<?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/"
	xmlns:georss="http://www.georss.org/georss" xmlns:geo="http://www.w3.org/2003/01/geo/wgs84_pos#" xmlns:media="http://search.yahoo.com/mrss/"
	>

<channel>
	<title>Through The Fire</title>
	<atom:link href="http://meteorhalley.wordpress.com/feed/" rel="self" type="application/rss+xml" />
	<link>http://meteorhalley.wordpress.com</link>
	<description>Meteor</description>
	<lastBuildDate>Fri, 04 Apr 2008 09:29:19 +0000</lastBuildDate>
	<generator>http://wordpress.com/</generator>
	<language>en</language>
	<sy:updatePeriod>hourly</sy:updatePeriod>
	<sy:updateFrequency>1</sy:updateFrequency>
	<cloud domain='meteorhalley.wordpress.com' port='80' path='/?rsscloud=notify' registerProcedure='' protocol='http-post' />
<image>
		<url>http://www.gravatar.com/blavatar/191e2921866b316158d054047fdecdc4?s=96&#038;d=http://s.wordpress.com/i/buttonw-com.png</url>
		<title>Through The Fire</title>
		<link>http://meteorhalley.wordpress.com</link>
	</image>
			<item>
		<title>The Sun</title>
		<link>http://meteorhalley.wordpress.com/2008/04/04/the-sun/</link>
		<comments>http://meteorhalley.wordpress.com/2008/04/04/the-sun/#comments</comments>
		<pubDate>Fri, 04 Apr 2008 09:28:24 +0000</pubDate>
		<dc:creator>meteorhalley</dc:creator>
				<category><![CDATA[Uncategorized]]></category>
		<category><![CDATA[The Fire Burn Of The Sunny Sun]]></category>

		<guid isPermaLink="false">http://meteorhalley.wordpress.com/?p=67</guid>
		<description><![CDATA[Video Storm Rage
&#60;object width=&#8221;425&#8243; height=&#8221;355&#8243;&#62;&#60;param name=&#8221;movie&#8221; value=&#8221;http://www.youtube.com/v/rb9jTeFcatU&#38;hl=en&#8221;&#62;&#60;/param&#62;&#60;param name=&#8221;wmode&#8221; value=&#8221;transparent&#8221;&#62;&#60;/param&#62;&#60;embed src=&#8221;http://www.youtube.com/v/rb9jTeFcatU&#38;hl=en&#8221; type=&#8221;application/x-shockwave-flash&#8221; wmode=&#8221;transparent&#8221; width=&#8221;425&#8243; height=&#8221;355&#8243;&#62;&#60;/embed&#62;&#60;/object&#62;
       <img alt="" border="0" src="http://stats.wordpress.com/b.gif?host=meteorhalley.wordpress.com&blog=3185850&post=67&subd=meteorhalley&ref=&feed=1" />]]></description>
			<content:encoded><![CDATA[<div class='snap_preview'><br /><p>Video Storm Rage</p>
<p>&lt;object width=&#8221;425&#8243; height=&#8221;355&#8243;&gt;&lt;param name=&#8221;movie&#8221; value=&#8221;<a href="http://www.youtube.com/v/rb9jTeFcatU&amp;hl=en%22%3E%3C/param%3E%3Cparam">http://www.youtube.com/v/rb9jTeFcatU&amp;hl=en&#8221;&gt;&lt;/param&gt;&lt;param</a> name=&#8221;wmode&#8221; value=&#8221;transparent&#8221;&gt;&lt;/param&gt;&lt;embed src=&#8221;<a href="http://www.youtube.com/v/rb9jTeFcatU&amp;hl=en">http://www.youtube.com/v/rb9jTeFcatU&amp;hl=en</a>&#8221; type=&#8221;application/x-shockwave-flash&#8221; wmode=&#8221;transparent&#8221; width=&#8221;425&#8243; height=&#8221;355&#8243;&gt;&lt;/embed&gt;&lt;/object&gt;</p>
<img alt="" border="0" src="http://feeds.wordpress.com/1.0/categories/meteorhalley.wordpress.com/67/" /> <img alt="" border="0" src="http://feeds.wordpress.com/1.0/tags/meteorhalley.wordpress.com/67/" /> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/gocomments/meteorhalley.wordpress.com/67/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/comments/meteorhalley.wordpress.com/67/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/godelicious/meteorhalley.wordpress.com/67/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/delicious/meteorhalley.wordpress.com/67/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/gostumble/meteorhalley.wordpress.com/67/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/stumble/meteorhalley.wordpress.com/67/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/godigg/meteorhalley.wordpress.com/67/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/digg/meteorhalley.wordpress.com/67/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/goreddit/meteorhalley.wordpress.com/67/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/reddit/meteorhalley.wordpress.com/67/" /></a> <img alt="" border="0" src="http://stats.wordpress.com/b.gif?host=meteorhalley.wordpress.com&blog=3185850&post=67&subd=meteorhalley&ref=&feed=1" /></div>]]></content:encoded>
			<wfw:commentRss>http://meteorhalley.wordpress.com/2008/04/04/the-sun/feed/</wfw:commentRss>
		<slash:comments>0</slash:comments>
	
		<media:content url="http://0.gravatar.com/avatar/80d91880e5e7c91d9244aaeb122d8aef?s=96&#38;d=identicon" medium="image">
			<media:title type="html">meteorhalley</media:title>
		</media:content>
	</item>
		<item>
		<title>Sun</title>
		<link>http://meteorhalley.wordpress.com/2008/04/04/sun/</link>
		<comments>http://meteorhalley.wordpress.com/2008/04/04/sun/#comments</comments>
		<pubDate>Fri, 04 Apr 2008 05:29:08 +0000</pubDate>
		<dc:creator>meteorhalley</dc:creator>
				<category><![CDATA[Uncategorized]]></category>

		<guid isPermaLink="false">http://meteorhalley.wordpress.com/?p=64</guid>
		<description><![CDATA[
The Sun 


