Tag Archives: Distant

Exoplanets dance around distant star in 12-year timelapse

Four Jupiter-mass exoplanets dance around their parent star in a stunning new timelapse collected over a dozen years.

The aim of the newly released video is to make the long orbits of these massive exoplanets more recognizable to a wide audience, Northwestern University astrophysicist Jason Wang said in a statement (opens in new tab).

“This video shows planets moving on a human time scale. I hope it enables people to enjoy something wondrous,” said Wang. In real life, the planet nearest the star HR8799 takes 45 years to make a single circuit. The world farthest away would take half a millennium (500 years) to go around the star once.

Related: 9 alien planet discoveries that were out of this world in 2022

A timelapse animation of the four exoplanets “dancing” around the star HR8799. (Image credit: Jason Wang/Northwestern University)

HR8799 is 1.5 times more massive than our sun and lies roughly 133 light-years from Earth in the constellation Pegasus. (By comparison, the closest star system to us, Alpha Centauri⁠, is a bit more than 4 light-years away.)

While a bit more massive than our sun, HR8799 is much more luminous: it has five times the intrinsic brightness of Earth’s start. HR8799 is also very young at just 30 million years, compared with our midlife sun, which is 4.5 billion years old. 

Three planets in the HR8799 system. The planets, thought to be gas giants more massive than Jupiter, were first imaged in 2008 and are shown here in a vortex coronagraph image. (Image credit: NASA/JPL-Caltech/Palomar Observatory)

HR8799 was the first star system ever to have its planets directly imaged, which was accomplished and announced in November 2008. The new timelapse uses footage from the W. M. Keck Observatory atop Maunakea in Hawaii. 

Keck has great advantages for astronomy: adaptive optics to compensate for the blurring effects of Earth’s atmosphere, and a coronagraph that blocks the light from the parent star, allowing the reflected-light “fireflies” (planets) to shine through.

Wang and his colleagues created one timelapse after using seven years of periodic observations. The newly released timelapse is an updated version, with 12 years of observations from when Wang’s team had access to the telescope.

“There’s nothing to be gained scientifically from watching the orbiting systems in a timelapse video, but it helps others appreciate what we’re studying,” Wang said. “It can be difficult to explain the nuances of science with words. But showing science in action helps others understand its importance.”

Elizabeth Howell is the co-author of “Why Am I Taller (opens in new tab)?” (ECW Press, 2022; with Canadian astronaut Dave Williams), a book about space medicine. Follow her on Twitter @howellspace (opens in new tab). Follow us on Twitter @Spacedotcom (opens in new tab) or Facebook (opens in new tab).



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Scientists Reveal The Most Distant Galaxy We’ve Ever Found : ScienceAlert

A galaxy whose light has traveled nearly 13.5 billion years to reach us has just been confirmed as the earliest galaxy found to date.

By studying the oxygen content of the galaxy with the Atacama Large Millimeter/submillimeter Array (ALMA), astronomers have precisely dated it to just 367 million years after the Big Bang, a time when the first lights in the Universe were still switching on and starting to propagate freely through space.

The result confirms observations made by JWST, and offers new information about the early Universe that tells us about the origins of the elements.

“The first images of the James Webb Space Telescope revealed so many early galaxies that we felt we had to test its results using the best observatory on Earth,” says astronomer Tom Bakx of Nagoya University in Japan.

“It was a very exciting time to be an observational astronomer, and we could track the status of the observations that will test the JWST results in real time.”

The galaxy, named GHZ2/GLASS-z12, was first spotted by JWST in July of last year, not long after the telescope opened its segmented golden eye on the infrared light of the Universe.

A paper in November detailed the discovery, dating the galaxy back to approximately 350 million years after the Big Bang, which took place around 13.8 billion years ago.

That’s actually pretty amazing, but any astronomical discovery is significantly more robust if it can be confirmed using an independent instrument.

So a team led by Bakx and astronomer Jorge Zavala of the National Astronomical Observatory of Japan turned to radio telescope ALMA to see what more they could learn about the fledgling galaxy.

They turned ALMA to the direction of GHZ2/GLASS-z12 and started looking for an emission signature on the radio spectrum associated with oxygen.

Since oxygen takes a relatively short time to form, it’s commonly used to learn more about galaxies in the early Universe. And when light enters oxygen, it is re-emitted at a specific wavelength range, resulting in a brighter line on that part of the spectrum.

The image of GHZ2/GLASS-z12 with the associated ALMA spectrum. (NASA/ESA/CSA/T. Treu, UCLA/NAOJ/T. Bakx, Nagoya U)

Each of the 66 12-meter radio antennae that make up ALMA were put to work, ultimately detecting an oxygen emission line close to the position of GHZ2/GLASS-z12. Follow-up analyses and statistical tests determined that the signal was real, and related to the galaxy.

“We were initially concerned about the slight variation in position between the detected oxygen emission line and the galaxy seen by Webb,” Bakx explains.

