCA.

The PCA shows Sudan_Kadruka1_4000BP located close to previously published early pastoralists in eastern Africa4,5, such as Kenya_EarlyPastoral_N (3800–4000 calBP) and Kenya_Pastoral_Neolithic (1500–3000 calBP). Kenya_EarlyPastoral_N is a group of two pastoralist individuals dated to the early stage of the eastern African Pastoral Neolithic, both of whom are genetically derived from admixture between two early northeastern African-related ancestries from Sudan and Northern Africa/Levant5. To estimate the level of noise resulting from the sparsity of our SNP data, we computed a standard error for the projected PCs of Sudan_Kadruka1_4000BP using a block jackknife approach. Specifically, we computed pseudo-values by deleting each chromosome of the genotype data in turn and then used the resulting estimates from the remaining data as input for the weighted jackknife calculation27. We find the standard errors of Sudan_Kadruka1_4000BP to be relatively small compared to overall genetic variation within Africa, which gives us confidence that the location calculated from the full data (Fig. 2a) is robust.

Despite the sparsity of the data, the PCA analyses conducted here clearly suggest a very close genetic relationship between Sudan_Kadruka1_4000BP and ancient eastern African pastoralist populations. To corroborate this finding, we also computed allele sharing rates with ancient populations from the Levant and Africa and present-day African populations at genomic sites where Sudan_Kadruka1_4000BP differs from the chimpanzee reference genome via outgroup-f3 (Sudan_Kadruka1_4000BP, population X; Chimpanzee). Figure 4a shows that Sudan_Kadruka1_4000BP shares the highest genetic affinity with ancient Levantine groups, ancient northern and Eastern Africans and modern Africans from northern Sahara and the Horn of Africa. We computed pairwise comparisons employing f4 (Sudan_Kadruka1_4000BP, Kenya_EarlyPastoral_N; population X, Chimp) to validate the close PC location between Sudan_Kadruka1_4000BP and Kenya_EarlyNeolithic_N. Consistent with PCA location, f4-statistic result confirms the genetic cladality between Sudan_Kadruka1_4000BP and Kenya_EarlyPastoral_N given that none of the tested populations breaks cladality significantly, suggesting that these two individuals are indistinguishable in terms of allele frequencies (Fig. 4b). Additionally, we show that in f4 (Kenya_EarlyPastoral_N, population X; Sudan_Kadruka1_4000BP, Chimp) results (Fig. 4c) that all tested ancient and modern African populations are either significantly positive (suggesting that they are less close to Kenya_EarlyPastoral_N compared to Sudan_Kadruka1_4000BP) or overlapping with zero, indicating equal genetic distance to both.

Figure 4

Genetic affinity with ancient African pastoralists. (a) Outgroup f3(Sudan_Kadruka1_4000BP, population X; Chimp). (b) f4(Sudan_Kadruka1_4000BP, Kenya_EarlyPastoral_N; population X, Chimp). (c) f4(Kenya_EarlyPastoral_N, population X; Sudan_Kadruka1_4000BP, Chimp). Population X includes published ancient African and Near Eastern populations and modern African populations from SGDP and HGDP data sets (Table S3). We plot two standard error bars for f3 and f4 statistics shown here and highlight statistically significant tests (Z-score > 3) in red color.

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Men With High IQ Are More Likely To Do This Unusual Activity

The study found a strong connection between intelligence and skill-based gambling.

Recent research shows that Finnish men with higher IQs are more likely to bet on horse racing.

According to recent study from researchers at the University of Eastern Finland and the University of Liverpool, men with higher IQs are more inclined to bet on horse races.

Men with higher numerical IQs were shown to be more likely to partake in skill-based gambling, such as horse racing, choose more complicated betting options, and spend more money, according to a study published in the Journal of Behavioral Decision Making.

More than 15,000 Finnish males who had taken an IQ test as part of their mandatory military duty while enlisting in the Finnish Defense Forces participated in the research. This was cross-referenced with thorough records on the men’s online gambling behavior as well as statistics from Statistics Finland on their socioeconomic standing, income, and level of education.

Women were not included in the data since Finnish legislation only requires males to complete military service and take an IQ test.

Commenting on the findings, Professor David Forrest from the University of Liverpool Management School said: “Our research found a strong correlation between men with a high IQ and those who take part in skilled gambling, such as betting on horse racing. It is important to note that our findings can’t necessarily be generalised to chance-based gambling, such as gaming machines. However, there is very little previous research on the association between intelligence and skills-based gambling and so finding such a strong link is significant.”

