Daily Archives: June 12, 2017

Sometimes, its our closest neighbors that are the most difficult to spy on. Case in point: The Luhman 16 AB system, which is the third-closest stellar system to our Sun, yet was not discovered until 2013. After three years of subsequent monitoring, a stack of 12 images taken with the Hubble Space Telescope (HST) has confirmed that the system is composed of two brown dwarfs and no third companion, as was originally suspected.

A team of astronomers led by Luigi Bedin watched the two visible stars, Luhman 16 A and Luhman 16 B, over the course of three years between August 22, 2014, and October 4, 2016. During this time, HST has imaged the system 12 times (with a thirteenth proposed visit in August 2018). Using these images, they were able to determine several orbital parameters of the stars, as well as more accurately measure their distance and search for any potential exoplanets in the system. Their results have been accepted for publication in the Monthly Notices of the Royal Astronomical Society.

Bedin and his team used their sequence of Hubble images to watch the two brown dwarfs dance across the sky. In particular, they were looking for a third potential body in the system, such as a large exoplanet, which had been indicated by the stars motion in previous observations with the European Southern Observatory's Very Large Telescope. However, according to Bedins group, the new Hubble measurements rule out the presence of a third body in the system, all the way down to planets of Neptunes mass with a period between one and two years. Thus, if the system does harbor exoplanets, they must be smaller than Neptune and take longer than one to two Earth years to circle their sun.

Brown dwarfs are often called failed stars because they are too small to sustain the fusion processes that create energy inside stars. While these bodies can sometimes fuse a hydrogen isotope known as deuterium, even this phase doesnt last very long, relatively speaking, leaving the star to essentially cool off over cosmic time and grow dark.

However, astronomers know that there are many more low-mass objects in the universe than high-mass ones. Thus, because of their increased number, these lower-mass objects are an extremely fertile place to look for exoplanets.

Luhman A and B circle each other once every two to four decades, with a distance between them of about 3 astronomical units (three times the distance between the Sun and Earth). The system itself is located within about 2 parsecs of the Sun, or 6.5 light-years. Only the Alpha Centauri system and Barnard's Star are closer.

Because the Luhman 16 AB system is so close to the Sun, its the perfect place to study brown dwarfs, which are hard to see because theyre both small and dim, up close. Bedins team plans to continue their study of the stars to both improve the precision of their measured orbital parameters and to search for ever-smaller, Earth-sized exoplanets in the system.

The rest is here:

Hubble spies on nearby brown dwarfs - Astronomy Magazine

Investigating how languages emerge and evolve. Using climate-change data to predict dust storms and bacterial meningitis outbreaks in Northern Africa. Understanding whether age-related diseases may stem from a common driver. Determining whether the presence of oxygen can be used to predict life on distant exoplanets.

Harvard scientists are known for pushing boundaries, but the projects funded through the 2017 Star Family Challenge for Promising Scientific Research are poised to take that reputation to new heights.

Created through a gift from James A. Star 83, the annual challenge funds high-risk, high-reward research that might not receive funding through other programs.

I want to salute the winners of the 2017 Star Family Challenge, Star said. This is a wonderful set of projects, and I look forward to hearing about them. I also want to thank Professor Randy Buckner and his committee for taking over from [former chairman] Doug Melton and moving the challenge forward.

As part of the program, the faculty members selected for the awards Jesse Snedeker, Elsie Sunderland, Caroline Buckee, Amy Wagers, and Robin Wordsworth made short presentations on their work to a standing-room-only crowd in the Faculty Room of University Hall.

We live in a time in which the funding of science faces threats, said Buckner, a professor of psychology and of neuroscience. It is unlikely the funding of science is going to become more risk-taking, more imaginative, or more centered on the blue-sky projects which excite so many people here today.

The need for the type of funding the Star Family Foundation is providing is going to become ever more critical, he continued. Your support means a very great deal.

Jesse Snedeker

Language is ubiquitous, said Snedeker, a professor of psychology, describing her project. Everywhere in the world you will find people talking to one another. These languages have many properties in common they all use nouns and verbs, they all have grammatical rules, and all languages are acquired by young children over a very short period. But there is also remarkable diversity of language they can vary in their words, in the specific grammatical structures that they allow, and in their sounds.

The basic question Snedeker hopes to address is one that has long been at the center of psychological research: Where does language come from?

Its an extremely difficult problem, she noted, because while the first humans left Africa at least 60,000 years ago, written records of language begin only about 5,000 years ago. What researchers can examine are the languages created by deaf communities.