The Sun (Latin: Sol) is the star at the center of the Solar System. It is a medium size star. The Earth and other matter (including other planets, asteroids, meteoroids, comets and dust) orbit the Sun, which by itself accounts for about 99.8% of the solar system&#8217;s mass. Energy from the Sun, in [...]<img alt="" border="0" src="http://stats.wordpress.com/b.gif?host=meteorhalley.wordpress.com&blog=3185850&post=64&subd=meteorhalley&ref=&feed=1" />]]></description>
			<content:encoded><![CDATA[<div class='snap_preview'><br /><table class="infobox" style="width:20em;">
<caption><b>The Sun</b> <a href="http://en.wikipedia.org/wiki/Image:Sun_symbol.svg" class="image" title="Sun symbol.svg"><img src="http://upload.wikimedia.org/wikipedia/commons/thumb/6/6f/Sun_symbol.svg/25px-Sun_symbol.svg.png" border="0" height="25" width="25" /></a></caption>
</table>
<p><a href="http://meteorhalley.files.wordpress.com/2008/04/270px-sun920607.jpg" title="270px-sun920607.jpg"><img src="http://meteorhalley.files.wordpress.com/2008/04/270px-sun920607.thumbnail.jpg" alt="270px-sun920607.jpg" /></a><br />
The <b>Sun</b> (<a href="http://en.wikipedia.org/wiki/Latin" title="Latin">Latin</a>: <span><i>Sol</i></span>) is the <a href="http://en.wikipedia.org/wiki/Star" title="Star">star</a> at the center of the <a href="http://en.wikipedia.org/wiki/Solar_System" title="Solar System">Solar System</a>. It is a medium size star. The <a href="http://en.wikipedia.org/wiki/Earth" title="Earth">Earth</a> and other matter (including other <a href="http://en.wikipedia.org/wiki/Planet" title="Planet">planets</a>, <a href="http://en.wikipedia.org/wiki/Asteroid" title="Asteroid">asteroids</a>, <a href="http://en.wikipedia.org/wiki/Meteoroid" title="Meteoroid">meteoroids</a>, <a href="http://en.wikipedia.org/wiki/Comet" title="Comet">comets</a> and <a href="http://en.wikipedia.org/wiki/Cosmic_dust" title="Cosmic dust">dust</a>) <a href="http://en.wikipedia.org/wiki/Orbit" title="Orbit">orbit</a> the Sun, which by itself accounts for about 99.8% of the <a href="http://en.wikipedia.org/wiki/Solar_system" class="mw-redirect" title="Solar system">solar system</a>&#8217;s <a href="http://en.wikipedia.org/wiki/Mass" title="Mass">mass</a>. <a href="http://en.wikipedia.org/wiki/Energy" title="Energy">Energy</a> from the Sun, in the form of sunlight and heat, supports almost all life on Earth via <a href="http://en.wikipedia.org/wiki/Photosynthesis" title="Photosynthesis">photosynthesis</a>, and drives the Earth&#8217;s <a href="http://en.wikipedia.org/wiki/Climate" title="Climate">climate</a> and weather.</p>
<p>The surface composition of the Sun consists of <a href="http://en.wikipedia.org/wiki/Hydrogen" title="Hydrogen">hydrogen</a> (about 74% of its mass, or 92% of its volume), <a href="http://en.wikipedia.org/wiki/Helium" title="Helium">helium</a> (about 24-25% of mass, 7% of volume), and trace quantities of other elements, including <a href="http://en.wikipedia.org/wiki/Iron" title="Iron">Fe</a>, <a href="http://en.wikipedia.org/wiki/Nickel" title="Nickel">Ni</a>, <a href="http://en.wikipedia.org/wiki/Oxygen" title="Oxygen">O</a>, <a href="http://en.wikipedia.org/wiki/Silicon" title="Silicon">Si</a>, <a href="http://en.wikipedia.org/wiki/Sulfur" title="Sulfur">S</a>, <a href="http://en.wikipedia.org/wiki/Magnesium" title="Magnesium">Mg</a>, <a href="http://en.wikipedia.org/wiki/Carbon" title="Carbon">C</a>, <a href="http://en.wikipedia.org/wiki/Neon" title="Neon">Ne</a>, <a href="http://en.wikipedia.org/wiki/Calcium" title="Calcium">Ca</a>, and <a href="http://en.wikipedia.org/wiki/Chromium" title="Chromium">Cr</a>.<sup><a href="http://en.wikipedia.org/wiki/Sun#cite_note-manuel1983-9">[10]</a></sup> <span></span>The Sun has a <a href="http://en.wikipedia.org/wiki/Stellar_classification" title="Stellar classification">spectral class</a> of G2V. <i>G2</i> implies that it has a surface temperature of approximately 5,780 <a href="http://en.wikipedia.org/wiki/Kelvin" title="Kelvin">K</a>, giving it a <a href="http://en.wikipedia.org/wiki/Color_temperature" title="Color temperature">white</a> color which, because of atmospheric <a href="http://en.wikipedia.org/wiki/Scattering" title="Scattering">scattering</a>, appears yellow as seen from the surface of the Earth. This is a subtractive effect, as the <a href="http://en.wikipedia.org/wiki/Rayleigh_scattering" title="Rayleigh scattering">preferential scattering</a> of blue photons (causing the sky color) removes enough blue light to leave a residual reddishness that is perceived as yellow. (When low enough in the sky, the Sun appears orange or red, due to this scattering.)</p>
<p>Its spectrum contains <a href="http://en.wikipedia.org/wiki/Spectral_line" title="Spectral line">lines</a> of ionized and neutral metals as well as very weak hydrogen lines. The <i>V</i> (<a href="http://en.wikipedia.org/wiki/Roman_numerals" title="Roman numerals">Roman five</a>) suffix indicates that the Sun, like most stars, is a <a href="http://en.wikipedia.org/wiki/Main_sequence" title="Main sequence">main sequence</a> star. This means that it generates its energy by <a href="http://en.wikipedia.org/wiki/Nuclear_fusion" title="Nuclear fusion">nuclear fusion</a> of <a href="http://en.wikipedia.org/wiki/Hydrogen" title="Hydrogen">hydrogen</a> nuclei into <a href="http://en.wikipedia.org/wiki/Helium" title="Helium">helium</a> and is in a state of <a href="http://en.wikipedia.org/wiki/Hydrostatic_equilibrium" title="Hydrostatic equilibrium">hydrostatic equilibrium</a>, neither contracting nor expanding over time. There are more than 100 million G2 class stars in our galaxy. Once regarded as a small and relatively insignificant star, the Sun is now known to be brighter than 85% of the stars in the <a href="http://en.wikipedia.org/wiki/Milky_Way" title="Milky Way">galaxy</a>, most of which are <a href="http://en.wikipedia.org/wiki/Red_dwarf" title="Red dwarf">red dwarfs</a>.</p>
<p>The Sun orbits the center of the <a href="http://en.wikipedia.org/wiki/Milky_Way" title="Milky Way">Milky Way</a> <a href="http://en.wikipedia.org/wiki/Galaxy" title="Galaxy">galaxy</a> at a distance of approximately 26,000 <a href="http://en.wikipedia.org/wiki/Light-year" title="Light-year">light-years</a> from the <a href="http://en.wikipedia.org/wiki/Galactic_center" class="mw-redirect" title="Galactic center">galactic center</a>, completing one revolution in about 225–250 million years. Its approximate <a href="http://en.wikipedia.org/wiki/Orbital_speed" title="Orbital speed">orbital speed</a> is 220 kilometers per second, plus or minus 20 km/s. This is equivalent to about one light-year every 1,400 years, and about one <a href="http://en.wikipedia.org/wiki/Astronomical_unit" title="Astronomical unit">AU</a> every 8 days. These measurements of galactic distance and speed are as accurate as we can get given our current knowledge, but will change as we learn more.<sup><a href="http://en.wikipedia.org/wiki/Sun#cite_note-Kerr-11"></a></sup></p>
<p>The Sun is currently traveling through the <a href="http://en.wikipedia.org/wiki/Local_Interstellar_Cloud" title="Local Interstellar Cloud">Local Interstellar Cloud</a> in the low-density <a href="http://en.wikipedia.org/wiki/Local_Bubble" title="Local Bubble">Local Bubble</a> zone of diffuse high-temperature gas, in the inner rim of the <a href="http://en.wikipedia.org/wiki/Orion_Arm" title="Orion Arm">Orion Arm</a> of the <a href="http://en.wikipedia.org/wiki/Milky_Way_Galaxy" class="mw-redirect" title="Milky Way Galaxy">Milky Way Galaxy</a>, between the larger <a href="http://en.wikipedia.org/wiki/Perseus_arm" class="mw-redirect" title="Perseus arm">Perseus</a> and <a href="http://en.wikipedia.org/wiki/Sagittarius_arm" class="mw-redirect" title="Sagittarius arm">Sagittarius arms</a> of the galaxy. Of the 50 <a href="http://en.wikipedia.org/wiki/Nearest_stars" class="mw-redirect" title="Nearest stars">nearest stellar systems</a> within 17 light years from the Earth, the Sun ranks 4th in <a href="http://en.wikipedia.org/wiki/Absolute_magnitude" title="Absolute magnitude">absolute magnitude</a> as a fourth magnitude star (M=4.83).</p>
<h3><span class="mw-headline">Atmosphere</span></h3>
<p><a href="http://meteorhalley.files.wordpress.com/2008/04/200px-solar_eclips_1999_4_nr.jpg" title="200px-solar_eclips_1999_4_nr.jpg"><img src="http://meteorhalley.files.wordpress.com/2008/04/200px-solar_eclips_1999_4_nr.thumbnail.jpg" alt="200px-solar_eclips_1999_4_nr.jpg" /></a><br />
The parts of the Sun above the photosphere are referred to collectively as the <i>solar atmosphere</i>. They can be viewed with telescopes operating across the <a href="http://en.wikipedia.org/wiki/Electromagnetic_spectrum" title="Electromagnetic spectrum">electromagnetic spectrum</a>, from radio through <a href="http://en.wikipedia.org/wiki/Visible_light" class="mw-redirect" title="Visible light">visible light</a> to <a href="http://en.wikipedia.org/wiki/Gamma_rays" class="mw-redirect" title="Gamma rays">gamma rays</a>, and comprise five principal zones: the <i>temperature minimum</i>, the <a href="http://en.wikipedia.org/wiki/Chromosphere" title="Chromosphere">chromosphere</a>, the <a href="http://en.wikipedia.org/wiki/Solar_transition_region" title="Solar transition region">transition region</a>, the <a href="http://en.wikipedia.org/wiki/Corona" title="Corona">corona</a>, and the <a href="http://en.wikipedia.org/wiki/Heliosphere" title="Heliosphere">heliosphere</a>. The heliosphere, which may be considered the tenuous outer atmosphere of the Sun, extends outward past the orbit of <a href="http://en.wikipedia.org/wiki/Pluto" title="Pluto">Pluto</a> to the <a href="http://en.wikipedia.org/wiki/Heliopause" class="mw-redirect" title="Heliopause">heliopause</a>, where it forms a sharp <a href="http://en.wikipedia.org/wiki/Shock_wave" title="Shock wave">shock front</a> boundary with the <a href="http://en.wikipedia.org/wiki/Interstellar_medium" title="Interstellar medium">interstellar medium</a>. The chromosphere, transition region, and corona are much hotter than the surface of the Sun. The reason why has not been conclusively proven; evidence suggests that <a href="http://en.wikipedia.org/wiki/Alfv%C3%A9n_wave" title="Alfvén wave">Alfvén waves</a> may have enough energy to heat the corona.<sup><a href="http://en.wikipedia.org/wiki/Sun#cite_note-30">[31]</a></sup></p>
<p>The coolest layer of the Sun is a temperature minimum region about 500 km above the photosphere, with a temperature of about 4,000 <a href="http://en.wikipedia.org/wiki/Kelvin" title="Kelvin">K</a>. This part of the Sun is cool enough to support simple molecules such as <a href="http://en.wikipedia.org/wiki/Carbon_monoxide" title="Carbon monoxide">carbon monoxide</a> and water, which can be detected by their absorption spectra.</p>
<p>Above the temperature minimum layer is a thin layer about 2,000 km thick, dominated by a spectrum of emission and absorption lines. It is called the <i>chromosphere</i> from the Greek root <i>chroma</i>, meaning color, because the chromosphere is visible as a colored flash at the beginning and end of <a href="http://en.wikipedia.org/wiki/Solar_eclipse" title="Solar eclipse">total eclipses of the Sun</a>. The temperature in the chromosphere increases gradually with altitude, ranging up to around 100,000 K near the top.</p>
<p><a href="http://meteorhalley.files.wordpress.com/2008/04/350px-171879main_limbflarejan12_lg.jpg" title="350px-171879main_limbflarejan12_lg.jpg"><img src="http://meteorhalley.files.wordpress.com/2008/04/350px-171879main_limbflarejan12_lg.thumbnail.jpg" alt="350px-171879main_limbflarejan12_lg.jpg" /></a></p>
<p>Above the <a href="http://en.wikipedia.org/wiki/Chromosphere" title="Chromosphere">chromosphere</a> is a <a href="http://en.wikipedia.org/wiki/Solar_transition_region" title="Solar transition region">transition region</a> in which the temperature rises rapidly from around 100,000 <a href="http://en.wikipedia.org/wiki/Kelvin" title="Kelvin">K</a> to coronal temperatures closer to one million K. The increase is because of a <a href="http://en.wikipedia.org/wiki/Phase_transition" title="Phase transition">phase transition</a> as <a href="http://en.wikipedia.org/wiki/Helium" title="Helium">helium</a> within the region becomes fully <a href="http://en.wikipedia.org/wiki/Ionization" title="Ionization">ionized</a> by the high temperatures. The transition region does not occur at a well-defined altitude. Rather, it forms a kind of <a href="http://en.wikipedia.org/wiki/Halo_%28optical_phenomenon%29" title="Halo (optical phenomenon)">nimbus</a> around chromospheric features such as <a href="http://en.wikipedia.org/wiki/Spicule_%28solar_physics%29" title="Spicule (solar physics)">spicules</a> and <a href="http://en.wikipedia.org/wiki/Solar_filament" class="mw-redirect" title="Solar filament">filaments</a>, and is in constant, chaotic motion. The transition region is not easily visible from Earth&#8217;s surface, but is readily observable from <a href="http://en.wikipedia.org/wiki/Outer_space" title="Outer space">space</a> by instruments sensitive to the <a href="http://en.wikipedia.org/wiki/Ultraviolet" title="Ultraviolet">far ultraviolet</a> portion of the <a href="http://en.wikipedia.org/wiki/Electromagnetic_spectrum" title="Electromagnetic spectrum">spectrum</a>.</p>
<p>The <a href="http://en.wikipedia.org/wiki/Corona" title="Corona">corona</a> is the extended outer atmosphere of the Sun, which is much larger in volume than the Sun itself. The corona merges smoothly with the <a href="http://en.wikipedia.org/wiki/Solar_wind" title="Solar wind">solar wind</a> that fills the <a href="http://en.wikipedia.org/wiki/Solar_system" class="mw-redirect" title="Solar system">solar system</a> and <a href="http://en.wikipedia.org/wiki/Heliosphere" title="Heliosphere">heliosphere</a>. The low corona, which is very near the surface of the Sun, has a particle density of 10<sup>14</sup>–10<sup>16</sup> m<sup>−3</sup>. (Earth&#8217;s atmosphere near sea level has a particle density of about 2×10<sup>25</sup> m<sup>−3</sup>.) The temperature of the corona is several million kelvin. While no complete theory yet exists to account for the temperature of the corona, at least some of its heat is known to be from <a href="http://en.wikipedia.org/wiki/Magnetic_reconnection" title="Magnetic reconnection">magnetic reconnection</a>.</p>
<p>The <a href="http://en.wikipedia.org/wiki/Heliosphere" title="Heliosphere">heliosphere</a> extends from approximately 20 solar radii (0.1 AU) to the outer fringes of the solar system. Its inner boundary is defined as the layer in which the flow of the <a href="http://en.wikipedia.org/wiki/Solar_wind" title="Solar wind">solar wind</a> becomes <i>superalfvénic</i>—that is, where the flow becomes faster than the speed of Alfvén waves. Turbulence and dynamic forces outside this boundary cannot affect the shape of the solar corona within, because the information can only travel at the speed of Alfvén waves. The solar wind travels outward continuously through the heliosphere, forming the solar magnetic field into a <a href="http://en.wikipedia.org/wiki/Parker_spiral" title="Parker spiral">spiral</a> shape, until it impacts the <a href="http://en.wikipedia.org/wiki/Heliopause" class="mw-redirect" title="Heliopause">heliopause</a> more than 50 AU from the Sun. In December 2004, the <a href="http://en.wikipedia.org/wiki/Voyager_program" title="Voyager program">Voyager 1 probe</a> passed through a shock front that is thought to be part of the heliopause. Both of the Voyager probes have recorded higher levels of energetic particles as they approach the boundary.</p>
<img alt="" border="0" src="http://feeds.wordpress.com/1.0/categories/meteorhalley.wordpress.com/64/" /> <img alt="" border="0" src="http://feeds.wordpress.com/1.0/tags/meteorhalley.wordpress.com/64/" /> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/gocomments/meteorhalley.wordpress.com/64/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/comments/meteorhalley.wordpress.com/64/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/godelicious/meteorhalley.wordpress.com/64/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/delicious/meteorhalley.wordpress.com/64/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/gostumble/meteorhalley.wordpress.com/64/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/stumble/meteorhalley.wordpress.com/64/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/godigg/meteorhalley.wordpress.com/64/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/digg/meteorhalley.wordpress.com/64/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/goreddit/meteorhalley.wordpress.com/64/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/reddit/meteorhalley.wordpress.com/64/" /></a> <img alt="" border="0" src="http://stats.wordpress.com/b.gif?host=meteorhalley.wordpress.com&blog=3185850&post=64&subd=meteorhalley&ref=&feed=1" /></div>]]></content:encoded>
			<wfw:commentRss>http://meteorhalley.wordpress.com/2008/04/04/sun/feed/</wfw:commentRss>
		<slash:comments>0</slash:comments>
	
