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authorYuri Chornoivan <yurchor@ukr.net>2016-10-03 11:10:53 (GMT)
committerYuri Chornoivan <yurchor@ukr.net>2016-10-03 11:10:53 (GMT)
commit3bccca1c952ed678859b51944447dbb9214e7a5e (patch)
tree5fcf64d746dd2f1560c16de426317f30916ad6fd
parent448aafe4c8e03021bb7e956cd5296bb4be3263d5 (diff)
Fix minor typo
-rw-r--r--kstars/kstars.kcfg2
1 files changed, 1 insertions, 1 deletions
diff --git a/kstars/kstars.kcfg b/kstars/kstars.kcfg
index b470722..b1c647b 100644
--- a/kstars/kstars.kcfg
+++ b/kstars/kstars.kcfg
@@ -762,7 +762,7 @@
<whatsthis>Check this if you use a large Dobsonian telescope.
Sorting by percentage current altitude is an easy way of determining what objects are well-placed for observation.
However, when using a large Dobsonian telescope, objects close to the zenith are hard to observe.
- Since tracking there corresponds to a rotation in azimuith, it is both counterintuitive and requires the observer to frequently move the ladder.
+ Since tracking there corresponds to a rotation in azimuth, it is both counterintuitive and requires the observer to frequently move the ladder.
The region around the zenith where this is particularly frustrating is called the Dobsonian hole.
This checkbox makes the observing list consider objects present in the hole as unfit for observation.</whatsthis>
<default>false</default>