<?xml version="1.0" encoding="UTF-8"?>
<rss version="2.0"
	xmlns:content="http://purl.org/rss/1.0/modules/content/"
	xmlns:wfw="http://wellformedweb.org/CommentAPI/"
	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/"
	xmlns:slash="http://purl.org/rss/1.0/modules/slash/"
	>

<channel>
	<title>The Big Foto &#187; solar system</title>
	<atom:link href="http://thebigfoto.com/tag/solar-system/feed" rel="self" type="application/rss+xml" />
	<link>http://thebigfoto.com</link>
	<description>Life stories in photos</description>
	<lastBuildDate>Fri, 10 Feb 2012 07:47:56 +0000</lastBuildDate>
		<language>en</language>
	<sy:updatePeriod>hourly</sy:updatePeriod>
	<sy:updateFrequency>1</sy:updateFrequency>
			<item>
		<title>Mars Dunes</title>
		<link>http://thebigfoto.com/mars-dunes</link>
		<comments>http://thebigfoto.com/mars-dunes#comments</comments>
		<pubDate>Thu, 30 Jun 2011 09:43:57 +0000</pubDate>
		<dc:creator>admin</dc:creator>
				<category><![CDATA[Space]]></category>
		<category><![CDATA[mars]]></category>
		<category><![CDATA[solar system]]></category>

		<guid isPermaLink="false">http://thebigfoto.com/?p=2282</guid>
		<description><![CDATA[Amazing recent detailed pics of Mars surface.
]]></description>
			<content:encoded><![CDATA[<p>Amazing recent detailed pics of Mars surface.</p>
]]></content:encoded>
			<wfw:commentRss>http://thebigfoto.com/mars-dunes/feed</wfw:commentRss>
		<slash:comments>0</slash:comments>
		</item>
		<item>
		<title>Earth&#8217;s gravity</title>
		<link>http://thebigfoto.com/earths-gravity</link>
		<comments>http://thebigfoto.com/earths-gravity#comments</comments>
		<pubDate>Mon, 20 Jul 2009 08:11:43 +0000</pubDate>
		<dc:creator>admin</dc:creator>
				<category><![CDATA[Space]]></category>
		<category><![CDATA[earth]]></category>
		<category><![CDATA[gravity]]></category>
		<category><![CDATA[solar system]]></category>

		<guid isPermaLink="false">http://thebigfoto.com/?p=925</guid>
		<description><![CDATA[After reading Newscientist&#8217;s article July eclipse is best chance to look for gravity anomaly by Phil McKenna, TBF has explored NASA&#8217;s archives to find out what our earth&#8217;s gravity looks like.
The total eclipse
The solar eclipse that will take place on Wednesday, July 22, 2009 will be a total eclipse of the Sun with a magnitude [...]]]></description>
			<content:encoded><![CDATA[<p>After reading Newscientist&#8217;s article <a href="http://www.newscientist.com/article/dn17481-july-eclipse-is-best-chance-to-look-for-gravity-anomaly.html">July eclipse is best chance to look for gravity anomaly</a> by Phil McKenna, TBF has explored NASA&#8217;s archives to find out what our earth&#8217;s gravity looks like.</p>
<p><strong>The total eclipse</strong><br />
The solar eclipse that will take place on Wednesday, <strong>July 22, 2009</strong> will be a total eclipse of the Sun with a magnitude of 1.080 that will be visible from a narrow corridor through northern India, eastern Nepal, northern Bangladesh, Bhutan, the northern tip of Myanmar, central China and the Pacific Ocean, including the Ryukyu Islands, Marshall Islands and Kiribati. <strong>The longest total solar eclipse of the 21st century</strong> has sparked tourist fever in eastern China, which according to experts is the best place to view the event.</p>
<p><strong>Gravity and the Earth&#8217;s Shape</strong><br />
Gravity is the force that is responsible for the weight of an object and is determined by how the material that makes up the Earth is distributed throughout the Earth. Because gravity changes over the surface of the Earth, the weight of an object changes along with it.</p>
<p>The colors in these images represent the gravity anomalies measured by <a href="http://www.csr.utexas.edu/grace/">Gravity Recovery and Climate Experiment (GRACE)</a>. One can define standard gravity as the value of gravity for a  perfectly smooth &#8216;idealized&#8217; Earth, and the gravity &#8216;anomaly&#8217; is a measure  of how actual gravity deviates from this standard. Red shows the areas  where gravity is stronger than the smooth, standard value and blue reveals  areas where gravity is weaker.</p>
<p>GRACE is a collaborative endeavor involving the Center for Space Research  at the University of Texas, Austin; NASA&#8217;s Jet Propulsion Laboratory,  Pasadena, Calif.; the German Space Agency and the German Research Center  for Geosciences, Potsdam. GRACE, twin satellites were launched in March 2002 and they are making detailed measurements of Earth&#8217;s gravity field which will lead to discoveries about gravity and Earth&#8217;s natural systems.</p>
]]></content:encoded>
			<wfw:commentRss>http://thebigfoto.com/earths-gravity/feed</wfw:commentRss>
		<slash:comments>4</slash:comments>
		</item>
		<item>
		<title>Saturn from space</title>
		<link>http://thebigfoto.com/saturn-from-space</link>
		<comments>http://thebigfoto.com/saturn-from-space#comments</comments>
		<pubDate>Wed, 01 Jul 2009 15:28:02 +0000</pubDate>
		<dc:creator>admin</dc:creator>
				<category><![CDATA[Nature]]></category>
		<category><![CDATA[Space]]></category>
		<category><![CDATA[astronomy]]></category>
		<category><![CDATA[cassini]]></category>
		<category><![CDATA[hubble]]></category>
		<category><![CDATA[saturn]]></category>
		<category><![CDATA[solar system]]></category>
		<category><![CDATA[voyager 2]]></category>

