Gliese 783

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Gl 783 A/B
Observation data
Epoch J2000      Equinox J2000
Constellation Sagittarius
Right ascension 20h 11m 11.94s [1]
Declination –36° 06′ 04.4″ [1]
Apparent magnitude (V) 5.31/11.5
Characteristics
Spectral type K2 V/M3.5V
U−B color index 0.46/?
B−V color index 0.86/?
Variable type None
Astrometry
Radial velocity (Rv) -129.8 km/s
Proper motion (μ) RA: 456.99 ± 0.33 [1] mas/yr
Dec.: -1574.64 ± 0.22 [1] mas/yr
Parallax (π) 166.25 ± 0.27[1] mas
Distance 19.62 ± 0.03 ly
(6.015 ± 0.010 pc)
Absolute magnitude (MV) 6.40/12.6
Details
Mass 0.82/0.20 M
Radius 0.71/0.28 R
Luminosity 0.23/0.000077 L
Temperature ? K
Metallicity 0.85/0.26
Rotation ?
Age 7.7 × 109[2] years
Other designations
279 G. Sagittarii, HR 7703, CD -36°13940, HD 191408, GCTP 4782.00, LHS 486/487, LFT 1529/1530, LTT 7988/7989, SAO 211885, HIP 99461.

Gliese 783 (279 G. Sagittarii) is a binary star system in the constellation of Sagittarius. It is 19.87 light years from Earth, and it has an absolute magnitude of +5.32. In space, Gliese 783 is approaching the solar system at a velocity of approximately 140 kilometers per second. At this rate, it will be 6.7 light years away in 40,000 years, and ten times brighter than its current state. The two stars are separated by an angle of 7.1", corresponding to a distance of about 43 AUs.

References [edit]

  1. ^ a b c d e van Leeuwen, F. (2007). "HIP 99461". Hipparcos, the New Reduction. Retrieved 2009-12-12. 
  2. ^ Mamajek, Eric E.; Hillenbrand, Lynne A. (November 2008). "Improved Age Estimation for Solar-Type Dwarfs Using Activity-Rotation Diagnostics". The Astrophysical Journal 687 (2): 1264–1293. arXiv:0807.1686. Bibcode:2008ApJ...687.1264M. doi:10.1086/591785. 

External links [edit]