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<rss version="2.0" xmlns:opensearch="http://a9.com/-/spec/opensearch/1.1/" xmlns:media="http://search.yahoo.com/mrss/"><channel><title>Views of the Solar System: Planetary Interiors: Zazzle.com Store: </title><link>http://feed.zazzle.com/z.2/api/find.aspx?cg=196084222140689264&amp;ft=rss&amp;ch=solarviews&amp;ou=%2fsolarviews%2frss%3fcg%3d196084222140689264</link><description></description><language>en-us</language><pubDate>Fri, 24 May 2013 19:31:17 GMT</pubDate><ttl>60</ttl><opensearch:totalResults>5</opensearch:totalResults><opensearch:startIndex>1</opensearch:startIndex><opensearch:itemsPerPage>60</opensearch:itemsPerPage><opensearch:Query role="request" searchTerms="" />
<item><guid isPermaLink="false">http://www.zazzle.com/interior_of_jupiter_poster-228777464954418660</guid><pubDate>Sun, 13 Nov 2005 01:39:57 GMT</pubDate><title><![CDATA[Interior of Jupiter Poster]]></title><link>http://www.zazzle.com/interior_of_jupiter_poster-228777464954418660</link><author>solarviews</author><description><![CDATA[



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</div>]]></description><price>$21.65</price><media:title><![CDATA[Interior of Jupiter]]></media:title><media:description><![CDATA[This picture illustrates the internal structure of Jupiter. The
outer layer is primarily composed of molecular hydrogen. At
greater depths the hydrogen starts resembling a liquid.
At 10,000 kilometers
below Jupiter&#39;s cloud top liquid hydrogen reaches a pressure
of 1,000,000 bar with a temperature of 6,000&#176; K. At this
state hydrogen changes into a phase of liquid metallic
hydrogen. In this state, the hydrogen atoms break down yeilding
ionized protons and electrons similar to the Sun&#39;s interior.
Below this is a layer dominated by ice where &quot;ice&quot; denotes a soupy
liquid mixture of water, methane, and ammonia under high temperatures
and pressures. Finally at the center is a rocky or rocky-ice core
of up to 10 Earth masses.]]></media:description><media:price>$21.65</media:price><media:thumbnail url="http://rlv.zcache.com/interior_of_jupiter_poster-r95b404de2c424caabdd22fc4b6e4382e_cus_8byvr_152.jpg" /><media:content url="http://rlv.zcache.com/interior_of_jupiter_poster-r95b404de2c424caabdd22fc4b6e4382e_cus_8byvr_500.jpg" /><media:keywords><![CDATA[jupiter, internal, structure, cut-away, planet, solar, system, interior]]></media:keywords><media:rating scheme="urn:mpaa">g</media:rating></item>

<item><guid isPermaLink="false">http://www.zazzle.com/the_interior_of_mars_posters-228990433044253261</guid><pubDate>Sat, 12 Nov 2005 18:16:04 GMT</pubDate><title><![CDATA[The Interior of Mars Posters]]></title><link>http://www.zazzle.com/the_interior_of_mars_posters-228990433044253261</link><author>solarviews</author><description><![CDATA[



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</div>]]></description><price>$21.65</price><media:title><![CDATA[The Interior of Mars]]></media:title><media:description><![CDATA[The current understanding of the interior of Mars suggests that it
can be modeled with a thin crust, similar to Earth&#39;s, a mantle and a core.
Using four parameters, the Martian core size and mass can be determined.
However, only three out of the four are known and include the total mass,
size of Mars, and the moment of inertia. Mass and size was determined accurately
from early missions. The moment of inertia was determined from
Viking lander and Pathfinder Doppler data, by measuring the
precession rate of Mars. The fourth parameter, needed to complete the
interior model, will be obtained from future spacecraft missions.
With the three known parameters, the model is significantly
constrained. If the Martian core is dense (composed of iron) similar
to Earth&#39;s or SNC meteorites thought to originate from Mars, then
the minimum core radius would be about 1300 kilometers. If the
core is made out of less-dense material such as a mixture of sulfur
and iron, the maximum radius would probably be less than 2000 kilometers.]]></media:description><media:price>$21.65</media:price><media:thumbnail url="http://rlv.zcache.com/the_interior_of_mars_posters-r3f3cc251fe8744eba26549b8e0329206_cus_8byvr_152.jpg" /><media:content url="http://rlv.zcache.com/the_interior_of_mars_posters-r3f3cc251fe8744eba26549b8e0329206_cus_8byvr_500.jpg" /><media:keywords><![CDATA[mars, solar, system, interior, structure, planet, cut-away]]></media:keywords><media:rating scheme="urn:mpaa">g</media:rating></item>

<item><guid isPermaLink="false">http://www.zazzle.com/the_interior_of_the_earth_posters-228246424799982418</guid><pubDate>Sat, 12 Nov 2005 18:05:59 GMT</pubDate><title><![CDATA[The Interior of the Earth Posters]]></title><link>http://www.zazzle.com/the_interior_of_the_earth_posters-228246424799982418</link><author>solarviews</author><description><![CDATA[



