HD 156846

Star in the constellation Ophiuchus From Wikipedia, the free encyclopedia

HD 156846 is a binary star[8] system in the equatorial constellation of Ophiuchus, positioned a degree SSE of Messier 9.[12] It has a yellow hue and is just barely bright enough to be visible to the naked eye with an apparent visual magnitude of 6.5. The system is located at a distance of 156 light years from the Sun based on parallax. It is drifting closer with a radial velocity of −68.5 km/s, and is predicted to come to within 85.0 light-years in about 476,000 years.[9]

Quick facts Constellation, Right ascension ...
HD 156846
Observation data
Epoch J2000      Equinox ICRS
Constellation Ophiuchus[1]
A
Right ascension 17h 20m 34.31089s[2]
Declination −19° 20 01.4917[2]
Apparent magnitude (V) 6.506[3]
B
Right ascension 17h 20m 34.31093s[4]
Declination −19° 20 01.4944[4]
Apparent magnitude (V) 14.10[5]
Characteristics
A
Evolutionary stage main sequence[2]
Spectral type G1V[6]
B−V color index 0.557[3]
B
Evolutionary stage main sequence[7]
Spectral type M4V[8]
Astrometry
Radial velocity (Rv)−68.50±0.22[9] km/s
Absolute magnitude (MV)+3.055[3]
A
Proper motion (μ) RA: −137.076±0.029[2] mas/yr
Dec.: −143.378±0.019[2] mas/yr
Parallax (π)20.9684±0.0229 mas[2]
Distance155.5 ± 0.2 ly
(47.69 ± 0.05 pc)
Details
A
Mass1.35±0.045[3] M
Radius2.12±0.12[3] R
Luminosity5.07[9] L
Surface gravity (log g)3.92±0.08[3] cgs
Temperature5,969±44[3] K
Metallicity [Fe/H]+0.17±0.04[3] dex
Rotational velocity (v sin i)5.05±0.50[3] km/s
Age2.8+0.1
−0.2
[9] Gyr
B
Mass0.59[8] M
Radius0.56[10] R
Luminosity0.049[10] L
Temperature3,592[10] K
Other designations
HD 156846, HIP 84856, HR 6441, WDS J17206-1920[11]
A: BD−19°4605, GC 23420, SAO 160474
B: TIC 75673521, 2MASS J17203464-1919599
Database references
SIMBADdata
B
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The primary, component A, is a G-type star with a stellar classification of G1V.[6] The absolute visual magnitude of this star is 1.13 magnitudes above the main sequence, indicating it has evolved slightly off the main sequence.[3] It has 1.35 times the mass of the Sun and 2.12 times the Sun's radius.[3] The star is an estimated 2.8[9] billion years old and is spinning with a projected rotational velocity of 5 km/s.[3] It is radiating five[9] times the luminosity of the Sun from its photosphere at an effective temperature of 5,969 K.[3]

The magnitude 14.1 secondary companion, component B, was discovered by the American astronomer R. G. Aitken in 1910.[5] It lies at an angular separation of 5.1 from the primary, corresponding to a projected separation of 250 AU. This is a red dwarf with a class of M4V and has an estimated 59% of the Sun's mass.[8]

Planetary system

On 26 October 2007, a planet HD 156846 b was found orbiting the primary star by Tamuz, using the radial velocity method.[13] It has an orbital period of 0.98 years and a large eccentricity of 0.85. The estimated mass of this object is, at a minimum, 10.6 times the mass of Jupiter. If it were following the same orbit within the Solar System, it would have a perihelion within the orbit of Mercury and an aphelion outside the orbit of Mars.[3]

More information Companion (in order from star), Mass ...
The HD 156846 planetary system[3]
Companion
(in order from star)
Mass Semimajor axis
(AU)
Orbital period
(days)
Eccentricity Inclination
(°)
Radius
b ≥10.57±0.29 MJ 1.096±0.021 359.5546±0.0071 0.84785±0.00050
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See also

References

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