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<!--Generated by Site-Server v@build.version@ (http://www.squarespace.com) on Wed, 26 Aug 2026 04:43:46 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>Tue, 25 Aug 2026 20:53:33 +0000</lastBuildDate><language>en-US</language><generator>Site-Server v@build.version@ (http://www.squarespace.com)</generator><description><![CDATA[]]></description><item><title>MWP1 and ALV1: Ancient Planetary Nebulae in Cygnus</title><category>2026</category><dc:creator>Charles Lillo</dc:creator><pubDate>Wed, 26 Aug 2026 04:00:43 +0000</pubDate><link>https://www.aapod2.com/blog/mwp1-and-alv1</link><guid isPermaLink="false">5debd4b16fcd7b02905712ff:5debd4f1c2fab6555bff00b5:6a8c4c062359447689949095</guid><description><![CDATA[This narrowband deep-field image highlights two faint planetary nebulae 
situated against a rich background of ionized gas clouds in the 
constellation Cygnus. Near the lower-center of the field sits MWP1, an 
extraordinarily large and ancient bipolar planetary nebula (~150,000 years 
old) glowing with prominent bluish-cyan Oxygen-III shell emissions. Just to 
its lower-left lies ALV1, a fainter, asymmetric planetary nebula shaped by 
surrounding stellar winds. The surrounding field is swept with intricate 
red Hydrogen-alpha filaments and faint cosmic dust, creating a striking 
dual-color contrast across the star-studded field.]]></description><content:encoded><![CDATA[<figure class="
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                <img data-stretch="false" data-image="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/e06be2b5-0669-4ec6-bf06-5b94cb51c04c/MWP1scaled50.png" data-image-dimensions="3096x2053" 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/e06be2b5-0669-4ec6-bf06-5b94cb51c04c/MWP1scaled50.png?format=1000w" width="3096" height="2053" 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/e06be2b5-0669-4ec6-bf06-5b94cb51c04c/MWP1scaled50.png?format=100w 100w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/e06be2b5-0669-4ec6-bf06-5b94cb51c04c/MWP1scaled50.png?format=300w 300w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/e06be2b5-0669-4ec6-bf06-5b94cb51c04c/MWP1scaled50.png?format=500w 500w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/e06be2b5-0669-4ec6-bf06-5b94cb51c04c/MWP1scaled50.png?format=750w 750w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/e06be2b5-0669-4ec6-bf06-5b94cb51c04c/MWP1scaled50.png?format=1000w 1000w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/e06be2b5-0669-4ec6-bf06-5b94cb51c04c/MWP1scaled50.png?format=1500w 1500w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/e06be2b5-0669-4ec6-bf06-5b94cb51c04c/MWP1scaled50.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> MWP1 and ALV1</p><p data-rte-preserve-empty="true"><strong>Copyright:</strong> Alexandros Filothodoros</p><p data-rte-preserve-empty="true"><strong>Date image was taken:</strong> July 29, 2026</p><p data-rte-preserve-empty="true"><strong>Location:</strong> Zielona Góra, 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> MWP1 is an ancient and unusually large bipolar planetary nebula in Cygnus, located roughly 4,500 light-years away. Its estimated age is around 150,000 years, much longer than the typical lifespan of planetary nebulae. ALV1 is another faint planetary nebula in the same field, featuring an asymmetric shape likely caused by stellar winds.<br><br>Capturing this signal presented extra challenges, as the data was acquired during summer's "white nights," and the Ha shots, in particular, were taken under an almost full Moon.