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<!--Generated by Site-Server v@build.version@ (http://www.squarespace.com) on Tue, 06 Oct 2026 04:05:07 GMT
--><rss xmlns:content="http://purl.org/rss/1.0/modules/content/" xmlns:wfw="http://wellformedweb.org/CommentAPI/" xmlns:itunes="http://www.itunes.com/dtds/podcast-1.0.dtd" xmlns:dc="http://purl.org/dc/elements/1.1/" xmlns:media="http://www.rssboard.org/media-rss" version="2.0"><channel><title>AAPOD2 Image Archives - AAPOD2.COM</title><link>https://www.aapod2.com/blog/</link><lastBuildDate>Mon, 05 Oct 2026 19:49:23 +0000</lastBuildDate><language>en-US</language><generator>Site-Server v@build.version@ (http://www.squarespace.com)</generator><description><![CDATA[]]></description><item><title> Sh2-114 &#x2014; The Flying Dragon Nebula in HOO-RGB</title><category>2026</category><dc:creator>Charles Lillo</dc:creator><pubDate>Tue, 06 Oct 2026 04:00:39 +0000</pubDate><link>https://www.aapod2.com/blog/89au9rc2qs5yac3ji6c70m7e690wja</link><guid isPermaLink="false">5debd4b16fcd7b02905712ff:5debd4f1c2fab6555bff00b5:6ac3fd15e27a2a04878f9e1e</guid><description><![CDATA[Sharpless 114 (Sh2-114, LBN 347), commonly referred to as the Flying Dragon 
Nebula, is a faint emission nebula located approximately 3,000 light-years 
away in the constellation Cygnus. Exhibiting a complex morphology with 
long, thread-like filaments of ionized gas, its spectral signature is 
dominated by deep red Hydrogen-Alpha emission alongside subtle doubly 
ionized oxygen cyan regions. While cataloged primarily as an ha region, its 
delicate arc structures and the absence of a clear central ionizing star 
lead astronomers to debate whether it is driven by ionizing stellar 
radiation, an ancient supernova remnant, or an energetic stellar wind-blown 
bubble interacting with the interstellar medium.]]></description><content:encoded><![CDATA[<figure class="
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                <img data-stretch="false" data-image="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/250ac9de-f370-4e47-ab4f-6943800fb96a/Flying+Dragon_FrancescoIanniello_AAPOD2.jpg" data-image-dimensions="5382x3588" data-image-focal-point="0.5,0.5" alt="" data-load="false" elementtiming="system-image-block" data-sqsp-image-classic-block-image src="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/250ac9de-f370-4e47-ab4f-6943800fb96a/Flying+Dragon_FrancescoIanniello_AAPOD2.jpg?format=1000w" width="5382" height="3588" sizes="(max-width: 640px) 100vw, (max-width: 767px) 100vw, 100vw" onload="this.classList.add(&quot;loaded&quot;)" srcset="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/250ac9de-f370-4e47-ab4f-6943800fb96a/Flying+Dragon_FrancescoIanniello_AAPOD2.jpg?format=100w 100w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/250ac9de-f370-4e47-ab4f-6943800fb96a/Flying+Dragon_FrancescoIanniello_AAPOD2.jpg?format=300w 300w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/250ac9de-f370-4e47-ab4f-6943800fb96a/Flying+Dragon_FrancescoIanniello_AAPOD2.jpg?format=500w 500w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/250ac9de-f370-4e47-ab4f-6943800fb96a/Flying+Dragon_FrancescoIanniello_AAPOD2.jpg?format=750w 750w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/250ac9de-f370-4e47-ab4f-6943800fb96a/Flying+Dragon_FrancescoIanniello_AAPOD2.jpg?format=1000w 1000w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/250ac9de-f370-4e47-ab4f-6943800fb96a/Flying+Dragon_FrancescoIanniello_AAPOD2.jpg?format=1500w 1500w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/250ac9de-f370-4e47-ab4f-6943800fb96a/Flying+Dragon_FrancescoIanniello_AAPOD2.jpg?format=2500w 2500w" loading="lazy" decoding="async" data-loader="sqs">

            
          
        
          
        

        
      
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  <p data-rte-preserve-empty="true"><strong>Image Title:</strong> Sh2-114 — The Flying Dragon Nebula in HOO-RGB</p><p data-rte-preserve-empty="true"><strong>Copyright:</strong> Francesco Ianniello Photography</p><p data-rte-preserve-empty="true"><strong>Date image was taken:</strong> August 12, 2026</p><p data-rte-preserve-empty="true"><strong>Location:</strong> Nerpio Italian Project Remote Observatory (Spain)<br>Bortle 3 (SQM 21.70)</p><p data-rte-preserve-empty="true"><strong>Data Acquisition Method:</strong> Other</p><p data-rte-preserve-empty="true"><strong>Description and Details:</strong> Revealing the delicate, ghostly filaments of Sharpless 114, captured over 36 hours of total integration time from the dark skies of Nerpio.<br><br>Deep Sky Facts:<br><br>Location and Nature: Floating within the constellation Cygnus, this faint H-II emission nebula displays intricate filamentary structures so fine that they often resemble an ancient supernova remnant rather than a typical star-forming region.<br><br>The Red Glow of Hydrogen: Dominant, vivid red filaments trace Hydrogen-Alpha emission. This vibrant color reveals exactly where ionized hydrogen gas is recombining, emitting photons in the red part of the visible spectrum.<br><br>The Faint Touch of Oxygen: Subtle, ghostly cyan-blue regions highlight doubly ionized oxygen [O III]. Capturing this extremely faint emission required over 20 hours of dedicated integration to successfully distinguish it from the dense background of the Milky Way. Technical Details (Astro_Nipro):<br><br>Target: Sharpless 114 (Sh2-114) / Flying Dragon Nebula<br><br>Telescope: ASA 250/900 f/3.6<br><br>Mount: ioptron CEM 120 EC<br><br>Camera: player one astronomy Poseidon-M (IMX571 mono)<br><br>Filters / Palette: Antlia Pro 3nm (HOO-RGB)<br><br>Integration Time: 36h 10m Total (HA: 15h | OIII: 20h 40m | R: 10m | G: 10m | B: 10m)<br><br>Software: Voyager (Acquisition), PixInsight, PhotoshopCC2025<br><br>Acquisition: Astro_Nipro Team<br><br>Editing: @francesco_ianniello_astrophoto</p><p data-rte-preserve-empty="true"><strong>Name:</strong> Francesco Ianniello</p><p data-rte-preserve-empty="true"><strong>Website, Instagram or Facebook Profile:</strong> <a href="https://www.francescoianniellophotography.it/">https://www.francescoianniellophotography.it/</a>, @francesco_ianniello_astrophoto</p>]]></content:encoded><media:content type="image/jpeg" url="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/250ac9de-f370-4e47-ab4f-6943800fb96a/Flying+Dragon_FrancescoIanniello_AAPOD2.jpg?format=1500w" medium="image" isDefault="true" width="1500" height="1000"><media:title type="plain">Sh2-114 &#x2014; The Flying Dragon Nebula in HOO-RGB</media:title></media:content></item><item><title>Titans of the Night: 509 Hours on the Vulcan Nebula</title><category>2026</category><dc:creator>Charles Lillo</dc:creator><pubDate>Mon, 05 Oct 2026 04:00:54 +0000</pubDate><link>https://www.aapod2.com/blog/the-vulcan-nebula</link><guid isPermaLink="false">5debd4b16fcd7b02905712ff:5debd4f1c2fab6555bff00b5:6ac10410eb3007723f7c48ab</guid><description><![CDATA[The Vulcan Nebula (cataloged as WPS 46) is a faint deep-sky emission and 
reflection nebula situated roughly two degrees west of the famous spiral 
galaxies Messier 81 and Messier 82 in the constellation Ursa Major. 
Discovered and brought to prominence by amateur astrophotographers 
capturing ultra-deep exposure widefield integration data, the object is 
embedded within extensive integrated flux nebula (IFN) clouds, dust and 
ionized gas floating above the plane of the Milky Way that are lit up by 
ambient starlight and ionized by surrounding stars like TYC 4376-968-1. 
Because of its extremely low surface brightness, bringing out its faint 
blue-green oxygen structures and hydrogen-alpha filaments requires hundreds 
of hours of total integration time across multiple optical systems and 
dark-sky sites.]]></description><content:encoded><![CDATA[<figure class="
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                <img data-stretch="false" data-image="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/1791034450656-EIF55TN8I1Y31VUIZCDS/Vulcan.jpg" data-image-dimensions="4600x2837" data-image-focal-point="0.5,0.5" alt="" data-load="false" elementtiming="system-image-block" data-sqsp-image-classic-block-image src="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/1791034450656-EIF55TN8I1Y31VUIZCDS/Vulcan.jpg?format=1000w" width="4600" height="2837" sizes="(max-width: 640px) 100vw, (max-width: 767px) 100vw, 100vw" onload="this.classList.add(&quot;loaded&quot;)" srcset="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/1791034450656-EIF55TN8I1Y31VUIZCDS/Vulcan.jpg?format=100w 100w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/1791034450656-EIF55TN8I1Y31VUIZCDS/Vulcan.jpg?format=300w 300w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/1791034450656-EIF55TN8I1Y31VUIZCDS/Vulcan.jpg?format=500w 500w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/1791034450656-EIF55TN8I1Y31VUIZCDS/Vulcan.jpg?format=750w 750w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/1791034450656-EIF55TN8I1Y31VUIZCDS/Vulcan.jpg?format=1000w 1000w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/1791034450656-EIF55TN8I1Y31VUIZCDS/Vulcan.jpg?format=1500w 1500w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/1791034450656-EIF55TN8I1Y31VUIZCDS/Vulcan.jpg?format=2500w 2500w" loading="lazy" decoding="async" data-loader="sqs">

            
          
        
          
        

        
      