Working with the deaf community in Nicaragua, Snedeker and colleagues plan to collect data on shared words, grammatical rules, and social networks among students from the 1970s through the 1990s with the goal of understanding how language changed over time.

What other researchers have discovered is that the first cohort those students that came into the schools in the 70s had shared signs for certain words and ordered narratives, but they do not reliably mark which argument is the subject and which is the object with either word order, like English, or case marking, like Russian or Turkish, Snedeker said. But by the time the later cohorts come in, they use verbal inflection about 50 percent of the time, and subject, object, verb word order the rest of the time.

This rapid pattern of evolution of language raises some interesting questions, Snedeker added. The first were going to be asking is: Why havent these older signers picked up on what the younger people around them are doing? Theyre part of a larger community, yet they havent adopted the regularities that the 20- and 30-year-olds are using.

Working with Martin Nowak, a professor of biology and mathematics and director of the Program for Evolutionary Dynamics, and Annemarie Kocab, a Ph.D. candidate in psychology, Snedeker hopes to create computational models that can provide new insight into the social dynamics that drive language.

Amy Wagers

When you consider the greatest risk factor for many diseases, says Wagers, the Forst Family Professor of Stem Cell and Regenerative Biology, it all comes down to one word: aging.

There is growing evidence that diseases such as cancer, cardiac disease, and cognitive decline today viewed as separate medical challenges could be treated by targeting their age-related roots, Wagers said.

The underlying goal of this project is to understand the fundamental physiological processes of the natural process of aging, and then understand how those impact health, Wagers said. [With] that understanding, can we develop therapies or other interventions that allow us to take aim at that root cause, or develop strategies that could be applied across different diseases of aging which have typically been thought of as independent.

The notion that many age-related diseases may share a common driver was inspired in part by the discovery of mutations in circulating blood cells that accumulate with age and lead to clonal hematopoiesis problems in the formation of blood. Wagers and colleagues hope to investigate a new hypothesis that those mutations, and the problems they cause, may be a common driver of age-associated dysfunction across organ systems.

What this project will allow us to do is clarify the relevance of these age-related [mutations], Wagers said. This will allow us to understand whether there is therapeutic value in targeting those clones.

Working with Lee Rubin, a professor of stem cell and regenerative biology, and Richard T. Lee, a professor of stem cell and regenerative biology and of medicine, Wagers plans to use CRISPR technology to introduce specific mutations associated with clonal hematopoiesis in humans into young and middle-aged mice, and monitor the rate of emergence of age-associated pathologies in three different organ systems: skeletal muscle, the brain, and the heart.

Elsie Sunderland

Seasonal change and illness often go hand in hand, but in West Africa, the combination can be deadly.

Every year, dust storms across the region are accompanied by devastating epidemics of bacterial meningitis, which has a mortality rate of 50 percent when left untreated, said Sunderland, the Thomas D. Cabot Associate Professor of Environmental Science and Engineering at the John A. Paulson School of Engineering and Applied Sciences and an associate professor of environmental science and engineering at the Harvard T.H. Chan School of Public Health.

Though its thought that the dust irritates the throat, making people more susceptible to disease, Sunderland plans to test an alternative hypothesis that meningitis bacteria are carried on the winds that drive those dust storms.

Microbes can be transported on aerosols like dust, Sunderland said. And these dust storms are very much a function of global climate so the intensity of these storms has been changing quite a bit over the last number of years. This is a very dynamic phenomenon that we are trying to link to the spread of meningitis in the area.

Sunderlands partner on the project is Buckee, an infectious disease epidemiologist from the Harvard Chan School, who said that while there has long been evidence of correlation between the dust storms and the outbreaks, the mechanism behind the link has been unclear.

Along with Buckee, Sunderland has recruited help from Tovi Lehmann of the National Institutes of Health, who samples insect populations on wind currents in Mali using helium balloons, and Stephen Bentley, a bacterial genomics expert at the Wellcome Trust Sanger Institute.

The group plans to use helium balloons and microbial collection devices to sample aerosols transported by winds in Mali, sequence the bacterial genomes that are collected, and assess the risk of atmospheric spread of meningitis and other windborne pathogens.

The idea is to provide some metrics to use for modeling to better understand these outbreaks, and to potentially use for forecasting, Sunderland said. Thats a major benefit for the practice of public health and being able to identify where vulnerable populations are.

Robin Wordsworth

With every discovery of a new exoplanet, interest in the idea that one may hold extraterrestrial life gains momentum. But how will that life be detected if the technology doesnt exist to send probes into deep space?

