Astronomy:RX J1856.5-3754

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RX J1856.5-3754
RX J1856.5-3754.jpg
X-ray image of RX J1856.5-3754
Observation data
Equinox J2000.0]] (ICRS)
Constellation Corona Australis
Right ascension  18h 56m 35s [1]
Declination −37° 54′ 36″[1]
Apparent magnitude (V) ~25.6[1]
Mass0.9 M
Radius19–41 km
Age1 million years
Other designations
RX J185635-3754, 1ES 1853-37.9, 1RXS J185635.1-375433
Database references

RX J1856.5-3754 (also called RX J185635-3754, RX J185635-375, and various other designations) is a nearby neutron star in the constellation Corona Australis.

Discovery and location

File:Zooming in on the very faint neutron star RX J1856.5-3754.ogg RX J1856.5-3754 is thought to have formed in a supernova explosion of its companion star about one million years ago and is moving at 108 km/s across the sky. It was discovered in 1992, and observations in 1996 confirmed that it is a neutron star, the closest to Earth discovered.[2]

It was originally thought to be about 150–200 light-years away,[3] but further observations using the Chandra X-ray Observatory in 2002 indicate that its distance is greater—about 400 light-years.[4][5]

RX J1856 is one of the Magnificent Seven, a group of young neutron stars at distances between 200 and 500 parsecs (652 and 1630 light years) of Earth.

Quark star hypothesis

By combining Chandra X-ray Observatory and Hubble Space Telescope data, astronomers previously estimated that RX J1856 radiates like a solid body with a temperature of 700,000 °C and has a diameter of about 4–8 km. This estimated size was too small to reconcile with the standard models of neutron stars, therefore it was suggested that it might be a quark star.[4]

However, later refined analysis[5][6] of improved Chandra and Hubble observations revealed that the surface temperature of the star is lower, only 434,000 °C, and respectively the diameter is larger, about 14 km (with account of the effects of general relativity, the observed radius appears about 17 km).[5] Thus, RX J1856.5-3754 is now excluded from the list of quark star candidates.[6]

See also

  • 3C 58, a possible quark star.


  1. 1.0 1.1 1.2 RX J185635-3754 - an Isolated Neutron Star, F. M. Walter, web page at the Department of Physics and Astronomy, State University of New York at Stony Brook. Accessed on line June 29, 2007.
  2. Rees, Martin (2012) Universe. Dorling Kindersley. p. 528
  3. "The Mystery of the Lonely Neutron Star". European Southern Observatory press release, September 11, 2000. Accessed online at May 20, 2007.
  4. 4.0 4.1 Drake J. J. (2002). "Is RX J1856.5-3754 a Quark Star?". Astrophys. J. 572 (2): 996–1001. doi:10.1086/340368. Bibcode2002ApJ...572..996D. 
  5. 5.0 5.1 5.2 Ho W. C. G. (2007). "Magnetic hydrogen atmosphere models and the neutron star RX J1856.5–3754". Monthly Notices of the Royal Astronomical Society 375 (2): 821–830. doi:10.1111/j.1365-2966.2006.11376.x. Bibcode2007MNRAS.375..821H. 
  6. 6.0 6.1 Truemper, J. E.; Burwitz, V.; Haberl, F.; Zavlin, V. E. (June 2004). "The puzzles of RX J1856.5-3754: neutron star or quark star?". Nuclear Physics B: Proceedings Supplements 132: 560–565. doi:10.1016/j.nuclphysbps.2004.04.094. Bibcode2004NuPhS.132..560T. 

External links