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{ | ||
"date": "2023-06-23T07:00:00-04:00", | ||
"title": "Hubble Glimpses a Glistening Cluster", | ||
"canonical_url": "https://www.nasa.gov/image-feature/goddard/2023/hubble-glimpses-a-glistening-cluster", | ||
"image_url": "https://www.nasa.gov/sites/default/files/thumbnails/image/hubble_ngc6544_potw2325a.jpg", | ||
"image_alt": "The view is filled with small stars, on a dark background. Stars become much denser and brighter around a core just right of center. Most of the stars are small, but some are larger with a round, brightly colored glow and four sharp diffraction spikes.", | ||
"author": "Andrea Gianopoulos" | ||
} | ||
--- | ||
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The teeming stars of the globular cluster NGC 6544 glisten in this image from the NASA/ESA [Hubble Space Telescope](/mission_pages/hubble/main/index.html). This cluster of tightly bound stars lies more than 8,000 light-years away from Earth and is, like all globular clusters, a densely populated region of tens of thousands of stars. | ||
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This image of NGC 6544 combines data from two of Hubble’s instruments, the [Advanced Camera for Surveys](/content/observatory-instruments-advanced-camera-for-surveys) and [Wide Field Camera 3](/content/observatory-instruments-wide-field-camera-3), as well as two separate astronomical observations. The first observation was designed to find a visible counterpart to the radio pulsar discovered in NGC 6544. A pulsar is the rapidly spinning remnant of a dead star, emitting twin beams of electromagnetic radiation like a vast astronomical lighthouse. This pulsar rotates particularly quickly, and astronomers turned to Hubble to help determine how this object evolved in NGC 6544. | ||
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The second observation which contributed data to this image was also designed to find the visible counterparts of objects detected at other electromagnetic wavelengths. Instead of matching up sources to a pulsar, however, astronomers used Hubble to search for the counterparts of faint X-ray sources. Their observations could help explain how clusters like NGC 6544 change over time. | ||
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_**Text credit: European Space Agency (ESA) | ||
Image credit: ESA/Hubble & NASA, W. Lewin, F. R. Ferraro**_ | ||
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#### **_Media Contact:_** | ||
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**_Claire Andreoli_** | ||
**_NASA's_** [**_Goddard Space Flight Center_**](http://www.nasa.gov/goddard), **_Greenbelt, MD_** | ||
[**_[email protected]_**](mailto:[email protected]) |