One possible method, says Wordsworth, an assistant professor of environmental science and engineering at SEAS, may be in detecting oxygen in the atmosphere of other planets.

Whats really fascinating and exciting about this to me is that for the first time on a large scale this question of extraterrestrial life is no longer something which is purely in literature or science fiction, Wordsworth said. Its something we can start to address scientifically.

Though there is wide evidence that oxygen in Earths atmosphere is due to the presence of life, there is debate about whether the gas is a reliable biosignature, because recent research has shown that some planets can produce oxygen-rich atmospheres abiotically.

In an effort to resolve that debate, Wordsworth and collaborators David Charbonneau, a professor of astronomy, and Dimitar Sasselov, Phillips Professor of Astronomy and director of the Harvard Origins of Life Initiative, plan to construct advanced planetary evolution models that incorporate atmospheric, surface, and interior processes to simulate the early years of a planets development the period that most affects a planets oxygen accumulation.

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Inquiring minds rewarded - Harvard Gazette

HE WAS a Gisborne Astronomical Society star but the late Huon Chandler preferred to stay out of the limelight, says society president John Drummond of his long-time friend.

Mr Chandler was the societys long-standing treasurer and public nights presenter.

Devoted to the society since the early 1970s, the Cook Observatory was like his second home, said Mr Drummond in his eulogy.

Few know he paid the monthly power bills out of his own pocket when the society was at its ebb.

He also regularly mowed the grass around the Cook Observatory for years and painted over graffiti as soon as it appeared on the observatory.

Mr Chandler ran public nights every Tuesday for about 25 years and his talks on cosmology and others aspects of astronomy were legendary.

Those public nights even made it into the New Zealand Lonely Planet section on Gisborne.

There are undoubtedly many other things that Huon did for the society and observatory that even I dont know, said Mr Drummond.

Born in Dunedin in 1947, Mr Chandler joined the Inland Revenue Department on leaving school. When his family moved to Gisborne a few years later, he moved here too.

He met his future wife, Carol, during a holiday in USA and in 1976. They married in Gisborne and raised two boys, Joseph and Matthew.

Mr Chandlers varied career usually included a computer.

A passionate reader, Mr Chandler had a particular penchant for science fiction and loved fantasy games.

When computer fantasy games became available, he was in his element.

He was equally in his element on starry nights.

Mr Drummond recalls those nights.

We discussed everything from astronomy, to politics, to God and, of course his family, which he always spoke of with pride and excitement.

I remember one night on the roof of the Cook Observatory when Huon and I were observing a meteor shower.

We got to talking about the movie Blazing Saddles and noticed more meteors.

Later we revisited that comedy-western and again saw an increase in meteors.

This happened a number of times during the night. It was a unique experience to us both and one that we joked about for many years after.

Mr Chandler died on May 26 after several months of illness.

Farewell my old meteor-observing buddy, said Mr Drummond.

May you shine like a star in your new abode forever.

HE WAS a Gisborne Astronomical Society star but the late Huon Chandler preferred to stay out of the limelight, says society president John Drummond of his long-time friend.

Mr Chandler was the societys long-standing treasurer and public nights presenter.

Devoted to the society since the early 1970s, the Cook Observatory was like his second home, said Mr Drummond in his eulogy.

Few know he paid the monthly power bills out of his own pocket when the society was at its ebb.

He also regularly mowed the grass around the Cook Observatory for years and painted over graffiti as soon as it appeared on the observatory.

Mr Chandler ran public nights every Tuesday for about 25 years and his talks on cosmology and others aspects of astronomy were legendary.

Those public nights even made it into the New Zealand Lonely Planet section on Gisborne.

There are undoubtedly many other things that Huon did for the society and observatory that even I dont know, said Mr Drummond.

Born in Dunedin in 1947, Mr Chandler joined the Inland Revenue Department on leaving school. When his family moved to Gisborne a few years later, he moved here too.

He met his future wife, Carol, during a holiday in USA and in 1976. They married in Gisborne and raised two boys, Joseph and Matthew.

Mr Chandlers varied career usually included a computer.

A passionate reader, Mr Chandler had a particular penchant for science fiction and loved fantasy games.

When computer fantasy games became available, he was in his element.

He was equally in his element on starry nights.

Mr Drummond recalls those nights.

We discussed everything from astronomy, to politics, to God and, of course his family, which he always spoke of with pride and excitement.

I remember one night on the roof of the Cook Observatory when Huon and I were observing a meteor shower.

We got to talking about the movie Blazing Saddles and noticed more meteors.

