Wow, what a beauty! While we’ve all turned our attentions to the new James Webb Space Telescope, this image proves Hubble has still has got it where it counts.
This new image from the Hubble Space Telescope shows the heart of the globular cluster NGC 6638 in the constellation Sagittarius. This star-studded cluster contains tens of thousands to millions of stars, all tightly bound together by gravity. Globular clusters have a higher concentration of stars towards their centers, and this observation highlights that density.
This image was taken with Hubble’s Wide Field Camera 3 and the Advanced Camera for Surveys.
Like so many things that Hubble has observed since it launched to space in 1989, this venerable telescope has revolutionized the study of globular clusters. With its instruments and clear vision above Earth’s atmosphere, Hubble has been able to study what kind of stars make up globular clusters, how they evolve, and the role of gravity in these dense systems.
What Hubble Has Shown Us About Globular Clusters
Globular clusters are found in nearly all galaxies. They are the largest and most massive type of star clusters, and they tend to be older and denser than open clusters. From Hubble, we’ve learned that the typical distance between stars in a globular cluster is about one light year. But at the central core of a cluster where the concentration of stars is the highest, the distance there between stars averages about a third of a light year, or thirteen times closer than Proxima Centauri is to our Sun.
The Milky Way has more than 150 known globular star clusters, but with Hubble and now JWST, both telescopes will continue to search for more that may be out there and tell us more about these ancient beauties.
You can find zoomable versions of this image here, as well as larger versions and wallpaper downloads.