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  <id>56</id>
  <title>Astronomy Picture of the Day [ko]</title>
  <updated>2026-07-01T20:05:05+00:00</updated>
  <author>
    <name>Unknown</name>
  </author>
  <link href="https://apod.nasa.gov/" rel="alternate"/>
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  <subtitle>Astronomy Picture of the Day</subtitle>
  <entry>
    <id>https://apod.nasa.gov/apod/ap260702.html</id>
    <title>Sibling Supernova Remnants</title>
    <updated>2026-07-02T03:00:00+00:00</updated>
    <author>
      <name>Jerry Bonnell (UMCP)</name>
    </author>
    <content type="html">&lt;img alt="Against a bright field of stars, a yellow nebula with blue details,
	  a purple filament on the left and a bright star on the right." src="https://apod.nasa.gov/apod/image/2607/sibling_supernovae_1024.jpg" /&gt;&lt;br /&gt;&lt;b&gt; Explanation: &lt;/b&gt;

    What happens when one of the stars in a  &lt;a href="https://science.nasa.gov/universe/stars/multiple-star-systems/"&gt;binary&lt;/a&gt; goes supernova?

    This &lt;a href="https://science.nasa.gov/missions/fermi/nasas-fermi-sibling-supernova-remnants/"&gt;image&lt;/a&gt; combines visible (yellow), ultraviolet (purple) and infrared light (cyan, red and orange) to show two &lt;a href="https://apod.com/ap260206.html"&gt;supernova remnants&lt;/a&gt; and their surrounding environment, about 6,000 light-years away.

    The younger one is the well-known &lt;a href="https://apod.com/ap231226.html"&gt;Jellyfish Nebula&lt;/a&gt; in the center (mostly in yellow).

    If we could see it by eye, it would appear &lt;a href="https://en.wikipedia.org/wiki/IC_443"&gt;larger than the full moon&lt;/a&gt; in the sky.

    The filament shown in purple is part of an older, overlapping supernova remnant, &lt;a href="https://arxiv.org/pdf/2007.03226"&gt;G189.6+3.3&lt;/a&gt;.

    A &lt;a href="https://ui.adsabs.harvard.edu/abs/2026AAS...24743307M/abstract"&gt;new study&lt;/a&gt; used data from &lt;a href="https://www.nasa.gov/"&gt;NASA&lt;/a&gt;'s &lt;a href="https://science.nasa.gov/mission/fermi/"&gt;Fermi Gamma-ray Space Telescope&lt;/a&gt; to piece together their &lt;a href="https://humsci.stanford.edu/feature/researchers-uncover-evidence-sibling-supernovas"&gt;story&lt;/a&gt;.

    Astronomers believe that there were two stars in a binary system, then the first one exploded as a supernova, &lt;a href="https://images.unsplash.com/vector-1741055269495-7abf86aab37a"&gt;kicking&lt;/a&gt; away its companion, which also exploded as a supernova tens of thousands of years later, creating the superimposed supernova remnants we see today.

    The bright star on the right is actually a triple star system named &lt;a href="https://en.wikipedia.org/wiki/Eta_Geminorum"&gt;Propus&lt;/a&gt;.</content>
    <link href="https://apod.nasa.gov/apod/ap260702.html"/>
    <summary type="html">What happens when one of the stars in a  binary goes supernova?

