Checking: python3-jplephem-2.24-2.fc42.noarch.rpm
          python3-jplephem-2.24-2.fc42.src.rpm
============================ rpmlint session starts ============================
rpmlint: 2.8.0
configuration:
    /usr/lib/python3.14/site-packages/rpmlint/configdefaults.toml
    /etc/xdg/rpmlint/fedora-spdx-licenses.toml
    /etc/xdg/rpmlint/fedora.toml
    /etc/xdg/rpmlint/scoring.toml
    /etc/xdg/rpmlint/users-groups.toml
    /etc/xdg/rpmlint/warn-on-functions.toml
rpmlintrc: [PosixPath('/tmp/tmphsxe0_m9')]
checks: 32, packages: 2

python3-jplephem.noarch: E: spelling-error ('ephemeris', 'Summary(en_US) ephemeris -> hemispheric, hemispheres, hemisphere')
python3-jplephem.noarch: E: spelling-error ('ephemerides', '%description -l en_US ephemerides -> shepherdesses, shepherdess')
python3-jplephem.src: E: spelling-error ('ephemeris', 'Summary(en_US) ephemeris -> hemispheric, hemispheres, hemisphere')
python3-jplephem.src: E: spelling-error ('ephemerides', '%description -l en_US ephemerides -> shepherdesses, shepherdess')
python3-jplephem.spec: W: no-%check-section
python3-jplephem.noarch: W: incoherent-version-in-changelog 2.24 ['2.24-2.fc42', '2.24-2']
python3-jplephem.noarch: E: description-line-too-long A Python implementation of the math that standard JPL ephemerides use to predict raw (x,y,z) planetary positions.
python3-jplephem.src: E: description-line-too-long A Python implementation of the math that standard JPL ephemerides use to predict raw (x,y,z) planetary positions.
 2 packages and 0 specfiles checked; 6 errors, 2 warnings, 7 filtered, 6 badness; has taken 0.3 s