James Webb Space Telescope Reveals Oldest Star Clusters in the Universe

Webb SMACS 0723 Crop

Thousands of galaxies flood this near-infrared, high-resolution image of galaxy cluster SMACS 0723. Credit: NASA, ESA, CSA, STScI

A team of astronomers used the James Webb Telescope (JWST) to identify the most distant globular clusters ever discovered. These dense groups of millions of stars may be relics containing the first and oldest stars in the universe.

The early analysis of Webb’s First Deep Field image, which depicts some of the universe’s earliest galaxies, was published recently in The Astrophysical Journal Letters. The work was conducted by a team of Canadian astronomers, including experts from the Dunlap Institute for Astronomy & Astrophysics in the University of Toronto’s Faculty of Arts & Science.

“JWST was built to find the first stars and the first galaxies and to help us understand the origins of complexity in the universe, such as the chemical elements and the building blocks of life,” says Lamiya Mowla, a post-doctoral researcher at the Dunlap Institute for Astronomy & Astrophysics and co-lead author of the study, which was carried out by the CAnadian NIRISS Unbiased Cluster Survey (CANUCS) team.

“This discovery in Webb’s First Deep Field is already providing a detailed look at the earliest phase of star formation, confirming the incredible power of JWST.”

Sparkler Galaxy Infographic

The researchers studied the Sparkler galaxy located in Webb’s First Deep Field and used JWST to determine that five of the sparkling objects around it are globular clusters. Credit: Image via Canadian Space Agency with images from NASA, ESA, CSA, STScI; Mowla, Iyer et al. 2022

In the finely detailed Webb’s First Deep Field image, the astronomers quickly zeroed in on what they’ve dubbed “the Sparkler galaxy.” Located nine billion light years away, this galaxy got its name from the compact objects appearing as small yellow-red dots surrounding it, referred to by the researchers as “sparkles.” The research team determined that these sparkles could either be young clusters actively forming stars – born three billion years after the Big Bang at the peak of star formation – or old globular clusters. Globular clusters are ancient collections of stars from a galaxy’s infancy and contain clues about its earliest phases of formation and growth.

From an initial analysis of 12 of these compact objects, the researcher team determined that five of them are not only globular clusters but among the oldest ones known.

“Looking at the first images from JWST and discovering old globular clusters around distant galaxies was an incredible moment – one that wasn’t possible with previous Hubble Space Telescope imaging,” says Kartheik G. Iyer, a post-doctoral researcher at the Dunlap Institute for Astronomy & Astrophysics and co-lead author of the study.

“Since we could observe the sparkles across a range of wavelengths, we could model them and better understand their physical properties – like how old they are and how many stars they contain. We hope the knowledge that globular clusters can be observed at from such great distances with JWST will spur further science and searches for similar objects.”

Gravitational Lensing in Action

Gravitational lensing is used by astronomers to study very distant and very faint galaxies. Credit: NASA, ESA & L. Calçada

The Milky Way galaxy is known to have about 150 globular clusters, but how and when exactly these dense clumps of stars formed is not well understood. Astronomers know that globular clusters can be extremely old, but it is incredibly challenging to measure their ages. Using very distant globular clusters to age-date the first stars in distant galaxies has not been done before and is only possible with JWST.

“These newly identified clusters were formed close to the first time it was even possible to form stars,” says Mowla. “Because the Sparkler galaxy is much farther away than our own Milky Way, it is easier to determine the ages of its globular clusters. We are observing the Sparkler as it was nine billion years ago, when the universe was only four-and-a-half billion years old, looking at something that happened a long time ago. Think of it as guessing a person’s age based on their appearance – it’s easy to tell the difference between a five- and 10-year-old, but hard to tell the difference between a 50- and 55-year-old.”

Until now, astronomers could not see the surrounding compact objects of the Sparkler galaxy with the Hubble Space Telescope. This changed with JWST’s increased resolution and sensitivity, unveiling the tiny dots surrounding the galaxy for the first time in Webb’s First Deep Field image. The Sparkler galaxy is special because it is magnified by a factor of 100 due to an effect called gravitational lensing – where the SMACS 0723 galaxy cluster in the foreground distorts what is behind it, much like a giant magnifying glass. Moreover, gravitational lensing produces three separate images of the Sparkler, allowing astronomers to study the galaxy in greater detail.

Researchers Reveal a Galaxy Sparkling With the Universe’s Oldest Star Clusters

From left: Kartheik Iyer, Vince Estrada-Carpenter, Guillaume Desperez, Lamiya Mowla, Marcin Sawicki, Victoria Strait, Gabe Brammer and Kate Gould (on laptop screen), Ghassan Sarrouh, Chris Willott, Bob Abraham, Gael Noirot, Yoshi Asada, Nick Martis, Credit: Photo courtesy of Lamiya Mowla and Kartheik Iyer

“Our study of the Sparkler highlights the tremendous power in combining the unique capabilities of JWST with the natural magnification afforded by gravitational lensing,” says CANUCS team lead Chris Willott from the National Research Council’s Herzberg Astronomy and Astrophysics Research Centre. “The team is excited about more discoveries to come when JWST turns its eye on the CANUCS galaxy clusters next month.”

The researchers combined new data from JWST’s Near-Infrared Camera (NIRCam) with Hubble Scape Telescope archival data. NIRCam detects faint objects using longer and redder wavelengths to observe past what is visible to the human eye and even the Hubble Space Telescope. Both magnifications due to the lensing by the galaxy cluster and the high resolution of JWST are what made observing compact objects possible.

The Canadian-made Near-Infrared Imager and Slitless Spectrograph (NIRISS) instrument on the JWST provided independent confirmation that the objects are old globular clusters because the researchers did not observe oxygen emission lines – emissions with measurable spectra given off by young clusters that are actively forming stars. NIRISS also helped unravel the geometry of the triply lensed images of the Sparkler.

“JWST’s made-in-Canada NIRISS instrument was vital in helping us understand how the three images of the Sparkler and its globular clusters are connected,” says Marcin Sawicki, a professor at Saint Mary’s University who is Canada Research Chair in Astronomy and co-author of the study. “Seeing several of the Sparkler’s globular clusters imaged three times made it clear that they are orbiting around the Sparkler galaxy rather than being simply in front of it by chance.”

JWST will observe the CANUCS fields starting in October 2022, leveraging its data to examine five massive clusters of galaxies, around which the researchers expect to find more such systems. Future studies will also model the galaxy cluster to understand the lensing effect and execute more robust analyses to explain the star formation histories.

Reference: “The Sparkler: Evolved High-redshift Globular Cluster Candidates Captured by JWST” by Lamiya Mowla, Kartheik G. Iyer, Guillaume Desprez, Vicente Estrada-Carpenter, Nicholas S. Martis, Gaël Noirot, Ghassan T. Sarrouh, Victoria Strait, Yoshihisa Asada, Roberto G. Abraham, Gabriel Brammer, Marcin Sawicki, Chris J. Willott, Marusa Bradac, René Doyon, Adam Muzzin, Camilla Pacifici, Swara Ravindranath and Johannes Zabl, 29 September 2022, The Astrophysical Journal Letters.
DOI: 10.3847/2041-8213/ac90ca

Collaborating institutions include York University and institutions in the United States and Europe. The research was supported by the Canadian Space Agency and the Natural Sciences and Engineering Research Council of Canada.

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