		<media:content url="http://0.gravatar.com/avatar/80d91880e5e7c91d9244aaeb122d8aef?s=96&#38;d=identicon" medium="image">
			<media:title type="html">meteorhalley</media:title>
		</media:content>

		<media:content url="http://upload.wikimedia.org/wikipedia/commons/thumb/6/6f/Sun_symbol.svg/25px-Sun_symbol.svg.png" medium="image" />

		<media:content url="http://meteorhalley.files.wordpress.com/2008/04/270px-sun920607.thumbnail.jpg" medium="image">
			<media:title type="html">270px-sun920607.jpg</media:title>
		</media:content>

		<media:content url="http://meteorhalley.files.wordpress.com/2008/04/200px-solar_eclips_1999_4_nr.thumbnail.jpg" medium="image">
			<media:title type="html">200px-solar_eclips_1999_4_nr.jpg</media:title>
		</media:content>

		<media:content url="http://meteorhalley.files.wordpress.com/2008/04/350px-171879main_limbflarejan12_lg.thumbnail.jpg" medium="image">
			<media:title type="html">350px-171879main_limbflarejan12_lg.jpg</media:title>
		</media:content>
	</item>
		<item>
		<title>Saturn</title>
		<link>http://meteorhalley.wordpress.com/2008/04/03/saturn/</link>
		<comments>http://meteorhalley.wordpress.com/2008/04/03/saturn/#comments</comments>
		<pubDate>Thu, 03 Apr 2008 05:36:12 +0000</pubDate>
		<dc:creator>meteorhalley</dc:creator>
				<category><![CDATA[Uncategorized]]></category>

		<guid isPermaLink="false">http://meteorhalley.wordpress.com/?p=62</guid>
		<description><![CDATA[Saturn

Saturn (pronounced /ˈsætɚn/) is the sixth planet from the Sun and the second largest planet in the Solar System, after Jupiter. Along with the planets Jupiter, Uranus, Neptune it is classified as a gas giant (also known as a Jovian planet, after the planet Jupiter). It was named after the Roman god Saturnus, equated to [...]<img alt="" border="0" src="http://stats.wordpress.com/b.gif?host=meteorhalley.wordpress.com&blog=3185850&post=62&subd=meteorhalley&ref=&feed=1" />]]></description>
			<content:encoded><![CDATA[<div class='snap_preview'><br /><h1 class="firstHeading">Saturn</h1>
<p><a href="http://meteorhalley.files.wordpress.com/2008/04/240px-saturn_from_cassini_orbiter_2004-10-06.jpg" title="240px-saturn_from_cassini_orbiter_2004-10-06.jpg"><img src="http://meteorhalley.files.wordpress.com/2008/04/240px-saturn_from_cassini_orbiter_2004-10-06.thumbnail.jpg" alt="240px-saturn_from_cassini_orbiter_2004-10-06.jpg" /></a></p>
<p><b>Saturn</b> (<a href="http://en.wikipedia.org/wiki/Help:Pronunciation" title="Pronunciation">pronounced</a> <span title="Pronunciation in the International Phonetic Alphabet (IPA)" class="IPA">/ˈsætɚn/</span>) is the sixth <a href="http://en.wikipedia.org/wiki/Planet" title="Planet">planet</a> from the <a href="http://en.wikipedia.org/wiki/Sun" title="Sun">Sun</a> and the second largest planet in the <a href="http://en.wikipedia.org/wiki/Solar_System" title="Solar System">Solar System</a>, after <a href="http://en.wikipedia.org/wiki/Jupiter" title="Jupiter">Jupiter</a>. Along with the planets <a href="http://en.wikipedia.org/wiki/Jupiter" title="Jupiter">Jupiter</a>, <a href="http://en.wikipedia.org/wiki/Uranus" title="Uranus">Uranus</a>, <a href="http://en.wikipedia.org/wiki/Neptune" title="Neptune">Neptune</a> it is classified as a <a href="http://en.wikipedia.org/wiki/Gas_giant" title="Gas giant">gas giant</a> (also known as a Jovian planet, after the planet Jupiter). It was named after the Roman god <a href="http://en.wikipedia.org/wiki/Saturn_%28mythology%29" title="Saturn (mythology)">Saturnus</a>, equated to the <a href="http://en.wikipedia.org/wiki/Greek_mythology" title="Greek mythology">Greek</a> <a href="http://en.wikipedia.org/wiki/Cronus" title="Cronus">Kronos</a> (the Titan father of <a href="http://en.wikipedia.org/wiki/Zeus" title="Zeus">Zeus</a>) and the Babylonian <a href="http://en.wikipedia.org/wiki/Ninurta" title="Ninurta">Ninurta</a>. Saturn&#8217;s symbol represents the god&#8217;s <a href="http://en.wikipedia.org/wiki/Sickle" title="Sickle">sickle</a> (<a href="http://en.wikipedia.org/wiki/Unicode" title="Unicode">Unicode</a>: <span class="Unicode">♄</span>). The day in the week <a href="http://en.wikipedia.org/wiki/Saturday" title="Saturday">Saturday</a> gets its name from the planet.</p>
<p>The planet Saturn is composed of <a href="http://en.wikipedia.org/wiki/Hydrogen" title="Hydrogen">hydrogen</a>, with small proportions of <a href="http://en.wikipedia.org/wiki/Helium" title="Helium">helium</a> and trace elements.<sup><a href="http://en.wikipedia.org/wiki/Saturn#cite_note-Voyager_Summary_1-9">[10]</a></sup> The interior consists of a small core of rock and ice, surrounded by a thick layer of <a href="http://en.wikipedia.org/wiki/Metallic_hydrogen" title="Metallic hydrogen">metallic hydrogen</a> and a gaseous outer layer. The outer <a href="http://en.wikipedia.org/wiki/Atmosphere" title="Atmosphere">atmosphere</a> is generally bland in appearance, although long-lived features can appear. <a href="http://en.wikipedia.org/wiki/Wind_speed" title="Wind speed">Wind speeds</a> on Saturn can reach 1,800 km/h, significantly faster than those on Jupiter. Saturn has a planetary <a href="http://en.wikipedia.org/wiki/Magnetic_field" title="Magnetic field">magnetic field</a> intermediate in strength between that of Earth and the more powerful field around Jupiter.</p>
<p>Saturn has a prominent system of <a href="http://en.wikipedia.org/wiki/Rings_of_Saturn" title="Rings of Saturn">rings</a>, consisting mostly of <a href="http://en.wikipedia.org/wiki/Ice" title="Ice">ice</a> particles with a smaller amount of rocky <a href="http://en.wikipedia.org/wiki/Debris" title="Debris">debris</a> and <a href="http://en.wikipedia.org/wiki/Cosmic_dust" title="Cosmic dust">dust</a>. Sixty known moons orbit the planet. <a href="http://en.wikipedia.org/wiki/Titan_%28moon%29" title="Titan (moon)">Titan</a>, Saturn&#8217;s largest and the Solar System&#8217;s second largest moon (after <a href="http://en.wikipedia.org/wiki/Jupiter" title="Jupiter">Jupiter</a>&#8217;s <a href="http://en.wikipedia.org/wiki/Ganymede_%28moon%29" title="Ganymede (moon)">Ganymede</a>), is larger than the planet <a href="http://en.wikipedia.org/wiki/Mercury_%28planet%29" title="Mercury (planet)">Mercury</a> and is the only moon in the Solar System to possess a significant atmosphere.</p>
<img alt="" border="0" src="http://feeds.wordpress.com/1.0/categories/meteorhalley.wordpress.com/62/" /> <img alt="" border="0" src="http://feeds.wordpress.com/1.0/tags/meteorhalley.wordpress.com/62/" /> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/gocomments/meteorhalley.wordpress.com/62/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/comments/meteorhalley.wordpress.com/62/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/godelicious/meteorhalley.wordpress.com/62/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/delicious/meteorhalley.wordpress.com/62/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/gostumble/meteorhalley.wordpress.com/62/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/stumble/meteorhalley.wordpress.com/62/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/godigg/meteorhalley.wordpress.com/62/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/digg/meteorhalley.wordpress.com/62/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/goreddit/meteorhalley.wordpress.com/62/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/reddit/meteorhalley.wordpress.com/62/" /></a> <img alt="" border="0" src="http://stats.wordpress.com/b.gif?host=meteorhalley.wordpress.com&blog=3185850&post=62&subd=meteorhalley&ref=&feed=1" /></div>]]></content:encoded>
			<wfw:commentRss>http://meteorhalley.wordpress.com/2008/04/03/saturn/feed/</wfw:commentRss>
		<slash:comments>0</slash:comments>
	
		<media:content url="http://0.gravatar.com/avatar/80d91880e5e7c91d9244aaeb122d8aef?s=96&#38;d=identicon" medium="image">
			<media:title type="html">meteorhalley</media:title>
		</media:content>

		<media:content url="http://meteorhalley.files.wordpress.com/2008/04/240px-saturn_from_cassini_orbiter_2004-10-06.thumbnail.jpg" medium="image">
			<media:title type="html">240px-saturn_from_cassini_orbiter_2004-10-06.jpg</media:title>
		</media:content>
	</item>
		<item>
		<title>Neptune</title>
		<link>http://meteorhalley.wordpress.com/2008/04/03/neptune/</link>
		<comments>http://meteorhalley.wordpress.com/2008/04/03/neptune/#comments</comments>
		<pubDate>Thu, 03 Apr 2008 05:33:48 +0000</pubDate>
		<dc:creator>meteorhalley</dc:creator>
				<category><![CDATA[Uncategorized]]></category>

		<guid isPermaLink="false">http://meteorhalley.wordpress.com/2008/04/03/neptune/</guid>
		<description><![CDATA[Neptune

