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    <title>Astronomy Picture of the Day RSS Feed</title>
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    <description>
	<![CDATA[
	<p>
	The
	<a href="http://apod.nasa.gov/apod/">Astronomy Picture of the Day</a>
	is a wonderful web site that puts up a different astronomy-related
	picture every day.
	However, the site does not have an RSS feed.
	This page fixes that deficiency.
	]]>
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    <language>en-us</language>
    <lastBuildDate>Wed, 12 Aug 2026 13:06:00 GMT</lastBuildDate>
    <generator>ACME Labs custom shell script</generator>
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	<title>Astronomy Picture of the Day RSS Feed</title>
	<link>http://www.acme.com/jef/apod/</link>
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    <item>
	<title><![CDATA[Perseids Over a Little Planet]]></title>
	<link>http://apod.nasa.gov/apod/ap260812.html</link>
	<pubDate>Wed, 12 Aug 2026 13:06:00 GMT</pubDate>
	<description>
	    <![CDATA[
	    <a href="http://apod.nasa.gov/apod/ap260812.html"><img src="https://apod.nasa.gov/apod/image/2608/A_Planet_of_Meteors_1024.jpg" /></a>
<title>Perseids Over a Little Planet</title>
    

    It looks like a view from the <a href="https://en.wikipedia.org/wiki/The_Little_Prince">Little Prince</a>'s planet.

    The <a href="https://www.instagram.com/p/DFQUjv5sEVU/">featured image</a> is a throwback to the <a href="https://apod.nasa.gov/apod/ap250812.html">2024 Perseid meteor shower</a>, surrounded in this <a href="https://paulbourke.net/panorama/littleplanet/">projection</a> by the <a href="https://www.youtube.com/watch?v=marHFTga9r8">Bieszczady Mountains</a> in <a href="https://en.wikipedia.org/wiki/Poland">Poland</a>.

    Visible in the sky is the arch of the <a href="https://imagine.gsfc.nasa.gov/science/objects/milkyway1.html">Milky Way</a>, along with several <a href="https://science.nasa.gov/universe/stories/quick-reads/decoding-nebulae/">nebulas</a> in red and over a hundred meteors pointing to the <a href="https://en.wikipedia.org/wiki/Radiant_(meteor_shower)">radiant</a>.
    
    The Perseids are <a href="https://www.planetary.org/articles/your-guide-meteor-shower">easily visible</a> and quite popular in the Northern Hemisphere summer. (Watching meteor showers in the winter is less convenient for a <a href="https://images.unsplash.com/photo-1433162653888-a571db5ccccf">good reason</a>).
    
    This year they are expected to offer an even more dazzling spectacle than usual, because the <a href="https://earthsky.org/astronomy-essentials/everything-you-need-to-know-perseid-meteor-shower/">peak</a> coincides with a <a href="https://apod.nasa.gov/apod/ap221001.html">new moon</a>.

    The 2026 Perseid meteor shower will peak tonight with as many as <a href="https://www.nasa.gov/blogs/watch-the-skies/2026/08/05/summer-star-shower-watch-the-perseids-with-nasa/">50-100 meteors per hour</a>, when the Earth's path crosses through debris left behind by <a href="https://science.nasa.gov/solar-system/comets/109p-swift-tuttle/">Comet Swift-Tuttle</a>.

    Typically, the <a href="https://science.nasa.gov/solar-system/meteors-meteorites/perseids/">best times</a> for seeing the meteors are between midnight and pre-dawn.

    You won't need binoculars to <a href="https://mcdonaldobservatory.org/meteor-showers/">see the meteors</a>, but a lawn chair and a dark sky location help.

    
	    ]]>
	</description>
    </item>

    <item>
	<title><![CDATA[ APOD: 2026 August 11 – Six Moons of Saturn]]></title>
	<link>http://apod.nasa.gov/apod/ap260811.html</link>
	<pubDate>Tue, 11 Aug 2026 13:06:00 GMT</pubDate>
	<description>
	    <![CDATA[
	    <a href="http://apod.nasa.gov/apod/ap260811.html"><img src="https://apod.nasa.gov/apod/image/2608/2026-08-05-0609_7-SaturnSystem_c.jpg" /></a>
<title> APOD: 2026 August 11 – Six Moons of Saturn</title>

<a href="https://en.wikipedia.org/wiki/Moons_of_Saturn">How many moons does Saturn have?</a>

While the total will likely continue to grow,
as of June 2026 the ringed gas giant had
293 confirmed moons.

That's easily more
<a href="http://ssd.jpl.nasa.gov/?sat_discovery">than any other planet</a>
of the Solar System, including ruling gas giant
Jupiter with a mere 115 confirmed moons.

Most of Saturn's known moons are small, irregular satellites.

Many are only few kilometers to a fraction of a kilometer across and
<a href="https://en.wikipedia.org/wiki/Moons_of_Saturn#Irregular_moons">grouped in</a>
tilted outer orbits.

Six of its largest satellites can be seen here, though,
in this sharp telescopic
<a href="https://app.astrobin.com/i/ztmhhp">Saturnian family portrait</a>
taken on August 5.

Larger than Earth's Moon and even slightly larger than
inner planet Mercury,
<a href="http://solarsystem.nasa.gov/planets/profile.cfm?Object=Sat_Titan">Titan</a>,
with a diameter of 5,150 kilometers, is at lower right.

You can also spot icy major moons
<a href="https://apod.nasa.gov/apod/ap100511.html">Mimas</a>,
<a href="https://apod.nasa.gov/apod/ap091208.html">Tethys</a>,
<a href="https://apod.nasa.gov/apod/ap120208.html">Enceladus</a>,
<a href="https://apod.nasa.gov/apod/ap070801.html">Dione</a>, and
<a href="https://apod.nasa.gov/apod/ap080513.html">Rhea</a> in the frame.

Saturn's first known natural satellite, Titan was
<a href="https://apod.nasa.gov/apod/ap050325.html">discovered in 1655</a> by
Dutch astronomer Christiaan Huygens.

During the space age Voyager and
<a href="https://science.nasa.gov/mission/cassini/science/moons/">Cassini discoveries</a>
have added to the
<a href="https://ui.adsabs.harvard.edu/abs/2025PSJ.....6..283A/abstract">swelling ranks</a>
of Saturnian moons.

	    ]]>
	</description>
    </item>

    <item>
	<title><![CDATA[ APOD: 2026 August 10 – Three Galaxy Pairs  ]]></title>
	<link>http://apod.nasa.gov/apod/ap260810.html</link>
	<pubDate>Mon, 10 Aug 2026 13:06:00 GMT</pubDate>
	<description>
	    <![CDATA[
	    <a href="http://apod.nasa.gov/apod/ap260810.html"><img src="https://apod.nasa.gov/apod/image/2608/Three3GalaxyPairs_Sampaio_960.jpg" /></a>
<title> APOD: 2026 August 10 – Three Galaxy Pairs  </title>
Each of these pairs of galaxies is different. 

The two 
<a href="https://science.nasa.gov/universe/galaxies/"
>galaxies</a> at the top are likely 
<a href="https://c8.alamy.com/comp/2BC0K5D/two-cats-sitting-in-safe-social-distance-separated-by-an-open-drainage-channel-in-the-street-with-natural-stone-paving-in-a-greek-village-cyclades-2BC0K5D.jpg"
>not interacting</a>, at least presently. 