		<guid isPermaLink="false">http://thebigfoto.com/?p=849</guid>
		<description><![CDATA[NASA&#8217;s Cassini mission has been orbiting Saturn for five Earth years as of June 30, 2009. That&#8217;s about one sixth of a Saturnian year, enough time for the spacecraft to have observed seasonal changes in the planet, its moons and sunlight&#8217;s angle on the dramatic rings.
Saturn is the sixth planet from the Sun and the [...]]]></description>
			<content:encoded><![CDATA[<p>NASA&#8217;s Cassini mission has been orbiting Saturn for five Earth years as of June 30, 2009. That&#8217;s about one sixth of a Saturnian year, enough time for the spacecraft to have observed seasonal changes in the planet, its moons and sunlight&#8217;s angle on the dramatic rings.</p>
<p>Saturn is the sixth planet from the Sun and the second largest planet in the Solar System, after Jupiter. Saturn, along with Jupiter, Uranus and Neptune, is classified as a gas giant.</p>
<p>Saturn has a prominent system of rings, consisting mostly of ice particles with a smaller amount of rocky debris and dust. Sixty-one known moons orbit the planet, not counting hundreds of &#8220;moonlets&#8221; within the rings. Titan, Saturn&#8217;s largest and the Solar System&#8217;s second largest moon (after Jupiter&#8217;s Ganymede), is larger than the planet Mercury and is the only moon in the Solar System to possess a significant atmosphere. [<a href="http://en.wikipedia.org/wiki/Saturn" target="_blank">Wikipedia</a>]</p>
]]></content:encoded>
			<wfw:commentRss>http://thebigfoto.com/saturn-from-space/feed</wfw:commentRss>
		<slash:comments>7</slash:comments>
		</item>
		<item>
		<title>High resolution Mars craters</title>
		<link>http://thebigfoto.com/high-resolution-mars-craters</link>
		<comments>http://thebigfoto.com/high-resolution-mars-craters#comments</comments>
		<pubDate>Tue, 09 Jun 2009 22:45:50 +0000</pubDate>
		<dc:creator>admin</dc:creator>
				<category><![CDATA[Space]]></category>
		<category><![CDATA[craters]]></category>
		<category><![CDATA[mars]]></category>
		<category><![CDATA[solar system]]></category>

