Stellar Still Births Revealed
Researchers have discovered that brown dwarfs may well be stellar ‘miscarriages’ that should be treated as a
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separate class of celestial body in addition to stars and planets. To date, they had been merely regarded as stars which were below normal size. Brown dwarfs (BDs) are what scientists call objects which populate the galaxies apart from the stars. Unlike the latter, they cannot develop high-yield hydrogen fusion, as in the interior of our sun, due to their low mass (less than about eight percent of the sun’s mass). However, in addition to this, brown dwarfs and stars also seem to be different in their ‘mating behavior.’
Stars often occur in pairs, which dance around each other. The intimacy of this dance, however, varies a great deal. Sometimes the gap is smaller than one radius of the Earth’s orbit (also known as Astronomical Unit or AU). However, sometimes the two partners can keep apart by many thousands of AUs. “Things are different with brown dwarfs,” astrophysicist Ingo Thies of the Bonn Argelander Institute of Astronomy at the University of Bonn explains. “The orbital radiuses of BD pairs are cut off above about 15 AUs; BD pairs with greater distances are the exception.”
What is more, there are hardly any mixed pairs consisting of suns and brown dwarfs — far fewer than expected. This phenomenon is also known as brown dwarf desert. “According to the classical model there ought not to be these differences,” Professor Pavel Kroupa of the Argelander Institute explains. “According to this, both brown dwarfs and stars ought to emerge from interstellar clouds of gas which become concentrated because of the attraction of their mass. But, if this was the case, these celestial bodies should behave in similar ways.”
Despite this contradiction, the astronomic community has previously stuck to the theory of a joint origin. However, Ingo Thies and Pavel Kroupa have now shown empirically for the first time that brown dwarfs must be seen as a class of objects which is separate from the stars. “For this we analyzed the masses of newly born stars,” Ingo Thies explains. “This revealed a jump in the distribution of mass which makes the division in the stellar population apparent.”
Death of an embryonic star
But how are brown dwarfs born? As long ago as 2001, the Danish researcher Bo Reipurth, Britain’s Cathie Clarke and the Spanish astronomer Eduardo Delgado-Donate had the idea that brown dwarfs could be interpreted as stellar ‘miscarriages:’ a system consisting of three embryonic stars disintegrates due to the mutual attraction of masses, and the lightest object is catapulted out of the system. The physical mechanism itself has long been known: even the U.S. light space probes Pioneer and Voyager were hurled off onto their voyage of no return by the planet’s gravity.
Another possibility would be that brown dwarfs form in the outermost regions of emergent stars and become separated from them. This can, for example, occur as the result of a close encounter with a third star. Since almost all stars are born in star clusters, such encounters are not unusual. It is also possible that both scenarios of cosmic miscarriages take place.
Both theories predict that brown dwarfs can only emerge at the birth of stars, which is similar to the situation with planets. Thus, there are presumably three quite different celestial bodies: planets, brown dwarfs and stars.
The researchers will be publishing their results in the journal Monthly Notices of the Royal Astronomical Society.
