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Iota Herculis

Iota Herculis
Hercules Historical View.png
Historical view of the Hercules constellation showing Iota Herculis as one of the hero's feet.
Observation data
Epoch J2000      Equinox J2000
Constellation Hercules
Right ascension 17h 39m 27.8864s
Declination +46° 00′ 22.795″
Apparent magnitude (V) 3.7497
Characteristics
Spectral type B3IV
U−B color index –0.71
B−V color index –0.18
Variable type Beta Cephei
Astrometry
Radial velocity (Rv) –20.0 km/s
Proper motion (μ) RA: 7.48 mas/yr
Dec.: 4.53 mas/yr
Parallax (π) 7.17 ± 0.13mas
Distance 455 ± 8 ly
(139 ± 3 pc)
Absolute magnitude (MV) –1.97
Details
Mass 6.7 ± 0.1 M
Radius 5.29 ± 0.45 R
Luminosity 2,500 L
Surface gravity (log g) 3.82 ± 0.06 cgs
Temperature 18,070 ± 294 K
Metallicity [Fe/H] –0.40 dex
Rotational velocity (v sin i) 11 km/s
Age 37.8 ± 8.6 Myr
Other designations
ι Her, 85 Her, HR 6588, BD +46° 2349, HD 160762, FK5 663, HIP 86414, SAO 46872, GC 23965, CCDM J17395+4601A
Database references
SIMBAD data

Iota Herculis (ι Her, ι Herculis) is a fourth-magnitude star in the constellation Hercules. The luminary shares an etymological similarity with the star Rigel in the constellation of Orion, as both stars refer to one of the feet of each mythological hero.

In Chinese, 天棓 (Tiān Bàng), meaning Celestial Flail, refers to an asterism consisting of ι Herculis, ξ Draconis, ν Draconis, β Draconis and γ Draconis. Consequently, ι Herculis itself is known as 天棓五 (Tiān Bàng wu, English: the Fifth Star of Celestial Flail.)

Iota Herculis is a B-type subgiant star that is at the end of its hydrogen fusion stage. With a stellar classification B3IV, it is considerably larger than the Sun, having a mass that is 6.5 times solar and a radius 5.3 times. Though its apparent magnitude is only 3.79, it is 2,500 times more luminous than the Sun, yielding an absolute magnitude of -2.11, brighter in fact than the most of the hot B stars in the Pleiades open star cluster. The Hipparcos satellite mission estimated its distance at roughly 152 parsecs (pc) from Earth, or 496 light years (ly) away; an updated parallax measurement from Floor van Leeuwen in 2007, however, puts the distance at 455ly with a much tighter error factor of only 8ly.


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Wikipedia

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