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Affichage des articles dont le libellé est ASTRONOMY - M41: The Little Beehive Star Cluster. Afficher tous les articles
Affichage des articles dont le libellé est ASTRONOMY - M41: The Little Beehive Star Cluster. Afficher tous les articles

25/02/2025

ASTRONOMY - M41: The Little Beehive Star Cluster

2025 February 25
A starscape is shown with red filaments running 
diagonally from the lower left to the upper right.
Many bright blue stars are visible across the center
of the frame. 
Please see the explanation for more detailed information.

M41: The Little Beehive Star Cluster
Image Credit & Copyright: Xinran Li

Explanation: Why are there so many bright blue stars? Stars are usually born in clusters, and the brightest and most massive of these stars typically glow blue. Less-bright, non-blue stars like our Sun surely also exist in this M41 star cluster but are harder to see. A few bright orange-appearing red giant stars are visible. The red-light filaments are emitted by diffuse hydrogen gas, a color that was specifically filtered and enhanced in this image. In a hundred million years or so, the bright blue stars will have exploded in supernovas and disappeared, while the slightly different trajectories of the fainter stars will cause this picturesque open cluster to disperse. Similarly, billions of years ago, our own Sun was likely born into a star cluster like M41, but it has long since drifted apart from its sister stars. The featured image was captured over four hours with Chilescope T2 in Chile

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