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PSR J0738−4042 is the first pulsar observed to have been affected by asteroids.[2]
| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Puppis |
| Right ascension | 07h 38m 32.329s |
| Declination | −40° 42' 40.94" |
| Characteristics | |
| Spectral type | Pulsar |
| Astrometry | |
| Distance | 37,000 ly |
| Details | |
| Rotation | 374.919985032 ms[1] |
| Database references | |
| SIMBAD | data |
It was originally discovered in 1968.[1] In 2013 scientists at the University of Oxford, Hartebeesthoek Observatory and CSIRO announced that they had observed changes in the pulsar's spin rate and the shape of its radio pulse indicating that asteroids were encountering it, including one with a mass of about a billion tons.[3]
We think the pulsar's radio beam zaps the asteroid, vaporising it. But the vaporised particles are electrically charged and they slightly alter the process that creates the pulsar's beam.
— Dr. Ryan Shannon, [2]
The scientists suggested that the material blown out from the explosion which formed the pulsar could have fallen back towards it, developing a disk of debris including asteroids.[4]
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