<br><br>Exposure Data:<br>Ha: 62 x 600 sec (10.3 hours)<br>OIII: 46 x 600 sec (7.6 hours)<br>Total Integration Time: 18 hours<br>Equipment:<br>Telescope: Askar 65PHQ<br>Camera: Player One Poseidon-M Pro<br>Mount: Pegasus Astro NYX-88 Harmonic Gear Mount<br>Filters: Antlia 3nm Ha Antlia 3nm OIII<br>Filter Wheel: Player One Phoenix Wheel 7x36mm</p><p data-rte-preserve-empty="true"><strong>Name:</strong> Alexandros Filothodoros</p><p data-rte-preserve-empty="true"><strong>Website or Facebook Profile:</strong> <a target="_blank" href="http://www.facebook.com/alex.filothodoros">http://www.facebook.com/alex.filothodoros</a></p>]]></content:encoded><media:content type="image/png" url="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/e06be2b5-0669-4ec6-bf06-5b94cb51c04c/MWP1scaled50.png?format=1500w" medium="image" isDefault="true" width="1500" height="995"><media:title type="plain">MWP1 and ALV1: Ancient Planetary Nebulae in Cygnus</media:title></media:content></item><item><title>The Deer Lick Group (NGC 7331) &amp; Stephan’s Quintet (HCG 92) in a Sea of IFN</title><category>2026</category><dc:creator>Charles Lillo</dc:creator><pubDate>Tue, 25 Aug 2026 04:00:11 +0000</pubDate><link>https://www.aapod2.com/blog/w577jqajvtdk3byev5zo0545qf6me7</link><guid isPermaLink="false">5debd4b16fcd7b02905712ff:5debd4f1c2fab6555bff00b5:6a8c481cf703d4271b7844ba</guid><description><![CDATA[This deep-field astrophotography image captures a rich section of the night 
sky featuring the prominent spiral galaxy NGC 7331 (the anchor of the Deer 
Lick Group), visible near the right-center with its bright core, pronounced 
dust lanes, and elongated disk. Accompanied by smaller background companion 
galaxies, the region is set against a faint, intricate web of Integrated 
Flux Nebula (IFN)—dust clouds residing high above the Milky Way's galactic 
plane that reflect the combined starlight of our galaxy. Nearby within the 
same field sits Stephan’s Quintet (HCG 92), a famous compact group of 
interacting galaxies showing tidal tails and gravitational distortion. The 
dark backdrop of deep space is filled with a dense field of distant 
background galaxies and pinpoint field 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/ac461bdb-1a27-4957-845e-3f9419fd4c72/Ruleofthirds.jpg" data-image-dimensions="5000x3750" 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/ac461bdb-1a27-4957-845e-3f9419fd4c72/Ruleofthirds.jpg?format=1000w" width="5000" height="3750" 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/ac461bdb-1a27-4957-845e-3f9419fd4c72/Ruleofthirds.jpg?format=100w 100w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/ac461bdb-1a27-4957-845e-3f9419fd4c72/Ruleofthirds.jpg?format=300w 300w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/ac461bdb-1a27-4957-845e-3f9419fd4c72/Ruleofthirds.jpg?format=500w 500w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/ac461bdb-1a27-4957-845e-3f9419fd4c72/Ruleofthirds.jpg?format=750w 750w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/ac461bdb-1a27-4957-845e-3f9419fd4c72/Ruleofthirds.jpg?format=1000w 1000w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/ac461bdb-1a27-4957-845e-3f9419fd4c72/Ruleofthirds.jpg?format=1500w 1500w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/ac461bdb-1a27-4957-845e-3f9419fd4c72/Ruleofthirds.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> The Deer Lick Group (NGC 7331) &amp; Stephan’s Quintet (HCG 92) in a Sea of IFN — LRGB from Vermont</p><p data-rte-preserve-empty="true"><strong>Copyright:</strong> Michele Bayliss</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> Weybridge, VT</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> **Integration:**<br>L: 16h 25m<br>R: 8h 40m<br>G: 9h 10m<br>B: 7h 30m<br>**Total: 41h 45m**<br><br>**Image Description:**<br>This two-year project captures NGC 7331 and the Deer Lick Group immersed in the extremely faint galactic cirrus and integrated flux nebula surrounding the field. The image also includes Stephan’s Quintet (HCG 92). Data from the first season captured Type Ia supernova SN 2025rbs near the center of NGC 7331, and its signal remains within the final two-year integration.