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Kappa Herculis information


κ Herculis

Historical view of the Hercules constellation showing Marfik (κ Her) as the hero's left "elbow".
Observation data
Epoch J2000      Equinox J2000
Constellation Hercules
κ Her A
Right ascension 16h 08m 04.52481s[1]
Declination 17° 02′ 49.1150″[1]
Apparent magnitude (V) 4.994[2]
κ Her B
Right ascension 16h 08m 04.95406s[3]
Declination 17° 03′ 15.6853″[3]
Apparent magnitude (V) 6.25[4]
Characteristics
Spectral type G7III + K0IV[5]
U−B color index +0.630[citation needed]
B−V color index +0.931[citation needed]
Variable type suspected[6]
Astrometry
κ Her A
Radial velocity (Rv)−10.50[7] km/s
Proper motion (μ) RA: −34.062[8] mas/yr
Dec.: −6.585[8] mas/yr
Parallax (π)8.5601 ± 0.1338 mas[8]
Distance381 ± 6 ly
(117 ± 2 pc)
Absolute magnitude (MV)-45[9]
κ Her B
Radial velocity (Rv)+32.21[10] km/s
Proper motion (μ) RA: −19.465[11] mas/yr
Dec.: −25.142[11] mas/yr
Parallax (π)8.1307 ± 0.0502 mas[11]
Distance401 ± 2 ly
(123.0 ± 0.8 pc)
Details
κ Her A
Mass3.17[12] M
Radius16[8] R
Luminosity148[9] L
Surface gravity (log g)2.90[12] cgs
Temperature5,119[12] K
Metallicity [Fe/H]+0.04[12] dex
Rotational velocity (v sin i)9.9[13] km/s
Age309[9] Myr
κ Her B
Radius11[11] R
Luminosity55[11] L
Temperature4,750[11] K
Metallicity [Fe/H]+0.131[14] dex
Rotational velocity (v sin i)1.0[13] km/s
Other designations
Marsic, κ Her, 7 Herculis, CCDM J16081+1703, NSV 7471, AAVSO 1603+17, WDS 16081+1703
A: HR 6008, HD 145001, HIP 79043, BD +77°2964
B: HR 6009, HD 145000, HIP 79045, BD +77°2965
Database references
SIMBADκ Her
κ Her A
κ Her B

Kappa Herculis (κ Herculis, abbreviated Kappa Her, κ Her) is an optical double star in the constellation of Hercules. The two components, Kappa Herculis A (Marsic /ˈmɑːrsɪk/, the traditional name of the system)[15] and B, were 27.3 arc seconds apart in 2000. Based on parallax measurements from the Hipparcos mission, κ Her A is about 113 parsecs (370 light-years) from the Sun and κ Her B is 600 parsecs (2,000 light-years); more recent parallax measurements suggest that B is around 5% more distant than A.

A faint third component Kappa Herculis C is just over 1 arc-minute away.[16] It is at the same distance as κ Her A and has an almost-identical space motion.[17]

The star 8 Herculis forms a naked eye pair with Kappa Herculis 14′ away.

  1. ^ a b Cite error: The named reference hipparcosA was invoked but never defined (see the help page).
  2. ^ Cite error: The named reference tycho2 was invoked but never defined (see the help page).
  3. ^ a b Cite error: The named reference hipparcosB was invoked but never defined (see the help page).
  4. ^ Cite error: The named reference ubv was invoked but never defined (see the help page).
  5. ^ Cite error: The named reference mk was invoked but never defined (see the help page).
  6. ^ Cite error: The named reference gcvs was invoked but never defined (see the help page).
  7. ^ Cite error: The named reference pulkovo was invoked but never defined (see the help page).
  8. ^ a b c d Cite error: The named reference dr2A was invoked but never defined (see the help page).
  9. ^ a b c Cite error: The named reference takeda was invoked but never defined (see the help page).
  10. ^ Cite error: The named reference coravel was invoked but never defined (see the help page).
  11. ^ a b c d e f Cite error: The named reference dr2B was invoked but never defined (see the help page).
  12. ^ a b c d Cite error: The named reference liu was invoked but never defined (see the help page).
  13. ^ a b Cite error: The named reference medeiros was invoked but never defined (see the help page).
  14. ^ Cite error: The named reference franchini was invoked but never defined (see the help page).
  15. ^ Davis, George A. (1944). "The pronunciations, derivations, and meanings of a selected list of star names". Popular Astronomy. 52: 8–30. Bibcode:1944PA.....52....8D.
  16. ^ Cite error: The named reference wds was invoked but never defined (see the help page).
  17. ^ Cite error: The named reference dr2C was invoked but never defined (see the help page).

