Researchers at U of T Mississauga tap immersive technologies to improve palliative care – News@UofT

Researchers at the University of Toronto are looking to the virtual world to improve the quality of life for those in palliative care.

Cosmin Munteanu, assistant professor at U of T MississaugasInstitute for Communication, Culture, Informationand Technology, and PhD studentSho Conteare exploring how virtual reality (VR) devices can be used to enhance peoples experiences.

The impetus for the study, funded by the Canadian Institutes of Health Research,came from Contes experiences as a volunteer at a Toronto hospice. During some of his pre-pandemic visits, Conte took along some VR equipment (one of hishobbies) to entertain clients. He found himself using Google Earth to explore places they wanted to visit or revisit.

The reception was incredible super emotional and super effective, Munteanu says, notingthose in palliative care often have limited mobility and fewopportunities to enjoy new experiences.

The lack of social participation has been exacerbated by the recent pandemic. Conte notes he hasnt been able to see his client since March due to COVID-19.

Its a bit upsetting to me, just thinking about that, if I was in that situation, he says.

VR may be a way to break through the social isolation whether caused by the pandemic or the nature of palliative care itself and open new opportunities to facilitate social participation.

I see VR as a window into these virtual experiences that are immersive and very lived. Its not as good as the real thing, but in light of their mobility challenges, it works really well, Conte says.

It may also be a tool that helps provide a more holistic approach to end-of-life care.

We have a very good palliative care system in Canada, says Munteanu, although he notes there tends to be a medical focus.

Its the soft side thats often neglected.

With VR, patients can embark on virtual trips, share virtual travel experiences with family members, reminisce about the past and share stories while looking at Google Street View. VR could also give them a means to have an immersive experience, augment personal connections or even escape the confines of the hospice and meet others in a virtual setting.

The pandemic has put a temporary hold on exploring ways to put VR in the hands of palliative care patients because its not currently safe to work with such a vulnerable group. So, Conte has pivoted his research to focus on helping clinicians have difficult planning discussions with patients.

Studies show that 90 per cent of people want to have conversations about planning their care if things go badly, but only about 10 per cent have those conversations, Conte says. Having conversations and planning before its too late is one of the biggest predictors of quality at end of life.

Hes now turning to VR to help practitioners prepare for these emotionally charged discussions that happen too infrequently. Using a 3D chatbot that provides rich, simulated responses based on a serious illness conversation guide, medical studentsrecord themselves having a conversation about advanced care planning. They then review the conversation through VR, where they can see it from the other persons perspective, giving them a tool for critical self-reflection, learning and training. The goal is to help caregivers gain the confidence to talk about sensitive issues.

Munteanu explains that the immersive technology could be used to develop more empathetic and more attentive listening skills that, in turn, help improve the social and personal aspects of palliative care.

Its not that people arent doing all they can, he says. [But]here are so many more opportunities to make it even better.

Meanwhile, Munteanus Technologies for Aging Gracefully (TAG)lab is part of a three-year international research and development project that has received 1.5 million euros from the European Unions Assisted Augmented Living touse of emerging technologies improve the quality of life of palliative care recipients, their family caregivers and professional care providers.

The studies are putting the U of T Mississaugas TAG lab at the forefront of innovation.

Theres a lot of good research on the medical side, Munteanu says, butits time for everything else to catch up.

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Can Taking a Vitamin D Supplement Help You Lose Weight? – Everyday Health

When looking into the connection between vitamin D and weight loss, researchers often use supplements in their studies, rather than tracking a subjects sun exposure or food.

Thats because pills are standardized and can be given in high doses to quickly up a study participants vitamin D level. For example, a study published in July 2018 in the International Journal of Preventive Medicine gave subjects who were overweight or had obesity 50,000 IU of vitamin D (an amount well above the recommended limit of 4,000 IU per day, or 28,000 IU per week, per the NIH) each week for six weeks. Researchers found in this small study that the subjects weight, BMI, waist circumference, and hip circumference all decreased significantly, and their vitamin D levels increased significantly, after taking this high vitamin D supplement regime. However, thats not a safe amount of vitamin D to take for weight loss (or any other reason) in the real world.

Although scientists havent done much research on eating vitamin D-rich foods and weight loss, theyre definitely still worth consuming. What we know is that foods high in D tend to be healthy anyways salmon, mackerel, mushrooms, vitamin D-fortified milk, which are part of a healthier diet, versus processed foods so consuming these would likely help with weight loss, says Agarwal.

And while researchers dont typically track sun exposure, getting a little sun the old-fashioned way isnt a bad idea, but its important to not overdose on sun, which can up your risk of skin cancer, according to Harvard Health Publishing.

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Can Taking a Vitamin D Supplement Help You Lose Weight? - Everyday Health

Pope finances 168 projects in Latin America and the Caribbean – Malaysian Christian News

By Robin GomesThe Popes charitable initiatives in Latin America and the Caribbean are carried out largely through the Populorum Progressio Foundation for Latin America and the Caribbean, operating under the Vaticans Dicastery for Promoting Integral Human Development.

During the annual meeting held online, July 29-30, the board of directors of the Populorum Progressio Foundation selected 138 social development projects from among the numerous proposals, developed by the Latin American and Caribean communities and regions most in need.

In addition to these, another 30 food aid projects already in operation, were approved earlier by the board of directors in June. This was in response to a request by Pope Francis, as a collaboration between the Foundation and the Vatican Covid-19 Commission, which the Pontiff established in March in the Dicastery, in collaboration with other dicasteries of the Roman Curia and other agencies. The 168 projects in 23 countries express the Church's concern and love for the entire human family in the face of the ongoing pandemic.

The board of directors also analyzed the consequences of the coronavirus pandemic in the region. The projects selected aim at helping mitigate the short and mid-term effects of the virus.

At the virtual meeting, Cardinal Peter Turkson, the prefect of the Dicastery, who is the president of the Foundation, thanked and encouraged the members to continue working with dedication and enthusiasm on behalf of those who need their support in this difficult situation.

Among the several participants in the annual meeting were representatives of the Committee for Charitable Interventions in favour of the Third World of the Italian Bishops Conference (CEI), which finances most of the projects. Also present were delegates from Cross Catholic Outreach, an American charity that has been funding a significant number of them since 2018.

In collaboration with the Italian Church, the Foundation aims at promoting the integral human development of farmers communities (campesinos), indigenous peoples and African Americans of Latin America and the Caribbean. This way, it bears witness to the closeness of the Pope through the works of charity that are accomplished.

In the face of this crisis of global proportions that we are experiencing, these projects are intended to be a tangible sign of the Pope's charity, said a statement issued at the end of the meeting. It also appealed to all Christians and people of goodwill to practice the virtue of charity and solidarity ever better, ensuring that during this pandemic "no one is left behind", as the Holy Father Pope Francis has asked.

Founded in 1992 by Saint Pope John Paul II, on the occasion of the 5th centenary of the evangelization of the Americas, the Foundation is headquartered at the Vaticans Dicastery for Promoting Integral Human Development, while its operations secretariat is in Bogot, Colombia.

There are 3 other foundations for papal charities within the Dicastery, namely, the John Paul II Foundation for the Sahel, Justice and Peace Foundation and the Good Samaritan Foundation.Vatican News

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Pope finances 168 projects in Latin America and the Caribbean - Malaysian Christian News

Haiti is Planning to Reopen to Tourists – Caribbean News – caribbeannationalweekly.com

Last week, Myriam Jean, Haitis Minister of Tourism, Raina Forbin President of the Haitian Tourist Association (ATH) and Dr. Yves Gaston Delourches, Representative of the Ministry of Public Health indicated that Haiti is considering plans for the reopening of the country as a tourism destination.

The protocol being planned to reopen the tourism sector aims to reassure tourists and operators of the tourism sector and the staff of tourist establishments of prevention against COVID-19.

Meeting to discuss the protocols for reopening the tourism sector, Minister Jean said, Today more than ever, we must reassure travelers, restore confidence in the tourist chain and have a healthy and quality tourist offer in the context of Covid-19, are the objectives of this protocol, stressing that a team from the Ministry will be set up whose mission will be to monitor the proper application of the measures in all tourist establishments.

Raina Forbin gave assurance the ATH will make provisions to guarantee the health protection of tourism employees and tourists who choose Haiti as their tourism destination Haiti, affirming This is what we can do to prove to the whole world that the country is opening again to tourists by full security, stressing that in all establishments with more than 5 employees the presence of a health worker will be compulsory.

Yves Gaston Delourches, recalled We are not at the end of our troubles it is true that the incidences of COVID-19 are decreasing in Haiti but we must remain vigilant. This is why all infection prevention and control measures are part of any protocol to reopen the country to tourists.

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Javier Bardems black mouth goo in Pirates of the Caribbean, explained – Polygon

With the Pirates of the Caribbean movies more accessible than ever, and a summer season void of blockbusters, this month were diving deep into Disneys swashbuckling series. Grab your cutlass and hoist the colors: here be Polygons take on all things PotC.

