Quasar jets are thousands of light-years long – Cosmos

The very-high-energy gamma ray emission from quasars are not concentrated in the region close to their central black holes but in fact extend over several thousand light-years along jets of plasma, new research reveals.

Writing in the journal Nature, a team of more than 200 astrophysicists from 13 countries describes its observations using the HESS observatory in Namibia which, it says, shake up current scenarios for the behaviour of these jets.

The work was carried out as part of the international High Energy Stereoscopic System (HESS) collaboration, and led by the CNRS and CEA in France, the Max Planck Society and other German research institutions and universities.

They studied the highly luminous Centaurus A the closest radio galaxy to Earth at unparalleled resolution for more than 200 hours, enabling them to identify the region emitting the very high-energy radiation while studying the trajectory of the plasma jets.

In recent years, scientists have observed the Universe using gamma rays, which form part of the cosmic rays that constantly bombard the Earth. They originate from regions where particles are accelerated to huge energies.

Gamma rays are emitted by a wide range of cosmic objects, including quasars, which are active galaxies with a highly energetic nucleus. The intensity of the radiation emitted can vary over very short timescales of up to one minute.

It has therefore been assumed that the source of this radiation is very small and located in the vicinity of a supermassive black hole.

However, the researchers say they have shown that the gamma ray source extends over several thousand light-years. This in turn indicates that particle acceleration does not take place solely in the vicinity of the black hole, but along the entire length of the plasma jets.

Based on these results, the authors suggest the particles are reaccelerated by stochastic processes along the jet, and that many radio galaxies with extended jets accelerate electrons to extreme energies and might emit gamma-rays. This might explain the origins of a substantial fraction of the diffuse extragalactic gamma background radiation.

Here we report observations of Centaurus A at teraelectronvolt energies that resolve its large-scale jet, the authors write in their paper.

We interpret the data as evidence for the acceleration of ultrarelativistic electrons in the jet and favour the synchrotron explanation for the X-rays.

Given that this jet is not exceptional in terms of power, length or speed, it is possible that ultrarelativistic electrons are commonplace in the large-scale jets of radio-loud active galaxies.

Theres never been a more important time to explain the facts, cherish evidence-based knowledge and to showcase the latest scientific, technological and engineering breakthroughs. Cosmos is published by The Royal Institution of Australia, a charity dedicated to connecting people with the world of science. Financial contributions, however big or small, help us provide access to trusted science information at a time when the world needs it most. Please support us by making a donation or purchasing a subscription today.

Link:

Quasar jets are thousands of light-years long - Cosmos

The Antares Star is larger than the Sun, reveals a new map of the atmosphere – Republic World – Republic World

A new study conducted by a team of international scientists has found that the Antares star is much larger than its earlier prediction. As per reports, the star can even fit Saturns orbit inside it. A team of astronomers has designed a detailed map of the atmosphere which depicts the red supergiant star Antares. According to research, the size of the star shall depend on the wavelength of light it is observed with. The new study of the Antares star was published in the Journal Astronomy & Astrophysics.

ALSO READ: NASA's Next Mars Rover To Honour All Medical Workers Fighting The Coronavirus Battle

Previous research of the Antares star predicted that the Antares star was about 700 times larger than the sun. However, the research also concluded that proportion to the sun was subject to change when mapped in a different spectrum. Further, as per studies, the Antares star is regarded as the largest star in the universe, in terms of volume. The Antares star is also the 15th brightest star in the night sky and the brightest star in the constellation of Scorpius.

The Antares star is a Red Supergiant star. These stars are quite large and remain cool until the end of their lifetime. As per studies, these stars may soon run out of fuel and even collapse. By utilizing their stellar winds, these stars are capable of launching heavy elements into space. Such phenomenaalso worktowards providing a building block of life in the universe.

ALSO READ: NASA Lights Fire On Spacecraft To Test Safety Measures In Lead Up To 2024 Moon Mission

In order to the study Antares atmosphere, the team of astronomers utilized the readings of Very Large Array (VLA) and Atacama Large Millimeter (ALMA)/ submillimeter Array. While the ALMA map helped to observe shorter wavelengths close to the surface of Antares, the VLA map helped to observe longer wavelengths, farther from the stars atmosphere. These readings helped to design the most detailed map of Stars, besides the Sun. The recent study also revealed that the Antares chromosphere was much cooler as compared to the chromosphere of the sun. The study also helped to find the origination point of the winds.

ALSO READ: NASA Wants You To Help Drive Mars Rover Curiosity, And You Do Not Need A Driver's Licence!

Chris Carilli of the National Radio Astronomy Observatory gave a statement to a media portal whereby he mentioned that the National Radio Astronomy Observatory regarded the night sky as points of light. He felt that the map of the Supergiant Antares star was a true testament to technological advances in interferometry. He also said that the observations would help man to be closer to the universe.

ALSO READ: Kathy Lueders Becomes The First Ever Female Director Of Human Explorations At NASA

Go here to see the original:

The Antares Star is larger than the Sun, reveals a new map of the atmosphere - Republic World - Republic World

Mystery of a massive neutron star merger in Milky Way explained by new astrophysics theory – Firstpost

FP TrendingMay 20, 2020 13:15:44 IST

Scientists had announced earlier this year that they had detected a second gravitational wave signal fromacollision of two neutron stars. The event, which wasdubbed GW190425,resulted inthe two massive neutron stars mergingto form a binary objectlargerthan any other binary neutron star system formed by this processobserved till date.

The combined mass was 3.4 times the mass of the sun, according to the researchers. The team of astrophysicistsargue that they might have anexplanationfor the formation of the massive binary star.

An artist's illustration of merging neutron stars. The rippling space-time grid represents gravitational waves that travel out from the collision, while the narrow beams show the bursts of gamma rays that are shot out just seconds after the gravitational waves. Image: NSf/LIGO/Sonoma State Uni/A Simonnet

The theory for its formation was put forward by researchers from Australias ARC Center of Excellence for Gravitational Wave Discovery (OzGrav), led by Isobel Romero-Shaw from Monash University. The researchers claim to have explained both the high mass of the binaryobject andwhysimilar systems arent observedusing traditional radio astronomy techniques.

As per Romero-Shaw, GW190425 was formed through a process called unstable case BB mass transfer. Itbeginswith a neutron star that has a stellar partner a helium (He) star with a carbon-oxygen (CO) core. If the helium part of the star expands enoughthat it engulfs the neutron star, the helium cloud of the neutron star ends uppulling its stellar partnercloser beforethe clouddissipates and a binary object is formed from the two objects merging.

"The carbon-oxygen core of the star then explodes in a supernova and collapses to a neutron star, Romero explains. Thebinary neutron stars that form in this manner can be significantly more massive than those that are observed through radio waves, he adds.

Find latest and upcoming tech gadgets online on Tech2 Gadgets. Get technology news, gadgets reviews & ratings. Popular gadgets including laptop, tablet and mobile specifications, features, prices, comparison.

Read this article:

Mystery of a massive neutron star merger in Milky Way explained by new astrophysics theory - Firstpost

UWMadison astrophysicists donate computing resources to aid COVID-19 research | WIPAC – Wisconsin IceCube Particle Astrophysics Center – University of…

The IceCube Neutrino Observatory is possibly the worlds strangest telescope. Located at the South Pole, it is made up of over 5,000 basketball-sized light sensors embedded in a cubic kilometer of ice. Thousands of computers back at the University of WisconsinMadison, IceCubes lead institution, scour data from those sensors for evidence of elusive subatomic particles that originate in outer space: astrophysical neutrinos.

Now, some of these computing resources are being used to simulate something differentprotein folding of SARS-CoV-2, the coronavirus responsible for COVID-19. How proteins fold into three-dimensional shapes is difficult to predict but has big effects on biological interactions, like those between a virus and its host. These simulations will help researchers understand how the virus compromises human immune systems and reproduces.

While IceCube remains operational, its home research center at UWMadison, the Wisconsin IceCube Particle Astrophysics Center, WIPAC, is temporarily providing some of its available computing resources to Folding@home. This citizen-science distributed-computing project crowdsources computationally intensive tasks like simulating protein dynamics. Distributed computing projects like Folding@home combine the power of thousands of individual computers contributed by their owners to process different portions of data simultaneously, significantly speeding up their results.

It just feels right to make the effort to share computing resources from fields as far removed from virology as neutrino astrophysics, says Kael Hanson, director of WIPAC. Were pleased to aid in research that could ultimately lead everyone impacted by the current COVID-19 situation out of the crisis.

Folding@home started in 1999, but it has recently seen a surge in interest as people seek ways to help researchers understand COVID-19. They include Benedikt Riedel, global computing coordinator for the IceCube Neutrino Observatory and computing manager at WIPAC.

Riedel had been in touch with his scientific computing collaborators since mid-March to discuss how they could help the COVID-19 effort. When he heard from them about Folding@home, Riedel suggested supporting it to WIPAC administration, who then received approval from IceCubes primary funder, the National Science Foundation. Since the donated computing cycles primarily come from already available resources, they do not significantly hamper WIPAC or IceCube projects.

These are unprecedented times, and I feel like we should do what we can to help other researchers, says Riedel. So far it is going well, and I am hoping that we can continue to donate even after this ends.