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of the enclosure, consisting of Alpha Serpentis, Beta Herculis, Gamma Herculis, Kappa Herculis, Gamma Serpentis, Beta Serpentis, Delta Serpentis, Epsilon...

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borderline of the enclosure, consisting of Delta Ophiuchi, Beta Herculis, Gamma Herculis, Kappa Herculis, Gamma Serpentis, Beta Serpentis, Alpha Serpentis, Delta...

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borderline of the enclosure, consisting of Delta Ophiuchi, Beta Herculis, Gamma Herculis, Kappa Herculis, Gamma Serpentis, Beta Serpentis, Alpha Serpentis, Delta...

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Asteroseismology

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Virginis and ZZ Ceti stars are thought to be excited by the kappa mechanism; V777 Herculis stars by convective blocking. A number of past, present and...

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Table of stars with Bayer designations

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designated Psi HerculisHerculis, ψ Her) by Bayer, after Ptolemy – Bayer’s Uranometria and Bayer letters Bayer also by mistake catalogued Kappa Ceti under...

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pole nearer the stars in the constellation Hercules, pointing towards Tau Herculis around 18,400 AD. The celestial pole will then return to the stars in constellation...

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Indi Star 3.11 Nu Hydrae Star 3.11 Kappa Centauri Binary star system 3.12 Beta Columbae Star 3.13 Delta Herculis Binary star system 3.139 3.12 HR 3803...

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Thuban

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from 3942 BC, when it superseded Tau Herculis as the pole star, until 1793 BC, when it was superseded by Kappa Draconis. It was closest to the pole in...

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Subgiant

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B3: ι Herculis B5: τ Herculis A2: β Aurigae, λ Ursae Majoris, β Serpentis A3: δ Herculis F2: δ Geminorum, ζ Serpentis F5: Procyon, 110 Herculis F6: τ...

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List of proper names of stars

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Cambridge University Press. p. 170. ISBN 0-521-44921-9. Kaler, James B. "Saiph (Kappa Orionis)". Stars. University of Illinois. Archived from the original on...

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Cepheid variable

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as well as Delta Cephei. Type II Cepheids include: W Virginis and BL Herculis. Anomalous Cepheids include: XZ Ceti (overtone pulsation mode) and BL Boötis...

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Pyxis

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varies between magnitudes 6.99 and 7.83 over 159 days. VY Pyxidis is a BL Herculis variable (type II Cepheid), ranging between apparent magnitudes 7.13 and...

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Petrozavodsk phenomenon

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Draconis, Psi Herculis, Kappa Coronae Borealis and Delta Coronae Borealis. The object stopped near Gamma Cephei at an azimuth of 220°. Near Kappa Coronae Borealis...

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Bayer designation

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Andromedae = Delta Pegasi, Beta Tauri = Gamma Aurigae, and Nu Boötis = Psi Herculis. (He catalogued Fomalhaut only once, as Alpha Piscis Austrini.) When the...

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Instability strip

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Studies of DB White Dwarfs: The Instability Strip of the Pulsating DB (V777 Herculis) Stars". The Astrophysical Journal. 516 (2): 887. Bibcode:1999ApJ...516...

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List of Arabic star names

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Type II Cepheid

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of their period. Stars with periods between 1 and 4 days are of the BL Herculis subclass and 10–20 days belong to the W Virginis subclass. Stars with periods...

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to be known and is hard to measure directly. A few systems, such as DI Herculis, have been measured as test cases for general relativity. Henry Cavendish...

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