Science
'We just discovered the impossible': How giant baby galaxies are shaking up our understanding of the early universe – Phys.org


“Look at this,” says Erica’s message. She is poring over the very first images from the brand new James Webb Space Telescope (JWST).
It is July 2022, barely a week after those first images from the revolutionary super telescope were released. Twenty-five years in the making, a hundred to a thousand times more powerful than any previous telescope, one of the biggest and most ambitious scientific experiments in human history: it is hard to not speak in superlatives, and it is all true.
The telescope took decades to build, because it had to be made foldable to fit on top of a rocket and be sent into the coldness of space, 1.5 million kms from Earth. Here, far from the heat glow of the Earth, JWST can detect the faintest infrared light from the distant universe.
Little did I know that among the pictures is a small red dot that will shake up our understanding of how the first galaxies formed after the Big Bang. After months of analysis, my colleagues and I just published our results in Nature.
Hunting new kinds of galaxies
Erica and I are on the hunt to discover new types of galaxies. Galaxies that the venerable Hubble Space Telescope had missed, even after decades of surveying the sky.
She and I go back 15 years. We met when she was a first-year student at a Californian liberal arts college and I was a freshly minted Ph.D. straight out of university, just starting my first gig as a researcher in Los Angeles. JWST was only a distant rumor.
Somehow, many years later, our paths crossed again, and now Assistant Professor Erica Nelson of the University of Colorado and I are finding ourselves at the tip of the spear attacking the first data of a very real JWST.
“UFOs,” she calls the new galaxies, and I can read a giant grin between the lines: “ultra-red flattened objects”, because they all look like flying saucers. In the color images they appear very red because all the light is coming out in the infrared, while the galaxies are invisible at wavelengths humans can see.
Infrared is JWST’s superpower, allowing it to spy the most distant galaxies. Ultraviolet and visible light from the first stars and galaxies that formed after the Big Bang is stretched out by the expansion of the universe as it travels towards us, so by the time the light reaches us we see it as infrared light.


Impossibly early, impossibly massive galaxies
All of Erica’s galaxies look like saucers, except one. I stare at the little red dot on the screen. That is no UFO. And then it hits me: This is something very different. Much more important.
I run the analysis software on the little pinprick and it spits out two numbers: distance 13.1 billion light years, mass 100 billion stars, and I nearly spit out my coffee. We just discovered the impossible. Impossibly early, impossibly massive galaxies.
At this distance, the light took 13 billion years to reach us, so we are seeing the galaxies at a time when the universe was only 700 million years old, barely 5% of its current age of 13.8 billion years. If this is true, this galaxy has formed as many stars as our present-day Milky Way. In record time.
And where there is one, there are more. One day later I had found six.
Astronomy’s missing link?
Could we have discovered astronomy’s missing link? There has been a long-standing puzzle in galaxy formation. As we look out in space and back in time, we see the “corpses” of fully formed, mature galaxies appear seemingly out of nowhere around 1.5 billion years after the Big Bang.
These galaxies have stopped forming stars. Dead galaxies, we call them, and some astronomers are obsessed with them. The stellar ages of these dead galaxies suggest they must have formed much earlier in the universe, but Hubble has never been able to spot their earlier, living stages.
Early dead galaxies are truly bizarre creatures, packing as many stars as the Milky Way, but in a size 30 times smaller. Imagine an adult, weighing 100 kilos, but standing 6cm tall. Our little red dots are equally bizarre. They look like baby versions of the same galaxies, also weighing in at 100 kilos, with a height of 6cm.
Too many stars, too early