IceCubes computing resources consist of roughly 5,000 traditional computers using CPUs (central processing units) and 300 computers using GPUs (graphical processing units), each containing massive numbers of simple parallel computing elements. As a member of the Open Science Grida national distributed-computing partnership that provides high-throughput computing resources to science projects around the countryIceCube had already been sharing computing resources for other projects. Dozens of other Open Science Grid members are also contributing their resources to COVID-19 research.

WIPAC is able to contribute to Folding@home thanks to software that manages the allocation of the centers diverse computing resources to different users competing computational tasks. Specifically, WIPAC uses tools from the HTCondor software suite that was developed and is maintained by UWMadisons Center for High Throughput Computing (CHTC) to effectively manage the computational workload.

The long partnership between WIPAC and CHTC is founded on a commitment to share resources and knowledge, says Miron Livny, director of the CHTC. It is gratifying to see this partnership contributing to the computing challenge of protein folding of SARS-CoV-2.

The first protein-folding simulations received high priority and will continue to be executed along with the day-in-day-out IceCube workload, which is continually submitted to the system. You can follow WIPACs contributions to Folding@home here.

Contact:

press@icecube.wisc.edu

608-515-3831

Go here to see the original:

UWMadison astrophysicists donate computing resources to aid COVID-19 research | WIPAC - Wisconsin IceCube Particle Astrophysics Center - University of...

Astronomers discover a massive rotating disk galaxy in the early universe – UC Santa Cruz

Most massive disk galaxies like our Milky Way formed gradually, reaching their large mass relatively late in the 13.8 billion-year history of the universe. But the discovery by an international team of astronomers of a massive rotating disk galaxy, seen when the universe was only ten percent of its current age, challenges the traditional models of galaxy formation.

The discovery, reported May 20 in Nature, was made with the Atacama Large Millimeter/submillimeter Array (ALMA). Galaxy DLA0817g, nicknamed the Wolfe Disk after the late astronomer Arthur M. Wolfe, is the most distant rotating disk galaxy ever observed. The unparalleled power of ALMA made it possible to see this galaxy spinning at 170 miles (272 kilometers) per second, similar to our Milky Way.

Its properties are astonishingly similar to our own galaxy, despite being only 1.5 billion years old, said coauthor J. Xavier Prochaska, professor of astronomy and astrophysics at UC Santa Cruz.

While previous studies hinted at the existence of these early rotating gas-rich disk galaxies, thanks to ALMA we now have unambiguous evidence that they occur as early as 1.5 billion years after the Big Bang, said lead author Marcel Neeleman of the Max Planck Institute for Astronomy in Heidelberg, Germany

How did the Wolfe Disk form?

The discovery of the Wolfe Disk provides a challenge for many galaxy formation simulations, which predict that massive galaxies at this point in the evolution of the cosmos grew through many mergers of smaller galaxies and hot clumps of gas.

Most galaxies that we find early in the universe look like train wrecks because they underwent consistent and often violent merging, explained Neeleman. These hot mergers make it difficult to form well-ordered, cold, rotating disks like we observe in our present universe.

In most galaxy formation scenarios, galaxies only start to show a well-formed disk around 6 billion years after the Big Bang. The fact that the astronomers found such a disk galaxy when the universe was only ten percent of its current age indicates that other growth processes must have dominated.

We think the Wolfe Disk has grown primarily through the steady accretion of cold gas, Prochaska said. Still, one of the questions that remains is how to assemble such a large gas mass while maintaining a relatively stable, rotating disk.

Star formation

The team also used the National Science Foundations Karl G. Jansky Very Large Array (VLA) and the NASA/ESA Hubble Space Telescope to learn more about star formation in the Wolfe Disk. In radio wavelengths, ALMA looked at the galaxys movements and mass of atomic gas and dust, while the VLA measured the amount of molecular massthe fuel for star formation. Hubble observed massive stars in ultraviolet light.

The star formation rate in the Wolfe Disk is at least ten times higher than in our own galaxy, Prochaska said. It must be one of the most productive disk galaxies in the early universe.

A normal galaxy

The Wolfe Disk was first discovered by ALMA in 2017. Neeleman and his team found the galaxy when they examined the light from a more distant quasar. The light from the quasar was absorbed as it passed through a massive reservoir of hydrogen gas surrounding the galaxy, which is how it revealed itself. Rather than looking for direct light from extremely bright, but more rare galaxies, astronomers used this absorption method to find fainter and more normal galaxies in the early universe.

The fact that we found the Wolfe Disk using this method tells us that it belongs to the normal population of galaxies present at early times, said Neeleman. When our newest observations with ALMA surprisingly showed that it is rotating, we realized that early rotating disk galaxies are not as rare as we thought and that there should be a lot more of them out there.

In addition to Neeleman and Prochaska, the coauthors of the paper include Nissim Kanekar at the National Center for Radio Astrophysics in Pune, India, and Mark Rafelski at the Space Telescope Science Institute.

The Atacama Large Millimeter/submillimeter Array (ALMA), an international astronomy facility, is a partnership of the European Organization for Astronomical Research in the Southern Hemisphere (ESO), the U.S. National Science Foundation (NSF), and the National Institutes of Natural Sciences (NINS) of Japan in cooperation with the Republic of Chile. ALMA construction and operations are led by ESO on behalf of its Member States; by the National Radio Astronomy Observatory (NRAO), managed by Associated Universities, Inc. (AUI), on behalf of North America; and by the National Astronomical Observatory of Japan (NAOJ) on behalf of East Asia.

Read more:

Astronomers discover a massive rotating disk galaxy in the early universe - UC Santa Cruz

This Bionic Eye Is Better Than a Real One, Scientists Say – Futurism

Researchers say theyve created a proof-of-concept bionic eye that could surpass the sensitivity of a human one.

In the future, we can use this for better vision prostheses and humanoid robotics, researcher Zhiyong Fan, at the Hong Kong University of Science and Technology, told Science News.

The eye, as detailed in a paper published in the prestigious journal Nature today, is in essence a three dimensional artificial retina that features a highly dense array of extremely light-sensitive nanowires.

The team, led by Fan, lined a curved aluminum oxide membrane with tiny sensors made of perovskite, a light-sensitive material thats been used in solar cells.

Wires that mimic the brains visual cortex relay the visual information gathered by these sensors to a computer for processing.

The nanowires are so sensitive they could surpass the optical wavelength range of the human eye, allowing it to respond to 800 nanometer wavelengths, the threshold between visual light and infrared radiation.

That means it could see things in the dark when the human eye can no longer keep up.

A human user of the artificial eye will gain night vision capability, Fan told Inverse.

The researchers also claim the eye can react to changes in light faster than a human one, allowing it to adjust to changing conditions in a fraction of the time.

Each square centimeter of the artificial retina can hold about 460 million nanosize sensors, dwarfing the estimated 10 million cells in the human retina. This suggests that it could surpass the visual fidelity of the human eye.

Fan told Inverse that we have not demonstrated the full potential in terms of resolution at this moment, promising that eventually a user of our artificial eye will be able to see smaller objects and further distance.

Other researchers who were not involved in the project pointed out that plenty of work still has to be done to eventually be able to connect it to the human visual system, as Scientific American reports.

But some are hopeful.

I think in about 10 years, we should see some very tangible practical applications of these bionic eyes, Hongrui Jiang, an electrical engineer at the University of WisconsinMadison who was not involved in the research, told Scientific American.

READ MORE: A new artificial eye mimics and may outperform human eyes [Science News]

More on bionic eyes: SCIENTISTS PLUGGED A BIONIC EYE DIRECTLY INTO THIS WOMANS BRAIN

Here is the original post:

This Bionic Eye Is Better Than a Real One, Scientists Say - Futurism

Formation of pair of baby planets around their parent star captured in remarkable first – Firstpost

FP TrendingMay 20, 2020 14:13:43 IST

Astronomersat the W M Keck Observatory in Hawaii have captured the first-ever images a pair of giant planets being born around their parent star PDS 70. They achieve the feat using anovel infrared pyramid wavefront sensor, whichoffers adaptive optics (AO) correction in astrophysics detectors.

The team of researchers published their findings in The Astronomical Journal.

PDS 70 is a star located roughly 370 light-years from us, in the constellation of Centaurus. The star, which is technically classified as aK7-type pre-main sequence star, is a young star at5.4million years old, and alsogoes by'V* V1032 Cen' and 'IRAS 14050-4109'.

An artist's impression of the PDS 70 star system. The two planets are seen clearing a gap in the protoplanetary disk from which they were born. (Not to scale). Image credit: W M Keck Observatory

A report in Phys.orgnotes that PDS 70 is the first known multi-planetary systemin which astronomers have witnessed planet formation in action. The first direct image of PDS 70b (one ofthe newbornplanets orbiting PDS 70), was taken in 2018, the report adds. It was followed by images of the second planet PDS 70c in 2019.

There was some confusion when the two protoplanets were first photographed, lead author of the study, Dr Jason Wang, toldTechExplorist.

"Planet embryos form from a disk of dust and gas surrounding a newborn star. This circumstellar material accretes onto the protoplanet, creating a kind of smokescreen that makes it difficult to differentiate the dusty, gaseous disk from the developing planet in an image, he added.

An infrared image of the newborn planet PDS 70 b and its circumplanetary disc. The size of the solar system given for comparison. Image: V Christiaens et al./ESO

For further clarification, the researchers developed a method to disentangle the image signals from the circumstellar disk and the protoplanets. Subsequently, they were able to take pictures of the baby planets and confirm their existence.

The researchers knew the disks shape should be an asymmetrical ring around the star whereas a planet should be a single point in the image, Wang said.

