Using data from ESA's XMM-Newton X-ray observatory, an international group of astrophysicists has discovered a spinning neutron star that seems to be tumbling slowly - a find that could provide new insight into the evolution and structure of these super-dense objects. Spinning neutron stars, also known as pulsars, generally rotate on highly stable axes. Thanks to their periodic signals, emitted either in radio or X-ray wavelengths, they can serve as very accurate astronomical clocks. Regarding pulsar RX J0720.4-3125, however, the team found that over the past four and a half years, its temperature has been rising - until very recently,...