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-rw-r--r--kstars/kstars/ksplanet.h6
1 files changed, 3 insertions, 3 deletions
diff --git a/kstars/kstars/ksplanet.h b/kstars/kstars/ksplanet.h
index c30e40e7..5e66b879 100644
--- a/kstars/kstars/ksplanet.h
+++ b/kstars/kstars/ksplanet.h
@@ -30,7 +30,7 @@
*(Earth and Pluto have their own specialized classes derived from KSPlanetBase).
*@note The Sun is subclassed from KSPlanet.
*
- *KSPlanet contains internal classes to manage the computations of a planet's position.
+ *KSPlanet tqcontains internal classes to manage the computations of a planet's position.
*The position is computed as a series of sinusoidal sums, similar to a Fourier
*transform. See "Astronomical Algorithms" by Jean Meeus or the file README.planetmath
*for details.
@@ -83,7 +83,7 @@ protected:
virtual bool findGeocentricPosition( const KSNumbers *num, const KSPlanetBase *Earth=NULL );
/**@class OrbitData
- *This class contains doubles A,B,C which represent a single term in a planet's
+ *This class tqcontains doubles A,B,C which represent a single term in a planet's
*positional expansion sums (each sum-term is A*COS(B+C*T)).
*@author Mark Hollomon
*@version 1.0
@@ -103,7 +103,7 @@ protected:
typedef TQPtrVector<OrbitData> OBArray[6];
-/**OrbitDataColl contains three groups of six QPtrVectors. Each TQPtrVector is a
+/**OrbitDataColl tqcontains three groups of six QPtrVectors. Each TQPtrVector is a
*list of OrbitData objects, representing a single sum used in computing
*the planet's position. A set of six of these vectors comprises the large
*"meta-sum" which yields the planet's Longitude, Latitude, or Distance value.