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  <p data-rte-preserve-empty="true"><strong>Image Title:</strong> Titans of the Night: 509 Hours on the Vulcan Nebula</p><p data-rte-preserve-empty="true"><strong>Copyright:</strong> Team Ager: Aarón de la Casa · Alex Capdevila · Daniel Trueba · Gerard Tàrtalo · Jordi Jofre · Manel Martin · Oscar Royes · Toni Fabiani</p><p data-rte-preserve-empty="true"><strong>Date image was taken:</strong> April 15, 2026</p><p data-rte-preserve-empty="true"><strong>Location:</strong> Team Ager network: seven located in the Sierra del Montsec, together with the Albatàrrec Observatory. (Lleida, Spain)</p><p data-rte-preserve-empty="true"><strong>Data Acquisition Method:</strong> Personal Telescope Setup</p><p data-rte-preserve-empty="true"><strong>Description and Details:</strong> Eight members. Eight observatories. Ten telescopes. 509 hours of integration.<br><br>This image of the faint Vulcan Nebula is the result of a collaborative project developed by Team Ager, an eight-member group united by a shared passion for deep-sky astrophotography and dark skies.<br>Over more than 22 months, we combined data from eight observatories forming part of the Team Ager network: seven located in the Sierra del Montsec, together with the Albatàrrec Observatory, which contributed a significant part of the project's data.<br><br>A total of 10 refracting telescopes, ranging from 54 to 140 mm in aperture, contributed to the project using different cameras, focal lengths, and filter configurations. The final result contains 509 hours of actual integration, corresponding to approximately 3,244 long-exposure frames.<br><br>The integration time was distributed across 28.4 hours of luminance, 33.1 hours of RGB, 211.95 hours of Hα, and 235.55 hours of OIII. The exceptionally large amount of narrowband integration allowed us to reach particularly deep into the faintest structures of the nebula, revealing a complex network of interstellar gas and filaments.<br>The final processing was carried out in PixInsight, integrating all the data from the different instruments and observatories into a single image. The reddish structures are dominated by hydrogen-alpha emission, while the blue and turquoise structures reveal the contribution of ionized oxygen.<br><br>But the depth achieved extends beyond the nebula itself. M81 (Bode's Galaxy) and M82 (the Cigar Galaxy) are clearly visible in the field, accompanied by numerous much fainter background galaxies.<br><br>More than an individual image, Vulcan is the result of 22 months of shared work, eight observatories, ten telescopes, and 509 hours of integration, demonstrating how far amateur astrophotography can reach when knowledge, equipment, and collective effort are brought together in a single project.</p><p data-rte-preserve-empty="true"><strong>Name:</strong> Alex Capdevila Corral</p><p data-rte-preserve-empty="true"><strong>Website, Instagram or Facebook Profile:</strong> <a href="https://www.instagram.com/alex.c.c_astrophotography/">https://www.instagram.com/alex.c.c_astrophotography/</a> <a href="https://www.instagram.com/trueba_d/">https://www.instagram.com/trueba_d/</a> <a href="https://www.instagram.com/gerardtartalo/">https://www.instagram.com/gerardtartalo/</a> <a href="https://www.instagram.com/jordi_jofre_astro/">https://www.instagram.com/jordi_jofre_astro/</a> <a href="https://www.instagram.com/toni_fabiani/">https://www.instagram.com/toni_fabiani/</a> <a href="https://www.instagram.com/ithil_astro/">https://www.instagram.com/ithil_astro/</a> <a href="https://www.instagram.com/astromirades/">https://www.instagram.com/astromirades/</a></p>]]></content:encoded><media:content type="image/jpeg" url="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/1791034450656-EIF55TN8I1Y31VUIZCDS/Vulcan.jpg?format=1500w" medium="image" isDefault="true" width="1500" height="925"><media:title type="plain">Titans of the Night: 509 Hours on the Vulcan Nebula</media:title></media:content></item><item><title>Waning last-quarter mineral Moon</title><category>2026</category><dc:creator>Charles Lillo</dc:creator><pubDate>Sun, 04 Oct 2026 04:00:13 +0000</pubDate><link>https://www.aapod2.com/blog/waning-last-quarter-mineral-moon</link><guid isPermaLink="false">5debd4b16fcd7b02905712ff:5debd4f1c2fab6555bff00b5:6ac103050a625b034f03ac41</guid><description><![CDATA[Lunar regolith is a layer of fine dust, fragmented rock, glass spheres, and 
mineral grains covering the Moon's bedrock, formed by billions of years of 
meteoroid impacts, solar wind, and radiation exposure without atmospheric 
weathering or organic matter. Over 98% of its mass is composed of oxygen, 
silicon, iron, aluminum, calcium, magnesium, and titanium, primarily 
structured in minerals like plagioclase feldspar, pyroxenes, olivine, and 
ilmenite. Its composition varies significantly by region: the light-colored 
Lunar Highlands are rich in aluminum-heavy anorthosite, whereas the dark 
Lunar Maria feature basaltic flows higher in iron and titanium. Due to 
constant space weathering, regolith also unique features agglutinates 
(grains welded together by impact-melted glass), nanophase metallic iron, 
and embedded solar-wind volatiles like helium-3 and hydrogen.]]></description><content:encoded><![CDATA[<figure class="
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                <img data-stretch="false" data-image="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/7f2c44b8-f4a6-43ea-b6a8-3e36f11e3b03/LunaMinerale_C11HD_ASI2600MM_IRUVCut_2Pannelli_25ms_G56_150frames_20261003-0429_final_low.jpg" data-image-dimensions="3904x5000" data-image-focal-point="0.5,0.5" alt="" data-load="false" elementtiming="system-image-block" data-sqsp-image-classic-block-image src="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/7f2c44b8-f4a6-43ea-b6a8-3e36f11e3b03/LunaMinerale_C11HD_ASI2600MM_IRUVCut_2Pannelli_25ms_G56_150frames_20261003-0429_final_low.jpg?format=1000w" width="3904" height="5000" sizes="(max-width: 640px) 100vw, (max-width: 767px) 100vw, 100vw" onload="this.classList.add(&quot;loaded&quot;)" srcset="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/7f2c44b8-f4a6-43ea-b6a8-3e36f11e3b03/LunaMinerale_C11HD_ASI2600MM_IRUVCut_2Pannelli_25ms_G56_150frames_20261003-0429_final_low.jpg?format=100w 100w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/7f2c44b8-f4a6-43ea-b6a8-3e36f11e3b03/LunaMinerale_C11HD_ASI2600MM_IRUVCut_2Pannelli_25ms_G56_150frames_20261003-0429_final_low.jpg?format=300w 300w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/7f2c44b8-f4a6-43ea-b6a8-3e36f11e3b03/LunaMinerale_C11HD_ASI2600MM_IRUVCut_2Pannelli_25ms_G56_150frames_20261003-0429_final_low.jpg?format=500w 500w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/7f2c44b8-f4a6-43ea-b6a8-3e36f11e3b03/LunaMinerale_C11HD_ASI2600MM_IRUVCut_2Pannelli_25ms_G56_150frames_20261003-0429_final_low.jpg?format=750w 750w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/7f2c44b8-f4a6-43ea-b6a8-3e36f11e3b03/LunaMinerale_C11HD_ASI2600MM_IRUVCut_2Pannelli_25ms_G56_150frames_20261003-0429_final_low.jpg?format=1000w 1000w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/7f2c44b8-f4a6-43ea-b6a8-3e36f11e3b03/LunaMinerale_C11HD_ASI2600MM_IRUVCut_2Pannelli_25ms_G56_150frames_20261003-0429_final_low.jpg?format=1500w 1500w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/7f2c44b8-f4a6-43ea-b6a8-3e36f11e3b03/LunaMinerale_C11HD_ASI2600MM_IRUVCut_2Pannelli_25ms_G56_150frames_20261003-0429_final_low.jpg?format=2500w 2500w" loading="lazy" decoding="async" data-loader="sqs">

            
          
        
          
        

        
      
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  <p data-rte-preserve-empty="true"><strong>Image Title:</strong> Waning last-quarter mineral Moon</p><p data-rte-preserve-empty="true"><strong>Copyright:</strong> Alessandro Ravagnin</p><p data-rte-preserve-empty="true"><strong>Date image was taken:</strong> October 03, 2026</p><p data-rte-preserve-empty="true"><strong>Location:</strong> Romano d'Ezzelino</p><p data-rte-preserve-empty="true"><strong>Data Acquisition Method:</strong> Personal Telescope Setup</p><p data-rte-preserve-empty="true"><strong>Description and Details:</strong> Sometimes the best observing sessions are completely unplanned.<br><br>I woke up around 5 a.m. and, unable to fall asleep again, stepped outside to have a look at the sky. Jupiter was shining brightly in the east, the Moon was high above, while Orion and Sirius dominated the southern sky. The atmosphere was remarkably clear and steady — simply too inviting to go back to bed!<br><br>So I opened my observatory and spent the early morning capturing this high-resolution mosaic of the waning last-quarter Moon.<br><br>The image was processed in a “mineral Moon” rendition, enhancing the subtle color differences across the lunar surface associated with variations in the composition and properties of the lunar regolith.<br><br>Even after so many years under the stars, mornings like this can still bring back the same sense of wonder.</p><p data-rte-preserve-empty="true"><strong>Name:</strong> Alessandro Ravagnin</p><p data-rte-preserve-empty="true"><strong>Website, Instagram or Facebook Profile:</strong> <a href="https://astrotrex.wordpress.com/">https://astrotrex.wordpress.com/</a></p>]]></content:encoded><media:content type="image/jpeg" url="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/7f2c44b8-f4a6-43ea-b6a8-3e36f11e3b03/LunaMinerale_C11HD_ASI2600MM_IRUVCut_2Pannelli_25ms_G56_150frames_20261003-0429_final_low.jpg?format=1500w" medium="image" isDefault="true" width="1500" height="1921"><media:title type="plain">Waning last-quarter mineral Moon</media:title></media:content></item><item><title>The Corona Australis Nebula</title><category>2026</category><dc:creator>Charles Lillo</dc:creator><pubDate>Sat, 03 Oct 2026 04:00:41 +0000</pubDate><link>https://www.aapod2.com/blog/ngc-6726/6727</link><guid isPermaLink="false">5debd4b16fcd7b02905712ff:5debd4f1c2fab6555bff00b5:6abf9d1585ed9f61cf24a248</guid><description><![CDATA[NGC 6726/6727 is a prominent pair of reflection nebulae located within the 
southern constellation Corona Australis, situated approximately 420 to 500 
light-years from Earth. As reflection nebulae, they do not produce their 
own visible light through gas ionization; instead, fine interstellar dust 
particles efficiently scatter shorter wavelengths of starlight, creating a 
characteristic vibrant blue glow (Rayleigh scattering). This ethereal light 
is primarily energized and reflected by nearby hot, young stars embedded in 
the cloud, including the variable star TY Crs, as well as HD 176386 and HD 
176269.]]></description><content:encoded><![CDATA[<figure class="
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  <p data-rte-preserve-empty="true"><strong>Image Title:</strong> The Corona Australis Nebula</p><p data-rte-preserve-empty="true"><strong>Copyright:</strong> Tiago Rocha</p><p data-rte-preserve-empty="true"><strong>Date image was taken:</strong> September 06, 2026</p><p data-rte-preserve-empty="true"><strong>Location:</strong> Guanambi - Bahia - Brasil</p><p data-rte-preserve-empty="true"><strong>Data Acquisition Method:</strong> Personal Telescope Setup</p><p data-rte-preserve-empty="true"><strong>Description and Details:</strong> The Corona Australis Nebula (NGC 6726/6727) is one of the most elegant masterpieces of the southern sky. Unlike large, reddish emission nebulae, it stands out for its bluish textures and dark dust clouds that seem to paint space in three dimensions. Its characteristic blue glow comes from a reflection nebula, where fine cosmic dust scatters light from hot, newly born stars. This ethereal glow is framed by dense, dark molecular clouds that meander through space, blocking light from the galactic background and creating an incredible sense of depth.<br><br>Photo settings:<br><br>• ToupTek Hope D60 telescope;<br>• ToupTek GS 100 guide scope;<br>• ToupTek SkyEye26AC PLUS camera;<br>• Exos 2 (EQ5) mount with OnstepX E4;<br>• ZWO EFW;<br>• UV/IR-cut filter (integrated);<br>• 6 hours of exposure with 300s frames;<br>• Astro Scient Observatory;</p><p data-rte-preserve-empty="true"><strong>Name:</strong> Tiago Rocha</p><p data-rte-preserve-empty="true"><strong>Website, Instagram or Facebook Profile:</strong> <a href="https://www.instagram.com/astro_scient/">https://www.instagram.com/astro_scient/</a></p>]]></content:encoded><media:content type="image/jpeg" url="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/a2353f5a-8d77-4dda-b232-541af5666ef7/Image24.jpg?format=1500w" medium="image" isDefault="true" width="1302" height="902"><media:title type="plain">The Corona Australis Nebula</media:title></media:content></item><item><title>LBN 331 - Omicron Cygni</title><category>2026</category><dc:creator>Charles Lillo</dc:creator><pubDate>Fri, 02 Oct 2026 04:00:16 +0000</pubDate><link>https://www.aapod2.com/blog/lbn-331-also-known-as-the-cygnus-waves</link><guid isPermaLink="false">5debd4b16fcd7b02905712ff:5debd4f1c2fab6555bff00b5:6abeb5cade5e6d571c0b5035</guid><description><![CDATA[LBN 331 (also known as the "Cygnus Waves") is a faint, sweeping emission 
nebula situated in the Cygnus constellation near Omicron² Cygni (o2 Cyg) 
and 31/32 Cygni. Composed predominantly of delicate, filamentary tendrils 
of ionized hydrogen (Hα) and oxygen (O III), this low-surface-brightness 
deep-sky object is excited by radiation from neighboring massive stars and 
requires long-exposure astrophotography with narrowband filtering to 
properly capture against the dense background of the Milky Way plane.]]></description><content:encoded><![CDATA[<figure class="
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                <img data-stretch="false" data-image="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/e5010de3-5a6c-46dc-9eb6-0726445466cb/LBN331_HOO.jpg" data-image-dimensions="9000x6000" data-image-focal-point="0.5,0.5" alt="" data-load="false" elementtiming="system-image-block" data-sqsp-image-classic-block-image src="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/e5010de3-5a6c-46dc-9eb6-0726445466cb/LBN331_HOO.jpg?format=1000w" width="9000" height="6000" sizes="(max-width: 640px) 100vw, (max-width: 767px) 100vw, 100vw" onload="this.classList.add(&quot;loaded&quot;)" srcset="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/e5010de3-5a6c-46dc-9eb6-0726445466cb/LBN331_HOO.jpg?format=100w 100w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/e5010de3-5a6c-46dc-9eb6-0726445466cb/LBN331_HOO.jpg?format=300w 300w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/e5010de3-5a6c-46dc-9eb6-0726445466cb/LBN331_HOO.jpg?format=500w 500w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/e5010de3-5a6c-46dc-9eb6-0726445466cb/LBN331_HOO.jpg?format=750w 750w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/e5010de3-5a6c-46dc-9eb6-0726445466cb/LBN331_HOO.jpg?format=1000w 1000w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/e5010de3-5a6c-46dc-9eb6-0726445466cb/LBN331_HOO.jpg?format=1500w 1500w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/e5010de3-5a6c-46dc-9eb6-0726445466cb/LBN331_HOO.jpg?format=2500w 2500w" loading="lazy" decoding="async" data-loader="sqs">

            
          
        
          
        

        
      