The study does not provide a definitive answer on why men with higher IQs would enjoy betting on horse racing, but the researchers believe this could be because men with higher IQs enjoy the mathematical challenge posed by such skill-based betting.

Associate Professor Jani Saastamoinen of the University of Eastern Finland said: “Betting could be compared to solving crossword puzzles. Perhaps, bettors like to crunch numbers and find the winning horses – even though they know they’ll end up losing money in the long run.”

Reference: “Does IQ predict engagement with skill-based gambling? Large-scale evidence from horserace betting” by Niko Suhonen, Jani Saastamoinen, David Forrest and Tuomo Kainulainen, 4 September 2022, Journal of Behavioral Decision Making.
DOI: 10.1002/bdm.2300



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Tonga volcano blast was unusual, could even warm the Earth

NEW YORK (AP) — When an undersea volcano erupted in Tonga in January, its watery blast was huge and unusual — and scientists are still trying to understand its impacts.

The volcano, known as Hunga Tonga-Hunga Ha’apai, shot millions of tons of water vapor high up into the atmosphere, according to a study published Thursday in the journal Science.

The researchers estimate the eruption raised the amount of water in the stratosphere — the second layer of the atmosphere, above the range where humans live and breathe — by around 5%.

Now, scientists are trying to figure out how all that water could affect the atmosphere, and whether it might warm Earth’s surface over the next few years.

“This was a once-in-a-lifetime event,” said lead author Holger Voemel, a scientist at the National Center for Atmospheric Research in Colorado.

Big eruptions usually cool the planet. Most volcanoes send up large amounts of sulfur, which blocks the sun’s rays, explained Matthew Toohey, a climate researcher at the University of Saskatchewan who was not involved in the study.

The Tongan blast was much soggier: The eruption started under the ocean, so it shot up a plume with much more water than usual. And since water vapor acts as a heat-trapping greenhouse gas, the eruption will probably raise temperatures instead of lowering them, Toohey said.

It’s unclear just how much warming could be in store.

Karen Rosenlof, a climate scientist at the National Oceanic and Atmospheric Administration who was not involved with the study, said she expects the effects to be minimal and temporary.

“This amount of increase might warm the surface a small amount for a short amount of time,” Rosenlof said in an email.

The water vapor will stick around the upper atmosphere for a few years before making its way into the lower atmosphere, Toohey said. In the meantime, the extra water might also speed up ozone loss in the atmosphere, Rosenlof added.

But it’s hard for scientists to say for sure, because they’ve never seen an eruption like this one.

The stratosphere stretches from around 7.5 miles to 31 miles (12 km to 50 km) above Earth and is usually very dry, Voemel explained.

Voemel’s team estimated the volcano’s plume using a network of instruments suspended from weather balloons. Usually, these tools can’t even measure water levels in the stratosphere because the amounts are so low, Voemel said.

Another research group monitored the blast using an instrument on a NASA satellite. In their study, published earlier this summer, they estimated the eruption to be even bigger, adding around 150 million metric tons of water vapor to the stratosphere — three times as much as Voemel’s study found.

Voemel acknowledged that the satellite imaging might have observed parts of the plume that the balloon instruments couldn’t catch, making its estimate higher.

Either way, he said, the Tongan blast was unlike anything seen in recent history, and studying its aftermath may hold new insights into our atmosphere.

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The Associated Press Health and Science Department receives support from the Howard Hughes Medical Institute’s Department of Science Education. The AP is solely responsible for all content.

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Unusual ‘revived’ pulsars could detect gravitational waves

Paul M. Sutter (opens in new tab) is an astrophysicist at SUNY (opens in new tab) Stony Brook and the Flatiron Institute, host of “Ask a Spaceman (opens in new tab) and “Space Radio (opens in new tab),” and author of “How t (opens in new tab)o Die in Space.”

Astronomers hope to use pulsars scattered around the galaxy as a giant gravitational wave detector. But why do we need them, and how do they work?

Gravitational waves, or ripples in the fabric of space-time, from all sorts of sources constantly slosh throughout the universe. Right now, you are being slightly stretched and squeezed as wave after wave passes through you. Those waves come from merging black holes, the explosions of giant stars and even the earliest moments of the Big Bang.