“But we performed detailed tests on the observations to confirm that this really is a robust detection, and it is very difficult to explain through any other interpretation.”

The very slight distance between the galaxy and the oxygen emission could suggest that violent explosions or interactions stripped the galaxy of a great deal of its gas, blowing it out into intergalactic space.

The team dated their observations to a more precise 367 million years after the Big Bang. And, based on the brightness of the emission line, they were able to infer that the galaxy had relatively quickly formed high abundances of elements heavier than hydrogen and helium.

This is very interesting. The early Universe, before stars came along, was mostly made up of hydrogen with a smaller amount of helium. Then stars formed; in their hot, dense cores, they started smashing atoms together, creating heavier elements.

But these elements were locked inside the stars; it wasn’t until the stars had died, exploding in spectacular supernovae, that heavier elements were able to spread through interstellar space.

This presence of oxygen so early in the Universe gives us some clues about the timing and evolution of these first stars, which we have yet to see directly.

“These deep ALMA observations provide robust evidence of the existence of galaxies within the first few hundred million years after the Big Bang, and confirms the surprising results from the Webb observations,” Zavala says.

“The work of JWST has only just begun, but we are already adjusting our models of how galaxies form in the early Universe to match these observations. The combined power of Webb and the radio telescope array ALMA give us the confidence to push our cosmic horizons ever closer to the dawn of the Universe.”

The research has been published in the Monthly Notices of the Royal Astronomical Society.

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How Our View of the Distant Universe Could Slowly Fade Away

Toni Santana-Ros is an asteroid hunter. 

At nightfall, after the day’s final scenes of flamingo sunbeams fade to black, he peers up at the sky to watch space rocks swimming along our solar system’s gravitational tides. Sometimes, he sees shards casually cruising next to Earth, greeting telescopes with a gentle “hey,” never to be observed again. But occasionally, he catches one on a crash course with our delicate blue orb. 

Last year, Santana-Ros, a planetary scientist at the University of Alicante in Spain, sprang into action when astronomers realized an asteroid named 2022 WJ1 was headed straight for the border of Canada and the US. With barely four hours on the clock, he mustered his team to help pinpoint how menacing this asteroid would be. What towns would it threaten? Would it be like the dinosaur-killing Chicxulub or merely make a “plop” sound before sinking into a sturdy body of water? 

“Luckily,” he concluded, “the object was small and just produced a spectacular fireball.”

But what if such a time-sensitive asteroid warning had been sent out in November 2020, when Santana-Ros’ telescopes were shut down because of bushfires ravaging the region and covering lenses with inky layers of ash? Or in February of 2021, when bushfire debris made its way into some telescopes, forcing astronomers to dismount instruments and pull blobs of soot from them after the wind settled? 

“Climate change is already affecting astronomy and my work,” Santana-Ros said. 

Time and again, studies have shown that climate change is leading to an increase in wildfire occurrence and severity as the years go by. With our present greenhouse gas emission trajectory, some models even predict that the risk of very large wildfires in the US will increase sixfold by the middle of the century.

During his telescope shutdowns, Santana-Ros said, he’d received the interruption news while comfortably at home. “There was no big drama.” 

But those blazes prevented his team from using telescopes for a few weeks. 

“The bottom line here is that this time we were lucky and we missed just some regular observations,” he said. “Next time, we might be facing a real threat.”

An astronomical problem

Over the last few decades, climate change has altered our relationship with Earth. 

Global industries still burn coal to make cheap power, diffuse dangerous fossil fuel waste into the atmosphere, force our planet to heat up, and ultimately fuel devastation like the wildfires responsible for the interruption of Santana-Ros’ research. Meanwhile, scientists are trying to learn how to shelter endangered animals left without homes because deforestation has ruined wildlife habitats, as well as how to deal with cyclones tearing apart coastal villages. 

It’s almost like we aren’t part of our planet anymore, no longer blended into its environment like the oak trees and butterflies with which we share cosmic material. It’s as if we’re fighting to regain our rightful place as Earthlings. 

But amid such chaos, astronomers are starting to think about another heartbreaking angle to the crisis. Not only has our relationship with Earth grown fraught, but climate change could stain our relationship with the rest of the universe, too.

With global warming ramping up, ground-based telescopes will find it harder to alert us about asteroids, show us glistening galaxies and deliver views of mysterious exoplanets populating the rest of eternity – wonders that unite us underneath our layers of disagreement, as evidenced by the ubiquitous love we witnessed for NASA’s James Webb Space Telescope two Christmases ago.

Cyclones, floods, fires and droughts are becoming the norm in astronomy hubs like Hawaii and New Mexico. Sites like the Les Makes Observatory were hit by severe storms at the same time Santana-Ros had to contend with wildfires near his tools in Australia.

And it’s not just full-on disasters that we have to worry about. It’s also the smaller things: changes in temperature, humidity, steady weather – elements telescopes usually rely on to operate in tip-top shape. 

