Over 40 stars in a galaxy billions of light-years away were photographed, offering a glimpse into an era when the universe was only half as old as it is now.
Astronomers using the James Webb Space Telescope have accomplished a monumental feat in the field of astronomy by observing individual stars in a galaxy over 6.5 billion light-years away. This milestone, enabled by gravitational lensing and the telescope’s sensitivity, not only challenges previous observational limits but also opens new avenues for understanding the universe’s structure and the mysteries of dark matter.
Cosmic Breakthrough in Astronomy
Seeing individual stars halfway across the observable universe has long been thought impossible — like using binoculars to spot grains of dust on the moon. But an international team of astronomers, led by researchers at the University of Arizona’s Steward Observatory, achieved just that, thanks to a remarkable cosmic phenomenon.
Using NASA’s James Webb Space Telescope (JWST), the team observed a galaxy located nearly 6.5 billion light-years from Earth, from a time when the universe was just half its current age. In this distant galaxy, they identified a surprising number of individual stars, made visible through the combined effects of gravitational lensing — a natural magnification caused by massive objects bending light — and JWST’s exceptional light-collecting power.
Their findings, published on January 6 in Nature Astronomy, set a new record: the largest number of individual stars ever detected in the distant universe. This breakthrough also offers a new pathway to explore one of the cosmos’s greatest enigmas — dark matter.
Unveiling Distant Stars
Most galaxies, including our Milky Way, are home to tens of billions of stars. In nearby galaxies like Andromeda, astronomers can study stars individually. But in galaxies billions of light-years away, the stars blur together, their light traveling for eons before reaching us. This blending has posed a significant challenge for scientists seeking to understand how galaxies form and evolve.
“To us, galaxies that are very far away usually look like a diffuse, fuzzy blob,” said lead study author Yoshinobu Fudamoto, an assistant professor at Chiba University in Japan and a visiting scholar at Steward Observatory. “But actually, those blobs consist of many, many individual stars. We just can’t resolve them with our telescopes.”
Recent advances in astronomy have opened new possibilities by leveraging gravitational lensing – a natural magnification effect caused by the strong gravitational fields of massive objects. As predicted by Albert Einstein, gravitational lenses can amplify the light of distant stars by factors of hundreds or even thousands, making them detectable with sensitive instruments like JWST.
Gravitational Lensing and the Dragon Arc
“These findings have typically been limited to just one or two stars per galaxy,” Fudamoto said. “To study stellar populations in a statistically meaningful way, we need many more observations of individual stars.”
Fengwu Sun, a former U of A graduate student who is now a postdoctoral scholar at the Center for Astrophysics | Harvard & Smithsonian, stumbled on a treasure trove of such stars when he was inspecting JWST images of a galaxy known as the Dragon Arc, located along the line of sight from Earth behind a massive cluster of galaxies called Abell 370. Due to its gravitational lensing effect, Abell 370 stretches the Dragon Arc’s signature spiral into an elongated shape – like a hall of mirrors of cosmic proportions.
In December 2022 and 2023, JWST obtained two pictures of the Dragon Arc. Within these images, astronomers counted 44 individual stars whose brightness changed over time due to variations in the gravitational lensing landscape.
“This groundbreaking discovery demonstrates, for the first time, that studying large numbers of individual stars in a distant galaxy is possible,” Sun said – as long as nature is there to lend a helping hand.
Microlensing Reveals New Insights
However, even extremely strong gravitational magnification from a galaxy cluster is not sufficient to magnify individual stars in galaxies even farther away. In this case, the discovery was made possible by a serendipitous alignment of “lucky stars.”
“Inside the galaxy cluster, there are many stars floating around that are not bound by any galaxy,” said co-author Eiichi Egami, a research professor at Steward Observatory. “When one of them happens to pass in front of the background star in the distant galaxy along the line of sight with Earth, it acts as a microlens, in addition to the macrolensing effect of the galaxy cluster as a whole.”
The combined effects of macrolensing and microlensing dramatically increase the magnification factor, allowing JWST to pick up individual stars that otherwise would be too far and faint to be detected at all.
Because the stars inside the magnifying cluster move relative to the target stars in the distant galaxy and Earth, the alignment of microlenses in this natural “telescope” changes slightly over short timeframes – from a few days to a week. When they are perfectly aligned, the brightness and magnification of the distant stars increase dramatically, only to fade again shortly afterwards.
“By observing the same galaxy multiple times, we can spot stars in distant galaxies because they appear to pop in and out of existence,” Fudamoto said. “This is a result of the varying effective magnifications from the macro- and microlensing effect as the microlensing stars move in and out of the line of sight.”
The research team carefully analyzed colors of each of the stars inside the Dragon Arc and found that many are red supergiants, similar to Betelgeuse in the constellation of Orion, which is in the final stages of its life. This contrasts with earlier discoveries, which predominantly identified blue “supergiants” similar to Rigel and Deneb, which are among the brightest stars in the night sky. According to the researchers, this difference in stellar types also highlights the unique power of JWST observations at infrared wavelengths that could detect stars at lower temperatures.
Future JWST observations are expected to capture more magnified stars in the Dragon Arc galaxy. These efforts could lead to detailed studies of hundreds of stars in distant galaxies. Moreover, observations of individual stars could provide insight into the structure of gravitational lenses and even shed light on the elusive nature of dark matter.
Reference: “Identification of more than 40 gravitationally magnified stars in a galaxy at redshift 0.725” by Yoshinobu Fudamoto, Fengwu Sun, Jose M. Diego, Liang Dai, Masamune Oguri, Adi Zitrin, Erik Zackrisson, Mathilde Jauzac, David J. Lagattuta, Eiichi Egami, Edoardo Iani, Rogier A. Windhorst, Katsuya T. Abe, Franz Erik Bauer, Fuyan Bian, Rachana Bhatawdekar, Thomas J. Broadhurst, Zheng Cai, Chian-Chou Chen, Wenlei Chen, Seth H. Cohen, Christopher J. Conselice, Daniel Espada, Nicholas Foo, Brenda L. Frye, Seiji Fujimoto, Lukas J. Furtak, Miriam Golubchik, Tiger Yu-Yang Hsiao, Jean-Baptiste Jolly, Hiroki Kawai, Patrick L. Kelly, Anton M. Koekemoer, Kotaro Kohno, Vasily Kokorev, Mingyu Li, Zihao Li, Xiaojing Lin, Georgios E. Magdis, Ashish K. Meena, Anna Niemiec, Armin Nabizadeh, Johan Richard, Charles L. Steinhardt, Yunjing Wu, Yongda Zhu and Siwei Zou, 6 January 2025, Nature Astronomy.
DOI: 10.1038/s41550-024-02432-3
This project was supported by multiple funders including NASA and NSF.