However, the top galaxy with the blue stripe, 
<a href="https://apod.nasa.gov/apod/ap990510.html"
>NGC 4650A</a>, is a 
<a href="https://en.wikipedia.org/wiki/Polar-ring_galaxy"
>polar ring galaxy</a> and may be the result of a past 
<a href="https://apod.nasa.gov/apod/ap130514.html"
>galaxy collision</a>.

The two galaxies in the middle of the 
<a href="https://www.instagram.com/p/DZIts5qua6c/"
>featured image</a> appear like they could be 
<a href="https://en.wikipedia.org/wiki/Tidal_force"
>interacting gravitationally</a> -- but their 
<a href="https://ui.adsabs.harvard.edu/abs/1993A%26AS..100...47G/abstract"
>relative speeds</a> make this unlikely. 

Of these two, the larger galaxy, 
<a href="https://de.wikipedia.org/wiki/NGC_4650"
>NGC 4650</a>, is a 
<a href="https://science.nasa.gov/universe/galaxies/types/"
>spiral galaxy</a> with a 
<a href="https://apod.nasa.gov/apod/ap260517.html"
>bright bar of stars</a> across its center. 

The two galaxies at the bottom are 
<a href="https://encrypted-tbn0.gstatic.com/images?q=tbn:ANd9GcQ1gT_9ubUKcbFl8gNYAM1qF3muKpNh0HFlE9rl1cLFC-dJH1jh-WTH-aE&s=10"
>actively interacting</a>. 

Possibly in a billion years or so, NGC 4622A and NGC 4622B will 
<a href="https://apod.nasa.gov/apod/ap220606.html"
>merge</a> and become one single galaxy.

All of these galaxies are likely members of the larger 
<a href="https://en.wikipedia.org/wiki/Centaurus_Cluster"
>Centaurus Galaxy Cluster</a>. 


	    ]]>
	</description>
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    <item>
	<title><![CDATA[ APOD: 2026 August 9 – Contemplating the Sun ]]></title>
	<link>http://apod.nasa.gov/apod/ap260809.html</link>
	<pubDate>Sun, 09 Aug 2026 13:06:00 GMT</pubDate>
	<description>
	    <![CDATA[
	    <a href="http://apod.nasa.gov/apod/ap260809.html"><img src="https://apod.nasa.gov/apod/image/2608/sunsilhouettes_gilbert_960.jpg" /></a>
<title> APOD: 2026 August 9 – Contemplating the Sun </title>
Have you contemplated your home star recently? 

Featured here, a 
<a href="https://science.nasa.gov/sun/"
>Sun</a> partially eclipsed on the top left by the Moon 
is also seen eclipsed by 
<a href="https://apod.nasa.gov/apod/ap190818.html"
>earthlings</a> contemplating the eclipse below. 

This 
<a href="https://asterisk.apod.com/viewtopic.php?f=29&t=28633&start=25#p176102"
>spectacular menagerie</a> of silhouettes was taken in 2012 from the 
<a href="https://www.nps.gov/glca/index.htm"
>Glen Canyon National Recreation Area</a> near 
<a href="https://youtu.be/0NX1zt70ats">Page</a>, 
<a href="https://en.wikipedia.org/wiki/Arizona">Arizona</a>, 
<a href="https://en.wikipedia.org/wiki/United_States">USA</a>, 
where park rangers and astronomers <a href=
"https://dogsbestlife.com/wp-content/uploads/2017/09/training-multiple-dogs.jpg"
>expounded</a> on the 
<a href="https://apod.nasa.gov/apod/ap240303.html">unusual event</a> 
to interested gatherers. 

Also, faintly visible on the Sun's disk, 
just to the lower right of the dark Moon's disk, is a 
<a href="https://apod.nasa.gov/apod/ap260628.html">group of sunspots</a>. 

A <a href="https://science.nasa.gov/eclipses/future-eclipses/total-solar-eclipse-on-august-12-2026/"
>new solar eclipse</a> will occur this week and give many people in 
<a href="https://svs.gsfc.nasa.gov/5647"
>northern North America, Europe, and northwestern Africa</a> 
a new chance to contemplate a 
<a href="https://apod.nasa.gov/apod/ap230910.html"
>partially eclipsed Sun</a>.

A thin swath of 
<a href="https://science.nasa.gov/earth/facts/">Earth</a> from 
<a href="https://svs.gsfc.nasa.gov/5647">Greenland to Portugal</a> 
will further experience a 
<a href="https://apod.nasa.gov/apod/ap170820.html"
>total solar eclipse</a>.

An open question is whether any 
<a href="https://www.nasa.gov/blogs/watch-the-skies/2026/08/05/summer-star-shower-watch-the-perseids-with-nasa/">meteors</a> from the peaking 
<a href="https://apod.nasa.gov/apod/ap200810.html"
>Perseids</a> will be visible during totality. 


	    ]]>
	</description>
    </item>

    <item>
	<title><![CDATA[ APOD: 2026 August 8 – A Messier Moment for Tempel 2]]></title>
	<link>http://apod.nasa.gov/apod/ap260808.html</link>
	<pubDate>Sat, 08 Aug 2026 13:06:00 GMT</pubDate>
	<description>
	    <![CDATA[
	    <a href="http://apod.nasa.gov/apod/ap260808.html"><img src="https://apod.nasa.gov/apod/image/2608/10P_Tempel2_Globular_M30_20260729_DEBartlett600c.jpg" /></a>
<title> APOD: 2026 August 8 – A Messier Moment for Tempel 2</title>

Which of these is
<a href="https://apod.nasa.gov/apod/ap241005.html">not a comet</a>?

You guessed it -
the one on the right is a globular star cluster.

The diffuse greenish coma of periodic comet
<a href="https://ssd.jpl.nasa.gov/tools/sbdb_lookup.html#/?sstr=10P">10P/Tempel 2</a>
is at left in the frame.

In fact the globular star cluster is Messier 30,
also known as M30, or the 30th entry in astronomer
<a href="https://science.nasa.gov/people/explore-the-night-sky-hubbleatms-messier-catalog-bio/">Charles Messier's</a>
catalog of things which are not comets.

The well-known 18th century astronomer
kept a list of objects he observed, now his famous Messier
<a href="https://en.wikipedia.org/wiki/Messier_object">Catalogue of Nebulae and Star Clusters</a>,
which did not move from night to night against
the background stars and so were not the comets he was hunting for.

So the famous comet hunter would get the correct answer too, even
though his telescope would show both 10P/Tempel 2 and distant
star cluster as similar looking
faint and fuzzy objects in his field of view.

Recorded on July 29, this modern telescopic image
<a href="https://app.astrobin.com/i/bp809n?r=0">captures periodic comet Tempel 2</a>
as it briefly swept close on the sky to M30.

While the periodic comet's faint, narrow,
<a href="https://apod.nasa.gov/apod/ap260717.html">orbital dust trail</a> seems to pierce
the globular star cluster, Tempel 2 was a mere 3.5 light-minutes away.

<a href="https://science.nasa.gov/mission/hubble/science/explore-the-night-sky/hubble-messier-catalog/messier-30/">Messier 30</a>
is some 28,000 light-years distant.