Later we revisited that comedy-western and again saw an increase in meteors.

This happened a number of times during the night. It was a unique experience to us both and one that we joked about for many years after.

Mr Chandler died on May 26 after several months of illness.

Farewell my old meteor-observing buddy, said Mr Drummond.

May you shine like a star in your new abode forever.

See the article here:

Stalwart of astronomy and proud family man - Gisborne Herald

A team of astronomers has determined how the gas flow from a massive infant star is launched. The researchers used the Atacama Large Millimeter/submillimeter Array (ALMA) to observe the 10-solar-mass protostar Orion KL Source I in the Kleinmann-Low Nebula and obtained clear evidence of rotation in the outflow.

Artists impression of Orion KL Source I. The massive protostar is surrounded by a disk of gas and dust. The outflow is launched from the surface of the outer disk. Image credit: ALMA / ESO / NAOJ / NRAO.

Stars form from gas and dust floating in interstellar space. But, astronomers do not yet fully understand how it is possible to form the massive stars seen in space.

One key issue is gas rotation. The parent cloud rotates slowly in the initial stage and the rotation becomes faster as the cloud shrinks due to self-gravity.

Stars formed in such a process should have very rapid rotation, but this is not the case. The stars observed in the Universe rotate more slowly.

How is the rotational momentum dissipated? One possible scenario involves that the gas emanating from protostars.

If the gas outflow rotates, it can carry rotational momentum away from the system.

Astronomers have tried to detect the rotation of the outflow to test this scenario and understand its launching mechanism.

In a few cases signatures of rotation have been found, but it has been difficult to resolve clearly, especially around massive protostars.

Orion KL Source I observed with ALMA. The massive protostar is located in the center and surrounded by a gas disk (red). A bipolar gas outflow is ejected from the protostar (blue). Image credit: ALMA / ESO / NAOJ / NRAO / Hirota et al.

Dr. Tomoya Hirota, an astronomer at the National Astronomical Observatory of Japan (NAOJ) and SOKENDAI, and colleagues observed a protostar called Orion KL Source I in the Kleinmann-Low Nebula, the most active part of the Orion Nebula complex.

Thanks to its close vicinity and ALMAs advanced capabilities, Dr. Hirota and co-authors were able to reveal the nature of the outflow from Orion KL Source I.

We have clearly imaged the rotation of the outflow. In addition, the result gives us important insight into the launching mechanism of the outflow, Dr. Hirota said.

The new ALMA observations beautifully illustrate the rotation of the outflow: it rotates in the same direction as the gas disk surrounding the star; this strongly supports the idea that the outflow plays an important role in dissipating the rotational energy.

Furthermore, ALMA clearly shows that the outflow is launched not from the vicinity of Orion KL Source I itself, but rather from the outer edge of the disk. This morphology agrees well with the magnetocentrifugal disk wind model.

The findings appear today in the journal Nature Astronomy.

_____

Hirota et al. Disk-Driven Rotating Bipolar Outflow in Orion Source I. Nature Astronomy, published online June 12, 2017

Go here to see the original:

ALMA Observes Massive Protostar in Kleinmann-Low Nebula - Sci-News.com

The origin of the notorious Wow! Signala 72 second-long astronomical anomaly some scientists first thought to have been a signal from extraterrestrial lifehas been a constant source of speculation for alien hunters ever since it was recorded in 1977 by Ohio State University's Big Ear radio telescope.

Was it a radio signal sent by E.T. or just something more mundanely human?

A new scientific paper, published in the Journal of the Washington Academy of Sciences, claims to have finally nailed it, sparking a flurry of press coverage proclaiming the mystery finally solved. According to the study author, Antonio Paris of St. Petersburg College in Florida, the answer lies in a passing comet called 266P/Christensen (only discovered in 2006) that caused the 1420MHz 'Wow!' radio signal detected some forty years ago.

Paris' research claims to have confirmed that comets emit a 1420MHz signal. Thus, he goes on to argue, this is likely what the telescope picked up on when the comet passed in front of the area of the sky the it was pointed at.

But Paris' conclusion doesn't have fellow astronomers convinced.

"There are some problems with the analysis, which doesn't use many of the standard things one would do in radio astronomy," Chris Lintott, professor of astrophysics at the University of Oxford, told Motherboard.

"The paper appears in a journal that I hadn't heard of before Paris published his Wow/comet ideas in thereit may be peer reviewed, but it's not part of the astronomical mainstream and so I'd be worried about the quality of that review."

