jplephem 2.21+ds-1 source package in Ubuntu

Changelog

jplephem (2.21+ds-1) unstable; urgency=medium

  * New upstream release.

 -- Antonio Valentino <email address hidden>  Wed, 06 Dec 2023 06:59:08 +0000

Upload details

Uploaded by:
Debian Astronomy Maintainers
Uploaded to:
Sid
Original maintainer:
Debian Astronomy Maintainers
Architectures:
all
Section:
misc
Urgency:
Medium Urgency

See full publishing history Publishing

Series Pocket Published Component Section
Noble release universe misc

Builds

Noble: [FULLYBUILT] amd64

Downloads

File Size SHA-256 Checksum
jplephem_2.21+ds-1.dsc 2.1 KiB 7b930e1fbbf0e5875c63c23e4dfa88e72a2990bc64ef50ac0d5350602863da76
jplephem_2.21+ds.orig.tar.xz 34.3 KiB f2453cfca74232fbddd5dd94290c32b3ec3f37454d85dcdf9efa5c7355b67f26
jplephem_2.21+ds-1.debian.tar.xz 4.3 KiB 6693db4162d7e84cd47847a2e057cf0e9197a5d78e90693b7b4ce218f9d15460

Available diffs

No changes file available.

Binary packages built by this source

python3-jplephem: Use a JPL ephemeris to predict planet positions

 This package can load and use a Jet Propulsion Laboratory (JPL)
 ephemeris for predicting the position and velocity of a planet or other
 Solar System body. It currently supports binary SPK files (extension
 ".bsp") like those distributed by the Jet Propulsion Laboratory
 that are:
 .
  * Type 2 - positions stored as Chebyshev polynomials, with velocity
    derived by computing their derivative.
  * Type 3 - positions and velocities both stored explicitly as
    Chebyshev polynomials.
  * Type 9 - a series of discrete positions and velocities, with
    separate timestamps that do not need to be equally spaced. Currently
    there is only support for linear interpolation: for Type 9 ephemerides
    of polynomial degree 1, not of any higher degrees.
 .
 Even if an ephemeris isn't one of the above types, it is still possible
 to use jplephem to read its text comment and list the segments inside.