Astronomy:PSR J0437−4715

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Short description: Pulsar in the constellation Pictor
PSR J0437−47
Observation data
Equinox J2000.0]] (ICRS)
Constellation Pictor
Right ascension  04h 37m 15.81476s[1]
Declination −47° 15′ 08.6242″[1]
Apparent magnitude (V) 20.98±0.09[2]
Characteristics
Spectral type Pulsar
Astrometry
Proper motion (μ) RA: 121.453 mas/yr
Dec.: 71.457 mas/yr
Distance509.8 ly
(156.3[3] pc)
Details
Mass1.44[4] M☉
Other designations
PSR B0435−47, 1RXS J043714.5−471503
Database references
SIMBADdata

PSR J0437−4715 is a pulsar. Discovered in the Parkes 70 cm survey,[5] 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 the Solar System, PSR J0437-4715 is 156.3 parsecs or 509.8 light-years distant.[3]

This pulsar is distinguished by being the most stable natural clock known and is debatably more stable than man-made atomic clocks.[6][7] 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.[8] It is also the first of only two pulsars to have the full three-dimensional orientation of its orbit determined.[9]

Optical observations indicate that the binary companion of PSR J0437-4715 is most likely a low-mass helium white dwarf.[2] The pulsar is about 1.4 solar mass (M☉)[4] and the companion is about 0.25 M☉.[1] The pair revolve around each other every 5.75 days in nearly perfect circular orbits.[10]

See also

References

  1. ↑ 1.0 1.1 1.2 Verbiest, J. P. W.; Bailes, M.; van Straten, W.; Hobbs, G. B. et al. (2008). "Precision Timing of PSR J0437-4715: An Accurate Pulsar Distance, a High Pulsar Mass, and a Limit on the Variation of Newton's Gravitational Constant". The Astrophysical Journal 679 (1): 675. doi:10.1086/529576. Bibcode: 2008ApJ...679..675V. 
  2. ↑ 2.0 2.1 Bell, J. F.; Bailes, M.; Bessell, M. S. (1993). "Optical detection of the companion of the millisecond pulsar J0437–4715". Nature 364 (6438): 603. doi:10.1038/364603a0. Bibcode: 1993Natur.364..603B. 
  3. ↑ 3.0 3.1 Deller, A. T.; Verbiest, J. P. W.; Tingay, S. J.; Bailes, M. (2008). "Extremely High Precision VLBI Astrometry of PSR J0437-4715 and Implications for Theories of Gravity". The Astrophysical Journal 685 (1): L67–L70. doi:10.1086/592401. Bibcode: 2008ApJ...685L..67D. 
  4. ↑ 4.0 4.1 Reardon, D. J.; Hobbs, G.; Coles, W.; Levin, Y. et al. (2016). "Timing analysis for 20 millisecond pulsars in the Parkes Pulsar Timing Array". Monthly Notices of the Royal Astronomical Society 455 (2): 1751–1769. doi:10.1093/mnras/stv2395. Bibcode: 2016MNRAS.455.1751R. 
  5. ↑ Johnston, Simon; Lorimer, D. R.; Harrison, P. A.; Bailes, M.; Lynet, A. G.; Bell, J. F.; Kaspi, V. M.; Manchester, R. N. et al. (1993). "Discovery of a very bright, nearby binary millisecond pulsar". Nature 361 (6413): 613–615. doi:10.1038/361613a0. Bibcode: 1993Natur.361..613J. 
  6. ↑ "Timing stability". http://relativity.livingreviews.org/Articles/lrr-2005-7/articlesu18.html#x25-370004.3. 
  7. ↑ Hartnett, J. G.; Luiten, A. N. (2011). "Colloquium: Comparison of astrophysical and terrestrial frequency standards". Reviews of Modern Physics 83 (1): 1–9. doi:10.1103/RevModPhys.83.1. Bibcode: 2011RvMP...83....1H. 
  8. ↑ Becker, Werner; Trümper, Joachim (1993). "Detection of pulsed X-rays from the binary millisecond pulsar J0437 - 4715". Nature 365 (6446): 528. doi:10.1038/365528a0. Bibcode: 1993Natur.365..528B. 
  9. ↑ Van Straten, W.; Bailes, M.; Britton, M.; Kulkarni, S. R. et al. (2001). "A test of general relativity from the three-dimensional orbital geometry of a binary pulsar". Nature 412 (6843): 158–160. doi:10.1038/35084015. PMID 11449265. Bibcode: 2001Natur.412..158V. 
  10. ↑ "Tables of Binary and Millisecond Pulsars". http://relativity.livingreviews.org/Articles/lrr-2005-7/articlese7.html. 



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