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  <p data-rte-preserve-empty="true"><strong>Image Title:</strong> LBN 331 - Omicron Cygni</p><p data-rte-preserve-empty="true"><strong>Copyright:</strong> Eduardo Barbosa</p><p data-rte-preserve-empty="true"><strong>Date image was taken:</strong> August 14, 2026</p><p data-rte-preserve-empty="true"><strong>Location:</strong> Trevinca Skies - A Veiga, Spain.</p><p data-rte-preserve-empty="true"><strong>Data Acquisition Method:</strong> Remote Observatory (Commercial)</p><p data-rte-preserve-empty="true"><strong>Description and Details:</strong> A narrowband field beside Omicron² Cygni (32 Cygni) in Cygnus. Convincing impression of a supernova remnant (it isn't one). 39 hours total: 12h each Hα/OIII/SII plus 1h per RGB channel for the stars, mapped HOO with a synthetic luminance built from all three narrowband channels.<br><br>Captured remotely from Trevinca Skies, a privately operated remote site, with a Sky-Watcher Esprit 100ED, QHY268M and Astronomik filters. Processed in PixInsight and Affinity Photo.</p><p data-rte-preserve-empty="true"><strong>Name:</strong> Eduardo Barbosa</p><p data-rte-preserve-empty="true"><strong>Website, Instagram or Facebook Profile:</strong> <a href="http://eduardobarbosa.net">eduardobarbosa.net</a></p>]]></content:encoded><media:content type="image/jpeg" url="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/e5010de3-5a6c-46dc-9eb6-0726445466cb/LBN331_HOO.jpg?format=1500w" medium="image" isDefault="true" width="1500" height="1000"><media:title type="plain">LBN 331 - Omicron Cygni</media:title></media:content></item><item><title>Cosmic Bubbles Sh2-99 &amp; Sh2-100 in HOO-RGB</title><category>2026</category><dc:creator>Charles Lillo</dc:creator><pubDate>Thu, 01 Oct 2026 04:00:03 +0000</pubDate><link>https://www.aapod2.com/blog/sh2-99-sharpless-99-and-sh2-100</link><guid isPermaLink="false">5debd4b16fcd7b02905712ff:5debd4f1c2fab6555bff00b5:6abd5dc02454825018745099</guid><description><![CDATA[Sh2-99 (Sharpless 99) and Sh2-100 (Sharpless 100) are two H II emission 
nebulae and active star-forming regions located in the plane of the Milky 
Way within the constellation Cygnus.

Both regions are embedded in the larger W58 complex, a massive molecular 
cloud complex and powerful radio source situated thousands of light-years 
away along the Perseus Arm of the Milky Way.]]></description><content:encoded><![CDATA[<figure class="
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                <img data-stretch="false" data-image="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/9689acd4-8e31-4012-8355-15aaa5de4fa2/SH299_SH2100r-.jpg" data-image-dimensions="6207x4137" data-image-focal-point="0.5,0.5" alt="" data-load="false" elementtiming="system-image-block" data-sqsp-image-classic-block-image src="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/9689acd4-8e31-4012-8355-15aaa5de4fa2/SH299_SH2100r-.jpg?format=1000w" width="6207" height="4137" sizes="(max-width: 640px) 100vw, (max-width: 767px) 100vw, 100vw" onload="this.classList.add(&quot;loaded&quot;)" srcset="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/9689acd4-8e31-4012-8355-15aaa5de4fa2/SH299_SH2100r-.jpg?format=100w 100w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/9689acd4-8e31-4012-8355-15aaa5de4fa2/SH299_SH2100r-.jpg?format=300w 300w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/9689acd4-8e31-4012-8355-15aaa5de4fa2/SH299_SH2100r-.jpg?format=500w 500w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/9689acd4-8e31-4012-8355-15aaa5de4fa2/SH299_SH2100r-.jpg?format=750w 750w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/9689acd4-8e31-4012-8355-15aaa5de4fa2/SH299_SH2100r-.jpg?format=1000w 1000w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/9689acd4-8e31-4012-8355-15aaa5de4fa2/SH299_SH2100r-.jpg?format=1500w 1500w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/9689acd4-8e31-4012-8355-15aaa5de4fa2/SH299_SH2100r-.jpg?format=2500w 2500w" loading="lazy" decoding="async" data-loader="sqs">

            
          
        
          
        

        
      
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  <p data-rte-preserve-empty="true"><strong>Image Title:</strong> Cosmic Bubbles Sh2-99 &amp; Sh2-100 in HOO-RGB</p><p data-rte-preserve-empty="true"><strong>Copyright:</strong> Miguel García</p><p data-rte-preserve-empty="true"><strong>Date image was taken:</strong> August 14, 2026</p><p data-rte-preserve-empty="true"><strong>Location:</strong> A Veiga, Ourense, Galicia, Spain</p><p data-rte-preserve-empty="true"><strong>Data Acquisition Method:</strong> Remote Observatory (Commercial)</p><p data-rte-preserve-empty="true"><strong>Description and Details:</strong> Description:<br>Glow in the dense star-forming regions of the Sagitta/Cygnus complex, Sharpless 99 and Sharpless 100 are extremely faint HII regions surrounded by intricate dust structures and subtle ionized gas shells. Located thousands of light-years away along the plane of our Milky Way galaxy, these faint cosmic bubbles require exceptional exposure depth to reveal their delicate emission filaments and surrounding dark dust lanes.<br><br>Captured across multiple dark nights from A Veiga (Ourense, Spain), this deep nearly 52-hour integration combines broad-band RGB star color with narrow-band Hydrogen-alpha (Ha) and Oxygen III (OIII) data (HOO palette). The resulting image highlights the faint bluish OIII structures interwoven with the prominent red Ha glow while maintaining natural star colors and background dust detail.<br><br>Technical Details:<br><br>Target: Sharpless 99 (Sh2-99) &amp; Sharpless 100 (Sh2-100)<br><br>Date: August 2026<br><br>Location: A Veiga, Ourense, Galicia, Spain<br><br>Telescope: APM 107/700 Refractor<br><br>Camera: ZWO ASI 2600MM Pro<br><br>Filters: RGB + Narrowband Ha &amp; OIII (Baader 36mm)<br><br>Integration: ~52 hours total<br><br>Software: N.I.N.A., PHD2, PixInsight</p><p data-rte-preserve-empty="true"><strong>Name:</strong>  Miguel García</p><p data-rte-preserve-empty="true"><strong>Website, Instagram or Facebook Profile:</strong> <a href="https://www.facebook.com/people/Miguel-Garcia/pfbid02eHyDqMbWHdheFTkPFru9QapstDk7gQUnXHagUFfHHXQur2nBdrBWSkbF58yuxSkLl/">https://www.facebook.com/people/Miguel-Garcia/pfbid02eHyDqMbWHdheFTkPFru9QapstDk7gQUnXHagUFfHHXQur2nBdrBWSkbF58yuxSkLl/</a></p>]]></content:encoded><media:content type="image/jpeg" url="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/9689acd4-8e31-4012-8355-15aaa5de4fa2/SH299_SH2100r-.jpg?format=1500w" medium="image" isDefault="true" width="1500" height="1000"><media:title type="plain">Cosmic Bubbles Sh2-99 &amp; Sh2-100 in HOO-RGB</media:title></media:content></item><item><title>NGC 6819 &amp;8 the glowing interstellar medium of the Cygnus constellation</title><category>2026</category><dc:creator>Charles Lillo</dc:creator><pubDate>Wed, 30 Sep 2026 04:00:20 +0000</pubDate><link>https://www.aapod2.com/blog/ngc-6819</link><guid isPermaLink="false">5debd4b16fcd7b02905712ff:5debd4f1c2fab6555bff00b5:6abad6e5af4f1303980e3e62</guid><description><![CDATA[What makes NGC 6819 particularly remarkable to astronomers is its age and 
stellar population. Estimated to be between 2.3 and 2.5 billion years old, 
it is considerably older than typical open star clusters, which usually 
disperse after just a few hundred million years. Containing roughly 150 
member stars, with its brightest individuals shining between 10th and 12th 
magnitude—its high star density and intermediate age made it a primary 
target for NASA's Kepler space telescope to study asteroseismology, 
starspots, and the long-term evolution of stars.]]></description><content:encoded><![CDATA[<figure class="
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                <img data-stretch="false" data-image="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/c97d9970-9d2a-4600-b4fe-2830509b217e/NGC6819_jyb_2026.jpg" data-image-dimensions="4767x3178" data-image-focal-point="0.5,0.5" alt="" data-load="false" elementtiming="system-image-block" data-sqsp-image-classic-block-image src="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/c97d9970-9d2a-4600-b4fe-2830509b217e/NGC6819_jyb_2026.jpg?format=1000w" width="4767" height="3178" sizes="(max-width: 640px) 100vw, (max-width: 767px) 100vw, 100vw" onload="this.classList.add(&quot;loaded&quot;)" srcset="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/c97d9970-9d2a-4600-b4fe-2830509b217e/NGC6819_jyb_2026.jpg?format=100w 100w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/c97d9970-9d2a-4600-b4fe-2830509b217e/NGC6819_jyb_2026.jpg?format=300w 300w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/c97d9970-9d2a-4600-b4fe-2830509b217e/NGC6819_jyb_2026.jpg?format=500w 500w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/c97d9970-9d2a-4600-b4fe-2830509b217e/NGC6819_jyb_2026.jpg?format=750w 750w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/c97d9970-9d2a-4600-b4fe-2830509b217e/NGC6819_jyb_2026.jpg?format=1000w 1000w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/c97d9970-9d2a-4600-b4fe-2830509b217e/NGC6819_jyb_2026.jpg?format=1500w 1500w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/c97d9970-9d2a-4600-b4fe-2830509b217e/NGC6819_jyb_2026.jpg?format=2500w 2500w" loading="lazy" decoding="async" data-loader="sqs">

            
          
        
          
        

        
      
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  <p data-rte-preserve-empty="true"><strong>Image Title:</strong> NGC 6819 in the foreground of the glowing interstellar medium of the Cygnus constellation</p><p data-rte-preserve-empty="true"><strong>Copyright:</strong></p><p data-rte-preserve-empty="true"><strong>Date image was taken:</strong> August 11, 2026</p><p data-rte-preserve-empty="true"><strong>Location:</strong> Alqueva Dark Skies, Portugal</p><p data-rte-preserve-empty="true"><strong>Data Acquisition Method:</strong> Personal Telescope Setup</p><p data-rte-preserve-empty="true"><strong>Description and Details:</strong> Imaged from Portugal over 3 nights in August 2026 with an Astro-Physics 130mm mounted on an AP Mach1 mount.<br><br>The HOO image is the result of 7 hours of imaging through H and O filters to capture the nebulosity and 1.5 hours each through R, G and B filters to capture the stars.<br><br>NGC 6819 is a rich open star cluster located in the constellation Cygnus.<br><br>The faint red glow behind NGC 6819 is part of the widespread hydrogen-alpha emission nebulosity that fills much of Cygnus. It comes from thin clouds of ionized hydrogen gas, which emit strongly at the deep-red Hα wavelength of 656.3 nm when energized by ultraviolet radiation from nearby hot stars.</p><p data-rte-preserve-empty="true"><strong>Name:</strong> Jean Yves Beninger</p><p data-rte-preserve-empty="true"><strong>Website, Instagram or Facebook Profile:</strong> <a href="http://www.lesbeninger.com">www.lesbeninger.com</a></p>]]></content:encoded><media:content type="image/jpeg" url="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/c97d9970-9d2a-4600-b4fe-2830509b217e/NGC6819_jyb_2026.jpg?format=1500w" medium="image" isDefault="true" width="1500" height="1000"><media:title type="plain">NGC 6819 &amp;8 the glowing interstellar medium of the Cygnus constellation</media:title></media:content></item><item><title>vdB 152 (Wolf's Cave Nebula) and LDN 1221</title><category>2026</category><dc:creator>Charles Lillo</dc:creator><pubDate>Tue, 29 Sep 2026 04:00:24 +0000</pubDate><link>https://www.aapod2.com/blog/vdb-152-2026</link><guid isPermaLink="false">5debd4b16fcd7b02905712ff:5debd4f1c2fab6555bff00b5:6abad5d1792b002e1cc3cd3e</guid><description><![CDATA[Silent and ancient, a cosmic serpent glides through the northern sky. 
Caught in the delicate interplay between dust and starlight, the reflection 
nebula vdB 152 glows like a celestial torch at the tip of a towering, 
opaque dust lane known as LDN 1221. Here in the Cepheus Flare, cosmic dust 
grains scatter the soft light of the embedded star BVD 111, painting the 
dark canvas of space with vivid shades of blue. Surrounding this stellar 
sanctuary, dense interstellar dust clouds cloak the background stars, 
weaving intricate dark lanes that reveal the quiet, ongoing birth of stars 
within our Milky Way.]]></description><content:encoded><![CDATA[<figure class="
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                <img data-stretch="false" data-image="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/f194120e-1655-4edf-bcb4-b141e2122635/vdB-152.jpeg" data-image-dimensions="5933x3861" data-image-focal-point="0.5,0.5" alt="" data-load="false" elementtiming="system-image-block" data-sqsp-image-classic-block-image src="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/f194120e-1655-4edf-bcb4-b141e2122635/vdB-152.jpeg?format=1000w" width="5933" height="3861" sizes="(max-width: 640px) 100vw, (max-width: 767px) 100vw, 100vw" onload="this.classList.add(&quot;loaded&quot;)" srcset="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/f194120e-1655-4edf-bcb4-b141e2122635/vdB-152.jpeg?format=100w 100w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/f194120e-1655-4edf-bcb4-b141e2122635/vdB-152.jpeg?format=300w 300w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/f194120e-1655-4edf-bcb4-b141e2122635/vdB-152.jpeg?format=500w 500w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/f194120e-1655-4edf-bcb4-b141e2122635/vdB-152.jpeg?format=750w 750w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/f194120e-1655-4edf-bcb4-b141e2122635/vdB-152.jpeg?format=1000w 1000w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/f194120e-1655-4edf-bcb4-b141e2122635/vdB-152.jpeg?format=1500w 1500w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/f194120e-1655-4edf-bcb4-b141e2122635/vdB-152.jpeg?format=2500w 2500w" loading="lazy" decoding="async" data-loader="sqs">

