PSR J0002+6216

PSR J0002+6216, also dubbed the Cannonball Pulsar, is a pulsar discovered by the Einstein@Home project in 2017. It is one of the fastest moving pulsars known, and has moved 53 ly (5.0×1014 km; 3.1×1014 mi) away from the location of its formation supernova, where the remaining supernova nebula, CTB 1 (Abell 85[2]), is. Due to its speed in traversing the interstellar medium, at 1,127 km/s (700 mi/s), it is leaving a 13 ly (1.2×1014 km; 7.6×1013 mi) long wake tail. The pulsar is currently 6,500 ly (6.1×1016 km; 3.8×1016 mi) away in the Cassiopeia constellation. The star rotates at a rate of 8.7 times a second.[3][4]

PSR J0002+6216

Pulsar moving away from its Supernova Remnant, while leaving a trail made up of the interstellar medium
Credit: Composite by Jayanne English, University of Manitoba; F. Schinzel et al.; NRAO/AUI/NSF; DRAO/Canadian Galactic Plane Survey; and NASA/IRAS. [CC BY 3.0]
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Cassiopeia
Right ascension 00h 02m 58.17s [1]
Declination +62° 16 09.4 [1]
Astrometry
Total velocity1127 km/s
Distance6500 ly
(2,000 pc)
Characteristics
Evolutionary stage Pulsar
Database references
SIMBADdata

References

  1. "Abell 85". AstroSurf.
  2. "Astronomers Find Pulsar Hurtling Through Space". Sci-News.com. 22 March 2019.
  3. Dave Finley (19 March 2019). "Astronomers Find "Cannonball Pulsar" Speeding Through Space". National Radio Astronomy Observatory.

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