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APOD: 2025 February 25 B M41: The Little Beehive Star Cluster
<< Yesterday 25.02.2025
APOD: 2025 February 25 B M41: The Little Beehive Star Cluster
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.

<<  Fevral'    
Pn Vt Sr Cht Pt Sb Vs
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1995   1996   1997   1998
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2011   2012   2013   2014
2015   2016   2017   2018
2019   2020   2021   2022
2023   2024   2025  
Yanvar'
Fevral'
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Aprel'
Mai
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Avgust
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Authors & editors: Robert Nemiroff (MTU) & Jerry Bonnell (USRA)
NASA Web Site Statements, Warnings, and Disclaimers
NASA Official: Jay Norris. Specific rights apply.
A service of: LHEA at NASA / GSFC
& Michigan Tech. U.

Based on Astronomy Picture Of the Day
Publikacii s klyuchevymi slovami: stars - open cluster
Publikacii so slovami: stars - open cluster
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