Hubble Uncovers Ancient Stars in NGC 2210

by Santiago Fernandez
4 comments
NGC 2210

Located in the Large Magellanic Cloud, NGC 2210 is a globular cluster that holds significant interest for astronomers. Situated about 157,000 light-years from our planet, this cluster is relatively youthful compared to the universe, at about 11.6 billion years old. It stands out for being younger than many other clusters in both the LMC and our own Milky Way galaxy. This discovery is attributed to the combined efforts of ESA/Hubble & NASA, along with researchers A. Sarajedini and F. Niederhofer.

The globular cluster NGC 2210, residing in the Large Magellanic Cloud, is a dense collection of stars offering a glimpse into the formation and age of some of the oldest stellar clusters. Its proximity to Earth, at 157,000 light-years, and its relationship as a satellite galaxy to the Milky Way, enhance its significance in astronomical studies. These clusters are known for their longevity and stability, hosting thousands to millions of stars, making them key subjects in the study of ancient star populations.

Research conducted in 2017 using data that contributed to the image of NGC 2210 revealed its age to be around 11.6 billion years, making it the youngest in its group yet still only a few billion years younger than the universe. This finding was striking, as other globular clusters in the LMC surveyed were older, with four surpassing 13 billion years. This suggests that the oldest clusters in both the LMC and the Milky Way were formed around the same time, despite the independent formation of these galaxies.

In addition to its scientific value, NGC 2210 is noted for its breathtaking beauty, densely packed with stars. The night sky viewed from a planet within this cluster would be vastly different from our own, filled with a multitude of stars, creating a stellar environment far more crowded than what we experience on Earth.

Frequently Asked Questions (FAQs) about NGC 2210

What is NGC 2210?

NGC 2210 is a globular cluster located in the Large Magellanic Cloud, about 157,000 light-years from Earth. It is noteworthy for being 11.6 billion years old, making it slightly younger than the universe and younger than many other clusters in both the LMC and the Milky Way Galaxy.

Why is NGC 2210 significant in astronomical studies?

NGC 2210 is significant because of its age, which at approximately 11.6 billion years, provides insights into the formation and evolution of some of the ancient stellar clusters. Its younger age compared to other clusters in both the LMC and Milky Way offers unique perspectives on galactic development and star formation.

How was the age of NGC 2210 determined?

The age of NGC 2210 was determined through research and data analysis, including a 2017 study that used data contributing to the imaging of this cluster. This research placed NGC 2210’s age at around 11.6 billion years, making it one of the younger clusters in the Large Magellanic Cloud.

What makes NGC 2210 visually unique?

NGC 2210 is visually striking due to its dense concentration of stars. This high density creates a stunning astronomical phenomenon, particularly when viewed from a planet within the cluster, where the night sky would appear densely packed with stars, creating a highly crowded stellar environment.

More about NGC 2210

  • ESA/Hubble & NASA
  • Large Magellanic Cloud
  • Globular Clusters
  • Stellar Formation and Evolution
  • Astronomical Research Methods

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4 comments

Alex R December 4, 2023 - 7:37 pm

should have more on the Large Magellanic Cloud itself, it’s a fascinating galaxy with lots of mysteries.

Reply
Mike Johnson December 4, 2023 - 10:32 pm

great read but the article could use more info on how they actually determine the age of these clusters

Reply
Jane Smith December 5, 2023 - 2:12 am

really interesting article on NGC 2210, didn’t know it was that old, amazing how much we can learn about the universe

Reply
Sarah K. December 5, 2023 - 6:46 am

love the visual description, it’s like I can almost see the star-packed sky from here!

Reply

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