Iota Herculis
  | |
| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Hercules |
| Right ascension | 17h 39m 27.8864s[1] |
| Declination | +46° 00′ 22.795″[1] |
| Apparent magnitude (V) | 3.80[2] |
| Characteristics | |
| Spectral type | B3IV[1] |
| U−B color index | −0.71 |
| B−V color index | −0.18[3] |
| Variable type | Beta Cephei[4] |
| Astrometry | |
| Radial velocity (Rv) | −21.23±0.20[5] km/s |
| Proper motion (μ) | RA: +7.48[6] mas/yr Dec.: +4.53[6] mas/yr |
| Parallax (π) | 7.17±0.13 mas[6] |
| Distance | 455 ± 8 ly (139 ± 3 pc) |
| Absolute magnitude (MV) | −1.97[7] |
| Orbit[5] | |
| Period (P) | 111.5±0.1 days |
| Semi-major axis (a) | ≥12.68±0.74 R☉ |
| Eccentricity (e) | 0.53±0.03 |
| Argument of periastron (ω) (secondary) | 208.3+5.2 −5.0° |
| Semi-amplitude (K1) (primary) | 6.8+0.4 −0.3 km/s |
| Details | |
| Mass | 5.40+0.12 −0.08[5] M☉ |
| Radius | 4.74±0.34[8] R☉ |
| Luminosity | 2,489[2] L☉ |
| Surface gravity (log g) | 3.61±0.02[5] cgs |
| Temperature | 14,346+104 −96[5] K |
| Metallicity [Fe/H] | −0.40[9] dex |
| Rotational velocity (v sin i) | 6±1[2] km/s |
| Age | 37.8±8.6[10] 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 Herculis, ι Her) is a fourth-magnitude binary star in the constellation Hercules, 139 parsecs (450 light-years) away. The brightest is a β Cephei variable, a pulsating star.
Visibility
[edit | edit source]
Iota Herculis is dim enough that in cities with a lot of light pollution it is unlikely to be visible with the naked eye. In rural areas it will usually be visible, and for much of the Northern Hemisphere the star is circumpolar and visible year around.
Pole star
[edit | edit source]As a visible star, the proximity of Iota Herculis to the precessional path the Earth's North Pole traces across the celestial sphere makes it a pole star, a title currently held by Polaris. In 10,000 BCE it was the pole star, and in the future it will be again. While Polaris is only 0.5° off the precessional path Iota Herculis is 4° off.
| Preceded by | Pole star | Succeeded by |
|---|---|---|
| Vega | ~16,000 CE | Tau Herculis |
Properties
[edit | edit source]Iota Herculis is a spectroscopic binary having an orbital period of 111.5 days and a semi-major axis of at least 0.0590 au. The orbit is somewhat eccentric, at e = 0.53. Nothing is known about the companion.[5]
The primary component is a B-type subgiant star that is at the end of its hydrogen fusion stage.[13] With a stellar classification B3IV,[1] it is considerably larger than the Sun, having a mass that is 5.4 times solar[5] and a radius 4.7 times. Though its apparent magnitude is only 3.80, it is 2,500 times more luminous than the Sun, yielding an absolute magnitude of −2.11, brighter in fact than 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;[14] an updated parallax measurement from Floor van Leeuwen in 2007, however, puts the distance at 455 ly with a much tighter error factor of only 8 ly.[6]
A companion at a separation of about 30 au from Iota Herculis has been reported at the Washington Double Star Catalog, but it has been observed only once and is considered unconfirmed.[5] Another star has been identified with a common proper motion at an angular separation of 116 arcseconds and a visual magnitude of 12.1.[15] This would place it approximately 18,000 AU away, giving it an orbit of about 1 million years.[13] However, measurements by the Gaia spacecraft found it to be much farther away than Iota, and thus is not a member of the system.[5]
Etymology
[edit | edit source]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.[16] Consequently, ι Herculis itself is known as 天棓五 (Tiān Bàng wu, English: the Fifth Star of Celestial Flail).
References
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- ^ (in Chinese) 中國星座神話, written by 陳久金. Published by 台灣書房出版有限公司, 2005, Lua error in Module:Citation/CS1/Configuration at line 2172: attempt to index field '?' (a nil value)..
External links
[edit | edit source]- Jim Kaler's Stars, University of Illinois: IOTA HER (Iota Herculis)
- An Atlas of the Universe: Multiple Star Orbits