On Earth, we’ve developed incredibly sensitive gravitational wave detectors that have been able to sense brief-but-loud events, such as black hole mergers, which last only a few seconds but generate such enormous signals that we can detect them. (“Enormous” is a relative term here; the distortion resulting from the passing wave is less than the width of an atomic nucleus.) 

Related: The first telescope of its kind will hunt for sources of gravitational waves

But ground-based detectors have a much harder time finding low-frequency gravitational waves, since those take weeks, months or even years to pass through Earth. Those kinds of low-frequency waves come from mergers of giant black holes, which take a lot longer to merge than their smaller cousins do. Our detectors simply don’t have the sensitivity to measure those small differences over such long time spans. For that, we need a much, much larger detector.

So, instead of using instruments on the ground, we can use distant pulsars to help us measure gravitational waves. This is the idea behind so-called pulsar timing arrays. 

Powering up the pulsars 

Pulsars are already fantastic objects, and that’s especially true for the kinds of pulsars used as gravitational wave detectors.

Pulsars are the leftover cores of giant stars and are among the most exotic objects ever known to inhabit the cosmos. They are ultradense balls made almost purely of neutrons, with some electrons and protons thrown in for good measure. Those spinning charges power up incredibly strong magnetic fields — in some cases, the most powerful magnetic fields in the universe.

Those intense magnetic fields also whip up strong electric fields. Together, they power beams of radiation (if you’re getting Death Star vibes here, you’re not far off) that blast out from the magnetic poles in each direction. Those magnetic poles don’t always line up with the rotational axis of the pulsar, in much the same way Earth’s North and South magnetic poles don’t line up with our planet’s rotational axis.

This forces the beams of radiation to sweep out circles in the sky. When those beams cross over Earth, we see them as periodic flashes of radio emission, putting the “pulse” in “pulsar.”

Related: Gravitational waves play with fast spinning stars, study suggests

Pulsars are incredibly regular. They are so heavy, and spin so quickly, that we can use their flashes as extremely precise clocks. But most pulsars are susceptible to random starquakes (when the star’s contents shift around, disturbing the pulsar’s rotation), glitches and slowdowns that change their regularity. That means most pulsars aren’t good for studying gravitational waves.

So instead, timing arrays rely on a subset of pulsars known as millisecond pulsars, which, as the name suggests, have rotational periods of a few milliseconds. Astronomers think millisecond pulsars are “revived” pulsars, spun up to incredible speeds after infalling material from a companion star accelerates them like a grown-up pushing a kid on a schoolyard merry-go-round.

Because of their ludicrous speed, millisecond pulsars can maintain fantastic precision over very long timescales. For example, one pulsar, PSR B1937+21, has a rotational period of 1.5578064688197945 +/- 0.0000000000000004 seconds. That’s the same level of precision as our best atomic clocks.

And those millisecond pulsars are perfect gravitational wave detectors.

Timing the array

Here’s how it works. First, astronomers observe the rotational periods of as many millisecond pulsars as possible. If a gravitational wave passes over Earth, over a pulsar or even between us, then as it passes, it will change the distance between Earth and the pulsar. As the wave moves, the pulsar will appear slightly closer, then slightly farther, then slightly closer, and so on until the wave has moved on.

That change in distance will appear to us as changes in the rotational period. One flash from the pulsar may arrive a bit too soon; then another may arrive a little too late. For a typical gravitational wave, the shift in the timings is incredibly tiny — a change of just 10 or 20 nanoseconds every few months. But the measurements of the millisecond pulsars are sensitive enough that those changes can be detected — at least in principle.

The “array” part of “pulsar timing array” comes from studying many pulsars at once and looking for correlated movements: If a gravitational wave passes over one region of space, then all the timings from the pulsars in that direction will shift in unison. 

Many collaborations across the world have used radio telescopes to study pulsar timing arrays for decades. So far, they’ve had limited success, finding shifts in timings from various pulsars but no hints of correlations. But every year, the techniques get better, and the hope is that soon, these arrays will unlock a huge part of the gravitational wave universe.

Learn more by listening to the “Ask a Spaceman” podcast, available on iTunes (opens in new tab) and askaspaceman.com. Ask your own question on Twitter using #AskASpaceman or by following Paul @PaulMattSutter and facebook.com/PaulMattSutter.

Follow us on Twitter @Spacedotcom and on Facebook.  



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