	    ]]>
	</description>
    </item>

    <item>
	<title><![CDATA[Rubin's COSMOS Field]]></title>
	<link>http://apod.nasa.gov/apod/ap260807.html</link>
	<pubDate>Fri, 07 Aug 2026 13:06:00 GMT</pubDate>
	<description>
	    <![CDATA[
	    <a href="http://apod.nasa.gov/apod/ap260807.html"><img src="https://apod.nasa.gov/apod/image/2608/noirlab2618b_1024.jpg" /></a>
<title>Rubin's COSMOS Field</title>
    
    There are more than <a href="https://noirlab.edu/public/news/noirlab2618/">half a million galaxies</a> in the central panel of this <a href="https://noirlab.edu/public/images/noirlab2618b/">image</a> from the  <a href="https://rubinobservatory.org/">NSF-DOE Vera C. Rubin Observatory</a> in <a href="https://en.wikipedia.org/wiki/Chile">Chile</a>.

    This is the <a href="https://en.wikipedia.org/wiki/COSMOS_field">COSMOS field</a>, a patch of sky several times larger than the <a href="https://apod.nasa.gov/apod/ap251110.html">full moon</a>, first observed by <a href="https://science.nasa.gov/mission/hubble/">Hubble</a>.

    It has also been observed by <a href="https://science.nasa.gov/mission/webb/">Webb</a> and other telescopes because it contains comparatively few bright <a href="https://science.nasa.gov/universe/stars/">stars</a> from our own galaxy, offering a relatively unimpeded view of other galaxies outside the <a href="https://lco.global/spacebook/galaxies/the-milky-way-galaxy/">Milky Way</a>.

    The outer panels, numbered 1-10, show <a href="https://noirlab.edu/public/images/noirlab2618b/zoomable/">zoomed-in views</a> of the corresponding small regions highlighted in the central panel.

    The variety of galaxy shapes and sizes is <a href="https://images.unsplash.com/photo-1656340968218-f70f79d042a1">astonishing</a>.

    Some of them are so far away that their light has traveled for <a href="https://esahubble.org/science/age_size/">billions of years</a> before reaching Earth.

    Rubin will come back <a href="https://survey-strategy.lsst.io/baseline/ddf.html">every couple of days</a> to the COSMOS field as part of its ten-year <a href="https://rubinobservatory.org/news/action-rubin-lsst-begins">Legacy Survey of Space and Time</a>.

    It will allow a dynamic view of the COSMOS field and how the sky changes over time.
    
	    ]]>
	</description>
    </item>

    <item>
	<title><![CDATA[ APOD: 2026 August 6 – New Sharpest Image of the Sun Uncovers Instability  ]]></title>
	<link>http://apod.nasa.gov/apod/ap260806.html</link>
	<pubDate>Thu, 06 Aug 2026 13:06:00 GMT</pubDate>
	<description>
	    <![CDATA[
	    <a href="http://apod.nasa.gov/apod/ap260806.html"><img src="https://apod.nasa.gov/apod/image/2608/SunFlowers_NSO_960.jpg" /></a>
<title> APOD: 2026 August 6 – New Sharpest Image of the Sun Uncovers Instability  </title>
What does the new sharpest image of our Sun show?

Instability.

To be clear, a certain kind of interactive process called the 
<a href="https://en.wikipedia.org/wiki/Kelvin%E2%80%93Helmholtz_instability"
>Kelvin-Helmholtz instability</a> (KHI).

This instability can create 
<a href="https://www.bbc.com/news/world-us-canada-63912257"
>waves and swirls</a> when two streams flow past each other -- 
in this case variable streams of 
<a href="https://science.nasa.gov/learn/heat/big-ideas/big-idea-3-1/"
>solar magnetic plasma</a>.

Long hypothesized to occur on the 
<a href="https://apod.nasa.gov/apod/ap240615.html"
>Sun's surface</a>, 
KHI streaks and swirls were confirmed in 
just-released dramatic high-resolution 
images taken recently by the 
<a href="https://nso.edu/telescopes/inouye-solar-telescope/"
>Inouye Solar</a> 
<a href="https://youtu.be/vN8cnN7Nlh4">Telescope</a> in 
<a href="https://youtu.be/YPVLrSjKlh8">Hawaii</a>, 
<a href="https://en.wikipedia.org/wiki/United_States">USA</a>. 

The 
<a href="https://nso.edu/press-release/nsf-inouye-solar-telescope-enables-major-discovery-of-a-hidden-solar-process/"
>featured false-yellow image</a>, actually taken in deep blue, 
is the highest resolution image yet of 
<a href="https://apod.nasa.gov/apod/ap251207.html"
>the Sun</a> in 
<a href="https://science.nasa.gov/ems/09_visiblelight/"
>visible light</a>.

It spans about the radius of 
<a href="https://apod.nasa.gov/apod/ap260322.html"
>the Earth</a>, but its finest details are city sized. 

Visible are several smooth tops of 
<a href="https://apod.nasa.gov/apod/ap200203.html">changing solar granules</a>, while the edges of the flower-like 
structures have been found to harbor multiple 
<a href="https://scied.ucar.edu/image/kelvin-helmholtz-clouds"
>KHI swirls</a>. 

<a href="https://encrypted-tbn0.gstatic.com/images?q=tbn:ANd9GcREdooSerHyBwFsDYNPLDPzuJNwiZ7D_x8TKWp3KvPAQA&s=10"
>Future research</a> may investigate how the KHI helps move energy, 
magnetic fields, and may even heat the surrounding 
<a href="https://apod.nasa.gov/apod/ap230516.html"
>solar corona</a>. 


	    ]]>
	</description>
    </item>

    <item>
	<title><![CDATA[ APOD: 2026 August 5 – Spokes on Saturn's B Ring]]></title>
	<link>http://apod.nasa.gov/apod/ap260805.html</link>
	<pubDate>Wed, 05 Aug 2026 13:06:00 GMT</pubDate>
	<description>
	    <![CDATA[
	    <a href="http://apod.nasa.gov/apod/ap260805.html"><img src="https://apod.nasa.gov/apod/image/2608/saturn_spokes.gif" /></a>
<title> APOD: 2026 August 5 – Spokes on Saturn's B Ring</title>
Don’t get spooked by Saturn’s ghostly spokes! Today we feature a nearly two-hour timelapse of Saturn and its rings looping forwards and backwards. A day on Saturn is only 10 hours long, 
so two hours of observation covers quite a bit of its rotation. If you look closely, a ghoulish shadow appears and disappears as 
<a href="https://science.nasa.gov/resource/saturns-rings-2/">Saturn’s B ring</a> 
rotates. Decades of observation with 
<a href="https://science.nasa.gov/resource/ring-spokes-4/">Voyager 2</a>, 
<a href="https://science.nasa.gov/image-article/apod-2009-june-2-spokes-reappear-on-saturns-rings/">Cassini</a>, and 
<a href="https://science.nasa.gov/video-detail/hubble-saturn-oct2023-stsci-01hgxkq49bmac02hcazdvkea3f/">Hubble</a> 
show the appearance of Saturn’s spokes varies with 
<a href="https://www.planetary.org/space-images/saturns-seasons">the planet’s seasons</a>. 
Like Earth, Saturn’s 
<a href="https://www.youtube.com/watch?v=46G1foTIivo">spin axis</a> 
is tilted compared to the plane of its orbit around the Sun. During Saturn’s 
<a href="https://education.nationalgeographic.org/resource/equinox/">equinox</a>, 
the rings are 
<a href="https://science.nasa.gov/image-article/apod-2025-november-16-crossing-saturns-ring-plane/">less tilted</a> 
away from the Sun and the planet receives more evenly distributed sunlight and 
<a href="https://science.nasa.gov/sun/what-is-the-solar-wind/">solar wind</a>. 
Although their origin is still uncertain, Saturn’s spokes may be shadows of and reflections off of 
dust and ice levitating above the rings caused by 
<a href="https://science.nasa.gov/universe/overview/forces/#electromagnetic-force">electromagnetic</a> 
interactions between the solar wind and the planet’s magnetic field.