</p><p data-rte-preserve-empty="true"><strong>Name:</strong> Michele Bayliss</p><p data-rte-preserve-empty="true"><strong>Website, Instagram or Facebook Profile: </strong><a href="https://www.instagram.com/captured.cosmos/">@captured.cosmos</a></p>]]></content:encoded><media:content type="image/jpeg" url="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/ac461bdb-1a27-4957-845e-3f9419fd4c72/Ruleofthirds.jpg?format=1500w" medium="image" isDefault="true" width="1500" height="1125"><media:title type="plain">The Deer Lick Group (NGC 7331) &amp; Stephan’s Quintet (HCG 92) in a Sea of IFN</media:title></media:content></item><item><title>Saturn: Enceladus in transit and a cross-checked white spot</title><category>2026</category><dc:creator>Charles Lillo</dc:creator><pubDate>Mon, 24 Aug 2026 04:00:38 +0000</pubDate><link>https://www.aapod2.com/blog/saturn-enceladus-in-transit-and-a-cross-checked-white-spot</link><guid isPermaLink="false">5debd4b16fcd7b02905712ff:5debd4f1c2fab6555bff00b5:6a885b82527c682c49529078</guid><description><![CDATA[Captured on July 31, 2026, from Tunis, Tunisia, this detailed planetary 
observation of Saturn reveals a transient atmospheric white spot in the 
northern hemisphere, independently cross-checked and confirmed across two 
distinct optical setups. Simultaneous imaging via a 14-inch Celestron 
EdgeHD and a 16-inch Sky-Watcher Dobsonian utilizing four distinct filter 
configurations detected the feature at identical planetary coordinates; its 
persistence across deeper infrared wavelengths and higher-altitude 
Rayleigh-scattering bands indicates a vertically extended convective storm 
cell tied to seasonal northern atmospheric dynamics rather than a localized 
surface albedo artifact. The high-resolution composite additionally 
resolves fine internal ring dynamics—notably faint radial spokes in the B 
ring and a crisp Cassini Division separating it from the A ring—while 
capturing Enceladus in mid-transit alongside Tethys and Mimas positioned to 
the east. The overall data integration of 6 minutes and 40 seconds was 
processed using WinJUPOS, AutoStakkert!, and PixInsight to maximize 
cloud-deck contrast and optical alignment.]]></description><content:encoded><![CDATA[<figure class="
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                <img data-stretch="false" data-image="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/6eeaee68-9717-40b2-94f9-586d3db129c7/2026-07-31-0211_RGB_IR642_RP_SP_V06_Artifacts+Corrected.png" data-image-dimensions="1092x873" 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/6eeaee68-9717-40b2-94f9-586d3db129c7/2026-07-31-0211_RGB_IR642_RP_SP_V06_Artifacts+Corrected.png?format=1000w" width="1092" height="873" 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/6eeaee68-9717-40b2-94f9-586d3db129c7/2026-07-31-0211_RGB_IR642_RP_SP_V06_Artifacts+Corrected.png?format=100w 100w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/6eeaee68-9717-40b2-94f9-586d3db129c7/2026-07-31-0211_RGB_IR642_RP_SP_V06_Artifacts+Corrected.png?format=300w 300w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/6eeaee68-9717-40b2-94f9-586d3db129c7/2026-07-31-0211_RGB_IR642_RP_SP_V06_Artifacts+Corrected.png?format=500w 500w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/6eeaee68-9717-40b2-94f9-586d3db129c7/2026-07-31-0211_RGB_IR642_RP_SP_V06_Artifacts+Corrected.png?format=750w 750w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/6eeaee68-9717-40b2-94f9-586d3db129c7/2026-07-31-0211_RGB_IR642_RP_SP_V06_Artifacts+Corrected.png?format=1000w 1000w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/6eeaee68-9717-40b2-94f9-586d3db129c7/2026-07-31-0211_RGB_IR642_RP_SP_V06_Artifacts+Corrected.png?format=1500w 1500w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/6eeaee68-9717-40b2-94f9-586d3db129c7/2026-07-31-0211_RGB_IR642_RP_SP_V06_Artifacts+Corrected.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> Saturn: Enceladus in transit and a cross-checked white spot</p><p data-rte-preserve-empty="true"><strong>Copyright:</strong> Makrem Larnaout &amp; Hafedh Driss</p><p data-rte-preserve-empty="true"><strong>Date image was taken:</strong> July 31, 2026</p><p data-rte-preserve-empty="true"><strong>Location:</strong> Tunis, Tunisia</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> A bright feature in the northern hemisphere, confirmed on two independent setups with matching position and morphology.