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  <id>56</id>
  <title>Astronomy Picture of the Day [ko]</title>
  <updated>2026-06-26T20:05:03+00:00</updated>
  <author>
    <name>Unknown</name>
  </author>
  <link href="https://apod.nasa.gov/" rel="alternate"/>
  <generator uri="https://lkiesow.github.io/python-feedgen" version="1.0.0">python-feedgen</generator>
  <subtitle>Astronomy Picture of the Day</subtitle>
  <entry>
    <id>https://apod.nasa.gov/apod/ap260626.html</id>
    <title>Milky Way Urban Style</title>
    <updated>2026-06-26T03:00:00+00:00</updated>
    <author>
      <name>Jerry Bonnell (UMCP)</name>
    </author>
    <content type="html">&lt;img alt="See Explanation.  Clicking on the picture will download
the highest resolution version available." src="https://apod.nasa.gov/apod/image/2606/MilkyWaySeoulShingooLee800.jpg" /&gt;&lt;br /&gt;&lt;b&gt; Explanation: &lt;/b&gt; 

&lt;a href="https://apod.com/ap130411.html"&gt;In a cosmic vista&lt;/a&gt; you can never see, the
&lt;a href="https://www.nasa.gov/universe/galaxies/milky-way/"&gt;Milky Way&lt;/a&gt;
arcs through the night above Seoul, South Korea.

Remarkably, this
&lt;a href="https://www.instagram.com/leeshingoo/reel/DZhBG_nv03_/"&gt;urban night skyscape&lt;/a&gt;
reveals our galaxy's faintly luminous
central region and dark obscuring dust clouds in spite of the
&lt;a href="https://upload.wikimedia.org/wikipedia/commons/8/81/Seoul_%28175734251%29.jpeg"&gt;brilliant city lights&lt;/a&gt;.

To overcome the extreme
&lt;a href="https://www.earthdata.nasa.gov/dashboard/data-catalog/nighttime-lights-SE"&gt;light pollution&lt;/a&gt;
of the metropolitan area and record faint cosmic details,
an infrared filter was used to capture the night scene in a single exposure.

While the filter transmits predominately infrared light,
it still passes some
&lt;a href="https://apod.com/ap110716.html"&gt;visible light&lt;/a&gt;
to give the scene a natural appearance.

The view is from Seoul's Ttukseom Hangang Park,
with the Han River and a well lit railway bridge across the foreground.

The 123 story Lotte World Tower looms in the distance,
the tallest building in South Korea.</content>
    <link href="https://apod.nasa.gov/apod/ap260626.html"/>
    <summary type="html">&lt;img alt="See Explanation.  Clicking on the picture will download
the highest resolution version available." src="https://apod.nasa.gov/apod/image/2606/MilkyWaySeoulShingooLee800.jpg" /&gt;&lt;br /&gt;&lt;b&gt; Explanation: &lt;/b&gt; 

&lt;a href="https://apod.com/ap130411.html"&gt;In a cosmic vista&lt;/a&gt; you can never see, the
&lt;a href="https://www.nasa.gov/universe/galaxies/milky-way/"&gt;Milky Way&lt;/a&gt;
arcs through the night above Seoul, South Korea.

Remarkably, this
&lt;a href="https://www.instagram.com/leeshingoo/reel/DZhBG_nv03_/"&gt;urban night skyscape&lt;/a&gt;
reveals our galaxy's faintly luminous
central region and dark obscuring dust clouds in spite of the
&lt;a href="https://upload.wikimedia.org/wikipedia/commons/8/81/Seoul_%28175734251%29.jpeg"&gt;brilliant city lights&lt;/a&gt;.

To overcome the extreme
&lt;a href="https://www.earthdata.nasa.gov/dashboard/data-catalog/nighttime-lights-SE"&gt;light pollution&lt;/a&gt;
of the metropolitan area and record faint cosmic details,
an infrared filter was used to capture the night scene in a single exposure.

While the filter transmits predominately infrared light,
it still passes some
&lt;a href="https://apod.com/ap110716.html"&gt;visible light&lt;/a&gt;
to give the scene a natural appearance.

The view is from Seoul's Ttukseom Hangang Park,
with the Han River and a well lit railway bridge across the foreground.

The 123 story Lotte World Tower looms in the distance,
the tallest building in South Korea.</summary>
    <published>2026-06-26T03:00:00+00:00</published>
  </entry>
  <entry>
    <id>https://apod.nasa.gov/apod/ap260625.html</id>
    <title>Anticrepuscular Rays over Sicily</title>
    <updated>2026-06-25T03:00:00+00:00</updated>
    <author>
      <name>Jerry Bonnell (UMCP)</name>
    </author>
    <content type="html">&lt;img alt="A landscape with an open horizon shows
	    sunset color and coverging rays of light." src="https://apod.nasa.gov/apod/image/2606/crepuscular2_1024.jpg" /&gt;&lt;br /&gt;&lt;b&gt; Explanation: &lt;/b&gt;

    The &lt;a href="https://science.nasa.gov/sun/"&gt;Sun&lt;/a&gt; has just set... in the opposite side of the sky.