A recent paper, published last October in the journal Astronomy & Astrophysics, focuses on those crucial details while outlining an ominous future for astronomy. Its authors explore the specifics of what climate change could do to eight major optical telescopes scattered across the globe. Not just today, but by 2050. 

“Our results show that climate change will negatively impact the quality of astronomical observations,” they say, “and is likely to increase time lost due to bad site conditions.” 

Time lost, as in nights of stargazing compromised.

“My first reaction to the paper was ‘yikes’ – yet another depressing outcome of climate change,” said Clara Sousa-Silva, a quantum astrophysicist at Bard College. “I had not previously considered how it would affect future observations, but of course it makes perfect sense. Obviously, in the long list of tragedies that will come from a warming Earth, this is very far down the list of concerns, but it is nonetheless concerning.”

“Anecdotally,” she continued, though carefully noting the probability of confirmation bias, “observational colleagues have complained that there seem to be more and more nights lost to weather in recent years.”

Starlight’s barrier

Along with her advisors, Caroline Haslebacher, a doctoral student at the University of Bern in Switzerland and lead author of the recent study, realized no one had really looked into how climate change will affect astronomical observations, though Santana-Ros’ experience is evidence that damage is already being done. 

They quickly moved to fill the gap.

The team modeled what would happen to those eight telescope subjects as the globe heats up, eventually suggesting we’ll see an increase in what’s known as specific humidity and precipitable water vapor in the coming years. 

Essentially, this means the amount of water in the air will get higher because of climate change – a problematic situation because airborne water tends to absorb the same light telescopes are trying their hardest to catch.

“A lot of the most exciting astronomical observations are done at the very edge of instrumental capabilities,” Sousa-Silva said. “Any additional noise directly restricts the discoveries we can make.”

For instance, the study authors expect that on the extinct volcano of Mauna Kea in Hawaii, where many observatories lie, there’ll be an increase of 0.3 mm of water by the year 2050. Granted, such a miniature impact seemed quite soft when compared with other sites. “But still not zero,” John O’Meara, chief scientist at Mauna Kea’s Keck Observatory, said.

With this paper in mind, he’s particularly worried about increases in water vapor affecting not visible light but rather
infrared observations at the Hawaiian location. Such haze is very likely to pose problems for this category of light, which emanates from the distant universe. 

Because wavelengths stretch out as they move farther and farther away from our planet, they get redder and redder and redder over time until they turn into elusive infrared patterns – invisible to human eyes but analyzable with advanced machines. This is precisely the form of light signals that scientists love, the kind that could reveal to us what the universe was like when it flicked on for the first time. 

It’d be a shame for such a rich level of cosmic history to slowly fade away from our vantage point on Earth.

“Climate change effects were not historically included in site selection studies, and now we have a new variable to consider,” O’Meara said. 

Because of this, Haslebacher believes that going forward, we should analyze trends when building telescopes. 

“It is urgent for telescopes under construction,” she said, “since these canstill adapt their design for changing climate conditions, and telescopes in planning so that a minimally impacted site can be selected.” 

But even that effort may not be enough to offset the barriers this crisis will create. More water vapor simply reduces light transmission in some spectral bands. Or as Sousa-Silva puts it, “we will literally have less to look at.”

The lonely space machines

Since the Industrial Revolution, it’s almost like humanity has existed in a dissonant thought loop regarding climate change – one that has, expectedly, turned into a political debate. 

Last year, COP27 marked the 27th year that world leaders have met to discuss how to save Earth – and another year world scientists confirmed we’re pretty much failing.

“I have to emphasize at this point that we investigated the shared socioeconomic pathway scenario with the highest greenhouse gas emissions out of five possible pathways,” Haslebacher said of her paper. “Unfortunately, we are following this scenario today.”

In other words, the worst-case scenario is the scenario we’re currently living through.

Yet some policymakers and energy giants justify this kind of human rebellion against the natural world – and even encourage it – because fossil fuels give us inexpensive power. And without affordable energy, they worry, we’d need to dip into other financial budgets as penance for keeping our iPhone batteries a healthy green hue. 

But to sustain fossil fuel-driven power, we pay in other ways. 

“We know what we as a nation and a world need to do to avoid the worst effects, and yet we are largely unwilling to act at the scale that the situation demands,” O’Meara said. “I worry that it will take the first truly major catastrophe or conflict to wake us up, and by then, it may well be too late to avoid the next one.”

Further, the same pollution that’s heating up the globe is also bound to do things like thicken the atmosphere. 

“An optically thick atmosphere is one in which radiation travels less,” said Luigi Vidale, a professor of Climate System Science and Climate Hazards at the University of Reading and co-author of the study. “Although [our] models considered the highest future emission scenario, we may still have underestimated the impact of airborne pollution on local visibility.”

O’Meara explained it simply: “More clouds equals less visibility for faint objects equals less science.”

