From the October 2014 issue

Why do we see a flash instead of a constant signal from a millisecond pulsar, which spins 20-700 times per second? Is that not fast enough to maintain a steady beam of light?

Daniel Younker Minot, North Dakota
By | Published: October 27, 2014 | Last updated on May 18, 2023
X-ray millisecond pulsar
An artist’s impression of an accreting X-ray millisecond pulsar. The flowing material from the companion star forms a disk around the neutron star that is truncated at the edge of the pulsar magnetosphere.
NASA/Goddard Space Flight Center/Dana Berry
This is a good question. If we take signals from the brightest millisecond pulsars and send them to audio speakers, we hear a pure tone in the audio band and not individual pulses. So why should radio waves (or light) be any different?

The answer lies completely in the instrumentation we use. Millisecond pulsars emit beams of electromagnetic radiation as they rotate, much like lighthouses do here on Earth. The beams themselves — typically radio waves or sometimes X-rays or gamma rays — are quite narrow and last only a small fraction of one rotation. So, in principle, they really should look like pulses.

In the case of sound, our ears and minds blend those pulses together so that we perceive a tone in the same way that we hear a note and not individual vibrations of a violin string when it is played. Our eyes and minds work similarly slow and blur things out. The fastest pulsars that we could actually see pulsing (assuming they gave off optical light!) would rotate about 30 times per second — any faster and we would perceive the pulsar as simply being on all the time. The Crab Pulsar spins about 30 times per second, and some people have reported seeing it as a star that flickers in a strange way.

For scientific observations of pulsars, our instruments are specially designed to be much faster than human senses. We easily could detect the individual pulses from pulsars spinning more than a thousand times per second, assuming that the pulses were bright enough and that such rapidly rotating pulsars even exist (something I would love to prove with my own research).

Scott Ransom
National Radio Astronomy Observatory, Charlottesville, Virginia