NASA’s Webb Reaches New Milestone in Quest for Distant Galaxies

NASA's James Webb Space Telescope.
An international team of astronomers has used data from NASA's James Webb Space Telescope to report the discovery of the earliest galaxies confirmed to date. (Image: via NASA)

An international team of astronomers has used data from NASA’s James Webb Space Telescope to report the discovery of the earliest galaxies confirmed to date. The light from these galaxies has taken more than 13.4 billion years to reach us, as these galaxies date back to less than 400 million years after the big bang when the universe was only 2 percent of its current age.

Earlier data from Webb had provided candidates for such infant galaxies. These targets have been confirmed by obtaining spectroscopic observations, revealing characteristic and distinctive patterns in the fingerprints of light coming from these incredibly faint galaxies. Astronomer and co-author Emma Curtis-Lake from the University of Hertfordshire in the United Kingdom said:

“It was crucial to prove that these galaxies do, indeed, inhabit the early universe. It’s very possible for closer galaxies to masquerade as very distant galaxies. Seeing the spectrum revealed as we hoped, confirming these galaxies as being at the true edge of our view, some further away than Hubble could see! It is a tremendously exciting achievement for the mission.”

The observations resulted from a collaboration of scientists who led the development of two of the instruments on board Webb, the Near-Infrared Camera (NIRCam) and the Near-Infrared Spectrograph (NIRSpec). The investigation of the faintest and earliest galaxies was the leading motivation behind the concepts for these instruments.

In 2015 the instrument teams joined together to propose the JWST Advanced Deep Extragalactic Survey (JADES), an ambitious program that has been allocated just over one month of the telescope’s time spread over two years and is designed to provide a view of the early universe unprecedented in both depth and detail.

JADES is an international collaboration of more than eighty astronomers from ten countries. Co-author Marcia Rieke, the NIRCam principal investigator of the University of Arizona in Tucson, said:

“These results are the culmination of why the NIRCam and NIRSpec teams joined together to execute this observing program.”

Webb is providing the faintest and sharpest images yet obtained

The first round of JADES observations focused on the area in and around the Hubble Space Telescope’s Ultra Deep Field. For over 20 years, this small patch of the sky has been the target of nearly all large telescopes, building an exceptionally sensitive data set spanning the entire electromagnetic spectrum. Now Webb is adding its unique view, providing the faintest and sharpest images yet obtained.

The Webb Advanced Deep Extragalactic Survey (JADES) focused on the area in and around the Hubble Space Telescope’s Ultra Deep Field.
The Webb Advanced Deep Extragalactic Survey (JADES) focused on the area in and around the Hubble Space Telescope’s Ultra Deep Field. Using Webb’s NIRCam instrument, scientists observed the field in nine infrared wavelength ranges. From these images (shown at left), the team searched for faint galaxies visible in the infrared but whose spectra abruptly cut off at a critical wavelength known as the Lyman break. Webb’s NIRSpec instrument then yielded a precise measurement of each galaxy’s redshift (shown at right). Four galaxies studied are particularly special, as they were revealed to be at an unprecedentedly early epoch. These galaxies date back to less than 400 million years after the big bang when the universe was only 2% of its current age. In the background image, blue represents light at 1.15 microns (115W), green is 2.0 microns (200W), and red is 4.44 microns (444W). In the cutout images, blue is a combination of 0.9 and 1.15 microns (090W+115W), green is 1.5 and 2.0 microns (150W+200W), and red is 2.0, 2.77, and 4.44 microns (200W+277W+444W). (Image: M. Zamani (ESA / Webb), L. Hustak (STScI). Science: B. Robertson (UCSC), S. Tacchella (Cambridge), E. Curtis-Lake (Hertfordshire), S. Carniani (Scuola Normale Superiore), and the JADES Collaboration via NASA, ESA, CSA, and STScI)

The JADES program began with NIRCam, using over 10 days of mission time to observe the field in nine different infrared colors and produce exquisite images of the sky. The region is 15 times larger than the deepest infrared images produced by the Hubble Space Telescope, yet is even deeper and sharper at these wavelengths. The image is only the size a human appears when viewed from a mile away.

