PSR J2144−3933 is a pulsar about 180 parsecs (587 light-years) from Earth. It is the coldest known neutron star with a surface temperature less than 42000 Kelvin as measured by the Hubble Space Telescope.[1] It was previously thought to have a period of 2.84 seconds but is now known to have a period of 8.51 seconds, which is among the longest-known radio pulsar.
Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Grus |
Right ascension | 21h 44m 12.10s |
Declination | −39° 33′ 55.2″ |
Characteristics | |
Spectral type | Pulsar |
Variable type | None |
Astrometry | |
Distance | approx. 587 ly (approx. 180 pc) |
Details | |
Rotation | 8.51 s |
Other designations | |
EUVE J2144-39.6 | |
Database references | |
SIMBAD | data |
J2144−3933 is also notable for other reasons: its mean pulse profile is very narrow in comparison to the pulse period with a half-intensity width of less than one degree of longitude. It also has the lowest spindown luminosity of any pulsar at about 3×1021 watts.
Writing in Nature, astrophysicists M. D. Young and coworkers consider this object and suggest that its existence throws current theories into doubt. They state:
- Moreover, under the usual model assumptions, based on the neutron-star equations of state, this slowly rotating pulsar should not be emitting a radio beam. Therefore either the model assumptions are wrong, or current theories of radio emission must be revised[2]
The fact that J2144−3933 is the coldest observed neutron star has been exploited to constrain the properties of dark matter.[3][4][5]