<br>Telescope 1: SkyWatcher Dobsonian 16" + GreatStar ADK (modified eADK, Arduino based auto correction/autopilot) + Televue Powermate x4 + Player One C II (color) + Baader UV/IR cut filter + Player One M II (mono) + Sloan S'. 30 min integration.<br><br>Telescope 2: Celestron C14 EdgeHD + GreatStar ADK (modified eADK, Arduino based auto correction/autopilot) + Televue Powermate x2 + ZWO ASI462MM (mono), IR 642nm and Sloan R' filters. 30 min integration.<br><br>2 telescopes, 3 cameras, 4 filter configurations, consistent detection across all of them. IR642 penetrates deeper into cloud opacity layers, R'/S' are more sensitive to high altitude Rayleigh scattering; presence across both bands points to a vertically extended structure rather than a simple albedo variation, consistent with a small scale convective cell/storm tied to seasonal NH activity.<br><br>Rings: the B ring shows fine internal structure with faint radial spokes, alongside a clean, well defined Cassini Division separating it from the A ring.<br><br>Moons: Enceladus in transit, Tethys and Mimas visible to the east.<br><br>by Makrem Larnaout, Daniel H. DRISS<br><br>Published: Aug 2, 2026<br><br>Total integration: 6m 40s<br><br>Integration per filter:<br>- UV/IR Cut: 1m 40s (10000 × 0.01")<br>- Planetary: 1m 40s (10000 × 0.01")<br>- Photometric R: 1m 40s (10000 × 0.01")<br>- Baader SLOAN/SDSS-z_s' 1.25": 1m 40s (10000 × 0.01")<br><br>Equipment:<br>- Optics: Celestron EdgeHD 14", Sky-Watcher DOB 16" SynScan<br>- Cameras: Player One Mars-C, Player One Mars-M II, ZWO ASI462MM<br>- Mounts: JTW Astronomy Trident GTR, Sky-Watcher Dobson telescope N 305/1500 Skyliner FlexTube BD DOB GoTo<br>- Filters: Astronomik ProPlanet 642 BP IR-Pass 1.25", Baader SLOAN/SDSS-r' 1.25", Baader SLOAN/SDSS-z_s' 1.25", Baader UV/IR Cut / Luminance 1.25"<br>- Accessories: Greatstar ADK, Tele Vue 2x 1.25" Barlow (BLW-2125), Tele Vue 4.0x 2" Powermate (PMT-4201), ZWO EAF, ZWO EFW 7 x 2″, ZWO EFW mini (5 x 1.25″ / 5 x 31mm)<br>- Software: Adobe Photoshop, Emil Kraaikamp AutoStakkert!, Grischa Hahn WinJUPOS, Pleiades Astrophoto PixInsight, Torsten Edelmann FireCapture</p><p data-rte-preserve-empty="true"><strong>Name:</strong> Makrem Larnaout</p><p data-rte-preserve-empty="true"><strong>Website or Facebook Profile:</strong> <a target="_blank" href="http://www.facebook.com/makrem.larnaout">http://www.facebook.com/makrem.larnaout</a></p>]]></content:encoded><media:content type="image/png" url="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/6eeaee68-9717-40b2-94f9-586d3db129c7/2026-07-31-0211_RGB_IR642_RP_SP_V06_Artifacts+Corrected.png?format=1500w" medium="image" isDefault="true" width="1092" height="873"><media:title type="plain">Saturn: Enceladus in transit and a cross-checked white spot</media:title></media:content></item><item><title>The Dragon Has Returned to the Universe</title><category>2026</category><dc:creator>Charles Lillo</dc:creator><pubDate>Sun, 23 Aug 2026 04:00:10 +0000</pubDate><link>https://www.aapod2.com/blog/ngc6188-the-fighting-dragons-of-ara-in-narrowband-shoxl2fmxoxv5h0</link><guid isPermaLink="false">5debd4b16fcd7b02905712ff:5debd4f1c2fab6555bff00b5:6a8859b8eacc05285b439c1c</guid><description><![CDATA[Captured from Georgetown, New South Wales, Australia, between July 14 and 
July 22, 2026, this high-resolution narrowband image details NGC 6188, an 
active star-forming emission nebula located approximately 4,000 light-years 
away in the constellation Ara. Rendered in the Hubble Palette (SHO) with 
broad-band RGB star data for natural color accuracy, the false-color 
composite highlights distinct ionization fronts driven by the massive, 
young stars of the embedded open cluster NGC 6193. Strong stellar winds and 
