Observation data Epoch J2000 Equinox J2000 |
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Constellation | Boötes |
Right ascension | 14h 16m 09.9294s |
Declination | +51° 22′ 02.033″ |
Apparent magnitude (V) | 4.75 |
Characteristics | |
Spectral type | A9V |
U−B color index | 0.06 |
B−V color index | 0.2 |
R−I color index | 0.09 |
Variable type | Delta Scuti variable |
Astrometry | |
Radial velocity (Rv) | -18.7 km/s |
Proper motion (μ) | RA: -149.98 mas/yr Dec.: 89.42 mas/yr |
Parallax (π) | 33.54 ± 0.56 mas |
Distance | 97 ± 2 ly (29.8 ± 0.5 pc) |
Absolute magnitude (MV) | 4.96 |
Details | |
Mass | 3.1 M☉ |
Radius | 2.1 R☉ |
Luminosity | 40 L☉ |
Temperature | 7,500–10,000 K |
Rotation | 137 km/s 0,00212755 Year |
Other designations | |
Database references | |
SIMBAD | data |
Data sources: | |
Hipparcos Catalogue, CCDM (2002), Bright Star Catalogue (5th rev. ed.) |
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Database references | |
SIMBAD | data |
Iota Boötis (ι Boo, ι Boötis) is a star system in the constellation Boötes. It has the traditional name Asellus Secundus (Latin for "second donkey colt")[1] and the Flamsteed designation 21 Boötis.
This star, along with the other Asselus (θ Boo and κ Boo) and λ Boo, were Al Aulād al Dhiʼbah (ألعولد ألذعب - al aulād al dhiʼb), "the Whelps of the Hyenas".[2].
In Chinese, 梗河 (Tiān Qiāng), meaning Celestial Spear, refers to an asterism consisting of ι Boötis, κ2 Boötis and θ Boötis.[3] Consequently, ι Boötis itself is known as 天槍三 (Tiān Qiāng èr, English: the Second Star of Celestial Spear.)[4]
Iota Boötis is a double star, with components at an angular distance of 38.6 arcseconds, easily separated with binoculars. It is approximately 97 light years from Earth.
The primary component, Iota Boötis A, a spectroscopic binary, is a white A-type main sequence dwarf with a mean apparent magnitude of +4.75. It is classified as a Delta Scuti type variable star and its brightness varies from magnitude +4.73 to +4.78. The companion, Iota Boötis B, is a magnitude +8.27 star belonging to spectral class A2.
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