    This image combines visible (yellow), ultraviolet (purple) and infrared light (cyan, red and orange) to show two supernova remnants and their surrounding environment, about 6,000 light-years away</summary>
    <published>2026-07-02T03:00:00+00:00</published>
  </entry>
  <entry>
    <id>https://apod.nasa.gov/apod/ap260701.html</id>
    <title>The Cotton Candy Clouds of Rho Ophiuchi</title>
    <updated>2026-07-01T03:00:00+00:00</updated>
    <author>
      <name>Jerry Bonnell (UMCP)</name>
    </author>
    <content type="html">&lt;img alt="A handful of different types of clouds splatter across the image, with bright stars embedded within. Dust blocks some parts of the clouds. Many small stars cover the background, with a cluster of them sitting in the bottom right beneath all the clouds." src="https://apod.nasa.gov/apod/image/2607/rho_ophiuchi_800.jpg" /&gt;&lt;br /&gt;&lt;b&gt; Explanation: &lt;/b&gt; 
Although they look like cotton candy, you cannot eat these clouds! Taken in 
&lt;a href="https://www.youtube.com/watch?v=kH4w3Ev2uKg"&gt;Cádiz, Spain&lt;/a&gt;, 
&lt;a href="https://www.instagram.com/p/DZ0HKvRDNbW/"&gt;today's image&lt;/a&gt; 
features 
&lt;a href="https://apod.com/ap251025.html"&gt;the Rho Ophiuchi complex&lt;/a&gt;, 
a rich tapestry of young and old astronomical phenomena. This colorful cloud complex is a 
nearby star-forming region containing hundreds of 
&lt;a href="https://en.wikipedia.org/wiki/Young_stellar_object"&gt;young stellar objects&lt;/a&gt;, 
including 
&lt;a href="https://apod.com/ap250313.html"&gt;protostars&lt;/a&gt; and 
&lt;a href="https://astronomy.swin.edu.au/cosmos/T/T+Tauri+Stars"&gt;T Tauri stars&lt;/a&gt;. 
Light from 
&lt;a href="https://en.wikipedia.org/wiki/The_Three-Body_Problem_(novel)"&gt;the triple star system&lt;/a&gt; 
at its center 
&lt;a href="https://science.nasa.gov/ems/03_behaviors/"&gt;reflects&lt;/a&gt; 
off of small dust grains to create the blue 
&lt;a href="https://science.nasa.gov/universe/stories/quick-reads/decoding-nebulae/"&gt;reflection nebula&lt;/a&gt;. 
&lt;a href="https://science.nasa.gov/ems/10_ultravioletwaves/"&gt;Ultraviolet&lt;/a&gt; 
light from hot stars 
&lt;a href="https://astronomy.swin.edu.au/cosmos/i/Ionisation"&gt;ionizes&lt;/a&gt; 
the surrounding hydrogen gas, creating the red 
&lt;a href="https://apod.com/ap251021.html"&gt;emission nebula&lt;/a&gt;. 
&lt;a href="https://apod.com/ap250611.html"&gt;Antares&lt;/a&gt;, 
&lt;a href="https://theplanets.org/red-supergiant-star-facts/"&gt;a red supergiant&lt;/a&gt; 
big enough to engulf the Solar System’s 
&lt;a href="https://science.nasa.gov/asset/webb/asteroid-belts-illustration/"&gt;asteroid belt&lt;/a&gt;, 
lights up the yellow region. Dark 
&lt;a href="https://science.nasa.gov/universe/dust-in-the-stellar-wind-a-cosmological-primer/"&gt;interstellar dust&lt;/a&gt; 
blocks some of the complex’s color. Recent 
&lt;a href="https://www.youtube.com/watch?v=U3X8rZtVJOQ"&gt;JWST observations&lt;/a&gt; 
exhibit shadows cast by hidden 
&lt;a href="https://esawebb.org/wordbank/circumstellar-disc/"&gt;circumstellar disks&lt;/a&gt;, 
the beginning stages of planet formation. 
&lt;a href="https://science.nasa.gov/mission/hubble/science/explore-the-night-sky/hubble-messier-catalog/messier-4/"&gt;Messier 4&lt;/a&gt;, 
a globular cluster almost as old as the universe, sits in the bottom right and witnesses yet 
another chaotic burst of youth in the Milky Way.</content>
    <link href="https://apod.nasa.gov/apod/ap260701.html"/>
    <summary type="html">Although they look like cotton candy, you cannot eat these clouds! Taken in 
Cádiz, Spain, 
today's image 
features 
the Rho Ophiuchi complex, 
a rich tapestry of young and old astronomical phenomena</summary>
    <published>2026-07-01T03:00:00+00:00</published>
  </entry>
  <entry>
    <id>https://apod.nasa.gov/apod/ap260630.html</id>
    <title>Unusually Smooth Sections of Asteroid Itokawa</title>
    <updated>2026-06-30T03:00:00+00:00</updated>
    <author>
      <name>Jerry Bonnell (UMCP)</name>
    </author>
    <content type="html">&lt;img alt="Dark space surrounds a gray peanut sized object.
The object has a surface that has many rough nodules
but also some relatively smooth sections. 
Please see the explanation for more detailed information." src="https://apod.nasa.gov/apod/image/2606/itokawa07_hayabusa_1080.jpg" /&gt;&lt;br /&gt;&lt;b&gt; Explanation: &lt;/b&gt; 
Why are parts of this asteroid's surface so smooth? 

