Binary-pulsar periastron advance Created 2026-10-18 Updated 2026-11-05
Binary-pulsar periastron advance is the gradual rotation of the orbit's argument of periapsis . A closed Kepler orbit has a fixed direction of closest approach. In general relativity, the leading conservative correction makes the relative orbit precess even before gravitational radiation causes appreciable binary-pulsar orbital decay.
For nonspinning point masses , total mass , semimajor axis of the relative orbit and orbital eccentricity , the first post-Newtonian advance per orbit is
Divide by the orbital period and use Kepler's third law , where , to obtain
Here is in radians per unit time. The expansion assumes .
A pulsar acts as an orbital clock: the timing delay changes as the eccentric orbit turns relative to the line of sight. If this measured advance is dominated by the relativistic point-mass term, then determine the total mass , independently of the unknown orbital inclination. They do not separately determine both component masses. A second effect, such as the binary-pulsar Einstein delay, supplies another mass relation; additional timing parameters can then test the theory instead of merely fitting it.[ref]
Spin-induced quadrupoles, tidal deformation and higher relativistic orders can contribute in other regimes and must be modeled before interpreting all observed precession as this term. At , a separate periastron direction is undefined. Advance of this direction is conceptually distinct from decreasing : conservative precession by itself is not evidence of radiated orbital energy.
PSR B1913+16 2026-10-18
Russell Alan Hulse and Joseph Hooton Taylor Jr. discovered this binary pulsar at Arecibo in 1974; their January 1975 paper reports a roughly pulse period and orbital period. Its unseen companion was not detected as a second radio pulsar. Discovery of the orbit preceded the later binary-pulsar orbital decay test.[ref]
The 1993 Nobel Prize in Physics recognized the discovery.[ref]
By 1993, the system was interpreted as a pair of neutron stars.[ref]