89 Herculis
From Infogalactic: the planetary knowledge core
Observation data Epoch J2000 Equinox J2000 |
|
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Constellation | Hercules |
Right ascension | 17h 55m 25.18892s[1] |
Declination | 26° 02′ 59.9738″[1] |
Apparent magnitude (V) | 5.36[2] (5.34 - 5.54[3]) |
Characteristics | |
Evolutionary stage | post-AGB |
Spectral type | F2Ibe[4] |
U−B color index | −0.34[2] |
B−V color index | +0.34[2] |
Variable type | SRd[3] |
Astrometry | |
Radial velocity (Rv) | −28.5[5] km/s |
Proper motion (μ) | RA: 4.34[1] mas/yr Dec.: 5.89[1] mas/yr |
Parallax (π) | 0.76 ± 0.23[1] mas |
Distance | approx. 4,000 ly (approx. 1,300 pc) |
Absolute magnitude (MV) | −6.5[6] |
Details | |
Mass | 1.0[7] M☉ |
Radius | 71.0[7] R☉ |
Luminosity | 8,350[7] L☉ |
Surface gravity (log g) | 0.55[4] cgs |
Temperature | 6,550[4] K |
Metallicity | −0.5[4] |
Rotational velocity (v sin i) | 23[8] km/s |
Other designations | |
Database references | |
SIMBAD | data |
Exoplanet Archive | data |
89 Herculis is a fifth-magnitude star in the constellation Hercules. Located about 4,000 light years away, it is among a rare class of post-AGB stars - low mass stars in the last stages of their lives, highly inflated to appear as supergiants.[4]
89 Her is a spectroscopic binary system with the pair surrounded by a dusty disc. The system shows variable brightness and spectral line profiles.[9] The companion has a very low mass and luminosity and orbits the primary in 288 days.[4]
89 Her is classified as a semiregular variable star, V441 Her, varying from magnitude 5.3 to 5.5 in around 68 days.[3]
References
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External links
- Jim Kaler's Stars, University of Illinois: 89 HER (89 Herculis)
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Categories:
- Pages with reference errors
- Pages with broken file links
- Hercules (constellation)
- F-type supergiants
- Flamsteed objects
- HR objects
- Henry Draper Catalogue objects
- Durchmusterung objects
- Hipparcos objects
- Binary stars
- Objects named with variable star designations
- Post-asymptotic-giant-branch stars
- Emission-line stars