Basic data (System:1727)

C1900.0 :12148-0007
C2000.0 :121954357-00400049
Comp. :AB
Magn. : 3.89(V)
Spect. :A2IV


Identifiers:

Bayer $\eta$ VirBD +00 2926Flamsteed 15 VirGAIADR2 3695061317956684160
GAIADR3 3695061317956684160HD 107259HIP 60129HR 4689


Orbit

ElementValueStd. dev.
Period (d.):4791.9
Periastron time (xJD-2,400,000.0):38323.41
Reference T0/epoch:JD
Eccentricity:0.079
omega primary (deg.):1.4
K1 (km/s):4.820.24
K2 (km/s):
V0 (km/s):5.240.19
sigma residuals primary:
sigma residuals secondary:
#RV primary:71
#RV secondary:
Grade:3.0
Contributor:CHA
Status:PUB
Bibcode:1992AJ....103.1976H
Derived quantities (on the fly, from the above quantities)
a1sini (km):3.16613e+080
f(m) (sol.mass):0.05528820

Note

Abstract:
Eta Virginis is a bright (V = 3.89) triple system of composite
spectral type A2IV that has been observed for over a dozen years with
both spectroscopy and speckle interferometry. Analysis of the speckle
observations results in a long period of 13.1 years. This period is
also detected in residuals from the spectroscopic observations of the
71.7919-day short-period orbit. Elements of the long-period orbit
were determined separately using the observations of both techniques.
The more accurate elements from the speckle solution have been assumed
in a simultaneous spectroscopic determination of the short- and
long-period orbital elements.  The magnitude difference of the speckle
components suggests that lines of the third star should be visible in
the spectrum.  In our blue and red spectra only the Mg II line at 4481
angstroms appears to show a third component, however, and it is a very
broad and weak feature.  The equatorial rotational velocities of the
short-period pair are quite low, about 8 km/s each.

Radial velocities used in this orbit

xJDRad.Vel.O-C or errorWeightComponentOffsetComment
-2,400,000.0(km/s)(km/s)(km/s)
17710.6300.101a
17714.7500.701a
17716.6301.201a
17739.6103.601a
17989.8805.001a
18021.8105.801a
18031.8203.701a
18052.6204.601a
18077.6203.301a
18087.5802.601a
18089.6007.301a
18103.6105.401a
18355.7905.701a
18642.93010.001a
18706.74010.001a
18727.8209.901a
18736.7308.201a
18753.7909.001a
18757.9109.601a
18759.79010.601a
18764.70010.201a
43670.6059.501a
43671.6489.201a
44040.6165.501a
44178.0235.301a
44356.8343.601a
44357.6994.401a
44738.7432.301a
44739.7412.401a
45074.8431.101a
45075.7992.601a
45076.7691.501a
45078.8082.201a
45723.0090.701a
45784.8222.201a
45814.6721.001a
45855.7150.701a
46534.7093.601a
46583.7404.001a
46586.7164.201a
46866.8836.001a
46867.7905.601a
46868.7806.201a
46970.7236.801a
46971.6976.101a
46972.7195.301a
46974.6916.501a
47151.0358.201a
47152.0407.901a
47153.0777.301a
47244.8578.501a
47245.7527.901a
47246.9038.901a
47247.8978.401a
47248.9008.401a
47308.8078.301a
47309.8338.401a
47310.8218.401a
47312.8198.401a
47313.7819.301a
47555.9849.501a
47556.98810.701a
47623.76810.501a
47625.65310.001a
47626.83210.501a
47916.0509.501a
48004.75610.101a
48007.78110.301a
48056.64511.001a
48057.63311.001a
48345.7949.401a


Plot

Orbit
Encapsulated PostScript file

T. Merle

Valid HTML 4.01 Transitional