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M27 - The Dumbbell Nebula, Sarah Mathews
M27 - The Dumbbell Nebula
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M27 - The Dumbbell Nebula

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M27 - The Dumbbell Nebula, Sarah Mathews
M27 - The Dumbbell Nebula
Powered byPixInsight

M27 - The Dumbbell Nebula

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Description

Stellar Metamorphosis & The Fox
Nestled some 1,200 light-years away in the constellation Vulpecula, Latin for “little fox”, the remains of what was once a main sequence star, vibrantly glows in a final farewell.

M27, the Dumbbell Nebula, bears the ever-expanding markings of its progenitor star’s gaseous outer layers that were shelled off when it grew to a red giant, as it could no longer fuse hydrogen into helium. A marked point in a star of this size’s life cycle that signals a new chapter. One that we see now as a planetary nebula where the remaining core in a final battle with gravity, contracted into a dense, white dwarf star. The white dwarf sits center stage amidst what was once its own; still able to radiate enough energy to excite and illuminate the central knots and dumbbell-like clouds of gases that spans 2 light-years across, or about half the distance from our Sun to its nearest stellar neighbor, Alpha Centauri. 

Each planetary nebulae provides valuable insight by revealing what other stars are composed of. M27 contains several different types of gases, two of which seen here are hydrogen and oxygen. 

Eventually, the gas will expand so far outward that the nebula as we know it will fade and the gases will take part in a new celestial lifecycle.

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M27 - The Dumbbell Nebula, Sarah Mathews