    Pictured &lt;a href="https://www.instagram.com/p/DZxl4R-gi73/?img_index=1"&gt;here&lt;/a&gt; are &lt;a href="https://en.wikipedia.org/wiki/Anticrepuscular_rays"&gt;anticrepuscular rays&lt;/a&gt; apparently converging in the east in this image of the &lt;a href="https://en.wikipedia.org/wiki/Geology_of_Sicily"&gt;limestone plateau&lt;/a&gt; in the heart of the &lt;a href="https://www.italia.it/en/sicily/hyblaean-mountains"&gt;Hyblaean Mountains&lt;/a&gt; of southeastern &lt;a href="https://en.wikipedia.org/wiki/Sicily"&gt;Sicily&lt;/a&gt;, in Italy.

    How were these anticrepuscular rays formed, if the Sun &lt;a href="https://images.unsplash.com/photo-1598398386929-4d5370672e9f"&gt;wasn't there&lt;/a&gt;?

    After the Sun set (in the west, as usual) its light still illuminated a &lt;a href="https://www.instagram.com/p/DZxl4R-gi73/?img_index=2"&gt;cloud&lt;/a&gt; higher up in the sky.

    Partially blocked by the cloud, the sunlight produced &lt;a href="https://apod.com/ap200318.html"&gt;patterns&lt;/a&gt; of light and shadow, crossing the sky in parallel lines.

    Perspective makes it look like they converge in the east, in the same way that &lt;a href="https://images.unsplash.com/photo-1588127727253-e5f2faf4f541"&gt;train tracks&lt;/a&gt; appear to meet in the distance.

    This effect can also happen at &lt;a href="https://apod.com/ap240921.html"&gt;sunrise&lt;/a&gt;, only the directions are exchanged.

    In &lt;a href="https://cloudappreciationsociety.org/cloud-library/anti-crepuscular-rays/"&gt;rare&lt;/a&gt; cases, both &lt;a href="https://apod.com/ap100811.html"&gt;crepuscular&lt;/a&gt; and anticrepuscular rays can be seen &lt;a href="https://earthsky.org/earth/how-to-see-anticrepuscular-rays/"&gt;at the same time&lt;/a&gt;.</content>
    <link href="https://apod.nasa.gov/apod/ap260625.html"/>
    <summary type="html">&lt;img alt="A landscape with an open horizon shows
	    sunset color and coverging rays of light." src="https://apod.nasa.gov/apod/image/2606/crepuscular2_1024.jpg" /&gt;&lt;br /&gt;&lt;b&gt; Explanation: &lt;/b&gt;

    The &lt;a href="https://science.nasa.gov/sun/"&gt;Sun&lt;/a&gt; has just set... in the opposite side of the sky.

    Pictured &lt;a href="https://www.instagram.com/p/DZxl4R-gi73/?img_index=1"&gt;here&lt;/a&gt; are &lt;a href="https://en.wikipedia.org/wiki/Anticrepuscular_rays"&gt;anticrepuscular rays&lt;/a&gt; apparently converging in the east in this image of the &lt;a href="https://en.wikipedia.org/wiki/Geology_of_Sicily"&gt;limestone plateau&lt;/a&gt; in the heart of the &lt;a href="https://www.italia.it/en/sicily/hyblaean-mountains"&gt;Hyblaean Mountains&lt;/a&gt; of southeastern &lt;a href="https://en.wikipedia.org/wiki/Sicily"&gt;Sicily&lt;/a&gt;, in Italy.

    How were these anticrepuscular rays formed, if the Sun &lt;a href="https://images.unsplash.com/photo-1598398386929-4d5370672e9f"&gt;wasn't there&lt;/a&gt;?

    After the Sun set (in the west, as usual) its light still illuminated a &lt;a href="https://www.instagram.com/p/DZxl4R-gi73/?img_index=2"&gt;cloud&lt;/a&gt; higher up in the sky.

    Partially blocked by the cloud, the sunlight produced &lt;a href="https://apod.com/ap200318.html"&gt;patterns&lt;/a&gt; of light and shadow, crossing the sky in parallel lines.

    Perspective makes it look like they converge in the east, in the same way that &lt;a href="https://images.unsplash.com/photo-1588127727253-e5f2faf4f541"&gt;train tracks&lt;/a&gt; appear to meet in the distance.

    This effect can also happen at &lt;a href="https://apod.com/ap240921.html"&gt;sunrise&lt;/a&gt;, only the directions are exchanged.

    In &lt;a href="https://cloudappreciationsociety.org/cloud-library/anti-crepuscular-rays/"&gt;rare&lt;/a&gt; cases, both &lt;a href="https://apod.com/ap100811.html"&gt;crepuscular&lt;/a&gt; and anticrepuscular rays can be seen &lt;a href="https://earthsky.org/earth/how-to-see-anticrepuscular-rays/"&gt;at the same time&lt;/a&gt;.</summary>
    <published>2026-06-25T03:00:00+00:00</published>
  </entry>
  <entry>
    <id>https://apod.nasa.gov/apod/ap260622.html</id>
    <title>M27: The Dumbbell Nebula</title>
    <updated>2026-06-22T03:00:00+00:00</updated>
    <author>
      <name>Jerry Bonnell (UMCP)</name>
    </author>
    <content type="html">&lt;img alt="A starfield surrounds a large and colorful nebula.
Red spokes poke out from the outside of the nebula in
some directions, while a blue haze appears in other
directions. The nebula center is multicolored. 
Please see the explanation for more detailed information." src="https://apod.nasa.gov/apod/image/2606/M27_antonucci_960.jpg" /&gt;&lt;br /&gt;&lt;b&gt; Explanation: &lt;/b&gt; 
Is this what will become of our Sun? Quite possibly. 