The answer seems likely to do with the dynamics of an 
&lt;a href="https://science.nasa.gov/solar-system/asteroids/"&gt;asteroid&lt;/a&gt; that is a loose 
&lt;a href="https://daviddarling.info/encyclopedia/R/rubble-pile_asteroid.html"&gt;pile of rubble&lt;/a&gt; rather than a solid rock. 

The &lt;a href="https://apod.com/ap051116.html"&gt;unusual asteroid&lt;/a&gt; 
&lt;a href="https://science.nasa.gov/solar-system/asteroids/25143-itokawa/"&gt;Itokawa&lt;/a&gt; was visited by the 
&lt;a href="https://user.iiasa.ac.at/~marek/fbook/01/geos/ja.html"&gt;Japan&lt;/a&gt;ese spacecraft 
&lt;a href="https://science.nasa.gov/mission/hayabusa/"&gt;Hayabusa&lt;/a&gt; in 2005 which imaged and 
documented its unusual structure and mysterious 
&lt;a href="https://apod.com/ap051121.html"&gt;lack of craters&lt;/a&gt;. 

&lt;a href="https://www.science.org/doi/10.1126/science.1134390"&gt;Analyses of the border regions&lt;/a&gt; between smooth and rugged sections indicate that jostling of the asteroid might be creating segregation between large and small rocks near the surface, like the 
&lt;a href="https://en.wikipedia.org/wiki/Granular_convection"&gt;Brazil nut effect&lt;/a&gt;. 

The robotic Hayabusa actually 
&lt;a href="https://apod.com/ap190312.html"&gt;touched down&lt;/a&gt; 
on one of the smooth patches, dubbed the 
&lt;a href="https://global.jaxa.jp/article/special/hayabusa_sp3/p2_e.html"&gt;MUSES Sea&lt;/a&gt;, and collected 
&lt;a href="https://www.planetary.org/articles/3191"&gt;soil samples&lt;/a&gt;.

These samples were 
&lt;a href="https://global.jaxa.jp/article/special/hayabusa/index_e.html"&gt;returned to Earth&lt;/a&gt; and are not only 
giving clues to the ancient history of 
&lt;a href="https://apod.com/ap100619.html"&gt;this unusual asteroid&lt;/a&gt;, 
but also about the early years of our entire 
&lt;a href="https://eyes.nasa.gov/apps/solar-system/#/home"&gt;Solar System&lt;/a&gt;.

Computer simulations show that 500-meter &lt;a href="https://www.esa.int/ESA_Multimedia/Videos/2017/04/Visualisation_of_asteroid_Itokawa/(lang)"&gt;asteroid Itokawa&lt;/a&gt; may 
&lt;a href="https://i.ytimg.com/vi/1Kl4rNUTWCA/hqdefault.jpg"&gt;impact the Earth&lt;/a&gt; within the next few million years.</content>
    <link href="https://apod.nasa.gov/apod/ap260630.html"/>
    <summary type="html">Why are parts of this asteroid's surface so smooth? 