To name a few more consequences: Global warming could degrade the overall atmospheric qualities of a telescope’s site, forming the right conditions for turbulence during observations. It could prevent scientists from cooling their machines down to the right checkpoints before embarking on a project – and, truth be told, concerns are deep enough to impact not just astronomy, but all science.

“It will change our whole world,” Santana-Ros said. “It is quite likely that climate change can be the source of future financial crises, which in turn will have a negative effect on research funding.”

Funding for science projects is already a huge conundrum – most of the time, only those who win grants, awards, scholarships and other such prizes are able to pursue their work for years on end. 

So to add on to that, if we wait to act on climate change, and then something utterly drastic happens, we’d need to redirect resources from astronomy, medicine, chemistry, biology, botany and so on, into climate science. 

“There is still time for science and industry to lead us to a better climate future,” O’Meara said. “All we need is the resolve and the investment.” It’s becoming clearer that without immediate action, the promise of ground-based telescopes might one day become a thing of the past – dying out alongside all the other beautiful things humans are tasked with protecting from the catastrophe they created. 

At that point, the only link we’d have left to the stars would be our space-borne machines: the Webb Space Telescope, the Hubble – chunks of metal floating above a ravaged Earth, witnesses to humanity’s exit from the natural world.

“Plans for colonization of other planets are still sci-fi, and will still be for several decades,” Santana-Ros said. “Our only option to survive is to mitigate climate change.”

All images: Robert Rodriguez/CNET.

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Astronomers Capture Radio Signal From Distant Galaxy

One of the dishes of the Giant Metrewave Radio Telescope (GMRT) near Pune, Maharashtra, India. Credit: National Centre for Radio Astrophysics

Probing galaxies at much greater distances from Earth may now be within reach.

How do stars form in distant galaxies? Astronomers have long been trying to answer this question by detecting radio signals emitted by nearby galaxies. However, these signals become weaker the further away a galaxy is from Earth, making it difficult for current radio telescopes to pick up.

Now researchers from Montreal and India have captured a radio signal from the most distant galaxy so far at a specific wavelength known as the 21 cm line, allowing astronomers to peer into the secrets of the early universe. With the help of the Giant Metrewave Radio Telescope in India, this is the first time this type of radio signal has been detected at such a large distance.

Illustration showing detection of the signal from a distant galaxy. Credit: Swadha Pardesi

“A galaxy emits different kinds of radio signals. Until now, it’s only been possible to capture this particular signal from a galaxy nearby, limiting our knowledge to those galaxies closer to Earth,” says Arnab Chakraborty, a Post-Doctoral Researcher at McGill University under the supervision of Professor Matt Dobbs.

“But thanks to the help of a naturally occurring phenomenon called gravitational lensing, we can capture a faint signal from a record-breaking distance. This will help us understand the composition of galaxies at much greater distances from Earth,” he adds.

A look back in time to the early universe

For the first time, the researchers were able to detect the signal from a distant star-forming galaxy known as SDSSJ0826+5630 and measure its gas composition. The researchers observed the atomic mass of the gas content of this particular galaxy is almost twice the mass of the stars visible to us.

Image of the radio signal from the galaxy. Credit: Chakraborty & Roy/NCRA-TIFR/GMRT

The signal detected by the team was emitted from this galaxy when the universe was only 4.9 billion years old, enabling the researchers to glimpse into the secrets of the early universe. “It’s the equivalent to a look-back in time of 8.8 billion years,” says Chakraborty, who studies cosmology at McGill’s Department of Physics.

Picking up the signal from a distant galaxy

“Gravitational lensing magnifies the signal coming from a distant object to help us peer into the early universe. In this specific case, the signal is bent by the presence of another massive body, another galaxy, between the target and the observer. This effectively results in the magnification of the signal by a factor of 30, allowing the telescope to pick it up,” says co-author Nirupam Roy, an Associate Professor in the Department of Physics at the Indian Institute of Science.

According to the researchers, these results demonstrate the feasibility of observing faraway galaxies in similar situations with gravitational lensing. It also opens exciting new opportunities for probing the cosmic evolution of stars and galaxies with existing low-frequency radio telescopes.

Reference: “Detection of H I 21 cm emission from a strongly lensed galaxy at z ∼ 1.3” by Arnab Chakraborty and Nirupam Roy, 23 December 2022, Monthly Notices of the Royal Astronomical Society.
DOI: 10.1093/mnras/stac3696

The Giant Metrewave Radio Telescope was built and is operated by NCRA-TIFR. The research was funded by McGill University and the Indian Institute of Science.



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Record-Breaking Signal From Distant Galaxy Is Furthest of Its Kind Ever Detected : ScienceAlert

Hydrogen is a key building block of the cosmos. Whether stripped down to its charged core, or piled into a molecule, the nature of its presence can tell you a lot about the Universe’s features on the largest of scales.

For that reason astronomers are very interested in detecting signals from this element, wherever it can be found.