"So even if a planet appears to sit on top of the disk, which is the case with PDS 70c, based on our knowledge of how the disk looks throughout the whole image, we can infer how bright the disk should be at the location of the protoplanet and remove the disk signal. All thats leftover is the planets emission, he explained.

Find latest and upcoming tech gadgets online on Tech2 Gadgets. Get technology news, gadgets reviews & ratings. Popular gadgets including laptop, tablet and mobile specifications, features, prices, comparison.

Continue reading here:

Formation of pair of baby planets around their parent star captured in remarkable first - Firstpost

Biggest influencers in big data in Q1 2020: The top companies and individuals to follow – Verdict

GlobalData research has found the top big data influencers based on their performance and engagement online. Using research from GlobalDatas Influencer platform, Verdict has named ten of the most influential people in big data on Twitter during Q1 2020.

Ronald Van Loon is the director of Advertisement, which offers data consultancy, technology, and data engineering and automation solutions to its partners and clients. A known thought leader, Ronald believes that big data, AI, autonomous cars, analytics, and more are some technology areas that will be filling up with new job opportunities.

Twitter followers: 217,826

GlobalData influencer score: 100

Ganapathi Pulipaka is a chief data scientist at Accenture. He has developed a number of deep learning and machine learning programs and published them on GitHub and medium.com.

Twitter followers: 87,390

GlobalData influencer score: 96

Kirk Borne is an advisor and principal data scientist at Booz Allen Hamilton. An astrophysicist and big data advisor, Kirk specialises in data mining, data analytics, machine learning, and computational astrophysics, among others.

Kirk has engaged in several NASA projects, including its astronomy centre and its space science data operations for more than 20 years.

Twitter followers: 258,119

GlobalData influencer score: 86

Dr Iain Brown is a big data consultant and the head of data science for SAS UK&I. Over the past decade he has worked across a number of sectors, providing thought leadership on the topics of risk, AI and machine learning.

Twitter followers: 123,490

GlobalData influencer score: 68

Spiros Margaris is a venture capitalist and founder of Margaris Ventures. He is the first international influencer to have achieved The Triple Crown ranking.

Twitter followers: 96,901

GlobalData influencer score: 62

Yves Mulkers is a data strategist and the founder of 7wData, a digital publication that covers all types of news on data. As a data integration specialist, Yves focuses on data organisation and data architecture capabilities of an organisation. He provides technical expertise and vision on analytics, business intelligence, and data related issues.

Twitter followers: 97,174

GlobalData influencer score: 59

Mike Quindazzi is a digital alliances sales leader at PWC. He helps drive business results by offering consulting on emerging technologies such as drones, 3D printing, blockchain, IoT, big data, and robotics, among others. He has worked with brands such as Microsoft, SAP, Amazon, and Oracle, and has helped shape innovative approaches to solving their problems. Quindazzi is of the opinion that big data keeps getting bigger.

Twitter followers: 151,521

GlobalData influencer score: 58

Evan Kirstel is a top B2B tech influencer and co-creator of eVira Health, which offers consulting, product development, and business development strategies for the health tech community. He has worked with eminent brands such as IBM, Intel, and AT&T, among others to maximise their visibility and scale across 5G, blockchain, AI, cloud, IoT, AR, VR, big data, and analytics.

Twitter followers: 285,163

GlobalData influencer score: 57

Marcus Borba is the creator of Borba Consulting, an advisory and research firm which solves complex data challenges of companies through tools such as analytics, big data, and business intelligence. Regarded as one of the top data science and business intelligence influencers, Marcus has also contributed to publications such as SAPs and Microstrategys eBook.

Twitter followers: 38,723

GlobalData influencer score: 54

Michael Fisher is a tech evangelist and senior systems analyst at the Whitcraft Group. He is regarded as a top influencer of technologies such as cyber security, IoT, 5G, VR, and fintech, and specialises in areas such as cyber security, consulting, and infrastructure architecture, among others.

Twitter followers: 81,637

GlobalData influencer score: 53

GlobalData is this websites parent business intelligence company.

See the rest here:

Biggest influencers in big data in Q1 2020: The top companies and individuals to follow - Verdict

Embedded in the community: Outstanding physics student is a third-generation ASU student – ASU Now

May 18, 2020

Editor's note:This story is part of a series of profiles ofnotable spring 2020 graduates.

Weighing the pros and cons, considering multiple variables, and a little bit of faith all roll into deciding where to pursue higher education. Fortunately for Department of Physics graduate Tanner Wolfram, the choice was simple. Wolfram enjoyed many travel opportunities during his undergraduate years. Photo courtesy of Tanner Wolfram. Download Full Image

An award-winning and published student, Wolfram is part of the third generation in his family to graduate from Arizona State University.

My family came to ASU forever, Wolfram said. My grandmother came here when I think it was still called Arizona State College. My mom went here, all of her sisters, my dad, and I think one of his siblings.

With such a rich history in his own family, Wolfram has had a front-row seat on ASU's evolution through decades of family stories.

My grandmother talks about how the original Palm Walk used to be different; she called it a small school, he said.

Patricia Reagan, Wolframs maternal grandmother, attended Arizona State College in 1953, before the 1958 vote to change the school name to the one we are used to today. And, in the past 60 years, that small school has sky-rocketed to a sprawling, innovative New American University with nearly 120,000 students spread across four campuses and several locations.

Thats one of the coolest things for me to see, maybe, being here just a little longer than a lot of students, said Wolfram. I got to see so many new buildings and so many new research areas develop here at ASU. To hear about them through emails, and things from the campus, and just to hear about all the progressions ASU is making, thats pretty cool."

Through family involvement in campus activities over the years, Wolfram saw the Tempe campus shift and evolve through his parents' eyes, listening to their stories and commentary on changes and new elements. Both his parents graduated from ASU in 1984.

When asked which changes seemed most remarkable, Wolframs father, Scott Wolfram, said, The addition of the whole science complex with Biodesign, theSchool of Earth and Space Explorationand then the addition of Barrett.

I think the new architectural designs are really beautiful. I also love the plant life that accents the campus, said Wolframs mother, Deborah Estrada. Im also really pleased that there are many places for the students to eat and hang out.

Wolframs earliest memory of ASU is of walking around the Tempe campus with his mother, who brought him to see the sights and also to participate in various campus activities for children, from bowling to violin lessons.

My mom says that the first thing I did at ASU was be part of the psychology child study lab. Obviously, I dont remember this, since I was something like 3 or 4, he said.

Wolfram remembers spending plenty of time in the Bateman Physical Sciences Center during events like ASUs Open Door, and Earth and Space Exploration Day. Fitting, then, that this is the building where he would spend so much time as a physics student.

Wolfram enjoys a broad range of interests and passions and loves to learn. In addition to school and community activities, both at ASU and otherwise, he grew up watching the Science Channel. As time went on and people started asking him what he wanted to do after graduation, he noticed a definite pattern in his favorite shows programs like Neil deGrasse Tyson's "Star Talk" and "How the Universe Works" heavily featured expert guests to explore varying topics.

I kept seeing their titles: astrophysicist, astrophysicist, Wolfram said.

He started as an astrophysics major, but soon switched to physics, not wanting to specialize too early.

I think that is the key, I really wanted a big foundation in physics, he said.

This foundation would help keep his options open and give him the freedom to explore his varied interests without the pressure of locking into a lifelong career path.

Wolfram likes options and has many interests besides his love of physics. In addition to his physics coursework, he enjoyed a wide range of extracurricular activities and completed two foreign language minors, Spanish and Chinese, and participated in a study abroad program in China.

He is very interested in politics, language, learning about new cultures and international relations. His many travel opportunities during his undergraduate years gave him insight, perspective and new experiences that he cant wait to take with him into whatever life holds in store next.

Building his solid foundation in physics, Wolfram also found new interests in his major. One of his favorite subjects, and perhaps his proudest accomplishment, was completing the full undergraduate quantum coursework including acing the notoriously difficult Quantum Physics III.

That one I worked really hard for, he said. It was a hard class. It was areallyhard class. The tests are very challenging; its very demanding. Im glad in the end that I had done enough to get the A.

Despite the level of difficulty, or perhaps because of it, Wolfram found he quite enjoyed abstract and theoretical topics.

Ive always liked things that are a little abstract, a little not-so-here, not so physical, he said. Problems and questions often stayed on his mind for weeks afterward.

I think I like the thinking side of it, he said. Just kind of sit with myself and ponder. You know, probably those were my favorite classes.

He also appreciated the close friendships formed with his classmates, as they all took on such challenging courses together.

I have to say, I really like the department here, thats a really big thing, said Wolfram.

It was a lot of fun because we would all be in the same classes. You know, we worked together, we generally studied together, so that was always fun, and kept things very interesting learning things with them and from them. That was one of the things I really liked about ASU.

Wolfram is currently considering graduate programs. Is there a chance he will end up moving into astrophysics, the topic that launched his undergraduate journey? Perhaps. He certainly hasnt lost his curiosity about the universe.

When asked what project he would tackle if suddenly gifted $40 million, he said he would devote it to furthering space exploration.

My personal viewpoint is that we have a lot of time (hopefully) here on Earth, but I think we should also spend part of that time trying to explore farther out, try to make new worlds, and new things, he said.

Thats probably way far in the distant future, he said. But if thats something I could have helped work on, getting people to different worlds even if I only contributed a little, minor thing that would be interesting.