After the critical failure and colossal box office haul of 2011s On Stranger Tides, something had to be done to save the stray-but-viable Pirates of the Caribbean franchise.

The answer was obvious: Hire Oscar-winning actor Javier Bardem to dwibble oily spittle fwom his mwouth wike a big piwhate baby.

Though known as a handsome Spanish star, Bardem had a history of playing peculiar baddies before stepping on board Pirates of the Caribbean: Dead Men Tell No Tales. In 2007, he picked up his Academy Award for playing the bolt-stunner-wielding assassin Anton Chigurh in the Coen brothers No Country for Old Men. Five years later, he faced off against James Bond as the blonde, jawless genius Raoul Silva in Skyfall. If the role required hair, makeup, or costume special effects, Bardem was game, and Dead Men Tell No Tales demanded his greatest transformation.

In directors Joachim Rnning and Espen Sandbergs fivequel, the undead captain Armando Salazar appears to be floating in the water even as he walks the dry deck of a ship. His hair ebbs and flows in the air, suspended by an invisible tide. A crackling set of scars give him a facade akin to Frankensteins monster. Plus hes choking on goo! Disgusting amounts of sludge seep out of his mouth as he talks to the mannequin playing Will Turners son.

As mom-blog Tools 2 Tiaras reported at the time of release, Bardem was not fond of the leaky gunk, but was more than happy to reveal the secrets of the ooze. It was a liquid, he said. They told me it was supposed to be like chocolate, chocolate my ass. That tasted worse than that, so, and they were supposed to put it on the teeth. I said give me that, so I drunk it and then I went to play the first scene, I think it was with Geoffrey Rush and it starts to pour out of my mouth and he was very disgusted. [LAUGHTER] And I thought it was like a rage pouring out, right? Its not blood. Its like the rage of the character coming out, like something more physical, like a bull.

We gave Bardem an Oscar for sporting a horrible bowl cut, but he earns a Razzie for spitting pure rage on Geoffrey Rush? Hollywood makes no goddamn sense!

I wish I could say I will never forget the time I saw Javier Bardem heave black grease out of his mouth as he pontificated on the woes of being an undead sea captain, but the truth is I could barely remember whether or not I saw Dead Men Tell No Tales in theaters. All I remembered was a hazy memory of Bardems goop acting. Was it even as gloriously vile as I thought, or had Rnning and Sandbergs messy character choice been fused with another daring act of oral expulsion that I held in high esteem?

Looking back at Dead Men Tell No Tales, which just arrived to Disney Plus in July, and at my own history of watching characters with leaky orifices, the answer is that the secreting Armando Salazar that I knew was more of a construct than I had ever believed. Without being on the set with a measuring cup, Id estimate Bardem spits out about 1/4th of a cup of black good out of his mouth in his first scene. Spooky, but nothing a few paper towels could handle.

So how did I conjure this exacerbated imagined version of Salazar? Who set the bar for spewing liquid out of ones face? After a journey through the mind, its clear that when I saw Dead Men Tell No Tales the first time, I was under the influence of Kids in the Hall. While I think Bardem deserves an Oscar for bringing obsidian spit up to the big screen, Dave Foley deserves at least 14 Emmys for going the distance in 1995.

Foley was a comedic iconoclast who never saw a bag of foul-looking liquid he couldnt hide under his quote and expel for laughs. In another sketch, he went four minutes on a mock date with a stream of blood shooting out of his ear. In Personal, his boss character is the victim of brown stuff coming out of his mouth. Its tremendous.

Kids in the Hall was in constant rotation on Comedy Central in the late 90s and early 2000s, molding the senses of humor of young lads like I. Twenty years later, when Dead Men Tell No Tales graced the screen, my brain was ready for Armando Salazar to close-talk spit all over his victims while enunciating his words. Foley ran the first leg of the race, and Javier Bardem grabbed the baton. But the performance didnt sit well with audiences who werent as familiar with the art of performative gushing: The movie once again made millions around the world, but wound up with a dismal 30% on Rotten Tomatoes.

Though Salazar met his end in the final scenes of Dead Men Tell No Tales, Rnning and Sandberg are set to return as directors of Pirates 6. To them I would say: double down. Hire Dave Foley. Get the black goo crankin this time. People understand now.

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Javier Bardems black mouth goo in Pirates of the Caribbean, explained - Polygon

See the ‘space butterfly’ astronomers captured from thousands of light years away – CNN

So named for its resemblance to the winged insect, the "butterfly" is actually a planetary nebula -- a giant cloud of gas that forms around an ancient star that hasn't yet exploded. The European Space Observatory's (ESO) aptly named Very Large Telescope, stationed in host country Chile, recently captured a vibrant image of the interstellar object.

It's known as NGC 2899 (NGC stands for New General Catalogue, which lists nebulae and other astral bodies like this one). It's located somewhere between 3,000 and 6,500 light years away from Earth in the constellation Vela, which is visible in the Southern Hemisphere.

This planetary nebula isn't long for this universe. Ultraviolet radiation lights up the shells of gas surrounding the star and causes them to shine quite brightly, the ESO said -- but only for a few thousand years before they break up. That's a relatively short life span in astronomy.

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See the 'space butterfly' astronomers captured from thousands of light years away - CNN

Astronomical First: Differences Detected Between Discs of Active and Non-Active Galaxies – SciTechDaily

A study led by researchers at the Instituto de Astrofsica de Canarias (IAC), making comparison between the discs of several pairs of spiral galaxies, active and non-active, concludes that in the discs of the former the rotational motion of the stars is of greater importance. This study, just accepted for publication in Astronomy & Astrophysics Letters, is the first evidence for large scale dynamical differences between active and non-active galaxies in the local universe. The astronomers participating are from the Instituto de Astrofsica de Canarias (IAC) and the University of La Laguna (ULL); as well as the NatiAstronomical First: Differences Detected Between Discs of Active and Non-active Galaxiesonal Autonomous University of Mexico (UNAM), the Complutense University of Madrid (UCM) and the Instituto de Astrofsica de Andalucia (IAA).

There is now evidence that the supermassive black holes at the centers of the majority of galaxies have a basic influence on their evolution. In some of them, the black hole is ingesting the material surrounding it at a very high rate, emitting a large quantity of energy. In those cases we say that the galaxy has an active nucleus (AGN). The material which feeds the AGN must initially be quite distant from the nucleus, in the disc of the galaxy, rotating around its center. This gas must, one way or another, have been braked in order to fall into the central zone, a process known as loss of angular momentum.

Image illustrating the comparison between an active spiral galaxy (orange box) and its non-active twin (blue box). Credit: Gabriel Prez Daz, SMM (IAC)

Studying the mechanisms which control the relation between the active nucleus and the rest of the galaxy -explains Ignacio del Moral Castro, a doctoral student in the IAC and the University of La Laguna (ULL) and first author of the article- is necessary to understand how these objects form and evolve, and to be able to throw light on this question we need to compare active and non-active galaxies. With this purpose, the main idea of my doctoral thesis is centred on the study and comparison of galaxies which are almost twin, but with the difference being nuclear activity.

The work has consisted of comparing the dynamics of the galactic discs of various active/non-active pairs. The researchers used data from the CALIFA survey (Calar Alto Legacy Integral Field Area). This contains spectroscopic data over complete 2D fields for more than 600 galaxies, taken at the Calar Alto Observatory in Almera, which allow observations of virtually the whole of each galaxy, so that its global characteristics can be studied.

Previously, in the majority of studies the procedure used was the identification of a sample of active galaxies within a large survey, which were then compared to the rest of the galaxies in the survey having similar properties that do not show nuclear activity. However, this time, the researchers used a novel method: they performed one-to-one comparisons. Firstly, they identified active spiral galaxies in the CALIFA sample, and for each of them they looked for a non-active galaxy which had equivalent global properties, i.e. with the same mass, brightness, orientation and so on, and very similar in appearance.

Using this method the team put forward two scenarios to explain the dynamical differences between active and non-active galaxies. In the first, the explanation would be that it is the trace of the angular momentum transfer between the gas which has fallen into the centre and the material which remains in the disc. The second attributes the difference to the infall of gas from outside, via the capture of small nearby satellite galaxies, in which case, this capture should occur more frequently in the active galaxies. Both scenarios are compatible with this result and they are not mutually exclusive.

The result surprised us; we really didnt expect to find this type of differences on a large scale, give that the duration of the active phase is very short in comparison with the lifetime of a galaxy, and with the time needed to produce morphological and dynamical changes, says Begoa Garca Lorenzo, and IAC researcher, and a coauthor of the article.

Up to now we thought that all galaxies go through active phases during their lifetimes, but this result could mean that this is not the case, which would imply a major change to current models, adds Cristina Ramos Almeida, also an IAC researcher and coauthor of the article.

