<?xml version="1.0" encoding="UTF-8"?><rss version="2.0"
	xmlns:content="http://purl.org/rss/1.0/modules/content/"
	xmlns:dc="http://purl.org/dc/elements/1.1/"
	xmlns:atom="http://www.w3.org/2005/Atom"
	xmlns:sy="http://purl.org/rss/1.0/modules/syndication/"
		>
<channel>
	<title>Comments on: Mercury from space</title>
	<atom:link href="http://thebigfoto.com/mercury-from-space/feed" rel="self" type="application/rss+xml" />
	<link>http://thebigfoto.com/mercury-from-space</link>
	<description>Life stories in photos</description>
	<lastBuildDate>Fri, 03 Feb 2012 02:20:52 +0000</lastBuildDate>
		<sy:updatePeriod>hourly</sy:updatePeriod>
	<sy:updateFrequency>1</sy:updateFrequency>
		<item>
		<title>By: Solar System</title>
		<link>http://thebigfoto.com/mercury-from-space/comment-page-1#comment-1718</link>
		<dc:creator>Solar System</dc:creator>
		<pubDate>Fri, 11 Feb 2011 15:16:14 +0000</pubDate>
		<guid isPermaLink="false">http://thebigfoto.com/?p=408#comment-1718</guid>
		<description>Fantastic pics. Can&#039;t wait till March 18th this year when Messenger will begin its orbit around Mecury.</description>
		<content:encoded><![CDATA[<p>Fantastic pics. Can&#8217;t wait till March 18th this year when Messenger will begin its orbit around Mecury.</p>
]]></content:encoded>
	</item>
	<item>
		<title>By: Mohd. Moeen H. Raza</title>
		<link>http://thebigfoto.com/mercury-from-space/comment-page-1#comment-1287</link>
		<dc:creator>Mohd. Moeen H. Raza</dc:creator>
		<pubDate>Sat, 20 Mar 2010 18:15:36 +0000</pubDate>
		<guid isPermaLink="false">http://thebigfoto.com/?p=408#comment-1287</guid>
		<description>Mercury (planet), second smallest of the planets in the solar system. Mercury orbits closest to the Sun of all the planets, at an average distance of approximately 58 million km (about 36 million mi, or 0.3871 astronomical unit (AU)). An AU is equal to the average distance between the Earth and the Sun, or about 150 million km (93 million mi). The planet’s diameter is 4,879 km (3,032 mi), and its volume and mass are about one-eighteenth that of Earth. Mercury’s mean density, 5.4 g/cm³, is nearly as great as that of Earth and is higher than that of any of the other planets. The force of gravity on the planet&#039;s surface is about one-third of that on Earth&#039;s surface or about twice the surface gravity on the Moon. Mercury has no moons of its own.

Mercury revolves once about the Sun every 87.97 days. Radar observations of the planet show that it rotates only once every 58.65 days, two-thirds of its period of revolution. Only three of the planet’s days, therefore, occur during every two of its years. The side facing the Sun gets very hot, while the side facing away quickly cools to frigid temperatures. Mercury was named for the messenger of the gods in Roman mythology. 

The point in Mercury&#039;s orbit at which the planet is closest to the Sun (called the planet’s perihelion) moves a tiny amount every orbit, too much to be accounted for by the gravitational influence of other planets. The observation of these changes in Mercury&#039;s perihelion was one of the first confirmations of Einstein’s theory of relativity, which predicted their existence.</description>
		<content:encoded><![CDATA[<p>Mercury (planet), second smallest of the planets in the solar system. Mercury orbits closest to the Sun of all the planets, at an average distance of approximately 58 million km (about 36 million mi, or 0.3871 astronomical unit (AU)). An AU is equal to the average distance between the Earth and the Sun, or about 150 million km (93 million mi). The planet’s diameter is 4,879 km (3,032 mi), and its volume and mass are about one-eighteenth that of Earth. Mercury’s mean density, 5.4 g/cm³, is nearly as great as that of Earth and is higher than that of any of the other planets. The force of gravity on the planet&#8217;s surface is about one-third of that on Earth&#8217;s surface or about twice the surface gravity on the Moon. Mercury has no moons of its own.</p>