More:

Embedded in the community: Outstanding physics student is a third-generation ASU student - ASU Now

Peter Brancazio, Who Explored the Physics of Sports, Dies at 81 – The New York Times

This obituary is part of a series about people who have died in the coronavirus pandemic. Read about others here.

Peter J. Brancazio, a physics professor who debunked concepts like the rising fastball (physically impossible) and Michael Jordans apparently endless hang time (much shorter than fans believed), died on April 25 in Manhasset, N.Y. He was 81.

The cause was complications of the novel coronavirus, his son Larry said.

Professor Brancazio, who taught at Brooklyn College for more than 30 years, was one of a small number of sports-minded physicists whose research anticipated the use of the advanced statistics that are now accessible through computerized tracking technology. His work, which he began in the 1980s, was filled with terms like launching angle (how high a ball is hit, in degrees) and spin rate (the measurement of a pitch in revolutions per minute) that are now part of baseballs lingua franca. (Launch angle, not launching angle, is the term now widely used.)

Although he was obsessed with basketball, Professor Brancazio was best known for what he had to say about baseball, notably his explanation that a so-called rising fastball could not rise even if pitches thrown by fireballers like Nolan Ryan had seemingly been doing that for decades.

The rising fastball is an illusion, Professor Brancazio told The Kansas City Star in 1987.

Gravity, he said, makes everything fall, even baseballs, and no one can throw one fast enough and with enough spin to overcome gravitys natural force. The rising fastball just looks as if its rising, he said. Its really just not dropping as far as a typical fastball.

A fastball thrown at 90 miles per hour and 1,800 revolutions per minute would drop three feet when it reached home plate, he said. But a fastball that is thrown with still more backspin will fall only two and a half feet, a six-inch difference that creates the illusion of rising.

Professor Brancazio, whose tools included a calculator and a TRS-80 computer, wrote about his research in professional journals; in magazines like Popular Mechanics; and in the 1984 book Sport Science: Physical Laws and Optimum Performance.

Several fans were asked during the segment to guess how long Jordan seemed to hang in the air. Their guesses ranged from six to 10 seconds.

No, Professor Brancazio, said. Even Jordan was subject to gravity. His hang time was only 0.9 seconds.

Later that year, Professor Brancazio elaborated on the physics of hang time for Popular Mechanics. In an article about the science of slam dunks, he devised a formula that determined that a 36-inch vertical leap would equal hang time of 0.87 seconds and that a four-foot vertical leap would equal one second.

No small part of Jordans greatness is the fact that he seems to cover enormous horizontal distances in the air, Professor Brancazio wrote. He accentuates this illusion by releasing his shots on the way down, rather than at the peak of his trajectory.

Peter John Brancazio was born on March 22, 1939, in the Astoria section of Queens. His mother, Ann (Salomone) Brancazio, was an actuarial worker for The Hartford, an insurance company. His father, also named Peter, sorted mail for the Post Office.

When Professor Brancazio and his future wife, Ronnie Kramer, were dating as teenagers, she gave him a gift that would help guide him in his professional life: a telescope. It made him want to study astronomy, she said.

After graduating with a bachelors degree in engineering science from New York University in 1959, he Brancazio earned a masters in nuclear engineering from Columbia University a year later. He began teaching physics at Brooklyn College in 1963 while working toward a Ph.D. in astrophysics from N.Y.U.

During his 34 years at Brooklyn College, he was also a director of the colleges observatory.

Professor Brancazio wrote his first sports article, about basketball, for The American Journal of Physics in 1981. In it, he calculated the optimum launching angles for shots from various distances on the floor.

Having distilled the lessons of shooting on the schoolyards of Astoria, he found that a ball was best launched at an angle of 45 degrees, plus half the angle of the incline from the shooters hand to the front of the rim of the basket, or about 50 to 55 degrees.

He had, he admitted, a personal reason for writing the paper.

In truth, he wrote, the major purpose of this research was to find some means to compensate for the authors stature (5 10 in sneakers), inability to leap more than eight inches off the floor, and advancing age.

His intellectual detour into baseball, basketball and other sports enlivened his classes and made him part of a small group of physicists who brought science to sports, among them the Yale professor Robert Adair, who wrote the 1990 book The Physics of Baseball.

Michael Lisa, a professor of physics at the Ohio State University, said that when he did the research for his 2016 book The Physics of Sports, Professor Brancazios book had been an inspiration. His book is a favorite among physicists for its clear, accurate treatment, Professor Lisa said. d.

Professor Brancazio had no doubt that the people he most wanted to impress athletes would disdain his research. And he knew why, or at least why they did in the era before advanced training techniques transformed athletic achievement.

Larry Bird does not need to be told to release his shots at the optimum launching angle, he wrote in The American Journal of Physics in 1988, nor does Dwight Gooden have to understand the Magnus effect in order to throw a devastating curveball.

Professor Brancazio retired from Brooklyn College in 1997 and then briefly taught adult education courses there and at Queens College. He lectured on science, religion and astronomy at Hutton House, part of Long Island University, from 1999 until last year.

In addition to his wife and his son Larry, Professor Brancazio is survived by another son, David, and five grandchildren.

Professor Brancazio became a sought-after physicist in the news media when sports met science. During Game 1 of the 1991 World Series, for instance, CBS introduced SuperVision, a computerized animation of the path and speed of pitches. One pitch, by Jack Morris of the Minnesota Twins, clocked in at 94 miles per hour when it left his right hand and was the same speed when it landed in the catchers mitt.

CBSs analysts were impressed. But when asked a day later, Professor Brancazio said that a ball could not maintain the same speed on its path of 60 feet 6 inches.

The ball has to slow down by air resistance, he told The New York Times in 1991. No way it can maintain speed or pick up speed. It should lose 9 percent of its speed along the way.

The inventor of SuperVision acknowledged the error, saying that the speeds had probably been rounded off the ball might have left Morriss hand at 94.4 m.p.h. but had landed at 93.6.

A pitch that maintained its speed, it turned out, was as magical as a rising fastball.

Here is the original post:

Peter Brancazio, Who Explored the Physics of Sports, Dies at 81 - The New York Times

Scientists have discovered a star that is almost as old as the Universe, is in its last stages of life – Firstpost

FP TrendingMay 19, 2020 16:07:42 IST

A team of scientists has discovered a star that is nearly as old as the universe.

The study, which was published in the journal Monthly Notices of the Royal Astronomical Society Letters, says that the star has already reached the last stages of its life.

According to a report in Science Alert, the red giant star named SMSS J160540.18144323.1 was found to have the lowest iron levels of any star yet analysed in the galaxy.

The report mentioned astronomer Thomas Nordlander of the ARC Centre of Excellence for All-Sky Astrophysics in 3 Dimensions and the Australian National University as saying that the anaemic star likely formed just a few hundred million years after the Big Bang. He added that the star has iron levels 1.5 million times lower than that of the Sun.

The formation of a star during the early Universe. Image Credit: Wise, Abel, Kaehler (KIPAC/SLAC)

Nordlander said the low iron levels indicate that the star is extremely old, as the very early Universe had no metals at all. The first stars were primarily made up of hydrogen and helium.

As per a report in Science News, the spectroscopic analysis showed the star had an iron content of just one part per 50 billion, which according to Nordlander is like one drop of water in an Olympic swimming pool.

The report added that the exploding star was just 10 times more massive than the Sun. It had exploded so feebly that the heavy elements had fallen back on the remnant neutron star itself.

Only a very small amount of newly-formed iron escaped the fallen star's gravity and went on to form a new star one of the first-second generation stars that has now been discovered.

Find latest and upcoming tech gadgets online on Tech2 Gadgets. Get technology news, gadgets reviews & ratings. Popular gadgets including laptop, tablet and mobile specifications, features, prices, comparison.

Go here to read the rest:

Scientists have discovered a star that is almost as old as the Universe, is in its last stages of life - Firstpost

Russian Astrophysicists Trace Neutrinos Mysterious Ghost Particles From Where No One Had Expected – SciTechDaily

The Russian RATAN-600 telescope helps to understand the origin of cosmic neutrinos. Credit: Daria Sokol/MIPT Press Office

Russian researchers trace high-energy neutrino origins to black holes in far-off quasars.

Russian astrophysicists have come close to solving the mystery of where high-energy neutrinos come from in space. The team compared the data on the elusive particles gathered by the Antarctic neutrino observatory IceCube and on long electromagnetic waves measured by radio telescopes. Cosmic neutrinos turned out to be linked to flares at the centers of distant active galaxies, which are believed to host supermassive black holes. As matter falls toward the black hole, some of it is accelerated and ejected into space, giving rise to neutrinos that then coast along through the universe at nearly thespeed of light.

The study was published on May 12, 2020, in the Astrophysical Journal.

Neutrinos are mysterious particles so tiny that researchers do not even know their mass. They pass effortlessly through objects, people, and even entire planets. High-energy neutrinos are created when protons accelerate to nearly the speed of light.

The Russian astrophysicists focused on the origins of ultra-high-energy neutrinos, at 200 trillion electron volts or more. The team compared the measurements of the IceCube facility, buried inthe Antarctic ice, with a large number of radio observations. Theelusive particles were found toemerge during radio frequency flares at the centers of quasars.

Quasars are sources of radiation at the centers of some galaxies. They are comprised by amassive black hole that consumes matter floating in a disk around it and spews out extremely powerful jets of ultrahot gas.