            
          
        
          
        

        
      
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  <p data-rte-preserve-empty="true"><strong>Image Title:</strong> vdB 152 (Wolf's Cave Nebula) and LDN 1221</p><p data-rte-preserve-empty="true"><strong>Copyright:</strong> Deval Singh</p><p data-rte-preserve-empty="true"><strong>Date image was taken:</strong> September 10, 2026</p><p data-rte-preserve-empty="true"><strong>Location:</strong> Hanle, Ladakh (india)</p><p data-rte-preserve-empty="true"><strong>Data Acquisition Method:</strong> Personal Telescope Setup</p><p data-rte-preserve-empty="true"><strong>Description and Details:</strong> Silent and ancient, a cosmic serpent glides through the northern sky. Caught in the delicate interplay between dust and starlight, the reflection nebula vdB 152 glows like a celestial torch at the tip of a towering, opaque dust lane known as LDN 1221. Here in the Cepheus Flare, cosmic dust grains scatter the soft light of the embedded star BVD 111, painting the dark canvas of space with vivid shades of blue. Surrounding this stellar sanctuary, dense interstellar dust clouds cloak the background stars, weaving intricate dark lanes that reveal the quiet, ongoing birth of stars within our Milky Way.<br><br>Captured under the pristine Bortle 1 skies of the Hanle Dark Sky Reserve in Ladakh, India, this image highlights the incredible transparency of high-altitude night skies. Even without the aid of dual-narrowband filters, the ultra-dark conditions allowed a standard broadband setup to reveal not only the subtle brown dust and blue reflection details, but also the faint background H-alpha filaments and delicate OIII emissions woven throughout the region.<br><br>Acquisition Details:<br>Targets: vdB 152 (Wolf's Cave Nebula) and LDN 1221<br>Location: Hanle Dark Sky Reserve, Ladakh, India (Bortle 1)<br>Event: HDSR Hanle Star Party (September 2026)<br>Telescope: Askar SQA55<br>Camera: ZWO ASI2600MC Air<br>Mount: ZWO AM5<br>Filter: ZWO IR/UV Cut<br>Integration: 7h 30m (150 x 180 sec)<br>Calibration: Darks, Flats, and Biases</p><p data-rte-preserve-empty="true"><strong>Name:</strong> Deval Singh</p><p data-rte-preserve-empty="true"><strong>Website, Instagram or Facebook Profile:</strong> instagram : @Rtastronomy, facebook : Deval SIngh</p>]]></content:encoded><media:content type="image/jpeg" url="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/f194120e-1655-4edf-bcb4-b141e2122635/vdB-152.jpeg?format=1500w" medium="image" isDefault="true" width="1500" height="976"><media:title type="plain">vdB 152 (Wolf's Cave Nebula) and LDN 1221</media:title></media:content></item><item><title>Minkowski 2-51 Planetary Nebula</title><category>2026</category><dc:creator>Charles Lillo</dc:creator><pubDate>Mon, 28 Sep 2026 04:00:31 +0000</pubDate><link>https://www.aapod2.com/blog/the-minkowski-2-51-planetary-nebula</link><guid isPermaLink="false">5debd4b16fcd7b02905712ff:5debd4f1c2fab6555bff00b5:6ab572f461cebe6eaae3839c</guid><description><![CDATA[The Minkowski 2-51 Planetary Nebula (also designated as M 2-51 or PN 
G103.2+00.6) is a faint planetary nebula located roughly 6,300 light-years 
away in the constellation Cepheus. Discovered in 1947 by the 
German-American astronomer Rudolph Minkowski using objective-prism survey 
plates at Mount Wilson, the nebula represents the expanding, glowing shell 
of ionized gas expelled by an aging, low- to intermediate-mass star 
entering its final evolutionary stages. Sometimes informally nicknamed the 
"Little Ring Nebula," it measures under 1 arcminute in angular size (around 
39 to 56 arcseconds) and shines dimly at an optical magnitude of 
approximately 13.5.]]></description><content:encoded><![CDATA[<figure class="
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                <img data-stretch="false" data-image="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/f080f86f-cdfe-41bf-9694-ef063511bd78/2026+09-19+-+Minkowski+2-51+Planetary+Nebula+%28165mm+and+102mm%29.jpg" data-image-dimensions="3236x2679" data-image-focal-point="0.5,0.5" alt="" data-load="false" elementtiming="system-image-block" data-sqsp-image-classic-block-image src="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/f080f86f-cdfe-41bf-9694-ef063511bd78/2026+09-19+-+Minkowski+2-51+Planetary+Nebula+%28165mm+and+102mm%29.jpg?format=1000w" width="3236" height="2679" sizes="(max-width: 640px) 100vw, (max-width: 767px) 100vw, 100vw" onload="this.classList.add(&quot;loaded&quot;)" srcset="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/f080f86f-cdfe-41bf-9694-ef063511bd78/2026+09-19+-+Minkowski+2-51+Planetary+Nebula+%28165mm+and+102mm%29.jpg?format=100w 100w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/f080f86f-cdfe-41bf-9694-ef063511bd78/2026+09-19+-+Minkowski+2-51+Planetary+Nebula+%28165mm+and+102mm%29.jpg?format=300w 300w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/f080f86f-cdfe-41bf-9694-ef063511bd78/2026+09-19+-+Minkowski+2-51+Planetary+Nebula+%28165mm+and+102mm%29.jpg?format=500w 500w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/f080f86f-cdfe-41bf-9694-ef063511bd78/2026+09-19+-+Minkowski+2-51+Planetary+Nebula+%28165mm+and+102mm%29.jpg?format=750w 750w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/f080f86f-cdfe-41bf-9694-ef063511bd78/2026+09-19+-+Minkowski+2-51+Planetary+Nebula+%28165mm+and+102mm%29.jpg?format=1000w 1000w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/f080f86f-cdfe-41bf-9694-ef063511bd78/2026+09-19+-+Minkowski+2-51+Planetary+Nebula+%28165mm+and+102mm%29.jpg?format=1500w 1500w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/f080f86f-cdfe-41bf-9694-ef063511bd78/2026+09-19+-+Minkowski+2-51+Planetary+Nebula+%28165mm+and+102mm%29.jpg?format=2500w 2500w" loading="lazy" decoding="async" data-loader="sqs">

            
          
        
          
        

        
      
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  <p data-rte-preserve-empty="true"><strong>Image Title:</strong> Minkowski 2-51 Planetary Nebula</p><p data-rte-preserve-empty="true"><strong>Copyright:</strong> Douglas J Struble</p><p data-rte-preserve-empty="true"><strong>Date image was taken:</strong> September 19, 2026</p><p data-rte-preserve-empty="true"><strong>Location:</strong> Taylor, MI USA</p><p data-rte-preserve-empty="true"><strong>Data Acquisition Method:</strong> Personal Telescope Setup</p><p data-rte-preserve-empty="true"><strong>Description and Details:</strong> Minkowski 2-51 (M 2-51) is a planetary nebula, cataloged as PN G103.2+00.6. It is the ionized circumstellar material expelled during the late evolutionary stages of a low- to intermediate-mass star. It’s not captured often and tried to do it justice.<br><br>The nebula consists primarily of gas expelled from the progenitor star during its asymptotic giant branch (AGB) evolution. After losing its outer envelope, the star's exposed core became extremely hot and began ionizing the previously expelled material.<br><br>The resulting nebula emits strongly through collisionally excited forbidden lines and hydrogen recombination lines.</p><p data-rte-preserve-empty="true"><strong>Name:</strong> Douglas Struble</p><p data-rte-preserve-empty="true"><strong>Website, Instagram or Facebook Profile:</strong> <a href="https://www.facebook.com/AstrophotographyByDouglasJStruble/">https://www.facebook.com/AstrophotographyByDouglasJStruble/</a></p>]]></content:encoded><media:content type="image/jpeg" url="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/f080f86f-cdfe-41bf-9694-ef063511bd78/2026+09-19+-+Minkowski+2-51+Planetary+Nebula+%28165mm+and+102mm%29.jpg?format=1500w" medium="image" isDefault="true" width="1500" height="1242"><media:title type="plain">Minkowski 2-51 Planetary Nebula</media:title></media:content></item><item><title>Pelican Nebula and Neighbors</title><category>2026</category><dc:creator>Charles Lillo</dc:creator><pubDate>Sun, 27 Sep 2026 04:00:29 +0000</pubDate><link>https://www.aapod2.com/blog/pelican-nebula-and-neighbors</link><guid isPermaLink="false">5debd4b16fcd7b02905712ff:5debd4f1c2fab6555bff00b5:6ab5718cac495f5135abd379</guid><description><![CDATA[The Pelican Nebula (cataloged as IC 5070 and IC 5067) is a large emission 
nebula situated approximately 1,800 to 2,000 light-years away in the 
constellation Cygnus. Spanning roughly 30 light-years across, it is a 
dynamic star-forming region whose glowing, ionized gas clouds trace an 
outline resembling a pelican's head and bill. This visible glow is caused 
by strong ultraviolet radiation from nearby massive stars—most notably 
Deneb and the energetic stars in the neighboring North America Nebula (NGC 
7000), from which the Pelican is separated by a dark, dense lane of 
interstellar dust known as LDN 935.]]></description><content:encoded><![CDATA[<figure class="
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  <p data-rte-preserve-empty="true"><strong>Image Title:</strong> Pelican Nebula and Neighbors</p><p data-rte-preserve-empty="true"><strong>Copyright:</strong> Maciej Enerlich</p><p data-rte-preserve-empty="true"><strong>Date image was taken:</strong> September 18, 2026</p><p data-rte-preserve-empty="true"><strong>Location:</strong> Rudka 12-100<br>Poland</p><p data-rte-preserve-empty="true"><strong>Data Acquisition Method:</strong> Personal Telescope Setup</p><p data-rte-preserve-empty="true"><strong>Description and Details:</strong> This image of the Pelican Nebula and its surrounding Cygnus clouds is based almost entirely on narrowband data.<br><br>The final result combines 8 h 50 min of dual-band Ha/OIII data captured with the Optolong L-Ultimate and 7 h 30 min of dedicated SII data acquired through the SVBony SV227 5 nm filter, with only a very small amount of unfiltered data added. The total integration time is 16 h 26 min with 300s frames. I also used 18 and 6s frames with no filter for rgb stars<br><br>My goal with this project was not only to reveal the rich structure of the region — the glowing emission, dark dust lanes and subtle transitions across the field — but also to build an SHO-style narrowband image using a one-shot color camera.<br><br>Even though I use a ZWO ASI2600MC Pro, I try to create SHO images to show that this kind of processing is not reserved only for mono cameras. Of course, a monochrome setup remains the more direct and flexible solution for true narrowband imaging, but I wanted this image to demonstrate that it is still possible to experiment with the SHO palette and achieve a satisfying result with an OSC/MC camera as well.<br><br>For me, this is part of the fun: exploring how far a color camera can be pushed in narrowband work, and showing that SHO can also be an interesting creative path for MC users.<br><br>Equipment:<br>Telescope: Askar 103 APO + 0.8× reducer<br>Camera: ZWO ASI2600MC Pro<br>Mount: Proxisky Ragdoll 17 Pro<br>Filters: Optolong L-Ultimate 2", SVBony SV227 SII 5 nm 2"<br>Acquisition: ZWO ASIAIR Mini, ZWO EAF<br>Processing: PixInsight, Astro Pixel Processor, Adobe Photoshop</p><p data-rte-preserve-empty="true"><strong>Name:</strong> Maciej Enerlich</p><p data-rte-preserve-empty="true"><strong>Website, Instagram or Facebook Profile:</strong> Instagram: <a href="https://www.instagram.com/macieje.astrofotografia/">https://www.instagram.com/macieje.astrofotografia/</a></p>]]></content:encoded><media:content type="image/jpeg" url="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/d57d0a2a-7879-487e-8279-40ad2a9d9fc7/Pelikan+FB.jpg?format=1500w" medium="image" isDefault="true" width="1500" height="1014"><media:title type="plain">Pelican Nebula and Neighbors</media:title></media:content></item><item><title>LDN 1082 (Sea Horse)</title><category>2026</category><dc:creator>Charles Lillo</dc:creator><pubDate>Sat, 26 Sep 2026 04:00:19 +0000</pubDate><link>https://www.aapod2.com/blog/the-seahorse-nebula-ldn-1082</link><guid isPermaLink="false">5debd4b16fcd7b02905712ff:5debd4f1c2fab6555bff00b5:6ab56c1cc3163c62877c9c40</guid><description><![CDATA[The Seahorse Nebula (cataloged as LDN 1082 or Barnard 150) is a prominent 
dark absorption nebula situated approximately 1,200 light-years away from 
Earth in the northern constellation Cepheus. Unlike glowing emission or 
reflection nebulae, this object is composed of dense, cold cosmic dust and 
interstellar gas that emits no visible light of its own. Instead, it acts 
as an opaque silhouette, obscuring the rich, bright star fields of the 
Milky Way lying directly behind it.]]></description><content:encoded><![CDATA[<figure class="
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                <img data-stretch="false" data-image="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/2075ce30-e930-4dea-9139-59fce9d787d3/LDN1082_Small.jpg" data-image-dimensions="2680x1989" data-image-focal-point="0.5,0.5" alt="" data-load="false" elementtiming="system-image-block" data-sqsp-image-classic-block-image src="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/2075ce30-e930-4dea-9139-59fce9d787d3/LDN1082_Small.jpg?format=1000w" width="2680" height="1989" sizes="(max-width: 640px) 100vw, (max-width: 767px) 100vw, 100vw" onload="this.classList.add(&quot;loaded&quot;)" srcset="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/2075ce30-e930-4dea-9139-59fce9d787d3/LDN1082_Small.jpg?format=100w 100w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/2075ce30-e930-4dea-9139-59fce9d787d3/LDN1082_Small.jpg?format=300w 300w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/2075ce30-e930-4dea-9139-59fce9d787d3/LDN1082_Small.jpg?format=500w 500w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/2075ce30-e930-4dea-9139-59fce9d787d3/LDN1082_Small.jpg?format=750w 750w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/2075ce30-e930-4dea-9139-59fce9d787d3/LDN1082_Small.jpg?format=1000w 1000w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/2075ce30-e930-4dea-9139-59fce9d787d3/LDN1082_Small.jpg?format=1500w 1500w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/2075ce30-e930-4dea-9139-59fce9d787d3/LDN1082_Small.jpg?format=2500w 2500w" loading="lazy" decoding="async" data-loader="sqs">

