A Binary Pulsar in a 53-minute Orbit.

Spider pulsars are neutron stars that have a companion star in a close orbit. The companion star sheds material to the neutron star, spinning it up to millisecond rotation periods, while the orbit shortens to hours. The companion is eventually ablated and destroyed by the pulsar wind and radiation1,2 . They are key for studying the evolutionary link between accreting X-ray pulsars and isolated millisecond pulsars, pulsar irradiation effects, and the birth of massive neutron stars3-6 . Black widow pulsars in extremely compact orbits (as short as 62 minutes7 ) have companions with masses ≪ 0.1 M⊙ . They may have evolved from redback pulsars with companion masses ~ 0.1 - 0.4 M⊙ and orbital periods less than one day8 . If true, then there should be a population of millisecond pulsars with moderate mass companions and very short orbital periods9 , but hitherto no such system was known. Here we report radio observations of the binary millisecond pulsar PSR J1953+1844 (M71E) that show it to have an orbital period of 53.3 minutes and a companion with a mass of ~ 0.07 M⊙ . It is a faint X-ray source, and located 2.5 arcminutes from the center of the globular cluster M71.