Neptune (pronounced /ˈnɛptjuːn/) is the eighth and farthest planet from the Sun in the Solar System. It is the fourth largest planet by diameter, and the third largest by mass. Neptune is 17 times the mass of Earth and is slightly more massive than its near-twin Uranus, which is 15 Earth masses and less dense. [...]<img alt="" border="0" src="http://stats.wordpress.com/b.gif?host=meteorhalley.wordpress.com&blog=3185850&post=60&subd=meteorhalley&ref=&feed=1" />]]></description>
			<content:encoded><![CDATA[<div class='snap_preview'><br /><h1 class="firstHeading">Neptune</h1>
<p><a href="http://meteorhalley.files.wordpress.com/2008/04/240px-neptune.jpg" title="240px-neptune.jpg"><img src="http://meteorhalley.files.wordpress.com/2008/04/240px-neptune.thumbnail.jpg" alt="240px-neptune.jpg" /></a><br />
<b>Neptune</b> (<a href="http://en.wikipedia.org/wiki/Help:Pronunciation" title="Pronunciation">pronounced</a> <span title="Pronunciation in the International Phonetic Alphabet (IPA)" class="IPA">/ˈnɛptjuːn/</span>) is the eighth and farthest <a href="http://en.wikipedia.org/wiki/Planet" title="Planet">planet</a> from the <a href="http://en.wikipedia.org/wiki/Sun" title="Sun">Sun</a> in the <a href="http://en.wikipedia.org/wiki/Solar_System" title="Solar System">Solar System</a>. It is the fourth largest planet by diameter, and the third largest by mass. Neptune is 17 times the mass of <a href="http://en.wikipedia.org/wiki/Earth" title="Earth">Earth</a> and is slightly more massive than its near-twin <a href="http://en.wikipedia.org/wiki/Uranus" title="Uranus">Uranus</a>, which is 15 Earth masses and less dense. The planet is named after the <a href="http://en.wikipedia.org/wiki/Neptune_%28mythology%29" title="Neptune (mythology)">Roman god of the sea</a>. Its <a href="http://en.wikipedia.org/wiki/Astronomical_symbol" class="mw-redirect" title="Astronomical symbol">astronomical symbol</a> is <a href="http://en.wikipedia.org/wiki/Image:Neptune_symbol.svg" class="image" title="Astronomical symbol for Neptune."><img src="http://upload.wikimedia.org/wikipedia/commons/thumb/4/47/Neptune_symbol.svg/20px-Neptune_symbol.svg.png" alt="Astronomical symbol for Neptune." border="0" height="20" width="20" /></a>, a stylized version of the god Neptune&#8217;s <a href="http://en.wikipedia.org/wiki/Trident" title="Trident">trident</a>.</p>
<p>Discovered on <a href="http://en.wikipedia.org/wiki/September_23" title="September 23">September 23</a>, <a href="http://en.wikipedia.org/wiki/1846" title="1846">1846</a>, Neptune was the first planet found by mathematical prediction rather than regular observation. Unexpected changes in the orbit of Uranus led astronomers to deduce the <a href="http://en.wikipedia.org/wiki/Gravitation" title="Gravitation">gravitational</a> <a href="http://en.wikipedia.org/wiki/Perturbation_%28astronomy%29" title="Perturbation (astronomy)">perturbation</a> of an unknown planet. Neptune was found within a degree of the predicted position. The moon <a href="http://en.wikipedia.org/wiki/Triton_%28moon%29" title="Triton (moon)">Triton</a> was found shortly thereafter, but none of the planet&#8217;s other 12 <a href="http://en.wikipedia.org/wiki/Moons_of_Neptune" title="Moons of Neptune">moons</a> were discovered before the 20th century. Neptune has been visited by only one spacecraft, <i><a href="http://en.wikipedia.org/wiki/Voyager_2" title="Voyager 2">Voyager 2</a></i>, which flew by the planet on <a href="http://en.wikipedia.org/wiki/August_25" title="August 25">August 25</a>, <a href="http://en.wikipedia.org/wiki/1989" title="1989">1989</a>.</p>
<p>Neptune&#8217;s <a href="http://en.wikipedia.org/wiki/Atmosphere" title="Atmosphere">atmosphere</a> is primarily composed of <a href="http://en.wikipedia.org/wiki/Hydrogen" title="Hydrogen">hydrogen</a> and <a href="http://en.wikipedia.org/wiki/Helium" title="Helium">helium</a> along with traces of <a href="http://en.wikipedia.org/wiki/Methane" title="Methane">methane</a>. The methane in the atmosphere, in part, accounts for the planet&#8217;s <a href="http://en.wikipedia.org/wiki/Azure_%28color%29" title="Azure (color)">blue</a> appearance.<sup><a href="http://en.wikipedia.org/wiki/Neptune#cite_note-bluecolour-10"></a></sup> Neptune also has the strongest winds of any planet in the solar system, measured as high as 2,100 <a href="http://en.wikipedia.org/wiki/Kilometres_per_hour" title="Kilometres per hour">kilometres per hour</a> (1,300 <a href="http://en.wikipedia.org/wiki/Miles_per_hour" title="Miles per hour">mph</a>). At the time of the 1989 <i><a href="http://en.wikipedia.org/wiki/Voyager_2" title="Voyager 2">Voyager 2</a></i> <a href="http://en.wikipedia.org/wiki/Planetary_flyby" class="mw-redirect" title="Planetary flyby">flyby</a>, its southern hemisphere possessed a <a href="http://en.wikipedia.org/wiki/Great_Dark_Spot" title="Great Dark Spot">Great Dark Spot</a> comparable to the <a href="http://en.wikipedia.org/wiki/Great_Red_Spot" title="Great Red Spot">Great Red Spot</a> on <a href="http://en.wikipedia.org/wiki/Jupiter" title="Jupiter">Jupiter</a>. Neptune&#8217;s temperature at its cloud tops is usually close to −218 <a href="http://en.wikipedia.org/wiki/Celsius" title="Celsius">°C</a> (55.1 <a href="http://en.wikipedia.org/wiki/Kelvin" title="Kelvin">K</a>), one of the coldest in the solar system, due to its great distance from the Sun. The temperature in Neptune&#8217;s centre is about 7,000 °C (7,270 K), which is comparable to the Sun&#8217;s surface and similar to most other known planets. Neptune has a faint and fragmented <a href="http://en.wikipedia.org/wiki/Planetary_ring" title="Planetary ring">ring system</a>, which may have been detected during the 1960s but was only indisputably confirmed by <i>Voyager 2</i>.</p>
<img alt="" border="0" src="http://feeds.wordpress.com/1.0/categories/meteorhalley.wordpress.com/60/" /> <img alt="" border="0" src="http://feeds.wordpress.com/1.0/tags/meteorhalley.wordpress.com/60/" /> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/gocomments/meteorhalley.wordpress.com/60/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/comments/meteorhalley.wordpress.com/60/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/godelicious/meteorhalley.wordpress.com/60/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/delicious/meteorhalley.wordpress.com/60/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/gostumble/meteorhalley.wordpress.com/60/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/stumble/meteorhalley.wordpress.com/60/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/godigg/meteorhalley.wordpress.com/60/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/digg/meteorhalley.wordpress.com/60/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/goreddit/meteorhalley.wordpress.com/60/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/reddit/meteorhalley.wordpress.com/60/" /></a> <img alt="" border="0" src="http://stats.wordpress.com/b.gif?host=meteorhalley.wordpress.com&blog=3185850&post=60&subd=meteorhalley&ref=&feed=1" /></div>]]></content:encoded>
			<wfw:commentRss>http://meteorhalley.wordpress.com/2008/04/03/neptune/feed/</wfw:commentRss>
		<slash:comments>0</slash:comments>
	
		<media:content url="http://0.gravatar.com/avatar/80d91880e5e7c91d9244aaeb122d8aef?s=96&#38;d=identicon" medium="image">
			<media:title type="html">meteorhalley</media:title>
		</media:content>

		<media:content url="http://meteorhalley.files.wordpress.com/2008/04/240px-neptune.thumbnail.jpg" medium="image">
			<media:title type="html">240px-neptune.jpg</media:title>
		</media:content>

		<media:content url="http://upload.wikimedia.org/wikipedia/commons/thumb/4/47/Neptune_symbol.svg/20px-Neptune_symbol.svg.png" medium="image">
			<media:title type="html">Astronomical symbol for Neptune.</media:title>
		</media:content>
	</item>
		<item>
		<title>Uranus</title>
		<link>http://meteorhalley.wordpress.com/2008/04/03/uranus/</link>
		<comments>http://meteorhalley.wordpress.com/2008/04/03/uranus/#comments</comments>
		<pubDate>Thu, 03 Apr 2008 05:32:12 +0000</pubDate>
		<dc:creator>meteorhalley</dc:creator>
				<category><![CDATA[Uncategorized]]></category>

		<guid isPermaLink="false">http://meteorhalley.wordpress.com/?p=58</guid>
		<description><![CDATA[Uranus