Reference: Larger R in the disc of isolated active spiral galaxies than in their non-active twins byI. del Moral-Castro, B. Garca-Lorenzo, C. Ramos Almeida, T. Ruiz-Lara, J. Falcn-Barroso, S.F. Snchez, P. Snchez-Blzquez, I. Mrquez and J. Masegosa, 14 July 2020, Astronomy & Astrophysics Letters.DOI: 10.1051/0004-6361/202038091arXiv: 2006.12654

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The best place to see stars from Earth also happens to be the coldest place on the planet – Space.com

If you want the clearest view of the night sky, you'll have to pack a warm jacket.

Dome A, or Dome Argus, an ice dome perched high on the Antarctic Plateau, could be the ideal place to get a clear view of the stars from Earth, according to a new study conducted by an international team of researchers. A telescope situated at that remote location, thought to be the naturally coldest place on Earth, could reveal clearer, better night sky views than the same telescope located anywhere else.

"A telescope located at Dome A could out-perform a similar telescope located at any other astronomical site on the planet," University of British Columbia astronomer Paul Hickson, a co-author of the study, said in a statement.

Related: Night sky, August 2020: What you can see this month [maps]

"The combination of high altitude, low temperature, long periods of continuous darkness, and an exceptionally stable atmosphere makes Dome A a very attractive location for optical and infrared astronomy. A telescope located there would have sharper images and could detect fainter objects," Hickson said.

The chilly location, which is about halfway between the South Pole and the eastern coast of Antarctica, about 746 miles (1,200 kilometers) inland and with an altitude of 2.5 miles (4 kilometers), makes for an ideal observing spot for a number of reasons.

For one: it has very weak turbulence. In astronomy, atmospheric turbulence can seriously reduce a telescope's image quality. It makes stars "twinkle," and the measurement of this effect is described as "seeing." Less turbulence (or the lower the "seeing" measurement) is considered better, and at Dome A it is fairly low.

While observatories in locations along the equator at locations including Chile and Hawai'i have "seeing" measurements between 0.6 and 0.8 arcseconds, the Antarctic typically has much lower ranges. For example, Dome C, another Antarctic location has a "seeing" range between 0.23 and 0.36 arcseconds.

But, the authors estimate in this study, the lowest part of the atmosphere is thinner at Dome A than at Dome C. Because of this difference, the researchers calculate that Dome A has nighttime seeing ranging from 0.31 to as low as 0.13 arcseconds, which is astoundingly low.

The researchers found that the measurements taken from Dome A, which were taken at a height of 26 feet (8 meters), were much better than those from Dome C, which were taken both at 26 feet (8 meters) and even higher up at 66 feet (20 meters).

Now, with seriously frigid temperatures, frost is an issue that presents itself to astronomers looking to set up a telescope at the site. But, despite the technical difficulties that pop up when trying to make observations at a site this remote and cold, this team of researchers thinks that Dome A could lend itself to some pretty spectacular skywatching.

The researchers were able to have a telescope work in Antarctica completely automatically for seven months. They believe that other instruments could withstand the Antarctic temperatures, which have been said to fall as low as 90 C (130 F) to 98 C (144 F).

This work was published July 29 in the journal Nature.

Email Chelsea Gohd at cgohd@space.com or follow her on Twitter @chelsea_gohd. Follow us on Twitter @Spacedotcom and on Facebook.

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TAAL Files Second Patent for Layer 1 Token Technology to Enable Smart Contracts Built on Bitcoin SV and in Direct Competition to Ethereum ERC-20…

VANCOUVER, BC, Aug. 6, 2020 /PRNewswire/ -TAAL Distributed Information Technologies Inc. (CSE: TAAL) (FWB: 9SQ) (OTCQB: OTC: TAALF) ("TAAL" or the "Company") announces that its operating subsidiary has filed a second patent application (the "Patent Application") with the United Kingdom patent office with respect to its newly acquired Layer 1 token blockchain technology for the BSV (Bitcoin SV) network.

Layer 1 tokens are validated by computers operating on the blockchain directly, unlike more common Layer 2 token systems which require separate Layer 2 protocol servers. Processing transactions directly on the network is synergistic with TAAL's vision and roadmap for its core business of blockchain transaction processing as it allows different ways of creating more transactions and thus facilitates an expansion of the fee market available to TAAL. The fee market is an important pillar of TAAL's revenue strategy.

Bitcoin SV has proven scalability in both transaction volume/capacity and block size that has been demonstrated on the BSV stress test network (1 gigabyte sustained) and BSV main network (360 megabyte peak) that is unequaled by any other blockchain technology. Jerry Chan, TAAL's CEO, said "We are proud to be involved in delivering this ground-breaking initiative to market and look forward to working with our enterprise clients and development partners to expand the ecosystem for smart contract technology on the Bitcoin SV platform."

Layer 1 tokens, to this point, has been primarily the domain of Ethereum, whose ecosystem of Layer 1 tokens is currently recognised as the largest in the blockchain industry, and this technology opens the door for the migration of legitimate tokens that require enterprise level scaling to the Bitcoin SV network.

In April 2020, TAAL entered into a US$1m licensing deal with nChain Group Holdings Limited ("nChain") to secure access to critical IP to support its development of transaction processing capabilities. This patent builds on top of nChain's extensive intellectual property portfolio and creates an array of opportunities for innovative and disruptive solutions which are at the heart of the blockchain technology delivered by Satoshi Nakamoto when he published his Bitcoin white paper in 2008.

The Patent Application will underpin the launch of associated technologies and platforms and reinforces Bitcoin SV's position as the leader for enterprise use cases.

In consideration of acquiring the intellectual property underlying the Patent Application, TAAL's operating subsidiary has entered into a royalty agreement with the inventor.

Developers and enterprise clients wanting to discuss use cases and/or access to this Layer 1 token technology should contact TAAL via [emailprotected].

About TAAL Distributed Information Technologies Inc.

TAAL is a Canadian-based technology company leading in enterprise scale blockchainbased information management and security through Bitcoin SV and other SHA-256 based digital asset platforms.

The CSE, nor its Regulation Services Provider, accepts no responsibility for the adequacy or accuracy of this release.

CAUTIONARY STATEMENT REGARDING FORWARD-LOOKING INFORMATION

Certain statements included in this news release constitute "forward-looking information" as defined under applicable Canadian securities legislation. The words "will", "intends", "expects" and similar expressions are intended to identify forward-looking information, although not all forward-looking information will contain these identifying words. Specific forward-looking information contained in this news release includes, but is not limited to statements regarding: the expansion of the transaction processing fee market, the launch of technologies and platforms associated with Layer 1 tokens and the viability of the BSV network as an alternative to the Ethereum network. These statements are based on factors and assumptions related to historical trends, current conditions and expected future developments. Since forward-looking information relates to future events and conditions, by its very nature it requires making assumptions and involves inherent risks and uncertainties. TAAL cautions that although it is believed that the assumptions are reasonable in the circumstances, these risks and uncertainties give rise to the possibility that actual results may differ materially from expectations. Material risk factors include the future acceptance of Bitcoin SV and other digital assets and risks related to information processing using those platforms, the ability for TAAL to leverage intellectual property into viable income streams and other risks set out in Item 20 Risk Factors of TAAL's Form 2A Listing Statement dated July 31, 2018 and elsewhere in TAAL's continuous disclosure filings available on SEDAR at http://www.sedar.com. Given these risks, undue reliance should not be placed on the forward-looking information contained herein. Other than as required by law, TAAL undertakes no obligation to update any forward-looking information to reflect new information, subsequent or otherwise.

SOURCE Taal Distributed Information Technologies Inc.

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Washington Must End the Russian Roulette in Moldova – Geopoliticalmonitor.com

One year ago, the Republic of Moldova was plunged into constitutional crisis. Foreign diplomats, from EU Enlargement Commissioner Johannes Hahn to US Ambassador Derek Hogan, hailed a new democratic era for the country. Their remit was to prevent Chisinau from suffering the same fate as Kyiv. Despite their noble claims, the result has been disastrous. Pro-European economist Maia Sandu served as prime minister for just four months, before she was purged from office by the international communitys other coalition partner, President Igor N. Dodon. Meanwhile opposition leader and US ally Vladimir Plahotniuc is seeking asylum in the United States. In recent days, Interpol has refused to issue the red notice sought by the Russian Federation against the businessman, on grounds that his arrest is politically motivated. This corresponds with a report from the government of Estonia which details a long-term campaign to destroy Plahotniucs name via election interference, cyber attacks and online propaganda. Given his long-time relationship with politicians on both sides of the aisle, including senior members of the current administration, the United States failure to support a key anti-Kremlin ally is undermining American influence in Russias backyard. Unless the State Department allies with Putins enemiesthere are fewer more prominent than Plahotniucwe will cede Moldova to Moscow. War, as in Kyiv, is perfectly possible in Chisinau. We must act now.

