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Affichage des articles dont le libellé est ASTRONOMY - M27: The Dumbbell Nebula. Afficher tous les articles
Affichage des articles dont le libellé est ASTRONOMY - M27: The Dumbbell Nebula. Afficher tous les articles

30/05/2023

ASTRONOMY - M27: The Dumbbell Nebula

 2023 May 30

An expansive interstellar gas cloud is shown with an orange
interior and outer blue filaments. Many stars are visible in
the dark background. 
Please see the explanation for more detailed information.

M27: The Dumbbell Nebula
Image Credit & Copyright: Patrick A. Cosgrove

Explanation: Is this what will become of our Sun? Quite possibly. The first hint of our Sun's future was discovered inadvertently in 1764. At that time, Charles Messier was compiling a list of diffuse objects not to be confused with comets. The 27th object on Messier's list, now known as M27 or the Dumbbell Nebula, is a planetary nebula, one of the brightest planetary nebulae on the sky and visible with binoculars toward the constellation of the Fox (Vulpecula). It takes light about 1000 years to reach us from M27, featured here in colors emitted by sulfur (red), hydrogen (green) and oxygen (blue). We now know that in about 6 billion years, our Sun will shed its outer gases into a planetary nebula like M27, while its remaining center will become an X-ray hot white dwarf star. Understanding the physics and significance of M27 was well beyond 18th century science, though. Even today, many things remain mysterious about planetary nebulas, including how their intricate shapes are created.

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