The first hint of our 
&lt;a href="https://science.nasa.gov/sun/"&gt;Sun&lt;/a&gt;'s future 
was discovered inadvertently in
&lt;a href="https://en.wikipedia.org/wiki/1764"&gt;1764&lt;/a&gt;.

At that time,
&lt;a href="https://en.wikipedia.org/wiki/Charles_Messier"&gt;Charles Messier&lt;/a&gt; was compiling a list
of diffuse objects not to be confused with comets.

The 27th object on
&lt;a href="http://www.seasky.org/astronomy/astronomy-messier.html"&gt;Messier's list&lt;/a&gt;, now known as
&lt;a href="https://apod.com/ap080626.html"&gt;M27&lt;/a&gt; or the Dumbbell Nebula, is a
&lt;a href="https://apod.com/planetary_nebulae.html"&gt;planetary nebula&lt;/a&gt;,
one of the brightest
&lt;a href="https://en.wikipedia.org/wiki/Planetary_nebula"&gt;planetary nebula&lt;/a&gt;s on the sky and visible with binoculars
toward the &lt;a href="https://spaceplace.nasa.gov/constellations/en/"&gt;constellation&lt;/a&gt; of the Fox (&lt;a href="https://en.wikipedia.org/wiki/Vulpecula"&gt;Vulpecula&lt;/a&gt;).

It takes light about 1000 years to reach us from M27, 
featured here in colors enhanced by red for  
&lt;a href="https://en.wikipedia.org/wiki/H-alpha"&gt;hydrogen&lt;/a&gt; 
and blue for 
&lt;a href="https://periodic.lanl.gov/8.shtml"&gt;oxygen&lt;/a&gt;.

We now know that in about 6 billion years, 
&lt;a href="https://apod.com/ap251207.html"&gt;our Sun&lt;/a&gt; will 
&lt;a href="https://en.wikipedia.org/wiki/Sun#After_core_hydrogen_exhaustion"&gt;shed its outer gases&lt;/a&gt; into a 
&lt;a href="https://en.wikipedia.org/wiki/Planetary_nebula#Morphology"&gt;planetary nebula&lt;/a&gt; like M27, 
while its remaining center will become an 
&lt;a href="https://science.nasa.gov/ems/11_xrays"&gt;X-ray&lt;/a&gt; hot 
&lt;a href="https://apod.com/ap000910.html"&gt;white dwarf&lt;/a&gt; star. 

Understanding the physics and significance of
&lt;a href="https://apod.nasa.gov/cgi-bin/apod/apod_search?tquery=M27"&gt;M27&lt;/a&gt; was well beyond 18th century science, though.

Even today, many things 
&lt;a href="https://s-media-cache-ak0.pinimg.com/originals/70/ce/c3/70cec30919aefe50ada3bd8e0e6239e6.jpg"&gt;remain mysterious&lt;/a&gt; about
&lt;a href="https://apod.com/ap230416.html"&gt;planetary nebulas&lt;/a&gt;, including &lt;a href="https://en.wikipedia.org/wiki/Planetary_nebula#Current_issues_in_planetary_nebula_studies"&gt;how&lt;/a&gt; their 
&lt;a href="https://apod.com/ap210425.html"&gt;intricate&lt;/a&gt; 
&lt;a href="https://apod.com/ap200721.html"&gt;shapes&lt;/a&gt; are created.</content>
    <link href="https://apod.nasa.gov/apod/ap260622.html"/>
    <summary type="html">&lt;img alt="A starfield surrounds a large and colorful nebula.
Red spokes poke out from the outside of the nebula in
some directions, while a blue haze appears in other
directions. The nebula center is multicolored. 
Please see the explanation for more detailed information." src="https://apod.nasa.gov/apod/image/2606/M27_antonucci_960.jpg" /&gt;&lt;br /&gt;&lt;b&gt; Explanation: &lt;/b&gt; 
Is this what will become of our Sun? Quite possibly. 

The first hint of our 
&lt;a href="https://science.nasa.gov/sun/"&gt;Sun&lt;/a&gt;'s future 
was discovered inadvertently in
&lt;a href="https://en.wikipedia.org/wiki/1764"&gt;1764&lt;/a&gt;.

At that time,
&lt;a href="https://en.wikipedia.org/wiki/Charles_Messier"&gt;Charles Messier&lt;/a&gt; was compiling a list
of diffuse objects not to be confused with comets.