There is a problem, however. These little red dots have too many stars, too early. Stars form out of hydrogen gas, and fundamental cosmological (“Big Bang”) theory makes hard predictions on how much gas is available to form stars.
To produce these galaxies so quickly, you almost need all the gas in the universe to turn into stars at near 100% efficiency. And that is very hard, which is the scientific term for impossible. This discovery could transform our understanding of how the earliest galaxies in the universe formed.
The implication is that there is different channel, a fast track, that produces monster galaxies very quickly, very efficiently. A fast track for the top 1%.
In a way, each of these candidates can be considered a “black swan.” The confirmation of even one would rule out our current “all swans are white” model of galaxy formation, in which all early galaxies grow slowly and gradually.
Checking the fingerprints
The first step to solve this mystery is to confirm the distances with spectroscopy, where we put the light of each of these galaxies through a prism, and split it into its rainbow-like fingerprint. This will tell us the distance to 0.1% accuracy.
It will also tell us what is producing the light, whether it is stars or something else more exotic.
By chance, about a month ago, JWST already targeted one of the six candidate massive galaxies and it turned out to be a distant baby quasar. A quasar is a phenomenon that occurs when gas falls into a supermassive black hole at the center of a galaxy and starts to shine brightly.
This is really exciting on the one hand, because the origin of supermassive black holes in galaxies is not understood either, and finding baby quasars might just hold the key. On the other hand, quasars can outshine their entire host galaxy, so it is impossible to tell how many stars are there and whether the galaxy is really that massive.
Could that be the answer for all of them? Baby quasars everywhere? Probably not, but it will take another year to investigate the remaining galaxies and find out.
One black swan down, five to go.
More information:
Ivo Labbé et al, A population of red candidate massive galaxies ~600 Myr after the Big Bang, Nature (2023). DOI: 10.1038/s41586-023-05786-2
Provided by
The Conversation
This article is republished from The Conversation under a Creative Commons license. Read the original article.
Citation:
‘We just discovered the impossible’: How giant baby galaxies are shaking up our understanding of the early universe (2023, February 25)
retrieved 25 February 2023
from https://phys.org/news/2023-02-impossible-giant-baby-galaxies-early.html
This document is subject to copyright. Apart from any fair dealing for the purpose of private study or research, no
part may be reproduced without the written permission. The content is provided for information purposes only.
Science
James Webb spots swirling, gritty clouds on remote planet


|
Researchers observing with NASA’s James Webb Space Telescope have pinpointed silicate cloud features in a distant planet’s atmosphere. The atmosphere is constantly rising, mixing, and moving during its 22-hour day, bringing hotter material up and pushing colder material down.
The resulting brightness changes are so dramatic that it is the most variable planetary-mass object known to date. The team, led by Brittany Miles of the University of Arizona, also made extraordinarily clear detections of water, methane and carbon monoxide with Webb’s data, and found evidence of carbon dioxide. This is the largest number of molecules ever identified all at once on a planet outside our solar system.
Cataloged as VHS 1256 b, the planet is about 40 light-years away and orbits not one, but two stars over a 10,000-year period. “VHS 1256 b is about four times farther from its stars than Pluto is from our sun, which makes it a great target for Webb,” Miles said. “That means the planet’s light is not mixed with light from its stars.”
Higher up in its atmosphere, where the silicate clouds are churning, temperatures reach a scorching 1,500 degrees Fahrenheit (815 degrees Celsius).
Within those clouds, Webb detected both larger and smaller silicate dust grains, which are shown on a spectrum. “The finer silicate grains in its atmosphere may be more like tiny particles in smoke,” noted co-author Beth Biller of the University of Edinburgh in Scotland. “The larger grains might be more like very hot, very small sand particles.”
VHS 1256 b has low gravity compared to more massive brown dwarfs, which means that its silicate clouds can appear and remain higher in its atmosphere where Webb can detect them. Another reason its skies are so turbulent is the planet’s age. In astronomical terms, it’s quite young. Only 150 million years have passed since it formed—and it will continue to change and cool over billions of years.