The answer seems likely to do with the dynamics of an 
asteroid that is a loose 
pile of rubble rather than a solid rock</summary>
    <published>2026-06-30T03:00:00+00:00</published>
  </entry>
  <entry>
    <id>https://apod.nasa.gov/apod/ap260629.html</id>
    <title>M82: Galaxy with a Supergalactic Wind</title>
    <updated>2026-06-29T03:00:00+00:00</updated>
    <author>
      <name>Jerry Bonnell (UMCP)</name>
    </author>
    <content type="html">&lt;img alt="A starfield surrounds an unusual object with 
a band of diffuse white crossing horizontally.
Emanating out from the band toward both the top
and the bottom of the frame is an orange and red
nebula.  
Please see the explanation for more detailed information." src="https://apod.nasa.gov/apod/image/2606/M82_HubbleWebb_960.jpg" /&gt;&lt;br /&gt;&lt;b&gt; Explanation: &lt;/b&gt; 
Why is the Cigar Galaxy billowing red smoke? 

&lt;a href="https://en.wikipedia.org/wiki/Messier_82"&gt;M82&lt;/a&gt;, as this
&lt;a href="https://en.wikipedia.org/wiki/Starburst_galaxy"&gt;starburst galaxy&lt;/a&gt; is also known, was stirred up by a
&lt;a href="https://apod.com/ap250507.html"&gt;recent pass&lt;/a&gt; near large
&lt;a href="https://apod.com/spiral_galaxies.html"&gt;spiral&lt;/a&gt; galaxy
&lt;a href="https://apod.com/ap250327.html"&gt;M81&lt;/a&gt;.  

This doesn't fully 
&lt;a href="https://apod.com/ap240415.html"&gt;explain&lt;/a&gt; 
the source of the red-glowing outwardly
&lt;a href="https://youtu.be/WOLUDpYhzp0?t=34"&gt;expanding gas&lt;/a&gt; and dust, however.  

&lt;a href="https://ui.adsabs.harvard.edu/abs/1999ApJ...523..575L/abstract"&gt;Evidence&lt;/a&gt; indicates that this gas and dust is being
driven out by the combined emerging
&lt;a href="https://science.nasa.gov/science-news/news-articles/effects-of-the-solar-wind"&gt;particle winds&lt;/a&gt; of many stars, together creating a galactic
&lt;a href="http://ned.ipac.caltech.edu/level5/March01/Heckman/frames.html"&gt;superwind&lt;/a&gt;.  

The dust particles are 
&lt;a href="https://ui.adsabs.harvard.edu/abs/2019PASJ...71...87Y/abstract"&gt;thought to originate&lt;/a&gt; 
in M82's interstellar medium and are actually 
&lt;a href="https://www.jstor.org/stable/26058972"&gt;similar in size&lt;/a&gt; to particles in cigar smoke. 

The &lt;a href="https://science.nasa.gov/asset/webb/m82-cigar-galaxy-webb-hubble/"&gt;featured photographic mosaic&lt;/a&gt; combines images taken in 
&lt;a href="https://science.nasa.gov/ems/09_visiblelight/"&gt;visible light&lt;/a&gt; from the 
&lt;a href="https://science.nasa.gov/mission/hubble/"&gt;Hubble Space Telescope&lt;/a&gt; and images taken in 
&lt;a href="https://science.nasa.gov/ems/07_infraredwaves/"&gt;infrared light&lt;/a&gt; from 
&lt;a href="https://science.nasa.gov/mission/webb/"&gt;James Webb Space Telescope&lt;/a&gt;. 

It shows the light-colored central galaxy nearly 
&lt;a href="https://apod.com/ap250904.html"&gt;edge on&lt;/a&gt; across the 
image center with tremendous orange and red colored 
filaments of gas and dust 
&lt;a href="https://www.reddit.com/media?url=https%3A%2F%2Fi.redd.it%2Fg0gsyf954m261.jpg"&gt;extending&lt;/a&gt; both up and down. 

The filaments extend for over 10,000
&lt;a href="https://spaceplace.nasa.gov/light-year/"&gt;light year&lt;/a&gt;s.