The 27th object on
&lt;a href="http://www.seasky.org/astronomy/astronomy-messier.html"&gt;Messier's list&lt;/a&gt;, now known as
&lt;a href="https://apod.com/ap080626.html"&gt;M27&lt;/a&gt; or the Dumbbell Nebula, is a
&lt;a href="https://apod.com/planetary_nebulae.html"&gt;planetary nebula&lt;/a&gt;,
one of the brightest
&lt;a href="https://en.wikipedia.org/wiki/Planetary_nebula"&gt;planetary nebula&lt;/a&gt;s on the sky and visible with binoculars
toward the &lt;a href="https://spaceplace.nasa.gov/constellations/en/"&gt;constellation&lt;/a&gt; of the Fox (&lt;a href="https://en.wikipedia.org/wiki/Vulpecula"&gt;Vulpecula&lt;/a&gt;).

It takes light about 1000 years to reach us from M27, 
featured here in colors enhanced by red for  
&lt;a href="https://en.wikipedia.org/wiki/H-alpha"&gt;hydrogen&lt;/a&gt; 
and blue for 
&lt;a href="https://periodic.lanl.gov/8.shtml"&gt;oxygen&lt;/a&gt;.

We now know that in about 6 billion years, 
&lt;a href="https://apod.com/ap251207.html"&gt;our Sun&lt;/a&gt; will 
&lt;a href="https://en.wikipedia.org/wiki/Sun#After_core_hydrogen_exhaustion"&gt;shed its outer gases&lt;/a&gt; into a 
&lt;a href="https://en.wikipedia.org/wiki/Planetary_nebula#Morphology"&gt;planetary nebula&lt;/a&gt; like M27, 
while its remaining center will become an 
&lt;a href="https://science.nasa.gov/ems/11_xrays"&gt;X-ray&lt;/a&gt; hot 
&lt;a href="https://apod.com/ap000910.html"&gt;white dwarf&lt;/a&gt; star. 

Understanding the physics and significance of
&lt;a href="https://apod.nasa.gov/cgi-bin/apod/apod_search?tquery=M27"&gt;M27&lt;/a&gt; was well beyond 18th century science, though.

Even today, many things 
&lt;a href="https://s-media-cache-ak0.pinimg.com/originals/70/ce/c3/70cec30919aefe50ada3bd8e0e6239e6.jpg"&gt;remain mysterious&lt;/a&gt; about
&lt;a href="https://apod.com/ap230416.html"&gt;planetary nebulas&lt;/a&gt;, including &lt;a href="https://en.wikipedia.org/wiki/Planetary_nebula#Current_issues_in_planetary_nebula_studies"&gt;how&lt;/a&gt; their 
&lt;a href="https://apod.com/ap210425.html"&gt;intricate&lt;/a&gt; 
&lt;a href="https://apod.com/ap200721.html"&gt;shapes&lt;/a&gt; are created.</summary>
    <published>2026-06-22T03:00:00+00:00</published>
  </entry>
  <entry>
    <id>https://apod.nasa.gov/apod/ap260621.html</id>
    <title>Keogram: The Sky in 2025</title>
    <updated>2026-06-21T03:00:00+00:00</updated>
    <author>
      <name>Jerry Bonnell (UMCP)</name>
    </author>
    <content type="html">&lt;img alt="An image of the sky over the Netherlands
taken every 15 seconds during 2025. Visible are night, day,
solstices, equinoxes, moonglow, the blue hour, and more.
Please see the explanation for more detailed information." name="imagename1" src="https://apod.nasa.gov/apod/image/2606/Keogram2025_Bassa_960.jpg" /&gt;&lt;br /&gt;&lt;b&gt; Explanation: &lt;/b&gt; 
What if you could see the entire sky -- all at once -- for an entire year?

That, very nearly, is what is pictured here. 

Every 15 seconds during 2025, an 
&lt;a href="https://apod.com/ap011119.html"&gt;all-sky camera&lt;/a&gt; took an image of the sky over the 
&lt;a href="https://en.wikipedia.org/wiki/Netherlands"&gt;Netherlands&lt;/a&gt;.

Central 
&lt;a href="https://commons.wikimedia.org/wiki/File:Keogram_explainer.gif"&gt;columns&lt;/a&gt; from these images were then aligned 
and combined to create the featured
&lt;a href="https://victoriaweather.ca/keogram.php#:~:text=What%20is%20a%20keogram"&gt;keogram&lt;/a&gt;, with January at the top, 
December at the bottom, 
and the middle of the night 
running vertically just left of center.

&lt;a href="https://i1.sndcdn.com/artworks-000064777927-e3ahj5-t500x500.jpg"&gt;What do we see?&lt;/a&gt; 

Most obviously, the daytime 
&lt;a href="https://spaceplace.nasa.gov/blue-sky/en/"&gt;sky is mostly blue&lt;/a&gt;, while the nighttime sky is mostly black. 

The twelve 
&lt;a href="https://apod.com/ap220301.html"&gt;light bands&lt;/a&gt; 
crossing the night sky are caused by the 
&lt;a href="https://theskylive.com/how-bright-is-moon"&gt;glow&lt;/a&gt; of the 
&lt;a href="https://science.nasa.gov/moon/"&gt;Moon&lt;/a&gt;.

