Black Holes, Pulsars & Quasars · Constellation Vulpecula

PSR B1919+21

Reference data for PSR B1919+21: 1.3373-second spin period, 1967 Cambridge discovery by Jocelyn Bell Burnell, and radio pulsar properties.

Right Ascension (J2000.0)19h 21m 44.81s
Declination (J2000.0)+21° 53′ 02.2″
Primary ClassificationCanonical Radio Pulsar
Best Observing SeasonSummer to Early Autumn (July–October)

Provenance-Backed Scientific Measurements

Every measurement below preserves its unit, uncertainty interval, observational method, reference epoch, quality status, and primary catalog source. See Uncertainty & Provenance for how competing measurements are handled.

Astrometric, Photometric, and Physical Parameters for PSR B1919+21
ParameterValueUncertaintyMethod & EpochQuality StatusSource Archive
Distance2300 ly± 400 lyEstimated from dispersion measure DM = 12.44 pc/cm³ and galactic electron-density models.high-confidenceSIMBAD Astronomical Database (CDS)
Spin Period0.000015478 d± 1e-9 dBarycentric rotation period of 1.337302 seconds.definitiveSIMBAD Astronomical Database (CDS)
Estimated Mass1.4 M☉± 0.15 M☉Dynamical binary mass function or relativistic Shapiro delaymodel-dependentSIMBAD Astronomical Database (CDS)
Proper Motion (RA)17 mas/yr± 4 mas/yrMulti-epoch VLBI or Gaia DR3 astrometryhigh-confidenceSIMBAD Astronomical Database (CDS)
Proper Motion (Dec)32 mas/yr± 6 mas/yrMulti-epoch VLBI or Gaia DR3 astrometryhigh-confidenceSIMBAD Astronomical Database (CDS)
Characteristic Age0.0157 Gyr± 0.001 GyrMagnetic dipole spin-down characteristic agehigh-confidenceSIMBAD Astronomical Database (CDS)
Measurement Uncertainties & Competing Solutions: The first pulsar ever discovered, identified in November 1967 by Jocelyn Bell Burnell and Antony Hewish as a 1.337-second periodic radio source in Vulpecula. Estimated from dispersion measure DM = 12.44 pc/cm³ and galactic electron-density models. Barycentric rotation period of 1.337302 seconds.

J2000 Equatorial Sky Chart & Culmination Altitude

The chart below plots PSR B1919+21 (CP 1919) — First Known Pulsar at RA 19h 21m 44.81s, Dec +21° 53′ 02.2″ within Vulpecula, alongside peak meridian transit altitudes for 40°N and 30°S observers. Use the RA/Dec Coordinate Converter to compute exact culmination altitude for your latitude.

J2000 Equatorial Sky Position (Vulpecula) +90° 0° −90° 24h 12h RA 0h Peak Meridian Altitude 72° 40°N Lat 38° 30°S Lat RA: 19h 21m 44.81s Dec: +21° 53′ 02.2″ Epoch: J2000.0 First-party vector diagram derived from IAU / CDS SIMBAD / Gaia DR3 astrometry.

Astrophysical Context & Structure

In late 1967, graduate student Jocelyn Bell (now Jocelyn Bell Burnell) was analyzing miles of paper chart-recorder rolls from the 81.5-megahertz Interplanetary Scintillation Array near Cambridge, England, when she noticed a quarter-inch patch of 'scruff' that reappeared every sidereal day at right ascension 19h 19m in Vulpecula. High-speed recordings on November 28, 1967, resolved the signal into a train of sharp radio pulses repeating with clockwork precision every 1.33730 seconds. Jokingly dubbed 'LGM-1' (Little Green Men-1) before three more pulsars were found across the sky, the source was cataloged as CP 1919 (Cambridge Pulsar 1919) and proved the existence of rapidly rotating magnetized neutron stars.

PSR B1919+21 is a middle-aged canonical radio pulsar with a characteristic spin-down age near 15.7 million years and a surface dipole magnetic field of roughly 1.4 trillion gauss. Located about 2,300 light-years away, its radio emission displays classic 'drifting subpulses'—individual sub-components within the 40-millisecond pulse window that march systematically in phase from pulse to pulse as plasma carousels circulate above the neutron star's magnetic polar cap.

Beyond transforming relativistic astrophysics, the stacked radio pulse profile of CP 1919 published in the 1970 Cambridge Encyclopedia of Astronomy became one of the most recognizable graphics in popular culture when graphic designer Peter Saville featured it on the cover of Joy Division's 1979 debut album Unknown Pleasures.

Practical Visual Observing Guide

Minimum InstrumentRadio, X-ray, or large-aperture professional optical/IR instrumentation
Recommended MagnificationMulti-wavelength astrophysical reference target
Best Evening SeasonSummer to Early Autumn (July–October)
  • Emits exclusively in radio waves and weak X-rays; no optical counterpart is visible in amateur or mid-sized professional telescopes.
  • Its 1.337-second pulse period and 40 ms pulse width are steepest at low radio frequencies (80–400 MHz).
  • Located in western Vulpecula, roughly 3.5 degrees northwest of the Coathanger asterism (Collinder 399).

Catalog Cross-Identifications & Aliases

Common Aliases: CP 1919 · PSR J1921+2153 · LGM-1

Cross-Catalog Identifiers for PSR B1919+21
Catalog AuthorityIdentifier
SIMBADCP 1919
Related Object · Taurus

Crab Pulsar (PSR B0531+21 Neutron Star)

Coordinates, 33.08 ms spin period, 16.5-mag optical flashes, spin-down luminosity, and high-aperture observing guide for the Crab Pulsar.

Reference Guide

Celestial Coordinates (RA & Dec) Explained

Practical reference to J2000 equatorial coordinates: Right Ascension (RA in hours, minutes, seconds), Declination (Dec in degrees), and sexagesimal conversion.

Reference Guide

Proper Motion, Radial Velocity & Redshift

How astronomers combine tangential proper motion (mas/yr), Doppler radial velocity (km/s), and cosmological redshift (z) to reconstruct 3D space motion.

Scientific Sources & Dataset Provenance