Kappa Hydrae

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κ Hydrae
Observation data
ICRS
)
Constellation Hydra
Right ascension 09h 40m 18.36496s[1]
Declination −14° 19′ 56.2675″[1]
Apparent magnitude (V) 5.06[2]
Characteristics
Spectral type B4 IV/V[3]
U−B color index −0.57[2]
B−V color index −0.15[2]
Variable type Suspected[4][5]
Distance
440 ± 20 ly
(134 ± 5 pc)
Absolute magnitude (MV)−0.98[7]
Details
Myr
HIP 47452, HR 3849, SAO 155388.[12]
Database references
SIMBADdata

κ Hydrae, Latinised as Kappa Hydrae, is a solitary

mas.[1] It may be a variable star, meaning it undergoes repeated fluctuations in brightness by at least 0.1 magnitude.[5]

This is an

projected rotational velocity of 115.0 km/s,[11] and is only about 31 million years old.[3] The star radiates 328 times the solar luminosity from its outer atmosphere[9] at an effective temperature of 16,150 K.[10]

Name

This star was one of the set assigned by the 16th century astronomer Al Tizini[14] to Al Sharāsīf (ألشراسيف), the Ribs (of Hydra), which included the stars from β Crateris westward through κ Hydrae.[15][16]

According to the catalogue of stars in the Technical Memorandum 33-507 - A Reduced Star Catalog Containing 537 Named Stars, Al Sharāsīf were the title for two stars : β Crateris as Al Sharasīf II and κ Hydrae as Al Sharasīf I.[17]

In

Extended Net, refers to an asterism consisting of Kappa Hydrae, Upsilon1 Hydrae, Lambda Hydrae, Mu Hydrae, HD 87344, and Phi1 Hydrae.[18] Consequently, Kappa Hydrae itself is known as 張宿五 (Zhāng Xiù wǔ), "the Fifth Star of Extended Net".[19]

References