The thinnest 
&lt;a href="https://www.astron.nl/~bassa/keogram/"&gt;part&lt;/a&gt;
of the black hourglass shape occurs during the summer 
&lt;a href="https://svs.gsfc.nasa.gov/14366/"&gt;solstice&lt;/a&gt;, like 
&lt;a href="https://en.wikipedia.org/wiki/June_solstice"&gt;today&lt;/a&gt;, 
when days are the longest, while the thickest part occurs at the winter 
&lt;a href="https://apod.com/ap210620.html"&gt;solstice&lt;/a&gt;.

Equinoxes can also be located in the keogram, for example 
the northern-spring 
&lt;a href="https://apod.com/ap220320.html"&gt;equinox&lt;/a&gt; from one year ago is about 
three-quarters of the way up.</content>
    <link href="https://apod.nasa.gov/apod/ap260621.html"/>
    <summary type="html">&lt;img alt="An image of the sky over the Netherlands
taken every 15 seconds during 2025. Visible are night, day,
solstices, equinoxes, moonglow, the blue hour, and more.
Please see the explanation for more detailed information." name="imagename1" src="https://apod.nasa.gov/apod/image/2606/Keogram2025_Bassa_960.jpg" /&gt;&lt;br /&gt;&lt;b&gt; Explanation: &lt;/b&gt; 
What if you could see the entire sky -- all at once -- for an entire year?

That, very nearly, is what is pictured here. 

Every 15 seconds during 2025, an 
&lt;a href="https://apod.com/ap011119.html"&gt;all-sky camera&lt;/a&gt; took an image of the sky over the 
&lt;a href="https://en.wikipedia.org/wiki/Netherlands"&gt;Netherlands&lt;/a&gt;.

Central 
&lt;a href="https://commons.wikimedia.org/wiki/File:Keogram_explainer.gif"&gt;columns&lt;/a&gt; from these images were then aligned 
and combined to create the featured
&lt;a href="https://victoriaweather.ca/keogram.php#:~:text=What%20is%20a%20keogram"&gt;keogram&lt;/a&gt;, with January at the top, 
December at the bottom, 
and the middle of the night 
running vertically just left of center.

&lt;a href="https://i1.sndcdn.com/artworks-000064777927-e3ahj5-t500x500.jpg"&gt;What do we see?&lt;/a&gt; 

Most obviously, the daytime 
&lt;a href="https://spaceplace.nasa.gov/blue-sky/en/"&gt;sky is mostly blue&lt;/a&gt;, while the nighttime sky is mostly black. 

The twelve 
&lt;a href="https://apod.com/ap220301.html"&gt;light bands&lt;/a&gt; 
crossing the night sky are caused by the 
&lt;a href="https://theskylive.com/how-bright-is-moon"&gt;glow&lt;/a&gt; of the 
&lt;a href="https://science.nasa.gov/moon/"&gt;Moon&lt;/a&gt;.

The thinnest 
&lt;a href="https://www.astron.nl/~bassa/keogram/"&gt;part&lt;/a&gt;
of the black hourglass shape occurs during the summer 
&lt;a href="https://svs.gsfc.nasa.gov/14366/"&gt;solstice&lt;/a&gt;, like 
&lt;a href="https://en.wikipedia.org/wiki/June_solstice"&gt;today&lt;/a&gt;, 
when days are the longest, while the thickest part occurs at the winter 
&lt;a href="https://apod.com/ap210620.html"&gt;solstice&lt;/a&gt;.

Equinoxes can also be located in the keogram, for example 
the northern-spring 
&lt;a href="https://apod.com/ap220320.html"&gt;equinox&lt;/a&gt; from one year ago is about 
three-quarters of the way up.</summary>
    <published>2026-06-21T03:00:00+00:00</published>
  </entry>
  <entry>
    <id>https://apod.nasa.gov/apod/ap260620.html</id>
    <title>Daytime Moon Meets Evening Star</title>
    <updated>2026-06-20T03:00:00+00:00</updated>
    <author>
      <name>Jerry Bonnell (UMCP)</name>
    </author>
    <content type="html">&lt;img alt="See Explanation.  Clicking on the picture will download
the highest resolution version available." src="https://apod.nasa.gov/apod/image/2606/Venus_Moon_2026_06_17_1024.jpg" /&gt;&lt;br /&gt;&lt;b&gt; Explanation: &lt;/b&gt; 

Venus is now appearing on
&lt;a href="https://science.nasa.gov/solar-system/whats-up-june-2026-skywatching-tips-from-nasa/"&gt;the celestial stage&lt;/a&gt;
as Earth's brilliant evening star, performing with
the Moon, other wandering planets, and bright stars
in western skies.

&lt;a href="https://earthsky.org/astronomy-essentials/visible-planets-tonight-mars-jupiter-venus-saturn-mercury/"&gt;For evening sky gazers&lt;/a&gt;
on June 17, the celestial beacon rose after sunset close by
a young, slender, crescent Moon.

&lt;a href="https://in-the-sky.org/news.php?id=20260617_16_100"&gt;But from some locations&lt;/a&gt; the Moon could be seen to occult or pass in
front of Venus.

And from a backyard observatory in
southern British Columbia, Canada, the
lunar occultation was played out in daylight.

