avril 19, 2025
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Hubble showed a spiral galaxy in the constellation of whale

Hubble showed a spiral galaxy in the constellation of whale


In the picture the galaxy is located “face” to the ground

Photo: ESA/Hubble & NASA, LC HO, D. Thilker

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The Hubble Space Telescope has recorded the amazing spiral galaxy of Massier 77, located in the constellation of the whale at a distance of 45 million light years from Earth.

Photo Published European Space Agency.

On it the galaxy is located « face » to us. In the center of the frame is a bright core surrounded by twisted spiral sleeves, littered with pink outbreaks of new stars and dark red dusty matter.

The atmosphere is complemented by a bright star in the lower left corner and numerous dull stars against its background.

Some dull stars can be seen around the galaxy

A large plan of spiral galaxy

Photo: ESA/Hubble & NASA, LC HO, D. Thilker

Massier 77 was first recorded in 1780 by the French astronomer Pierre Menshen. It was later included in the famous astronomer catalog – a list of objects that are easy to confuse with comets.

For a long time, scientists have considered it simply a nebula or star cluster. Only over a hundred years later it became known that it was a full -fledged galaxy, separate from the Milky Way.

Mescier 77 also has a different name – « Kalmar Galaxy ». It is caused by an unusual structure – filamentous formations that envelop the galaxy, like a tentacle. It is not only a striking visual effect, but also an example of how modern technologies allow us to open the nature of objects in the universe deeper.

A preliminary shot of a squid galaxy who made « Hubble » was published In 2013. The updated image presented by scientists today combines the latest observations with different filters and improved processing methods.

Hubble before Helped The International Astronomy Group is a breakthrough in the study of one of the most mysterious planets of the solar system – Uranus. Using the space telescope data, the researchers were able to determine with the unprecedented accuracy at what speed the inner part of the planet rotates.



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