On Moldova, some Western diplomats were dishonest. Others were misled. The majority were disinterested and misguided. While elevating Sandu to the office of Prime Minister was a rational reform, Plahotniucs experience in officewhich was certainly imperfectstill underwrote stability in a quasi-democracy facing crisis. Instead, personal disputes with junior U.S diplomats in Chisinau appear to have colored Ambassador Derek Hogans view on which coalition party to pick as a partner. These were in Hogans interests, but not the United States, as time has now proven. Hogan pushed for Igor N. Dodon to remain president despite the fact that Moldovas president considers Vladimir Putin a personal friend, and the fact that his brother counts the Russian Prosecutor General Yuri Chaikas son as a business partner. Now, Dodons dictatorship is no less deadly than that which Viktor V. Yanukovych created in Ukraine. Authoritarianism on the European Unions eastern border has flourished in the smokescreen created by the COVID-19 pandemic. After months of testimony on the Mueller probe and President Trumps exoneration, it is apparent that Russias malign influence on democracy is real. The consensus is bipartisan. It is also bilateral. Great Britain has learned that Russia was able to influence referendum outcomes. As the U.S presidential election nears, we should view this threat with real concern, and continue to build relationships with our friends in the region. Moldova provides a case in point for what can go wrong when we underestimate our enemys power. Through poor communication, we have ending up backing the Kremlin and its proxies. We have also enriched Putins inner circle, and its most powerful oligarchs.

During three decades of attempted reform, the United States and the European Union have fought tooth and nail to install some semblance of plurality in Moldovaa nation facing a geopolitical threat from Russia, and one that is also in the throes of a post-Communist identity crisis. Unlike some of its neighbors, Moldovas deep suspicion of Russia, and reservations about the European path have become logical constructsbased on the Nazi Anti-Aggression Pact, which split the state from Romaniabefore handing the state to Stalin. Churchill did not intercede. Neither did NATO. When Russian separatists tried to split the nation in two, during a vicious civil war that raged in the early 1990s, a swathe of Moldova attempted to secede. Guarded by peacekeepers from the Russian Federation, Transnistria is still trapped in a frozen conflict with Moldova now. Moldovans concurrently accept the cruelty of geopolitics when it comes to state building. While the Baltic states moved to plurality, post-Communist Moldova suffered two-fold insanity of transition to a market economy, under the oxymoronic madness of rule by a post-Communist Communist Party. Maia Sandu was not a product of that government. Neither was Vladimir Plahotniuc. Tellingly, the former Communist whom we picked to steer Moldova in 2019 is now the Wests handpicked president. We can all agree that Dodons past is ugly. A large number of Moldovans, and their media outlets, accuse Dodon of actions in the present that are even more unsavory. To others, Dodons use of fabricated scandals to fell his critics are criminal acts.

Since Plahotniucs arrival in the United States, independent media outlets have leaked video footage which shows Moldovas pro-Kremlin President extorting Plahotniuc for several million dollarsin footage where Dodon apparently explicitly confirms financial support of the Kremlin for the Socialist Party of Moldova. By this time, Plahotniuc had already survived two assassination attempts in opposition politics, and faced anothereven without the payment that Dodon allegedly requested. Maia Sandu suffered no less humiliating attacks. Media outlets controlled by President Dodons brother undermined the young female reformer by misreporting a deal she had allegedly signed with Chancellor Merkel that would grant Syrian refugees residence in Moldova. Dodonwho is a strident homophobealso used his family affiliated media empire to stoke hatred against the gay community, by using a photograph of Sandu crossing the road with another woman to prevaricate about her sexuality. These attacks are thought to have granted Dodon the percentage points needed to defeat Sandu in the presidential election. This is not what Euro-Atlanticist foreign policy should endorse. The Moldovan electorate feels likewise.

Half the country has left to seek work abroadwith as many as two million migrants now working off the book in the European Union. As migrant workers who clean apartments, labor on construction sites, and tend to livestock, they supported the principal of Europe by supporting Moldova. In the political chaos preceding 2009, Moldovans wired billions in remittance income home. This made the country the worlds second highest dependent on foreign labor in the world. A European Moldova, aligned with the European Union, should mean a Moldova built on worka quality which Americans understand so readily. We risk undermining our hard work, and theirs, unless we act quickly and decisively. Mistakes were made in 2019. If we dont intervene, there will soon be no time to right our errors. Anyone versed on Moldovas plight would recognize that the constitutional crisis of 2019 gave Western diplomats a simple choice, which demanded compromisenot iconoclasm. Sadly, John Bolton had only just been dismissed, creating obvious communication gaps with Mike Pompeos team. This is certainly not the United States problem, especially as both House and Senate were preoccupied with the Mueller probe. Less sympathy is owed to Ambassador Hogan, or his European colleagueswho saw intervention in Moldova for short term benefit as an opportune time to secure a good press release. This publicity victory for an embattled European Union has imperiled Moldova. The individuals responsiblebesides Hoganare no longer in office.

Sticking with Vladimir Plahotniucs powerful, and at least partially effectual Democratic Party, meant recognizing that things hadnt gone to plan. This editorial must not be read to mean this. Rather, this editorial posits the importance of realpolitik in a difficult region, and the recognition that a period of progress with Plahotniuc warranted compromise during the negotiations of 2019. Even Plahotniucs critics concede with the benefit of hindsight that compromising with the former PDM leader was preferable to clearing the path to a Dodon presidency.

Due to personal disputes, the vested opinions of several diplomats, a breakdown of communication with the State Department, and rifts in the European Union, Moldovans believeas they have right tothat the West has abrogated all responsibility for the foreign policy atrocity that now constrains their lives. Plahotniuc has always shown a clear preference for the GOP, with his relationship with the Republican Party likely pinned on its economic message and shared belief in the threat posed by the Russian Federation. Maia Sandu is a gifted politician, and proven reform advocate, who also deserves our supportthough she has often experienced difficulties in standing strong against Russias geopolitical games, and standing firm against Putins aims. The GOP now seems the only force capable of wrenching the state from Vladimir V. Putins appointee, and preventing Moldovas literal absorption by Russia. Unless we act soon, the billion-dollar legacy of foreign aid and bilateral relationships built between Chisinau and Washington will be that we, the West, ceded Moldova to Moscow by reckless negotiationbefore handing the keys to Vladimir Putins puppet. And turning off the lights.

The views expressed in this article are those of the authors alone and do not necessarily reflect those of Geopoliticalmonitor.com or any institutions with which the authors are associated.

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Washington Must End the Russian Roulette in Moldova - Geopoliticalmonitor.com

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Superstitions and Gambling – Ways That Gamblers Are Superstitious – BestUSCasinos.org

Here is the dictionary.com definition of superstition:

Superstition: [ soo-per-stish-uhn ], a belief or notion, not based on reason or knowledge, in or of the ominous significance of a particular thing, circumstance, occurrence, proceeding, or the like.

We all have our superstitious beliefs, like dont cross the path of a black cat, dont walk under a ladder, or make a wish when the clock reads 11:11.

When we were little girls, my sister and I thought if we held our breath when we passed a cemetery until we saw a church, the ghosts of the dead wouldnt get our souls.

What happens if there is no church for like five miles?

You pass out, Beth. Thats what.

I know because it happened to me.

You know who a very superstitious bunch is?

Gamblers, thats who.

Is this because this is really a hobby of luck and chance?

Is it because we are human and want to control things that are not humanly possible to control?

This post looks at the popular superstitious beliefs in gambling and why humans (gamblers specifically) are superstitious.

There are a lot of superstitions within the gambling community. Here is a list of the top seven gambling superstitions:

Many gamblers will not accept their payouts in American $50.00 bills. This superstition has Mafia ties. In the heyday of the American Mafia, when a mob member would kill someone, they would leave a $50.00 bill in the victims pocket when they buried the body.

This superstition is tied to Asian cultures, specifically Chinese culture. The Chinese believe that red represents wealth and luck.

If you look closely, many casinos will have red in their dcor. A lot of gamblers will wear red shirts or even red socks when they are gambling at a casino.

I couldnt find any history of the explanation of this one. Many gamblers believe that using a side entrance will increase their chances of winning.

When the MGM Grand opened in 1996, the casinos main entrance was through a large lion. This was lousy juju for many visitors.

Not only were they wary of using the main entrance, entering through the beasts mouth was even more bad luck to some Chinese gamblers.

The MGM eventually changed the entrance to more traditional doors. They replaced the original lion with a 100,000-pound bronze statue of a lion above the entrance.

You never count your money when youre sitting at the table, therell be time enough for counting when the dealings done. ~ The Gambler by Kenny Rogers.

It is believed by many gamblers that its bad luck to count your money while still at the table. Some casinos take this superstition so seriously that they advise their visitors not to count their money while at their tables.

This superstition most likely has ties that go back to a much more polite time. It is said that if you cross your legs while gambling that you will cross out your luck.

I have a theory on this one, and I couldnt find any history to back the origins of this superstition. So here it is:

Ladies were discouraged from gambling. Theyre still are a tiny minority in real money poker tournaments. Women crossed their legs when they sat as per societal rules.

