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| A field of space with a dozen white foreground stars and a number of small, yellow background galaxies. [Image Credit: NASA, ESA, D. Li (Utoronto), Image Processing: J. DePasquale (STScI)] |
Astronomers using the Hubble Space Telescope have discovered a galaxy, dubbed Candidate Dark Galaxy-2 (CDG-2), located about 300 million light-years away, that appears to be composed of at least 99.9% dark matter. This makes it one of the most extreme examples of a dark-matter-dominated galaxy ever observed.
Key Facts About CDG-2
- Discovery Tool: Hubble Space Telescope
- Distance: ~300 million light-years from the Earth
- Composition: At least 99.9% dark matter, with vanishingly few visible stars
- Detection Method: Identified through the presence of four globular clusters orbiting an otherwise invisible mass
- Visibility: Nearly invisible in optical wavelengths
Why This Matters
- Dark Galaxies: CDG-2 is a strong candidate for the long-hypothesized class of “dark galaxies.”
- Cosmological Significance: Dark matter outweighs normal matter in the universe by about 5-to-1.
- Scientific Opportunity: Studying CDG-2 could help astronomers understand galaxy formation when star birth is suppressed.
Comparison: Typical Galaxy vs. CDG-2
| Feature | Typical Spiral Galaxy (e.g., Milky Way) | CDG-2 (Candidate Dark Galaxy) |
|---|---|---|
| Dark Matter Fraction | ~85–90% | ~99.9% |
| Visible Stars | Hundreds of billions | Almost none (detected via clusters) |
| Detection Method | Direct observation of stars & gas | Indirect, via globular clusters |
| Brightness | High, easily visible | Extremely faint, nearly invisible |
Challenges & Open Questions
- Verification: Further observations needed, possibly using radio telescopes or gravitational lensing.
- Formation Myst ery: Why did CDG-2 fail to form stars?
- Implications: More galaxies like CDG-2 could reshape our understanding of cosmic structure.


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