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    <title>USGS Astrogeology Hot Topics - Hubble</title>
    <link>http://astrogeology.usgs.gov/HotTopics/</link>
    <description>USGS Astrogeology news, features, and updates</description>
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<pubDate>Tue, 09 Jan 2007 00:30:46 GMT</pubDate>

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        <title>RSS: USGS Astrogeology Hot Topics - Hubble - USGS Astrogeology news, features, and updates</title>
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<item>
    <title>Hubble Captures a Rare Eclipse on Uranus</title>
    <link>http://astrogeology.usgs.gov/HotTopics/index.php?/archives/207-Hubble-Captures-a-Rare-Eclipse-on-Uranus.html</link>
            <category>Hubble</category>
    
    <comments>http://astrogeology.usgs.gov/HotTopics/index.php?/archives/207-Hubble-Captures-a-Rare-Eclipse-on-Uranus.html#comments</comments>
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    <author>nospam@example.com (HotTopicsJournalist)</author>
    <content:encoded>
    
&lt;h3&gt;&lt;font color=&quot;#0080ff&quot;&gt;&lt;/font&gt;&lt;/h3&gt;&lt;p&gt;&lt;a href=&quot;http://www.seti.org/atf/cf/{B0D4BC0E-D59B-4CD0-9E79-113953A58644}/uranus%20eclipse_lg.jpg&quot;&gt;&lt;img border=&quot;0&quot; src=&quot;http://www.seti.org/atf/cf/{B0D4BC0E-D59B-4CD0-9E79-113953A58644}/uranus%20eclipse_sm.jpg&quot; alt=&quot;Uranus Eclipse&quot;/&gt;&lt;/a&gt;&lt;br /&gt;Arial traverses Uranus&lt;br/&gt;&lt;font size=&quot;1&quot;&gt;click for larger image&lt;/font&gt;&lt;/p&gt;&lt;p&gt;This NASA Hubble Space Telescope image is a never-before-seen astronomical alignment of a moon traversing the face of Uranus, and its accompanying shadow. The white dot near the center of Uranus blue-green disk is the icy moon Ariel. The 700-mile-diameter satellite is casting a shadow onto the cloud tops of Uranus. To an observer on Uranus, this would appear as a solar eclipse, where the moon briefly blocks out the Sun as its shadow races across Uranuss cloud tops. Though such &amp;quot;transits&amp;quot; by moons across the disks of their parents are commonplace for some other gas giant planets, such as Jupiter, the satellites of Uranus orbit the planet in such a way that they rarely cast shadows on the planet&#039;s surface. Uranus is tilted so that its spin axis lies nearly in its orbital plane. The planet is essentially tipped over on its side. The moons of Uranus orbit the planet above the equator, so their paths align edge-on to the Sun only every 42 years. This color composite image was created from images at three wavelengths in near infrared light obtained with Hubbles Advanced Camera for Surveys on July 26, 2006.  &lt;a href=&quot;http://www.seti.org/rages&quot;&gt;Dr. Kathy Rages&lt;/a&gt;, of the SETI Institute, made the identification of the bright spot as Ariel.&lt;/p&gt;&lt;p class=&quot;credit&quot;&gt;&lt;span class=&quot;import&quot;&gt;Credit:&lt;/span&gt; &lt;a href=&quot;http://www.nasa.gov/&quot;&gt;NASA&lt;/a&gt;, &lt;a href=&quot;http://www.spacetelescope.org/&quot;&gt;ESA&lt;/a&gt;, L. Sromovsky (University of Wisconsin, Madison), H. Hammel (Space Science Institute), and K. Rages (SETI)&lt;/p&gt; 
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    <pubDate>Tue, 12 Sep 2006 16:46:22 -0700</pubDate>
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<item>
    <title>Orion's Inner Beauty</title>
    <link>http://astrogeology.usgs.gov/HotTopics/index.php?/archives/198-Orions-Inner-Beauty.html</link>
            <category>Hubble</category>
    
