document.write('<table width=100% cellspacing=1 cellpadding=3 border=0><tr><td align=\'Left\' width=100% valign=top ><font face=\'Times\' size=\'2\' color=\'#000000\'><a href=\'http:\/\/www.classicalastronomy.com\/news\/anmviewer.asp?a=45&z=19\'><b>Time Zones<\/b><\/a><\/font><br><font face=\'Times\' size=\'2\' color=\'#000000\'>Our modern time zones are another proof that the Earth is spherical in shape. <\/font><a href=\'http:\/\/www.classicalastronomy.com\/news\/anmviewer.asp?a=45&z=19\'><\/a><\/font><\/td><\/tr><tr><td align=\'Left\' width=100% valign=top ><font face=\'Times\' size=\'2\' color=\'#000000\'><a href=\'http:\/\/www.classicalastronomy.com\/news\/anmviewer.asp?a=46&z=19\'><b>The Sky Down Under - Our Visit to the Southern Hemisphere<\/b><\/a><\/font><br><font face=\'Times\' size=\'2\' color=\'#000000\'>A trip from the USA to New Zealand helps illustrate the differences between the sky of the northern hemisphere and the southern hemisphere.<\/font><a href=\'http:\/\/www.classicalastronomy.com\/news\/anmviewer.asp?a=46&z=19\'><\/a><\/font><\/td><\/tr><tr><td align=\'Left\' width=100% valign=top ><font face=\'Times\' size=\'2\' color=\'#000000\'><a href=\'http:\/\/www.classicalastronomy.com\/news\/anmviewer.asp?a=176&z=19\'><b>Standard Time<\/b><\/a><\/font><br><font face=\'Times\' size=\'2\' color=\'#000000\'>In the modern world, we use &quot;Standard Time&quot; in which the whole world is divided into 24 time zones. As a result, on any day of the year at any latitude, the times of actual sunrise and sunset vary depending on your location within a time zone.<\/font><a href=\'http:\/\/www.classicalastronomy.com\/news\/anmviewer.asp?a=176&z=19\'><\/a><\/font><\/td><\/tr><tr><td align=\'Left\' width=100% valign=top ><font face=\'Times\' size=\'2\' color=\'#000000\'><a href=\'http:\/\/www.classicalastronomy.com\/news\/anmviewer.asp?a=161&z=19\'><b>Latitude and Declination<\/b><\/a><\/font><br><font face=\'Times\' size=\'2\' color=\'#000000\'>On the Earth, we measure position on the globe by the coordinates of latitude and longitude.  Latitude measures position from North to South.  In the sky, celestial positions are given in coordinates of &quot;Declination&quot; and &quot;Right Ascension.&quot; <\/font><a href=\'http:\/\/www.classicalastronomy.com\/news\/anmviewer.asp?a=161&z=19\'><\/a><\/font><\/td><\/tr><\/table>');