A Chameleon Star in an Ancient Cluster ✎ express

Original: "No country for old stars -Spectroscopic confirmation of the first intermediate-age RR Lyrae in the open cluster Trumpler 5"
arXiv:2604.11955 · 2026-04-13 · arXiv non-exclusive · independent analysis · 1 min
A pulsating star poses as a contemporary of ancient suns, but it was actually born recently.

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In the open cluster Trumpler 5, where hundreds of stars move together, one star behaves like a teenager among elders. It pulsates — expanding and contracting, changing brightness every few hours. Such pulsating stars, classical Cepheids and RR Lyrae, are typically considered contemporaries of ancient globular clusters: they are over 10 billion years old. But this star, judging by its motion and chemistry, is only 2–5 billion years old.

Astronomers aimed two powerful telescopes at it, PEPSI on the Large Binocular Telescope and GHOST on the Gemini-South telescope, and captured its spectrum, like fingerprints. By measuring the star's velocity from several observations, they found it is moving at 50.57 km/s, while the cluster itself moves at 50.76 km/s. The probability of a chance coincidence is two thousandths of a percent. The star is definitely part of this family.

The star's metallicity [Fe/H] = –0.40—like its cluster neighbors. But scandium, yttrium, and barium in its atmosphere are notably deficient: scandium is four times less abundant than in the other cluster stars. The same 'depletion' is seen in isolated metal-rich RR Lyrae stars.

So, RR Lyrae stars are not always old and metal-poor. Some are born in the galaxy's disk, like our Sun, and live only a couple of billion years. This breaks the established picture: previously, one such star could date an entire cluster as ancient. Now we must be more careful — age can be deceptive.

The cluster Trumpler 5 is located in the constellation Puppis and is about 2.5 thousand light-years away. Its age is estimated at 2–5 billion years — similar to our Sun.

In Stanislaw Lem's novel 'Solaris', the planet's ocean pulsates, changing its shape, a distant metaphor for stellar pulsations.

Scientists
Emmy NoetherWolfgang PauliEnrico FermiPaul DiracFritz ZwickyChien-Shiung Wu
Concepts
young star red dwarf habitability rare earth metal red dwarf planets stellar age trappist 1 open cluster metal poor stellar population wolf rayet star red dwarf globular cluster young stellar object red giant brown dwarf desert