So, if youre expected to sit when you gamble at a table, youre (women) expected to cross your legs. If women were discouraged from gambling, a mens game, then it would make sense it would become a superstition to cross their legs while gambling.

Just my two cents. Do with it what you will.

The number 13 has been bad luck as long as I can remember. It even signifies death in some cultures. This superstition goes deeper than gambling.

Have you ever noticed that hotels dont have a 13th floor?

Its because of this long-held belief that this is an unlucky number.

Hotels usually do have a 13th floor. It is just not listed on the directory or elevators. This dreaded floor is traditionally used for housekeeping and maintenance needs.

Many gamblers believe that black is an unlucky color. Its the color equivalent of the number 13.

This superstition is unfortunate for roulette and card game players because black is a significant color. Roulette only has two color choices, red and black.

Could you imagine never betting on black when playing roulette?

Youre cutting your chances in half.

Whistling or singing at a table is said to anger the gambling gods. To be honest, its kind of just plain annoying.

We are all at this table for the same goal to win some money. Winning money while gambling takes concentration. If someone is singing or whistling at the table, that is distracting. Come on, man.

So besides possibly angering the gambling gods by whistling or singing during a game of Texas hold em, you are probably annoying your table mates. Dont be that guy.

This is not all the superstitions that gamblers have, by any means.

Do any of these works?

Maybe.

But gambling is a combination of skill and chance.

Who knows if they do work?

Humans like to believe theyre in control, and by believing in these superstitious practices, you might just convince yourself you have a leg up.

Humans are weird. Lets just get that on the table. We are the only species that wont step on a crack in the sidewalk because it could bring us bad luck.

Maybe its our highly developed brains that give us the ability to convince ourselves if we do this one thing, this other thing (that has nothing directly to do with the other) wont happen.

I did some research. I was reading on the basics behind humans propensity for superstitious beliefs. I found some interesting stuff.

Besides the fact that we really like to get ourselves worked up into a frenzy of our own making, superstitious beliefs seem to be linked to when we were new to this planet.

If a human, lets call him Peter, is out hunting and gathering, and he hears grass blowing in the wind, he might run. Last week, Peter heard the same sound, but it was a lion stalking him for dinner.

It doesnt matter what caused the grass to make noise, Peter knows it could be a threat to his life. Run or be killed. It is better to run, and its just the wind than not running and it being an actual lion.

This is a fight or flight response. Peter goes on to teach his family (possibly the tribe) that you should run if the grass makes any noise. Better safe than sorry.

This newfound tactic against the lions has proven to work. Only two people have been killed by the lions this month. So now humans run if the grass makes noise.

As humans evolve, grass making noise in the wind might become a sign of bad luck because of our ancestors need to not be eaten alive.

See where this is going?

Humans do what they must to survive. When we first got here, there were a lot of things and animals that couldve ended us. Because we have such an advanced problem-solving brain, we can make choices that save our lives.

So that grass blowing in the wind could be why now its bad luck to whistle at the table.

I dont know the historical evolution behind whistling, but it makes sense in my head, right?

Its just like red being a lucky color. Somewhere in the Chinese culture, it gave someone a leg up over someone else. Their luck continues, and now they only wear red when they need good luck.

Red now equals luck in Chinese culture. These beliefs bleed over into other cultures as time goes on. Now red is a universal sign of luck.

The takeaway is that superstitious beliefs evolved out of the need for survival. The grass blowing in the wind was so ingrained in the early human society that when the threat of being a lions lunch disappeared, the fear stayed.

That fear evolved with whatever the new or next threat represented. So, Peters running from the grass is now not applicable, but its part of our evolution. Just like red, 13 is an unlucky number. You get the gist.

When it comes to gambling, were looking for the easiest way to increase your luck. Skill will only get you so far. SO that arcane thing that you think helped you win that one time is now a belief. Gamblers are a superstitious crowd and for a good reason.

There are a ton more superstition that I didnt include. There are some crazy ones out there. Like did you know in Malta, if your right hand itches youre about to give away a bunch of money?

Id hate it if it were true.

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From the Italian Renaissance to the stars: an exciting approach to fulfilling GEs > News > USC Dornsife – USC Dornsife College of Letters, Arts…

Two pioneering, new general education courses come online for this fall, offering students a richer, broader way to learn and to acquire diverse academic skills. [7 min read]

The ItalianRenaissance has long been considered the bastion of powerful Renaissance men, such as Michelangelo and Leonardo da Vinci, whoseachievements have traditionally defined the period. A new general education (GE) course will challenge this premise by exploring gender, religion, sexuality and race through both art and literature.

The course is one of two new integrated GE online courses being offered this fallby USC Dornsife College of Letters, Arts and Sciences as part of a pilot program that brings faculty experts together from different fields to give students an in-depth exploration of topics from more than one disciplinary perspective. These pioneering courses aim to teach students innovative ways of thinking.

Several years of planning have gone into the design of the courses, which are part of a larger effort by USC Dornsife to provide exciting educational opportunities for all students.

The courses will not be taught every year, so if students are interested, they are advised to enroll now.

The Italian Renaissance: a new perspective

Margaret Rosenthal, professor of Italian, comparative literature and English, and Lisa Pon, professor of art history, offer the literary and visual immersion into Renaissance Italy. Their eight-unit paired course unfolds in twice weekly three-hour classes;each professor will teach 80 minutes back to back with a break in between each class.

Pon will teach the arthistory/visual culture part of this integrative GE, Art, Power and Identity in Renaissance Italy (AHIS 304m),while Rosenthal will teach Gender and Sexuality in Renaissance Italy (ITAL 350g).

Rosenthal and Pon describe the integrative GE as two courses in synergy that will offer a fuller and richer picture of the period.

Professor Rosenthal is going to look at poetry and texts, and Im going to look at pictures and think about spaces, Pon says.

Everything taught in Professor Rosenthals class is going to be built upon and expanded by my class and vice versa, Pon says.

By taking this pair of courses, students will learn to harness a number of different skills from discovering how to look at different types of evidence, exploring texts, looking at hand-held objects, thinking about what it means to read a picture all of which will help to set them up academically for the rest of their degree.

Challenging traditional perspectives

Rosenthal notes that women played a strong role in Renaissance literature, through their participation in literary salons and as patrons of literature and the arts, while both sexes during this period challenged restrictive and traditional notions about gender,religion, race and sexuality.

Students will study Michelangelos love poems to a young male aristocrat as well as his intense, spiritual sonnets to an aristocratic woman poet from Rome, in which he shares with her all of his spiritual doubts and worries about salvation as a result of his desires for same-sex love.

Well also look at a courtesan poet who is selling her body for financial gain but also having a lot of difficulty with her male patrons, Rosenthal says. She wants to assert herself, and we see moments when they want to either honor her or take her down as a scapegoat for the plague of Venice because shes becoming too powerful in Venetian society.

Course work will range from creative writing projects, in which students are invited to emulate a celebrated writer of the period, to mapping the journey of four teenage boys who traveled from Japan to Rome to see the Pope in 1580.

Incorporating new voices

Pon says she finds it exciting to expand thinking about the Renaissance beyond its traditionally acclaimed figures mostly white, male and privileged to incorporate other voices and experiences.

When we discuss popes andmilitary heroes, we also read love poems, letters and essays by courtesans, widows andnuns, she and Rosenthal wrote in their course description. When we consider the lives of Catholics, we will also study thevaried experiences of pagans, Jews, Muslims, and Moors.

So why is it useful to study the Italian Renaissance?

One reason is because it was a period in which a certain society was coming to terms with the fact that they were far more multicultural than they maybe wanted to admit, Pon says. To try to capture that, and improve our understanding of it, is a way for us to better comprehend and deal with our own time.

To that end, Rosenthal plans to start the course with Boccaccio's Decameron, a collection of stories written about individuals escaping an epidemic of bubonic plague, which she plans to connect with the current pandemic.

Pon thinks the fact that the course reflects issues we are currently dealing with, such as gender equality, Black Lives Matter and the pandemic, makes the course particularly approachable.

Its a way for students to understand and have tools for the world theyre living in now, she says.

Representing physics and astronomy through the arts

Vahe Peroomian, associate professor (teaching) of physics and astronomy, will teach The Physical World and the Universe (110Lxg) and Dana Milstein, assistant professor (teaching) of writing, will teach Representations of Physics and Astronomy in the Arts (111xg), as an integrative course which marries basic, conceptual physics and astronomy with a visualization of the sciences and the arts.

Peroomian and Milstein say its very rare, and possibly even unique, to find an integrative course of the type that USC Dornsife is offering that is co-taught as one course and that offers equal weight and relevancy in both physics and humanities or social sciences.

Peroomian points out that the course is much greater than the sum of its parts.

You can take the physics 100 course or the astro 100 course separately, you can take any visualization course or any humanities GE course, but each will give you their own silo, without really broadening and applying that knowledge, he says.