	    ]]>
	</description>
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    <item>
	<title><![CDATA[ APOD: 2026 August 4 – Curious Cometary Knots in the Helix Nebula ]]></title>
	<link>http://apod.nasa.gov/apod/ap260804.html</link>
	<pubDate>Tue, 04 Aug 2026 13:06:00 GMT</pubDate>
	<description>
	    <![CDATA[
	    <a href="http://apod.nasa.gov/apod/ap260804.html"><img src="https://apod.nasa.gov/apod/image/2608/HelixKnots_JWST_960.jpg" /></a>
<title> APOD: 2026 August 4 – Curious Cometary Knots in the Helix Nebula </title>
What causes unusual knots of gas and dust in 
<a href="https://en.wikipedia.org/wiki/Planetary_nebula"
>planetary nebulas</a>? 

Seen also in the 
<a href="https://apod.nasa.gov/apod/ap230814.html">Ring Nebula</a>, the 
<a href="https://apod.nasa.gov/apod/ap260622.html">Dumbbell Nebula</a> and 
<a href="https://apod.nasa.gov/apod/ap060709.html">NGC 2392</a>, 
the knots' existence was not initially predicted, and their origins are still 
<a href="https://dogwithblog.in/wp-content/uploads/2014/08/head-tilt-flappy-ears.jpg">not well understood</a>. 

Pictured <a href="https://science.nasa.gov/asset/webb/helix-nebula-nircam/"
>here</a> is a fascinating image of 
<a href="https://science.nasa.gov/asset/webb/helix-nebula-context-vista-and-webb/">part</a> of the 
<a href="https://apod.nasa.gov/apod/ap250729.html">Helix Nebula</a> by the 
<a href="https://science.nasa.gov/mission/webb/"
>James Webb Space Telescope</a> showing tremendous detail in 
<a href="https://science.nasa.gov/ems/07_infraredwaves/"
>infrared light</a>.

The cometary knots have masses similar to the 
<a href="https://science.nasa.gov/earth/facts/"
>Earth</a> but have sizes typically several times the orbit of Pluto. 

<a href="https://ui.adsabs.harvard.edu/abs/1996AJ....111.1630O/abstract"
>One hypothesis</a> for the fragmentation and 
evolution of the knots includes existing gas being 
<a href="https://en.wikipedia.org/wiki/Rayleigh%E2%80%93Taylor_instability"
>driven out</a> by a less dense but highly energetic 
<a href="https://en.wikipedia.org/wiki/Stellar_wind"
>stellar wind</a> of the central evolving star. 

The <a href="https://en.wikipedia.org/wiki/Helix_Nebula"
>Helix Nebula</a> is one of the closest examples of a 
<a href="https://esahubble.org/wordbank/planetary-nebula/"
>planetary nebula</a> created at the end of the 
<a href="https://science.nasa.gov/resource/the-life-cycle-of-a-sun-like-star-annotated/">life of a Sun-like star</a>. 

Given a technical designation of NGC 7293, the 
<a href="https://science.nasa.gov/asset/webb/helix-nebula-mini-poster/"
   >Helix Nebula</a> lies about 650 
<a href="https://spaceplace.nasa.gov/light-year/en/"
>light-year</a>s away towards the constellation of Water Carrier 
(<a href=" https://en.wikipedia.org/wiki/Aquarius_(constellation)"
>Aquarius</a>).


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	<title><![CDATA[ APOD: 2026 August 3 – Vaporizing Meteor Photobombs the Lacerta Nebula ]]></title>
	<link>http://apod.nasa.gov/apod/ap260803.html</link>
	<pubDate>Mon, 03 Aug 2026 13:06:00 GMT</pubDate>
	<description>
	    <![CDATA[
	    <a href="http://apod.nasa.gov/apod/ap260803.html"><img src="https://apod.nasa.gov/apod/image/2608/MeteorGecko_Burnett_1080.jpg" /></a>
<title> APOD: 2026 August 3 – Vaporizing Meteor Photobombs the Lacerta Nebula </title>
What's happening to this meteor?

This <a href="https://apod.nasa.gov/apod/ap240809.html">bright meteor streak</a> 
appeared and disappeared quickly during a long exposure of the 
<a href="https://apod.nasa.gov/apod/ap250910.html">Great Lacerta Nebula</a>, 
seen faintly in red toward the center of the image.

The <a href=
"https://starchild.gsfc.nasa.gov/docs/StarChild/solar_system_level2/meteoroids.html"
>meteoroid</a>, likely a small pebble, 
<a href="https://www.astroleague.org/what-are-meteors-and-why-do-they-glow/"
>creates its glow</a> partly by heating and exciting surrounding air in 
<a href="https://science.nasa.gov/earth/earth-atmosphere/earths-atmosphere-a-multi-layered-cake/">Earth's atmosphere</a>, 
but itself vaporizes and leaves wind-blown gas and dust with 
<a href="https://apod.nasa.gov/apod/ap230724.html">colors</a> that give clues to its composition. 

The featured image was captured last month from 
<a href="https://deathvalleyobservatories.com/find-our-location/"
>Death Valley Observatories</a> in 
<a href="https://en.wikipedia.org/wiki/Nevada">Nevada</a>, 
<a href="https://user.iiasa.ac.at/~marek/fbook/04/print/us.html"
>USA</a>. 

This month, though, is particularly good for 
<a href="https://apod.nasa.gov/apod/ap250821.html">seeing meteors</a>.

Presently there are 
<a href="https://science.nasa.gov/solar-system/meteors-meteorites/delta-aquariids/">three</a> 
<a href="https://en.wikipedia.org/wiki/Alpha_Capricornids">meteor</a> 
<a href="https://apod.nasa.gov/apod/ap250812.html">showers</a> ongoing, 
although they are currently 
<a href="https://encrypted-tbn0.gstatic.com/images?q=tbn:ANd9GcREbUigD3ZOb-3oCWkhrRoLJ7de6EcqbfEk2JmNOISeKw&s=10"
>competing for visibility</a> with the glow of a bright 
<a href="https://apod.nasa.gov/apod/ap231112.html">gibbous Moon</a>. 

The most active of these showers, the 
<a href="https://science.nasa.gov/solar-system/meteors-meteorites/perseids/"
>Perseids</a>, will be busiest in about 10 days -- 
after <a href="https://svs.gsfc.nasa.gov/5587/"
>the Moon</a> has dimmed considerably. 

This year, the 
<a href="https://earthsky.org/astronomy-essentials/everything-you-need-to-know-perseid-meteor-shower/">Perseids peak</a> nearly coincides with not only a 
<a href="https://assets.science.nasa.gov/dynamicimage/assets/science/psd/solar/2023/09/m/moon_phases.png"
>new Moon</a>, but, from some locations, one that 
<a href="https://apod.nasa.gov/apod/ap240310.html">totally eclipses</a> the 
<a href="https://science.nasa.gov/sun/">Sun</a>. 


