Trigonometric series for the coordinate of the objects in the solar system II, the Outer Planets.
Trigonometric series for approximate positions of some objects in the solar system have been developed by a nonlinear method of least squares. These give heliocentric and geocentric positions of the five outer planets. They are valid for the years 1950 to 2060 with a precision of 1". Key Words: method of least squares-trigonometric series-coordinates of celestial objects-multi-periodic phenomena
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| Main Author: | |
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| Format: | Journal Contribution biblioteca |
| Language: | Japanese |
| Published: |
1981
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| Online Access: | http://hdl.handle.net/1834/16250 |
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