Basic data (System:947)
C1900.0 | : | 17033+5436
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C2000.0 | : | 170520116+54281215
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Comp. | : | B
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Magn. | : | 5.83
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Spect. | : | F7V
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Identifiers:
Bayer $\mu$ Dra | BD +54 1857 | Flamsteed 21 Dra | GAIADR2 1420101696287738368
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GAIADR3 1420101696287738368 | HD 154905 | HIP 83608
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Orbit
Element | | Value | Std. dev.
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Period (d.) | : | 2270. |
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Periastron time (xJD-2,400,000.0) | : | 42309. |
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Reference T0/epoch | : | JD
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Eccentricity | : | 0.43 |
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omega primary (deg.) | : | 205. |
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K1 (km/s) | : | 2.8 |
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K2 (km/s) | : | |
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V0 (km/s) | : | -16.5 |
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sigma residuals primary | : |
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sigma residuals secondary | : |
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#RV primary | : |
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#RV secondary | : |
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Grade | : | 1.0
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Contributor | : | DAO
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Status | : | PUB
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Bibcode | : | 1979AnTok..17..158I
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Derived quantities (on the fly, from the above quantities) |
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a1sini (km) | : | 7.89084e+07 | 0
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f(m) (sol.mass) | : | 0.00381398 | 0
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Note
This is the fainter component of A.D.S. 10345, for which a number of orbits
have been computed. Even the period of the visual pair is uncertain, however,
except for the fact that it is to be measured in centuries. The component A is
similar in magnitude and spectral type. Ishida finds evidence for a
low-amplitude variation in the velocity of B, which he ascribes to binary
motion. Confirmation is desirable. There is also a companion C, 13.8m at about
13".
Plot
Encapsulated PostScript file
T. Merle