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python313-skyfield-1.54-2.1 RPM for noarch

From OpenSuSE Ports Tumbleweed for noarch

Name: python313-skyfield Distribution: openSUSE Tumbleweed
Version: 1.54 Vendor: openSUSE
Release: 2.1 Build date: Thu Jul 16 04:10:57 2026
Group: Unspecified Build host: reproducible
Size: 2317321 Source RPM: python-skyfield-1.54-2.1.src.rpm
Packager: http://bugs.opensuse.org
Url: https://github.com/skyfielders/python-skyfield/
Summary: Elegant astronomy for Python
A Python astronomy package that makes it easy to generate high precision
research-grade positions for planets and Earth satellites.

Provides

Requires

License

MIT

Changelog

* Thu Jul 16 2026 Steve Kowalik <steven.kowalik@suse.com>
  - Due to pandas changes, add pytz to BuildRequires.
* Fri Apr 24 2026 Ben Greiner <code@bnavigator.de>
  - Update to 1.54
    * Skyfield’s internal table for the ∆T Earth orientation
      parameter has been updated, so observations extend to this
      month and predictions to January 2027. Compared to the previous
      version of Skyfield, this changes the Earth’s rotation angle by
      up to 0.2 arcseconds in 2025 and 1.1 arcseconds in 2026.
    * The apparent() method now accepts an optional deflectors=
      argument that lets callers control the list of bodies (by
      default the Sun, Jupiter, and Saturn) for which the deflection
      of light is computed. Callers can provide an empty list to turn
      deflection off.
    * The two routines find_risings() and find_settings() now skip
      deflection when computing the target’s apparent position, which
      increases their speed by around 30%. The routines aim for only
      millisecond precision, while deflection only makes a difference
      of microseconds.
    * You can now subtract a NumPy array of floating point TT days
      from a Skyfield Time object of the same length; previously,
      only a plain int or float was supported as the subtrahend.
    * Bugfix: the apparent() method in previous Skyfield versions was
      using the wrong coordinates for Earth’s center when computing
      how Earth’s gravity deflects positions for topocentric
      observers. This has been fixed, and Skyfield’s test suite shows
      that agreement with the Naval Observatory’s high-precision
      NOVAS library has improved from 0.5 mas to 0.01 mas for
      topocentric positions. (Astrometric positions were already
      agreeing at the 0.01 mas level.)
  - Skyfield v1.53
    * Fix: calling observe() on a position generated by an ephemeris
      with multiple segments per target, like DE441, was raising an
      exception
  - Skyfield v1.52
    * Fix: on rare occasions the find_risings() and find_settings()
      routines could return an invalid result if no rising or setting
      was found, instead of returning the moment of transit as their
      fallback result. #1057
    * Fix: if the altaz() method was given a position with a NaN
      coordinate, and was passed temperature_C and pressure_mbar
      parameters with which to compute refraction, then it would loop
      forever. #1046
    * Fix: the new mean_equator_and_equinox_of_date reference frame
      was off by nearly 0.02 arcseconds because it applied precession
      but forgot to apply the frame tie between ICRS and J2000.
    * To avoid deprecation warnings on recent Pythons, Skyfield now
      avoids Python’s datetime.utcnow() method, and avoids applying
      the ~ unary operator.
  - Skyfield v1.51
    * Skyfield now supports ephemeris files like de441.bsp that have
      two or more segments per target. In earlier versions of
      Skyfield, only one segment per target would get used, which for
      de441.bsp was cutting the range of supported dates in half.
      [#691]
    * The documentation now uses the newer name .xyz, which has been
      quietly supported for around three years, for the ICRF
      attribute that was originally named .position and holds its
      position vector. The old name (which will continue to be
      supported) could lead to code that looked a little redundant,
      asking for the position of a position:
      position = mars.at(t)
      x, y, z = position.position
      So Skyfield now encourages code to ask for position.xyz
      instead. An advantage is that the new name is self-documenting:
      the name reminds the user that it is a 3-vector of Cartesian
      components.
    * Skyfield’s internal table for the ∆T Earth orientation
      parameter has been updated, so that its predictions now extend
      to 2026-02-28.
    * Fix: the find_events() Earth satellite method was returning an
      empty list of events if the only event in the time period was a
      lone rising or setting. It should now detect and return them.
      [#856] #996 #1017
    * Fix: the find_events() Earth satellite method, faced with a
      single pass that was very close to the start time, was
      returning an inaccurate setting time. It should now return an
      accurate setting time. #1000
    * Fix: the find_events() Earth satellite method would miss a
      rising that came a fraction of a second before the
