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authortpearson <tpearson@283d02a7-25f6-0310-bc7c-ecb5cbfe19da>2011-06-11 04:44:41 +0000
committertpearson <tpearson@283d02a7-25f6-0310-bc7c-ecb5cbfe19da>2011-06-11 04:44:41 +0000
commita374efce3a207b39514be3c52264091400ce297e (patch)
tree77bdf654b55826d4f59b53a5621310206bcaead1 /kstars/kstars/kssun.cpp
parentf81a494f3957d5cf38c787973415597941934727 (diff)
downloadtdeedu-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.cpp2
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() );