From 0b8ca6637be94f7814cafa7d01ad4699672ff336 Mon Sep 17 00:00:00 2001 From: Darrell Anderson Date: Tue, 21 Jan 2014 22:06:48 -0600 Subject: Beautify docbook files --- tde-i18n-en_GB/docs/tdeedu/kstars/meridian.docbook | 41 +++------------------- 1 file changed, 5 insertions(+), 36 deletions(-) (limited to 'tde-i18n-en_GB/docs/tdeedu/kstars/meridian.docbook') diff --git a/tde-i18n-en_GB/docs/tdeedu/kstars/meridian.docbook b/tde-i18n-en_GB/docs/tdeedu/kstars/meridian.docbook index 067464da584..17284fabcf8 100644 --- a/tde-i18n-en_GB/docs/tdeedu/kstars/meridian.docbook +++ b/tde-i18n-en_GB/docs/tdeedu/kstars/meridian.docbook @@ -1,41 +1,10 @@ -Jason Harris +Jason Harris -The Local Meridian -Local Meridian -Hour Angle Celestial Sphere -The Local Meridian is an imaginary Great Circle on the Celestial Sphere that is perpendicular to the local Horizon. It passes through the North point on the Horizon, through the Celestial Pole, up to the Zenith, and through the South point on the Horizon. Because it is fixed to the local Horizon, stars will appear to drift past the Local Meridian as the Earth spins. You can use an object's Right Ascension and the Local Sidereal Time to determine when it will cross your Local Meridian (see Hour Angle). +The Local Meridian +Local Meridian +Hour Angle Celestial Sphere +The Local Meridian is an imaginary Great Circle on the Celestial Sphere that is perpendicular to the local Horizon. It passes through the North point on the Horizon, through the Celestial Pole, up to the Zenith, and through the South point on the Horizon. Because it is fixed to the local Horizon, stars will appear to drift past the Local Meridian as the Earth spins. You can use an object's Right Ascension and the Local Sidereal Time to determine when it will cross your Local Meridian (see Hour Angle). -- cgit v1.2.1