In many ways, the team considers these findings to be the first “coins” pulled out of a spectrum that researchers view as a treasure chest of data. In many ways, they’ve only begun identifying its contents. “We’ve identified silicates, but better understanding which grain sizes and shapes match specific types of clouds is going to take a lot of additional work,” Miles said. “This is not the final word on this planet—it is the beginning of a large-scale modeling effort to fit Webb’s complex data.”
Although all of the features the team observed have been spotted on other planets elsewhere in the Milky Way by other telescopes, other research teams typically identified only one at a time. “No other telescope has identified so many features at once for a single target,” said co-author Andrew Skemer of the University of California, Santa Cruz. “We’re seeing a lot of molecules in a single spectrum from Webb that detail the planet’s dynamic cloud and weather systems.”
The team came to these conclusions by analyzing data known as spectra gathered by two instruments aboard Webb, the Near-Infrared Spectrograph (NIRSpec) and the Mid-Infrared Instrument (MIRI). Since the planet orbits at such a great distance from its stars, the researchers were able to observe it directly, rather than using the transit technique or a coronagraph to take this data.
There will be plenty more to learn about VHS 1256 b in the months and years to come as this team—and others—continue to sift through Webb’s high-resolution infrared data. “There’s a huge return on a very modest amount of telescope time,” Biller added. “With only a few hours of observations, we have what feels like unending potential for additional discoveries.”
What might become of this planet billions of years from now? Since it’s so far from its stars, it will become colder over time, and its skies may transition from cloudy to clear.
The researchers observed VHS 1256 b as part of Webb’s Early Release Science program, which is designed to help transform the astronomical community’s ability to characterize planets and the disks where they form.
The team’s paper, entitled “The JWST Early Release Science Program for Direct Observations of Exoplanetary Systems II: A 1 to 20 Micron Spectrum of the Planetary-Mass Companion VHS 1256-1257 b,” will be published in The Astrophysical Journal Letters.
The work is currently published on the arXiv preprint server.
More information:
Brittany E. Miles et al, The JWST Early Release Science Program for Direct Observations of Exoplanetary Systems II: A 1 to 20 Micron Spectrum of the Planetary-Mass Companion VHS 1256-1257 b, arXiv (2022). DOI: 10.48550/arxiv.2209.00620
Provided by
NASA
Citation:
James Webb spots swirling, gritty clouds on remote planet (2023, March 22)
retrieved 22 March 2023
from https://phys.org/news/2023-03-james-webb-swirling-gritty-clouds.html
This document is subject to copyright. Apart from any fair dealing for the purpose of private study or research, no
part may be reproduced without the written permission. The content is provided for information purposes only.





Science
Parade of planets: Jupiter, Mercury, Venus, Uranus and Mars alignment
|
Sky-gazers will be treated to a parade of planets near the end of month when Jupiter, Mercury, Venus, Uranus and Mars will appear together in the night sky.
On March 28, a large planetary alignment will take place when the five planets appear just after sunset, all within a 50-degree sector of the sky, according to sky tracking site Starwalk.
Jupiter and Mercury will appear near the horizon, in the constellation Pisces, while Venus will be visible higher in the sky on the constellation Aries, the sky-tracking site noted.
Next, Uranus will line up nearby but a pair of binoculars may be required to get a glimpse of the planet. Finally, Mars will appear higher in the sky, near the moon, to complete the five-planet alignment.
“Although March 28 is the best day for observation, the alignment will be visible several days before and after that date,” the website explained.
If the weather isn’t in your favour next week, there will be other opportunities to catch a planetary alignment this year, including another five-planet alignment on June 17. Mercury, Uranus, Jupiter, Neptune, and Saturn will be on parade that evening.





Science
‘Astronomical lightshow’


|
Next year, 2024, is Solar Eclipse Year.
On April 8, 2024, a total solar eclipse will be visible from the south Pacific Ocean, northern Mexico, across the U.S. and through the Atlantic provinces of Canada.
More importantly, the total solar eclipse will be visible from southwestern Newfoundland, in the areas of Stephenville and across central Newfoundland through Terra Nova Park and Gander.
A partial eclipse will be visible across the province, with St. John’s and Corner Brook just outside the range of a total eclipse, an 80 per cent eclipse in Labrador City and a 70 per cent eclipse in Nain.
The 2024 solar eclipse will be the first eclipse crossing the province since 1970 and the only one until 2079.
For many, this is a once-in-a-lifetime event to see a total solar eclipse in Newfoundland and Labrador.
“Solar eclipses are special events in many cultures and have allowed scientists to make great discoveries.”
We are fortunate to even be able to observe a solar eclipse.
The Earth is the only place in our solar system where there is a moon that is about the same size in the sky (0.5 degree) as the sun.
Solar eclipses are special events in many cultures and have allowed scientists to make great discoveries.
When the moon passes in front of the sun, most of the light is blocked and we can see the sun’s corona (more about the corona below).
A note: make sure to wear appropriate eye protection during an eclipse to look at the sun.