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</div>]]></description><price>$21.65</price><media:title><![CDATA[The Interior of the Earth]]></media:title><media:description><![CDATA[Seismic data of the Earth has led to a model of the interior that
partitions it into a core, mantle, and crust. The crust
is approximately 30 kilometers thick. The mantle is approximately
2,840 kilometers thick, and the core radius is approximately 3,500
kilometers thick. Each partition can be further divided into smaller
regions. The crust can be classified as oceanic or continental,
the mantle as upper and lower, and the core as outer liquid
and inner solid.
&lt;P&gt;
Pictured in this cutaway view of the Earth is the crust, mantle,
liquid outer core, and solid inner core.]]></media:description><media:price>$21.65</media:price><media:thumbnail url="http://rlv.zcache.com/the_interior_of_the_earth_posters-r8e4ab109b53a4b269b97a08b15b56449_cus_8byvr_152.jpg" /><media:content url="http://rlv.zcache.com/the_interior_of_the_earth_posters-r8e4ab109b53a4b269b97a08b15b56449_cus_8byvr_500.jpg" /><media:keywords><![CDATA[earth, interior, cut-away, solar, system, planet, internal, structure]]></media:keywords><media:rating scheme="urn:mpaa">g</media:rating></item>

<item><guid isPermaLink="false">http://www.zazzle.com/the_interior_of_venus_print-228434940684334496</guid><pubDate>Sat, 12 Nov 2005 16:09:35 GMT</pubDate><title><![CDATA[The Interior of Venus Print]]></title><link>http://www.zazzle.com/the_interior_of_venus_print-228434940684334496</link><author>solarviews</author><description><![CDATA[



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</div>]]></description><price>$21.50</price><media:title><![CDATA[The Interior of Venus]]></media:title><media:description><![CDATA[This picture shows a cutaway view of the possible internal
structure of Venus. The image was created from Mariner 10
images used for the outer atmospheric layer. The surface
was taken from Magellan radar images. The interior
characteristics of Venus are inferred from gravity field
and magnetic field measurements by Magellan and prior
spacecraft. The crust is shown as adark red, the mantle as
a lighter orange-red, and the core yellow.
&lt;p&gt;
What is known about the Venusian interior comes primarily from 
the Venera, Pioneer Venus and Magellan spacecraft. Before these
explorers, scientists thought that Venus would have
tectonic processes similar to that of Earth&#39;s mantle convection.
Venus and Earth are both similar in size and presumable the
same composition. However, Venus showed no sign of plate tectonism,
and appears to have a single plate which makes it very different
from Earth.]]></media:description><media:price>$21.50</media:price><media:thumbnail url="http://rlv.zcache.com/the_interior_of_venus_print-r4bad3781fd774e08b4daadfc1a841c96_z6m_8byvr_152.jpg" /><media:content url="http://rlv.zcache.com/the_interior_of_venus_print-r4bad3781fd774e08b4daadfc1a841c96_z6m_8byvr_500.jpg" /><media:keywords><![CDATA[venus, interior, internal, structure, solar, system, planet]]></media:keywords><media:rating scheme="urn:mpaa">g</media:rating></item>

<item><guid isPermaLink="false">http://www.zazzle.com/interior_of_mercury_posters-228457731421940152</guid><pubDate>Sat, 12 Nov 2005 13:58:04 GMT</pubDate><title><![CDATA[Interior of Mercury Posters]]></title><link>http://www.zazzle.com/interior_of_mercury_posters-228457731421940152</link><author>solarviews</author><description><![CDATA[



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</div>]]></description><price>$21.50</price><media:title><![CDATA[Interior of Mercury]]></media:title><media:description><![CDATA[Most of what is known about the internal structure of Mercury comes from
data acquired by the Mariner 10 spacecraft that flew past the planet
in 1973 and 1974. Mercury is about a third of the size of Earth, yet
its density is comparable to that of Earth. This indicates that Mercury
has a large core roughly the size of Earth&#39;s moon or about 75% of
the planet&#39;s radius. The core is likely composed of 60 to 70% iron
by mass.
Mariner 10&#39;s measurements of the planet reveals a dipolar magnetic field
possibly produced by a partially molten core.
A solid rocky mantle surrounds the core with a thin crust of about 100
kilometers.]]></media:description><media:price>$21.50</media:price><media:thumbnail url="http://rlv.zcache.com/interior_of_mercury_posters-r2215e80f355242e68fe89d12f3313229_z6m_8byvr_152.jpg" /><media:content url="http://rlv.zcache.com/interior_of_mercury_posters-r2215e80f355242e68fe89d12f3313229_z6m_8byvr_500.jpg" /><media:keywords><![CDATA[mercury, interior, internal, structure, solar, system]]></media:keywords><media:rating scheme="urn:mpaa">g</media:rating></item>
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