    <comments>http://astrogeology.usgs.gov/HotTopics/index.php?/archives/198-Orions-Inner-Beauty.html#comments</comments>
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    <author>nospam@example.com (HotTopicsJournalist)</author>
    <content:encoded>
    &lt;p /&gt;&lt;div class=&quot;serendipity_imageComment_center&quot; style=&quot;width: 360px;&quot;&gt;&lt;div class=&quot;serendipity_imageComment_img&quot;&gt;&lt;img width=&quot;360&quot; hspace=&quot;5&quot; height=&quot;450&quot; border=&quot;0&quot; align=&quot;left&quot; src=&quot;http://astrogeology.usgs.gov/HotTopics/uploads/STAR.jpg&quot; alt=&quot;Sword of Orion&quot; /&gt;&lt;/div&gt;&lt;div align=&quot;center&quot; class=&quot;serendipity_imageComment_txt&quot;&gt;360X450&lt;/div&gt;&lt;/div&gt;&lt;p&gt;This infrared image from NASA&#039;s Spitzer Space Telescope shows the Orion nebula, our closest massive star-making factory, 1,450 light-years from Earth. The nebula is close enough to appear to the naked eye as a fuzzy star in the sword of the popular hunter constellation. &lt;/p&gt;&lt;p&gt;The nebula itself is located on the lower half of the image, surrounded by a ring of dust. It formed in a cold cloud of gas and dust and contains about 1,000 young stars. These stars illuminate the cloud, creating the beautiful nebulosity, or swirls of material, seen here in infrared. &lt;/p&gt;&lt;p&gt;This image shows infrared light captured by Spitzer&#039;s infrared array camera. Light with wavelengths of 8 and 5.8 microns (red and orange) comes mainly from dust that has been heated by starlight. Light of 4.5 microns (green) shows hot gas and dust; and light of 3.6 microns (blue) is from starlight. &lt;/p&gt;&lt;p&gt;&lt;a href=&quot;http://www.spitzer.caltech.edu/Media/releases/ssc2006-16/ssc2006-16a.shtml?msource=09906&amp;tr=y&amp;auid=1880045&quot;&gt;Take a look or download Orion&#039;s Portrait at medium or high resolution.&lt;/a&gt;&lt;/p&gt;&lt;p&gt;Credit: NASA-Spitzer Space Telescope &lt;/p&gt;&lt;p /&gt; 
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    <pubDate>Tue, 15 Aug 2006 09:49:53 -0700</pubDate>
    <guid isPermaLink="false">http://astrogeology.usgs.gov/HotTopics/index.php?/archives/198-guid.html</guid>
    
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<item>
    <title>New Discoveries at Uranus</title>
    <link>http://astrogeology.usgs.gov/HotTopics/index.php?/archives/106-New-Discoveries-at-Uranus.html</link>
            <category>Hubble</category>
    
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    <author>nospam@example.com (HotTopicsJournalist)</author>
    <content:encoded>
    &lt;div class=&quot;serendipity_imageComment_right&quot; style=&quot;width: 200px;&quot;&gt;&lt;div class=&quot;serendipity_imageComment_img&quot;&gt;&lt;a href=&quot;http://astrogeology.usgs.gov/HotTopics/uploads/Astronomy/uranus20labeled20large.jpg&quot;&gt;&lt;img width=&quot;200&quot; hspace=&quot;5&quot; height=&quot;160&quot; border=&quot;0&quot; align=&quot;right&quot; src=&quot;http://astrogeology.usgs.gov/HotTopics/uploads/Astronomy/uranus20labeled20large.th.jpg&quot; alt=&quot;Fully-labeled composite image&quot;/&gt;&lt;/a&gt;&lt;/div&gt;&lt;div class=&quot;serendipity_imageComment_txt&quot;&gt;Fully-labeled composite image
&lt;br /&gt;&lt;br /&gt;&lt;span style=&quot;font-style: italic;&quot;&gt;Credit: NASA, ESA, and M. Showalter (SETI Institute)
&lt;/span&gt;&lt;br /&gt;&lt;br /&gt;&lt;span style=&quot;font-style: italic;&quot;&gt;800x640&lt;/span&gt;&lt;/div&gt;&lt;/div&gt; 
Deep exposure of Uranus taken with the Hubble Space Telescope reveal
two small moons and two faint rings.  All orbit outside of Uranus&#039;s
previously known (main) ring system, but interior to the large,
classical moons.  The outer new moon, U XXVI Mab, orbits at roughly
twice the radius of the main rings and shares its orbit with a dust
ring.  The second moon, U XXVII Cupid, orbits just interior to the
satellite Belinda.  A second ring falls between the orbits of Portia
and Rosalind, in a region with no known source bodies.  Collectively,
these constitute a densely-packed, rapidly varying and possibly
unstable dynamical system.&lt;br /&gt;&lt;br /&gt;&lt;a href=&quot;http://www.seti.org/site/pp.asp?c=ktJ2J9MMIsE&amp;b=1313191&quot;&gt;&lt;span style=&quot;font-weight: bold;&quot;&gt;More: SETI &lt;/span&gt;- New Discoveries at Uranus&lt;/a&gt;&lt;br /&gt;
     
