Nu Draconis

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𝜈 Draconis

𝜈 Draconis in optical light
Observation data
Epoch J2000      Equinox J2000
Constellation Draco
𝜈1 Dra
Right ascension 17h 32m 10.56856s[1]
Declination +55° 11′ 03.2739″[1]
Apparent magnitude (V) +4.88[2]
𝜈2 Dra
Right ascension 17h 32m 16.02464s[1]
Declination +55° 10′ 22.6504″[1]
Apparent magnitude (V) +4.88[2]
Characteristics
𝜈1 Dra
Spectral type A8Vm[3] (kA3hF0mF0[4])
U−B color index +0.03[2]
B−V color index +0.26[2]
𝜈2 Dra
Spectral type A4IVm[3] (kA3hF1mF0[4])
U−B color index +0.04[2]
B−V color index +0.27[2]
Distance
99.4 ± 0.5 ly
(30.5 ± 0.2 pc)
Semi-amplitude
(K1)
(primary)
10.0 km/s
Details
𝜈1 Dra
Rotational velocity (v sin i)
68[9] km/s
HR 6555, SAO 30450[14]
Database references
SIMBAD𝜈 Dra
𝜈1 Dra
𝜈2 Dra

Nu Draconis (also known as 𝜈 Dra, 𝜈 Draconis, where 𝜈 is the Greek letter

spectroscopic binary star system.[14]

This star, along with β Dra (Rastaban), γ Dra (Eltanin), μ Dra (Alrakis) and ξ Dra (Grumium) were Al ʽAwāïd, "the Mother Camels", which was later known as the Quinque Dromedarii.[15]

In

Chinese name for 𝜈 Draconis itself is 天棓二 (Tiān Bàng èr, English: the Second Star of Celestial Flail.)[17]

The two stars of the visual binary are considered to be a common proper motion pair on the basis of their very similar

radial velocities, and proper motions, although no orbital motion can be observed.[18]

𝜈1 Draconis is an

calcium K lines, F0 if determined from its hydrogen lines, and F0 if determined from other metallic spectral lines.[4]

𝜈2 Draconis is a spectroscopic binary with a period of 38 days. The two stars are separated by 0.267 au on average, and they have an almost circular orbit with an eccentricity of 0.03.[19][6] The primary is also an Am star, while the secondary has a low mass and luminosity and is only inferred from the orbital movement of the more massive star.[7]

References

External links