Beautify docbook files

1 files changed, 5 insertions, 40 deletions

diff --git a/tde-i18n-en_GB/docs/tdeedu/kstars/equinox.docbook b/tde-i18n-en_GB/docs/tdeedu/kstars/equinox.docbook
index 8b4a0611550..8cc41f4568e 100644
--- a/tde-i18n-en_GB/docs/tdeedu/kstars/equinox.docbook
+++ b/tde-i18n-en_GB/docs/tdeedu/kstars/equinox.docbook
@@ -1,44 +1,9 @@
 <sect1 id="ai-equinox">
 <sect1info>
-<author
-><firstname
->Jason</firstname
-> <surname
->Harris</surname
-> </author>
+<author><firstname>Jason</firstname> <surname>Harris</surname> </author>
 </sect1info>
-<title
->The Equinoxes</title>
-<indexterm
-><primary
->Equinoxes</primary>
-<seealso
->Celestial Equator</seealso
-> <seealso
->Ecliptic</seealso
-> </indexterm>
-<para
->Most people know the Vernal and Autumnal Equinoxes as calendar dates, signifying the beginning of the Northern hemisphere's Spring and Autumn, respectively. Did you know that the equinoxes are also positions in the sky? </para
-><para
->The <link linkend="ai-cequator"
->Celestial Equator</link
-> and the <link linkend="ai-ecliptic"
->Ecliptic</link
-> are two <link linkend="ai-greatcircle"
->Great Circles</link
-> on the <link linkend="ai-csphere"
->Celestial Sphere</link
->, set at an angle of 23.5 degrees. The two points where they intersect are called the <firstterm
->Equinoxes</firstterm
->. The <firstterm
->Vernal Equinox</firstterm
-> has coordinates RA=0.0 hours, Dec=0.0 degrees. The <firstterm
->Autumnal Equinox</firstterm
-> has coordinates RA=12.0 hours, Dec=0.0 degrees. </para
-><para
->The Equinoxes are important for marking the seasons. Because they are on the <link linkend="ai-ecliptic"
->Ecliptic</link
->, the Sun passes through each equinox every year. When the Sun passes through the Vernal Equinox (usually on March 21st), it crosses the <link linkend="ai-cequator"
->Celestial Equator</link
-> from South to North, signifying the end of Winter for the Northern hemisphere. Similarly, whenthe Sun passes through the Autumnal Equinox (usually on September 21st), it crosses the Celestial Equator from North to South, signifying the end of Winter for the Southern hemisphere. </para>
+<title>The Equinoxes</title>
+<indexterm><primary>Equinoxes</primary>
+<seealso>Celestial Equator</seealso> <seealso>Ecliptic</seealso> </indexterm>
+<para>Most people know the Vernal and Autumnal Equinoxes as calendar dates, signifying the beginning of the Northern hemisphere's Spring and Autumn, respectively. Did you know that the equinoxes are also positions in the sky? </para><para>The <link linkend="ai-cequator">Celestial Equator</link> and the <link linkend="ai-ecliptic">Ecliptic</link> are two <link linkend="ai-greatcircle">Great Circles</link> on the <link linkend="ai-csphere">Celestial Sphere</link>, set at an angle of 23.5 degrees. The two points where they intersect are called the <firstterm>Equinoxes</firstterm>. The <firstterm>Vernal Equinox</firstterm> has coordinates RA=0.0 hours, Dec=0.0 degrees. The <firstterm>Autumnal Equinox</firstterm> has coordinates RA=12.0 hours, Dec=0.0 degrees. </para><para>The Equinoxes are important for marking the seasons. Because they are on the <link linkend="ai-ecliptic">Ecliptic</link>, the Sun passes through each equinox every year. When the Sun passes through the Vernal Equinox (usually on March 21st), it crosses the <link linkend="ai-cequator">Celestial Equator</link> from South to North, signifying the end of Winter for the Northern hemisphere. Similarly, whenthe Sun passes through the Autumnal Equinox (usually on September 21st), it crosses the Celestial Equator from North to South, signifying the end of Winter for the Southern hemisphere. </para>
 </sect1>