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    <pubDate>Fri, 06 Jan 2006 12:00:00 -0700</pubDate>
    <guid isPermaLink="false">http://astrogeology.usgs.gov/HotTopics/index.php?/archives/106-guid.html</guid>
    
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<item>
    <title>Hubble Prospects For Resources on The Moon</title>
    <link>http://astrogeology.usgs.gov/HotTopics/index.php?/archives/103-Hubble-Prospects-For-Resources-on-The-Moon.html</link>
            <category>Hubble</category>
    
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    <author>nospam@example.com (BlogAdmin)</author>
    <content:encoded>
    &lt;div style=&quot;width: 200px;&quot; class=&quot;serendipity_imageComment_right&quot;&gt;&lt;div class=&quot;serendipity_imageComment_img&quot;&gt;&lt;img width=&quot;200&quot; hspace=&quot;5&quot; height=&quot;158&quot; border=&quot;0&quot; align=&quot;right&quot; src=&quot;http://astrogeology.usgs.gov/HotTopics/uploads/Astronomy/136335main_image3_lg.th.jpg&quot; alt=&quot;Apollo 17 Landing Site&quot; /&gt;&lt;/div&gt;&lt;div class=&quot;serendipity_imageComment_txt&quot;&gt;Apollo 17 Landing Site, HST and Apollo mission images. &lt;span style=&quot;font-style: italic;&quot;&gt;NASA/ESA/HST Moon Team&lt;/span&gt;&lt;/div&gt;&lt;/div&gt; Although U.S. astronauts have visited the moon before, they only spent
a few days there, making short forays into the barren landscape. A new &lt;a href=&quot;javascript:openNASAWindow(&#039;http://www.nasa.gov/missions/solarsystem/explore_main.html&#039;)&quot;&gt;Vison for Space Exploration&lt;/a&gt;,
announced by President George W. Bush in January 2004, calls for the
establishment of human outposts on the moon and later, human
exploration of Mars. This time, we&#039;re going back to stay. &lt;br /&gt;&lt;br /&gt;To prepare for potential manned missions to the Earth&#039;s Moon, NASA scientists are using the Hubble Space Telescope to
hunt for resources, such as oxygen, that are essential for people to
survive and to sustain their existence on the lunar surface. Hubble&#039;s
preliminary observations and results are promising. A preliminary assessment of the Hubble observations pinpoints possible
locations of ilmenite, a titanium oxide rich in oxygen, at the Apollo
17 landing region. Ilmenite is a potentially key resource because it
contains easily extracted oxygen, which can be used for breathing and
for rocket fuel. Since the moon doesn&#039;t have an atmosphere, scientists
must hunt for oxygen in lunar soils if we are to learn to live off the
land.&lt;br /&gt;&lt;br /&gt;&lt;a href=&quot;http://www.nasa.gov/vision/universe/solarsystem/hubble_moon.html&quot;&gt;&lt;span style=&quot;font-weight: bold;&quot;&gt;More: NASA&lt;/span&gt; - Hubble Prospects For Resources on The Moon&lt;/a&gt;&lt;br /&gt;&lt;br /&gt;&lt;br /&gt;
   