            
          
        
          
        

        
      
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  <p data-rte-preserve-empty="true"><strong>mage Title:</strong> LDN 1082 (Sea Horse)</p><p data-rte-preserve-empty="true"><strong>Copyright:</strong> 2026 Jürgen Terp</p><p data-rte-preserve-empty="true"><strong>Date image was taken:</strong> September 10, 2026</p><p data-rte-preserve-empty="true"><strong>Location:</strong> Puntagorda, Spain (La Palma)</p><p data-rte-preserve-empty="true"><strong>Data Acquisition Method:</strong> Personal Telescope Setup</p><p data-rte-preserve-empty="true"><strong>Description and Details:</strong> Between the end of one Calima and the arrival of the next, I was lucky enough to have two beautiful nights under the stars on La Palma, spending them capturing the Seahorse Nebula in Cepheus.<br><br>I used my William Optics RedCat 51 on a Sky-Watcher Star Adventurer GTi, my compact mobile setup for trips and vacations. The first night was especially memorable: calm conditions, no wind gusts, and wonderfully dark skies. After a day surrounded by the beauty of La Palma, there is something truly special about spending the night beneath its stars.<br><br>9–10 September 2026<br>14 hours total integration time<br>169 × 300 s</p><p data-rte-preserve-empty="true"><strong>Name:</strong> Jürgen Terpe</p><p data-rte-preserve-empty="true"><strong>Website, Instagram or Facebook Profile:</strong> <a href="https://app.astrobin.com/u/JuergenTerpe">https://app.astrobin.com/u/JuergenTerpe</a></p>]]></content:encoded><media:content type="image/jpeg" url="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/2075ce30-e930-4dea-9139-59fce9d787d3/LDN1082_Small.jpg?format=1500w" medium="image" isDefault="true" width="1500" height="1113"><media:title type="plain">LDN 1082 (Sea Horse)</media:title></media:content></item><item><title>A Galactic Farewell to Summer</title><category>2026</category><dc:creator>Charles Lillo</dc:creator><pubDate>Fri, 25 Sep 2026 04:00:51 +0000</pubDate><link>https://www.aapod2.com/blog/a-galactic-farewell-to-summer</link><guid isPermaLink="false">5debd4b16fcd7b02905712ff:5debd4f1c2fab6555bff00b5:6ab5695d5351d14f90877109</guid><description><![CDATA[On the night between September 11 and 12, together with my dear friend 
Filippo, companion of countless astrophotography adventures, we planned a 
night photography session to bid farewell to the summer Milky Way. The 
noticeably cooler conditions compared with the previous months, together 
with the Galactic Center setting during the early hours of the evening, 
encouraged us to choose a nearby coastal location for our images.

Finally, with a sky free from the excessive humidity of summer, we had the 
chance to carry out more meaningful tests with our UV/IR-cut modified 
cameras and explore the wonders of the cosmos with greater accuracy and 
detail. The unique scenery offered by our coastline would also help enhance 
a spectacle that was already magnificent on its own.
With the best intentions, we spent hours taking exposures, trying to 
collect as much light as possible from stars and nebulae far away in both 
space and time.]]></description><content:encoded><![CDATA[<figure class="
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                <img data-stretch="false" data-image="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/e32f9c73-a02a-4ad5-ad27-2009df6ba794/via_lattea_marina_di_modica.jpg" data-image-dimensions="1920x2400" data-image-focal-point="0.5,0.5" alt="" data-load="false" elementtiming="system-image-block" data-sqsp-image-classic-block-image src="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/e32f9c73-a02a-4ad5-ad27-2009df6ba794/via_lattea_marina_di_modica.jpg?format=1000w" width="1920" height="2400" sizes="(max-width: 640px) 100vw, (max-width: 767px) 100vw, 100vw" onload="this.classList.add(&quot;loaded&quot;)" srcset="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/e32f9c73-a02a-4ad5-ad27-2009df6ba794/via_lattea_marina_di_modica.jpg?format=100w 100w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/e32f9c73-a02a-4ad5-ad27-2009df6ba794/via_lattea_marina_di_modica.jpg?format=300w 300w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/e32f9c73-a02a-4ad5-ad27-2009df6ba794/via_lattea_marina_di_modica.jpg?format=500w 500w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/e32f9c73-a02a-4ad5-ad27-2009df6ba794/via_lattea_marina_di_modica.jpg?format=750w 750w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/e32f9c73-a02a-4ad5-ad27-2009df6ba794/via_lattea_marina_di_modica.jpg?format=1000w 1000w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/e32f9c73-a02a-4ad5-ad27-2009df6ba794/via_lattea_marina_di_modica.jpg?format=1500w 1500w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/e32f9c73-a02a-4ad5-ad27-2009df6ba794/via_lattea_marina_di_modica.jpg?format=2500w 2500w" loading="lazy" decoding="async" data-loader="sqs">

            
          
        
          
        

        
          
          <figcaption data-sqsp-image-classic-block-caption-container class="image-caption-wrapper">
            <p data-rte-preserve-empty="true"><strong>Image Title:</strong> A Galactic Farewell to Summer - and Not Only That…</p><p data-rte-preserve-empty="true"><strong>Copyright:</strong> Salvatore Cerruto</p><p data-rte-preserve-empty="true"><strong>Location:</strong> Marina di Modica, Sicily, Italy</p><p data-rte-preserve-empty="true"><strong>Data Acquisition Method:</strong> Other</p><p data-rte-preserve-empty="true"><strong>Description and Details:</strong> <br><br>During the session, and again in the following days, I was already thinking about how I would approach the post-processing in order to obtain the result I had in mind.<br>I had roughly planned the workflow: alignment, calibration and stacking in Siril, followed by refinement and blending with the landscape in Photoshop.<br>It is a workflow I have learned over the years through many hours of study, countless attempts, mistakes, and even entire projects discarded after spending hours in front of the computer.<br>The process has become fairly reproducible by now, but it can still require a very different amount of work each time. The starting conditions are never quite the same, and something that appears straightforward on paper can easily become much more complicated.<br><br>And this is where the second farewell begins…<br><br>After years of spending so many hours behind a computer processing my images, this time I decided to experiment with something different and put OpenAI's new frontier model, ChatGPT Astra, to the test. I downloaded the files from my SD card, organized them into just a couple of folders and, essentially, told it:<br>"Take care of it. These are my RAW files, these are the light frames, these are the dark frames, and this is the landscape. Use Siril and Photoshop and deliver the finished image."<br><br>The mouse cursor began moving on its own.<br><br>About ten minutes later, it presented me with a Milky Way image that I would have struggled to improve upon myself - and certainly not in ten minutes.<br><br>But most importantly, the image had not been artificially generated.<br><br>What I was looking at was already there, inside my files.<br>It was the signal I had actually captured a few nights earlier on my camera sensor. It was real light from the sky, light that had travelled through space, reached Earth, and been recorded during those hours spent beside the sea.<br>The artificial intelligence had not invented that Milky Way. It had worked with the real signal contained in my RAW files, trying to extract as much information from it as possible.<br>After only a few manual stylistic adjustments, the image was essentially complete. I would say that around 90 percent of the final work had already been done.<br><br>And from that moment on, a series of conflicting thoughts began to emerge - some positive, others much less so.<br>On one hand, perhaps I can finally devote more of my time to what I find most beautiful and rewarding about astrophotography: contemplating the night sky during an imaging session and discovering places where we become guests of darkness and silence, places where we can slow down and reconnect with the cosmos.<br>It is an experience that modern human beings are gradually losing.<br>On the other hand, there is a feeling that is difficult to ignore.<br>A machine can understand my intentions and perform the work better - or at least far more quickly - than I could do it myself.<br>The creative process of slowly revealing the sculpture hidden inside a rough block of marble, something that had been an integral part of my photography for years, suddenly seems as though it may no longer necessarily need me.<br><br>There is the excitement of having reached a new frontier, but also the bittersweet feeling of having left something behind.<br>The more enthusiastic part of me says that a new journey can only begin when something is left behind. The more cautious part wonders whether all of this could make me intellectually lazy, preventing me from continuing the path of study, experimentation, mistakes and countless hours of work that brought me to where I am today.<br>Perhaps, with time, these still-disordered thoughts will eventually converge into a new understanding.<br><br>But one thing seems certain:<br>the world - photography included, but certainly not photography alone - is changing at an unprecedented pace.<br><br>Technical data:<br>Nikon D800 + Sigma ART 35mm f/1.4<br>- 60 frames for the sky at f/4, ISO-1250, 45 seconds<br>- 8 frames for the foreground at f/4, ISO-800, 60 seconds<br>Post: Siril + Photoshop + ChatGPT Astra</p><p data-rte-preserve-empty="true"><strong>Name:</strong> Salvatore Cerruto</p><p data-rte-preserve-empty="true"><strong>Website, Instagram or Facebook Profile:</strong> <a href="https://www.instagram.com/salvatore_cerruto/">https://www.instagram.com/salvatore_cerruto/</a></p>
          </figcaption>
        
      
        </figure>]]></content:encoded><media:content type="image/jpeg" url="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/e32f9c73-a02a-4ad5-ad27-2009df6ba794/via_lattea_marina_di_modica.jpg?format=1500w" medium="image" isDefault="true" width="1500" height="1875"><media:title type="plain">A Galactic Farewell to Summer</media:title></media:content></item><item><title>Gecko and Friends</title><category>2026</category><dc:creator>Charles Lillo</dc:creator><pubDate>Thu, 24 Sep 2026 04:00:22 +0000</pubDate><link>https://www.aapod2.com/blog/gecko-and-friends</link><guid isPermaLink="false">5debd4b16fcd7b02905712ff:5debd4f1c2fab6555bff00b5:6ab3e09ecd5fa91d69821af6</guid><description><![CDATA[Apart from the Gecko Nebula itself and the dominating bright red hydrogen 
clouds the numerous „small“ background galaxies make this image special.

