PSR B1828-11 [SEP] constellation
PSR B1828−11
PSR B1828-11 (also known as PSR B1828-10) is a pulsar approximately 10,000 light-years away in the constellation of Scutum. The star exhibits variations in the timing and shape of its pulses: this was at one stage interpreted as due to a possible planetary system in orbit around the pulsar, though the model required an anomalously large second period derivative of the pulse times. The planetary model was later discarded in favour of precession effects as the planets could not cause the observed shape variations of
PANDA experiment
- PAR thrust
- PEPS effect
- PETRA
- PGM-19 Jupiter
- PHENIX
- PHOBOS experiment
- PHOSFOS
- PICASSO
- PIND
- PITZ
- PLATYPUS
- PLUTO reactor
- PM3 (chemistry)
- POLYGON experiment
- POVM
- PQS (chemical)
- PS210 experiment
- PSR B1828-10
- PSR B1913+16
- PSR J0737-3039
- PSR J1614–2230
- PUREX
- PVLAS
- PVT (physics)