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Home Astronomy

Very Massive Telescope snaps beautiful shot of Milky Method’s star-studded core (photograph)

February 20, 2024
in Astronomy
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Very Massive Telescope snaps beautiful shot of Milky Method’s star-studded core (photograph)
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A brand new view from the European Southern Observatory’s (ESO) Very Massive Telescope (VLT) captures the ample star-forming area on the middle of the Milky Method. 

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The VLT, situated in Chile’s Atacama Desert, snapped an infrared picture of a area known as Sagittarius C (Sgr C), which is situated about 300 light-years from the Milky Method’s central supermassive black gap, Sagittarius A*. Sgr C is dwelling to a whole bunch of hundreds of stars, numerous that are seen within the newly launched picture. 

“The middle of the Milky Method is probably the most prolific star-forming area in your entire galaxy,” ESO officers mentioned in a statement releasing the brand new picture on Feb. 12. “Nevertheless, astronomers have solely discovered a fraction of the younger stars they anticipated right here.” 

Associated: Superb house views by ESO’s Very Massive Telescope (pictures)

Much more stars born are believed to be situated on this area, which is a prolific stellar nursery. Nevertheless, clouds of mud and fuel block the starlight and obscure our view, based on the assertion. 

“There may be ‘fossil’ proof that many extra stars have been born within the latest previous than those we truly see,” ESO officers mentioned within the assertion. “It’s because trying in the direction of the middle of the galaxy will not be a simple job.”

Utilizing the HAWK-I infrared digital camera on the VLT, astronomers have been capable of peer by way of these clouds to see the densely packed star inhabitants of Sgr C. The VLT information revealed a chemical composition that means this area of the Milky Method is a promising candidate for internet hosting newly shaped stars. 

In truth, a latest research, published Jan. 23 within the journal Astronomy & Astrophysics, discovered that Sgr C was a lot richer in younger stars than different areas close to the galactic middle. This may assist astronomers establish new areas during which to search for different obscured younger stars, based on the assertion. 



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