      corresponding culmination. It should now find both. #559
    * Fix: bodies with Kepler orbits (like comets and asteroids) were
      incorrectly returning positions with only a single dimension if
      given a Time that was an array but had only one element. This
      could cause the rising and setting almanac routines to raise a
      ValueError if they found only a single rising or setting. #959
    * Fix: the position vectors for Kepler orbit bodies, like comets
      and asteroids, now have a useful .target_name like 'Ceres' or
      '1P/Halley' instead of the less informative value 'str'.
  - Skyfield v1.50
    * A new mean_equator_and_equinox_of_date coordinate frame lets
      users generate the same coordinates that an almanac might give.
    * Skyfield now offers a Solar System Barycenter object, so users
      don’t have to construct the position themselves: SSB.at(t)
      returns a position whose coordinates and velocity are both zero
      in the ICRS.
    * The routines added last year, find_risings() and
      find_settings(), could occasionally miss a sunrise or moonrise
      at high latitudes like 70°N where the Sun or Moon barely crests
      the horizon. This has been fixed at a moderate cost to their
      runtime. #998
    * Skyfield no longer tries to protect users by raising an
      exception if, contrary to the usual custom in astronomy, they
      ask for ra.degrees or dec.hours. So users no longer need to add
      an underscore prefix (_degrees or _hours) to bypass the
      exception, though both names will keep working to support
      legacy code.
    * The time methods utc_datetime() and
      utc_datetime_and_leap_second() now intercept the ValueError
      that Python raises for a negative year or a Julian-only leap
      day, and replace the generic error message with a more specific
      one. #957 #992
    * If you call load.timescale(builtin=False) to download an
      updated copy of the IERS finals2000A.all Earth orientation data
      file, Skyfield now fetches the file with HTTPS, since their old
      FTP server seems to have disappeared. #1019
  - Skyfield v1.49
    * A new from_omm() Earth Satellite constructor has been added to
      load satellite elements from modern OMM data instead of from
      old TLE data. The Earth satellite documentation now describes
      two OMM formats and shows how to load satellites from each one.
      [#763]
    * If you print an instance of the PlanetaryConstants class to the
      screen, it will list all of the segments that it has loaded
      from binary kernels. #952
    * The Skyfield documentation is no longer installed alongside the
      Python code, reducing the size of Skyfield by around 25%. Users
      who need offline access to the documentation will now need to
      download it separately.
  - Disable python314 tests: gh#brandon-rhodes/assay#17
* Sun Mar 24 2024 Ben Greiner <code@bnavigator.de>
  - Update to 1.48
    * Times now support the ``<`` operator, so Python can sort them.
    * For convenience, geoids like :data:`~skyfield.toposlib.wgs84`
      have a new attribute
      :data:`~skyfield.toposlib.Geoid.polar_radius`.
    * You can no longer subtract two positions unless they have the
      same ``.center``.  Otherwise, a ``ValueError`` is raised.  This
      check has always been performed when you subtract vector
      functions, but it was missing from the position subtraction
      routine.
    * On days that the Sun fails to rise and set in the Arctic and
      Antarctic, the new rising and setting routines now correctly
      set the value ``False`` not only for sunrise but also for
      sunset.
  - Reenable Python 3.12 testing with a new assay
* Sun Feb 04 2024 Ben Greiner <code@bnavigator.de>
  - Update to 1.47
    * Added faster and more accurate almanac routines
      :func:`~skyfield.almanac.find_risings()` and
      :func:`~skyfield.almanac.find_settings()` and
      :func:`~skyfield.almanac.find_transits()`.
    * Skyfield’s internal table for the ∆T Earth orientation
      parameter has been updated, so that its predictions now extend
      to 2025-01-18.
    * Constellation abbreviations are now consistent between the
      :func:`~skyfield.api.load_constellation_map()` table and the
      :func:`~skyfield.api.load_constellation_names()` list.
      Previously, ``CVn`` and ``TrA`` had been mis-capitalized in the
      list as ``Cvn`` and ``Tra``.
  - Skip testing python312: gh#brandon-rhodes/assay#15 still an issue
* Fri Nov 24 2023 Paolo Stivanin <info@paolostivanin.com>
  - Update to 1.46:
    * The :func:`~skyfield.almanac.oppositions_conjunctions()` routine
      now measures ecliptic longitude using the ecliptic of each
      specific date, rather than always using the J2000 ecliptic,
      which should improve its accuracy by several seconds.
    * Skyfield’s internal table for the ∆T Earth orientation parameter
      has been updated, so that its predictions now extend to 2024-04-13.
    * Bugfix: Skyfield was giving values several kilometers off
      when computing the elevation above ground level of a target that
      was positioned directly above the Earth’s north or south pole.