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    <pubDate>Sat, 12 Nov 2005 14:25:01 -0700</pubDate>
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<item>
    <title>Hubble Spots Possible New Moons Around Pluto</title>
    <link>http://astrogeology.usgs.gov/HotTopics/index.php?/archives/102-Hubble-Spots-Possible-New-Moons-Around-Pluto.html</link>
            <category>Hubble</category>
    
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    <author>nospam@example.com (BlogAdmin)</author>
    <content:encoded>
    &lt;div class=&quot;serendipity_imageComment_left&quot; style=&quot;width: 200px;&quot;&gt;&lt;div class=&quot;serendipity_imageComment_img&quot;&gt;&lt;a href=&quot;http://astrogeology.usgs.gov/HotTopics/uploads/Astronomy/137121main1_hst_pluto2_516.jpg&quot;&gt;&lt;img width=&quot;200&quot; hspace=&quot;5&quot; height=&quot;150&quot; border=&quot;0&quot; alt=&quot;HST images showing two new candidate satellites orbiting around Pluto&quot; align=&quot;left&quot; src=&quot;http://astrogeology.usgs.gov/HotTopics/uploads/Astronomy/137121main1_hst_pluto2_516.th.jpg&quot; /&gt;&lt;/a&gt;&lt;/div&gt;&lt;div class=&quot;serendipity_imageComment_txt&quot;&gt;HST images showing two new candidate satellites orbiting around Pluto&lt;/div&gt;&lt;/div&gt; The Hubble Space Telescope images shown left, taken by the Advanced
Camera for Surveys, reveal Pluto, its large moon Charon, and
the planet&#039;s two new candidate satellites. Between May 15 and
May 18, 2005, Charon, and the potential moons, provisionally
designated P1 and P2, all appear to rotate counterclockwise
around Pluto.  P1 and P2 move less than Charon because
they are farther from Pluto, and therefore would be orbiting
at slower speeds. P1 and P2 are thousands of times less bright
than Pluto and Charon. The enhanced-color images of Pluto (the
brightest object) and Charon (to the right of Pluto) were
constructed by combining short exposure images.  The images of the new satellites were made
from longer exposures. &lt;br /&gt;&lt;br /&gt;&lt;a href=&quot;http://www.nasa.gov/vision/universe/solarsystem/hubble_pluto.html&quot;&gt;&lt;span style=&quot;font-weight: bold;&quot;&gt;More: NASA&lt;/span&gt; - &lt;span class=&quot;bold&quot;&gt;Hubble Spots Possible New Moons Around Pluto&lt;/span&gt;&lt;/a&gt;    - view more images and get the full story on this exciting discovery!&lt;br /&gt;&lt;br /&gt;&lt;br /&gt;
  
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    <pubDate>Sat, 12 Nov 2005 14:18:03 -0700</pubDate>
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    <title>Hubble's Eye on Mars</title>
    <link>http://astrogeology.usgs.gov/HotTopics/index.php?/archives/31-Hubbles-Eye-on-Mars.html</link>
            <category>Hubble</category>
    
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    <author>nospam@example.com (HotTopics)</author>
    <content:encoded>
    &lt;div class=&quot;serendipity_imageComment_left&quot; style=&quot;width: 200px;&quot;&gt;&lt;div class=&quot;serendipity_imageComment_img&quot;&gt;&lt;a href=&quot;http://astrogeology.usgs.gov/HotTopics/uploads/Other/49599main_Mars_close.jpg&quot;&gt;&lt;img width=&quot;200&quot; hspace=&quot;5&quot; height=&quot;200&quot; border=&quot;0&quot; align=&quot;left&quot; alt=&quot;NASA&#039;s Hubble Space Telescope snapshot of Mars&quot; src=&quot;http://astrogeology.usgs.gov/HotTopics/uploads/Other/49599main_Mars_close.th.jpg&quot; /&gt;&lt;/a&gt;&lt;/div&gt;&lt;div class=&quot;serendipity_imageComment_txt&quot;&gt;&lt;span style=&quot;font-weight: bold;&quot;&gt;NASA&#039;s Hubble Space Telescope snapshot of Mars&lt;/span&gt;