Our findings indicate that high-energy neutrinos are born in active galactic nuclei, particularly during radio flares. Since both the neutrinos and the radio waves travel at the speed of light, they reach the Earth simultaneously, said the studys first author Alexander Plavin.

Plavin is a PhD student at Lebedev Physical Institute of the Russian Academy of Sciences(RAS) and the Moscow Institute of Physics and Technology. As such, he is one of the few young researchers to obtain results of that caliber at the outset of their scientific career.

After analyzing around 50 neutrino events detected by IceCube, the team showed that these particles come from bright quasars seen by a network of radio telescopes around the planet. The network uses the most precise method of observing distant objects in the radio band: very long baseline interferometry. This method enables assembling a giant telescope by placing many antennas across the globe. Among the largest elements of this network is the 100-meter telescope of the Max Planck Society in Effelsberg.

Additionally, theteam hypothesized that the neutrinos emerged during radio flares. To test this idea, the physicists studied the data of the Russian RATAN-600 radio telescope in the North Caucasus. The hypothesis proved highly plausible despite the common assumption that high-energy neutrinos are supposed to originate together with gamma rays.

Previous research on high-energy neutrino origins had sought their source right under the spotlight. We thought we would test an unconventional idea, with little hope of success. But we got lucky! Yuri Kovalev from Lebedev Institute, MIPT, and the Max Planck Institute for Radio Astronomy commented. The data from years of observations on international radio telescope arrays enabled that very exciting finding, and the radio band turned out to be crucial in pinning down neutrino origins.

At first the results seemed too good to be true, but after carefully reanalyzing the data, we confirmed that the neutrino events were clearly associated with the signals picked up by radio telescopes, Sergey Troitsky from the Institute for Nuclear Research of RAS added. We checked that association based on the data of yearslong observations of the RATAN telescope of the RAS Special Astrophysical Observatory, and the probability of the results being random is only 0.2%. This is quite a success for neutrino astrophysics, and our discovery now calls for theoretical explanations.

The team intends to recheck the findings and figure out the mechanism behind the neutrino origins in quasars using the data from Baikal-GVD, an underwater neutrino detector in Lake Baikal, which is in the final stages of construction and already partly operational. The so-called Cherenkov detectors, used to spot neutrinos including IceCube and Baikal-GVD rely on alarge mass of water or ice as a means of both maximizing the number of neutrino events and preventing the sensors from accidental firing. Of course, continued observations of distant galaxies with radio telescopes are equally crucial to this task.

Reference: Observational Evidence for the Origin of High-energy Neutrinos in Parsec-scale Nuclei of Radio-bright Active Galaxies by Alexander Plavin, Yuri Y. Kovalev, Yuri A. Kovalev and Sergey Troitsky, 12 May 2020, The Astrophysical Journal.DOI: 10.3847/1538-4357/ab86bdarXiv: 2001.00930

Original post:

Russian Astrophysicists Trace Neutrinos Mysterious Ghost Particles From Where No One Had Expected - SciTechDaily

The Weight of the Universe Physicists Challenge the Standard Model of Cosmology – SciTechDaily

The Universe contains unimaginably many objects. Cosmologists are trying to weigh them all. ESO/T. Preibisc

Results from physicists in Bochum have challenged the Standard Model of Cosmology. Infrared data, which have recently been included in the analysis, could be decisive.

Bochum cosmologists headed by Professor Hendrik Hildebrandt have gained new insights into the density and structure of matter in the Universe. Several years ago, Hildebrandt had already been involved in a research consortium that had pointed out discrepancies in the data between different groups. The values determined for matter density and structure differed depending on the measurement method. A new analysis, which included additional infrared data, made the differences stand out even more. They could indicate that this is the flaw in the Standard Model of Cosmology.

Rubin, the science magazine of Ruhr-Universitt Bochum, has published a report on Hendrik Hildebrandts research. The latest analysis of the research consortium, called Kilo-Degree Survey, was published in the journal Astronomy and Astrophysics in January 2020.

Cosmologist Hendrik Hildebrandt is looking for answers to fundamental questions about the Universe, for example how great the density of matter is in space. Credit: Roberto Schirdewahn

Research teams can calculate the density and structure of matter based on the cosmic microwave background, a radiation that was emitted shortly after the Big Bang and can still be measured today. This is the method used by the Planck Research Consortium.

The Kilo-Degree Survey team, as well as several other groups, determined the density and structure of matter using the gravitational lensing effect: as high-mass objects deflect light from galaxies, these galaxies appear in a distorted form in a different location than they actually are when viewed from Earth. Based on these distortions, cosmologists can deduce the mass of the deflecting objects and thus the total mass of the Universe. In order to do so, however, they need to know the distances between the light source, the deflecting object and the observer, among other things. The researchers determine these distances with the help of redshift, which means that the light of distant galaxies arrives on Earth shifted into the red range.

In order to determine the density of matter in the universe using the gravitational lensing effect, cosmologists look at distant galaxies, which usually appear in the shape of an ellipse. These ellipses are randomly oriented in the sky.On its way to Earth, the light from the galaxies passes high-mass objects, such as clusters of galaxies that contain large quantities of invisible dark matter. As a result light is deflected, and the galaxies appear distorted when viewed from Earth.Since the light travels a long way, it is repeatedly deflected by high-mass objects. Light from galaxies that are close to each other mostly passes the same objects and is thus deflected in a similar way.Neighboring galaxies therefore tend to be distorted in a similar way and point in the same direction, although the effect is exaggerated here. Researchers explore this tendency in order to deduce the mass of the deflecting objects.Credit: Agentur der RUB

To determine distances, cosmologists therefore take images of galaxies at different wavelengths, for example one in the blue, one in the green and one in the red range; they then determine the brightness of the galaxies in the individual images. Hendrik Hildebrandt and his team also include several images from the infrared range in order to determine the distance more precisely.

Previous analyses had already shown that the microwave background data from the Planck Consortium systematically deviate from the gravitational lensing effect data. Depending on the data set, the deviation was more or less pronounced; it was most pronounced in the Kilo-Degree Survey. Our data set is the only one based on the gravitational lensing effect and calibrated with additional infrared data, says Hendrik Hildebrandt, Heisenberg professor and head of the RUB research group Observational Cosmology in Bochum. This could be the reason for the greater deviation from the Planck data.

To verify this discrepancy, the group evaluated the data set of another research consortium, the Dark Energy Survey, using a similar calibration. As a result, these values also deviated even more strongly from the Planck values.

High-mass objects in the Universe are not perfect lenses. As they deflect light, they create distortions. The resulting images appear like looking through the foot of a wine glass. Credit: Roberto Schirdewahn

Scientists are currently debating whether the discrepancy between the data sets is actually an indication that the Standard Model of Cosmology is wrong or not. The Kilo-Degree Survey team is already working on a new analysis of a more comprehensive data set that could provide further insights. It is expected to provide even more precise data on matter density and structure in spring 2020.

Reference: KiDS+VIKING-450: Cosmic shear tomography with optical and infrared data by H. Hildebrandt, F. Khlinger, J. L. van den Busch, B. Joachimi, C. Heymans, A. Kannawadi, A. H. Wright, M. Asgari, C. Blake, H. Hoekstra, S. Joudaki, K. Kuijken, L. Miller, C. B. Morrison, T. Trster, A. Amon, M. Archidiacono, S. Brieden, A. Choi, J. T. A. de Jong, T. Erben, B. Giblin, A. Mead, J. A. Peacock, M. Radovich, P. Schneider, C. Sifn and M. Tewes, 13 January 2020, Astronomy & Astrophysics.DOI: 10.1051/0004-6361/201834878

Read the original here:

The Weight of the Universe Physicists Challenge the Standard Model of Cosmology - SciTechDaily

Hot Super-Earth Discovered Orbiting Ancient Star | Astronomy – Sci-News.com

An international team of astronomers has discovered a close-in super-Earth exoplanet in the HD 164922 planetary system.

An artists impression of the super-Earth exoplanet HD 164922d. Image credit: Sci-News.com.

HD 164922 is a bright G9-type star located approximately 72 light-years away in the constellation of Hercules.

Also known as Gliese 9613 or LHS 3353, the star is slightly smaller and less massive than the Sun and is 9.6 billion years old.

HD 164922 is known to host two massive planets: the temperate sub-Neptune HD 164922c and the Saturn-mass planet HD 164922b in a wide orbit.

The sub-Neptune is 12.9 times more massive than Earth, and orbits the parent star once every 75.8 days at a distance of 0.35 AU (astronomical units).

The Saturn-like planet has a mass 0.3 times that of Jupiter and an orbital period of 1,201 days at a distance of 2.2 AU.

In a new study, Dr. Serena Benatti from the INAF Astronomical Observatory of Palermo and colleagues searched for additional low-mass planets in the inner region of the HD 164922 system.

The astronomers analyzed 314 spectra of the host star collected by HARPS-N (High Accuracy Radial velocity Planet Searcher for the Northern hemisphere), a spectrograph on the Telescopio Nazionale Galileo at the Roque de los Muchachos Observatory, La Palma, Canary Islands, Spain.

We monitored this target in the framework of the Global Architecture of Planetary Systems (GAPS) project focused on finding close-in low-mass companions in systems with outer giant planets, they said.

The team detected an additional inner super-Earth with a minimum mass of 4 times that of the Earth.

Named HD 164922d, the planet orbits the star once every 12.5 days at a distance of 0.1 AU.