However, it teems with nearly 100,000 galaxies, each caught at some moment in their history, billions of years in the past. Co-author Brant Robertson from the University of California Santa Cruz, a member of the NIRCam science team, said:

“For the first time, we have discovered galaxies only 350 million years after the big bang, and we can be absolutely confident of their fantastic distances. To find these early galaxies in such stunningly beautiful images is a special experience.”

From these images, the galaxies in the early universe can be distinguished by a tell-tale aspect of their multi-wavelength colors. Light is stretched in wavelength as the universe expands, and the light from these youngest galaxies has been stretched by a factor of up to 14.

Astronomers search for faint galaxies that are visible in the infrared but whose light abruptly cuts off at a critical wavelength. The location of the cutoff within each galaxy’s spectrum is shifted by the universe’s expansion. The JADES team scoured the Webb images looking for these distinctive candidates.

This image taken by the James Webb Space Telescope highlights the region of study by the Webb Advanced Deep Extragalactic Survey (JADES)
This image taken by the James Webb Space Telescope highlights the region of study by the Webb Advanced Deep Extragalactic Survey (JADES). This area is in and around the Hubble Space Telescope’s Ultra Deep Field. Scientists used Webb’s NIRCam instrument to observe the field in nine different infrared wavelength ranges. From these images, the team searched for faint galaxies that are visible in the infrared but whose spectra abruptly cut off at a critical wavelength. They conducted additional observations (not shown here) with Webb’s NIRSpec instrument to measure each galaxy’s redshift and reveal the properties of the gas and stars in these galaxies. In this image, blue represents light at 1.15 microns (115W), green is 2.0 microns (200W), and red is 4.44 microns (444W). (Image: M. Zamani (ESA/Webb). Science: B. Robertson (UCSC), S. Tacchella (Cambridge), E. Curtis-Lake (Hertfordshire), S. Carniani (Scuola Normale Superiore), and the JADES Collaboration via NASA, ESA, CSA)

They then used the NIRSpec instrument for a single observation period spanning three days totaling 28 hours of data collection. The team collected the light from 250 faint galaxies, allowing astronomers to study the patterns imprinted on the spectrum by the atoms in each galaxy.

This yielded a precise measurement of each galaxy’s redshift and revealed the properties of the gas and stars in these galaxies. Astronomer and co-author Stefano Carniani from Scuola Normale Superiore in Italy said:

“These are by far the faintest infrared spectra ever taken. They reveal what we hoped to see: a precise measurement of the cutoff wavelength of light due to the scattering of intergalactic hydrogen.”

Four of the galaxies studied are particularly special, as they were revealed to be at an unprecedentedly early epoch. The results provided spectroscopic confirmation that these four galaxies lie at redshifts above 10, including two at redshift 13. This corresponds to a time when the universe was approximately 330 million years old, setting a new frontier in the search for far-flung galaxies.

These galaxies are extremely faint because of their great distance from us. Astronomers can now explore their properties thanks to Webb’s exquisite sensitivity. Astronomer and co-author Sandro Tacchella from the University of Cambridge in the United Kingdom explained:

“It is hard to understand galaxies without understanding the initial periods of their development. Much as with humans, so much of what happens later depends on the impact of these early generations of stars. So many questions about galaxies have been waiting for the transformative opportunity of Webb, and we’re thrilled to be able to play a part in revealing this story.”

JADES will continue in 2023 with a detailed study of another field centered on the iconic Hubble Deep Field and then return to the Ultra Deep Field for another round of deep imaging and spectroscopy. Many more candidates in the field await spectroscopic investigation, with hundreds of hours of additional time already approved.

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 our universe’s mysterious structures and origins 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).

Provided by NASA [Note: Materials may be edited for content and length.]

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