&lt;p&gt;
NASA&#039;s Hubble Space Telescope took this snapshot of Mars 11 hours before the planet made its closest approach to Earth. The two planets are 34,648,840 miles (55,760,220 km) apart. This image was made from a series of exposures taken between 6:20 p.m. and 7:12 p.m. EDT Aug. 26 with Hubble&#039;s Wide Field and Planetary Camera 2.
&lt;/p&gt;
&lt;p&gt;&lt;span style=&quot;font-style: italic;&quot;&gt;
Photo credit: NASA/J. Bell (Cornell U.) and M. Wolff (SSI)&lt;/span&gt;
&lt;/p&gt;
&lt;p&gt;
330 x 330, 32 KB
&lt;/p&gt;&lt;p /&gt;&lt;/div&gt;&lt;/div&gt; NASA&#039;s Hubble Space Telescope made observations of the planet Mars on
August 26 and 27, when Earth and Mars were closer together than they
have been in the last 60,000 years. As Hubble&#039;s high-resolution images
of the Red Planet are received at the Space Telescope Science Institute
and are digitally processed by the Mars observing team, they will be
released to the public and news media via the Internet. The Hubble
images are the sharpest views of Mars ever taken from Earth. They
reveal surface details as small as 17 miles (24 km) across. Though
NASA&#039;s Mars-orbiting spacecraft can photograph the Red Planet in much
finer detail, Hubble routinely serves as a &amp;quot;weather satellite&amp;quot; for
tracking atmospheric changes on Mars and for probing its geology on a
global scale.&lt;br /&gt;&lt;br /&gt;&lt;p&gt;
&lt;a href=&quot;http://www.nasa.gov/vision/universe/watchtheskies/HST_Mars_Photos.html&quot;&gt;&lt;strong&gt;
                              More: NASA&lt;/strong&gt; -
                              Hubble Space Telescope&#039;s Viewing Plans For Earth&#039;s &#039;Close Encounter&#039; With Mars&lt;/a&gt;
&lt;/p&gt;
&lt;p&gt;
&lt;a href=&quot;http://skyandtelescope.com/printable/observing/objects/planets/article_988.asp&quot;&gt;&lt;strong&gt;
                              Link: Sky &amp;amp; Telescope&lt;/strong&gt; -
                              Mars at Its All-Time Finest&lt;/a&gt;
&lt;br clear=&quot;all&quot; /&gt;&lt;/p&gt;
   
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    <pubDate>Wed, 27 Aug 2003 12:00:00 -0700</pubDate>
    <guid isPermaLink="false">http://astrogeology.usgs.gov/HotTopics/index.php?/archives/31-guid.html</guid>
    
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<item>
    <title>A Cold New World</title>
    <link>http://astrogeology.usgs.gov/HotTopics/index.php?/archives/53-A-Cold-New-World.html</link>
            <category>Hubble</category>
    
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    <author>nospam@example.com (HotTopics)</author>
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    NASA&#039;s Hubble Space Telescope measured the largest object in the
solar system seen since the discovery of Pluto 72 years ago. The icy
world 2002 LM60, dubbed &amp;quot;Quaoar&amp;quot; by its discoverers, measures 1300
kilometers wide - approximately half the size of Pluto. Just a curious
point of light until recently, Quaoar lies a billion kilometers beyond
Pluto.&lt;br /&gt;&lt;br /&gt; 
&lt;p&gt;
&lt;a href=&quot;http://science.nasa.gov/headlines/y2002/07oct_newworld.htm&quot;&gt;&lt;strong&gt;
                              More: Science@NASA&lt;/strong&gt; -
                              A Cold New World&lt;/a&gt;&lt;br /&gt;&lt;br /&gt;
&lt;/p&gt;
  
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    <pubDate>Tue, 08 Oct 2002 12:00:00 -0700</pubDate>
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