In a surprising discovery, astronomers have found a globular star cluster in the Andromeda galaxy that contains a record-breaking low amount of metals.
The stars in the cluster, called RBC EXT8, have on average 800 times less iron than our sun and are three times more iron-poor than the previous globular cluster record-holder. RBC EXT8 is also extremely deficient in magnesium.
The study, published October 15 in Science, was led by Søren Larsen of Radboud University in the Netherlands, working closely with three UC Santa Cruz astronomers: Jean Brodie, professor emeritus of astronomy and astrophysics at UCSC and director of the Centre for Astrophysics and Supercomputing at Swinburne University, Australia; Aaron Romanowsky, a research associate at UC Observatories and professor of astronomy at San Jose State University; and UCSC graduate student Asher Wasserman.
“I'm amazed that this remarkable star cluster was just sitting under our noses,” Romanowsky said. “It is one of the brightest clusters in the Andromeda galaxy and known for decades, yet no one had checked it out in detail. It shows how the universe still has many surprises for us to discover. It also reminds us to check our assumptions—in this case, it was assumed enough clusters had been investigated to know how anemic they can be.”
A globular cluster is a large, dense collection of thousands to millions of ancient stars that move together as a tight-knit group through a galaxy. Until now, astronomers thought large globular clusters had to contain a considerable amount of heavy elements.
“This discovery is exciting because the idea of a ‘metallicity floor’ for globular clusters, that must contain some minimum amount of heavy metals, underpinned so much of our thinking about how these very old star clusters formed in the early universe,” Brodie said. “Our finding contradicts the standard picture, and that is always fun!”
Hydrogen and helium are the two main elements created after the Big Bang. Heavier elements such as iron and magnesium formed later. Finding a massive globular cluster like RBC EXT8 that is extremely impoverished in metals defies current formation models, calling into question some of our ideas about the birth of stars and galaxies in the young universe.
“Our finding shows that massive globular clusters could form in the early universe out of gas with only a small ‘sprinkling’ of elements other than hydrogen and helium. This is surprising because such pristine gas was thought to be in building blocks too small to form such massive star clusters,” said Larsen.
The researchers observed RBC EXT8 using Keck Observatory’s High-Resolution Echelle Spectrometer (HIRES) in October of 2019. The globular cluster was not originally on the program, but the team had a couple of hours of observing time left and decided to aim the Keck I telescope at the cluster, whose stellar content had not yet been studied in detail. The team made spectroscopic observations to determine RBC EXT8’s metal content and used three archive images from CFHT to determine its size and estimate its mass. Their remarkable result came as quite a surprise.
“It is observationally challenging to obtain a detailed analysis of the chemical composition of globular clusters in the Andromeda galaxy, which is in the Northern Hemisphere of the sky,” said Brodie. “The HIRES capability at Keck is uniquely well-suited to meet this challenge.”
In the future, the researchers hope to find more “metal-lite” globular clusters and solve the mystery about their origin.
