Using the unique infrared sensitivity of NASA’s James Webb Space Telescope, researchers can examine ancient galaxies to probe secrets of the early universe. Now, an international team of astronomers has identified bright hydrogen emission from a galaxy in an unexpectedly early time in the universe’s history. The surprise finding is challenging researchers to explain how this light could have pierced the thick fog of neutral hydrogen that filled space at that time.
The Webb telescope discovered the
incredibly distant galaxy JADES-GS-z13-1, observed to exist just 330 million
years after the big bang, in images taken by Webb’s NIRCam (Near-Infrared
Camera) as part of the James Webb Space Telescope Advanced Deep Extragalactic
Survey (JADES). Researchers used the galaxy’s brightness in different infrared
filters to estimate its redshift, which measures a galaxy’s distance from Earth based
on how its light has been stretched out during its journey through expanding
space.
Image A: JADES-GS-z13-1 in the
GOODS-S field (NIRCam Image)
The incredibly distant galaxy JADES-GS-z13-1, observed
just 330 million years after the big bang, was initially discovered with deep
imaging from NASA’s James Webb Space Telescope’s NIRCam (Near-Infrared Camera).
Now, an international team of astronomers definitively has identified powerful
hydrogen emission from this galaxy at an unexpectedly early period in the
universe’s history. JADES-GS-z-13 has a redshift (z) of 13, which is an
indication of its age and distance.
NASA, ESA, CSA, JADES Collaboration, J. Witstok
(University of Cambridge/University of Copenhagen), P. Jakobsen (University of
Copenhagen), A. Pagan (STScI), M. Zamani (ESA/Webb)
Image B: JADES-GS-z13-1 (NIRCam
Close-Up)
This image shows the galaxy JADES GS-z13-1 (the red
dot at center), imaged with NASA’s James Webb Space Telescope’s NIRCam
(Near-Infrared Camera) as part of the JWST Advanced Deep Extragalactic Survey
(JADES) program. These data from NIRCam allowed researchers to identify
GS-z13-1 as an incredibly distant galaxy, and to put an estimate on its
redshift value. Webb’s unique infrared sensitivity is necessary to observe
galaxies at this extreme distance, whose light has been shifted into infrared
wavelengths during its long journey across the cosmos.
NASA, ESA, CSA, JADES Collaboration, J. Witstok
(University of Cambridge/University of Copenhagen), P. Jakobsen (University of
Copenhagen), M. Zamani (ESA/Webb)
The NIRCam imaging yielded an initial redshift estimate of 12.9. Seeking to
confirm its extreme redshift, an international team lead by Joris Witstok of
the University of Cambridge in the United Kingdom, as well as the Cosmic Dawn
Center and the University of Copenhagen in Denmark, then observed the galaxy
using Webb’s Near-Infrared Spectrograph instrument.
In the resulting spectrum, the redshift was confirmed to be 13.0. This equates
to a galaxy seen just 330 million years after the big bang, a small fraction of
the universe’s present age of 13.8 billion years old. But an unexpected feature
stood out as well: one specific, distinctly bright wavelength of light, known
as Lyman-alpha emission, radiated by hydrogen atoms. This emission was far
stronger than astronomers thought possible at this early stage in the
universe’s development.
“The early universe was bathed in a
thick fog of neutral hydrogen,” explained Roberto Maiolino, a team member from
the University of Cambridge and University College London. “Most of this haze
was lifted in a process called reionization, which was completed about one
billion years after the big bang. GS-z13-1 is seen when the universe was only
330 million years old, yet it shows a surprisingly clear, telltale signature of
Lyman-alpha emission that can only be seen once the surrounding fog has fully
lifted. This result was totally unexpected by theories of early galaxy
formation and has caught astronomers by surprise.”
Image C: JADES-GS-z13-1 Spectrum
Graphic
NASA’s James Webb Space Telescope has detected
unexpected light from a distant galaxy. The galaxy JADES-GS-z13-1, observed
just 330 million years after the big bang (corresponding to a redshift of
z=13.05), shows bright emission from hydrogen known as Lyman-alpha emission.
This is surprising because that emission should have been absorbed by a dense
fog of neutral hydrogen that suffused the early universe.
NASA, ESA, CSA, J. Witstok (University of Cambridge,
University of Copenhagen), J. Olmsted (STScI)
Before and during the era of reionization, the immense amounts of neutral hydrogen fog surrounding galaxies
blocked any energetic ultraviolet light they emitted, much like the filtering
effect of colored glass. Until enough stars had formed and were able to ionize
the hydrogen gas, no such light — including Lyman-alpha emission — could escape
from these fledgling galaxies to reach Earth. The confirmation of Lyman-alpha
radiation from this galaxy, therefore, has great implications for our
understanding of the early universe.
“We really shouldn’t have found a galaxy
like this, given our understanding of the way the universe has evolved,” said
Kevin Hainline, a team member from the University of Arizona. “We could think
of the early universe as shrouded with a thick fog that would make it
exceedingly difficult to find even powerful lighthouses peeking through, yet
here we see the beam of light from this galaxy piercing the veil. This
fascinating emission line has huge ramifications for how and when the universe
reionized.”
The source of the Lyman-alpha radiation
from this galaxy is not yet known, but it may include the first light from the
earliest generation of stars to form in the universe.
“The large bubble of ionized hydrogen
surrounding this galaxy might have been created by a peculiar population of
stars — much more massive, hotter, and more luminous than stars formed at later
epochs, and possibly representative of the first generation of stars,” said
Witstok. A powerful active galactic nucleus, driven by one of the first supermassive black holes, is another
possibility identified by the team.
This research was published Wednesday in
the journal Nature.
The James Webb Space Telescope is the world's premier space science observatory. Webb is solving mysteries in our solar system, looking beyond to distant worlds around other stars, and probing 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).
Source: NASA’s Webb Sees Galaxy Mysteriously Clearing Fog of Early Universe - NASA Science
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