Now the light signature of uncharged, atomic hydrogen has been measured further from Earth than ever before, by some margin. The Giant Metrewave Radio Telescope (GMRT) in India has picked up a signal with a lookback time – the time between the light being emitted and being detected – of a huge 8.8 billion years.

Image of the radio signal from the galaxy. (Chakraborty & Roy/NCRA-TIFR/GMRT)

That gives us an exciting glimpse of some of the earliest moments in the Universe, which is currently estimated to be in the region of 13.8 billion years old.

“A galaxy emits different kinds of radio signals,” says cosmologist Arnab Chakraborty, from McGill University in Canada. “Until now, it’s only been possible to capture this particular signal from a galaxy nearby, limiting our knowledge to those galaxies closer to Earth.”

In this case, the radio signal emitted by atomic hydrogen is a light wave with a length of 21 centimeters. Long waves aren’t very energetic, nor is the light intense, making it difficult to detect at a distance; the previous record lookback time stood at a mere 4.4 billion years.

Due to the vast distance it traveled before being intercepted by the GMRT, the 21 centimeter emission line had been stretched by expanding space to 48 centimeters, a phenomenon described as the redshifting of light.

The team used gravitational lensing to detect the signal, which originates from a distant star-forming galaxy called SDSSJ0826+5630. Gravitational lensing is where light is magnified as it follows the curving space surrounding a massive object that sits between our telescopes and the original source, effectively acting as a huge lens.

Illustration showing how gravitational lensing works. (Swadha Pardesi)

“In this specific case, the signal is bent by the presence of another massive body, another galaxy, between the target and the observer,” says astrophysicist Nirupam Roy, from the Indian Institute of Science.

“This effectively results in the magnification of the signal by a factor of 30, allowing the telescope to pick it up.”

The results of this study will give astronomers hope for being able to make other similar observations in the near future: the distances and lookback times that were previously off limits are very much now within reason. If the stars align, that is.

Atomic hydrogen is formed as hot, ionized gas from the surroundings of a galaxy starts to fall onto the galaxy, cooling down along the way. Eventually, it turns into molecular hydrogen, and then into stars.

Being able to look back so far in time can teach us more about how our own galaxy formed in the beginning, as well as leading astronomers towards a better understanding of how the Universe behaved when it was just getting started.

These latest findings will “open up exciting new possibilities for probing the cosmic evolution of neutral gas with existing and upcoming low-frequency radio telescopes in the near future,” write the researchers in their published paper.

The research has been published in the Monthly Notices of the Royal Astronomical Society.

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Astronomers from Canada, IISc detect signal from distant galaxy

Astronomers from McGill University in Canada and the Indian Institute of Science (IISc) have used data from the Giant Metrewave Radio Telescope (GMRT), in Pune, to detect a radio signal originating from atomic hydrogen in an extremely distant galaxy. 

The IISc said on Monday that the astronomical distance over which the signal has been picked up is “the largest so far by a large margin”.

The findings have been published in the Monthly Notices of the Royal Astronomical Society.

While detection of radio waves with 21 cm wavelength, emitted by atomic hydrogen, is possible through low-frequency radio telescopes like GMRT, the “extremely weak” nature of the radio signal makes it nearly impossible to detect emissions from a distant galaxy.

The most distant galaxy detected through the 21-cm emission, so far, was at redshift z=0.376.

The value denotes the look-back time, or the time elapsed between the detection and the original emission; in this case, 4.1 billion years.

Arnab Chakraborty, postdoctoral researcher at the Department of Physics and Trottier Space Institute of McGill University, and Nirupam Roy, associate professor, department of Physics, IISc, used data from GMRT to detect a radio signal from atomic hydrogen in a distant galaxy at redshift z=1.29.

IISc said in an official statement that the signal was emitted when the universe was only 4.9 billion years old, which translated to a look-back time of 8.8 billion
years.

Atomic hydrogen – formed when hot ionised gas from the surrounding medium of a galaxy falls onto the galaxy, and cools – and its subsequent change into molecular hydrogen leads to the formation of stars. Studying the evolution of neutral gas, therefore, becomes critical in understanding the evolution of galaxies.

The GMRT was built and is operated by National Centre for Radio Astrophysics – Tata Institute of Fundamental Research, Pune. The research was funded by McGill and IISc.

The astronomers traced the detection to a phenomenon called gravitational lensing, which causes the light emitted by the source to bend due to the presence of another massive body, “such as an early type elliptical galaxy,” between the observer and the target galaxy, resulting in a signal that is magnified. “In this specific case, the magnification of the signal was about a factor of 30, allowing us to see through the high redshift universe,” Roy said.

The detection significantly increases possibilities in observing atomic gas from galaxies at cosmological distances and studying the cosmic evolution of neutral gas with low-frequency radio telescopes.

Yashwant Gupta, Centre Director at NCRA, called detection of neutral hydrogen in emission from the distant universe one of GMRT’s “key science goals”.

