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A Blob and a Star

Photo credit: www.astronomy.com

A Glimpse into the Cosmos: The Globular Cluster M68 and Variable Star HD 109799

In the fascinating realm of astronomy, numerous objects captivate the attention of both amateur stargazers and seasoned astrophysicists alike. One such pair is the globular cluster M68 located in the constellation Hydra, which appears adjacent to the variable star HD 109799. The following exploration delves into these celestial phenomena, underscoring their significance in our understanding of the universe.

The Celestial Bodies at Play

M68 is a stunning globular cluster positioned in the lower left quadrant of the image. Globular clusters are dense collections of stars that orbit galaxies, often appearing as bright, spherical groups. These clusters are typically very old, giving astronomers vital clues about the early stages of star formation and galactic evolution.

Contrasting with M68, the variable star HD 109799 occupies the upper right corner of the image. Notably, in the year 2021, researchers established HD 109799’s classification as a member of the γ Doradus variable stars. This group is characterized by unique pulsating properties, where the changes in brightness are influenced by gravity-induced waves, reminiscent of undulating patterns on a water surface.

Significance of the γ Doradus Stars

The classification of HD 109799 as a γ Doradus star provides insights into stellar behavior and structure. These stars typically exhibit periodic brightness changes due to pulsations in their outer layers. Studying such variability enhances our comprehension of stellar mechanics and the underlying physics governing such pulsations, revealing the intricacies of stellar lifecycles.

Observational Opportunities

For astronomy enthusiasts interested in observing these remarkable celestial bodies, M68 and HD 109799 offer a spectacular view with the right equipment. Even amateur astronomers can capture images of these objects through the use of telescopes equipped with suitable filters and detectors.

The findings regarding the population and characteristics of stars within the M68 cluster, along with the properties of HD 109799, continue to enrich our understanding of the cosmos, emphasizing the ongoing quest for knowledge in the field of astronomy.

Source
www.astronomy.com

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