		<guid isPermaLink="false">http://thebigfoto.com/?p=769</guid>
		<description><![CDATA[Another visit to the High Resolution Imaging Science Experiment (HiRISE) of the University of Arizona, this time I have picked some craters and parts of craters from their Mars photos. First visit was about Phobos &#038; Deimos, Mars moons .
]]></description>
			<content:encoded><![CDATA[<p>Another visit to the <a href="http://hirise.lpl.arizona.edu/">High Resolution Imaging Science Experiment (HiRISE) of the University of Arizona</a>, this time I have picked some craters and parts of craters from their Mars photos. First visit was about <a href="http://thebigfoto.com/phobos-deimos-mars-moons ">Phobos &#038; Deimos, Mars moons</a> .</p>
]]></content:encoded>
			<wfw:commentRss>http://thebigfoto.com/high-resolution-mars-craters/feed</wfw:commentRss>
		<slash:comments>3</slash:comments>
		</item>
		<item>
		<title>Jupiter from space</title>
		<link>http://thebigfoto.com/jupiter-from-space</link>
		<comments>http://thebigfoto.com/jupiter-from-space#comments</comments>
		<pubDate>Tue, 21 Apr 2009 22:20:54 +0000</pubDate>
		<dc:creator>admin</dc:creator>
				<category><![CDATA[Space]]></category>
		<category><![CDATA[astronomy]]></category>
		<category><![CDATA[jupiter]]></category>
		<category><![CDATA[solar system]]></category>

		<guid isPermaLink="false">http://thebigfoto.com/?p=612</guid>
		<description><![CDATA[Jupiter is the fifth planet from the Sun and the largest planet within the Solar System. It is two and a half times as massive as all of the other planets in our Solar System combined. Jupiter is classified as a gas giant, along with Saturn, Uranus and Neptune. Together, these four planets are sometimes [...]]]></description>
			<content:encoded><![CDATA[<p><strong>Jupiter</strong> is the fifth planet from the Sun and the largest planet within the <a href="http://thebigfoto.com/tag/solar-system">Solar System</a>. It is two and a half times as massive as all of the other planets in our Solar System combined. Jupiter is classified as a gas giant, along with Saturn, Uranus and Neptune. Together, these four planets are sometimes referred to as the Jovian planets.</p>
<p>The planet Jupiter is primarily composed of hydrogen with a small proportion of helium; it may also have a rocky core of heavier elements under high pressure.</p>
<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 <a href="http://thebigfoto.com/mercury-from-space">Mercury</a>.</p>
<p>[<a href="http://en.wikipedia.org/wiki/Jupiter" target="_blank">Wikipedia</a>]</p>
]]></content:encoded>
			<wfw:commentRss>http://thebigfoto.com/jupiter-from-space/feed</wfw:commentRss>
		<slash:comments>11</slash:comments>
		</item>
		<item>
		<title>Mercury from space</title>
		<link>http://thebigfoto.com/mercury-from-space</link>
		<comments>http://thebigfoto.com/mercury-from-space#comments</comments>
		<pubDate>Mon, 23 Mar 2009 19:39:22 +0000</pubDate>
		<dc:creator>admin</dc:creator>
				<category><![CDATA[Space]]></category>
		<category><![CDATA[astronomy]]></category>
		<category><![CDATA[mercury]]></category>
		<category><![CDATA[solar system]]></category>

		<guid isPermaLink="false">http://thebigfoto.com/?p=408</guid>
		<description><![CDATA[Mercury is the closest planet to the Sun. Its diameter is 40% smaller than Earth and 40% larger than the Moon. It is even smaller than Jupiter&#8217;s moon Ganymede and Saturn&#8217;s moon Titan.
In Roman mythology Mercury is the god of commerce, travel and thievery, the Roman counterpart of the Greek god Hermes, the messenger of [...]]]></description>
			<content:encoded><![CDATA[<p><strong>Mercury </strong>is the closest planet to the Sun. Its diameter is 40% smaller than Earth and 40% larger than the Moon. It is even smaller than Jupiter&#8217;s moon Ganymede and Saturn&#8217;s moon Titan.</p>
<p>In Roman mythology Mercury is the god of commerce, travel and thievery, the Roman counterpart of the Greek god Hermes, the messenger of the Gods. The planet probably received this name because it moves so quickly across the sky.</p>
]]></content:encoded>
			<wfw:commentRss>http://thebigfoto.com/mercury-from-space/feed</wfw:commentRss>
		<slash:comments>8</slash:comments>
		</item>
		<item>
		<title>Venus from space</title>
		<link>http://thebigfoto.com/venus-from-space</link>
		<comments>http://thebigfoto.com/venus-from-space#comments</comments>
		<pubDate>Thu, 05 Mar 2009 08:09:00 +0000</pubDate>
		<dc:creator>admin</dc:creator>
				<category><![CDATA[Europe]]></category>
		<category><![CDATA[Space]]></category>
		<category><![CDATA[planet]]></category>
		<category><![CDATA[solar system]]></category>
		<category><![CDATA[venus]]></category>