intense ultraviolet radiation carve dark, dense dust structures while 
exciting surrounding atomic gases, mapped here as sulfur II (red), 
hydrogen-alpha (green/gold), and oxygen III (blue). Acquired using a fast 
RASA 1100 V2 telescope paired with a full-frame ZWO ASI6200MM-Pro camera on 
an EQ6R-Pro mount, the image integrates 29.5 hours of total exposure (1,761 
individual sub-frames) processed in PixInsight to resolve intricate shock 
fronts, dark globule boundaries, and subtle elemental boundaries across the 
region.]]></description><content:encoded><![CDATA[<figure class="
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                <img data-stretch="false" data-image="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/3ed0e51a-bbb4-44b7-9910-cda3db17a3c9/2026+DRAGONS+CROP01-80.jpg" data-image-dimensions="4950x3302" 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/3ed0e51a-bbb4-44b7-9910-cda3db17a3c9/2026+DRAGONS+CROP01-80.jpg?format=1000w" width="4950" height="3302" 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/3ed0e51a-bbb4-44b7-9910-cda3db17a3c9/2026+DRAGONS+CROP01-80.jpg?format=100w 100w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/3ed0e51a-bbb4-44b7-9910-cda3db17a3c9/2026+DRAGONS+CROP01-80.jpg?format=300w 300w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/3ed0e51a-bbb4-44b7-9910-cda3db17a3c9/2026+DRAGONS+CROP01-80.jpg?format=500w 500w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/3ed0e51a-bbb4-44b7-9910-cda3db17a3c9/2026+DRAGONS+CROP01-80.jpg?format=750w 750w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/3ed0e51a-bbb4-44b7-9910-cda3db17a3c9/2026+DRAGONS+CROP01-80.jpg?format=1000w 1000w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/3ed0e51a-bbb4-44b7-9910-cda3db17a3c9/2026+DRAGONS+CROP01-80.jpg?format=1500w 1500w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/3ed0e51a-bbb4-44b7-9910-cda3db17a3c9/2026+DRAGONS+CROP01-80.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> The Dragon Has Returned to the Universe</p><p data-rte-preserve-empty="true"><strong>Copyright:</strong> Ando Anderso</p><p data-rte-preserve-empty="true"><strong>Date image was taken:</strong> July 22, 2026</p><p data-rte-preserve-empty="true"><strong>Location:</strong> Georgetown, Newcastle, NSW, Australia, Earth</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> NGC6188 - The Fighting Dragons of Ara. In Narrowband SHO.<br>Sub Frames - RGB used to get the correct star colours.<br>Red 138 x 10sec<br>Green 144 x 10sec<br>Blue 150 x 10sec<br>Sub Frames - Narrowband, to get the nebula gas colour separation<br>Ha 364 x 60sec<br>S2 599 x 60sec<br>O3 726 x 60sec<br>Total subs 1761mins or 29.5hours.<br>Captured from the 14th of July to the 22nd of July 2026.<br>Telescope - RASA 1100V2 620mm focal @ F2.2<br>Camera - ZWO ASI6200MM-PRO 62mPix full frame<br>Mount - EQ6R-PRO<br>Processed in Pixinsight and Affinity.</p><p data-rte-preserve-empty="true"><strong>Name:</strong> Mark Anderson</p><p data-rte-preserve-empty="true"><strong>Website or Facebook Profile:</strong> <a target="_blank" href="http://thenas.com.au/">http://theNAS.com.au</a></p><p data-rte-preserve-empty="true"></p>]]></content:encoded><media:content type="image/jpeg" url="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/3ed0e51a-bbb4-44b7-9910-cda3db17a3c9/2026+DRAGONS+CROP01-80.jpg?format=1500w" medium="image" isDefault="true" width="1500" height="1001"><media:title type="plain">The Dragon Has Returned to the Universe</media:title></media:content></item><item><title>Full Moon</title><category>2026</category><dc:creator>Charles Lillo</dc:creator><pubDate>Sat, 22 Aug 2026 04:00:42 +0000</pubDate><link>https://www.aapod2.com/blog/full-moon</link><guid isPermaLink="false">5debd4b16fcd7b02905712ff:5debd4f1c2fab6555bff00b5:6a885885e829ab2d4edc2800</guid><description><![CDATA[Captured from Faggiano, Italy, on July 29, 2026, this high-resolution lunar 
mosaic details the near side of Earth's Moon during the full phase. 
