The Lost Child in the Phoenix Stellar Family ✛

Original: "Revisiting the enigmatic sixth star cluster in the Fornax dwarf spheroidal galaxy"
arXiv:2608.27270v1 · 2026-08-27 · CC BY 4.0 · 1 min
The faint cluster Fornax 6 turns out to be a true star cluster, not a random grouping of stars.

In the stellar family of the Phoenix galaxy, there are five old globular clusters, and the sixth child was long considered a foundling. The object Fornax 6 looked like a random grouping of stars, not a true family. Astronomers debated whether it had the right to be called a cluster.

New work measured the velocities and chemical composition of stars in this object. It turned out that 43 stars move together, like members of one family. Their age is about 3 billion years, which is much younger than the other Phoenix clusters. Moreover, these stars contain more heavy elements than the old clusters. This means Fornax 6 is indeed a cluster, but unusually young and metal-rich.

Fornax 6 was first noticed by Harlow Shapley in 1939 as a "very faint cluster," but it was then forgotten for a long time, considered a random grouping of stars.

Why does this matter? Previously, it was thought that all clusters in dwarf galaxies are very old and metal-poor. Fornax 6 shows that young clusters can also form in such galaxies. This will help us better understand how stellar families form in small galaxies.

Fornax 6 was first noted by Harlow Shapley in 1939 as a "very faint cluster," but was then largely forgotten, being dismissed as a random grouping of stars.

Scientists
Fritz ZwickyWilliam HerschelJan Oort
Concepts
dwarf galaxy red dwarf globular cluster trappist 1 saturn galaxy cluster galactic center large magellanic cloud exoplanets around red dwarfs sulfur stellar remnant star formation rate galactic halo composition strange quark quark star stellar age galaxy donor star young stellar object