Kepler star trio find is mystery to astroseismologists
By - - BBC NEWS SCIENCE & ENVIRONMENT WEBSITE
Added: Sat, 09 Apr 2011 17:01:59 UTC

Binary stars are well-known, but it seems these trinary systems may also be common
The graceful dance between three stars seen by the Kepler telescope has drawn the attention of astronomers because it is not accompanied by a song.
Most stars are known to generate great booming sounds in their interiors, and Kepler can spot the resulting change in the light that they emit.
However, astronomers reporting in Science say a red giant they have spotted is unexpectedly quiet.
HD181068A is orbited by two smaller, red dwarf stars that orbit each other.
The study of the sounds within stars is known as astroseismology, and a separate report in Science details the findings of more than 500 stars whose deep rumblings Kepler has measured.
As convection processes within stars move masses of material up from the core, great pressure waves - in essence, sound waves of very low frequency - are created.
As the gases are compressed and rarefied, temperature changes lead to changes in the light that escapes the stars.
The sounds within the stars, and the clues they give into the stars' makeup, can be inferred from these small changes in the "light curves" that telescopes such as Kepler measure.
Triple play But HD181068 is an unusual case - firstly because it is a "triply eclipsing" system. From Kepler's viewpoint, the two smaller binary stars pass in front of one another as they orbit each other, and they in turn pass in front of the red giant.
Just what is going on in the system can be worked out from measuring the tiny amounts of light that are blocked by each star at each stage of the trio's waltz.
It is not the first triply eclipsing system that Kepler has spotted; that honour goes to KOI 126, also reported in Science, in February.
But the red giant's silence has confounded the new study's lead author Aliz Derekas, of Eotvos University in Hungary.
"This red giant star should pulsate," she told BBC News.
"We now know all red giants show some oscillations - the surface of the star should show some waves that should be in the light curve. We can estimate the period of these oscillations, and this red giant doesn't show that period."
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