I collected the data for this image of the Gecko Nebula (LBN 437) in 
constellation Lacerta during 7 nights in August/September 2026 with a small 
refractor and an OSC camera from my balcony in Eltville, Germany - Bortle 
class 5.

The image represents 30.4 hours of total exposure time (15.9h without 
filter and 14.5h dual narrowband) - taken with following equipment:
telescope: Askar SQA85
camera: ZWO ASI2600MC Air
mount: ZWO AM5N
filter: Optolong L-eXtreme (Ha/OIII)]]></description><content:encoded><![CDATA[<figure class="
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                <img data-stretch="false" data-image="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/6b25a12e-9c45-46a7-81ed-ef31b0f843e4/LBN_437_478x120s_NF_2026-08-22_296x120s_LeXt_2026-09-07final2.jpg" data-image-dimensions="3856x5937" data-image-focal-point="0.5,0.5" alt="" data-load="false" elementtiming="system-image-block" data-sqsp-image-classic-block-image src="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/6b25a12e-9c45-46a7-81ed-ef31b0f843e4/LBN_437_478x120s_NF_2026-08-22_296x120s_LeXt_2026-09-07final2.jpg?format=1000w" width="3856" height="5937" sizes="(max-width: 640px) 100vw, (max-width: 767px) 100vw, 100vw" onload="this.classList.add(&quot;loaded&quot;)" srcset="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/6b25a12e-9c45-46a7-81ed-ef31b0f843e4/LBN_437_478x120s_NF_2026-08-22_296x120s_LeXt_2026-09-07final2.jpg?format=100w 100w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/6b25a12e-9c45-46a7-81ed-ef31b0f843e4/LBN_437_478x120s_NF_2026-08-22_296x120s_LeXt_2026-09-07final2.jpg?format=300w 300w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/6b25a12e-9c45-46a7-81ed-ef31b0f843e4/LBN_437_478x120s_NF_2026-08-22_296x120s_LeXt_2026-09-07final2.jpg?format=500w 500w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/6b25a12e-9c45-46a7-81ed-ef31b0f843e4/LBN_437_478x120s_NF_2026-08-22_296x120s_LeXt_2026-09-07final2.jpg?format=750w 750w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/6b25a12e-9c45-46a7-81ed-ef31b0f843e4/LBN_437_478x120s_NF_2026-08-22_296x120s_LeXt_2026-09-07final2.jpg?format=1000w 1000w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/6b25a12e-9c45-46a7-81ed-ef31b0f843e4/LBN_437_478x120s_NF_2026-08-22_296x120s_LeXt_2026-09-07final2.jpg?format=1500w 1500w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/6b25a12e-9c45-46a7-81ed-ef31b0f843e4/LBN_437_478x120s_NF_2026-08-22_296x120s_LeXt_2026-09-07final2.jpg?format=2500w 2500w" loading="lazy" decoding="async" data-loader="sqs">

            
          
        
          
        

        
      
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  <p data-rte-preserve-empty="true"><strong>Image Title:</strong> Gecko and Friends</p><p data-rte-preserve-empty="true"><strong>Copyright:</strong> Dirk Fuchs</p><p data-rte-preserve-empty="true"><strong>Date image was taken:</strong> September 07, 2026</p><p data-rte-preserve-empty="true"><strong>Location:</strong> Eltville, Germany (Bortle 5)</p><p data-rte-preserve-empty="true"><strong>Data Acquisition Method:</strong> Personal Telescope Setup</p><p data-rte-preserve-empty="true"><strong>Description and Details:</strong> Apart from the Gecko Nebula itself and the dominating bright red hydrogen clouds the numerous „small“ background galaxies make this image special.<br><br>I collected the data for this image of the Gecko Nebula (LBN 437) in constellation Lacerta during 7 nights in August/September 2026 with a small refractor and an OSC camera from my balcony in Eltville, Germany - Bortle class 5.<br><br>The image represents 30.4 hours of total exposure time (15.9h without filter and 14.5h dual narrowband) - taken with following equipment:<br>telescope: Askar SQA85<br>camera: ZWO ASI2600MC Air<br>mount: ZWO AM5N<br>filter: Optolong L-eXtreme (Ha/OIII)<br><br>Stacked, cropped and processed with Siril (including GraXpert, RC Astro and VeraLux plugins), Ha channel from dual narrowband data added to RGB image with Continuum Subtraction.<br>Some final adjustments with Photoshop Elements.</p><p data-rte-preserve-empty="true"><strong>Name:</strong> Dirk Fuchs <br><strong>Website, Instagram or Facebook Profile: @deepsky.traveller</strong></p>]]></content:encoded><media:content type="image/jpeg" url="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/6b25a12e-9c45-46a7-81ed-ef31b0f843e4/LBN_437_478x120s_NF_2026-08-22_296x120s_LeXt_2026-09-07final2.jpg?format=1500w" medium="image" isDefault="true" width="1500" height="2310"><media:title type="plain">Gecko and Friends</media:title></media:content></item><item><title>IC 434 &amp; M42</title><category>2026</category><dc:creator>Charles Lillo</dc:creator><pubDate>Wed, 23 Sep 2026 04:00:24 +0000</pubDate><link>https://www.aapod2.com/blog/the-famous-horsehead-nebula-barnard-33</link><guid isPermaLink="false">5debd4b16fcd7b02905712ff:5debd4f1c2fab6555bff00b5:6ab282cbe46b96713fd2878f</guid><description><![CDATA[This wide-field view captures the famous Horsehead Nebula (Barnard 33), a 
dark cloud of dense interstellar dust silhouetted against the glowing red 
emission nebula IC 434 in the constellation Orion. Located roughly 1,300 to 
1,500 light-years away near the star Alnitak, the region is sculpted by 
intense radiation and stellar winds from nearby massive stars, which ionize 
the surrounding hydrogen gas and light up neighboring reflection nebulae 
like NGC 2023.]]></description><content:encoded><![CDATA[<figure class="
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                <img data-stretch="false" data-image="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/d761b8ed-d9b3-4d66-8f5b-e7084b1d57f6/103240.jpg" data-image-dimensions="10644x6872" data-image-focal-point="0.5,0.5" alt="" data-load="false" elementtiming="system-image-block" data-sqsp-image-classic-block-image src="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/d761b8ed-d9b3-4d66-8f5b-e7084b1d57f6/103240.jpg?format=1000w" width="10644" height="6872" sizes="(max-width: 640px) 100vw, (max-width: 767px) 100vw, 100vw" onload="this.classList.add(&quot;loaded&quot;)" srcset="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/d761b8ed-d9b3-4d66-8f5b-e7084b1d57f6/103240.jpg?format=100w 100w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/d761b8ed-d9b3-4d66-8f5b-e7084b1d57f6/103240.jpg?format=300w 300w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/d761b8ed-d9b3-4d66-8f5b-e7084b1d57f6/103240.jpg?format=500w 500w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/d761b8ed-d9b3-4d66-8f5b-e7084b1d57f6/103240.jpg?format=750w 750w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/d761b8ed-d9b3-4d66-8f5b-e7084b1d57f6/103240.jpg?format=1000w 1000w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/d761b8ed-d9b3-4d66-8f5b-e7084b1d57f6/103240.jpg?format=1500w 1500w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/d761b8ed-d9b3-4d66-8f5b-e7084b1d57f6/103240.jpg?format=2500w 2500w" loading="lazy" decoding="async" data-loader="sqs">

            
          
        
          
        

        
      
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  <p data-rte-preserve-empty="true"><strong>Image Title:</strong> IC &amp; M42</p><p data-rte-preserve-empty="true"><strong>Copyright:</strong> Olivier Bernard</p><p data-rte-preserve-empty="true"><strong>Date image was taken:</strong> September 19, 2026</p><p data-rte-preserve-empty="true"><strong>Location:</strong> Gourette 64 France Bortle 3</p><p data-rte-preserve-empty="true"><strong>Data Acquisition Method:</strong> Personal Telescope Setup</p><p data-rte-preserve-empty="true"><strong>Description and Details:</strong> Acquisition details: Astro-modified Canon EOS R6 with a Canon EF 300mm f/2.8L USM, mounted on a Sky-Watcher HEQ5 Pro and guided with a Lacerta MGEN-3. Antlia ALP-T Dual Band 5nm Highspeed filter. 70 × 300-second exposures, totalling 5 hours 50 minutes, captured from Gourette under Bortle 3 skies on September 18–19, 2026. Acquisition with APT and processing with PixInsight.</p><p data-rte-preserve-empty="true"><strong>Name:</strong> Olivier Bernard</p>]]></content:encoded><media:content type="image/jpeg" url="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/d761b8ed-d9b3-4d66-8f5b-e7084b1d57f6/103240.jpg?format=1500w" medium="image" isDefault="true" width="1500" height="968"><media:title type="plain">IC 434 &amp; M42</media:title></media:content></item><item><title>IC 2944 in (HS)(HS)OO palette</title><category>2026</category><dc:creator>Charles Lillo</dc:creator><pubDate>Tue, 22 Sep 2026 04:00:37 +0000</pubDate><link>https://www.aapod2.com/blog/running-chicken-nebula-ic-2944</link><guid isPermaLink="false">5debd4b16fcd7b02905712ff:5debd4f1c2fab6555bff00b5:6ab15ae01e80f2044917abeb</guid><description><![CDATA[In Thiago Prado's featured submission, the target for this technique is IC 
2944, also known as the Running Chicken Nebula.

Located in the southern constellation Centaurus, IC 2944 is an open cluster 
with an associated emission nebula characterized by intricate ionization 
fronts, dense dark globule structures (Bok globules), and subtle 
transitions between Sulfur-II and Hydrogen-alpha emissions.


The (SH)(SH)OO palette technique is a custom false-color composition method 
used in narrowband astrophotography to combine data captured through 
standard Sulfur-II, Hydrogen-alpha , and Oxygen-III filters.

It modifies the traditional SHO (Hubble Palette) and HOO color-mapping 
schemes to achieve better contrast, dynamic range, and highlight retention 
for intricate nebula structures.]]></description><content:encoded><![CDATA[<figure class="
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                <img data-stretch="false" data-image="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/3bf510e9-19c2-4cff-b042-f95c85cde9ba/SHOOD2.jpg" data-image-dimensions="4528x3713" data-image-focal-point="0.5,0.5" alt="" data-load="false" elementtiming="system-image-block" data-sqsp-image-classic-block-image src="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/3bf510e9-19c2-4cff-b042-f95c85cde9ba/SHOOD2.jpg?format=1000w" width="4528" height="3713" sizes="(max-width: 640px) 100vw, (max-width: 767px) 100vw, 100vw" onload="this.classList.add(&quot;loaded&quot;)" srcset="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/3bf510e9-19c2-4cff-b042-f95c85cde9ba/SHOOD2.jpg?format=100w 100w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/3bf510e9-19c2-4cff-b042-f95c85cde9ba/SHOOD2.jpg?format=300w 300w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/3bf510e9-19c2-4cff-b042-f95c85cde9ba/SHOOD2.jpg?format=500w 500w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/3bf510e9-19c2-4cff-b042-f95c85cde9ba/SHOOD2.jpg?format=750w 750w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/3bf510e9-19c2-4cff-b042-f95c85cde9ba/SHOOD2.jpg?format=1000w 1000w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/3bf510e9-19c2-4cff-b042-f95c85cde9ba/SHOOD2.jpg?format=1500w 1500w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/3bf510e9-19c2-4cff-b042-f95c85cde9ba/SHOOD2.jpg?format=2500w 2500w" loading="lazy" decoding="async" data-loader="sqs">

            
          
        
          
        

        
      
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  <p data-rte-preserve-empty="true"><strong>Image Title:</strong> IC 2944 in (HS)(HS)OO palette</p><p data-rte-preserve-empty="true"><strong>Copyright:</strong> Thiago Prado</p><p data-rte-preserve-empty="true"><strong>Date image was taken:</strong> April 24, 2026</p><p data-rte-preserve-empty="true"><strong>Location:</strong> Ponta Grossa, Paraná, Brazil.</p><p data-rte-preserve-empty="true"><strong>Data Acquisition Method:</strong> Personal Telescope Setup</p><p data-rte-preserve-empty="true"><strong>Description and Details:</strong> IC 2944, the Running Chicken Nebula, is an absolute joy to image. It features intricate detail that is typically rendered in HOO or SHO. For this capture, I experimented with a custom palette by creating a synthetic (SH) channel—combining the S and H channels based on a weighted average of their respective SNRs. Using this (SH) layer for Red and Luminance in an (SH)(SH)OO combination brought out subtle structures that standard blends often miss.<br><br>Setup: Askar 80 PhQ f/5.7, ASI2600MM, Optolong RGB filters for stars and SHO (7nm) filters. Total integration time: 11h 55min. Bortle 7.</p><p data-rte-preserve-empty="true"><strong>Name:</strong> Thiago Prado</p><p data-rte-preserve-empty="true"><strong>Website, Instagram or Facebook Profile:</strong> <a href="https://www.instagram.com/astro.ut/">https://www.instagram.com/astro.ut/</a></p>]]></content:encoded><media:content type="image/jpeg" url="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/1790023766942-7VPHNANZ4TLD32UZH9R6/SHOOD2.jpg?format=1500w" medium="image" isDefault="true" width="1500" height="1230"><media:title type="plain">IC 2944 in (HS)(HS)OO palette</media:title></media:content></item><item><title>Montes Apenninus</title><dc:creator>Charles Lillo</dc:creator><pubDate>Mon, 21 Sep 2026 04:00:03 +0000</pubDate><link>https://www.aapod2.com/blog/z5j2qi6mi2xnfkj3p5emgqaja8uhk1</link><guid isPermaLink="false">5debd4b16fcd7b02905712ff:5debd4f1c2fab6555bff00b5:6aafddeb157ef7269b6b78b8</guid><description><![CDATA[The Montes Apenninus (Lunar Apennines) is a rugged, prominent mountain 
range located on the northern near side of the Moon, forming the dramatic 
southeastern boundary of the vast Mare Imbrium (Sea of Rains) impact basin. 
Created roughly 3.9 billion years ago during the cataclysmic impact event 
that excavated the Imbrium basin, the range stretches for nearly 600 
kilometers (370 miles) and features towering peaks such as Mons Huygens, 
which rises about 5.5 kilometers high. Unlike Earth's tectonic mountain 
chains, these mountains represent the uplifted outer rim of a giant impact 
crater, characterized by steep, jagged scarps facing the smooth lava plains 
of Mare Imbrium and gentler, sloping topography descending into the lunar 
highlands.