Uranus (pronounced /ˈjʊərənəs/ or /jʊˈreɪnəs/) is the seventh planet from the Sun and the third-largest and fourth-most massive planet in the solar system. It is named after the ancient Greek deity of the sky (Uranus, Οὐρανός), the father of Kronos (Saturn) and grandfather of Zeus (Jupiter). Uranus was the first planet discovered in modern times. [...]<img alt="" border="0" src="http://stats.wordpress.com/b.gif?host=meteorhalley.wordpress.com&blog=3185850&post=58&subd=meteorhalley&ref=&feed=1" />]]></description>
			<content:encoded><![CDATA[<div class='snap_preview'><br /><h1 class="firstHeading">Uranus</h1>
<p><a href="http://meteorhalley.files.wordpress.com/2008/04/240px-uranus_voyager_2.jpg" title="240px-uranus_voyager_2.jpg"><img src="http://meteorhalley.files.wordpress.com/2008/04/240px-uranus_voyager_2.thumbnail.jpg" alt="240px-uranus_voyager_2.jpg" /></a><br />
<b>Uranus</b> (<a href="http://en.wikipedia.org/wiki/Help:Pronunciation" title="Pronunciation">pronounced</a> <span title="Pronunciation in the International Phonetic Alphabet (IPA)" class="IPA">/ˈjʊərənəs/</span> or <span title="Representation in the International Phonetic Alphabet (IPA)" class="IPA">/jʊˈreɪnəs/</span>) is the seventh <a href="http://en.wikipedia.org/wiki/Planet" title="Planet">planet</a> from the <a href="http://en.wikipedia.org/wiki/Sun" title="Sun">Sun</a> and the third-largest and fourth-most massive planet in the <a href="http://en.wikipedia.org/wiki/Solar_system" class="mw-redirect" title="Solar system">solar system</a>. It is named after the ancient Greek deity of the sky (<a href="http://en.wikipedia.org/wiki/Uranus_%28mythology%29" title="Uranus (mythology)">Uranus</a>, <i><a href="http://en.wiktionary.org/wiki/%CE%BF%E1%BD%90%CF%81%CE%B1%CE%BD%CF%8C%CF%82" class="extiw" title="οὐρανός"><span>Οὐρανός</span></a></i>), the father of <a href="http://en.wikipedia.org/wiki/Cronus" title="Cronus">Kronos</a> (<a href="http://en.wikipedia.org/wiki/Saturn_%28mythology%29" title="Saturn (mythology)">Saturn</a>) and grandfather of <a href="http://en.wikipedia.org/wiki/Zeus" title="Zeus">Zeus</a> (<a href="http://en.wikipedia.org/wiki/Jupiter_%28mythology%29" title="Jupiter (mythology)">Jupiter</a>). Uranus was the first planet discovered in <a href="http://en.wikipedia.org/wiki/Modern_times" class="mw-redirect" title="Modern times">modern times</a>. Though it is visible to the naked eye like the five <a href="http://en.wikipedia.org/wiki/Classical_planet" class="mw-redirect" title="Classical planet">classical planets</a>, it was never recognized as a planet by ancient observers due to its dimness. Sir <a href="http://en.wikipedia.org/wiki/William_Herschel" title="William Herschel">William Herschel</a> announced its discovery on <a href="http://en.wikipedia.org/wiki/March_13" title="March 13">March 13</a>, <a href="http://en.wikipedia.org/wiki/1781" title="1781">1781</a>, expanding the known boundaries of the <a href="http://en.wikipedia.org/wiki/Solar_system" class="mw-redirect" title="Solar system">solar system</a> for the first time in modern history. This was also the first discovery of a planet made using a <a href="http://en.wikipedia.org/wiki/Telescope" title="Telescope">telescope</a>.</p>
<p>Uranus and <a href="http://en.wikipedia.org/wiki/Neptune" title="Neptune">Neptune</a> have internal and <a href="http://en.wikipedia.org/wiki/Atmospheric_chemistry" title="Atmospheric chemistry">atmospheric compositions</a> different from those of the larger <a href="http://en.wikipedia.org/wiki/Gas_giant" title="Gas giant">gas giants</a> <a href="http://en.wikipedia.org/wiki/Jupiter_%28planet%29" class="mw-redirect" title="Jupiter (planet)">Jupiter</a> and <a href="http://en.wikipedia.org/wiki/Saturn_%28planet%29" class="mw-redirect" title="Saturn (planet)">Saturn</a>. As such, astronomers sometimes place them in a separate category, the &#8220;<a href="http://en.wikipedia.org/wiki/Ice_giant" class="mw-redirect" title="Ice giant">ice giants</a>&#8220;. Uranus&#8217; atmosphere, while similar to Jupiter and Saturn in being composed primarily of <a href="http://en.wikipedia.org/wiki/Hydrogen" title="Hydrogen">hydrogen</a> and <a href="http://en.wikipedia.org/wiki/Helium" title="Helium">helium</a>, contains a higher proportion of &#8220;ices&#8221; such as <a href="http://en.wikipedia.org/wiki/Water" title="Water">water</a>, <a href="http://en.wikipedia.org/wiki/Ammonia" title="Ammonia">ammonia</a> and <a href="http://en.wikipedia.org/wiki/Methane" title="Methane">methane</a>, along with the usual traces of <a href="http://en.wikipedia.org/wiki/Hydrocarbon" title="Hydrocarbon">hydrocarbons</a>. It is the coldest planetary atmosphere in the Solar System, with a minimum temperature of 49 <a href="http://en.wikipedia.org/wiki/Kelvin" title="Kelvin">K</a> (−224 <a href="http://en.wikipedia.org/wiki/Celsius" title="Celsius">°C</a>). It has a complex, layered <a href="http://en.wikipedia.org/wiki/Cloud" title="Cloud">cloud</a> structure, with water thought to make up the lowest clouds, and methane thought to make up the uppermost layer of clouds.</p>
<p>Like the other giant planets, Uranus has a <a href="http://en.wikipedia.org/wiki/Ring_system" class="mw-redirect" title="Ring system">ring system</a>, a <a href="http://en.wikipedia.org/wiki/Magnetosphere" title="Magnetosphere">magnetosphere</a>, and numerous <a href="http://en.wikipedia.org/wiki/Natural_satellite" title="Natural satellite">moons</a>. The Uranian system has a unique configuration among the planets because its <a href="http://en.wikipedia.org/wiki/Axis_of_rotation" class="mw-redirect" title="Axis of rotation">axis of rotation</a> is tilted sideways, nearly into the plane of its revolution about the Sun; its north and south poles lie where most other planets have their equators. Seen from Earth, Uranus&#8217; rings can appear to circle the planet like an <a href="http://en.wikipedia.org/wiki/Target_archery" title="Target archery">archery target</a> and its moons revolve around it like the hands of a clock, though in 2007 and 2008 the rings appear edge-on. In 1986, images from <i><a href="http://en.wikipedia.org/wiki/Voyager_2" title="Voyager 2">Voyager 2</a></i> showed Uranus as a virtually featureless planet in visible light without the cloud bands or <a href="http://en.wikipedia.org/wiki/Storms" class="mw-redirect" title="Storms">storms</a> associated with the other giants. However, terrestrial observers have seen signs of <a href="http://en.wikipedia.org/wiki/Season" title="Season">seasonal</a> change and increased <a href="http://en.wikipedia.org/wiki/Weather" title="Weather">weather</a> activity in recent years as Uranus approached its <a href="http://en.wikipedia.org/wiki/Equinox" title="Equinox">equinox</a>. The <a href="http://en.wikipedia.org/wiki/Wind" title="Wind">wind</a> speeds on Uranus can reach 250 meters per second.</p>
<img alt="" border="0" src="http://feeds.wordpress.com/1.0/categories/meteorhalley.wordpress.com/58/" /> <img alt="" border="0" src="http://feeds.wordpress.com/1.0/tags/meteorhalley.wordpress.com/58/" /> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/gocomments/meteorhalley.wordpress.com/58/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/comments/meteorhalley.wordpress.com/58/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/godelicious/meteorhalley.wordpress.com/58/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/delicious/meteorhalley.wordpress.com/58/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/gostumble/meteorhalley.wordpress.com/58/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/stumble/meteorhalley.wordpress.com/58/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/godigg/meteorhalley.wordpress.com/58/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/digg/meteorhalley.wordpress.com/58/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/goreddit/meteorhalley.wordpress.com/58/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/reddit/meteorhalley.wordpress.com/58/" /></a> <img alt="" border="0" src="http://stats.wordpress.com/b.gif?host=meteorhalley.wordpress.com&blog=3185850&post=58&subd=meteorhalley&ref=&feed=1" /></div>]]></content:encoded>
			<wfw:commentRss>http://meteorhalley.wordpress.com/2008/04/03/uranus/feed/</wfw:commentRss>
		<slash:comments>0</slash:comments>
	
		<media:content url="http://0.gravatar.com/avatar/80d91880e5e7c91d9244aaeb122d8aef?s=96&#38;d=identicon" medium="image">
			<media:title type="html">meteorhalley</media:title>
		</media:content>

		<media:content url="http://meteorhalley.files.wordpress.com/2008/04/240px-uranus_voyager_2.thumbnail.jpg" medium="image">
			<media:title type="html">240px-uranus_voyager_2.jpg</media:title>
		</media:content>
	</item>
		<item>
		<title>Jupiter The Giant Epicenter</title>
		<link>http://meteorhalley.wordpress.com/2008/04/02/jupiter-the-giant-epicenter/</link>
		<comments>http://meteorhalley.wordpress.com/2008/04/02/jupiter-the-giant-epicenter/#comments</comments>
		<pubDate>Wed, 02 Apr 2008 12:43:02 +0000</pubDate>
		<dc:creator>meteorhalley</dc:creator>
				<category><![CDATA[Uncategorized]]></category>

		<guid isPermaLink="false">http://meteorhalley.wordpress.com/2008/04/02/jupiter-the-giant-epicenter/</guid>
		<description><![CDATA[Jupiter

Jupiter (pronounced /ˈdʒuːpɨtɚ/) 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, along with Saturn, Uranus and Neptune, is classified as a gas giant. Together, these four planets [...]<img alt="" border="0" src="http://stats.wordpress.com/b.gif?host=meteorhalley.wordpress.com&blog=3185850&post=56&subd=meteorhalley&ref=&feed=1" />]]></description>
			<content:encoded><![CDATA[<div class='snap_preview'><br /><h1 class="firstHeading">Jupiter</h1>
<p><a href="http://meteorhalley.files.wordpress.com/2008/04/240px-jupiter.jpg" title="240px-jupiter.jpg"><img src="http://meteorhalley.files.wordpress.com/2008/04/240px-jupiter.thumbnail.jpg" alt="240px-jupiter.jpg" /></a></p>
<p><b>Jupiter</b> (<a href="http://en.wikipedia.org/wiki/Help:Pronunciation" title="Pronunciation">pronounced</a> <span title="Pronunciation in the International Phonetic Alphabet (IPA)" class="IPA">/ˈdʒuːpɨtɚ/</span>) is the fifth <a href="http://en.wikipedia.org/wiki/Planet" title="Planet">planet</a> from the <a href="http://en.wikipedia.org/wiki/Sun" title="Sun">Sun</a> and the <a href="http://en.wikipedia.org/wiki/Solar_system_by_size" class="mw-redirect" title="Solar system by size">largest</a> planet within the <a href="http://en.wikipedia.org/wiki/Solar_System" title="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, along with <a href="http://en.wikipedia.org/wiki/Saturn" title="Saturn">Saturn</a>, <a href="http://en.wikipedia.org/wiki/Uranus" title="Uranus">Uranus</a> and <a href="http://en.wikipedia.org/wiki/Neptune" title="Neptune">Neptune</a>, is classified as a <a href="http://en.wikipedia.org/wiki/Gas_giant" title="Gas giant">gas giant</a>. Together, these four planets are sometimes referred to as the <b><a href="http://en.wikipedia.org/wiki/Jovian_planet" class="mw-redirect" title="Jovian planet">Jovian planets</a></b>, where <i>Jovian</i> is the <a href="http://en.wikipedia.org/wiki/Adjective" title="Adjective">adjectival</a> form of Jupiter.</p>
<p>The planet was known by <a href="http://en.wikipedia.org/wiki/Astronomer" title="Astronomer">astronomers</a> of ancient times and was associated with the mythology and religious beliefs of many cultures. The <a href="http://en.wikipedia.org/wiki/Ancient_Rome" title="Ancient Rome">Romans</a> named the planet after the <a href="http://en.wikipedia.org/wiki/Roman_mythology" title="Roman mythology">Roman god</a> <a href="http://en.wikipedia.org/wiki/Jupiter_%28mythology%29" title="Jupiter (mythology)">Jupiter</a>.<sup><a href="http://en.wikipedia.org/wiki/Jupiter#cite_note-etymologyonline-9"></a></sup> When viewed from Earth, Jupiter can reach an <a href="http://en.wikipedia.org/wiki/Apparent_magnitude" title="Apparent magnitude">apparent magnitude</a> of −2.8, making it the third brightest object in the <a href="http://en.wikipedia.org/wiki/Night_sky" title="Night sky">night sky</a> after the <a href="http://en.wikipedia.org/wiki/Moon" title="Moon">Moon</a> and <a href="http://en.wikipedia.org/wiki/Venus" title="Venus">Venus</a>. (However, at certain points in its orbit, <a href="http://en.wikipedia.org/wiki/Mars" title="Mars">Mars</a> can briefly exceed Jupiter&#8217;s brightness.)</p>
<p>The planet Jupiter is primarily composed of <a href="http://en.wikipedia.org/wiki/Hydrogen" title="Hydrogen">hydrogen</a> with a small proportion of <a href="http://en.wikipedia.org/wiki/Helium" title="Helium">helium</a>; it may also have a rocky core of heavier elements under high pressure. Because of its rapid rotation, Jupiter&#8217;s shape is that of an <a href="http://en.wikipedia.org/wiki/Oblate_spheroid" title="Oblate spheroid">oblate spheroid</a> (it possesses a slight but noticeable bulge around the equator). The outer atmosphere is visibly segregated into several bands at different latitudes, resulting in turbulence and storms along their interacting boundaries. A prominent result is the <a href="http://en.wikipedia.org/wiki/Great_Red_Spot" title="Great Red Spot">Great Red Spot</a>, a giant storm that is known to have existed since at least the seventeenth century. Surrounding the planet is a faint <a href="http://en.wikipedia.org/wiki/Planetary_ring" title="Planetary ring">planetary ring</a> system and a powerful <a href="http://en.wikipedia.org/wiki/Magnetosphere" title="Magnetosphere">magnetosphere</a>. There are also at least 63 moons, including the four large moons called the <a href="http://en.wikipedia.org/wiki/Galilean_moons" title="Galilean moons">Galilean moons</a> that were first discovered by <a href="http://en.wikipedia.org/wiki/Galileo_Galilei" title="Galileo Galilei">Galileo Galilei</a> in 1610. <a href="http://en.wikipedia.org/wiki/Ganymede_%28moon%29" title="Ganymede (moon)">Ganymede</a>, the largest of these moons, has a diameter greater than that of the planet <a href="http://en.wikipedia.org/wiki/Mercury_%28planet%29" title="Mercury (planet)">Mercury</a>.</p>
<p>Jupiter has been explored on several occasions by robotic spacecraft, most notably during the early <a href="http://en.wikipedia.org/wiki/Pioneer_program" title="Pioneer program">Pioneer</a> and <a href="http://en.wikipedia.org/wiki/Voyager_program" title="Voyager program">Voyager</a> flyby missions and later by the <a href="http://en.wikipedia.org/wiki/Galileo_%28spacecraft%29" title="Galileo (spacecraft)">Galileo orbiter</a>. The latest probe to visit Jupiter was the Pluto-bound <a href="http://en.wikipedia.org/wiki/New_Horizons" title="New Horizons">New Horizons</a> spacecraft in late February 2007. The probe <a href="http://en.wikipedia.org/wiki/Gravitational_slingshot" class="mw-redirect" title="Gravitational slingshot">used</a> the gravity from Jupiter to increase its speed and adjust its trajectory toward Pluto, thereby saving years of travel. Future targets for exploration include the possible ice-covered liquid ocean on the Jovian moon <a href="http://en.wikipedia.org/wiki/Europa_%28moon%29" title="Europa (moon)">Europa</a>.</p>
<img alt="" border="0" src="http://feeds.wordpress.com/1.0/categories/meteorhalley.wordpress.com/56/" /> <img alt="" border="0" src="http://feeds.wordpress.com/1.0/tags/meteorhalley.wordpress.com/56/" /> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/gocomments/meteorhalley.wordpress.com/56/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/comments/meteorhalley.wordpress.com/56/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/godelicious/meteorhalley.wordpress.com/56/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/delicious/meteorhalley.wordpress.com/56/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/gostumble/meteorhalley.wordpress.com/56/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/stumble/meteorhalley.wordpress.com/56/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/godigg/meteorhalley.wordpress.com/56/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/digg/meteorhalley.wordpress.com/56/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/goreddit/meteorhalley.wordpress.com/56/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/reddit/meteorhalley.wordpress.com/56/" /></a> <img alt="" border="0" src="http://stats.wordpress.com/b.gif?host=meteorhalley.wordpress.com&blog=3185850&post=56&subd=meteorhalley&ref=&feed=1" /></div>]]></content:encoded>
			<wfw:commentRss>http://meteorhalley.wordpress.com/2008/04/02/jupiter-the-giant-epicenter/feed/</wfw:commentRss>
		<slash:comments>0</slash:comments>
	