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Astronomers find the most distant stars in our galaxy halfway to Andromeda

This illustration shows the Milky Way galaxy’s inner and outer halos. A halo is a spherical cloud of stars surrounding a galaxy. Credit: NASA, ESA, and A. Feild (STScI)

Astronomers have discovered more than 200 distant variable stars known as RR Lyrae stars in the Milky Way’s stellar halo. The most distant of these stars is more than a million light years from Earth, almost half the distance to our neighboring galaxy, Andromeda, which is about 2.5 million light years away.

The characteristic pulsations and brightness of RR Lyrae stars make them excellent “standard candles” for measuring galactic distances. These new observations have allowed the researchers to trace the outer limits of the Milky Way’s halo.

“This study is redefining what constitutes the outer limits of our galaxy,” said Raja GuhaThakurta, professor and chair of astronomy and astrophysics at UC Santa Cruz. “Our galaxy and Andromeda are both so big, there’s hardly any space between the two galaxies.”

GuhaThakurta explained that the stellar halo component of our galaxy is much bigger than the disk, which is about 100,000 light years across. Our solar system resides in one of the spiral arms of the disk. In the middle of the disk is a central bulge, and surrounding it is the halo, which contains the oldest stars in the galaxy and extends for hundreds of thousands of light years in every direction.

“The halo is the hardest part to study because the outer limits are so far away,” GuhaThakurta said. “The stars are very sparse compared to the high stellar densities of the disk and the bulge, but the halo is dominated by dark matter and actually contains most of the mass of the galaxy.”

Yuting Feng, a doctoral student working with GuhaThakurta at UCSC, led the new study and is presenting their findings in two talks at the American Astronomical Society meeting in Seattle on January 9 and 11.

According to Feng, previous modeling studies had calculated that the stellar halo should extend out to around 300 kiloparsecs or 1 million light years from the galactic center. (Astronomers measure galactic distances in kiloparsecs; one kiloparsec is equal to 3,260 light years.) The 208 RR Lyrae stars detected by Feng and his colleagues ranged in distance from about 20 to 320 kiloparsecs.

“We were able to use these variable stars as reliable tracers to pin down the distances,” Feng said. “Our observations confirm the theoretical estimates of the size of the halo, so that’s an important result.”

The findings are based on data from the Next Generation Virgo Cluster Survey (NGVS), a program using the Canada-France-Hawaii Telescope (CFHT) to study a cluster of galaxies well beyond the Milky Way. The survey was not designed to detect RR Lyrae stars, so the researchers had to dig them out of the dataset. The Virgo Cluster is a large cluster of galaxies that includes the giant elliptical galaxy M87.

“To get a deep exposure of M87 and the galaxies around it, the telescope also captured the foreground stars in the same field, so the data we used are sort of a by-product of that survey,” Feng explained.

According to GuhaThakurta, the excellent quality of the NGVS data enabled the team to obtain the most reliable and precise characterization of RR Lyrae at these distances. RR Lyrae are old stars with very specific physical properties that cause them to expand and contract in a regularly repeating cycle.

“The way their brightness varies looks like an EKG—they’re like the heartbeats of the galaxy—so the brightness goes up quickly and comes down slowly, and the cycle repeats perfectly with this very characteristic shape,” GuhaThakurta said. “In addition, if you measure their average brightness, it is the same from star to star. This combination is fantastic for studying the structure of the galaxy.”

The sky is full of stars, some brighter than others, but a star may look bright because it is very luminous or because it is very close, and it can be hard to tell the difference. Astronomers can identify an RR Lyrae star from its characteristic pulsations, then use its observed brightness to calculate how far away it is. The procedures are not simple, however. More distant objects, such as quasars, can masquerade as RR Lyrae stars.

“Only astronomers know how painful it is to get reliable tracers of these distances,” Feng said. “This robust sample of distant RR Lyrae stars gives us a very powerful tool for studying the halo and testing our current models of the size and mass of our galaxy.”

This study is based on observations obtained with MegaPrime/MegaCam, a joint project of CFHT and CEA/IRFU, at the Canada-France-Hawaii Telescope (CFHT), which is operated by the National Research Council (NRC) of Canada, the Institut National des Sciences de l’Univers of the Centre National de la Recherche Scientifique (CNRS) of France, and the University of Hawaii.

More information:
Conference: American Astronomical Society meeting in Seattle

Provided by
University of California – Santa Cruz

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Distant Memories of Fear Lurk in Your Brain, And We May Have Found Their Hiding Place : ScienceAlert

Recollections of traumatic events can continue to resurface in the brain long after the moment has passed, leading to conditions such as post-traumatic stress disorder (PTSD).

While it’s clear the area of the brain called the hippocampus plays a central role in the memory’s formation, the physical nature of fear’s long-term storage as a ‘remote memory’ has remained elusive.

In a new study on mice, scientists from the University of California, Riverside, in the US have outlined some of the key mechanisms through which remote fear memories are consolidated, and identified the physical embodiment of distant fears in a prominent part of our brains.