		<guid isPermaLink="false">http://thebigfoto.com/?p=278</guid>
		<description><![CDATA[Venus is the second-closest planet to the Sun, orbiting it every 224.7 Earth days. The planet is named after Venus, the Roman goddess of love. It is the brightest natural object in the night sky, except for the Moon.
Classified as a terrestrial planet, it is sometimes called Earth&#8217;s &#8220;sister planet&#8221;, because they are similar in [...]]]></description>
			<content:encoded><![CDATA[<p><strong>Venus </strong>is the second-closest planet to the Sun, orbiting it every 224.7 Earth days. The planet is named after Venus, the Roman goddess of love. It is the brightest natural object in the night sky, except for the Moon.</p>
<p>Classified as a terrestrial planet, it is sometimes called <strong>Earth&#8217;s &#8220;sister planet&#8221;</strong>, because they are similar in size, gravity, and bulk composition. Venus is covered with an opaque layer of highly reflective clouds of sulfuric acid, preventing its surface from being seen from space in visible light; this was a subject of great speculation until some of its secrets were revealed by planetary science in the twentieth century. Venus has the densest atmosphere of all the terrestrial planets, consisting mostly of carbon dioxide, as it has no carbon cycle to lock carbon back into rocks and surface features, nor organic life to absorb it in biomass. It has become so hot that the earth-like oceans that the young Venus is believed to have possessed have totally evaporated, leaving a dusty dry desertscape with many slab-like rocks.</p>
<p>Compose this kind of images is not easy and requires lot of efforts. For example check foto 12 composition job:</p>
<blockquote><p>Magellan synthetic aperture radar mosaics from the three eight-month cycles of Magellan radar mapping are mapped onto a computer-simulated globe to create this image. Magellan obtained coverage of 98 percent of the surface of Venus. Remaining gaps are filled with data from previous missions, (the Soviet Venera 15 and 16 radar and Pioneer Venus Orbiter altimetry) and data from Earth-based radar observations from the Arecibo radio telescope. Simulated color is used to enhance small-scale structures. The simulated hues are based on color images recorded by the Venera 13 and 14 landing craft. Maxwell Montes, the planet&#8217;s highest mountain at 11 kilometers (6.6 miles) above the average elevation, is the bright feature in the lower center of the image. Other terrain types visible in this image include tessera, ridge belts, lava flows, impact craters and coronae. The image was produced by the Solar System Visualization Project and the Magellan Science team at the Jet Propulsion Laboratory Multimission Image Processing Laboratory. The Magellan mission is managed by JPL for NASA&#8217;s Office of Space Science.</p></blockquote>
<p>Or  foto 13 composition job:</p>
<blockquote><p>The Magellan spacecraft imaged more than 98% of Venus at a resolution of about 100 meters; the effective resolution of this image is about 3 km. A mosaic of the Magellan images (most with illumination from the west) forms the image base. Gaps in the Magellan coverage were filled with images from the Earth-based Arecibo radar in a region centered roughly on 0 degree latitude and longitude, and with a neutral tone elsewhere (primarily near the south pole). The composite image was processed to improve contrast and to emphasize small features, and was color-coded to represent elevation. Gaps in the elevation data from the Magellan radar altimeter were filled with altimetry from the Venera spacecraft and the U.S. Pioneer Venus missions. An orthographic projection was used, simulating a distant view of one hemisphere of the planet. The Magellan mission was managed for NASA by Jet Propulsion Laboratory (JPL), Pasadena, CA. Data processed by JPL, the Massachusetts Institute of Technology, Cambridge, MA, and the U.S. Geological Survey, Flagstaff, AZ.</p></blockquote>
]]></content:encoded>
			<wfw:commentRss>http://thebigfoto.com/venus-from-space/feed</wfw:commentRss>
		<slash:comments>3</slash:comments>
		</item>
	</channel>
</rss>