		<media:content url="http://0.gravatar.com/avatar/80d91880e5e7c91d9244aaeb122d8aef?s=96&#38;d=identicon" medium="image">
			<media:title type="html">meteorhalley</media:title>
		</media:content>

		<media:content url="http://meteorhalley.files.wordpress.com/2008/04/240px-jupiter.thumbnail.jpg" medium="image">
			<media:title type="html">240px-jupiter.jpg</media:title>
		</media:content>
	</item>
		<item>
		<title>Earth Of The Fountins Heel</title>
		<link>http://meteorhalley.wordpress.com/2008/04/02/earth-of-the-fountins-heel/</link>
		<comments>http://meteorhalley.wordpress.com/2008/04/02/earth-of-the-fountins-heel/#comments</comments>
		<pubDate>Wed, 02 Apr 2008 12:39:18 +0000</pubDate>
		<dc:creator>meteorhalley</dc:creator>
				<category><![CDATA[Uncategorized]]></category>

		<guid isPermaLink="false">http://meteorhalley.wordpress.com/?p=54</guid>
		<description><![CDATA[Earth

Earth (pronounced /ˈɝːθ/) is the third planet from the Sun and is the largest of the terrestrial planets in the Solar System in both diameter and mass. It is also referred to as the Earth, Planet Earth, the World, and Terra.
Home to millions of species, including humans, Earth is the only place in the universe [...]<img alt="" border="0" src="http://stats.wordpress.com/b.gif?host=meteorhalley.wordpress.com&blog=3185850&post=54&subd=meteorhalley&ref=&feed=1" />]]></description>
			<content:encoded><![CDATA[<div class='snap_preview'><br /><h1 class="firstHeading">Earth</h1>
<p><a href="http://meteorhalley.files.wordpress.com/2008/04/240px-the_earth_seen_from_apollo_17.jpg" title="Earth"><img src="http://meteorhalley.files.wordpress.com/2008/04/240px-the_earth_seen_from_apollo_17.thumbnail.jpg" alt="Earth" /></a></p>
<p><b>Earth</b> (<a href="http://en.wikipedia.org/wiki/Help:Pronunciation" title="Pronunciation">pronounced</a> <span title="Pronunciation in the International Phonetic Alphabet (IPA)" class="IPA">/ˈɝːθ/</span>) is the third <a href="http://en.wikipedia.org/wiki/Planet" title="Planet">planet</a> from the <a href="http://en.wikipedia.org/wiki/Sun" title="Sun">Sun</a> and is the largest of the <a href="http://en.wikipedia.org/wiki/Terrestrial_planet" title="Terrestrial planet">terrestrial planets</a> in the <a href="http://en.wikipedia.org/wiki/Solar_System" title="Solar System">Solar System</a> in both <a href="http://en.wikipedia.org/wiki/Diameter" title="Diameter">diameter</a> and <a href="http://en.wikipedia.org/wiki/Mass" title="Mass">mass</a>. It is also referred to as <i>the Earth</i>, <i>Planet Earth</i>, <i>the <a href="http://en.wikipedia.org/wiki/World" title="World">World</a></i>, and <i><a href="http://en.wiktionary.org/wiki/Terra" class="external text" title="http://en.wiktionary.org/wiki/Terra" rel="nofollow">Terra</a></i>.</p>
<p>Home to millions of <a href="http://en.wikipedia.org/wiki/Species" title="Species">species</a>, including <a href="http://en.wikipedia.org/wiki/Human" title="Human">humans</a>, Earth is the only place in the <a href="http://en.wikipedia.org/wiki/Universe" title="Universe">universe</a> where <a href="http://en.wikipedia.org/wiki/Life" title="Life">life</a> is known to exist. Scientific evidence indicates that the planet formed <a href="http://en.wikipedia.org/wiki/Age_of_the_Earth" title="Age of the Earth">4.54 billion years</a> ago,<sup><a href="http://en.wikipedia.org/wiki/Earth#cite_note-10"></a></sup> and life appeared on its surface within a billion years. Since then, Earth&#8217;s <a href="http://en.wikipedia.org/wiki/Biosphere" title="Biosphere">biosphere</a> has significantly altered <a href="http://en.wikipedia.org/wiki/Earth%27s_atmosphere" title="Earth's atmosphere">the atmosphere</a> and other <a href="http://en.wikipedia.org/wiki/Abiotic" class="mw-redirect" title="Abiotic">abiotic</a> conditions on the planet, enabling the proliferation of <a href="http://en.wikipedia.org/wiki/Aerobic_organisms" class="mw-redirect" title="Aerobic organisms">aerobic organisms</a> as well as the formation of the <a href="http://en.wikipedia.org/wiki/Ozone_layer" title="Ozone layer">ozone layer</a> which, together with Earth&#8217;s <a href="http://en.wikipedia.org/wiki/Magnetic_field" title="Magnetic field">magnetic field</a>, blocks harmful radiation, permitting life on land.</p>
<p>Earth&#8217;s <a href="http://en.wikipedia.org/wiki/Crust_%28geology%29" title="Crust (geology)">outer surface</a> is divided into several rigid segments, or <a href="http://en.wikipedia.org/wiki/Tectonic_plate" class="mw-redirect" title="Tectonic plate">tectonic plates</a>, that gradually migrate across the surface over periods of <a href="http://en.wikipedia.org/wiki/Geologic_time_scale" title="Geologic time scale">many millions of years</a>. About 71% of the surface is covered with <a href="http://en.wikipedia.org/wiki/Seawater" title="Seawater">salt-water</a> <a href="http://en.wikipedia.org/wiki/Ocean" title="Ocean">oceans</a>, the remainder consisting of <a href="http://en.wikipedia.org/wiki/Continent" title="Continent">continents</a> and <a href="http://en.wikipedia.org/wiki/Island" title="Island">islands</a>; liquid <a href="http://en.wikipedia.org/wiki/Water" title="Water">water</a>, necessary for all known life, is not known to exist on any other planet&#8217;s surface.<sup><a href="http://en.wikipedia.org/wiki/Earth#cite_note-13"></a></sup> Earth&#8217;s interior remains active, with a thick layer of relatively solid <a href="http://en.wikipedia.org/wiki/Mantle_%28geology%29" title="Mantle (geology)">mantle</a>, a liquid outer core that generates a magnetic field, and a solid iron <a href="http://en.wikipedia.org/wiki/Inner_core" title="Inner core">inner core</a>.</p>
<p>Earth interacts with other objects in <a href="http://en.wikipedia.org/wiki/Outer_space" title="Outer space">outer space</a>, including the <a href="http://en.wikipedia.org/wiki/Sun" title="Sun">Sun</a> and the <a href="http://en.wikipedia.org/wiki/Moon" title="Moon">Moon</a>. At present, Earth orbits the Sun once for every roughly 366.26 times it rotates about its axis. This length of time is a <a href="http://en.wikipedia.org/wiki/Sidereal_year" title="Sidereal year">sidereal year</a>, which is equal to 365.26 <a href="http://en.wikipedia.org/wiki/Solar_day" class="mw-redirect" title="Solar day">solar days</a>.<sup><a href="http://en.wikipedia.org/wiki/Earth#cite_note-14">[15]</a></sup> The Earth&#8217;s axis of rotation is <a href="http://en.wikipedia.org/wiki/Axial_tilt" title="Axial tilt">tilted</a> 23.4° away from the <a href="http://en.wikipedia.org/wiki/Perpendicular" title="Perpendicular">perpendicular</a> to its <a href="http://en.wikipedia.org/wiki/Orbital_plane_%28astronomy%29" title="Orbital plane (astronomy)">orbital plane</a>,<sup><a href="http://en.wikipedia.org/wiki/Earth#cite_note-15">[16]</a></sup> producing seasonal variations on the planet&#8217;s surface with a period of one <a href="http://en.wikipedia.org/wiki/Tropical_year" title="Tropical year">tropical year</a> (365.24 solar days). Earth&#8217;s only known <a href="http://en.wikipedia.org/wiki/Natural_satellite" title="Natural satellite">natural satellite</a>, the Moon, which began orbiting it about 4.53 billion years ago, provides ocean <a href="http://en.wikipedia.org/wiki/Tide" title="Tide">tides</a>, stabilizes the axial tilt and gradually slows the planet&#8217;s rotation. A <a href="http://en.wikipedia.org/wiki/Comet" title="Comet">cometary</a> bombardment during the early history of the planet played a role in the formation of the oceans. Later, <a href="http://en.wikipedia.org/wiki/Asteroid" title="Asteroid">asteroid</a> impacts caused significant changes to the surface environment.</p>
<img alt="" border="0" src="http://feeds.wordpress.com/1.0/categories/meteorhalley.wordpress.com/54/" /> <img alt="" border="0" src="http://feeds.wordpress.com/1.0/tags/meteorhalley.wordpress.com/54/" /> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/gocomments/meteorhalley.wordpress.com/54/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/comments/meteorhalley.wordpress.com/54/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/godelicious/meteorhalley.wordpress.com/54/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/delicious/meteorhalley.wordpress.com/54/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/gostumble/meteorhalley.wordpress.com/54/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/stumble/meteorhalley.wordpress.com/54/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/godigg/meteorhalley.wordpress.com/54/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/digg/meteorhalley.wordpress.com/54/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/goreddit/meteorhalley.wordpress.com/54/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/reddit/meteorhalley.wordpress.com/54/" /></a> <img alt="" border="0" src="http://stats.wordpress.com/b.gif?host=meteorhalley.wordpress.com&blog=3185850&post=54&subd=meteorhalley&ref=&feed=1" /></div>]]></content:encoded>
			<wfw:commentRss>http://meteorhalley.wordpress.com/2008/04/02/earth-of-the-fountins-heel/feed/</wfw:commentRss>
		<slash:comments>0</slash:comments>
	