Because were going to be teaching this course together in the classroom at the same time and bouncing ideas off each other, were going to be talking about ideas that we couldnt even cover had a student taken these two courses separately with separate professors.

Students will read articles and writings that they never would be exposed to in a pure science GE class and seeing concepts that they wouldnt see in a humanities or an arts GE course, Peroomian explains.

The integrative course, Milstein says, emerged from the idea of human imagination.

While we dont always have the technology or the knowledge to understand our universe and astrophysics, what we do have is imagination, she notes. Scientists use that to help develop very complex, sophisticated ways of creating theories about the way the universe works that they cant even confirm.

For me, that mirrors how musicians, artists, photographers and movie makers also use their imagination to think about space, Milstein says. So, our course is really about the human mind and the human experience and trying to see what the commonalities are and how we have these overlaps, these synchronicities.

Acquire new skills

Milstein says the course doesnt focus uniquely on gaining expertise on the subject matter: Its also a model for how they want students to approach learning from their freshman year onwards.

This is really a course that teaches students how to inquire, how to discover, how to experience, and how to fail forward, she says.

Students on the course will learn a wealth of skills, including how to compose music, how to take photographs, how to do presentations, and how to not only conduct experiments, but also design them.

If students are looking for a class where theyre active agents in designing their learning, taking ownership of it and then transferring it out to real world practice, thats what they will get from this course that theyre not going to get anywhere else, she says.

One of the topics students will explore is the night sky, looking at scientific principles and exploring how humanists and social scientists have approached the same topic.

Peroomian will teach students how to create a star trails picture to visualize the rotation of the Earth and understand how the ancients misinterpreted that as the Earth being the steady and unchanging center of the universe and everything revolving around us.

Milstein will provide the humanities complement, exploring the lifecycle of the stars, the concept of relating to how stars are formed and how we understand our spatial placement with them. Students will read creative works by poet Adrienne Rich, look at how different cultures have mapped the stars and build their own digital map.

We really want to touch on all the learning points to be able to help students expand their minds, Milstein says. In a year from now, they may not remember anything about astrophysics or what Adrienne Rich or Isaac Newton had to say about the universe, but they will still have a trace of these skills that are going to carry over into their other fields and even their interaction with their family members and their friends and ultimately their careers.

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This Is How It All Ends – The New York Times

One is the Big Crunch. We know the universe has been expanding since the Big Bang. That is to say, space itself is expanding: Galaxies, stars and all other things in the cosmos move farther and farther apart. Its possible that the expansion will eventually slow, stop and reverse itself, like a ball thrown up in the air that then comes back down. And then? Catastrophe. High-energy particle jets and radiation from stars condense and ignite a conflagration. Nuclear explosions tear through stellar atmospheres, ripping apart the stars and filling space with hot plasma, Mack says. At this point, things are really very bad. You can tell shes enjoying this.

Alternatively, the expansion keeps on going until everything attenuates and fades into nothingness. This cosmic endgame is the one known as heat death. Youve heard of entropy: the inexorable tendency toward disorder described by the second law of thermodynamics. Its entropy that does us in. This scenario is a slow and agonizing one, Mack says, marked by increasing isolation, inexorable decay and an eons-long fade into darkness. Everything tends toward equilibrium, and equilibrium means death. Stars burn out, galaxies fade into darkness, even black holes evaporate. This notion has been with us since the development of thermodynamics in the 19th century. H. G. Wells visualized it this way in The Time Machine: It would be hard to convey the stillness of it. The darkness thickened. All else was rayless obscurity. A horror of this great darkness came on me.

Other possibilities involve dark energy, a still poorly understood business that seems to be the dominant component of our universe. A dark-energy apocalypse could tear apart the very fabric of reality, rendering any thinking creatures in the cosmos helpless as they watch their universe being ripped open around them, Mack says. Some paths to destruction arise from theories that involve parallel universes lurking in extra dimensions. A so-called ekpyrotic scenario imagines collisions of branes, three-dimensional universes ordinarily invisible to one another. At the fringes, the cosmological theories with the best jargon and cleverest names are often the most speculative.

Forty years ago, when much of this science was new, the physicist Freeman Dyson complained that some of his colleagues felt it was disreputable to study our universes destiny. He urged them to do it anyway. If our analysis of the long-range future leads us to raise questions related to the ultimate meaning and purpose of life, he wrote, then let us examine these questions boldly and without embarrassment.

This might seem like the wrong time for a book peering billions of years into the future to examine the ultimate doom and destruction. We have doom and destruction of our own to worry about, arriving faster and faster. These days many people wake up wondering if well make it past November. Plague is rampant. The Arctic Circle is on fire. Still, I found it helpful not reassuring, certainly, but mind-expanding to be reminded of our place in a vast cosmos. Mack puts it this way: When we ask the question, Can this all really go on forever?, we are implicitly validating our own existence, extending it indefinitely into the future, taking stock and examining our legacy.

It seems safe to say, though, that any meaning and purpose will have to be found in ourselves, not in the stars. The cosmic end times will bring no day of judgment, no redemption. All we can expect is the total obliteration of whatever universe remains and any intelligence that still abides there.

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This Is How It All Ends - The New York Times

Ben Collins The Stig Top Gear | Surrey – Surrey Life

PUBLISHED: 11:50 07 August 2020 | UPDATED: 14:58 07 August 2020

Ben Collins

Ben Collins was The Stig on Top Gear for eight years. Image: Dickie Dawson

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Surrey life began for me in 2002 when I got lost driving over the hogs back on my way to an interview. Sat nav was still a futuristic vision, one that only led you to the first few digits of a post code, and the former secret military base I was looking for wasnt on there.

The picturesque villages around Godalming with their pretty red brick buildings and ornate greens came as something of a surprise being so close to London. There was no time to savour the view because I was in danger of being late so I thumped through the gears to reach my destination.

As an aviation buff, Dunsfold Aerodrome was a heavenly facility with its history as a World War 2 fighter base and subsequently where the Harrier Jump Jet was developed. Past the security gates and a knackered Hawker Hunter jet fighter there were some large, tired iron sheds that turned out to be the grandly renamed Top Gear studios. A dilapidated portable office overlooked the figure-8 section of tarmac that was to become home for the next eight years.

It was here that I met the orchestrator of the program, Andy Wilman, as he shuffled out of his car bearing a clutch of folders. He ushered me into a Ford Focus and I lapped the circuit while he timed me on a stop watch. It was a hot day and the brakes did well not to catch fire. As for my progress I was none the wiser on whether I had passed muster until I received a call booking me for my first job on the program as a character called The Stig.

Not far away was another mecca of speed at Brooklands aerodrome and racing circuit near Weybridge, a venue that features heavily in my book about Aston Martin. Brooklands was built to gargantuan proportions to accommodate the fastest machines in the world back in 1907 but it was so well designed that with a little preservation we could have been using it today to host the worlds fastest motor races.

Watching Aston Martin come full circle over a century since it began in Lionel Martins mews garage and tracing the outlandish characters who developed the succession of superlative designs ever since has really changed my perception of British engineering and its adaptability. You can see that today with Surrey-based F1 teams like McLaren manufacturing advanced PPE equipment.

The story of Aston Martin is about their pursuit of perfectionism and I hope that it will inspire the next generation of budding engineers to dive in, think out of the box and keep innovating. If I promise to behave myself, perhaps they will let me have a go in their latest creations.

My Life in books

The book I loved as a child...

I resisted every adult campaign to convert me into a literate member of society. I escaped their clutches by discovering the Garfield series by Jim Davis and my passion for pithy, entertaining yarns began.

The book that inspired me as a teenager

Contact by Carl Sagan. With his total command of complex Astro-Physics he was still able to makethe subject relatable to an ignoramus like me as his story ripped through space, while weaving athrilling narrative about mankinds first contact with Extra Terrestrials.

The book Ive never finished

Theres a long list. The Enid Blyton series that I escaped through numerous windows. And, shamefully, Lord of the Rings a capital sin which leaves me damned to face a horde of Orks in the afterlife.

The book that moved me the most

Chickenhawk by Robert Mason relates his Vietnam War experiences as a Huey pilot and by the end of his descriptions of basic training you feel like you could fly one yourself. His sense of irony hits you deep in the pit in your stomach.

The book Im reading now...

Jack Reacher: A Wanted Man. Reacher is fixing more problems with an elbow strike to the temple and has picked up my thirst for a serial where I left off with Bernard Cornwells Sharpe series.

- ASTON MARTIN: Made in Britain by Ben Collins, published in hardback by Quercus on October 15 Ben will be speaking at this years Guildford Book Festival on Friday 9th October. Please check details on http://www.guildfordbookfestival.co.uk

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Ben Collins The Stig Top Gear | Surrey - Surrey Life

Mega Science On The Cover: Class XI Maharashtra Physics Text Shows Gravitational-Wave Detection By LIGO – Swarajya

School textbooks come in a variety of forms some engage and spark curiosity, others make it all about the information.

It's a full spectrum, really.