Geologically, the range encompasses several notable features, including 
Hadley Rille (Rima Hadley)—a deep, sinuous lava channel winding along its 
northern base near Mons Hadley and Mons Hadley Delta. This region achieved 
historical fame as the landing site for the Apollo 15 mission in 1971, 
where astronauts David Scott and James Irwin explored the mountainous 
terrain and retrieved ancient deep-crustal lunar rock samples like the 
famous Genesis Rock. Flanked by prominent impact structures like the 
58-kilometer-wide Eratosthenes Crater at its southwestern tip and the 
nested Conon Crater, the Apennine range remains a prime geological showcase 
and a favorite target for amateur lunar observations.]]></description><content:encoded><![CDATA[<figure class="
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                <img data-stretch="false" data-image="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/86af04cd-47d5-4f2b-8c31-f69b62600590/Montes+Apenninus.jpg" data-image-dimensions="1897x2969" data-image-focal-point="0.5,0.5" alt="" data-load="false" elementtiming="system-image-block" data-sqsp-image-classic-block-image src="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/86af04cd-47d5-4f2b-8c31-f69b62600590/Montes+Apenninus.jpg?format=1000w" width="1897" height="2969" sizes="(max-width: 640px) 100vw, (max-width: 767px) 100vw, 100vw" onload="this.classList.add(&quot;loaded&quot;)" srcset="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/86af04cd-47d5-4f2b-8c31-f69b62600590/Montes+Apenninus.jpg?format=100w 100w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/86af04cd-47d5-4f2b-8c31-f69b62600590/Montes+Apenninus.jpg?format=300w 300w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/86af04cd-47d5-4f2b-8c31-f69b62600590/Montes+Apenninus.jpg?format=500w 500w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/86af04cd-47d5-4f2b-8c31-f69b62600590/Montes+Apenninus.jpg?format=750w 750w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/86af04cd-47d5-4f2b-8c31-f69b62600590/Montes+Apenninus.jpg?format=1000w 1000w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/86af04cd-47d5-4f2b-8c31-f69b62600590/Montes+Apenninus.jpg?format=1500w 1500w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/86af04cd-47d5-4f2b-8c31-f69b62600590/Montes+Apenninus.jpg?format=2500w 2500w" loading="lazy" decoding="async" data-loader="sqs">

            
          
        
          
        

        
      
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  <p data-rte-preserve-empty="true"><strong>Image Title:</strong> Montes Apenninus</p><p data-rte-preserve-empty="true"><strong>Copyright:</strong> BEMAN ASTROPHOTOGRAPHY</p><p data-rte-preserve-empty="true"><strong>Date image was taken:</strong> August 24, 2026</p><p data-rte-preserve-empty="true"><strong>Location:</strong> Gran Canaria, Canary Islands</p><p data-rte-preserve-empty="true"><strong>Data Acquisition Method:</strong> Personal Telescope Setup</p><p data-rte-preserve-empty="true"><strong>Description and Details:</strong> Equipment:<br>Telescope - SkyWatcher Newton Black Diamond 200/1000<br>Camera - PlayerOne Ares M-Pro<br>Mount - SkyWatcher EQ6-R Pro<br>Filter - Astronomik ProPlanet 642 BP IR-Pass 2"<br><br>Exposures: 500</p><p data-rte-preserve-empty="true"><strong>Name:</strong> BEMAN ASTROPHOTOGRAPHY</p><p data-rte-preserve-empty="true"><strong>Website, Instagram or Facebook Profile:</strong> <a href="https://www.instagram.com/bemanastrophotography">https://www.instagram.com/bemanastrophotography</a></p>]]></content:encoded><media:content type="image/jpeg" url="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/86af04cd-47d5-4f2b-8c31-f69b62600590/Montes+Apenninus.jpg?format=1500w" medium="image" isDefault="true" width="1500" height="2348"><media:title type="plain">Montes Apenninus</media:title></media:content></item><item><title>Werner and Aliacensis Craters</title><category>2026</category><dc:creator>Charles Lillo</dc:creator><pubDate>Sun, 20 Sep 2026 04:00:09 +0000</pubDate><link>https://www.aapod2.com/blog/werner-and-aliacensis-craters</link><guid isPermaLink="false">5debd4b16fcd7b02905712ff:5debd4f1c2fab6555bff00b5:6aaef2a8ebacdc5f43e4290b</guid><description><![CDATA[This high-resolution capture highlights the rugged terrain of the lunar 
southern highlands, featuring the prominent impact crater Werner alongside 
neighboring Aliacensis. Werner, measuring roughly 70 kilometers in 
diameter, displays striking structural details including crisp, terraced 
inner walls, a well-defined rim, and a sharp central peak complex rising 
from its floor. Surrounding the pair is a heavily pockmarked, ancient lunar 
landscape sculpted by billions of years of cosmic impacts.]]></description><content:encoded><![CDATA[<figure class="
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                <img data-stretch="false" data-image="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/4bc91e93-b360-4bc6-906f-ccba3c3208b6/Werner-AliacensisCraters.png" data-image-dimensions="1418x1192" data-image-focal-point="0.5,0.5" alt="" data-load="false" elementtiming="system-image-block" data-sqsp-image-classic-block-image src="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/4bc91e93-b360-4bc6-906f-ccba3c3208b6/Werner-AliacensisCraters.png?format=1000w" width="1418" height="1192" sizes="(max-width: 640px) 100vw, (max-width: 767px) 100vw, 100vw" onload="this.classList.add(&quot;loaded&quot;)" srcset="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/4bc91e93-b360-4bc6-906f-ccba3c3208b6/Werner-AliacensisCraters.png?format=100w 100w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/4bc91e93-b360-4bc6-906f-ccba3c3208b6/Werner-AliacensisCraters.png?format=300w 300w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/4bc91e93-b360-4bc6-906f-ccba3c3208b6/Werner-AliacensisCraters.png?format=500w 500w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/4bc91e93-b360-4bc6-906f-ccba3c3208b6/Werner-AliacensisCraters.png?format=750w 750w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/4bc91e93-b360-4bc6-906f-ccba3c3208b6/Werner-AliacensisCraters.png?format=1000w 1000w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/4bc91e93-b360-4bc6-906f-ccba3c3208b6/Werner-AliacensisCraters.png?format=1500w 1500w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/4bc91e93-b360-4bc6-906f-ccba3c3208b6/Werner-AliacensisCraters.png?format=2500w 2500w" loading="lazy" decoding="async" data-loader="sqs">

            
          
        
          
        

        
      
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  <p data-rte-preserve-empty="true"><strong>Image Title:</strong> Werner and Aliacensis Craters</p><p data-rte-preserve-empty="true"><strong>Copyright:</strong> AstroAndre</p><p data-rte-preserve-empty="true"><strong>Date image was taken:</strong> September 03, 2026</p><p data-rte-preserve-empty="true"><strong>Location:</strong> Cassino, Italy</p><p data-rte-preserve-empty="true"><strong>Data Acquisition Method:</strong> Personal Telescope Setup</p><p data-rte-preserve-empty="true"><strong>Description and Details:</strong> High-resolution view of the prominent lunar crater Werner, featuring its terraced walls and distinct central peak, surrounded by a heavily cratered landscape.<br><br>Equipment &amp; Capture Details:<br>- Telescope: Omegon Dobson Advanced X 203/1200<br>- Camera: ZWO ASI662MC<br>- Accessories: 2x Barlow Lens, UV/IR cut filter<br><br>Software &amp; Processing:<br>Captured 10000 frames on FireCapture, processed on PIPP, Autostakkert, WaveSharp3 and GIMP. ~1500 frames stacked.</p><p data-rte-preserve-empty="true"><strong>Name:</strong> Andrew Parisi</p><p data-rte-preserve-empty="true"><strong>Website, Instagram or Facebook Profile:</strong> <a href="https://www.instagram.com/_astroandre_/?utm_source=ig_web_button_share_sheet">https://www.instagram.com/_astroandre_/?utm_source=ig_web_button_share_sheet</a></p>]]></content:encoded><media:content type="image/png" url="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/4bc91e93-b360-4bc6-906f-ccba3c3208b6/Werner-AliacensisCraters.png?format=1500w" medium="image" isDefault="true" width="1418" height="1192"><media:title type="plain">Werner and Aliacensis Craters</media:title></media:content></item><item><title>A glimpse around the Total Solar Eclipse in Spain 2026</title><category>2026</category><dc:creator>Charles Lillo</dc:creator><pubDate>Sat, 19 Sep 2026 04:00:37 +0000</pubDate><link>https://www.aapod2.com/blog/2026-total-solar-eclipse-over-len-spain</link><guid isPermaLink="false">5debd4b16fcd7b02905712ff:5debd4f1c2fab6555bff00b5:6aadb2d57c6a8b52e3025df6</guid><description><![CDATA[Captured during the August 12, 2026 total solar eclipse over León, Spain, 
this composite image by Engelbert Vollmer showcases the ethereal solar 
corona flanked by the rapid transition phases of totality. To bring out the 
intricate details of the Sun's outer atmosphere—a superheated plasma 
stretching millions of kilometers along magnetic field lines—the photograph 
was crafted using an HDR (High Dynamic Range) sequence. By bracket-exposing 
shots in 1 EV increments from 1/1000 second to 1/2 second, the camera 
captured both the dazzling highlights of the solar photosphere and the 
delicate, faint streamers of the outer corona, which were then digitally 
blended together.