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	<title><![CDATA[ APOD: 2026 August 2 – A Fire Rainbow over West Virginia ]]></title>
	<link>http://apod.nasa.gov/apod/ap260802.html</link>
	<pubDate>Sun, 02 Aug 2026 13:06:00 GMT</pubDate>
	<description>
	    <![CDATA[
	    <a href="http://apod.nasa.gov/apod/ap260802.html"><img src="https://apod.nasa.gov/apod/image/2608/FireRainbow_Harbig_960.jpg" /></a>
<title> APOD: 2026 August 2 – A Fire Rainbow over West Virginia </title>
What's happening to this cloud?

Ice crystals in a distant cirrus cloud are acting like little floating 
<a href="http://micro.magnet.fsu.edu/primer/java/scienceopticsu/newton/"
>prisms</a>.  

Known informally as a fire rainbow for its flame-like appearance, a 
<a href="https://en.wikipedia.org/wiki/Circumhorizon_arc">circumhorizon arc</a> 
appears parallel to the horizon.

For a <a href="https://www.atoptics.co.uk/halo/cha2.htm">circumhorizontal arc</a> 
to be visible, 
<a href="https://science.nasa.gov/sun/">the Sun</a> 
must be at least 58 degrees high in a sky where 
<a href="https://en.wikipedia.org/wiki/Cirrus_cloud">cirrus clouds</a> present below --  
in this case 
<a href="https://www.colweather.org.uk/gal-clouds-cirrus.php#Cirrus%20fibratus"
>cirrus fibratus</a>.  

The numerous, flat, 
<a href="http://www.atoptics.co.uk/halo/orplate.htm">hexagonal ice-crystals</a> 
that compose the 
<a href="https://en.wikipedia.org/wiki/Cirrus_cloud">cirrus cloud</a> must be 
<a href="https://www.atoptics.co.uk/halo/platcol.htm">aligned horizontally</a> 
to properly 
<a href="http://youtube.com/watch?v=U98KPM2b9IA">refract sunlight</a> in a collectively similar manner. 

Therefore, <a href="https://apod.nasa.gov/apod/ap190519.html">circumhorizontal</a>
<a href="https://apod.nasa.gov/apod/ap151215.html">arcs</a> are 
<a href="https://i.pinimg.com/550x/81/21/c0/8121c0291fa14d1fe52b9eb007741cac.jpg">somewhat unusual</a> to see. 

The <a href="https://www.facebook.com/photo?fbid=4794142133932422"
>featured fire rainbow</a> was photographed in 2021 near 
<a href="https://youtu.be/kROh8JwKnOk">North Fork Mountain</a> in 
<a href="https://en.wikipedia.org/wiki/West_Virginia">West Virginia</a>, 
<a href="https://en.wikipedia.org/wiki/United_States">USA</a>. 



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	<title><![CDATA[ APOD: 2026 August 1 – Buck Moon and Belt of Venus]]></title>
	<link>http://apod.nasa.gov/apod/ap260801.html</link>
	<pubDate>Sat, 01 Aug 2026 13:06:00 GMT</pubDate>
	<description>
	    <![CDATA[
	    <a href="http://apod.nasa.gov/apod/ap260801.html"><img src="https://apod.nasa.gov/apod/image/2608/FullMoon28-7-2026BrankoNadj1024.jpg" /></a>
<title> APOD: 2026 August 1 – Buck Moon and Belt of Venus</title>

<a href="https://earthsky.org/moon-phases/july-full-moon/">The Buck Moon</a>
is a traditional name for the full moon of July.

In this colorful Adriatic sea and skyscape captured on July 28 from
Krk Island along the coast of Croatia,
a full Buck Moon is just rising over distant mountains.

Since a full moon rises as the Sun sets,
<a href="https://nightsky.jpl.nasa.gov/media/documents/resources/EarthShadow3.pdf">Earth's shadow</a>
also rises in the twilight scene, a diffuse gray band extending above the
mountainous southeastern horizon.

Above Earth's shadow band is the pinkish
<a href="https://science.nasa.gov/image-article/apod-2006-june-15-gordel-van-venus/">antitwilight arch</a>.

That subtly tinted band of backscattered sunlight is more widely known as the
<a href="https://en.wikipedia.org/wiki/Belt_of_Venus">Belt of Venus</a>.

But as it shares the eastern horizon with the atmospheric
shadow of Earth and Belt of Venus,
this full Buck Moon seems to set the stage for the New Moon to come.

The New Moon of August 12 will cast its shadow on planet Earth in a much anticipated
<a href="https://www.nasa.gov/news-release/nasa-sets-coverage-for-august-northern-hemisphere-total-solar-eclipse/">total solar eclipse</a>.

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	<title><![CDATA[ APOD: 2026 July 31 – NGC 4372 and the Dark Doodad]]></title>
	<link>http://apod.nasa.gov/apod/ap260731.html</link>
	<pubDate>Fri, 31 Jul 2026 13:06:00 GMT</pubDate>
	<description>
	    <![CDATA[
	    <a href="http://apod.nasa.gov/apod/ap260731.html"><img src="https://apod.nasa.gov/apod/image/2607/DARK-DOODAD_1024.jpg" /></a>
<title> APOD: 2026 July 31 – NGC 4372 and the Dark Doodad</title>

The Dark Doodad Nebula drifts
<a href="https://apod.nasa.gov/apod/ap210101.html">through southern skies</a>,
a tantalizing target for binoculars toward the small constellation
<a href="http://en.wikipedia.org/wiki/Musca">Musca</a>, The Fly.

A dusty interstellar cloud, it's seen against
rich starfields just south of the Coalsack Nebula and the Southern Cross.

Stretching for about 3 degrees across this telescopic field of view, 
<a href="https://en.wikipedia.org/wiki/Dark_Doodad_Nebula">the Dark Doodad</a>
is punctuated near its southern tip (upper right) by yellowish
globular star cluster
<a href="http://spider.seds.org/spider/MWGC/n4372.html">NGC 4372</a>.

Of course NGC 4372 roams the halo of our
<a href="https://science.nasa.gov/resource/the-milky-way-galaxy/">Milky Way</a>
galaxy, a background object some 20,000 light-years away and only
by chance along our line-of-sight to the Dark Doodad.

About 700 light-years distant and over 30 light-years long,
the Dark Doodad's well defined silhouette belongs to the
<a href="https://arxiv.org/abs/1507.03742">potentially</a> star-forming
<a href="https://ui.adsabs.harvard.edu/abs/2024A%26A...687L...9E/abstract">Musca molecular cloud</a>.

The dusty Dark Doodad's delightfully alliterative moniker was first coined by
<a href="https://www.minorplanetcenter.net/db_search/show_object?utf8=%E2%9C%93&object_id=dicicco">astro-imager and writer</a>
Dennis di Cicco in 1986 while
observing Comet Halley from the Australian outback.

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	<title><![CDATA[Red Sun through Wildfire Smoke]]></title>
	<link>http://apod.nasa.gov/apod/ap260730.html</link>
	<pubDate>Thu, 30 Jul 2026 13:06:00 GMT</pubDate>
	<description>
	    <![CDATA[
	    <a href="http://apod.nasa.gov/apod/ap260730.html"><img src="https://apod.nasa.gov/apod/image/2607/red_sun_1024.jpg" /></a>
<title>Red Sun through Wildfire Smoke</title>
    
    This could be the view from an <a href="https://science.nasa.gov/exoplanets/">exoplanet</a> orbiting around a <a href="https://www.britannica.com/science/red-dwarf-star">red dwarf star</a>, but it is our own <a href="https://science.nasa.gov/sun/">Sun</a>.