The late Dr. Jay Pasachoff, an American astronomer, was so inspired by solar eclipses that he chased them around the world to experience more than 70 eclipses in about 50 years.
In a New York Times 2010 op-ed, he wrote: “There’s also the primal thrill this astronomical lightshow always brings the perfect alignment, in solemn darkness, of the celestial bodies that mean most to us.”
There is the thrill of observing solar eclipses and there is the thrilling science of them, too.
Thanks to solar eclipses, we learn about the sun’s corona, a thin layer of plasma that is just above the sun’s surface.
We normally can’t see it because it is so thin and has such a small density, but the temperature of the corona is about one million degrees Celsius.
It is believed that the corona is related to the sun’s magnetic field and to things like solar flares and mass ejections.
These flares and mass ejections impact the Earth through space weather and the aurorae — phenomena that those of us in the Northern Hemisphere recognize as the Northern Lights.
Scientific discovery
And it’s not just the sun.
Solar eclipses were important to provide some of the early evidence of Albert Einstein’s Theory of General Relativity.
Einstein predicted that light is bent by the gravity of stars.
So, if we can see stars behind the sun, they will appear to be in a slightly different location in the sky relative to each other than when we see them normally.
In 1919 scientists observed stars behind the sun that became visible during a solar eclipse and found that, indeed, their observations agreed with Einstein’s theory.
Town of Gander a major partner
Solar eclipses are fantastic events that connect humans to nature, celestial bodies and to the universe.
Next year’s celebration is an opportunity to celebrate science, nature and humanity.
Thanks to the enthusiasm and excitement of its staff and council, Prof. Svetlana Barkanova, Department of Physics, Grenfell Campus, and I are partnering with the Town of Gander to host a solar eclipse viewing party on April 8, 2024, and a science festival in the days before the eclipse.


The town is excited to be a major partner bringing people from across Newfoundland and Labrador to learn, discover and experience a total solar eclipse together.
The town has pledged to develop a budget to assist with the costs of this unique science festival, along with providing facilities, viewing sites and in-kind assistance.
The event is being planned in collaboration with a continuing science and community outreach program led by Prof. Barkanova and her team.
They deliver a large-scale scientific and cultural outreach program for youth in our province, especially rural youth, girls and Indigenous students, and is currently developing in-person and online seminars and workshops leading up to the solar eclipse.
“It is an ideal chance for us at Memorial to do what we do best — share what is great about our fields.”
This is a call to faculty, students and staff at Memorial University across all campuses to join in the celebration and help it grow and expand.
Not only will we have the opportunity to experience an amazing celestial event, it is a chance to come together in central Newfoundland and share the stories of what we do at Memorial from how we understand the sun and moon in astrophysics, in cultures, in literatures, in humanities and so on.
This is a call to action for your involvement; more participating colleagues means more public talks, Science on Tap events, outreach in schools and more.
It is an ideal chance for us at Memorial to do what we do best — share what is great about our fields and do so around this rare event in Newfoundland and Labrador.
Come join in for Solar Eclipse Year 2024 in Gander. Contact me via email.
Co-authored by Dr. Svetlana Barkanova, Department of Physics, Grenfell Campus, and Brian Williams, tourism development officer, Town of Gander.





-
Art24 hours ago
Daniel Sundahl creates memorial portraits for fallen EPS officers
-
Media13 hours ago
Why one county is suing social media companies
-
Health13 hours ago
‘Worsening spread’ of deadly fungal infection raising alarm in U.S.
-
Business14 hours ago
Shake Shack plans to expand to Canada next year
-
Economy11 hours ago
NOVA Chemicals sets bold ESG aspirations to lead the plastics circular economy
-
Economy18 hours ago
US interest-rate decision the world is watching
-
News21 hours ago
The Losani Family Foundation celebrates 10 years of giving back
-
Investment14 hours ago
Wall Street is thirsty for its next big investment opportunity: The West’s vanishing water