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Name: python3-ephem | Distribution: Mageia |
Version: 4.1.6 | Vendor: Mageia.Org |
Release: 1.mga10 | Build date: Thu Dec 19 09:36:38 2024 |
Group: Development/Python | Build host: localhost |
Size: 2488774 | Source RPM: python-ephem-4.1.6-1.mga10.src.rpm |
Packager: papoteur <papoteur> | |
Url: https://rhodesmill.org/pyephem/ | |
Summary: Python3 implementation of Ephem |
PyEphem provides scientific-grade astronomical computations for the Python programming language. Given a date and location on the Earth’s surface, it can compute the positions of the Sun and Moon, of the planets and their moons, and of any asteroids, comets, or earth satellites whose orbital elements the user can provide. Additional functions are provided to compute the angular separation between two objects in the sky, to determine the constellation in which an object lies, and to find the times at which an object rises, transits, and sets on a particular day. The numerical routines that lie behind PyEphem are those from the wonderful XEphem astronomy application, whose author, Elwood Downey, generously gave permission for us to use them as the basis for PyEphem.
LGPLv3
* Thu Dec 19 2024 papoteur <papoteur> 4.1.6-1.mga10 + Revision: 2126238 - new version 4.1.6 * Fri Feb 23 2024 daviddavid <daviddavid> 4.1.5-2.mga10 + Revision: 2043443 - rebuild for py3.12 * Sat Oct 21 2023 papoteur <papoteur> 4.1.5-1.mga10 + Revision: 2000003 - new 4.1.5
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Fabrice Bellet, Thu Jan 9 10:36:12 2025