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Double Star Calculator - Orbital Elements
- Revision:
$Rev: 1216 $
- Report created:
2025-07-11 16:27:50
WDS:
FIN337BC
WDS ID/Discoverer
P:
27.028
Orbital period (years)
a:
0.10855
Semi-major axis (arcseconds)
i:
16.8
Inclination (degrees)
Ω:
194.0
Longitude of ascending node (degrees)
T:
1995.040
Epoch of periastron passage (year)
e:
0.215
Eccentricity
ω:
13.0
Longitude of periastron (degrees)
Start-Year:
2012.0
Year
End-Year:
2038.0
Year
Epoch:
2025.0
Besselian Epoch
Position:
011948.33-003031.0
Epoch-2000 right ascension and declination
WDS-ID:
01198-0031
WDS designation
Discoverer Code:
FIN337BC
Discover designation and components
ADS number:
1081
Aitken Double Star catalog
HD number:
8036
HD catalog number
Hipparcos number:
6226
Hipparcos catalog number
V1:
7.4
Magnitude of the primary
V2:
7.6
Magnitude of the secondary
Equinox:
2000
Equinox
Date:
2009
Date of last observation
Orbit grade:
2
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 0.089 264.5
-------------------------
2012.0 0.124 56.9
2013.0 0.120 66.7
2014.0 0.115 77.3
2015.0 0.110 88.8
2016.0 0.105 101.4
2017.0 0.100 115.4
2018.0 0.095 130.8
2019.0 0.091 147.6
2020.0 0.088 165.8
2021.0 0.086 185.0
2022.0 0.085 205.1
2023.0 0.085 225.4
2024.0 0.086 245.4
2025.0 0.089 264.5
2026.0 0.094 282.0
2027.0 0.099 297.7
2028.0 0.105 311.7
2029.0 0.111 324.2
2030.0 0.117 335.5
2031.0 0.122 345.8
2032.0 0.126 355.3
2033.0 0.129 4.3
2034.0 0.131 13.0
2035.0 0.132 21.5
2036.0 0.131 30.0
2037.0 0.130 38.6
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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