Acquired using an SVBONY MK127 telescope at its native 1,500 mm focal 
length paired with a ZWO ASI224 camera, the final image is a mosaic 
assembled from 30 individual video panels. To mitigate atmospheric 
distortion while target was positioned roughly 25 degrees above the 
horizon, 4,000 frames were recorded per panel at a 3.0 ms exposure time, 
from which the sharpest 1,500 frames were selected and stacked. The 
resulting composite showcases key geological structures with exceptional 
contrast and resolution, including dark, volcanic basalt plains (maria), 
heavily cratered highlands, and bright, extensive impact ejecta rays 
emanating from geologically young craters.]]></description><content:encoded><![CDATA[<figure class="
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  <p data-rte-preserve-empty="true"><strong>Image Title:</strong> Full Moon</p><p data-rte-preserve-empty="true"><strong>Copyright:</strong> Raffaele Calcagno &amp; Francesco Nesca</p><p data-rte-preserve-empty="true"><strong>Date image was taken:</strong> July 29, 2026</p><p data-rte-preserve-empty="true"><strong>Location:</strong> Faggiano (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>&nbsp;&nbsp;Full Moon<br><br>&nbsp;On the night of July 29, 2026, while chatting and enjoying a few beers with Francesco Nesca, we came up with the idea for a new project. We decided to dedicate the entire night to our natural satellite, creating a high-resolution lunar mosaic that ultimately reached 425 GB of data, spread across 30 videos of 4,000 frames each, from which 1,500 of the best frames were selected and stacked for every single panel.<br><br>It was also the perfect opportunity to capture the first light of this fantastic SVBONY MK127 at its native 1500 mm focal length. The Moon was about 25° above the horizon, the night was pleasantly cool, providing moments of steadier seeing, and under these conditions we successfully completed the acquisition.<br><br>From there, the longest and quietest part began: processing every single video, frame by frame, until the final assembly of the mosaic, which was entirely processed by me.<br><br>I hope you enjoy it!<br><br>&nbsp;Technical Data<br><br>Telescope / Mount: SVBONY MK127 on HEQ5 Pro<br>Camera: ZWO ASI224<br>Filter: SVBONY UV/IR Cut 1.25”<br>Acquisition Software: SharpCap<br>Location: Faggiano (TA), Italy<br>Bortle Class: 6<br>Acquisition Date: July 29, 2026<br>Processing Software: RegiStax, Photoshop<br>Type: Lunar Mosaic<br>Panels/Videos: 30<br>Frames per Video: 4,000<br>Stacked Frames: 1,500 per panel<br>Gain: 150<br>Exposure: 3.0 ms<br>Total Data Size: 425 GB</p><p data-rte-preserve-empty="true"><strong>Name:</strong> Raffaele Calcagno</p>]]></content:encoded><media:content type="image/jpeg" url="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/297d4b8e-ca25-4edc-8727-7a74c88f0288/IMG_9335.jpeg?format=1500w" medium="image" isDefault="true" width="1500" height="1487"><media:title type="plain">Full Moon</media:title></media:content></item><item><title>Seahorse nebula - Barnard 150</title><category>2026</category><dc:creator>Charles Lillo</dc:creator><pubDate>Fri, 21 Aug 2026 04:00:25 +0000</pubDate><link>https://www.aapod2.com/blog/seahorse-nebula-barnard-150</link><guid isPermaLink="false">5debd4b16fcd7b02905712ff:5debd4f1c2fab6555bff00b5:6a875141ed359b773897da43</guid><description><![CDATA[Captured under the dark Bortle 3 skies of Lanuéjols, France during the 
Nuits du Causse Noir 2026 event, Maxime Senes (Azathoth Pics) presents a 
striking view of the Seahorse Nebula (Barnard 150). Imaging with a personal 
