Capotauro

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Capotauro (formally named CEERS ID U-100588) is an astronomical object detected by the James Webb Space Telescope (JWST) on the Cosmic Evolution Early Release Science (CEERS) Survey, [1] which could be an extremely distant Lyman-break galaxy with a photometric redshift (z) of 32, a dusty interloper galaxy with a redshift (z) of 6, a rogue planet or a Y2–Y3 spectral type brown dwarf.

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CEERS ID U-100588
Capotauro (astronomical object).png
Magnified image of Capotauro (CEERS ID U-100588) as observed by the JWST. Credit: G. Capriotti, G. Gandolfi et al.
Other designationsCapotauro
Observation data
(Epoch J2000)
Constellation Boötes
14h 19m 32.97s
Declination +52° 47 52.11
Redshift ~6 (dusty interloper galaxy hypothesis)
~32 (Lyman-break galaxy hypothesis)

It is characterized by a significant absence of light in certain wavelengths and a pronounced drop in others. Its paucity of light and spectral peculiarities make it an enigmatic object, defying conventional classifications and sparking debate about whether the standard cosmological model might need adjustments. [2]

The team named the mystery object after a mountain in Italy as they are based at the University of Padua. [3] Lead researcher Giovanni Gandolfi said: "Capotauro could be the farthest galaxy ever seen at a timescale that is compatible with the first stars and black holes to form in the universe". It has been compared to the hypothesised ' black hole star', which is a primordial black hole surrounded by a dense atmosphere. Other scientists have been sceptical about whether Capotauro is a galaxy however. [3]

If Capotauro is spectroscopically confirmed to be at redshift z=32, then it would have existed just 90 million years after the big bang. [4] This is nearly 200 million years before the current record holder MoM-z14 and would place Capotauro closer to the very beginning of time than any structure we have yet seen. A galaxy appearing only 90 million years after the big bang implies that current theories about how quickly structures had formed are at odds with these observations by Gandolfi and his team. However, there could be other explanations as well and the initial theory that Capotauro might be at such an extreme redshift is doubted. [4]

Capotauro appears to be very bright for a young galaxy. [5] The object's apparent luminosity implies a mass near a billion suns which is difficult to reconcile with current theories. Nicha Leethochawalit from the National Astronomical Research Institute of Thailand said "To achieve such a mass, the efficiency at which the galaxy turned gas into stars would have to be close to 100 percent", whereas an efficiency of 10-20% is thought to be more usual. Possibilities include: a black hole star, a brown dwarf, an ultra-young galaxy, a nearer dusty galaxy (or interloper) and a rogue or hostless planet. [5]

See also

References

  1. Gandolfi, G.; Rodighiero, G.; Bisigello, L.; Grazian, A.; Finkelstein, S. L.; Dickinson, M.; Castellano, M.; Merlin, E.; Calabrò, A.; Papovich, C.; Bianchetti, A.; Bañados, E.; Benotto, P.; Buitrago, F.; Daddi, E. (4 February 2025). "Ultra High-Redshift or Closer-by, Dust-Obscured Galaxies? Deciphering the Nature of Faint, Previously Missed F200W-Dropouts in CEERS". arXiv: 2502.02637v1 . Retrieved 12 October 2025.
  2. Gandolfi, Giovanni (1 September 2025). "Mysteries of Capotauro - investigating the puzzling nature of an extreme F356W-dropout". arXiv: 2509.01664v1 [astro-ph.GA].
  3. 1 2 O'Callaghan, Jonathan (25 September 2025). "Possible galaxy spotted by JWST could be the earliest we've ever seen". New Scientist . Retrieved 8 October 2025.
  4. 1 2 Morgan, Ashley (6 September 2025). "JWST May Have Just Spotted The Very First Galaxy In The Universe". Daily Galaxy. Retrieved 9 October 2025.
  5. 1 2 Ralls, Eric (12 September 2025). "Why the most distant galaxy ever seen might actually be an impostor". earth.com. Retrieved 9 October 2025.