"You may as well say it's due to ghosts or due to reality television"

So between interrogative tweets and doubting Reddit threads, Motherboard reached out to Paris to ask what's really going on.

"I have received over 500 emails this week about the Wow paper. About 99.99 percent appear [to be] positive reaction from the public and the scientific community," Paris told Motherboard in an email. "A handful, however, were from those who are still skeptical, mostly from the SETI (Search for Extraterrestrial Life) community. I suspect that SETI, who has used the Wow signal as a source of revenue, is nervous."

SETI, for its part, says such claims are preposterous: "We haven't made any money on the Wow signal whatsoever," Seth Shostak, senior astronomer for the SETI Institute, told Motherboard. "The charge we're making a lot of money off of it is bizarre. It's a bogus claim."

Shostak says he finds Paris's paper hard to believe based on what other astronomers have observed.

"The Ohio State radio telescope has two receivers on it. If it observes something in the sky, it's always reobserved 70 seconds later with a second feed," he said. "With Wow, it found it in one feed but it doesn't find it in the second. It's disappeared. A comet doesn't disappear in a minute. It doesn't move across the sky in a minute. It barely moves at all."

Paris said he had even received a phone call from a technician who helped build the Big Ear telescope who was excited that "the mystery has been solved." But Paris' research is still in the firing line.

"Saying 'The Wow signal might not be a comet if comets do something we haven't seen them doing' seems not very exciting."

"The claimed detectioneven if it's realis much, much weaker than the Wow signal, and lasts for longer. So at best the paper shows that comets are detectable in the radionot that they're capable of the kind of burst that produced the Wow signal," Lintott told Motherboard. "Saying 'The Wow signal might be a comet if comets do something we haven't seen them doing' seems not very exciting."

A Reddit user, also claiming to be a radio astronomer, posted a lengthy takedown of Paris' paper over the weekend, arguing, "This paper was also just really, really, really short on details that a radio astronomer would want, to the point where it likely wouldn't have passed a referee at a 'regular' journal."

The Wow! signal. Its name inspired by astronomer Jerry R. Ehman, who discovered the anomaly in August 1977. Image: Big Ear Radio Observatory and North American AstroPhysical Observatory (NAAPO).

But Paris has kicked back against what he calls an "emotional" response. "I am not in the business of responding to emotions," he told Motherboard. "There are too many people 'excited' or 'upset' about this project. Emotions should not have any part in science."

Shostak said that the comet explanation "would be an interesting result if true," but that the data just doesn't back it up: "You may as well say it's due to ghosts or due to reality television or something. If the explanation doesn't fit the data, you have to be a little suspect."

To that end, Lintott has spent the weekend putting together a public list of questions for Paris to answer about his paper, including contributions from other astronomers. The search for extraterrestrial life continues.

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Read more here:

The Controversy Over the Alien 'Wow!' Signal Is Astronomy's Greatest Beef - Motherboard

Waikato Museum exhibition "Te Whnau Mrama: The Heavenly Bodies" was a double-finalist at the New Zealand Museum Awards.

Curated by Dr Rangi Matamua, Dr Hemi Whaanga, Dr Ann Hardy and Hohepa Tuahine from the University of Waikato, the exhibition shines the spotlight on Mori astronomy and how it is being revitalised.

Supported by taonga, photographs and krero, Te Whnau Mrama opens the door on tuning into the stars and a better understanding of the history and meaning of Matariki.

Dr Rangi Matamua (Thoe) is an associate professor at the University ofWaikato.

He states, The right time to look for Matariki is at the end of June or the beginning or middle of July. That's Pipiri according to the Mori calendar. This year, its from July 17 to July 20 when the moon is in the Tangaroa phase in the month ofPipiri.

Matamua maintains that Mori astronomy is not practised as widely as it once was.

I want this system of knowledge of astronomy to be revitalised in our modern world. We haveforgottenhow to read the stars. However, the knowledge is still there today.

The exhibition was a finalist in the Excellence: Taonga Mori and Most Innovative Use of Te Reo Mori categories.

It incorporates Mori legend, tradition, architecture, music and history to convey the spoken and written language within the exhibition.

Although the exhibition was not a winner, Matamua maintains that the overall aim is the dissemination and revival of traditional Mori knowledge.

The hope is for Mori to return to the environment, to the origin of Mori language and philosophy, governing principals and protocols everything that came from the environment.

The Te Whnau Mrama: The Heavenly Bodies exhibition is on at Waikato Museum and runs until 13 July 2018.

Excerpt from:

Mori Astronomy exhibition double-finalist at NZ Museum Awards - Mori Television