		<media:content url="http://0.gravatar.com/avatar/80d91880e5e7c91d9244aaeb122d8aef?s=96&#38;d=identicon" medium="image">
			<media:title type="html">meteorhalley</media:title>
		</media:content>

		<media:content url="http://meteorhalley.files.wordpress.com/2008/04/240px-the_earth_seen_from_apollo_17.thumbnail.jpg" medium="image">
			<media:title type="html">Earth</media:title>
		</media:content>
	</item>
		<item>
		<title>Venus</title>
		<link>http://meteorhalley.wordpress.com/2008/04/02/venus/</link>
		<comments>http://meteorhalley.wordpress.com/2008/04/02/venus/#comments</comments>
		<pubDate>Wed, 02 Apr 2008 12:32:56 +0000</pubDate>
		<dc:creator>meteorhalley</dc:creator>
				<category><![CDATA[Uncategorized]]></category>

		<guid isPermaLink="false">http://meteorhalley.wordpress.com/?p=52</guid>
		<description><![CDATA[Venus

Venus (pronounced /ˈvinəs/) is the second-closest planet to the Sun, orbiting it every 224.7 Earth days. It is the brightest natural object in the night sky, except for the Moon, reaching an apparent magnitude of −4.6. Because Venus is an inferior planet, from Earth it never appears to venture far from the Sun: its elongation [...]<img alt="" border="0" src="http://stats.wordpress.com/b.gif?host=meteorhalley.wordpress.com&blog=3185850&post=52&subd=meteorhalley&ref=&feed=1" />]]></description>
			<content:encoded><![CDATA[<div class='snap_preview'><br /><h1 class="firstHeading">Venus</h1>
<p><a href="http://meteorhalley.files.wordpress.com/2008/04/240px-venus-real.jpg" title="Venus"><img src="http://meteorhalley.files.wordpress.com/2008/04/240px-venus-real.thumbnail.jpg" alt="Venus" /></a></p>
<p><b>Venus</b> (<a href="http://en.wikipedia.org/wiki/Help:Pronunciation" title="Pronunciation">pronounced</a> <span title="Pronunciation in the International Phonetic Alphabet (IPA)" class="IPA">/ˈvinəs/</span>) is the second-closest <a href="http://en.wikipedia.org/wiki/Planet" title="Planet">planet</a> to the <a href="http://en.wikipedia.org/wiki/Sun" title="Sun">Sun</a>, orbiting it every 224.7 Earth days. It is the brightest natural object in the night sky, except for the <a href="http://en.wikipedia.org/wiki/Moon" title="Moon">Moon</a>, reaching an <a href="http://en.wikipedia.org/wiki/Apparent_magnitude" title="Apparent magnitude">apparent magnitude</a> of −4.6. Because Venus is an <a href="http://en.wikipedia.org/wiki/Inferior_planet" class="mw-redirect" title="Inferior planet">inferior planet</a>, from <a href="http://en.wikipedia.org/wiki/Earth" title="Earth">Earth</a> it never appears to venture far from the Sun: its <a href="http://en.wikipedia.org/wiki/Elongation_%28astronomy%29" title="Elongation (astronomy)">elongation</a> reaches a maximum of 47.8°. Venus reaches its maximum brightness shortly before sunrise or shortly after sunset, for which reason it is often called the <i>Morning Star</i> or the <i>Evening Star</i>.</p>
<p>Classified as a <a href="http://en.wikipedia.org/wiki/Terrestrial_planet" title="Terrestrial planet">terrestrial planet</a>, it is sometimes called Earth&#8217;s &#8220;sister planet&#8221;, for the two are similar in size, gravity, and bulk composition. Venus is covered with an opaque layer of highly reflective <a href="http://en.wikipedia.org/wiki/Cloud" title="Cloud">clouds</a> of <a href="http://en.wikipedia.org/wiki/Sulfuric_acid" title="Sulfuric acid">sulfuric acid</a>, preventing its surface from being seen from space in <a href="http://en.wikipedia.org/wiki/Visible_light" class="mw-redirect" title="Visible light">visible light</a>; this was a subject of great speculation until some of its secrets were revealed by <a href="http://en.wikipedia.org/wiki/Planetary_science" title="Planetary science">planetary science</a> in the twentieth century. Venus has the densest <a href="http://en.wikipedia.org/wiki/Atmosphere" title="Atmosphere">atmosphere</a> of all the terrestrial planets, consisting mostly of <a href="http://en.wikipedia.org/wiki/Carbon_dioxide" title="Carbon dioxide">carbon dioxide</a>, as it has no <a href="http://en.wikipedia.org/wiki/Carbon_cycle" title="Carbon cycle">carbon cycle</a> 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 the young Venus is believed to have possessed have totally evaporated, leaving a dusty dry desertscape with many slab-like rocks. The best hypothesis is that the evaporated water vapor has dissociated and, with the lack of a planetary magnetic field, the hydrogen has been swept into interplanetary space by the solar wind. The <a href="http://en.wikipedia.org/wiki/Atmospheric_pressure" title="Atmospheric pressure">atmospheric pressure</a> at the planet&#8217;s surface is 92 times that of the Earth.</p>
<p>Venus&#8217;s surface has been mapped in detail only in the last 20 years, by Project <a href="http://en.wikipedia.org/wiki/Magellan_probe" title="Magellan probe">Magellan</a>. It shows evidence of extensive <a href="http://en.wikipedia.org/wiki/Volcano" title="Volcano">volcanism</a>, and the <a href="http://en.wikipedia.org/wiki/Sulfur" title="Sulfur">sulfur</a> in the atmosphere is taken by some experts to show that there has been some recent volcanism, but it is an enigma as to why no evidence of lava flow accompanies any of the visible <a href="http://en.wikipedia.org/wiki/Caldera" title="Caldera">caldera</a>. It is also noteworthy that there are a surprisingly low number of <a href="http://en.wikipedia.org/wiki/Impact_craters" class="mw-redirect" title="Impact craters">impact craters</a>. This demonstrates that the surface is relatively young, approximately half a billion years old. There is no evidence for <a href="http://en.wikipedia.org/wiki/Plate_tectonics" title="Plate tectonics">plate tectonics</a>, possibly because its crust is too strong to <a href="http://en.wikipedia.org/wiki/Subduction" title="Subduction">subduct</a> without water to make it less <a href="http://en.wikipedia.org/wiki/Viscous" class="mw-redirect" title="Viscous">viscous</a>, and some suggest that instead Venus loses its internal heat in a periodic massive resurfacing event.</p>
<p>The adjective <i>Venusian</i> is commonly used for items related to Venus, though the <a href="http://en.wikipedia.org/wiki/Latin" title="Latin">Latin</a> adjective is the rarely used <i>Venerean</i>; the now-archaic <i><a href="http://en.wikipedia.org/wiki/Cytherean" title="Cytherean">Cytherean</a></i> is still occasionally encountered. Venus is the only planet in the <a href="http://en.wikipedia.org/wiki/Solar_System" title="Solar System">Solar System</a> named after a female figure.<sup><a href="http://en.wikipedia.org/wiki/Venus#cite_note-5"></a></sup> although two <a href="http://en.wikipedia.org/wiki/Dwarf_planet" title="Dwarf planet">dwarf planets</a>—<a href="http://en.wikipedia.org/wiki/Ceres_%28dwarf_planet%29" title="Ceres (dwarf planet)">Ceres</a> and <a href="http://en.wikipedia.org/wiki/Eris_%28dwarf_planet%29" title="Eris (dwarf planet)">Eris</a>—also have female names.</p>
<img alt="" border="0" src="http://feeds.wordpress.com/1.0/categories/meteorhalley.wordpress.com/52/" /> <img alt="" border="0" src="http://feeds.wordpress.com/1.0/tags/meteorhalley.wordpress.com/52/" /> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/gocomments/meteorhalley.wordpress.com/52/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/comments/meteorhalley.wordpress.com/52/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/godelicious/meteorhalley.wordpress.com/52/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/delicious/meteorhalley.wordpress.com/52/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/gostumble/meteorhalley.wordpress.com/52/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/stumble/meteorhalley.wordpress.com/52/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/godigg/meteorhalley.wordpress.com/52/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/digg/meteorhalley.wordpress.com/52/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/goreddit/meteorhalley.wordpress.com/52/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/reddit/meteorhalley.wordpress.com/52/" /></a> <img alt="" border="0" src="http://stats.wordpress.com/b.gif?host=meteorhalley.wordpress.com&blog=3185850&post=52&subd=meteorhalley&ref=&feed=1" /></div>]]></content:encoded>
			<wfw:commentRss>http://meteorhalley.wordpress.com/2008/04/02/venus/feed/</wfw:commentRss>
		<slash:comments>0</slash:comments>
	
		<media:content url="http://0.gravatar.com/avatar/80d91880e5e7c91d9244aaeb122d8aef?s=96&#38;d=identicon" medium="image">
			<media:title type="html">meteorhalley</media:title>
		</media:content>

		<media:content url="http://meteorhalley.files.wordpress.com/2008/04/240px-venus-real.thumbnail.jpg" medium="image">
			<media:title type="html">Venus</media:title>
		</media:content>
	</item>
		<item>
		<title>Mercury</title>
		<link>http://meteorhalley.wordpress.com/2008/04/02/mercury/</link>
		<comments>http://meteorhalley.wordpress.com/2008/04/02/mercury/#comments</comments>
		<pubDate>Wed, 02 Apr 2008 12:28:23 +0000</pubDate>
		<dc:creator>meteorhalley</dc:creator>
				<category><![CDATA[Uncategorized]]></category>

		<guid isPermaLink="false">http://meteorhalley.wordpress.com/?p=50</guid>
		<description><![CDATA[Mercury

