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Hubble Confirms 'Cloud-9,' First Starless Dark-Matter Cloud Near M94

Deep Hubble imaging verified the starless nature of a radio-identified cloud, opening a new window on low-mass dark halos.

Overview

  • The object, interpreted as a Reionization‑Limited H I Cloud (RELHIC), is the first confirmed example of its kind and is reported in The Astrophysical Journal Letters with results presented at the AAS meeting.
  • Cloud‑9 lies roughly 14 million light‑years away on the outskirts of the spiral galaxy Messier 94 and appears physically associated with that system based on radio mapping.
  • Hubble’s Advanced Camera for Surveys found no stars within the VLA‑defined region, ruling out even an ultra‑faint dwarf and confirming the cloud is truly starless.
  • Radio measurements indicate a neutral hydrogen core about 4,900 light‑years across containing ~1 million solar masses of H I, implying an enclosing dark‑matter halo of ~5 billion solar masses.
  • First flagged by FAST and confirmed with the Green Bank Telescope and the VLA, Cloud‑9 provides a testbed for models of failed galaxy formation, and researchers say deeper surveys could uncover more such relics.