This stunning telescopic snapshot captured
&lt;a href="https://app.astrobin.com/u/debraceravolo?i=geo4yx"&gt;a scene in dramatically cloudy skies&lt;/a&gt;,
following Venus' hour long disappearance,
as the evening star emerged beyond the bright lunar limb.</content>
    <link href="https://apod.nasa.gov/apod/ap260620.html"/>
    <summary type="html">&lt;img alt="See Explanation.  Clicking on the picture will download
the highest resolution version available." src="https://apod.nasa.gov/apod/image/2606/Venus_Moon_2026_06_17_1024.jpg" /&gt;&lt;br /&gt;&lt;b&gt; Explanation: &lt;/b&gt; 

Venus is now appearing on
&lt;a href="https://science.nasa.gov/solar-system/whats-up-june-2026-skywatching-tips-from-nasa/"&gt;the celestial stage&lt;/a&gt;
as Earth's brilliant evening star, performing with
the Moon, other wandering planets, and bright stars
in western skies.

&lt;a href="https://earthsky.org/astronomy-essentials/visible-planets-tonight-mars-jupiter-venus-saturn-mercury/"&gt;For evening sky gazers&lt;/a&gt;
on June 17, the celestial beacon rose after sunset close by
a young, slender, crescent Moon.

&lt;a href="https://in-the-sky.org/news.php?id=20260617_16_100"&gt;But from some locations&lt;/a&gt; the Moon could be seen to occult or pass in
front of Venus.

And from a backyard observatory in
southern British Columbia, Canada, the
lunar occultation was played out in daylight.

This stunning telescopic snapshot captured
&lt;a href="https://app.astrobin.com/u/debraceravolo?i=geo4yx"&gt;a scene in dramatically cloudy skies&lt;/a&gt;,
following Venus' hour long disappearance,
as the evening star emerged beyond the bright lunar limb.</summary>
    <published>2026-06-20T03:00:00+00:00</published>
  </entry>
  <entry>
    <id>https://apod.nasa.gov/apod/ap260619.html</id>
    <title>Starry Night II</title>
    <updated>2026-06-19T03:00:00+00:00</updated>
    <author>
      <name>Jerry Bonnell (UMCP)</name>
    </author>
    <content type="html">&lt;img alt="A sunset sky is seen above a dark sloping horizon. A tall
tree is on the left. The sky is partly cloudy with a crescent
Moon on the upper right and a bright planet just to the right
of the tree. Next to the tree in the foreground on the right
is an easel showing the famous van Gogh painting Starry Night.
Please see the explanation for more detailed information." name="imagename1" src="https://apod.nasa.gov/apod/image/2606/StarryNight2_Guerra_960.jpg" /&gt;&lt;br /&gt;&lt;b&gt; Explanation: &lt;/b&gt; 
Does this scene look familiar?

It is a modern recreation of the famous painting 
&lt;a href="https://apod.com/ap191023.html"&gt;Starry Night&lt;/a&gt; by 
&lt;a href="https://en.wikipedia.org/wiki/Vincent_van_Gogh"&gt;Vincent van Gogh&lt;/a&gt;. 

Both 
&lt;a href="https://www.instagram.com/p/DX2Hp-OmsW8/"&gt;the image&lt;/a&gt; and the painting depict a tall tree on the left, 
a &lt;a href="https://science.nasa.gov/moon/moon-phases/"&gt;crescent moon&lt;/a&gt; on the upper right, 
the &lt;a href="https://science.nasa.gov/venus/"&gt;planet Venus&lt;/a&gt; 
just to the right of the tree, 
a foreground horizon rising from left to right, 
and &lt;a href="https://apod.com/ap250817.html"&gt;clouds&lt;/a&gt; above the horizon.

Differences include that the photograph was taken in mid-April earlier this year in 
&lt;a href="https://youtu.be/7t8oTjc7Y-M"&gt;Cascavel&lt;/a&gt;, 
&lt;a href="https://en.wikipedia.org/wiki/Brazil"&gt;Brazil&lt;/a&gt;, 
while the painting was composed in 
&lt;a href="https://youtu.be/JlcMFjwFHVA"&gt;Saint-Rémy-de-Provence&lt;/a&gt;, 
&lt;a href="https://en.wikipedia.org/wiki/France"&gt;France&lt;/a&gt;, in 1889. 

The &lt;a href="https://www.moma.org/collection/works/79802"&gt;original Starry Night&lt;/a&gt; is considered by many to be one of the three 
&lt;a href="https://www.nguyenartgallery.com/top-100-most-world-famous-paintings/"&gt;most famous paintings&lt;/a&gt; in the world today 
and a statement about the 
&lt;a href="https://www.reddit.com/r/aww/comments/2jqsdk/the_omg_cat/#lightbox"&gt;wonders&lt;/a&gt; of the night sky.

