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Supermassive Dark Star candidates seen by JWST.

Proceedings of the National Academy of Sciences of the United States of Americaยท2023
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Related Experiment Video

Updated: Jan 16, 2026

Identification of Metal Oxide Nanoparticles in Histological Samples by Enhanced Darkfield Microscopy and Hyperspectral Mapping
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Spectroscopic Supermassive Dark Star candidates.

Cosmin Ilie1, Sayed Shafaat Mahmud1, Jillian Paulin2

  • 1Department of Physics and Astronomy, Colgate University, Hamilton, NY 13346.

Proceedings of the National Academy of Sciences of the United States of America
|September 30, 2025
PubMed
Summary
This summary is machine-generated.

Early stars powered by dark matter (DM), known as Dark Stars (DSs), are analyzed using JWST data. Two candidates, JADES-GS-z11-0 and JADES-GS-z13-0, are spectroscopically consistent with DSs, with two new candidates identified.

Keywords:
Dark MatterJames Webb Space Telescopecosmologyhigh-z galaxiesstars

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Area of Science:

  • Astronomy and Astrophysics
  • Cosmology
  • Early Universe Studies

Background:

  • Dark Stars (DSs) are hypothetical early stars powered by dark matter (DM) annihilation or decay.
  • Previous research identified three photometric DS candidates (JADES-GS-z11-0, JADES-GS-z12-0, JADES-GS-z13-0) in 2023.
  • Understanding DSs is crucial for comprehending the early universe and galaxy formation.

Purpose of the Study:

  • To spectroscopically confirm or refute the DS interpretation of previously identified candidates.
  • To search for new DS candidates using JWST data.
  • To investigate potential environmental influences on DS formation and evolution.

Main Methods:

  • Follow-up spectroscopic analysis of photometric DS candidates using Near-Infrared Spectrograph (NIRSpec) on the James Webb Space Telescope (JWST).
  • Identification and analysis of spectral features, including He II absorption lines.
  • Cross-correlation with other observational data, such as Atacama Large Millimeter/submillimeter Array (ALMA) data.

Main Results:

  • JADES-GS-z11-0 and JADES-GS-z13-0 show spectroscopic consistency with a Dark Star interpretation.
  • Two new spectroscopic DS candidates, JADES-GS-z14-0 and JADES-GS-z14-1, were identified.
  • JADES-GS-z14-0 exhibits a tentative He II absorption line, a potential DS signature, and is the second most distant luminous object observed.
  • ALMA data suggests JADES-GS-z14-0 might be in a metal-rich environment, challenging the isolated DS model.

Conclusions:

  • Spectroscopic data supports the Dark Star hypothesis for JADES-GS-z11-0 and JADES-GS-z13-0.
  • The potential detection of a He II absorption line in JADES-GS-z14-0 is a significant finding.
  • The potential embedding of JADES-GS-z14-0 in a metal-rich environment necessitates theoretical revisions of Dark Star formation and evolution models.