<p>Mercury revolves once about the Sun every 87.97 days. Radar observations of the planet show that it rotates only once every 58.65 days, two-thirds of its period of revolution. Only three of the planet’s days, therefore, occur during every two of its years. The side facing the Sun gets very hot, while the side facing away quickly cools to frigid temperatures. Mercury was named for the messenger of the gods in Roman mythology. </p>
<p>The point in Mercury&#8217;s orbit at which the planet is closest to the Sun (called the planet’s perihelion) moves a tiny amount every orbit, too much to be accounted for by the gravitational influence of other planets. The observation of these changes in Mercury&#8217;s perihelion was one of the first confirmations of Einstein’s theory of relativity, which predicted their existence.</p>
]]></content:encoded>
	</item>
	<item>
		<title>By: Anonymous</title>
		<link>http://thebigfoto.com/mercury-from-space/comment-page-1#comment-837</link>
		<dc:creator>Anonymous</dc:creator>
		<pubDate>Thu, 30 Jul 2009 07:07:59 +0000</pubDate>
		<guid isPermaLink="false">http://thebigfoto.com/?p=408#comment-837</guid>
		<description>this is ss amazing!!! i also really liked the Jupiter one :]</description>
		<content:encoded><![CDATA[<p>this is ss amazing!!! i also really liked the Jupiter one :]</p>
]]></content:encoded>
	</item>
	<item>
		<title>By: Anonymous</title>
		<link>http://thebigfoto.com/mercury-from-space/comment-page-1#comment-576</link>
		<dc:creator>Anonymous</dc:creator>
		<pubDate>Thu, 07 May 2009 13:39:03 +0000</pubDate>
		<guid isPermaLink="false">http://thebigfoto.com/?p=408#comment-576</guid>
		<description>cool</description>
		<content:encoded><![CDATA[<p>cool</p>
]]></content:encoded>
	</item>
	<item>
		<title>By: Akeru, astronomía para todos.&#187; Blog Archive &#187; Un tour fotográfico por el Sistema Solar</title>
		<link>http://thebigfoto.com/mercury-from-space/comment-page-1#comment-509</link>
		<dc:creator>Akeru, astronomía para todos.&#187; Blog Archive &#187; Un tour fotográfico por el Sistema Solar</dc:creator>
		<pubDate>Wed, 22 Apr 2009 10:00:10 +0000</pubDate>
		<guid isPermaLink="false">http://thebigfoto.com/?p=408#comment-509</guid>
		<description>[...] Mercurio [...]</description>
		<content:encoded><![CDATA[<p>[...] Mercurio [...]</p>
]]></content:encoded>
	</item>
	<item>
		<title>By: Jupiter from space &#124; The Big Foto</title>
		<link>http://thebigfoto.com/mercury-from-space/comment-page-1#comment-508</link>
		<dc:creator>Jupiter from space &#124; The Big Foto</dc:creator>
		<pubDate>Tue, 21 Apr 2009 22:21:00 +0000</pubDate>
		<guid isPermaLink="false">http://thebigfoto.com/?p=408#comment-508</guid>
		<description>[...] There are also at least 63 moons, including the four large moons called the Galilean moons that were first discovered by Galileo Galilei in 1610. Ganymede, the largest of these moons, has a diameter greater than that of the planet Mercury. [...]</description>
		<content:encoded><![CDATA[<p>[...] There are also at least 63 moons, including the four large moons called the Galilean moons that were first discovered by Galileo Galilei in 1610. Ganymede, the largest of these moons, has a diameter greater than that of the planet Mercury. [...]</p>
]]></content:encoded>
	</item>
	<item>
		<title>By: Anonymous</title>
		<link>http://thebigfoto.com/mercury-from-space/comment-page-1#comment-444</link>
		<dc:creator>Anonymous</dc:creator>
		<pubDate>Fri, 17 Apr 2009 15:48:44 +0000</pubDate>
		<guid isPermaLink="false">http://thebigfoto.com/?p=408#comment-444</guid>
		<description>this is awesome!!!!!!!!!!!!!!!!!!!</description>
		<content:encoded><![CDATA[<p>this is awesome!!!!!!!!!!!!!!!!!!!</p>
]]></content:encoded>
	</item>
	<item>
		<title>By: Meneados que llegaron a portada &#124; NOVEDADES Y ULTIMAS TECNOLOGIAS</title>
		<link>http://thebigfoto.com/mercury-from-space/comment-page-1#comment-102</link>
		<dc:creator>Meneados que llegaron a portada &#124; NOVEDADES Y ULTIMAS TECNOLOGIAS</dc:creator>
		<pubDate>Wed, 25 Mar 2009 23:38:48 +0000</pubDate>
		<guid isPermaLink="false">http://thebigfoto.com/?p=408#comment-102</guid>
		<description>[...]  [...]</description>
		<content:encoded><![CDATA[<p>[...]  [...]</p>
]]></content:encoded>
	</item>
</channel>
</rss>