Today is (roughly) the 
&lt;a href="https://samsoriginalart.com/blogs/art/starry-night-facts-about-van-goghs-masterpiece"&gt;anniversary&lt;/a&gt; of the morning that 
van Gogh saw the sky that he later painted in 
&lt;a href="https://www.vangoghgallery.com/painting/starry-night.html"&gt;his version of Starry Night&lt;/a&gt;.</content>
    <link href="https://apod.nasa.gov/apod/ap260619.html"/>
    <summary type="html">&lt;img alt="A sunset sky is seen above a dark sloping horizon. A tall
tree is on the left. The sky is partly cloudy with a crescent
Moon on the upper right and a bright planet just to the right
of the tree. Next to the tree in the foreground on the right
is an easel showing the famous van Gogh painting Starry Night.
Please see the explanation for more detailed information." name="imagename1" src="https://apod.nasa.gov/apod/image/2606/StarryNight2_Guerra_960.jpg" /&gt;&lt;br /&gt;&lt;b&gt; Explanation: &lt;/b&gt; 
Does this scene look familiar?

It is a modern recreation of the famous painting 
&lt;a href="https://apod.com/ap191023.html"&gt;Starry Night&lt;/a&gt; by 
&lt;a href="https://en.wikipedia.org/wiki/Vincent_van_Gogh"&gt;Vincent van Gogh&lt;/a&gt;. 

Both 
&lt;a href="https://www.instagram.com/p/DX2Hp-OmsW8/"&gt;the image&lt;/a&gt; and the painting depict a tall tree on the left, 
a &lt;a href="https://science.nasa.gov/moon/moon-phases/"&gt;crescent moon&lt;/a&gt; on the upper right, 
the &lt;a href="https://science.nasa.gov/venus/"&gt;planet Venus&lt;/a&gt; 
just to the right of the tree, 
a foreground horizon rising from left to right, 
and &lt;a href="https://apod.com/ap250817.html"&gt;clouds&lt;/a&gt; above the horizon.

Differences include that the photograph was taken in mid-April earlier this year in 
&lt;a href="https://youtu.be/7t8oTjc7Y-M"&gt;Cascavel&lt;/a&gt;, 
&lt;a href="https://en.wikipedia.org/wiki/Brazil"&gt;Brazil&lt;/a&gt;, 
while the painting was composed in 
&lt;a href="https://youtu.be/JlcMFjwFHVA"&gt;Saint-Rémy-de-Provence&lt;/a&gt;, 
&lt;a href="https://en.wikipedia.org/wiki/France"&gt;France&lt;/a&gt;, in 1889. 

The &lt;a href="https://www.moma.org/collection/works/79802"&gt;original Starry Night&lt;/a&gt; is considered by many to be one of the three 
&lt;a href="https://www.nguyenartgallery.com/top-100-most-world-famous-paintings/"&gt;most famous paintings&lt;/a&gt; in the world today 
and a statement about the 
&lt;a href="https://www.reddit.com/r/aww/comments/2jqsdk/the_omg_cat/#lightbox"&gt;wonders&lt;/a&gt; of the night sky.

Today is (roughly) the 
&lt;a href="https://samsoriginalart.com/blogs/art/starry-night-facts-about-van-goghs-masterpiece"&gt;anniversary&lt;/a&gt; of the morning that 
van Gogh saw the sky that he later painted in 
&lt;a href="https://www.vangoghgallery.com/painting/starry-night.html"&gt;his version of Starry Night&lt;/a&gt;.</summary>
    <published>2026-06-19T03:00:00+00:00</published>
  </entry>
  <entry>
    <id>https://apod.nasa.gov/apod/ap260618.html</id>
    <title>Possible Supernova Remnant in Galactic Center</title>
    <updated>2026-06-18T03:00:00+00:00</updated>
    <author>
      <name>Jerry Bonnell (UMCP)</name>
    </author>
    <content type="html">&lt;img alt="A composite image shows a field of stars on a dark background,
	  together X-rays in blue and radio in red" src="https://apod.nasa.gov/apod/image/2606/sgrc.jpg" /&gt;&lt;br /&gt;&lt;b&gt; Explanation: &lt;/b&gt;

    Do you see that blue blob to the lower right of the image center?

    Astronomers think that it shows where a massive star &lt;a href="https://en.wikipedia.org/wiki/Type_II_supernova"&gt;exploded&lt;/a&gt; as a supernova whose light reached Earth &lt;a href="https://iopscience.iop.org/article/10.3847/1538-4357/ae547c"&gt;1,700 years ago&lt;/a&gt;.

    The &lt;a href="https://chandra.si.edu/photo/2026/sgrc/"&gt;image&lt;/a&gt; combines optical data from the &lt;a href="https://www2.ifa.hawaii.edu/research/Pan-STARRS.shtml"&gt;PanSTARRS&lt;/a&gt; telescopes in Hawaii (background stars in red, green, and blue), radio from the &lt;a href="https://www.sarao.ac.za/science/meerkat/"&gt;MeerKAT&lt;/a&gt; telescope in South Africa (large red cloud) and X-rays from &lt;a href="https://www.nasa.gov/"&gt;NASA&lt;/a&gt;'s &lt;a href="https://science.nasa.gov/mission/chandra/"&gt;Chandra X-ray Observatory&lt;/a&gt; and &lt;a href="https://www.esa.int/"&gt;ESA&lt;/a&gt;’s &lt;a href="https://www.cosmos.esa.int/web/xmm-newton"&gt;XMM-Newton&lt;/a&gt; (shown in blue).