    * Bugfix: the function skyfield.positionlib.ICRF.is_behind_earth()
      method was incorrectly returning True if the Earth was on the
      line that joins the two satellites, but over on the far side of
      the other satellite where it wasn’t really in the way.
    * The method skyfield.positionlib.ICRF.altaz() now lives on the
      main position class instead of in two specific subclasses.
      If the user mistakenly tries to call .altaz() on an instance
      of the skyfield.positionlib.Astrometric position
      subclass - which previously lacked the method - then a friendly
      exception is raised explaining their error.
* Sun Feb 19 2023 Ben Greiner <code@bnavigator.de>
  - Don't build for python311: gh#brandon-rhodes/assay#15
* Sat Jan 21 2023 Ben Greiner <code@bnavigator.de>
  - Update to v1.45
    * Bugfix: minor planets and comets in Skyfield 1.44 would raise
      an exception if asked for a position in the half of their orbit
      where they are inbound towards their perihelion.
  - Changelog v1.44
    * Skyfield’s internal table for the ∆T Earth orientation
      parameter has been updated, so that instead of including
      measurements only through December 2021 it now knows Earth
      orientation through September 2022.
    * Distance and velocity objects can now be created by calling
      their unit names as constructors, like d = Distance.km(5.0) and
      v = Velocity.km_per_s(0.343).
    * Updated the URL from which the Hipparcos database hip_main.dat
      is downloaded, following a change in the domain for the
      University of Strasbourg from u-strasbg.fr to unistra.fr.
* Thu Aug 11 2022 Ben Greiner <code@bnavigator.de>
  - Update to v1.43.1
    * An attempt at overly clever scripting resulted in a Skyfield
      1.43 release without a setup.py in its .tar.gz; within an hour,
      a Python 2.7 user had reported that Skyfield could no longer
      install. This release is identical to 1.43 but (hopefully)
      installs correctly for everyone!
  - Changelog v1.43
    * Fixed planetary_magnitude() so it works for Saturn even when
      the time is an array rather than a single time; also, improved
      its calculation slightly with respect to Uranus. #739
    * Improved load_comets_dataframe() so that parsing CometEls.txt
      with the most recent version of Pandas doesn’t stumble over the
      commas in the final field of (for example) Halley’s Comet and
      give the error ParserError: Error tokenizing data. C error:
      Expected 12 fields…saw 13. #707
  - Changelog v1.42
    * Added two new position methods phase_angle() and
      fraction_illuminated() that, given an illuminator (usually the
      Sun) as their argument, compute whether the observer is looking
      at the bright side or the dark side of the target body. They
      replace a pair of old functions in the almanac module.
    * The almanac routine moon_nodes() would sometimes skip nodes
      that were closer together than 14.0 days. It has been tightened
      down and should now detect all lunar nodes. #662
    * Time objects now feature a to_astropy() method.
    * The position method to_skycoord() now sets the frame attribute
      of the sky coordinate it returns, and for now only supports
      barycentric and geocentric positions. #577
  - Changelog v1.41
    * Times now support arithmetic: you can add or subtract from a
      time either a number representing days of Terrestrial Time (TT)
      or a Python timedelta which Skyfield interprets as TT days and
      seconds. #568
    * Fixed the .itrs_xyz vector of the geographic position returned
      by the subpoint_of() method. #673
    * Skyfield now uses HTTPS instead of FTP to download JPL
      ephemeris files like de421.bsp. This does risk raising an error
      for users whose machines have out-of-date root certificates.
      But it protects the connection from outside tampering, and will
      keep working if the ssd.jpl.nasa.gov FTP service is ever shut
      down — as happened earlier this year to FTP on NASA’s
      cddis.nasa.gov server. #666
  - Changelog v1.40
    * Extended the planetary_magnitude() routine to work with all the
      major planets, which upgrades it from a prototype feature to a
      production feature of Skyfield.
    * The subpoint() method has been deprecated, because users
      reported that its name was a poor match for its behavior. Four
      new methods have replaced it: latlon_of(), height_of(),
      geographic_position_of(), and subpoint_of(). #644
    * Added a timescale method linspace(). #617
    * The oppositions_conjunctions() routine, which was originally
      designed only for planets, can now also handle the Moon (which
      moves from opposition to conjunction much faster).
  - Update assay to 264.bb62d1f: better pickling handling
  - Update finals200A.all data
* Wed Apr 20 2022 pgajdos@suse.com
  - python-mock is not required for build
* Fri Aug 27 2021 Ben Greiner <code@bnavigator.de>
  - Run assay up to 3 times in case of flaky pickling errors

Files

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Fabrice Bellet, Sun Aug 2 03:14:27 2026