The 12-million light-year distant
&lt;a href="https://apod.com/ap040601.html"&gt;Cigar Galaxy&lt;/a&gt; is the
brightest galaxy in the sky in &lt;a href="https://coolcosmos.ipac.caltech.edu/page/what_is_infrared"&gt;infrared&lt;/a&gt; light and can be seen in visible light with a small
&lt;a href="https://science.howstuffworks.com/telescope.htm"&gt;telescope&lt;/a&gt; towards the &lt;a href="https://spaceplace.nasa.gov/constellations/"&gt;constellation&lt;/a&gt; of the Great Bear
(&lt;a href="https://en.wikipedia.org/wiki/Ursa_Major"&gt;Ursa Major&lt;/a&gt;).</content>
    <link href="https://apod.nasa.gov/apod/ap260629.html"/>
    <summary type="html">Why is the Cigar Galaxy billowing red smoke? 

M82, as this
starburst galaxy is also known, was stirred up by a
recent pass near large
spiral galaxy
M81</summary>
    <published>2026-06-29T03:00:00+00:00</published>
  </entry>
  <entry>
    <id>https://apod.nasa.gov/apod/ap260628.html</id>
    <title>AR 4478: Giant Sunspot Group</title>
    <updated>2026-06-28T03:00:00+00:00</updated>
    <author>
      <name>Jerry Bonnell (UMCP)</name>
    </author>
    <content type="html">&lt;img alt="The Sun is pictured in yellow with surface structure.
In the middle of the frame are many circuitous dark spots.
The edge of the Sun is visible at the top of the image. 
Please see the explanation for more detailed information." src="https://apod.nasa.gov/apod/image/2606/AR4478_vidal_960.jpg" /&gt;&lt;br /&gt;&lt;b&gt; Explanation: &lt;/b&gt; 
Right now, one of the largest sunspot groups in recent history is crossing the Sun. 

&lt;a href="https://www.spaceweatherlive.com/en/solar-activity/region/14478.html"&gt;Active Region 4478&lt;/a&gt; is not only big -- it's violent, showing tangled magnetic fields capable of throwing off huge clouds of particles into the
&lt;a href="https://science.nasa.gov/solar-system/"&gt;Solar System&lt;/a&gt;. 

Some of these &lt;a href="https://en.wikipedia.org/wiki/Coronal_mass_ejection"&gt;CME&lt;/a&gt;s might impact the Earth. 

At the extreme, these 
&lt;a href="https://www.spaceweather.gov/news/large-sunspot-group-rotate-earth-view-24-june"&gt;solar storm&lt;/a&gt;s could cause some 
&lt;a href="https://svs.gsfc.nasa.gov/5214/"&gt;Earth-orbiting satellites to malfunction&lt;/a&gt;, 
the &lt;a href="https://spaceplace.nasa.gov/atmosphere/en/"&gt;Earth's atmosphere&lt;/a&gt; to slightly distort, and &lt;a href="https://www.swpc.noaa.gov/sites/default/files/images/u33/finalBoulderPresentation042611%20%281%29.pdf"&gt;electrical power grids to surge&lt;/a&gt;. 

When impacting 
&lt;a href="https://science.nasa.gov/earth/earth-atmosphere/earths-atmosphere-a-multi-layered-cake/"&gt;Earth's upper atmosphere&lt;/a&gt;, 
these particles can produce 
&lt;a href="https://apod.com/ap230122.html"&gt;beautiful auroras&lt;/a&gt;.

Pictured here, 
&lt;a href="https://spaceweathergallery2.com/indiv_upload.php?upload_id=234253"&gt;AR 4478&lt;/a&gt; and its dark 
&lt;a href="https://en.wikipedia.org/wiki/Sunspot"&gt;sunspot&lt;/a&gt;s 
were captured in visible light a few days ago from 
&lt;a href="https://youtu.be/FGRvP8eoPdw"&gt;Barcelona&lt;/a&gt;, 
&lt;a href="https://en.wikipedia.org/wiki/Spain"&gt;Spain&lt;/a&gt;.  

