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HD 209856


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Apsidal Motion and Photometric Elements of the Eccentric Eclipsing Binary V401 Lacertae
New (UBV) photometric observations of the recently discovered eccentricorbit binary V401 Lacertae were analyzed by using the Wilson-Devinneyprogram. Seven new minimum times were estimated by using newobservations. The analysis of the light curves and all available minimumtimes has revealed that the system is detached, with the orbitaleccentricity e = 0.1734 ± 0.0003, the longitude of the periastronω = 63.°93 ± 0.°15, the rate of change of thelongitude of periastron dot{ω} = 0.°0200 ± 0.°0024cycle-1, corresponding to an apsidal motion period of U =96.2 ± 11.4 yr. The apsidal motion of the system has beenconfirmed by the significant difference on the longitude of periastron(ω) obtained from two light curves (Hipparcos and ourselves) intwo different epochs.

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观测天体数据

星座:蠍虎座
右阿森松:22h05m13.07s
赤纬:+49°18'45.5"
视星:8.247
距离:254.453 天文距离
右阿森松适当运动:0.2
赤纬适当运动:-14.9
B-T magnitude:8.409
V-T magnitude:8.261

目录:
适当名称   (Edit)
HD 1989HD 209856
TYCHO-2 2000TYC 3613-1887-1
USNO-A2.0USNO-A2 1350-15761687
HIPHIP 109026

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