en:documentation:computation_method_and_precision
Differences
This shows you the differences between two versions of the page.
| Both sides previous revisionPrevious revision | |||
| en:documentation:computation_method_and_precision [2018/12/06 10:38] – [Comets and asteroids equatorial positions] pch | en:documentation:computation_method_and_precision [2018/12/06 11:34] (current) – [Planets equatorial positions] pch | ||
|---|---|---|---|
| Line 28: | Line 28: | ||
| The position of the planets are computed using the JPL ephemeris or if no file are found for the current date, the library [[http:// | The position of the planets are computed using the JPL ephemeris or if no file are found for the current date, the library [[http:// | ||
| - | By default an extract of DE405 valid between 2000 and 2050 is supplied with the program. So the first thing to do if you want long term high precision planet position is to install a [[ftp:// | + | By default an extract of DE430 valid between 2000 and 2050 is supplied with the program. So the first thing to do if you want long term high precision planet position is to install a [[ftp:// |
| DE431 is recommended if you can afford the 2.5GB download. With this file you can compute precise planet position and nutation between -13000 and +17000. | DE431 is recommended if you can afford the 2.5GB download. With this file you can compute precise planet position and nutation between -13000 and +17000. | ||
en/documentation/computation_method_and_precision.1544089116.txt.gz · Last modified: 2018/12/06 10:38 by pch
