With the help of Zwicky Transient Facility (ZTF), at the California Institute of Technology, the students spent a night scanning the sky and discovering any unusual movement of the planets or stars. In this research, Kevin Burdge, the Caltech graduate student after combining months of ZTF data noticed an unique blinking pattern. He found that this pattern is created by a pair of white dwarfs.
The pair known as ZTF 1539+5027, create an orbit around each other and are roughly Earth sized. One is found to be a bit smaller and brighter than the other. It seems like the pair is blinking when the dimmer star passes in front of brighter star creating an eclipse. This pair has been found to be second fastest pair of orbiting white dwarfs.
Burdge told Space.com, “Scientists continue to debate over whether binary systems like this will eventually merge, with one of the dead stars consuming the other or if they remain with both bodies in orbit around one another.” He further added, “The gravitational waves they emit might cause them to merge in about 2,00,000 years.
However, it is expected that in 1,00,000 years, the star with smaller size shall start dumping matter over the larger star a process that stabilizes its orbit and prevent it from shrinking further, Burdge said. He also said, the slightly smaller and brighter star is unusually hot of around 50,000 Kelvin (about 90,000 degrees Fahrenheit or 49,982 degrees Celsius) i.e. approx 10 times hotter than the sun.
This pair has been identified as sources of gravitational waves that will be picked up by the future European space mission Laser Interferometer Space Antenna (LISA), which is scheduled to be launched in 2034.
This study, titled “General relativistic orbital decay in a seven minute orbital period eclipsing binary system” shall appear in July 25 issue of the Journal Nature.
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