SCR 1845−6357: Difference between revisions

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Revision as of 12:40, 7 March 2008

SCR 1845-6357
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Pavo
Right ascension 18h 45m 02.6s
Declination -63° 57' 48"
Apparent magnitude (V) +17.39
Characteristics
Spectral type M8.5
U−B color index ?
B−V color index ?
Variable type ?
Astrometry
Radial velocity (Rv)? km/s
Proper motion (μ) RA: 2,664 mas/yr
Dec.: 76.6 mas/yr
Parallax (π)259.45 ± 1.11 mas
Distance12.57 ± 0.05 ly
(3.85 ± 0.02 pc)
Absolute magnitude (MV)19.41

SCR 1845-6357 is a red dwarf star about 12.5 light-years away in the constellation Pavo. This star has a mass of about 7% of the Sun. However the measurements are still preliminary and are subject to change.

This star has been found to possess a brown dwarf companion, designated SCR 1845-6357 B. The companion, classified as a T-dwarf, orbits at a distance of 4.5 AU from the primary, has a mass between 9 and 65 times the mass of Jupiter, and an estimated effective temperature of 850K.


See also


References

  • Hambly, N.C., et al, 2005, "The Solar Neighborhood. VIII. Discovery of New High Proper Motion Nearby Stars Using the SuperCOSMOS Sky Survey", The Astronomical Journal, Vol. 128
  • Deacon, Niall R. et al, 2005, "The Solar Neighborhood. XI. The Trigonometric Parallax of SCR 1845-6357", The Astronomical Journal, Vol. 129.
  • B.A. Biller et al, 2006, "Discovery of a Brown Dwarf Very Close to the Sun: A Methane-rich Brown Dwarf Companion to the Low-Mass Star SCR 1845-6357", Astrophysical Journal Letters.


External links