HM Cancri
Binary star in the constellation Cancer
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Through Sun, Magnitude (astronomy) and Albert Einstein
Observations
As HM Cancri is a pair of white dwarfs, it has a relatively low optical luminosity. The 321.5 s modulation of HM Cancri was discovered serendipitously in 1999 thanks to the ROSAT mission working in the X-ray band. Optical follow-up observations with the ESO Very Large Telescope (VLT), Telescopio Nazionale Galileo (TNG) and Nordic Optical Telescope (NOT) allowed the counterpart to be identified, a relatively dim (20.7 magnitude in the B filter) object which shows an optical modulation at the same period detected in the X-ray band. The optical monitoring of the counterpart of HM Cancri during 2001-2004 clearly shows that the period is decreasing at a rate of about 1/1000 s each year. This result was confirmed by monitoring the source in the X-rays for several years.
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Relation to general relativity
The decreasing separation of the components of the system means that the system is losing orbital energy. Albert Einstein's theory of General Relativity predicts such a system will lose orbital energy through the generation of gravitational waves. Scientists believe that HM Cancri may be one of the strongest sources of gravitational waves in the Milky Way galaxy.