    <a href="https://www.instagram.com/p/DbH_V37lKyN/">This image</a> was taken on July 22, 2026, in the <a href="https://en.wikipedia.org/wiki/Okanagan">Okanagan region</a> in the Canadian province of <a href="https://www.supernaturalbc.com/">British Columbia</a>.

    <a href="https://fire.airnow.gov/">Wildfire smoke</a> from the <a href="https://en.wikipedia.org/wiki/Pacific_Northwest">Pacific Northwest</a> acted as a <a href="https://www.usa.canon.com/learning/training-articles/training-articles-list/being-safe-using-solar-filters">solar filter</a>, allowing the photographer to take this photo of the Sun directly.

    Several <a href="https://science.nasa.gov/sun/sunspots/">sunspots</a> are also visible in this eerie image; just below and right of the center is <a href="https://www.friendsofnasa.org/2026/07/fast-evolving-sunspot-ar-4493-larger.html">AR 4493</a>, a fast evolving, giant <a href="https://scied.ucar.edu/image/solar-active-regions-sunspots-uv-image">active solar region</a> and sunspot group.
    
    The smoke is made of tiny particles that help block and <a href="https://en.wikipedia.org/wiki/Mie_scattering">scatter</a> light with bluer <a href="https://science.nasa.gov/mission/hubble/science/science-behind-the-discoveries/wavelengths/">colors</a>, so the light we see coming from the Sun is <a href="https://apod.nasa.gov/apod/ap130829.html">dimmer and redder</a> than usual (but it is never safe to <a href="https://images.unsplash.com/photo-1505628346881-b72b27e84530">stare directly</a> at the Sun).

    Sunsets and sunrises are also <a href="https://weather.com/science/weather-explainers/news/2025-08-05-wildfire-smoke-red-sunset-sunrise-scattering-explained">more colorful</a> because of the smoke.  
    
    Some <a href="https://science.nasa.gov/exoplanets/resources/life-and-death/chapter-6/">6 billion years</a> from now, the Sun will actually start to turn redder as it approaches its <a href="https://science.nasa.gov/universe/stars/types/#red-giants">red giant</a> phase. 
    
    
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	<title><![CDATA[ APOD: 2026 July 29 – Psyche Receives Gravity Assist from Mars]]></title>
	<link>http://apod.nasa.gov/apod/ap260729.html</link>
	<pubDate>Wed, 29 Jul 2026 13:06:00 GMT</pubDate>
	<description>
	    <![CDATA[
	    <a href="http://apod.nasa.gov/apod/ap260729.html"><img src="" /></a>
<title> APOD: 2026 July 29 – Psyche Receives Gravity Assist from Mars</title>
Solar System bodies make deep space exploration more fuel efficient! 
<a href="https://science.nasa.gov/blogs/psyche/2026/07/17/nasas-psyche-mission-delivers-mars-flyby-data-time-lapse-video/">Today’s video</a> 
shows 
<a href="https://science.nasa.gov/mission/psyche/">the Psyche spacecraft</a> 
gaining speed and changing its trajectory with minimal fuel spent due to a 
<a href="https://science.nasa.gov/learn/basics-of-space-flight/primer/">gravity assist</a> 
from Mars in May 2026. Mars has an average orbital speed of almost 
87,000 km/h (54,000 mph) around the Sun. Its orbital motion and its gravity allowed Mars to 
pull Psyche along with it, increasing the spacecraft’s speed. Gravity assists have been used since 1959’s 
<a href="https://en.wikipedia.org/wiki/Luna_3">Luna 3 mission</a> 
to allow for spacecraft 
(<a href="https://www.youtube.com/watch?v=l8TA7BU2Bvo">the Voyagers</a>, 
<a href="https://apod.nasa.gov/apod/ap990826.html">Cassini</a>) 
to reach farther than they could with fuel alone. This assist helped the Psyche spacecraft on its journey 
to the Psyche asteroid, which it will reach in 2029. While passing Mars, the spacecraft tested instruments 
that will analyze the asteroid’s composition and magnetic field. This is the first mission to an asteroid 
<a href="https://www.planetary.org/space-missions/psyche">thought to be largely made of metal</a>, 
an essential building block for planets, rather than rock or ice.

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	<title><![CDATA[ APOD: 2026 July 28 – Barnards Loop over Twin Volcanoes ]]></title>
	<link>http://apod.nasa.gov/apod/ap260728.html</link>
	<pubDate>Tue, 28 Jul 2026 13:06:00 GMT</pubDate>
	<description>
	    <![CDATA[
	    <a href="http://apod.nasa.gov/apod/ap260728.html"><img src="https://apod.nasa.gov/apod/image/2607/LoopVolcanos_Laserna_960.jpg" /></a>
<title> APOD: 2026 July 28 – Barnards Loop over Twin Volcanoes </title>
What's connecting these two volcanoes?

In ancient folklore, the two volcanoes, 
<a href="https://youtu.be/Jwpue5dq_wA?t=171"
>Parinacota (left) and Pomerape (right)</a>, 
are connected by representing a 
<a href="https://qhapaqnan.qiri.cl/ancient-legends/"
>mythical</a> prince and princess who engaged in a forbidden romance. 

Beneath the ground, the 
<a href="https://science.nasa.gov/earth/earth-observatory/parinacota-volcano-south-america-76144/">two peaks</a> are not known to be 
connected by a common pool of 
<a href="https://apod.nasa.gov/apod/ap051002.html">hot magma</a>, 
and neither volcano has erupted in the past 1000 years. 

Above the ground, there is usually nothing in the sky that connects them -- except if you use careful timing and look from a specific location. 

The <a href="https://www.instagram.com/p/DXpszcJCY6n/"
>featured well-planned image</a> was captured from 
<a href="https://en.wikipedia.org/wiki/Bolivia">Bolivia</a> 
in mid-April with a series of camera exposures 
taken on the same day and from the same location. 

Then, <a href="https://apod.nasa.gov/apod/ap090224.html">Barnard's Loop</a> 
<a href="https://www.reddit.com/media?url=https%3A%2F%2Fi.redd.it%2F56kpgyhj47dg1.png">appeared</a> to connect the volcanic peaks.

Also visible in the image is the 
<a href="https://apod.nasa.gov/apod/ap260218.html">Orion Nebula</a> in the center, the star 
<a href="https://science.nasa.gov/universe/what-is-betelgeuse-inside-the-strange-volatile-star/">Betelgeuse</a> on the right, and the 
<a href="https://apod.nasa.gov/apod/ap200329.html">Rosette</a> 
<a href="https://apod.nasa.gov/apod/ap250214.html">Nebula</a> on the upper right. 


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	<title><![CDATA[ APOD: 2026 July 27 – NGC 7635: The Bubble Nebula ]]></title>
	<link>http://apod.nasa.gov/apod/ap260727.html</link>
	<pubDate>Mon, 27 Jul 2026 13:06:00 GMT</pubDate>
	<description>
	    <![CDATA[
	    <a href="http://apod.nasa.gov/apod/ap260727.html"><img src="https://apod.nasa.gov/apod/image/2607/Bubble_Piechnik_960.jpg" /></a>
<title> APOD: 2026 July 27 – NGC 7635: The Bubble Nebula </title>
What created this huge space bubble?