By understanding more about how these traumatic flashbacks get embedded, we might be able to improve therapies and treatments for those suffering them.

The researchers used mice engineered with nerve cells that could be identified easily during fear responses, along with a mix of viruses that cut important nervous pathways thought to be involved with memory consolidation, or helped identify key connections between neurons.

An electric shock served as a memory fear event for the transgenic mice. When the test subjects returned to the location of the shock a month later, they froze, indicating that remote fear memories stored somewhere in the brain were indeed being recalled.

Closely looking at various brain samples revealed a steady reinforcing of connections within a small group of memory neurons in what’s known as the prefrontal cortex (PFC) – an area responsible for decision making and cognitive behavior.

Fear memory neurons in red among other prefrontal cortex neurons in blue. (Cho Lab/UCR)

Further tests showed that when these particular memory neurons were severed, the mice were unable to recall remote fears, while still remembering more recent trauma. In other words, the PFC memory neurons form the physical structures, or engrams, for remote fear memories.

The mice were then exposed to the same locations but this time without the aversive stimulus. That was enough to reduce the fear response and change the circuitry of these neurons relevant to the traumatic event, the researchers demonstrated.

“It is the prefrontal memory circuits that are progressively strengthened after traumatic events and this strengthening plays a critical role in how fear memories mature to stabilized forms in the cerebral cortex for permanent storage,” says neuroscientist Jun-Hyeong Cho.

“Using a similar mechanism, other non-fear remote memories could also be permanently stored in the PFC.”

There’s more work to do to look at these mechanisms more closely. The researchers plan to see whether a selective weakening of the PFC memory circuits will suppress the recall of remote fear memories, which could then inform treatments in people.

“Interestingly, the extinction of remote fear memory weakened the prefrontal memory circuits that were previously strengthened to store the remote fear memory,” says Cho.

“Moreover, other manipulations that blocked the strengthening of the PFC memory circuits also prevented the recall of remote fear memory.”

Around 6 percent of the US population is expected to experience some form of PTSD in their lives, and knowing how these memories get stored and then brought back is going to be crucial in figuring out how to treat individuals with fear and trauma-based disorders.

The research has been published in Nature Neuroscience.

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It should take another 300 years for NASA’s Voyager 1 probe to reach the most distant region of our solar system. Until then, it’s cruising through the void between the stars.

An artist’s concept which shows NASA’s Voyager spacecraft against a backdrop of stars.NASA/JPL-Caltech

  • Voyagers 1 and 2 are exploring the mysterious region between stars called interstellar space.

  • NASA launched the twin probes in 1977 for a five-year mission to trek across the solar system.

  • It should take Voyager 1 40,000 years to reach another star, according to the space agency.

Some 14.8 billion miles from Earth, the Voyager 1 probe is cruising through the blackness of the interstellar medium — the unexplored space between stars. It’s the furthest human-made object from our planet.

Voyager 1 and Voyager 2 launched in 1977 within 16 days of one another with a design lifetime of five years to study Jupiter, Saturn, Uranus, Neptune, and their respective moons up close.

Now 45 years into their mission, they’ve each made history by boldly venturing beyond the boundary of our sun’s influence, known as the heliopause.

Both plucky spacecraft continue to send data back from beyond the solar system — and their cosmic journeys are far from over.

A diagram showing both of NASA’s Voyager probes in interstellar space as of November 2018.NASA/JPL-Caltech

In 300 years, Voyager 1 could see the Oort Cloud, and in 296,000 years, Voyager 2 could pass by Sirius

As part of an ongoing power-management effort that has ramped up in recent years, engineers have been powering down non-technical systems on board the Voyager probes, like their science-instruments heaters, hoping to keep them going through 2030.

After that, the probes will likely lose their ability to communicate with Earth.

Still, even after NASA shuts down their instruments and calls the Voyager mission to an end, the twin probes will continue to drift out in interstellar space.

NASA said that about 300 years from now, Voyager 1 should enter the Oort Cloud, a hypothetical spherical band full of billions of frozen comets. It should take another 30,000 years to reach the end of it.

An illustration of the Kuiper Belt and Oort Cloud in relation to our solar system.NASA

The spacecraft are taking different paths as they head out into deep space. Voyager 2 is only about 12.3 billion miles away from Earth today.

It should take the Voyager 1 probe approximately 40,000 years to reach AC+79 3888, a star in the constellation Camelopardalis, according to NASA.

The agency added that in some 296,000 years, Voyager 2 should drift by Sirius, the brightest star in the sky.

“The Voyagers are destined — perhaps eternally — to wander the Milky Way,” NASA said.

Hubble Space Telescope image of Sirius, the brightest star in our nighttime sky.NASA, ESA, H. Bond (STScI), and M. Barstow (University of Leicester)

‘It’s really remarkable that both spacecraft are still operating’

NASA designed the twin spacecraft to study the outer solar system. After completing their primary mission, the Voyagers kept chugging along, taking a grand tour of our solar system and capturing breathtaking cosmic views.

