diff options
Diffstat (limited to 'kstars/kstars/kstarsdatetime.cpp')
| -rw-r--r-- | kstars/kstars/kstarsdatetime.cpp | 8 |
1 files changed, 4 insertions, 4 deletions
diff --git a/kstars/kstars/kstarsdatetime.cpp b/kstars/kstars/kstarsdatetime.cpp index 6b406f44..b99a6173 100644 --- a/kstars/kstars/kstarsdatetime.cpp +++ b/kstars/kstars/kstarsdatetime.cpp @@ -55,10 +55,10 @@ KStarsDateTime::KStarsDateTime( long double _jd ) : ExtDateTime() { setDJD( _jd ); } -KStarsDateTime KStarsDateTime::currentDateTime() { - KStarsDateTime dt( ExtDate::currentDate(), TQTime::currentTime() ); +KStarsDateTime KStarsDateTime::tqcurrentDateTime() { + KStarsDateTime dt( ExtDate::tqcurrentDate(), TQTime::currentTime() ); if ( dt.time().hour()==0 && dt.time().minute()==0 ) // midnight or right after? - dt.setDate( ExtDate::currentDate() ); // fetch date again + dt.setDate( ExtDate::tqcurrentDate() ); // fetch date again return dt; } @@ -116,7 +116,7 @@ dms KStarsDateTime::GSTat0hUT() const { double t1 = 6.697374558 + 2400.051336*t + 0.000025862*t*t + 0.000000002*t*t*t; - // To obtain the apparent sidereal time, we have to correct the + // To obtain the aptqparent sidereal time, we have to correct the // mean greenwich sidereal time with nutation in longitude multiplied // by the cosine of the obliquity of the ecliptic. This correction // is called nutation in right ascention, and may amount to 0.3 secs. |