Blown by the wind from a star, this
<a href="https://www.exploratorium.edu/snacks/tag/bubbles"
>tantalizing</a>, head-like
apparition is cataloged as NGC 7635, but known simply
as the <a href="https://en.wikipedia.org/wiki/Bubble_Nebula"
>Bubble Nebula</a>.

Taken from 
<a href="https://youtu.be/2CHS7fdbX6o">Krakow</a>, 
<a href="https://en.wikipedia.org/wiki/Poland">Poland</a>, 
the 
<a href="https://www.flickr.com/photos/181668516@N04/54784480055/"
>featured view</a> utilizes a long exposure 
to reveal the intricate details of
<a href="https://apod.nasa.gov/apod/ap030617.html">this cosmic bubble</a> and its environment.

Although it looks delicate, the 10 
<a href="http://chandra.harvard.edu/photo/cosmic_distance.html">light-year</a> 
diameter bubble offers evidence of
<a href="https://apod.nasa.gov/apod/ap260715.html">violent processes</a> at work.

Seen here right of 
<a href="https://apod.nasa.gov/apod/ap170531.html">the Bubble</a>'s center, a bright
hot star is embedded in the nebula's 
<a href="https://en.wikipedia.org/wiki/Reflection_nebula"
>reflecting</a> dust.

A fierce 
<a href="http://en.wikipedia.org/wiki/Stellar_wind">stellar wind</a> 
and intense radiation from the 
<a href="https://science.nasa.gov/universe/stars/">star</a>, 
which likely has a mass 10 to 20 times that of the 
<a href="https://science.nasa.gov/sun/">Sun</a>,
has blasted out the
<a href="https://ui.adsabs.harvard.edu/abs/1995A%26A...295..509C/abstract"
>structure of glowing gas</a>
against denser material in a surrounding 
<a href="https://apod.nasa.gov/apod/ap230129.html">molecular cloud</a>.

The intriguing 
<a href="https://science.nasa.gov/image-detail/37893980612-307324af83-o/"
>Bubble Nebula</a> lies a mere 11,000 
<a href="https://spaceplace.nasa.gov/light-year/">light-year</a>s 
away toward the 
<a href="https://media.istockphoto.com/id/159176199/photo/cat.jpg?s=612x612&w=0&k=20&c=U34AGa5EN0xuBbrzpSygVHcR7RHuwWAivyH7hpHw_m0="
>boastful</a> constellation 
<a href="http://en.wikipedia.org/wiki/Cassiopeia_%28constellation%29"
>Cassiopeia</a>.


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	<title><![CDATA[ APOD: 2026 July 26 – Simulation TNG50: A Galaxy Cluster Forms ]]></title>
	<link>http://apod.nasa.gov/apod/ap260726.html</link>
	<pubDate>Sun, 26 Jul 2026 13:06:00 GMT</pubDate>
	<description>
	    <![CDATA[
	    <a href="http://apod.nasa.gov/apod/ap260726.html"><img src="" /></a>
<title> APOD: 2026 July 26 – Simulation TNG50: A Galaxy Cluster Forms </title>
How do clusters of galaxies form? 

Since our universe moves too slowly to watch, faster-moving computer simulations are created to help find out. 

One famous effort is 
<a href="https://www.tng-project.org/about/">TNG50</a> from 
<a href="https://www.tng-project.org/">IllustrisTNG</a>, an upgrade of the famous 
<a href="https://www.illustris-project.org/">Illustris Simulation</a>.

The first part of the 
<a href="https://www.tng-project.org/media/">featured video</a> 
tracks cosmic gas (mostly 
<a href="https://periodic.lanl.gov/1.shtml">hydrogen</a>) 
as it evolves into 
<a href="https://science.nasa.gov/universe/galaxies/">galaxies</a> and 
<a href="https://en.wikipedia.org/wiki/Galaxy_cluster">galaxy clusters</a> 
from the early universe to today, with brighter colors marking faster moving gas. 

As the universe matures, gas falls into 
<a href="https://en.wikipedia.org/wiki/Gravity_well">gravitational wells</a>, 
galaxies forms, galaxies spin, galaxies collide and merge, all while 
<a href="https://apod.nasa.gov/apod/ap991017.html">black holes form in galaxy centers</a> 
and expel surrounding gas at high speeds.

The second half of the video switches to tracking stars, showing a 
<a href="https://apod.nasa.gov/apod/ap251003.html">galaxy cluster</a> coming together, complete with 
<a href="https://apod.nasa.gov/apod/ap241213.html">stellar streams</a>. 

The outflow from black holes in 
<a href="https://arxiv.org/abs/1902.05553">TNG50</a> is surprisingly complex and details are being compared with our 
<a href="https://apod.nasa.gov/apod/ap250302.html">real universe</a>. 

<a href="https://ui.adsabs.harvard.edu/abs/2019MNRAS.490.3234N/abstract"
>Studying how</a> gas coalesced in the 
<a href="https://science.nasa.gov/mission/webb/early-universe/"
>early universe</a> helps humanity better understand how our 
<a href="https://science.nasa.gov/earth/facts/">Earth</a>, 
<a href="https://science.nasa.gov/sun/">Sun</a>, and 
<a href="https://www.openspaceproject.com/solar-system-videos"
>Solar System</a> originally formed.

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	</description>
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	<title><![CDATA[ APOD: 2026 July 25 – Tranquility and Serenity]]></title>
	<link>http://apod.nasa.gov/apod/ap260725.html</link>
	<pubDate>Sat, 25 Jul 2026 13:06:00 GMT</pubDate>
	<description>
	    <![CDATA[
	    <a href="http://apod.nasa.gov/apod/ap260725.html"><img src="https://apod.nasa.gov/apod/image/2607/TranquilitySerenity1024c.jpg" /></a>
<title> APOD: 2026 July 25 – Tranquility and Serenity</title>

The Seas of <a href="https://apod.nasa.gov/apod/ap190719.html">Tranquility</a>
and <a href="https://apod.nasa.gov/apod/ap240117.html">Serenity</a> are calm today.

They're calm most every day though, since they are actually
<a href="https://en.wikipedia.org/wiki/Lunar_mare">lunar maria</a>,
ancient lava flows filling in large impact
<a href="https://science.nasa.gov/moon/lunar-craters/#hds-sidebar-nav-6">basins on the Moon</a>.

Also known by Latin names Mare Tranquillitatis (right)
and Mare Serenitatis, the smooth dark lunar "seas" are
in stark contrast to the
bright cratered lunar highlands surrounding them in
this telescopic view.

Of course their names are based on the historical,
<a href="https://ui.adsabs.harvard.edu/abs/1969Moon....1...59K/abstract">pre-telescopic</a>
designations of lunar maria.

Easily visible to the unaided eye,
the broad features on the Moon's near side were imagined to be like the
expansive oceans of planet Earth.

On July 20, 1969, the Apollo 11 lunar module Eagle touched down on the Mare
Tranquillitatis (at lower right), establishing
<a href="https://lroc.im-ldi.com/images/563">Tranquility base</a> and the first
human presence
<a href="https://svs.gsfc.nasa.gov/4731/">on the Moon</a>.

