Globular Cluster NGC 6569: An Astronomical Treasure Trove | Hubble
Globular clusters are stable, tightly bound clusters containing tens of thousands to millions of stars, and are associated with all types of galaxies. The intense gravitational attraction of these closely packed clusters of stars means that globular clusters have a regular spherical shape with a densely populated center—as can be seen in the heart of this star-studded image.
This observation comes from an investigation of globular clusters which lie close to the center of the Milky Way. These objects have been avoided in previous surveys, as the dust spread throughout the center of our galaxy blocks light from these globular clusters and alters the colors of the stars residing in them. The last factor is particularly important for astronomers studying stellar evolution, as the colors of stars can give astronomers insights into their ages, compositions, and temperatures.
The astronomers who proposed these observations combined data from Hubble with data from astronomical archives, allowing them to measure the ages of globular clusters including NGC 6569. Their research also provided insights into the structure and density of globular clusters towards the center of the Milky Way.
Credit: ESA/Hubble & NASA, R. Cohen
Release Date: June 27, 2022
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