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Double Star Calculator - Orbital Elements
- Revision:
$Rev: 1216 $
- Report created:
2025-07-11 17:57:21
WDS:
BAG32CA,CB
WDS ID/Discoverer
P:
26.500
Orbital period (years)
a:
0.1109
Semi-major axis (arcseconds)
i:
91.1
Inclination (degrees)
Ω:
126.3
Longitude of ascending node (degrees)
T:
1915.000
Epoch of periastron passage (year)
e:
0.6
Eccentricity
ω:
277.3
Longitude of periastron (degrees)
Start-Year:
2012.0
Year
End-Year:
2038.0
Year
Epoch:
2025.0
Besselian Epoch
Position:
101936.27+195212.0
Epoch-2000 right ascension and declination
WDS-ID:
10200+1950
WDS designation
Discoverer Code:
BAG32CA,CB
Discover designation and components
ADS number:
7724
Aitken Double Star catalog
HD number:
.
HD catalog number
Hipparcos number:
.
Hipparcos catalog number
V1:
9.64
Magnitude of the primary
V2:
.
Magnitude of the secondary
Equinox:
Equinox
Date:
1942
Date of last observation
Orbit grade:
9
Orbit grade, ranging from 1 'definitive' to 5 'indeterminate'
Flags:
n
Flags
Image from the USNO WDS 6th Orbit Catalog (see Acknowledgements)
Click to expand/collapse ephemeris:
Year Sep[“] PA[°]
---------------------------------------------
2025.0 0.080 125.3
-------------------------
2012.0 0.073 308.5
2013.0 0.082 308.1
2014.0 0.090 307.7
2015.0 0.095 307.4
2016.0 0.098 307.2
2017.0 0.096 306.9
2018.0 0.089 306.6
2019.0 0.073 306.2
2020.0 0.043 305.4
2021.0 0.006 134.8
2022.0 0.050 126.8
2023.0 0.072 126.1
2024.0 0.080 125.7
2025.0 0.080 125.3
2026.0 0.075 124.8
2027.0 0.067 124.3
2028.0 0.057 123.7
2029.0 0.046 122.7
2030.0 0.033 121.0
2031.0 0.021 117.3
2032.0 0.008 101.6
2033.0 0.007 335.5
2034.0 0.020 316.3
2035.0 0.032 312.2
2036.0 0.045 310.5
2037.0 0.057 309.5
This result is provided without warranty. For all terms, see the Full Disclaimer .
Copyright (C) 2025. The Double Star Calculator and the results generated are licensed under CC BY-NC-SA 4.0 .
The Double Star Calculator - Orbital Elements makes use of the Washington Double Star Sixth Catalog of Orbits of Visual Binary Stars, maintained at the U.S. Naval Observatory .
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