Mercury (pronounced /ˈmɝkjʊəri/) is the innermost and smallest planet in the solar system, orbiting the Sun once every 88 days. Mercury is bright when viewed from Earth, ranging from −2.0 to 5.5 in apparent magnitude, but is not easily seen as its greatest angular separation from the Sun (greatest elongation) is only 28.3°: It can [...]<img alt="" border="0" src="http://stats.wordpress.com/b.gif?host=meteorhalley.wordpress.com&blog=3185850&post=50&subd=meteorhalley&ref=&feed=1" />]]></description>
			<content:encoded><![CDATA[<div class='snap_preview'><br /><p>Mercury</p>
<p><a href="http://meteorhalley.files.wordpress.com/2008/04/240px-mercury_in_color_-_prockter07.jpg" title="Mercury"><img src="http://meteorhalley.files.wordpress.com/2008/04/240px-mercury_in_color_-_prockter07.thumbnail.jpg" alt="Mercury" /></a></p>
<p><b>Mercury</b> (<a href="http://en.wikipedia.org/wiki/Help:Pronunciation" title="Pronunciation">pronounced</a> <span title="Pronunciation in the International Phonetic Alphabet (IPA)" class="IPA">/ˈmɝkjʊəri/</span>) is the innermost and smallest <a href="http://en.wikipedia.org/wiki/Planet" title="Planet">planet</a> in the <a href="http://en.wikipedia.org/wiki/Solar_system" class="mw-redirect" title="Solar system">solar system</a>, orbiting the <a href="http://en.wikipedia.org/wiki/Sun" title="Sun">Sun</a> once every 88 days. Mercury is bright when viewed from Earth, ranging from −2.0 to 5.5 in <a href="http://en.wikipedia.org/wiki/Apparent_magnitude" title="Apparent magnitude">apparent magnitude</a>, but is not easily seen as its greatest angular separation from the Sun (greatest <a href="http://en.wikipedia.org/wiki/Elongation_%28astronomy%29" title="Elongation (astronomy)">elongation</a>) is only 28.3°: It can only be seen in morning and evening <a href="http://en.wikipedia.org/wiki/Twilight" title="Twilight">twilight</a>. Comparatively little is known about it; the first of two <a href="http://en.wikipedia.org/wiki/Spacecraft" title="Spacecraft">spacecraft</a> to approach Mercury was <a href="http://en.wikipedia.org/wiki/Mariner_10" title="Mariner 10">Mariner 10</a> from 1974 to 1975, which mapped only about 45% of the planet’s surface.<sup><a href="http://en.wikipedia.org/wiki/Mercury_%28planet%29#cite_note-is_shr-4">[5]</a></sup> The second was the <a href="http://en.wikipedia.org/wiki/MESSENGER" title="MESSENGER">MESSENGER spacecraft</a>, which mapped another 30% of the planet during its flyby of <a href="http://en.wikipedia.org/wiki/January_14" title="January 14">January 14</a>, <a href="http://en.wikipedia.org/wiki/2008" title="2008">2008</a>.<sup><a href="http://en.wikipedia.org/wiki/Mercury_%28planet%29#cite_note-is_shr-4">[5]</a></sup> MESSENGER will make two more passes by Mercury, followed by orbital insertion in 2011, and will survey and map the entire planet.</p>
<p>Physically, Mercury is similar in appearance to the <a href="http://en.wikipedia.org/wiki/Moon" title="Moon">Moon</a>. It is heavily <a href="http://en.wikipedia.org/wiki/Impact_crater" title="Impact crater">cratered</a>, has no <a href="http://en.wikipedia.org/wiki/Natural_satellite" title="Natural satellite">natural satellites</a> and no substantial <a href="http://en.wikipedia.org/wiki/Celestial_body_atmosphere" class="mw-redirect" title="Celestial body atmosphere">atmosphere</a>. It has a large <a href="http://en.wikipedia.org/wiki/Iron" title="Iron">iron</a> <a href="http://en.wikipedia.org/wiki/Planetary_core" title="Planetary core">core</a>, which generates a <a href="http://en.wikipedia.org/wiki/Magnetic_field" title="Magnetic field">magnetic field</a> about 1% as strong as that of the <a href="http://en.wikipedia.org/wiki/Earth" title="Earth">Earth</a>.<sup><a href="http://en.wikipedia.org/wiki/Mercury_%28planet%29#cite_note-5">[6]</a></sup> It is an exceptionally dense planet due to the large size of its core. The surface temperatures on Mercury range from about 90 to 700 <a href="http://en.wikipedia.org/wiki/Kelvin" title="Kelvin">K</a> (−180 to 430 °C), with the <a href="http://en.wikipedia.org/wiki/Subsolar_point" title="Subsolar point">subsolar point</a> being the hottest and the bottoms of craters near the <a href="http://en.wikipedia.org/wiki/Geographical_pole" title="Geographical pole">poles</a> being the coldest.</p>
<p><a href="http://en.wikipedia.org/wiki/Mercury_%28planet%29#Ancient_astronomers">Recorded observations</a> of Mercury date back to the <a href="http://en.wikipedia.org/wiki/Sumer" title="Sumer">Sumerians</a> in the third millennium BC. Before the 4th century BC, Greek astronomers believed the planet to be two separate objects: one visible only at sunrise, which they called <a href="http://en.wikipedia.org/wiki/Apollo" title="Apollo">Apollo</a>; the other visible only at sunset, which they called <a href="http://en.wikipedia.org/wiki/Hermes" title="Hermes">Hermes</a>. The English name for the planet comes from the <a href="http://en.wikipedia.org/wiki/Ancient_Rome" title="Ancient Rome">Romans</a>, who named it after the Roman <a href="http://en.wikipedia.org/wiki/Roman_mythology" title="Roman mythology">god</a> <a href="http://en.wikipedia.org/wiki/Mercury_%28mythology%29" title="Mercury (mythology)">Mercury</a>, which they equated with the Greek <a href="http://en.wikipedia.org/wiki/Hermes" title="Hermes">Hermes</a>. The <a href="http://en.wikipedia.org/wiki/Astronomical_symbol" class="mw-redirect" title="Astronomical symbol">astronomical symbol</a> for Mercury is a stylized version of Hermes&#8217; <a href="http://en.wikipedia.org/wiki/Caduceus" title="Caduceus">caduceus</a>.</p>
<img alt="" border="0" src="http://feeds.wordpress.com/1.0/categories/meteorhalley.wordpress.com/50/" /> <img alt="" border="0" src="http://feeds.wordpress.com/1.0/tags/meteorhalley.wordpress.com/50/" /> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/gocomments/meteorhalley.wordpress.com/50/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/comments/meteorhalley.wordpress.com/50/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/godelicious/meteorhalley.wordpress.com/50/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/delicious/meteorhalley.wordpress.com/50/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/gostumble/meteorhalley.wordpress.com/50/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/stumble/meteorhalley.wordpress.com/50/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/godigg/meteorhalley.wordpress.com/50/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/digg/meteorhalley.wordpress.com/50/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/goreddit/meteorhalley.wordpress.com/50/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/reddit/meteorhalley.wordpress.com/50/" /></a> <img alt="" border="0" src="http://stats.wordpress.com/b.gif?host=meteorhalley.wordpress.com&blog=3185850&post=50&subd=meteorhalley&ref=&feed=1" /></div>]]></content:encoded>
			<wfw:commentRss>http://meteorhalley.wordpress.com/2008/04/02/mercury/feed/</wfw:commentRss>
		<slash:comments>0</slash:comments>
	
		<media:content url="http://0.gravatar.com/avatar/80d91880e5e7c91d9244aaeb122d8aef?s=96&#38;d=identicon" medium="image">
			<media:title type="html">meteorhalley</media:title>
		</media:content>

		<media:content url="http://meteorhalley.files.wordpress.com/2008/04/240px-mercury_in_color_-_prockter07.thumbnail.jpg" medium="image">
			<media:title type="html">Mercury</media:title>
		</media:content>
	</item>
		<item>
		<title>The George Evil Double Bush It</title>
		<link>http://meteorhalley.wordpress.com/2008/04/02/the-george-evil-double-bush-it/</link>
		<comments>http://meteorhalley.wordpress.com/2008/04/02/the-george-evil-double-bush-it/#comments</comments>
		<pubDate>Wed, 02 Apr 2008 12:19:13 +0000</pubDate>
		<dc:creator>meteorhalley</dc:creator>
				<category><![CDATA[Uncategorized]]></category>

		<guid isPermaLink="false">http://meteorhalley.wordpress.com/?p=48</guid>
		<description><![CDATA[US President George W Bush has urged Nato allies to send more troops to Afghanistan ahead of the alliance&#8217;s biggest-ever summit in Romania.
President Bush It set out his agenda in a pre-summit speech BULLSHIT
In a pre-summit speech in Bucharest, Mr Bush said &#8220;we cannot afford to lose Afghanistan&#8230; we must win&#8221;.
Romania and France are due [...]<img alt="" border="0" src="http://stats.wordpress.com/b.gif?host=meteorhalley.wordpress.com&blog=3185850&post=48&subd=meteorhalley&ref=&feed=1" />]]></description>
			<content:encoded><![CDATA[<div class='snap_preview'><br /><p><b>US President George W Bush has urged Nato allies to send more troops to Afghanistan ahead of the alliance&#8217;s biggest-ever summit in Romania.</b></p>
<p><a href="http://meteorhalley.files.wordpress.com/2008/04/_44532489_georgebush-ap226b.jpg" title="Evil"><img src="http://meteorhalley.files.wordpress.com/2008/04/_44532489_georgebush-ap226b.thumbnail.jpg?w=85&#038;h=101" alt="Evil" height="101" width="85" />President Bush It set out his agenda in a pre-summit speech BULLSHIT</a></p>
<p>In a pre-summit speech in Bucharest, Mr Bush said &#8220;we cannot afford to lose Afghanistan&#8230; we must win&#8221;.</p>
<p>Romania and France are due to send more troops and Mr Bush asked other nations &#8220;to step forward&#8221;.</p>
<p>He also renewed calls for Nato membership to be open to any European democracy that sought it. <!-- E SF --></p>
<p>The Nato-led force in Afghanistan currently numbers 47,000 troops from 40 nations. Commanders have called for a further 10,000 soldiers to be deployed.</p>
<p>Nato allies want the Bucharest summit, starting later on Wednesday, to send the message that it will stay in Afghanistan for as long as necessary.</p>
<img alt="" border="0" src="http://feeds.wordpress.com/1.0/categories/meteorhalley.wordpress.com/48/" /> <img alt="" border="0" src="http://feeds.wordpress.com/1.0/tags/meteorhalley.wordpress.com/48/" /> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/gocomments/meteorhalley.wordpress.com/48/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/comments/meteorhalley.wordpress.com/48/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/godelicious/meteorhalley.wordpress.com/48/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/delicious/meteorhalley.wordpress.com/48/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/gostumble/meteorhalley.wordpress.com/48/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/stumble/meteorhalley.wordpress.com/48/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/godigg/meteorhalley.wordpress.com/48/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/digg/meteorhalley.wordpress.com/48/" /></a> <a rel="nofollow" href="http://feeds.wordpress.com/1.0/goreddit/meteorhalley.wordpress.com/48/"><img alt="" border="0" src="http://feeds.wordpress.com/1.0/reddit/meteorhalley.wordpress.com/48/" /></a> <img alt="" border="0" src="http://stats.wordpress.com/b.gif?host=meteorhalley.wordpress.com&blog=3185850&post=48&subd=meteorhalley&ref=&feed=1" /></div>]]></content:encoded>
			<wfw:commentRss>http://meteorhalley.wordpress.com/2008/04/02/the-george-evil-double-bush-it/feed/</wfw:commentRss>
		<slash:comments>0</slash:comments>
	
		<media:content url="http://0.gravatar.com/avatar/80d91880e5e7c91d9244aaeb122d8aef?s=96&#38;d=identicon" medium="image">
			<media:title type="html">meteorhalley</media:title>
		</media:content>

		<media:content url="http://meteorhalley.files.wordpress.com/2008/04/_44532489_georgebush-ap226b.thumbnail.jpg" medium="image">
			<media:title type="html">Evil</media:title>
		</media:content>
	</item>
	</channel>
</rss>