Webb Telescope’s Infrared Vision Explores the Final Frontier
An unexpectedly rich “undiscovered country” of early galaxies that has been largely hidden until now has been found by NASA’s powerful James Webb Space Telescope.
Webb is unveiling a very rich universe where the first forming galaxies look remarkably different from the mature galaxies seen around us today. Two exceptionally bright galaxies that existed approximately 350 and 450 million years after the big bang were found by researchers. Astronomers are puzzled by the extreme brightness of these young galaxies. They are transforming gas into stars extremely rapidly and appear compacted in spherical or disk shapes that are much smaller than our Milky Way galaxy. The onset of stellar birth may have started just 100 million years after the big bang, which happened 13.8 billion years ago.
Follow-up spectroscopic observations with Webb should confirm the distances to these remote galaxies, and also reveal the rate of star formation and elemental abundances in the makeup of the early stars.
This video features an interview with Tommaso Treu, principal investigator of the GLASS-JWST Early Release Science Program (Grism Lens-Amplified Survey from Space). This program recently obtained an image of the galaxy cluster Abell 2744, also known as Pandora’s Cluster. In it, about 6,000 galaxies can be detected within a region of sky no larger than a grain of sand held at arm’s length. Initial analysis suggests that an unusual number of galaxies in the early universe were much brighter than expected.
NASA’s Webb Draws Back Curtain on Universe’s Early Galaxies
Just a few days after officially starting science operations, NASA’s James Webb Space Telescope propelled astronomers into a realm of early galaxies, previously hidden beyond the grasp of all other telescopes until now.
“Everything we see is new. Webb is showing us that there’s a very rich universe beyond what we imagined,” said Tommaso Treu of the University of California at Los Angeles, principal investigator on one of the Webb programs. “Once again the universe has surprised us. These early galaxies are very unusual in many ways.”
Two research papers, led by Marco Castellano of the National Institute for Astrophysics in Rome, Italy, and Rohan Naidu of the Harvard-Smithsonian Center for Astrophysics and the Massachusetts Institute of Technology in Cambridge, Massachusetts, have been published in the Astrophysical Journal Letters.
These initial findings are from a broader Webb research initiative involving two Early Release Science (ERS) programs: the Grism Lens-Amplified Survey from Space (GLASS), and the Cosmic Evolution Early Release Science Survey (CEERS).
With just four days of analysis, researchers found two exceptionally bright galaxies in the GLASS-JWST images. These galaxies existed approximately 450 and 350 million years after the big bang (with a redshift of approximately 10.5 and 12.5, respectively), though future spectroscopic measurements with Webb will help confirm.
“Everything we see is new. Webb is showing us that there’s a very rich universe beyond what we imagined. Once again the universe has surprised us. These early galaxies are very unusual in many ways.” — Tommaso Treu
“With Webb, we were amazed to find the most distant starlight that anyone had ever seen, just days after Webb released its first data,” said Naidu of the more distant GLASS galaxy, referred to as GLASS-z12, which is believed to date back to 350 million years after big bang. The previous record holder is galaxy GN-z11, which existed 400 million years after the big bang (redshift 11.1), and was identified in 2016 by Hubble and Keck Observatory in deep-sky programs.
“Based on all the predictions, we thought we had to search a much bigger volume of space to find such galaxies,” said Castellano.
“These observations just make your head explode. This is a whole new chapter in astronomy. It’s like an archaeological dig, and suddenly you find a lost city or something you didn’t know about. It’s just staggering,” added Paola Santini, fourth author of the Castellano et al. GLASS-JWST paper.
“While the distances of these early sources still need to be confirmed with spectroscopy, their extreme brightnesses are a real puzzle, challenging our understanding of galaxy formation,” noted Pascal Oesch at the University of Geneva in Switzerland, second author of the Naidu et al. paper.
The Webb observations nudge astronomers toward a consensus that an unusual number of galaxies in the early universe were so much brighter than expected. This will make it easier for Webb to find even more early galaxies in subsequent deep sky surveys, say researchers.