Its clear which approach the Maharashtra State Bureau of Textbook Production and Curriculum Research, Pune, intends to take.

The front page of the latest edition of the state boards Class XI physics textbook features a mega-science project of our times.

The cover shows the Laser Interferometer Gravitational-wave Observatory (LIGO) with a snapshot of gravitational waves detected in the event of a black hole merger.

It's a common refrain in India that textbooks carry outdated subject matter. Featuring real-world contemporary scientific work on the cover of the textbook sets a different example.

Somak Raychaudhury, director of the Inter-University Centre for Astronomy and Astrophysics, tweeted saying: "This is probably the best way to communicate to high school students what kind of facilities would be available for them if they study the subject well."

Explaining its cover, the textbook says: Since ages, mankind is awed by the sheer scale of the universe and is trying to understand the laws governing the same.

Today we observe the events in the universe with highly sophisticated instruments and laboratories such as the LIGO project seen on the cover.

The cover is designed by Vivekanand S Patil.

LIGO And Gravitational Waves

LIGO is an observatory in the United States of America that hunts for traces of extraordinary cosmic events that happened a long time ago, in the form of gravitational waves.

The idea of gravitational waves originated in Albert Einstein's theory of general relativity.

It remained a prediction for a century until it was confirmed in 2015 by LIGO gravitational waves were detected from 1.3 billion years ago after two spiralling black holes crashed into each other.

Some 50 different gravitational waves have been detected in the last five years.

Future projects like the Einstein Telescope and Cosmic Explorer promise to help refine our gravitational-wave view of the universe.

India is set to get its own gravitational-wave observatory too, as part of the international LIGO network. Not incidentally, it will be established in Maharashtra, whose school board is behind the textbook.

LIGO-India will be a collaborative effort; several Indian research institutions will work together with LIGO, US, and the international network to catch ripples in the fabric of space and time caused by spectacular events such as the collision of black holes or neutron stars unfolding in the universe.

The planned Indian initiative had received an in-principle nod from the government of India in 2016. Work has been underway since then in the form of identifying the site, acquiring the land, and building the observatory. The Department of Atomic Energy and the Department of Science and Technology are chiefly driving this work, which is expected to be completed by 2025.

Among the research institutions leading this scientific effort are the Inter-University Centre for Astronomy and Astrophysics, Pune; Institute for Plasma Research, Gandhinagar; and Raja Ramanna Centre for Advanced Technology, Indore.

A network of gravitational wave-observatories will expand our sight of the universe and enable us to see things not observable by the more conventional electromagnetic telescope.

While gravity observatories get built here on Earth, gravitational-wave detection in the future will happen even from space (the LISA project) and, if a more adventurous proposal is accepted, the Moon.

Read: Explained: The Idea Of An Observatory On The Moon To Detect Gravitational Waves

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Mega Science On The Cover: Class XI Maharashtra Physics Text Shows Gravitational-Wave Detection By LIGO - Swarajya

Scientists May Have Just Found The Youngest Neutron Star Ever – Forbes

At the core of all type II supernova explosions, a remnant of the original star is expected to ... [+] exist. SN 1987A, the closest supernova to Earth in generations, may have just had the first signature of its remnant spotted, and it appears to be a non-pulsing neutron star.

33 years ago, a supernova occurred just 168,000 light-years from Earth.

This new image of the supernova remnant SN 1987A was taken by the NASA/ESA Hubble Space Telescope in ... [+] January 2017 using its Wide Field Camera 3 (WFC3). Since its launch in 1990 Hubble has observed the expanding dust cloud of SN 1987A several times and this way helped astronomers to create a better understanding of these cosmic explosions.

Dubbed SN 1987A, it was the closest supernova directly observed since 1604.

In 1604, the last naked-eye supernova to occur in the Milky Way galaxy happened, known today as ... [+] Kepler's supernova. Although the supernova faded from naked-eye view by 1605, its remnant remains visible today, as shown here in an X-ray/optical/infrared composite. The bright yellow "streaks" are the only component still visible in the optical.

We first detected the neutrinos from it, and then, hours later, the explosive light.

When neutrinos from the supernova explosion SN 1987a arrived on Earth, they passed through enormous ... [+] tanks of matter lined with photomultiplier tubes, creating a signal based on neutrino interactions. This marked the birth of neutrino astronomy beyond the Sun, a science that has advanced tremendously over the past few decades.

Originating from the Large Magellanic Cloud, it was briefly visible to human eyes.

The remnant of supernova 1987a, located in the Large Magellanic Cloud some 165,000 light years away. ... [+] It was the closest observed supernova to Earth in more than three centuries, and reached a maximum magnitude of +2.8, clearly visible to the naked eye and significantly brighter than the host galaxy containing it.

For years, scientists examined this cataclysms afterglow, observing the bright, expanding gaseous shells.

For the past 33 years, astronomers have used the best tools available at humanity's disposal to ... [+] track the evolution of both the inner and outer components of the remnants of the famous, close supernova, SN 1987A. The inner, dusty core has remained mysterious, but the outer, expanding gaseous layers have revealed telling details for a long time.

But inside, embedded within dusty clouds, a remnant core must exist.

This montage shows the evolution of the supernova SN 1987A between 1994 and 2016, as seen by the ... [+] NASA/ESA Hubble Space Telescope. The supernova explosion was first spotted in 1987 and is among the brightest supernovae within the last 400 years. The outward-moving shockwave of material continues to collide with earlier ejecta, leading to brightening events at later times.

SN 1987A was a type II supernova: a blue supergiant exploding at its life cycles end.

The stars within the Tarantula nebula, part of the complex containing the remnant of SN 1987A, also ... [+] contain the enormous star cluster 30 Doradus, which contain some of the brightest, most massive blue supergiant stars known to humanity. Many of them will end their lives in type II supernovae, giving rise to neutron star or black hole remnants.

These explosions always create either neutron stars or black holes, but none had yet been discovered.

The anatomy of a very massive star throughout its life, culminating in a Type II Supernova when the ... [+] core runs out of nuclear fuel. The final stage of fusion is typically silicon-burning, producing iron and iron-like elements in the core for only a brief while before a supernova ensues. We believe that core-collapse supernovae produce a continuous spectrum of neutron stars to black holes, with no other realistic options for the core's remnant.

Many anticipated a central pulsars presence: analogous to the Crab Nebula.

Five different combined wavelengths show the true magnificence and diversity of phenomena at play in ... [+] the Crab Nebula. The X-ray data, in purple, shows the hot gas/plasma created by the central pulsar, which is clearly identifiable in both the individual and the composite image.

But not all neutron stars pulse; some simply emit high-temperature radiation.

The Atacama Large Millimetre/submillimetre Array, as photographed with the Magellanic clouds ... [+] overhead. A large number of dishes close together, as part of ALMA, helps bring out many of the faintest details at lower resolutions, while a smaller number of more distant dishes helps resolve the details from the most luminous locations. This has resolved features in dust clouds 168,000 light-years away to unprecedented detail.

ALMA, a high-resolution radio telescope array, just revealed a telling, critical signature.

Features in the central dusty core of the SN 1987A remnant, color coded by temperature, reveals a ... [+] hot source of radiation shrouded in dust. Based on the inferred temperature and flux from the source, it should be a very young, hot neutron star seen in an earlier stage than any ever discovered thus far.

ALMA saw a hot blob in the dusty center of SN 1987As remnant.

Extremely high-resolution ALMA images revealed a hot blob in the dusty core of Supernova 1987A ... [+] (inset), which could be the location of the missing neutron star. The red color shows dust and cold gas in the center of the supernova remnant, taken at radio wavelengths with ALMA. The green and blue hues reveal where the expanding shock wave from the exploded star is colliding with a ring of material around the supernova.

Its located exactly where the observed explosion would kick a remnant core.

This WolfRayet star is known as WR 31a, located about 30,000 light-years away in the constellation ... [+] of Carina. The outer nebula is expelled hydrogen and helium, while the central star burns at over 100,000 K. In the relatively near future, this star will explode in a supernova, enriching the surrounding interstellar medium with new, heavy elements, and likely imparting a significant kick to the stellar remnant left behind.

Black holes cant heat dust sufficiently; a very young neutron star is required.

Neutron stars are small objects, perhaps just 25-to-40 km across, but containing more mass than even ... [+] the Sun; they're like one giant atomic nucleus. In the early stages of life, they can be tremendously hot, with temperatures greater than even the hottest, bluest stars, but only emitting small amounts of overall luminosity, as their radiating surface area is tiny.

Its the youngest neutron star ever discovered: 33 years old.

The Cassiopeia A supernova remnant was not visible to the naked eye, but astronomers have determined ... [+] that it occurred in the 2nd half of the 17th century based on the remnant's properties. There is a neutron star that has been found at the center, but it's some ~320 years older than the remnant of SN 1987A.

As its evolution continues, we may even someday directly see it pulsing.