This target will not be observed with NASAs Transiting Exoplanets Survey Satellite (TESS), at least in Cycle 2, to verify if it transits, the researchers said.

Dedicated observations with ESAs CHarachterizing ExOPlanet Satellite (CHEOPS) could be proposed, but they can be severely affected by the uncertainty on the transit time.

The teams paper will be published in the journal Astronomy & Astrophysics.

_____

S. Benatti et al. 2020. The GAPS Programme at TNG XXIII. HD 164922 d: a close-in super-Earth discovered with HARPS-N in a system with a long-period Saturn mass companion. A&A, in press; arXiv: 2005.03368

Continue reading here:

Hot Super-Earth Discovered Orbiting Ancient Star | Astronomy - Sci-News.com

Exploring Astronomy Club and enduring COVID-19 The Mesa Press – Mesa Press

Astronomy Club is the only club at San Diego Mesa College that allows you to explore all that lies beyond the planet on which we live. Between the study, exploration and discovery of countless planets, stars, galaxies, comets, asteroids, and the infinite concept of space itself, its easy to see why astronomy is such a uniquely sought-after field of study. Marie Yokers, a student majoring in astrophysics, is the Astronomy Clubs current president. Upon attending the virtual presentation given by Jonny Kim, An Evening with an Astronaut on April 29, I noticed the event was organized by the San Diego Mesa Astronomy Club and reached out to its president.

Astronomy Club was originally founded in the fall semester of 2018 by Alexander Beltzer-Sweeney as founding president, with Ana Parra, Alex Hewett and Danny Rosales fulfilling the remaining crucial positions within the club.

The idea of a club based in science may sound off-putting to some, but Yokers extended this message to those unsure, I want to mimic what Dr. Kim had said, which was, Space is for everyone. It doesnt belong to anyone. The demographic absolutely reflects this sentiment. People come in from all walks of life, all ages, and all different experiences.

Space is vast, unknown, abstract, daunting and even confusing to some, but why is it important? Astronomy may not have daily applications like mathematics or English, but rather encompasses a broader realm of both academics and interest.

Yokers described the importance of this complex subject stating, Astronomy has played such a deep role in the development of the human race with agriculture, travel, culture, religion, etc. This begs the question, if astronomy is a more complex, all-encompassing subject, then how is it any less important than other subjects deemed essential? It isnt any less important. Astronomy is a field of study that observes all that lies outside of our atmosphere, and utilizes the knowledge and practices of physics, biology, geology and mathematics to continually broaden our understanding of the universe. These key traits, the nagging acknowledgement that there are many things we dont have answers for and the fascination with the possibility of life found outside of the world we know make astronomy a study, field, and practice all its own.

According to American Astronomical Society, astronomy is a rather small field in terms of career, which incidentally leads to high levels of competition for open positions.

If you browse classes online, Astronomy is a class offered at Mesa, so how is Astronomy club different from the class? First, its a club, and beyond that, Astronomy Club has its own constitution which includes the following two goals, To promote interest in astronomy and related space sciences on the San Diego Mesa College campus. Provide opportunities for members to learn more about astronomy & related space sciences through club outings, lectures, work-based learning opportunities, and internships.

Astronomy Club operates through a balance of volunteering, education and discussions. Due to COVID-19 shifts have been made. If you find yourself wondering what types of things happen in Astronomy Club, Yokers identified a few including film discussions, attending talks such as the one held at the Fleet Science Center earlier this year, attending the Astronomy Associations Star Parties which allows amateur astronomers to observe, practice and congregate in a fun learning environment, and various other activities. In the words of Yokers, Basically, if its space-related, we try to jump in to learn and have fun!

After taking a two-year hiatus break from school to work, Yokers returned in 2018 to revisit her interest in astrophysics and took Astronomy 101 at Mesa. About her choice to enroll in the class, It was the first class that I actually had a passion to do well in, and it was the first class that I really connected with the professor (Dr. Stojimirovic). I confided in Dr. Stojimirovic about wanting to pursue astrophysics as a career and she really helped push me in the correct direction.

It was at this point that Yokers found a role in Astronomy Club as treasurer and grew with it. Yokers went on to say, If I did not take that chance- I would not have met the great network of people that I have so much to credit to today.

Busy class or work schedules, the idea exploring personal interests, and the pressure to pursue the right education and career path can get overwhelming. Finding encouragement or inspiration from your family, a club, a friend or professor can give you the extra boost you may have needed.

At the moment, COVID-19 has taken a toll on classes, jobs, student clubs, businesses, and leisurely activities alike, yet strides are being made to ensure Astronomy Clubs continuance. Dont settle for locking yourself in your room with your now dust-coated textbooks, Yokers encouraged, My motto for the club post-virus has been keep moving forward. Would I step away from my physics homework for this event? If its a yes, then the event is a go.

At this time, Astronomy Club consists mainly of movie nights, game nights and discussion, with the occasional lecture found easily online. Among the present changes, Yokers mentioned the voting of new officers is hopefully taking place within the next two weeks, inviting anyone interested to reach out to the club email, astroclubmesa@gmail.com.

Astronomy Club meetings happen every Wednesday from 5:30 7 p.m., through Zoom for the time being. Once students are able to return to campus, the club meetings will be at the STEM Center.

With many student clubs derailed by COVID-19, and social distancing leading to feelings of loneliness and even lack of direction or drive, Astronomy Club will take you to the cosmos.

See the rest here:

Exploring Astronomy Club and enduring COVID-19 The Mesa Press - Mesa Press

A long-lost type of dark matter may resolve the biggest disagreement in physics – Times Famous

One of the deepest mysteries in physics, known as the Hubble tension, could be explained by a long-since vanished form of dark matter.

The Hubble tension, as Live Science has previously reported, refers to a growing contradiction in physics: The universe is expanding, but different measurements produce different results for precisely how fast that is happening. Physicists explain the expansion rate with a number, known as the Hubble constant (H0). H0 describes an engine of sorts thats driving things apart over vast distances across the universe. According to Hubbles Law (where the constant originated), the farther away something is from us, the faster its moving.

And there are two main ways of calculating H0. You can study the stars and galaxies we can see, and directly measure how fast theyre moving away. Or you can study the cosmic microwave background (CMB), an afterglow of the Big Bang that fills the entire universe, and encodes key information about its expansion.

Related: The 11 Biggest Unanswered Questions About Dark Matter

As the tools for performing each of these measurements have gotten more precise, however, its become clear that CMB measurement and direct measurements of our local universe produce incompatible answers.

Researchers have offered different explanations for the disparity, from problems with the measurements themselves to the possibility we live in a low-density bubble within the larger universe. Now, a team of physicists is suggesting that the universe might have fundamentally changed between the time after the Big Bang and today. If an ancient form of dark matter decayed out of existence, that loss would have changed the mass of the universe; and with less mass, there would be less gravity holding the universe together, which would have impact the speed at which the universe expands leading to the contradiction between the CMB and the direct measurements of the universes expansion rate.

There was a time, decades ago, when physicists suspected dark matter might be hot zipping around the universe at close to the speed of light, said Dan Hooper, head of the Theoretical Astrophysics Group at the Fermi National Accelerator Laboratory in Batavia, Illinois, and co-author of the new paper. But by the mid-1980s they were convinced that this unseen stuff that makes up most of the mass of the universe is likely slower-moving and cold. Physicists refer to the mostly widely-accepted model of the universe as Lambda-CDM, for Cold Dark Matter.

Still, Hooper told Live Science, the idea of warm dark matter a form of dark matter that falls somewhere in between the hot and cold models still gets some traction in the physics world. Some physicists speculate that dark matter is made of sterile neutrinos, for example, theoretical ghostly particles that barely interact with matter. This hypothetical dark matter would be much warmer than typical Lambda-CDM models allow, but not hot.

Another possibility is that most of the dark matter is cold, but maybe some of it is warm. And in our paper, the stuff thats warm isnt even stuff thats around today. Its stuff that was created in the early universe and after thousands or tens of thousands of years it started to decay. Its all gone by now, Hooper said.

Related: 11 fascinating facts about our Milky Way galaxy

That lost dark matters mass would have represented a significant chunk of the total mass of the universe when it existed, leading to a different expansion rate when the CMB formed just after the Big Bang. Now, billions of years later, it would be long gone. And all the stars and galaxies we can measure would be moving away from us at speeds determined by the universes current mass.

When you measure the local Hubble constant youre really measuring that thing: Youre measuring how fast things are moving apart from one another, youre measuring how fast space is expanding, Hooper said. But translating the CMB data into an expansion rate requires using a model, such as the Lambda-CDM. So if you get different measurements from the local measurements and the CMB measurement, maybe that models wrong.

Local measurements measurements of the region of space close enough to Earth for astronomers to precisely measure the speed and distance of individual objects dont require cosmological models to interpret, so theyre typically seen as more straightforward and robust.

Some researchers have still suggested there may be problems with our measurements of the local universe. But most attempts to resolve the Hubble tension involve tweaking Lambda-CDM somehow. Usually, they add something to the model that changes how the universe expands or evolves. This paper, Hooper said, is another step down that road.

Im not going to give the impression that it makes everything great, he said. Its not a perfect concordance among the data by any means. But it makes the tension less severe I dont know of any solution to this, other than the measurements are wrong, that reduces the tension [as much as youd need to fully solve the problem].

