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author | tpearson <tpearson@283d02a7-25f6-0310-bc7c-ecb5cbfe19da> | 2011-06-11 04:44:41 +0000 |
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committer | tpearson <tpearson@283d02a7-25f6-0310-bc7c-ecb5cbfe19da> | 2011-06-11 04:44:41 +0000 |
commit | a374efce3a207b39514be3c52264091400ce297e (patch) | |
tree | 77bdf654b55826d4f59b53a5621310206bcaead1 /kstars/kstars/kssun.cpp | |
parent | f81a494f3957d5cf38c787973415597941934727 (diff) | |
download | tdeedu-a374efce3a207b39514be3c52264091400ce297e.tar.gz tdeedu-a374efce3a207b39514be3c52264091400ce297e.zip |
TQt4 port kdeedu
This enables compilation under both Qt3 and Qt4
git-svn-id: svn://anonsvn.kde.org/home/kde/branches/trinity/kdeedu@1236073 283d02a7-25f6-0310-bc7c-ecb5cbfe19da
Diffstat (limited to 'kstars/kstars/kssun.cpp')
-rw-r--r-- | kstars/kstars/kssun.cpp | 2 |
1 files changed, 1 insertions, 1 deletions
diff --git a/kstars/kstars/kssun.cpp b/kstars/kstars/kssun.cpp index 5df14c59..fc9b312d 100644 --- a/kstars/kstars/kssun.cpp +++ b/kstars/kstars/kssun.cpp @@ -125,7 +125,7 @@ bool KSSun::findGeocentricPosition( const KSNumbers *num, const KSPlanetBase *Ea nutate(num); aberrate(num); - // We obtain the apparent geocentric ecliptic coordinates. That is, after + // We obtain the aptqparent geocentric ecliptic coordinates. That is, after // nutation and aberration have been applied. EquatorialToEcliptic( num->obliquity() ); |