“We’ve nailed something that is incredibly fascinating. These galaxies would have had to have started coming together maybe just 100 million years after the big bang. Nobody expected that the dark ages would have ended so early,” said Garth Illingworth of the University of California at Santa Cruz, a member of the Naidu/Oesch team. “The primal universe would have been just one hundredth its current age. It’s a sliver of time in the 13.8 billion-year-old evolving cosmos.”
Erica Nelson of the University of Colorado in Boulder, a member of the Naidu/Oesch team, noted that “our team was struck by being able to measure the shapes of these first galaxies; their calm, orderly disks question our understanding of how the first galaxies formed in the crowded, chaotic early universe.” This remarkable discovery of compact disks at such early times was only possible because of Webb’s much sharper images, in infrared light, compared to Hubble.
“These galaxies are very different than the Milky Way or other big galaxies we see around us today,” said Treu.
Illingworth emphasized the two bright galaxies found by these teams have a lot of light. He said one option is that they could have been very massive, with lots of low-mass stars, like later galaxies. Alternatively, they could be much less massive, consisting of far fewer extraordinarily bright stars, known as Population III stars. Long theorized, they would be the first stars ever born, blazing at blistering temperatures and made up only of primordial hydrogen and helium – before stars could later cook up heavier elements in their nuclear fusion furnaces. No such extremely hot, primordial stars are seen in the local universe.
“Indeed, the farthest source is very compact, and its colors seem to indicate that its stellar population is particularly devoid of heavy elements and could even contain some Population III stars. Only Webb spectra will tell,” said Adriano Fontana, second author of the Castellano et al. paper and a member of the GLASS-JWST team.
Present Webb distance estimates to these two galaxies are based on measuring their infrared colors. Eventually, follow-up spectroscopy measurements showing how light has been stretched in the expanding universe will provide independent verification of these cosmic yardstick measurements.
“Early Results from GLASS-JWST. I: Confirmation of Lensed z = 7 Lyman-break Galaxies behind the Abell 2744 Cluster with NIRISS” by Guido Roberts-Borsani, Takahiro Morishita, Tommaso Treu, Gabriel Brammer, Victoria Strait, Xin Wang, Marusa Bradac, Ana Acebron, Pietro Bergamini, Kristan Boyett, Antonello Calabró, Marco Castellano, Adriano Fontana, Karl Glazebrook, Claudio Grillo, Alaina Henry, Tucker Jones, Matthew Malkan, Danilo Marchesini, Sara Mascia, Charlotte Mason, Amata Mercurio, Emiliano Merlin, Themiya Nanayakkara, Laura Pentericci, Piero Rosati, Paola Santini, Claudia Scarlata, Michele Trenti, Eros Vanzella, Benedetta Vulcani and Chris Willott, 18 October 2022, Astrophysical Journal Letters.
“Two Remarkably Luminous Galaxy Candidates at z ˜ 10–12 Revealed by JWST” by Rohan P. Naidu, Pascal A. Oesch, Pieter van Dokkum, Erica J. Nelson, Katherine A. Suess, Gabriel Brammer, Katherine E. Whitaker, Garth Illingworth, Rychard Bouwens, Sandro Tacchella, Jorryt Matthee, Natalie Allen, Rachel Bezanson, Charlie Conroy, Ivo Labbe, Joel Leja, Ecaterina Leonova, Dan Magee, Sedona H. Price, David J. Setton, Victoria Strait, Mauro Stefanon, Sune Toft, John R. Weaver and Andrea Weibel, 17 November 2022, Astrophysical Journal Letters.
The James Webb Space Telescope is the world’s premier space science observatory. Webb will solve mysteries in our solar system, look beyond to distant worlds around other stars, and probe the mysterious structures and origins of our universe and our place in it. Webb is an international program led by NASA with its partners, ESA (European Space Agency) and CSA (Canadian Space Agency).
If I remember correctly, Hubble already saw 400 mly after the BB and Webb is expected to see 100-200 mly more back. So what is the bg deal with this 350 mly ‘discivery’? !
If I remember correctly, Hubble already saw 400 mly after the BB and Webb is expected to see 100-200 mly more back. So what is the big deal with this 350 mly ‘discovery’? !
It’s exciting both because it replace earlier expectations with new data and because it confirms JWST is exceeding expectations.
