James Webb Telescope Uncovers Possible Dark Stars

The James Webb Telescope initially classified these three objects (JADES-GS-z13-0, JADES-GS-z12-0, and JADES-GS-z11-0) as galaxies during the JWST Advanced Deep Extragalactic Survey (JADES) in December 2022. However, a team led by Katherine Freese at The University of Texas at Austin suggests that they may be "dark stars," theoretical entities that surpass our sun in size and brightness, fueled by the annihilation of dark matter particles. Credit:NASA/ESA

July 16, 2023


The James Webb Space Telescope (JWST) has made a groundbreaking discovery, capturing images that suggest the existence of "dark stars." These enigmatic objects, potentially much larger and brighter than our sun, are believed to be powered by the annihilation of dark matter particles. The findings, made by a team of astrophysicists led by Katherine Freese at the University of Texas at Austin, could provide vital insights into the elusive nature of dark matter, a fundamental puzzle in the realm of physics. In this article, we delve into the significance of this discovery and its implications for our understanding of the universe.

Unveiling the Dark Stars

The recent analysis of JWST images has revealed three intriguing objects, initially identified as galaxies in December 2022 as part of the JWST Advanced Deep Extragalactic Survey (JADES). These objects, designated as JADES-GS-z13-0, JADES-GS-z12-0, and JADES-GS-z11-0, are now being considered potential dark stars. Dark stars, if confirmed, hold the key to unraveling the mysteries of dark matter, which accounts for approximately 25% of the universe's composition.

Dark Matter: A Cosmic Enigma

Despite its significant presence in the cosmos, dark matter remains one of the most enigmatic phenomena in modern physics. Scientists hypothesize that dark matter consists of a novel type of elementary particle. Detecting and understanding these particles has been a primary focus of scientific exploration. Leading candidates, such as Weakly Interacting Massive Particles (WIMPs), are thought to collide and annihilate, generating heat that fuels the formation of dark stars. By studying these supermassive dark stars, researchers can glean valuable information about the properties and behavior of dark matter.

Unveiling the Nature of Dark Matter

Published in the Proceedings of the National Academy of Sciences, the research conducted by the team led by Katherine Freese brings us one step closer to unraveling the secrets of dark matter. Follow-up observations using JWST will examine the spectroscopic properties of the candidate dark stars. Variations in light intensity within specific frequency bands could serve as crucial evidence to confirm their nature.

Solving the Cosmological Conundrum

The discovery of dark stars may also help address a predicament posed by the JWST's observations: the abundance of large galaxies in the early universe seems to contradict predictions based on the standard model of cosmology. Katherine Freese suggests that instead of proposing entirely new theories, fine-tuning elements within the standard model could account for this discrepancy. The existence of dark stars, mimicking early galaxies, would align observational data with the simulations of galaxy formation.

The Radiance of Dark Stars

The three candidate dark stars identified by JWST—JADES-GS-z13-0, JADES-GS-z12-0, and JADES-GS-z11-0—were initially classified as galaxies, but they possess remarkable characteristics. A single dark star emits an intensity of light that can rival an entire galaxy of ordinary stars. Theoretically, dark stars can grow to several million times the mass of our sun and emit brightness up to 10 billion times greater. This extraordinary scale showcases the immense potential of dark stars as cosmic powerhouses.

The Genesis of Dark Star Theory

The concept of dark stars originated from a collaboration between Katherine Freese and Doug Spolyar, a former graduate student at the University of California, Santa Cruz. Curiosity surrounding the influence of dark matter on the first stars to form in the universe led to their groundbreaking work. Paolo Gondolo, an astrophysicist at the University of Utah, joined the team, and after years of development, they published their first paper on dark stars in the journal Physical Review Letters in 2008.

A Step Closer to the Truth

The research conducted by the team, including Katherine Freese, Cosmin Ilie, and Jillian Paulin ’23, sheds light on the possibility of dark stars and their link to dark matter. The implications of this discovery extend beyond astrophysics, offering valuable insights into the fundamental nature of our universe. With ongoing investigations and advancements in technology, we can anticipate the identification of more dark stars, bringing us closer to comprehending the enigma of dark matter.

The James Webb Telescope's remarkable glimpse into the potential existence of dark stars offers a glimmer of hope in our quest to understand dark matter. These theoretical objects, fueled by the annihilation of dark matter particles, could hold the key to unlocking the secrets of the universe. As researchers delve deeper into the spectroscopic properties of the candidate dark stars, we eagerly await further confirmation and the profound implications they may hold for our understanding of the cosmos. The discovery of dark stars represents a significant step forward in our ongoing exploration of the mysteries that lie beyond our visible universe.