Tau Ophiuchi

Multiple star in the constellation Ophiuchus From Wikipedia, the free encyclopedia

Tau Ophiuchi (τ Oph) is a multiple star in the constellation Ophiuchus, approximately 167 light years away based on parallax.[1] Its two main components are two yellow-white main sequence stars, A, of magnitude 5.24 and class F2V, and B, of magnitude 5.94 and class F5V,[2] orbiting each other with a period of 257 years and eccentricity around 0.77.[7] A is reported as a spectroscopic binary with a smaller star of 0.29 solar masses orbiting it every 186 days.[5] An additional component, C, has a separation of 100.8" and magnitude 11.28.[8]

Right ascension18h 03m 04.91992s[1]
Declination−08° 10 49.2586[1]
Apparentmagnitude(V)5.24 (A) / 5.94 (B) [2]
Quick facts Observation data Epoch J2000 Equinox J2000, Constellation ...
τ Ophiuchi
Location of τ Ophiuchi (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Ophiuchus
Right ascension 18h 03m 04.91992s[1]
Declination −08° 10 49.2586[1]
Apparent magnitude (V) 5.24 (A) / 5.94 (B) [2]
Characteristics
Spectral type F2V(A) / F5V (B) [2]
U−B color index +0.05 (A)[3]
B−V color index +0.38 (A)[3]
Astrometry
Radial velocity (Rv)−38.39[4] km/s
Proper motion (μ) RA: +15.78[1] mas/yr
Dec.: -37.79[1] mas/yr
Parallax (π)19.48±0.66 mas[1]
Distance167 ± 6 ly
(51 ± 2 pc)
Details
Mass1.54 (A) / 1.29 (B)[5] M
Surface gravity (log g)4.18 (A)[6] cgs
Temperature6,813 (A)[6] K
Other designations
BD−08°4549, CCDM J18031-0811AB, 69 Ophiuchi, HIP 88404, HD 164764+164765, HR 6733+6734, WDS J18031-0811AB
Database references
SIMBADdata
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References

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