Flanking the central eclipse image are brief, fleeting phenomena that 
lasted only seconds before and after totality. These edge sequences capture 
Baily's beads—tiny, brilliant points of light created when the final rays 
of sunlight stream through the rugged peaks, craters, and valleys along the 
Moon's silhouetted rim. Interspersed alongside bright pink solar 
prominences, these glowing beads merge into the diamond ring effect just as 
the Sun slips completely behind the Moon, offering a spectacular visual 
summary of the eclipse's most dynamic moments.]]></description><content:encoded><![CDATA[<figure class="
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                <img data-stretch="false" data-image="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/3a7902ec-152b-4799-ad89-bc6b9cdb2c31/Solar+Eclipse+2026+Sequence.JPG" data-image-dimensions="5843x3572" data-image-focal-point="0.5,0.5" alt="" data-load="false" elementtiming="system-image-block" data-sqsp-image-classic-block-image src="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/3a7902ec-152b-4799-ad89-bc6b9cdb2c31/Solar+Eclipse+2026+Sequence.JPG?format=1000w" width="5843" height="3572" sizes="(max-width: 640px) 100vw, (max-width: 767px) 100vw, 100vw" onload="this.classList.add(&quot;loaded&quot;)" srcset="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/3a7902ec-152b-4799-ad89-bc6b9cdb2c31/Solar+Eclipse+2026+Sequence.JPG?format=100w 100w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/3a7902ec-152b-4799-ad89-bc6b9cdb2c31/Solar+Eclipse+2026+Sequence.JPG?format=300w 300w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/3a7902ec-152b-4799-ad89-bc6b9cdb2c31/Solar+Eclipse+2026+Sequence.JPG?format=500w 500w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/3a7902ec-152b-4799-ad89-bc6b9cdb2c31/Solar+Eclipse+2026+Sequence.JPG?format=750w 750w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/3a7902ec-152b-4799-ad89-bc6b9cdb2c31/Solar+Eclipse+2026+Sequence.JPG?format=1000w 1000w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/3a7902ec-152b-4799-ad89-bc6b9cdb2c31/Solar+Eclipse+2026+Sequence.JPG?format=1500w 1500w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/3a7902ec-152b-4799-ad89-bc6b9cdb2c31/Solar+Eclipse+2026+Sequence.JPG?format=2500w 2500w" loading="lazy" decoding="async" data-loader="sqs">

            
          
        
          
        

        
      
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  <p data-rte-preserve-empty="true"><strong>Image Title:</strong> A glimpse around the Total Solar Eclipse in Spain 2026</p><p data-rte-preserve-empty="true"><strong>Copyright:</strong> Engelbert Vollmer</p><p data-rte-preserve-empty="true"><strong>Date image was taken:</strong> August 12, 2026</p><p data-rte-preserve-empty="true"><strong>Location:</strong> León, Spain</p><p data-rte-preserve-empty="true"><strong>Data Acquisition Method:</strong> Personal Telescope Setup</p><p data-rte-preserve-empty="true"><strong>Description and Details:</strong> The crescent of the sun grows narrower and narrower. The last rays shine through lunar valleys for a few seconds. Protuberances suddenly sparkle in brilliant red. The corona becomes visible - the sun’s outer atmosphere. An extremely thin, hot plasma that extends millions of kilometers into space along the sun’s magnetic field lines. For us a hundred seconds filled with fascination. Suddenly it’s over; a blinding beam of light dazzles and expands. And then the Sun is back - a narrow crescent appears and slowly grows larger. And we know that the 250-kilometer drive from our hotel on the rainy coast to León, Spain, was well worth it.<br><br>My sequence shows the corona as an HDR image taken in 1 EV increments from 1/1000 to 1/2 second. The sections to the left and right of the corona last only a few seconds—12 seconds on the left and 6 seconds on the right.</p><p data-rte-preserve-empty="true"><strong>Name:</strong> Engelbert Vollmer</p>]]></content:encoded><media:content type="image/jpeg" url="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/3a7902ec-152b-4799-ad89-bc6b9cdb2c31/Solar+Eclipse+2026+Sequence.JPG?format=1500w" medium="image" isDefault="true" width="1500" height="917"><media:title type="plain">A glimpse around the Total Solar Eclipse in Spain 2026</media:title></media:content></item><item><title>NCG 7023 IRIS NEBULA</title><category>2026</category><dc:creator>Charles Lillo</dc:creator><pubDate>Fri, 18 Sep 2026 04:00:24 +0000</pubDate><link>https://www.aapod2.com/blog/8lrz38kusb6rri1905d6ykamwiw31o</link><guid isPermaLink="false">5debd4b16fcd7b02905712ff:5debd4f1c2fab6555bff00b5:6aabf3e483d0c00d48f7e7f6</guid><description><![CDATA[The Iris Nebula (NGC 7023 or Caldwell 4) is a striking reflection nebula 
located roughly 1,300 to 1,400 light-years from Earth in the northern 
constellation Cepheus. Unlike emission nebulae that glow from ionized gas, 
the Iris Nebula shines by scattering starlight off vast clouds of 
interstellar dust. At its core lies HD 200775, a massive, hot, young star 
about ten times the mass of the Sun that provides the main illumination for 
the surrounding material. This glowing dust and gas spans approximately six 
light-years across, forming petal-like structures that give the nebula its 
distinctive flower-like appearance in deep-space imagery.]]></description><content:encoded><![CDATA[<figure class="
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                <img data-stretch="false" data-image="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/c3f5d673-df76-45ac-b991-2c8f236f297d/IRIS+5+NM.jpg" data-image-dimensions="2712x2557" data-image-focal-point="0.5,0.5" alt="" data-load="false" elementtiming="system-image-block" data-sqsp-image-classic-block-image src="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/c3f5d673-df76-45ac-b991-2c8f236f297d/IRIS+5+NM.jpg?format=1000w" width="2712" height="2557" sizes="(max-width: 640px) 100vw, (max-width: 767px) 100vw, 100vw" onload="this.classList.add(&quot;loaded&quot;)" srcset="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/c3f5d673-df76-45ac-b991-2c8f236f297d/IRIS+5+NM.jpg?format=100w 100w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/c3f5d673-df76-45ac-b991-2c8f236f297d/IRIS+5+NM.jpg?format=300w 300w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/c3f5d673-df76-45ac-b991-2c8f236f297d/IRIS+5+NM.jpg?format=500w 500w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/c3f5d673-df76-45ac-b991-2c8f236f297d/IRIS+5+NM.jpg?format=750w 750w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/c3f5d673-df76-45ac-b991-2c8f236f297d/IRIS+5+NM.jpg?format=1000w 1000w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/c3f5d673-df76-45ac-b991-2c8f236f297d/IRIS+5+NM.jpg?format=1500w 1500w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/c3f5d673-df76-45ac-b991-2c8f236f297d/IRIS+5+NM.jpg?format=2500w 2500w" loading="lazy" decoding="async" data-loader="sqs">

            
          
        
          
        

        
      
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  <p data-rte-preserve-empty="true"><strong>Image Title:</strong> NCG 7023 IRIS NEBULA</p><p data-rte-preserve-empty="true"><strong>Copyright:</strong> George Chatzifrantzis</p><p data-rte-preserve-empty="true"><strong>Date image was taken:</strong> August 07, 2026</p><p data-rte-preserve-empty="true"><strong>Location:</strong> Chalkidiki - Greece</p><p data-rte-preserve-empty="true"><strong>Data Acquisition Method:</strong> Personal Telescope Setup</p><p data-rte-preserve-empty="true"><strong>Description and Details:</strong> Equipment :<br>OTA : Celestron C11 XLT<br>Mount : Skywatcher EQ8<br>Camera : ZWO 533mm<br>Filters : Astronomik CLS,R,G,B<br>Guiding : Stellarvue SV80ST2 via Lodestar X2<br>Software : Dss - Pix - Ps<br>Exposure :<br>L : 22h30m<br>RGB : 3h<br>Location : Interstellar Observatory - Greece</p><p data-rte-preserve-empty="true"><strong>Name:</strong> George Chatzifrantzis</p><p data-rte-preserve-empty="true"><strong>Website, Instagram or Facebook Profile:</strong> <a href="https://www.facebook.com/GeorgeChatzifrantzis?locale=el_GR">https://www.facebook.com/GeorgeChatzifrantzis?locale=el_GR</a></p>]]></content:encoded><media:content type="image/jpeg" url="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/c3f5d673-df76-45ac-b991-2c8f236f297d/IRIS+5+NM.jpg?format=1500w" medium="image" isDefault="true" width="1500" height="1414"><media:title type="plain">NCG 7023 IRIS NEBULA</media:title></media:content></item><item><title>Owl Star Cluster NGC 457</title><category>2026</category><dc:creator>Charles Lillo</dc:creator><pubDate>Thu, 17 Sep 2026 04:00:14 +0000</pubDate><link>https://www.aapod2.com/blog/owl-star-cluster-ngc-457</link><guid isPermaLink="false">5debd4b16fcd7b02905712ff:5debd4f1c2fab6555bff00b5:6aaa9bc00920ee13b33e4670</guid><description><![CDATA[In the heart of the constellation Cassiopeia, approximately 7,900 
light-years from Earth, lies NGC 457, one of the most striking open 
clusters in the autumn sky. Known by the nicknames "Owl Cluster" or "ET 
Cluster," this group of stars immediately catches the eye due to the 
peculiar arrangement of its stars, which appear to outline the silhouette 
of a creature with large, bright eyes.]]></description><content:encoded><![CDATA[<figure class="
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  <p data-rte-preserve-empty="true"><strong>Image Title:</strong> Owl Star Cluster NGC 457</p><p data-rte-preserve-empty="true"><strong>Copyright:</strong> giacomo pro'</p><p data-rte-preserve-empty="true"><strong>Date image was taken:</strong> August 20, 2026</p><p data-rte-preserve-empty="true"><strong>Location:</strong> Torricella (TA) ITALY</p><p data-rte-preserve-empty="true"><strong>Data Acquisition Method:</strong> Personal Telescope Setup</p><p data-rte-preserve-empty="true"><strong>Description and Details:</strong> Nel cuore della costellazione di Cassiopea, a circa 7.900 anni luce dalla Terra, si trova NGC 457, uno degli ammassi aperti più suggestivi del cielo autunnale. Conosciuto con i soprannomi di Ammasso della Civetta o ET Cluster, questo gruppo di stelle colpisce immediatamente per la particolare disposizione dei suoi astri, che sembra delineare la sagoma di una creatura dalle grandi orbite luminose.<br>Scoperto da William Herschel nel 1787, NGC 457 è un giovane ammasso aperto, composto da numerose stelle nate dalla stessa nube di gas e legate ancora dalla gravità. La sua età relativamente giovane, stimata in alcune decine di milioni di anni, fa sì che tra le sue componenti siano presenti stelle molto luminose e massicce.<br>A dominare la scena sono Phi Cassiopeiae e HD 7902, due stelle particolarmente brillanti che contribuiscono a formare quelli che, nella celebre interpretazione figurativa, sembrano essere i grandi occhi della Civetta. La loro luminosità contrasta con quella delle numerose stelle più deboli che compongono il corpo e le "ali" dell'ammasso.<br>La forma che riconosciamo nell'immagine è naturalmente una straordinaria pareidolia cosmica: non esiste una struttura fisica che leghi le stelle secondo il disegno della Civetta. È la loro casuale disposizione prospettica, osservata dalla Terra, a creare questa figura così riconoscibile e affascinante.<br>NGC 457 rappresenta quindi uno degli esempi più belli di come l'astronomia possa incontrare l'immaginazione: un insieme di stelle nate dalla stessa nube interstellare che, a migliaia di anni luce di distanza, sembra trasformarsi nei grandi occhi di una creatura che osserva silenziosamente il cosmo.<br><br><strong>Description &amp; Details Translation</strong></p><p data-rte-preserve-empty="true">In the heart of the constellation Cassiopeia, approximately 7,900 light-years from Earth, lies NGC 457, one of the most striking open clusters in the autumn sky. Known by the nicknames "Owl Cluster" or "ET Cluster," this group of stars immediately catches the eye due to the peculiar arrangement of its stars, which appear to outline the silhouette of a creature with large, bright eyes.</p><p data-rte-preserve-empty="true">Discovered by William Herschel in 1787, NGC 457 is a young open cluster composed of numerous stars born from the same gas cloud and held together by gravity. Its relatively young age, estimated at a few tens of millions of years, means that very bright and massive stars are present among its components.</p><p data-rte-preserve-empty="true">Dominating the scene are Phi Cassiopeiae and HD 7902, two particularly brilliant stars that help form what, in the famous figurative interpretation, appear to be the Owl's large eyes. Their brightness contrasts with the numerous fainter stars that make up the body and "wings" of the cluster.</p><p data-rte-preserve-empty="true">The shape we recognize in the image is, of course, an extraordinary cosmic pareidolia: there is no physical structure linking the stars in the shape of an owl. It is their accidental perspective arrangement, as observed from Earth, that creates this recognizable and fascinating figure.</p><p data-rte-preserve-empty="true">NGC 457 thus represents one of the finest examples of how astronomy can meet imagination: a group of stars born from the same interstellar cloud that, thousands of light-years away, appears to transform into the large eyes of a creature silently observing the cosmos.<br> Light: 65 x 60 seconds<br> Filter: Optolong L-QEF<br> Camera: Asi 294 mc pro<br> Telescope: Sky-Watcher 200/1000 PDS (CUSTOM)<br> Mount: Skywatcher Eq 6-r Pro<br> Acquisition: Asiair Plus<br> Software: DSS - Pixinsight – Photoshop<br> Shots: 20/08/2026<br> Location: Torricella (TA) ITALY<br> Sky Bortle: 6<br> Author: PRO’ GIACOMO.</p><p data-rte-preserve-empty="true"><strong>Name:</strong> giacomo pro'</p><p data-rte-preserve-empty="true"><strong>Website, Instagram or Facebook Profile:</strong> <a href="https://www.facebook.com/giacomo.pro">https://www.facebook.com/giacomo.pro</a></p>]]></content:encoded><media:content type="image/jpeg" url="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/55083c0a-730c-4b64-a7c2-e53d0b008c58/NGC+457.jpg?format=1500w" medium="image" isDefault="true" width="1500" height="1079"><media:title type="plain">Owl Star Cluster NGC 457</media:title></media:content></item></channel></rss>