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PSR J0437-4715 is a pulsar. Discovered in the Parkes 70 cm survey, it remains the closest and brightest millisecond pulsar (MSP) known. The pulsar rotates about its axis 173.7 times per second and therefore completes a rotation every 5.75 milliseconds. It emits a searchlight-like radio beam that sweeps past the Earth each time it rotates. Currently the most precisely located object outside of our Solar System, PSR J0437-4715 is 156.3 parsecs or 509.8 light years distant. This pulsar is distinguished by being the most stable natural clock known and is debatably more stable than man-made atomic clocks.〔(Timing stability )〕 Its stability is about one part in 1015. Two other pulsars, PSR B1855+09 and PSR B1937+21 are known to be comparable in stability to atomic clocks, or about 3 parts in 1014. PSR J0437-4715 is the first MSP to have its X-ray emission detected and studied in detail. It is also the first of only two pulsars to have the full three-dimensional orientation of its orbit determined. Optical observations indicate that the binary companion of PSR J0437-4715 is most likely a low-mass helium white dwarf. The pulsar is about 1.8 solar mass () and the companion is about 0.25 . The pair revolve around each other every 5.75 days in nearly perfect circular orbits.〔(Tables of Binary and Millisecond Pulsars )〕 ==See also== *Binary pulsar 抄文引用元・出典: フリー百科事典『 ウィキペディア（Wikipedia）』 ■ウィキペディアで「PSR J0437-4715」の詳細全文を読む スポンサード リンク
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