“This result marks one of the cleanest and strongest detections of the effect of gravitational waves,” said Warren Brown of the Smithsonian Astrophysical Observatory (SAO).
The team discovered the white dwarf pair last year — white dwarfs are the remnant cores of stars like our Sun. The system, called SDSS J065133.338+284423.37 (J0651 for short), contains two white dwarf stars so close together — one-third of the Earth-Moon distance — that they make a complete orbit in less than 13 minutes.
“Every six minutes, the stars in J0651 eclipse each other as seen from Earth, which makes for an unparalleled and accurate clock some 3,000 light-years away,” said J.J. Hermes of the University of Texas at Austin.
Einstein’s general theory of relativity predicts that moving objects create subtle ripples in the fabric of space-time, called gravitational waves. Gravitational waves should carry away energy, causing the stars to inch closer together and orbit each other faster and faster. The team was able to detect this effect in J0651.
“Compared to April 2011 when we discovered this object, the eclipses now happen six seconds sooner than expected,” said Mukremin Kilic from the University of Oklahoma.
“This is a general relativistic effect you could measure with a wrist watch,” said SAO’s Warren Brown.
J0651 will provide an opportunity to compare future direct, space-based detection of gravitational waves with those inferred from the orbital decay, providing important benchmark tests of our understanding of the workings of gravity.
The team expects that the period will shrink more and more each year, with eclipses happening more than 20 seconds sooner than otherwise expected by May 2013. The stars will eventually merge in 2 million years. Future observations will continue to measure the orbital decay of this system as scientists attempt to understand how tides affect the merger of such stars.