R136a1: The Most Massive and Luminous Blue Hypergiant Star

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SUMMARY

R136a1 is the most massive star known, with an estimated mass of 265 solar masses and a luminosity of 8,700,000 times that of the Sun. This blue hypergiant star, part of the R136 super star cluster in the Tarantula Nebula, has been losing mass at a rate of 50 solar masses every few million years due to violent outbursts. The mass determination was conducted by astronomers at the University of Sheffield using the Very Large Telescope in Chile and data from the Hubble Space Telescope.

PREREQUISITES
  • Understanding of stellar classification, specifically blue hypergiants
  • Familiarity with the Eddington limit and its implications for stellar evolution
  • Knowledge of mass measurement techniques in astrophysics, including the use of telescopes
  • Awareness of the Tarantula Nebula and its significance in astronomy
NEXT STEPS
  • Research the characteristics and lifecycle of blue hypergiant stars
  • Explore the methods used for mass determination in stars, focusing on Very Large Telescope and Hubble Space Telescope data
  • Investigate the dynamics of super star clusters, particularly R136
  • Learn about the implications of mass loss in massive stars and its effects on stellar evolution
USEFUL FOR

Astronomers, astrophysics students, and anyone interested in stellar evolution and the characteristics of massive stars.

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R136a1, is a blue hypergiant star

Wikipedia said:
R136a1, is a blue hypergiant star, currently on record as the most massive star known, with an estimated 265 solar masses. The star also holds the record for the most luminous at 8,700,000 times the luminosity of the Sun. Like other hypergiant stars that sit above the Eddington limit, R136a1 has been shedding large portions of its own mass in violent outbursts. It is estimated that at its birth the star held 320 solar masses and has been losing 50 solar masses every few million years. It is a member of R136, a Super star cluster near the center of the 30 Doradus complex (also known as the Tarantula Nebula), in the Large Magellanic Cloud. The mass of the star was determined by astronomers at the University of Sheffield using Very Large Telescope in Chile and data from the Hubble Space Telescope.

Reference:
http://en.wikipedia.org/wiki/R136a1
 
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