	    ]]>
	</description>
    </item>

    <item>
	<title><![CDATA[ APOD: 2026 July 24 – RCW 86: Historical Supernova Remnant]]></title>
	<link>http://apod.nasa.gov/apod/ap260724.html</link>
	<pubDate>Fri, 24 Jul 2026 13:06:00 GMT</pubDate>
	<description>
	    <![CDATA[
	    <a href="http://apod.nasa.gov/apod/ap260724.html"><img src="https://apod.nasa.gov/apod/image/2607/RCW86Final1024.jpg" /></a>
<title> APOD: 2026 July 24 – RCW 86: Historical Supernova Remnant</title>

In 185 AD,
<a href="http://en.wikipedia.org/wiki/Chinese_astronomy">Chinese astronomers</a>
recorded the appearance of a new star in the Nanmen asterism.

That part of the sky is
identified with part of the southern constellation
<a href="https://en.wikipedia.org/wiki/Centaurus_in_Chinese_astronomy">Centaurus</a>
on modern star charts.

In fact, the new star was reported to be visible to the naked-eye for months
before it faded from view, and is now thought to be the earliest
<a href="http://arxiv.org/abs/astro-ph/0301603">recorded supernova</a>.

In this 21st century telescopic image,
the wispy outlines of a faint emission nebula
recognized as the remnant of that historical stellar explosion
can be traced against a starry background.

The ragged but roughly circular extent
of the nebula, cataloged as RCW 86,
represents interstellar gas ionized by the supernova's
still expanding shock wave.

<a href="https://chandra.harvard.edu/photo/2011/rcw86/">Space-based
images</a> indicate an abundance of the element iron in RCW 86 and
the absence of a neutron star or pulsar
<a href="https://arxiv.org/abs/1108.1207">within the remnant</a>,
suggesting that the original supernova was Type Ia.

<a href="https://apod.nasa.gov/apod/ap060728.html">Unlike the core collapse</a>
supernova explosion of a massive star, a
<a href="https://science.nasa.gov/mission/roman-space-telescope/type-ia-supernovae/">Type Ia supernova</a>
is a thermonuclear
<a href="https://apod.nasa.gov/apod/ap110430.html">detonation on a white dwarf</a>
star that has accreted material from its companion in a binary star system.

Near the plane of our
<a href="https://apod.nasa.gov/apod/ap110520.html">Milky Way</a>
galaxy and larger than the full moon on the sky this supernova remnant
is too faint to be seen by eye though.

RCW 86 is some 8,000 light-years distant and around 100 light-years
across.

	    ]]>
	</description>
    </item>

    <item>
	<title><![CDATA[The Large Magellanic Cloud]]></title>
	<link>http://apod.nasa.gov/apod/ap260723.html</link>
	<pubDate>Thu, 23 Jul 2026 13:06:00 GMT</pubDate>
	<description>
	    <![CDATA[
	    <a href="http://apod.nasa.gov/apod/ap260723.html"><img src="https://apod.nasa.gov/apod/image/2607/LMC_1024.jpg" /></a>
<title>The Large Magellanic Cloud</title>
    
    Have you ever seen <a href="https://www.youcanseethemilkyway.com/blog/what-galaxies-can-you-see-with-the-naked-eye">another galaxy</a> with your own eyes?

    The <a href="https://www.instagram.com/p/Da5kVNrkSwA/?img_index=1">featured image</a> shows the <a href="https://en.wikipedia.org/wiki/Large_Magellanic_Cloud">Large Magellanic Cloud</a> (LMC), one of the closest neighbors of our <a href="https://imagine.gsfc.nasa.gov/science/objects/milkyway1.html">Milky Way</a>.
    
    If you are anywhere south of <a href="https://oceanservice.noaa.gov/facts/latitude.html">latitude</a> 20&deg N (but the further south, the better), you can see it <a href="https://www.astronomy.com/observing/take-a-closer-look-at-the-large-magellanic-cloud/">with the unaided eye</a> if you go to a dark sky location, away from big cities and <a href="https://apod.nasa.gov/apod/ap200408.html">light polution</a>.

    It is a <a href="https://esahubble.org/wordbank/dwarf-galaxy/">dwarf</a> <a href="https://science.nasa.gov/universe/galaxies/types/#irregular-galaxies">irregular galaxy</a> about 163,000 light-years away, and a member of our <a href="http://www.atlasoftheuniverse.com/localgr.html">Local Group</a> of galaxies.

    Despite being small, with a total mass approximately equivalent to <a href="https://iopscience.iop.org/article/10.3847/1538-4357/ad1f58/pdf">10% - 20%</a> of the mass of the Milky Way, the LMC is very actively <a href="https://apod.nasa.gov/apod/ap260219.html">forming stars</a>.

    This is likely due in part to the gravitational <a href="https://images.unsplash.com/photo-1687425961065-46efeb465c66">push and pull</a> of tides caused by the Milky Way on the LMC.

    Some astronomers have predicted that it will <a href="https://www.sci.news/astronomy/large-magellanic-cloud-milky-way-collision-06788.html">collide</a> with the Milky Way in in about 2 billion years.
    
	    ]]>
	</description>
    </item>

    <item>
	<title><![CDATA[ APOD: 2026 July 22 – The Corona Australis Cloud and the Chandelier Cluster]]></title>
	<link>http://apod.nasa.gov/apod/ap260722.html</link>
	<pubDate>Wed, 22 Jul 2026 13:06:00 GMT</pubDate>
	<description>
	    <![CDATA[
	    <a href="http://apod.nasa.gov/apod/ap260722.html"><img src="https://apod.nasa.gov/apod/image/2607/corona_australis_1024.jpg" /></a>
<title> APOD: 2026 July 22 – The Corona Australis Cloud and the Chandelier Cluster</title>
The Southern Crown (Corona Australis) dazzles with young and ancient celestial jewels. 
<a href="https://apod.nasa.gov/apod/ap181129.html">The Corona Australis Cloud</a> 
is a collage of 
<a href="https://science.nasa.gov/universe/stories/quick-reads/decoding-nebulae/">reflection and emission nebulae</a> 
on the left of 
<a href="https://noirlab.edu/public/news/noirlab2617/?lang">today’s image</a>. 
At 430 light years away, this cloud is one of the closest 
<a href="https://science.nasa.gov/mission/webb/science-overview/science-explainers/webbs-star-formation-discoveries/">star-forming regions</a> 
to Earth. It contains gas cool enough (-260 Celsius or -440 Fahrenheit) to collapse into 
<a href="https://lco.global/spacebook/stars/protostar/">protostars</a>. 
Recently formed stars paint blue hues across the cloud as their light reflects off surrounding material. The waltz of the R Coronae Australis 
<a href="https://apod.nasa.gov/apod/ap970219.html">binary system</a> 
stirs up the nebula 
<a href="https://app.astrobin.com/i/2hti5p">NGC 6729</a>. 
The younger of the pair 
<a href="https://astronomy.swin.edu.au/cosmos/*/Ionisation">ionizes</a> 
nearby gas with its ultraviolet light, causing it to glow. 
<a href="https://science.nasa.gov/missions/hubble/hubble-spies-starry-chandelier/">The Chandelier Cluster</a> 
(NGC 6723) dangles from the top right, but is actually tens of thousands
of light years farther away than its apparent star-forming neighbor.
While NGC 6723 experienced multiple periods of star formation creating 
<a href="https://esahubble.org/images/potm2606a/"><i>slightly</i> younger</a> 
stars, the chandelier twinkles with stars almost as old as the universe.

	    ]]>
	</description>
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