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.
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^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.
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KappaHerculis (κ Herculis, abbreviated Kappa Her, κ Her) is an optical double star in the constellation of Hercules. The two components, Kappa Herculis...
Beta Herculis (β Herculis, abbreviated Beta Her, β Her), formally named Kornephoros /kɔːrˈnɛfərəs/, or Rutilicus, is a binary star and the brightest star...
of Left Wall Lambda Herculis Maasym 趙 Zhào The state of Zhao 天市左垣三 Tiān Shì Zuǒ Yuán sān the Third Star of Left Wall Mu Herculis 九河 Jiǔ Hé Jiuhe 天市左垣四...
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...
designated Psi Herculis (ψ Herculis, ψ Her) by Bayer, after Ptolemy – Bayer’s Uranometria and Bayer letters Bayer also by mistake catalogued Kappa Ceti under...
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...
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...
from 3942 BC, when it superseded Tau Herculis as the pole star, until 1793 BC, when it was superseded by Kappa Draconis.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...
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...
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...
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...
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...
Khosroshahi, Habib; Wasatonic, Rick (2013). "THE AGE AND MASS OF THE α HERCULIS TRIPLE-STAR SYSTEM FROM a MESA GRID OF ROTATING STARS WITH 1.3 ⩽ M / M...
Studies of DB White Dwarfs: The Instability Strip of the Pulsating DB (V777 Herculis) Stars". The Astrophysical Journal. 516 (2): 887. Bibcode:1999ApJ...516...
Hertzsprung SONG Telescope: Asteroseismology of the G5 Subgiant Star μ Herculis". The Astrophysical Journal. 836 (1): 142. arXiv:1701.03365. Bibcode:2017ApJ...
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...
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...