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Hubble Confirms 'Cloud‑9' as a Starless Dark‑Matter Halo Near M94

The finding points to a long‑predicted RELHIC, providing a rare test of how small halos fail to form stars.

Overview

  • Hubble’s Advanced Camera for Surveys resolved the field and found no stars, verifying a truly starless, gas‑rich system.
  • Measurements indicate roughly 1 million solar masses of neutral hydrogen bound by about 5 billion solar masses of dark matter.
  • The compact, approximately 4,900‑light‑year H I core lies around 14 million light‑years away in the vicinity of the spiral galaxy Messier 94.
  • The work, published in The Astrophysical Journal Letters in 2025, builds on initial radio detections by China’s FAST and confirmations from the VLA and Green Bank Telescope.
  • Minor distortions in the radio gas may hint at interaction with M94, and researchers caution that finding additional RELHICs will be observationally challenging.