Almost as large as 
&lt;a href="https://apod.com/ap240513.html"&gt;AR 3664&lt;/a&gt; was in 2024, the 
&lt;a href="https://www.instagram.com/p/DaDSAjilnC5/"&gt;AR 4478 sunspot group&lt;/a&gt; is so big that it is 
&lt;a href="https://people.com/thmb/kiAUaJce7MqVr5XwZFuOA3S10MU=/750x0/filters:no_upscale():max_bytes(150000):strip_icc():focal(999x0:1001x2):format(webp)/dog-eclipse-2000-ef0176770ff64e6b913f2af6e8273a24.jpg"&gt;visible just with glasses&lt;/a&gt; specially designed to view 
&lt;a href="https://science.nasa.gov/eclipses/future-eclipses/eclipse-2024/"&gt;solar eclipse&lt;/a&gt;s. 

This week, 
&lt;a href="https://apod.com/ap040808.html"&gt;skygazing enthusiasts&lt;/a&gt; all over the globe will not only be tracking AR 4478 during the day -- but keenly watching night skies for its 
&lt;a href="https://www.spaceweather.gov/communities/aurora-dashboard-experimental"&gt;corresponding bright auroras&lt;/a&gt;.</content>
    <link href="https://apod.nasa.gov/apod/ap260628.html"/>
    <summary type="html">Right now, one of the largest sunspot groups in recent history is crossing the Sun</summary>
    <published>2026-06-28T03:00:00+00:00</published>
  </entry>
  <entry>
    <id>https://apod.nasa.gov/apod/ap260627.html</id>
    <title>Mars Marathon by Perseverance</title>
    <updated>2026-06-27T03:00:00+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/PIA26726_figA1024c.jpg" /&gt;&lt;br /&gt;&lt;b&gt; Explanation: &lt;/b&gt; 

&lt;a href="https://science.nasa.gov/photojournal/nasas-hirise-captures-perseverance-marking-a-milestone-on-mars/"&gt;In this recent HiRISE&lt;/a&gt;
view from the Mars Reconnaissance Orbiter,
the little green dot indicated on the surface of the big Red Planet is the
&lt;a href="https://science.nasa.gov/mission/mars-2020-perseverance/"&gt;Perseverance&lt;/a&gt;
Mars rover.

Recorded on June 13, the car-sized, six-wheeled robot was imaged
a day before completing a Martian marathon,
traveling a total distance of 26.218 miles
(&lt;a href="https://en.wikipedia.org/wiki/Marathon#IAAF_and_world_records"&gt;42.195 kilometers&lt;/a&gt;)
since it began exploring the surface of Mars.

That equivalent marathon distance was achieved by Perseverance on its
mission sol (Martian day) 1,890, after about 5 Earth years
and 4 Earth months of driving.

Perseverance is continuing &lt;a href="https://apod.com/ap250928.html"&gt;to hunt&lt;/a&gt;
for biosignatures.

In the HiRISE image, the Mars rover's tracks
can be seen leading to
&lt;a href="https://science.nasa.gov/mission/mars-2020-perseverance/location-map/"&gt;its location&lt;/a&gt;
in an area west of its
&lt;a href="https://apod.com/ap210227.htm"&gt;landing site&lt;/a&gt; in Jezero crater near an
&lt;a href="https://science.nasa.gov/resource/perseverance-explores-the-jezero-crater-delta/"&gt;ancient river delta&lt;/a&gt;.</content>
    <link href="https://apod.nasa.gov/apod/ap260627.html"/>
    <summary type="html">In this recent HiRISE
view from the Mars Reconnaissance Orbiter,
the little green dot indicated on the surface of the big Red Planet is the
Perseverance
Mars rover</summary>
    <published>2026-06-27T03:00:00+00:00</published>
  </entry>
  <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">In a cosmic vista you can never see, the
Milky Way
arcs through the night above Seoul, South Korea</summary>
    <published>2026-06-26T03:00:00+00:00</published>
  </entry>
</feed>
