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Double Star Calculator - Orbital Elements
- Revision:
$Rev: 1216 $
- Report created:
2025-07-11 17:03:10
WDS:
BU1295AB
WDS ID/Discoverer
P:
26.340
Orbital period (years)
a:
0.1727
Semi-major axis (arcseconds)
i:
138.4
Inclination (degrees)
Ω:
12.6
Longitude of ascending node (degrees)
T:
1988.980
Epoch of periastron passage (year)
e:
0.846
Eccentricity
ω:
42.9
Longitude of periastron (degrees)
Start-Year:
2012.0
Year
End-Year:
2038.0
Year
Epoch:
2025.0
Besselian Epoch
Position:
043958.03+532823.7
Epoch-2000 right ascension and declination
WDS-ID:
04400+5328
WDS designation
Discoverer Code:
BU1295AB
Discover designation and components
ADS number:
3358
Aitken Double Star catalog
HD number:
29316
HD catalog number
Hipparcos number:
21730
Hipparcos catalog number
V1:
7.35
Magnitude of the primary
V2:
5.86
Magnitude of the secondary
Equinox:
Equinox
Date:
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 0.281 164.8
-------------------------
2012.0 0.141 124.6
2013.0 0.110 114.2
2014.0 0.075 94.6
2015.0 0.037 36.6
2016.0 0.059 217.7
2017.0 0.118 195.3
2018.0 0.159 186.7
2019.0 0.191 181.4
2020.0 0.216 177.5
2021.0 0.236 174.3
2022.0 0.252 171.6
2023.0 0.265 169.1
2024.0 0.274 166.9
2025.0 0.281 164.8
2026.0 0.285 162.8
2027.0 0.286 160.8
2028.0 0.286 158.8
2029.0 0.283 156.8
2030.0 0.277 154.7
2031.0 0.270 152.5
2032.0 0.260 150.2
2033.0 0.249 147.7
2034.0 0.234 144.9
2035.0 0.218 141.8
2036.0 0.198 138.0
2037.0 0.176 133.4
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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