Star
WOH G64
Also IRAS 04553-6825
A huge star in the Large Magellanic Cloud wrapped in a cocoon of dust, long classed as a red supergiant. What it is now is argued over.
Measured
- Distance
- 161,700 light-years
- Constellation
- Dorado
- Position (J2000)
- RA 4h 55m 11s, Dec −68.34°
How far, from the Sun
162,000 light-years. To cross it:
- Light162,000 years
- Voyager 1's speed2.87 billion years
- Driving at 100 km/h1.75 trillion years
Voyager 1 at the speed it moved outward over the year to 2026-10-25 (JPL Horizons). Driving: nonstop, never refuelling.
Facts
- Announced in 2024, the VLT Interferometer's first close-up image of a star in another galaxy shows this one, observed in December 2020.
- Its brightness and spectrum have changed since 2011. Muñoz Sánchez and colleagues read that as a change towards a yellow hypergiant; van Loon and Ohnaka (2026) still find titanium oxide in its spectrum and call it a red supergiant. Both suggest a companion star, which others find unproven.
- It is placed at the Large Magellanic Cloud's distance, measured from eclipsing binary stars.
Where this comes from
- Placed at the Large Magellanic Cloud's distance: Pietrzyński et al. 2019, eclipsing binaries (49.59 ± 0.55 kpc)
- This research has made use of the SIMBAD database, CDS, Strasbourg, France (Wenger et al. 2000, A&AS 143, 9).
- This research has made use of the VizieR catalogue access tool, CDS, Strasbourg, France (DOI: 10.26093/cds/vizier).
Every catalogue Ouranos draws is credited on the credits page.