Celestial hemisphere:  Northern  ·  Constellation: Orion (Ori)  ·  Contains:  The star Betelgeuse (αOri)
Betelgeuse, Bruce Rohrlach
Betelgeuse
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Betelgeuse

Betelgeuse, Bruce Rohrlach
Betelgeuse
Powered byPixInsight

Betelgeuse

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On Sunday night I imaged Betelgeuse (9th brightest star in the night sky) with the Newtonian. A pulsating red supergiant in Orion, Betelgeuse, and its neighbour Bellatrix, define the shoulders of Orion. It is thought to be a runaway star from the Orion OB1 group.

The life of Betelgeuse is one of: Live fast, die young and go out with a bang. High mass stars like Betelgeuse are very short-lived due to their rapid stellar evolution. Betelgeuse may only be ~6 million years old and is in the final million years of it's life. Compare this to the 4.6 billion year age of the sun.

Betelgeuse has a diameter that, if in place of our sun, would reach the orbit of Jupiter. Despite being mass-equivalent of 15-20 solar masses, it's extraordinary size (capable of containing 1.6 billion solar volumes) means its average density is less than the earth's atmosphere. Most of this star is so tenuous that Betelgeuse has often been called a "red-hot vacuum".

Currently, internal radiation pressure is expanding the star by counteracting the inward pull of gravity. In a relatively short period (estimates range from 100,000 to a million years for this rapidly evolving star) when its hydrogen fuel in the core runs out, outward radiation pressure will decrease and the star will implode before rebounding as a Type II supernova. Consensus is that whilst it would not pose a hazard to earth it would likely, for a period of a few months, outshine the moon and be visible during the day.

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Betelgeuse, Bruce Rohrlach