From CNN’s article:
“Previously, the earliest galaxy observed was GN-z11, which existed 400 million years after the big bang and was spotted by the Hubble Space Telescope in 2016.
“As soon as we started taking data, we discovered that there are many more distant galaxies than we were expecting,” said Tommaso Treu, principal investigator for the GLASS-JWST Early Release Science Program and professor at the University of California at Los Angeles.
“Somehow, the universe managed to form galaxies faster and earlier than we thought. Just a few hundred million years after the big bang, there were already lots of galaxies. JWST has opened up a new frontier, bringing us closer to understanding how it all began. And we’ve just started to explore it,” said Treu, who was a coauthor of an October study in The Astrophysical Journal Letters.”
“The Webb telescope has entered its fifth month of science operations and has proven to be more powerful and capturing sharper images than prelaunch expectations, said Dr. Jane Rigby, Webb operations project scientist at NASA’s Goddard Space Flight Center in Greenbelt, Maryland.
“These galaxies we’re talking about are bright,” Rigby said. “They were hiding just under the limits of what Hubble could do. They were right there waiting for us. We just had to go a little redder and go deeper than what Hubble could do.””
Mathematics is the language in which human write the universe. Topological vortices are natural gravitational fields. Their interaction and balance, covering all long-distance and short-range contributions of space-time movement, are fundamental to the evolution of cosmic matter movement.
Gravitational fields can be approximated by quantum gravity field theory, and while it is a tensor field it isn’t filled with vortices.
Matter movement mainly derives from the web of cosmological filaments and gravity contracting them and streaming gas and galaxies towards the web nodes. These filaments are imprints of the quantum fluctuations of the inflation field and has nothing to do with space expansion which in turn is a scale expansion and not “space-time movement”. From LCDM observations we know that the spacetime underlying our universe is stationary and non-rotating.
C.f. “Big Bang” and “Scale factor (cosmology)” in Wikipedia – this is basic knowledge.
One is vortex. More is different.
And see “Quantum gravity as a low energy effective field theory” in Scholarpedia for why we know there isn’t any vortices in the gravity field composition.
Topological vortex field behave a rotational motion around a relatively fixed guiding center, the nature of it is a gravitational field. The topological vortex field pairs can be the graviton pairs. Topologically trivial (N=0) graviton pairs undergo Kelvin motion, while nontrivial (N=±1) graviton pairs behave a rotational motion around a fixed guiding center. The point defects in the bifurcation processes of the graviton pairs generate or annihilate at the limit points, and encounter, split or merge at the bifurcation points of the 3-dimensional vector order parameter, and form unstable point defects system.
If you are interested, you can browse https://zhuanlan.zhihu.com/p/466343173.
From the companion paper “Early Results From GLASS-JWST. XII: The Morphology of Galaxies at the Epoch of Reionization” that studied a subset of 19 galaxies with a Lyman break redshift z = 7-12:
“We suggest a possible scenario that could at least qualitatively explain the observations. These galaxies are undergoing galaxy-scale rapid star formation. The timescales are extremely compressed given the young age of the Universe and the likely rising star formation rate (Finlator et al. 2011), leaving little time for the emergence of older stellar populations. … therefore they are likely well mixed. Dust extinction is not sufficient in quantity or patchiness to induce detectable differences. The clear detection of interacting systems is consistent with merging also contributing to the growth of these galaxies.”
“… these galaxies are compact, as shown in companion paper V …”.
So rapidly evolving, merging galaxies of either many small pop II stars or larger pop III stars, galaxies that likely starts out compact – though they need a larger and deeper galaxy set to test all this. Of course it is tempting to suggest that the concurrence of the end of dark ages and the dust unobscured galaxies are caused by the latter, and it seems it may be a possible explanation. From a press release authored by Holly Ober, University of California, Los Angeles:
“Scientists think that sometime within the universe’s first billion years radiation emitted by the first galaxies and possibly by the first black holes caused the hydrogen atoms to lose electrons, or ionize, preventing photons from “sticking” to them and clearing a pathway for the photons to travel across space. … Roberts-Borsani’s finding that galaxies formed faster and earlier than previously thought could confirm that they were the culprits of cosmic reionization.”
it goes forever and ever, it never ends!!!