'The Crib' is among the nearest open clusters to Earth. It is visible to the naked eye as a faint nebulous spot of apparent fourth magnitude. However, to discern its individual stars, one needs binoculars at the very least. It's interesting to note that 'The Crib' was among the first celestial objects to be studied through an instrument. Galileo, using his telescope in 1609, was able to distinguish approximately 40 stars in this cluster.
Of course, 'The Crib' contains far more stars than what Galileo observed back in the 17th century. Recent estimates suggest that the cluster is home to just over a thousand stars. These include 68 percent red dwarfs, 30 percent solar-type stars of classes F, G, and K, and the remaining 2 percent are bright A-type stars. The estimated total mass of this cluster is approximately 500-600 times that of the sun.
With an estimated age of around 600-700 million years, 'The Crib' has already witnessed the life cycle of its most massive stars. These O and B spectral type stars have either exploded into supernovae or transformed into white dwarfs, some of which have indeed been identified within the cluster itself.
Credit: Rolando Ligustri.
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