• Recently, in the first-ever comprehensive analysis of blue stragglers, Indian researchers have proposed a hypothesis for evolution of blue straggler stars.
  • Blue stragglers is a class of stars on open or globular clusters that stand out as they are bigger and bluer than the rest of the stars.

Important points:

  • These are unusually hot and bright stars found in the cores of ancient star clusters known as globulars.
  • A clue to their origin is that they are only found in dense stellar systems, where distances between stars are extremely small (a fraction of a light year).
  • Allan Sandage (an astronomer with Carnegie Observatories in Pasadena, California) discovered blue stragglers in the globular cluster M3 in 1952-53.
  • Most are located at least several thousand light-years away from the sun, and most are around 12 billion years old or more.
  • The Milky Way’s largest and brightest globular is Omega Centauri.
  • Blue straggler stars appear to violate standard theories of stellar evolution.
  • A bunch of stars born at the same time from the same cloud form a star cluster. Star formation happens in interstellar molecular clouds: opaque clumps of very cold gas and dust.
  • Under standard stellar evolution, as time passes, each star evolves differently depending on its mass, in which all stars born at the same time should lie on a clearly defined curve in the Hertzsprung-Russell diagram.
  • Hertzsprung-Russell diagram plots the temperature of stars against their luminosity or the colour of stars against their absolute magnitude. It shows a group of stars in various stages of their evolution.
  • By far the most prominent feature is the main sequence, which runs from the upper left (hot, luminous stars) to the bottom right (cool, faint stars) of the diagram.
  • In case of blue straggler, they evolve and move off the main sequence creating a bend in their track, known as the turnoff.
  • Since blue stragglers often lie well off this curve, they may undergo abnormal stellar evolution.
  • They appear to be lagging behind most of the other stars in the cluster in its evolution toward a cooler, reddish state.


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