Hoopers original proposal to his collaborators on the paper didnt involve warm dark matter at all, he said. Instead, he imagined a second, lost form of cold dark matter. But when they started to test that idea, he said, they found that this extra cold dark matter was screwing up the whole structure of the universe. Stars and galaxies formed in ways that didnt match what we see around us in the universe today. The decayed, lost form of dark matter, they concluded, had to be warm if it was going to fit observations.

The new paper doesnt determine what particles the lost dark matter might be made of, but strongly suggests that warm dark matter might have been made up of sterile neutrinos particles that other physicists also believe are likely out there.

Its definitely the thing that requires the fewest number of tooth fairies to make work, Hooper said. But other possibilities exist.

Whatever it is though, it must have turned into something even more exotic and feebly interacting when it decayed. Matter cant just stop existing; it has to transform into something else. If that something else were distributed differently through the universe, or interacted differently with other particles in the universe, that would change how the universe expanded.

So wed be surrounded in a bath of this dark radiation, Hooper said. Were already surrounded in a bath of neutrinos so this would just be a little bit more of that kind of stuff. Some sort of bath that fills the universe today of very, very inert forms of matter.

For now, researchers dont have methods for probing the for this sort of hidden radiation, Hooper said, so the idea remains speculative. The paper was published to the arXiv database April 13.

Originally published on Live Science.

Click Here To Read More

Like Loading...

Related

View post:

A long-lost type of dark matter may resolve the biggest disagreement in physics - Times Famous

Astronomers Find Earth’s Closest Black Hole (So Far) – The Wire

Featured image: An artists impression depicts the orbits of the two stars and the black hole in the HR 6819 triple system, made up of an inner binary with one star (orbit in blue) and a newly discovered black hole (orbit in red), as well as a third star in a wider orbit (also in blue), in this image released on May 6, 2020. Photo: ESO/L. Calcada/Handout via Reuters

Washington: Astronomers have spotted the closestblackholeto Earth ever discovered and are surprised about its living arrangements residing harmoniously with two stars in a remarkable celestial marriage that may end in a nasty breakup.

Theblackhole, at least 4.2 times the mass of the sun, is gravitationally bound to two stars in a so-called triple system roughly 1,000 light years from Earth, researchers said on Wednesday.

Just around the corner in cosmic terms, said Chile-based European Southern Observatory astronomer Thomas Rivinius, lead author of the study published in the journal Astronomy & Astrophysics.

A light year is the distance light travels in a year, 5.9 trillion miles (9.5 trillion km).

Blackholes are extraordinarily dense objects possessing gravitational pulls so powerful that not even light can escape. Some are monstrous like the one at our galaxys centre 26,000 light years from Earth that is four million times the suns mass.

Also read: A Surprisingly Big Black Hole Might Have Swallowed a Star From the Inside Out

Garden variety so-called stellar-massblackholes like the newly discovered one have the mass of a single star. This one probably began its life as a star up to 20 times the suns mass that collapsed into ablackholeat the end of its relatively short lifespan.

This triple system, called HR 6819, can be seen from Earths southern hemisphere with the naked eye, in the constellation Telescopium. Until now, the closest-knownblackholewas one perhaps three times further away.

Only a few dozen stellar-massblackholes previously were known. But there may be hundreds of millions or even a billion of them in the Milky Way, said astrophysicist and study co-author Petr Hadrava of the Academy of Sciences of the Czech Republic.

Thisblackhole, detected using an observatory in Chile, is minding its manners and has not shredded its two partners: stars about five or six times the mass of the sun. At least not yet.

The formation of ablackholeis a violent process, and most models would not have predicted a triple system could survive that but rather would fly apart, Rivinius said.

Theblackholeforms a pair with one of the two stars, as near to one another as the Earth is to the sun. The other star is much further away, orbiting the pair. This star spins so rapidly that it is misshapen, bulging at the equator.

The two stars are sufficiently distant from theblackholethat it is not pulling material from them. But in a few million years the closer star is expected to grow in size as part of its life cycle.

What happens then is uncertain, Rivinius said. The most spectacular outcome would be if theblackholeends up with that star inside it.

(Reuters)

Read the rest here:

Astronomers Find Earth's Closest Black Hole (So Far) - The Wire

Student mothers describe increased stressors as COVID-19 mixes home and work – Daily Northwestern

On a regular weekday during the COVID-19 pandemic, graduate students like Heather McCambly and Nikki McDaid-Morgan are teaching classes, grading and meeting with students while providing childcare.

McCambly, a SESP Ph.D. student who is in her fourth year studying racial justice, is collecting data on the pandemic while full-time parenting her 4-year-old daughter and ensuring she is emotionally supported.

Im trying to figure out how to help my kid keep learning and also mostly just be OK, McCambly said. (My child is) definitely feeling whats going on in the world and on this planet right now. And she needs a lot of attention.

Life-work balance has become difficult for many amid coronavirus, as remote work pushes the office into living spaces. Parents have had to balance childcare duties with professional duties. Women already bore the brunt of domestic work in heterosexual couples a dynamic highlighted further by the pandemic.

McCambly recently took her daughter to see a doctor because she was showing symptoms related to stress part of which comes from the drastic transition from daycare to homeschooling due to the pandemic.

Going to the doctors office during the pandemic, McCambly said, didnt feel safe. The experience compounded the stress.

I might put being a researcher before most things in my life, McCambly said. And for better or for worse.

Between McCambly and her husband, she said he performs more childcare than she does. Yet she told The Daily she still finds herself completing less and less academic work.

Shes not alone. Academic journal committees across subjects have seen the number of article submissions by female-identifying researchers plummet, with a deputy editor of the British Journal for the Philosophy of Science noting that she has never seen anything like it.

Even though not all female-identifying researchers are mothers or caregivers for elderly parents, they are more burdened with completing domestic work in heterosexual relationships, with childcare being one such task.

Disciplines such as astrophysics have witnessed up to 50 percent productivity loss, with submissions by female researchers to academic journalists noticeably decreasing. Comparative Political Studies, a journal that publishes on a subject less disproportionately male-dominated than astrophysics, has seen a consistent number of submissions by women this year and a 50 percent increase by men.

McDaid-Morgan, another SESP Ph.D. student who has two children, said she said she felt hyper-productive before the coronavirus closed Northwesterns campus.

Now, her timeline has been pushed back. McDaid-Morgans dissertation proposal, which she she was due to defend last month, has been delayed. Her 4-year-old is bedwetting again, partially due to stress. On top of this, the student is expected to produce the same level of academic work.

My identity is wrapped up in being a researcher and an educator and a learning scientist, McDaid-Morgan said. Now that we cant be on campus anymore, my own mental health has declined and its hard for me to get work done.

In the past, McDaid-Morgan tried to separate work from home because doing work at home may lead to the children feeling neglected. Now, she said she has no choice.

Both doctoral candidates told The Daily that they are a skewed example, as their partners play an equal or larger role in parenting and other household duties. They said they know a colleague whose partner is an essential worker and has to raise three children.

At the same time, both McCambly and McDaid-Morgans husbands are temporarily unemployed due to the pandemic. Academia is already a precarious workforce. If they graduate on course, they may not be entering a desirable job market.

Its really taking a lot out of me emotionally to reconcile, McCambly said. Ive done all the right things, Im continuing to do the right thing. I love my work. And I cannot count on my university right now to kind of have my back in this moment (and) long term in terms of making sure that I can pursue the academic career I came here to pursue.

Northwestern University Graduate Workers have been advocating for an additional year of funding since April through the hashtag #universal1yr and other organizing efforts.

The University has not acted to extend an additional year of funding to graduate students in light of the pandemic, despite receiving numerous endorsements of #universal1yr from the political science department, African American Studies department, the School of Communication and more.

During NUGWs May 1 virtual sit-in, Alcia Hernndez Grande, a Ph.D. candidate, said that doing graduate work and taking care of her young daughter full-time during a pandemic has taken away time from her studies.

As a graduate student (and) parent, my work time is limited, Hernndez Grande said. I am trying to do the best that I can, but without childcare, without the possibility of childcare, without knowing when childcare might be available, I am at the mercy of nap-times, I am at the mercy of my own energy levels as I try to do full-time parenting.

On the other side of the situation, the loss of time also takes away formative opportunities for children. McDaid-Morgan, who is from the Shoshone-Bannock Nation, helps design a summer program for indigenous youths. There, her children are able to interact and be part of the community. Due to the coronavirus, the camp is not happening this summer.

Adults are dealing with similar losses. McDaid-Morgan and McCambly, who is Latinx, are from communities disproportionately impacted by COVID-19. McDaid-Morgan said that Native Americans in Seattle who she collaborates with for research told her that instead of the funding and personal protective gear tribes asked for, the federal government sent them body bags.

At Northwestern, McDaid-Morgan used to go to the Center for Native American and Indigenous Research to meet up with members of the community. Now, she cant and said she is tired of sitting in front of computers to socialize.

Were all missing our community, McDaid-Morgan said. Its hard, and then its lonely.

Email: yunkyokim2022@u.northwestern.eduTwitter: @yunkyomoonk

Related Stories: Graduate workers hold #universal1yr rally on International Workers Day to highlight academic worker concerns Faculty and staff juggle parenting with remote work

Read the rest here:

Student mothers describe increased stressors as COVID-19 mixes home and work - Daily Northwestern

Search For Intelligent Alien Life: Galaxies That Are More Likely to Harbor Technologically Advanced Civilizations – SciTechDaily

Galaxies such as our own Milky Way are more likely to harbor intelligent, technologically advanced civilizations.

