Three years of staring lets scientists capture a neutron star “glitch”
The same magnetic fields that power the pulsar produce a bit of drag
as they sweep across the environment, gradually slowing the pulsar down.
And theorists have proposed that neutron stars can “glitch,”
experiencing a sudden speed-up. This occurs due to movement in the
star’s interior, which can exchange momentum between the superfluid
there and the crust surrounding it. Until now, however, our
understanding of glitches had remained limited to theory.
To understand glitches, a team of astronomers arranged to track the Vela pulsar for a period of three years using two radio telescopes (the Mount Pleasant observatory in Tasmania and the Ceduna Observatory
in Australia. During those three years, the astronomers observed a
grand total of one glitch. In a first, they managed to catch both the
glitch and every pulse that surrounded it, along with the polarization
of the light in each pulse.
The event lasted just a fraction of a second and was presaged by a
weak and very broad pulse. Ninety milliseconds later, when the next
pulse was expected to arrive, nothing happened. The next few pulses were
weak and had little indication of the strong polarization that was seen
in the pulses that arrived before the glitch. Checking through 100,000
pulses that were recorded during their observations showed there was
nothing like this behavior in the records.