    The large cloud is a &lt;a href="https://science.nasa.gov/mission/hubble/science/science-highlights/exploring-the-birth-of-stars/"&gt;star forming region&lt;/a&gt; called &lt;a href="https://en.wikipedia.org/wiki/Sagittarius_C"&gt;Sagittarius C&lt;/a&gt;, which is approximately 50 &lt;a href="https://science.nasa.gov/exoplanets/what-is-a-light-year/"&gt;light-years&lt;/a&gt; in extent and about 26,000 light-years from &lt;a href="https://apod.com/ap220206.html"&gt;Earth&lt;/a&gt;.

    It is located only about 260 light-years from the &lt;a href="https://apod.com/ap220513.html"&gt;supermassive black hole&lt;/a&gt; in the center of the Galaxy (off to the &lt;a href="https://apod.com/ap190708.html"&gt;left&lt;/a&gt; of the image).

    If the &lt;a href="https://images.unsplash.com/photo-1508311603478-ce574376c3cf"&gt;blue blob&lt;/a&gt; is confirmed to be a &lt;a href="https://imagine.gsfc.nasa.gov/science/objects/supernova_remnants.html"&gt;supernova remnant&lt;/a&gt;, it would be one of the closest ever discovered to the &lt;a href="https://science.nasa.gov/asset/webb/galactic-center-chandra-hubble-spitzer/"&gt;Galactic Center&lt;/a&gt;.

    In this &lt;a href="https://science.nasa.gov/asset/webb/sagittarius-c-nircam-image/"&gt;dense region&lt;/a&gt;, the deaths of massive stars are connected to the birth of new stars through gas and magnetic fields in a complex way.</content>
    <link href="https://apod.nasa.gov/apod/ap260618.html"/>
    <summary type="html">&lt;img alt="A composite image shows a field of stars on a dark background,
	  together X-rays in blue and radio in red" src="https://apod.nasa.gov/apod/image/2606/sgrc.jpg" /&gt;&lt;br /&gt;&lt;b&gt; Explanation: &lt;/b&gt;

    Do you see that blue blob to the lower right of the image center?

    Astronomers think that it shows where a massive star &lt;a href="https://en.wikipedia.org/wiki/Type_II_supernova"&gt;exploded&lt;/a&gt; as a supernova whose light reached Earth &lt;a href="https://iopscience.iop.org/article/10.3847/1538-4357/ae547c"&gt;1,700 years ago&lt;/a&gt;.

    The &lt;a href="https://chandra.si.edu/photo/2026/sgrc/"&gt;image&lt;/a&gt; combines optical data from the &lt;a href="https://www2.ifa.hawaii.edu/research/Pan-STARRS.shtml"&gt;PanSTARRS&lt;/a&gt; telescopes in Hawaii (background stars in red, green, and blue), radio from the &lt;a href="https://www.sarao.ac.za/science/meerkat/"&gt;MeerKAT&lt;/a&gt; telescope in South Africa (large red cloud) and X-rays from &lt;a href="https://www.nasa.gov/"&gt;NASA&lt;/a&gt;'s &lt;a href="https://science.nasa.gov/mission/chandra/"&gt;Chandra X-ray Observatory&lt;/a&gt; and &lt;a href="https://www.esa.int/"&gt;ESA&lt;/a&gt;’s &lt;a href="https://www.cosmos.esa.int/web/xmm-newton"&gt;XMM-Newton&lt;/a&gt; (shown in blue).

    The large cloud is a &lt;a href="https://science.nasa.gov/mission/hubble/science/science-highlights/exploring-the-birth-of-stars/"&gt;star forming region&lt;/a&gt; called &lt;a href="https://en.wikipedia.org/wiki/Sagittarius_C"&gt;Sagittarius C&lt;/a&gt;, which is approximately 50 &lt;a href="https://science.nasa.gov/exoplanets/what-is-a-light-year/"&gt;light-years&lt;/a&gt; in extent and about 26,000 light-years from &lt;a href="https://apod.com/ap220206.html"&gt;Earth&lt;/a&gt;.

    It is located only about 260 light-years from the &lt;a href="https://apod.com/ap220513.html"&gt;supermassive black hole&lt;/a&gt; in the center of the Galaxy (off to the &lt;a href="https://apod.com/ap190708.html"&gt;left&lt;/a&gt; of the image).

    If the &lt;a href="https://images.unsplash.com/photo-1508311603478-ce574376c3cf"&gt;blue blob&lt;/a&gt; is confirmed to be a &lt;a href="https://imagine.gsfc.nasa.gov/science/objects/supernova_remnants.html"&gt;supernova remnant&lt;/a&gt;, it would be one of the closest ever discovered to the &lt;a href="https://science.nasa.gov/asset/webb/galactic-center-chandra-hubble-spitzer/"&gt;Galactic Center&lt;/a&gt;.

    In this &lt;a href="https://science.nasa.gov/asset/webb/sagittarius-c-nircam-image/"&gt;dense region&lt;/a&gt;, the deaths of massive stars are connected to the birth of new stars through gas and magnetic fields in a complex way.</summary>
    <published>2026-06-18T03:00:00+00:00</published>
  </entry>
</feed>
