KU Hydrae

Star in the constellation Hydra From Wikipedia, the free encyclopedia

KU Hydrae is a binary star in the constellation Hydra. The primary star is an Alpha2 Canum Venaticorum variable with its apparent magnitude varying from 0.05 magnitudes over a period of 33.97 days.[7]

Right ascension09h 22m 50.856s[3]
Declination−09° 50 19.66[3]
Apparentmagnitude(V)6.51 to 6.53[4]
Quick facts Observation data Epoch J2000 Equinox J2000, Constellation ...
KU Hydrae

A visual band light curve for KU Hydrae, adapted from Adelman (2006)[1]
Observation data
Epoch J2000      Equinox J2000
Constellation Hydra[2]
Right ascension 09h 22m 50.856s[3]
Declination −09° 50 19.66[3]
Apparent magnitude (V) 6.51 to 6.53[4]
Characteristics
Spectral type Ap EuCrSr[5]
U−B color index +0.11[6]
B−V color index +0.22[6]
Variable type α2 CVn[7]
Astrometry
Radial velocity (Rv)+19.6±5.0 km/s
Proper motion (μ) RA: −27.94±0.61[3] mas/yr
Dec.: −13.01±0.36[3] mas/yr
Parallax (π)6.92±0.61 mas[3]
Distance470 ± 40 ly
(140 ± 10 pc)
Orbit[8]
NameKU Hya B
Period (P)52.98(37) yr
Semi-major axis (a)0.169(1)
Eccentricity (e)0.074(8)
Inclination (i)68.5(6)°
Longitude of the node (Ω)202.4(4)°
Periastron epoch (T)2020.20(45)
Argument of periastron (ω)
(secondary)
58.7(3.3)°
Details[7]
KU Hya A
Mass2.07 M
KU Hya B
Mass2.05 M
Other designations
BD−09° 2816, HD 81009, HIP 45999, HR 3724, SAO 136799, A 1342[5]
Database references
SIMBADdata
Close

This star was discovered to be a visual binary star by Robert Grant Aitken in 1906 and was given the double star designation A 1342.[9] Additional measurements of the position angle and angular separation showed a rapid orbital motion.[10]

References

Related Articles

Wikiwand AI