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-rw-r--r--kstars/kstars/kstarsdatetime.cpp2
1 files changed, 1 insertions, 1 deletions
diff --git a/kstars/kstars/kstarsdatetime.cpp b/kstars/kstars/kstarsdatetime.cpp
index b99a6173..25c3be0b 100644
--- a/kstars/kstars/kstarsdatetime.cpp
+++ b/kstars/kstars/kstarsdatetime.cpp
@@ -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 aptqparent sidereal time, we have to correct the
+ // To obtain the apparent 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.