As the core region of the SN 1987A remnant continues to evolve, the central dusty region will cool ... [+] off and much of the radiation obscured from it will become visible, while the central remnant will continue to cool and evolve as well. It's conceivable, when this occurs, that periodic radio pulses will become observable, revealing whether the central neutron star is a pulsar or not.

Mostly Mute Monday tells an astronomical story in images, visuals, and no more than 200 words. Talk less; smile more.

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Scientists May Have Just Found The Youngest Neutron Star Ever - Forbes

‘Roaming reactions’ study to shed new light on atmospheric molecules – Science Codex

A detailed study of roaming reactions - where atoms of compounds split off and orbit other atoms to form unexpected new compounds - could enable scientists to make much more accurate predictions about molecules in the atmosphere, including models of climate change, urban pollution and ozone depletion.

In a paper published today in the journal Science, a team of researchers from UNSW Sydney, University of Sydney, Emory University and Cornell University showed in unprecedented detail exactly what happens during roaming reactions of chemical compounds.

Professor Scott Kable, an atmospheric scientist who is also the head of UNSW's School of Chemistry, likens the study to lifting the hood on roaming reactions and seeing for the first time how the parts fit together. He says the study will give scientists new tools to understand the machinations of reactions in the atmosphere.

"Chemical reactions, where atoms are rearranged to make new substances, are occurring all the time in our atmosphere as a result of natural emission from plants and animals as well as human activity," Prof Kable says.

"Many of the key reactions in the atmosphere that contribute to photochemical smog and the production of carbon dioxide are initiated by sunlight, which can split molecules apart.

"For a long time, scientists thought these reactions happened in a simple way, that sunlight was absorbed and then the molecule explodes, sending atoms in different directions.

"But, in the last few years it was found that, where the energy from the sun was only just enough to break a chemical bond, the fragments perform an intimate dance before exchanging atoms and creating new, unanticipated, chemical products - known as roaming reactions.

"Our research shows these 'roaming' reactions exhibit unusual and unexpected features."

Prof Kable says in an experiment detailed in the paper, the researchers looked at the roaming reaction in formaldehyde (CH2O) and were surprised to see instead, two quite distinct signals, "which we could interpret as two distinct roaming mechanisms".

The theoretical and computational work was performed by a team in the US led by Professors Joel Bowman (Emory) and Paul Houston (Cornell). Prof Bowman observed that "detailed modelling of these reactions not only agree with the experimental findings, they provide insight into the motion of the atoms during the reaction".

Professor Meredith Jordan from University of Sydney says the experiments and theory results suggest roaming reactions straddle the classical and quantum worlds of physics and chemistry.

"Analysing the results with the incredible detail in both experiments and simulations allowed us to understand the quantum mechanical nature of roaming reactions. We expect these characteristics to be present in all roaming reactions," she says.

The results of this study will provide theoreticians with the data needed to hone their theories, which in turn will allow scientists to accurately predict the outcomes of sunlight-initiated reactions in the atmosphere.

Prof Kable says the study could also benefit scientists working in the areas of combustion and astrophysics, who use complex models to describe how molecules interact with each other in gaseous form.

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'Roaming reactions' study to shed new light on atmospheric molecules - Science Codex

‘A space race of sorts’: Stanford Space Initiative hopes to cross into space with a ‘rockoon’ – The Stanford Daily

The Krmn Line 100 km or 62 miles above sea level is where space arbitrarily starts. And through Project SpaceShot, the Stanford Space Initiative (SSI) plans to get there by December 2021 with a somewhat unusual rocket, nicknamed a rockoon.

The project, housed under both the Rockets and Balloons Teams at SSI, plans to have a zero-pressure high-altitude balloon carry a rocket 25 km up into the atmosphere. The spin-stabilized rocket will then launch through the balloon to complete the journey to 100 km, Project SpaceShot Co-Lead Ahmed Abdalla 22 explained.

Abdalla had actually first heard of the idea at his Admit Weekend in June 2018, and decided to join SSI because of its originality.

I thought either these people are just completely insane and they dont know what theyre doing, or theyre going to do something super exciting, Abdalla said.

In 2017, Berkeleys Space Enterprise announced Project Karman, their attempt to pass the Krmn Line, and challenged peer institutions to join the collegiate space race. Universities around the nation had been attempting the feat for years, but Berkeleys challenge prompted SSI to begin their attempt.

The University of Southern Californias Rocket Propulsion Laboratory (USCRPL) announced their victory on May 22, 2019 with 90% certainty. Their rocket, Traveler IV, was officially the first student-designed and student-built rocket to cross into space.

The 13-foot, 310 pound rocket is designed more traditionally than Project SpaceShots, using fins for stabilization and not utilizing a balloon.

A lot of people have focused on the bigger is better mentality, Abdalla said. You know, a bigger rocket, super intense fuels and muscle nearly all the way up there. SpaceShot has prided itself on trying to take a very ingenuitive approach that really shakes up what people expect from a suborbital launch system.

Abdalla explained that the prospect of a space race as a motivation for the project is second to the fact that it is an interesting engineering challenge.

SSI Balloons Team Co-Lead Aditeya Shukla 22 congratulates USCRPL for their successful launch but also feels that SSI is still in a space race of sorts.

Fortunately for us, nobody has sent a rocket to space from a balloon [to this scale], so were still in the more unique territory, Shukla said.

In space, balloons are normally used to fill the gap in the atmosphere that is too high for drones to reach but too low for satellites to orbit in order to obtain meteorological data or use cameras to monitor events like forest fires.

The idea to use a high-altitude balloon as a high launchpad for a rocket was born from SSIs storied experience with balloons; they broke the world record for the longest high-altitude flight with a latex balloon in 2016 and has since broken their own record again.

Since SSI is such a tight-knit community, the Balloons members were really interested in [Project SpaceShot], Shukla said. It was the balloons guys shooting up the idea that what if we launched the rocket from a much higher altitude so that we have less drag and we can actually go to space?

Designed in 1957 during the Space Race between the U.S. and the USSR, NASAs Project Far Side attempted a similar approach to getting into space. A rocket carrying scientific equipment was launched off a 200-foot carrier balloon. The rockets maximum altitude reached 6,440 km.

In the context of SSI, the atmospheric implications of launching a rocket from 25 km are a double-edged sword. Although the lower air pressure reduces drag, allowing the rocket to go farther, fins, which are normally used to stabilize rockets, are no longer sufficient.

Usually you can use the fins as a way to counter the force of gravity trying to take you down by using aerodynamic forces to say, Actually, I prefer the rocket to continue pointing this way, Abdalla said. And as long as the rocket points up, the motors will be pushing in whatever direction up is. But you cant do that at 25 km up.

Using the rockets own momentum to stabilize it through spinning is another way to get the rocket pointed in the right direction.

Its going to be spin-stabilized, like a bullet, where its going to spin really fast and then hopefully go out straight, SSI Rockets Team Co-Lead Maya Harris 22 said. And so its a really complicated project.

The idea of spin stabilization did not come about until this past year. Before then, the plan was to use a three-balloon system, and SSI had yet to figure out a stabilization technique.

Once the spin stabilization technology was agreed upon, Abdallas task was to design a system that would allow the rocket to spin as fast as was needed to maintain stability; the fastest speed they reached was 2,700 revolutions per minute. He is proud of the progress he has seen with ground launches that were completed before campus closed due to COVID-19.

Next year, because of the uncertainty surrounding lab accessibility and the lack of ability to conduct launches, the team will use simulations to make progress on their goals.

This is something that SSI actually has experience with, Shukla said; some members have worked with research labs and companies like SpaceX, who have done similar simulations. Members modified Open Rocket, a program that allows users to design their own rocket, to better fit the design of Project SpaceShot, renaming it Open Rockoon.

Normally, Open Rocket is open-source software where you can design any rocket and itll tell you all the details ranging from center of mass and center of gravity to how it will do with certain atmospheres, Shukla said. But Open Rockoon incorporates the balloon aspect of it and the spin aspect of it, so we can do much finer simulations that way.

The code, CAD, avionics, onboard electronics and any other aspect of Project SpaceShot that a person would need to replicate the rockoon is open-source.

What I think is really exciting for me about SpaceShot is the idea that we designed everything so if you wanted to send something to space with your high school or with your college rocketry team, you could really easily just do [so] on your own, Abdalla said.

This openness aligns with the clubs mission to teach about space.

SSIs model has always been to give resources and knowledge to anybody who needs it, irrespective of whether theyre part of the organization, Shukla said. So every other project is also as open-source as SpaceShot.

And so, in December of 2021, SSI hopes to cross into space, but the project itself means more than crossing an arbitrarily-defined line.

Astrophysics and astronomy has always been such a big part of my life, Adballa said, and so actually being able to achieve the goal of getting there would be fantastic. But what weve done so far and all the progress that weve made is already so rewarding.

Contact Alexandra Rozmarin at alexroz918 at gmail.com.

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'A space race of sorts': Stanford Space Initiative hopes to cross into space with a 'rockoon' - The Stanford Daily