On February 14, 1990, the Voyager 1 spacecraft captured the “Pale Blue Dot” image from almost 4 billion miles away. It’s an iconic image of Earth within a scattered ray of sunlight, and it’s the farthest view of Earth any spacecraft has captured.

The iconic “Pale Blue Dot” image taken by Voyager 1 on February 14, 1990.NASA/JPL-Caltech

For the last decade, Voyager 1 has been exploring interstellar space, which is full of gas, dust, and charged energetic particles. Voyager 2 reached interstellar space in 2018, six years after its twin.

Their observations of the interstellar gas they’re moving through has revolutionized astronomers’ understanding of this unexplored space beyond our own cosmic backyard.

“It’s really remarkable that both spacecraft are still operating and operating well — little glitches, but operating extremely well and still sending back this valuable data,” Suzanne Dodd, the project manager for the Voyager mission at NASA’s Jet Propulsion Laboratory, previously told Insider, adding, “They’re still talking to us.”

Read the original article on Business Insider

Read original article here

It should take another 300 years for NASA’s Voyager 1 probe to reach the most distant region of our solar system. Until then, it’s cruising through the void between the stars.

An artist’s concept which shows NASA’s Voyager spacecraft against a backdrop of stars.NASA/JPL-Caltech

  • Voyagers 1 and 2 are exploring the mysterious region between stars called interstellar space.

  • NASA launched the twin probes in 1977 for a five-year mission to trek across the solar system.

  • It should take Voyager 1 40,000 years to reach another star, according to the space agency.

Some 14.8 billion miles from Earth, the Voyager 1 probe is cruising through the blackness of the interstellar medium — the unexplored space between stars. It’s the furthest human-made object from our planet.

Voyager 1 and Voyager 2 launched in 1977 within 16 days of one another with a design lifetime of five years to study Jupiter, Saturn, Uranus, Neptune, and their respective moons up close.

Now 45 years into their mission, they’ve each made history by boldly venturing beyond the boundary of our sun’s influence, known as the heliopause.

Both plucky spacecraft continue to send data back from beyond the solar system — and their cosmic journeys are far from over.

A diagram showing both of NASA’s Voyager probes in interstellar space as of November 2018.NASA/JPL-Caltech

In 300 years, Voyager 1 could see the Oort Cloud, and in 296,000 years, Voyager 2 could pass by Sirius

As part of an ongoing power-management effort that has ramped up in recent years, engineers have been powering down non-technical systems on board the Voyager probes, like their science-instruments heaters, hoping to keep them going through 2030.

After that, the probes will likely lose their ability to communicate with Earth.

Still, even after NASA shuts down their instruments and calls the Voyager mission to an end, the twin probes will continue to drift out in interstellar space.

NASA said that about 300 years from now, Voyager 1 should enter the Oort Cloud, a hypothetical spherical band full of billions of frozen comets. It should take another 30,000 years to reach the end of it.

An illustration of the Kuiper Belt and Oort Cloud in relation to our solar system.NASA

The spacecraft are taking different paths as they head out into deep space. Voyager 2 is only about 12.3 billion miles away from Earth today.

It should take the Voyager 1 probe approximately 40,000 years to reach AC+79 3888, a star in the constellation Camelopardalis, according to NASA.

The agency added that in some 296,000 years, Voyager 2 should drift by Sirius, the brightest star in the sky.

“The Voyagers are destined — perhaps eternally — to wander the Milky Way,” NASA said.

Hubble Space Telescope image of Sirius, the brightest star in our nighttime sky.NASA, ESA, H. Bond (STScI), and M. Barstow (University of Leicester)

‘It’s really remarkable that both spacecraft are still operating’

NASA designed the twin spacecraft to study the outer solar system. After completing their primary mission, the Voyagers kept chugging along, taking a grand tour of our solar system and capturing breathtaking cosmic views.

On February 14, 1990, the Voyager 1 spacecraft captured the “Pale Blue Dot” image from almost 4 billion miles away. It’s an iconic image of Earth within a scattered ray of sunlight, and it’s the farthest view of Earth any spacecraft has captured.

The iconic “Pale Blue Dot” image taken by Voyager 1 on February 14, 1990.NASA/JPL-Caltech

For the last decade, Voyager 1 has been exploring interstellar space, which is full of gas, dust, and charged energetic particles. Voyager 2 reached interstellar space in 2018, six years after its twin.

Their observations of the interstellar gas they’re moving through has revolutionized astronomers’ understanding of this unexplored space beyond our own cosmic backyard.

“It’s really remarkable that both spacecraft are still operating and operating well — little glitches, but operating extremely well and still sending back this valuable data,” Suzanne Dodd, the project manager for the Voyager mission at NASA’s Jet Propulsion Laboratory, previously told Insider, adding, “They’re still talking to us.”

Read the original article on Business Insider

Read original article here