Giant elliptical galaxies are not as likely as previously thought to be cradles of technological civilizations such as our own, according to a recent paper by a University of Arkansas astrophysicist.

The paper, published May 1 in the journal Monthly Notices of the Royal Astronomical Society, contradicts a 2015 study that theorized giant elliptical galaxies would be 10,000 times more likely than spiral disk galaxies such as the Milky Way to harbor planets that could nurture advanced, technological civilizations.

The increased likelihood, the authors of the 2015 study argued, would be because giant elliptical galaxies hold many more stars and have low rates of potentially lethal supernovae.

But Daniel Whitmire, a retired professor of astrophysics who is an instructor in the U of A mathematics department, believes that the 2015 study contradicts a statistical rule called the principle of mediocrity, also known as the Copernican Principle, which states that in the absence of evidence to the contrary, an object or some property of an object should be considered typical of its class rather than atypical.

Historically, the principle has been employed several times to predict new physical phenomena, such as when Sir Isaac Newton calculated the approximate distance to the star Sirius by assuming that the sun is a typical star and then comparing the relative brightness of the two.

The 2015 paper had a serious problem with the principle of mediocrity, said Whitmire. In other words, why dont we find ourselves living in a large elliptical galaxy? To me this raised a red flag. Any time you find yourself as an outlier, i.e. atypical, then that is a problem for the principle of mediocrity.

He also had to show that most stars and therefore planets reside in large elliptical galaxies in order to nail down his argument that the earlier paper violated the principle of mediocrity.

According to the principle of mediocrity, Earth and its resident technological society should be typical, not atypical, of planets with technological civilizations elsewhere in the universe. That means that its location in a spiral-shaped disk galaxy should also be typical. But the 2015 paper suggests the opposite, that most habitable planets would not be located in galaxies similar to ours, but rather in large, spherical-shaped elliptical galaxies.

In his paper, Whitmire suggests a reason why large elliptical galaxies may not be cradles of life: They were awash in lethal radiation when they were younger and smaller, and they went through a series of quasar and star-burst supernovae events at that time.

The evolution of elliptical galaxies is totally different than the Milky Way, said Whitmire. These galaxies went through an early phase in which there is so much radiation that it would just completely have nuked any habitable planets in the galaxy and subsequently the star formation rate, and thus any new planets, went to essentially zero. There are no new stars forming and all the old stars have been irradiated and sterilized.

If habitable planets hosting intelligent life are unlikely in large elliptical galaxies, where most stars and planets reside, then by default galaxies such as the Milky Way will be the primary sites of these civilizations, as expected by the principle of mediocrity, Whitmire said.

Reference: The habitability of large elliptical galaxies by Daniel P Whitmire, 13 April 2020, Monthly Notices of the Royal Astronomical Society.DOI: 10.1093/mnras/staa957

Read the original:

Search For Intelligent Alien Life: Galaxies That Are More Likely to Harbor Technologically Advanced Civilizations - SciTechDaily

UWMadison announces its fourth round of cluster hires – University of Wisconsin-Madison

Artificial intelligence, ethics in technology, the origins of life, astrophysical data these exciting but complex subjects are the focus of the University of WisconsinMadisons fourth round of cluster hires, the Office of the Provost announced today.

The hires, which are made as a group across departments rather than individually within departments, build upon the universitys existing strengths. They foster collaborative research, education and outreach by creating new interdisciplinary areas of knowledge.

UWMadison first launched the Cluster Hiring Initiative in 1998 as an innovative partnership between the university, state and the Wisconsin Alumni Research Foundation. In its first phase, the initiative authorized nearly 50 clusters, adding nearly 150 new faculty members through several rounds of hiring. In 2017, the Office of the Provost authorized phase two of the initiative, with a goal of supporting at least 12 clusters.

Previous clusters were announced in April 2019 andSeptemberandFebruaryof 2018. This latest round brings the total of clusters supported to 19. In light of the COVID-19 pandemic, however, each cluster will be given at least two years to complete its hiring plans. New cluster competition will be suspended for at least the next academic year.

The latest cluster hires are:

Artificial Intelligence in Precision Medical Imaging and Diagnostics

Proposal advanced by: Thomas Grist, professor of radiology, medical physics and biomedical engineering; Kristin Eschenfelder, associate director of the School of Computing, Data and Information Sciences; Rob Nowak, professor of electrical and computer engineering, computer sciences, statistics and biomedical engineering; Vallabh Sambamurthy, dean of the Wisconsin School of Business.

Through new approaches to data acquisition and analysis, advances in artificial intelligence are poised to revolutionize the way in which medical imaging affects clinical care and scientific discoveries in medicine. This cluster outlines three key faculty positions that will be foundational to an expansion of UWMadisons leadership in the field. It will also address urgent opportunities for curriculum development in areas of interest to multiple colleges and schools on campus and extramural entities.

Next-generation medical imaging uses AI techniques to improve its diagnostic accuracy and predictive power, enabling advances in basic understanding of human disease, treatment monitoring and long-term surveillance of disease.

Collaborations like those forged by the cluster hire will contribute to the realization of the full potential of AI for precision medical imaging and diagnostics.

Ethics in Computing, Data, and Information

Proposal advanced by: Alan Rubel, professor in the Information School and director of the Center for Law, Society and Justice; Michael Titelbaum, Vilas Distinguished Achievement Professor and Chair of the Department of Philosophy; Loris DAntoni, professor of computer sciences; Aws Albarghouthi, professor of computer sciences; Noah Weeth Feinstein, director of the Holtz Center for Science, Technology and Society and a professor of curriculum and instruction and community and environmental sociology.

Computational systems, data analytics, artificial intelligence and algorithmic decision systems affect large and important facets of society, including governance, education, commerce, democracy and media. These tools can be used to advance social goods, but they can also go awry, used for bad purposes by bad actors. The tools can also reflect and engender unfair social structures.

To effectively address ethical issues in AI, data, and information systems requires collaboration between scholars working on computational systems, on the social facets of information technologies, and on conceptual and moral questions about how such systems function and how they are used.

UWMadison is well-positioned to be a world leader in these areas because of its current strengths and existing collaborations. The cluster proposes hiring three faculty members working on distinct facets of the ethics of computing, data and information.

Exploring the Origins of Life Across the Galaxy

Proposal advanced by: Sebastian Heinz, professor and chair of astronomy; David Baum, professor of botany; Judith Burstyn, professor and chair of chemistry; Greg Tripoli, professor and chair of atmospheric and oceanic sciences; Jeff Hardin, professor and chair of integrative biology; Ken Cameron, professor and chair of botany; Chuck DeMets, professor and chair of geoscience; Annie Bauer, assistant professor of geoscience; Tristan LEcuyer, professor of atmospheric and oceanic sciences; Robert Mathieu, professor of astronomy; Steve Meyers, professor of geoscience; Phillip Newmark, professor of integrative biology; Andrew Vanderburg, assistant professor of astronomy; Susanna Widicus Weaver, professor of chemistry; John Yin, professor of chemical and biological engineering; Tehshik Yoon, professor of chemistry; Ke Zhang, assistant professor of astronomy.

Questions about the origins and nature of life are as old as humanity itself. Today, the search for understanding the origin of life extends to the cosmos, as recent work has uncovered countless planets orbiting stars throughout the Milky Way, each potentially bearing life of its own. But how do we detect life on planets we can never visit? And how do we know how common life might be if we dont know how it arose on Earth?

The search for evidence of life on other planets is by nature interdisciplinary. Chemistry, biology and geoscience combine to understand how life arose on our planet and how it might have done so on other worlds, while astronomy and atmospheric sciences can probe for evidence of that life from light-years away. This cluster will allow the hiring of researchers who straddle these fields and who can bridge the gaps between expertise across the participating departments. The group will also establish the Wisconsin Center for Origins Research to house new and existing faculty and encourage new collaborations in astrobiology.

Breakthrough Science with Multi-messenger Astrophysical Data

Proposal advanced by: Albrecht Karle, professor of physics; Keith Bechtol, assistant professor of physics; Francis Halzen, professor of physics; Kael Hanson, professor of physics; Sebastian Heinz, professor and chair of astronomy; Sebastian Raschka, assistant professor of statistics; Justin Vandenbroucke, associate professor of physics; Jun Zhu, professor and chair of statistics; Ellen Zweibel, professor of astronomy.

For millennia, humans learned about the night sky only from the light from distant stars. But recently, astrophysicists have gained access to signals that go beyond light. These messengers about the universe include gravitational waves and neutrinos ghostly particles that rarely interact with other matter. UWMadison is the headquarters of the worlds largest neutrino observatory, IceCube, which surveys a billion tons of Antarctic ice for signs of rare neutrino collisions.

Now, the IceCube project is preparing for a major upgrade to generation two. This cluster hire will invest in the astronomy, physics and statistics faculty necessary to continue and expand UWMadisons leadership in multi-messenger astrophysics. This data-heavy field requires collaborations between these three fields to probe the constant stream of information recorded by IceCube and to find the sources of the neutrinos that stream toward Earth. That analysis can help answer fundamental questions about the physical laws governing the universe and help us understand complex phenomena like black holes and cosmic rays.

Share via Facebook

Share via Twitter

Share via Linked In

Share via Email

See the rest here:

UWMadison announces its fourth round of cluster hires - University of Wisconsin-Madison