telescope setup, Senes collected 59 unfiltered sub-exposures of 300 seconds 
each to reveal the intricate, dark dust lanes winding through this iconic 
cosmic silhouette.]]></description><content:encoded><![CDATA[<figure class="
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  <p data-rte-preserve-empty="true"><strong>Image Title:</strong> Seahorse nebula - Barnard 150</p><p data-rte-preserve-empty="true"><strong>Copyright:</strong> Azathoth Pics</p><p data-rte-preserve-empty="true"><strong>Upload Image File (Max Size 10MB):</strong> <a target="_blank" href="https://drive.google.com/open?id=1tR3x0HurLIUSlivvWiOYH1EfaCK-x_jD">https://drive.google.com/open?id=1tR3x0HurLIUSlivvWiOYH1EfaCK-x_jD</a></p><p data-rte-preserve-empty="true"><strong>Date image was taken:</strong> July 19, 2026</p><p data-rte-preserve-empty="true"><strong>Location:</strong> Lanuéjols, Gard (France)<br>Nuits du Causse Noir 2026</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> Picture taken during the NCN2026 event<br>Bortle 3 sky<br>59 images of 300 seconds<br>No filter used</p><p data-rte-preserve-empty="true"><strong>Name:</strong> Maxime Senes</p><p data-rte-preserve-empty="true"><strong>Email:</strong> <a target="_blank" href="mailto:azathoth.pics@gmail.com">azathoth.pics@gmail.com</a></p><p data-rte-preserve-empty="true"><strong>Website or Facebook Profile:</strong> <a target="_blank" href="https://app.astrobin.com/u/AzathothPics#gallery">https://app.astrobin.com/u/AzathothPics#gallery</a></p>]]></content:encoded><media:content type="image/png" url="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/87740339-4745-4c42-96d8-262030c9511a/seahorse-B150-+nofil-1-2.png?format=1500w" medium="image" isDefault="true" width="1500" height="2255"><media:title type="plain">Seahorse nebula - Barnard 150</media:title></media:content></item><item><title>GigaVeil: 1 billion pixels, 300 hours, 35 panels, and 5 contributors on the Veil Nebula</title><category>2026</category><dc:creator>Charles Lillo</dc:creator><pubDate>Thu, 20 Aug 2026 04:00:46 +0000</pubDate><link>https://www.aapod2.com/blog/gigaveil-1-billion-pixels-300-hours-35-panels-and-5-contributors-on-the-veil-nebula</link><guid isPermaLink="false">5debd4b16fcd7b02905712ff:5debd4f1c2fab6555bff00b5:6a860cb0bafe283687660983</guid><description><![CDATA[The Veil Nebula is a massive, expanding supernova remnant—the expanding 
shell of ionized gas left behind when a star roughly 20 times the mass of 
the Sun exploded around 10,000 to 20,000 years ago—where high-velocity 
shockwaves collide with surrounding interstellar clouds to excite atoms of 
doubly ionized oxygen ($\text{OIII}$, glowing in vivid cyan) and 
hydrogen-alpha ($\text{H}\alpha$, glowing in deep red). Capturing this vast 
structure in uniform high resolution required a collaborative imaging 
project bringing together five astrophotographers across Delaware and 
Texas: Gavin Bent, Brian Nietfeld, Hunter Outten, Kaleb Jordan, and Stan 
Williams. Over more than 318 total hours of exposure time using a variety 
of focal lengths, filters, and optics, the team stitched together a 
35-panel, 1-gigapixel mosaic that reveals intricate filamentary shock 
fronts, surrounding ambient hydrogen clouds, and faint nearby targets such 
as the rarely imaged planetary nebula PA28.]]></description><content:encoded><![CDATA[<figure class="
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  <p data-rte-preserve-empty="true"><strong>Image Title:</strong> GigaVeil: 1 billion pixels, 300 hours, 35 panels, and 5 contributors on the Veil Nebula</p><p data-rte-preserve-empty="true"><strong>Copyright:</strong> Gavin Bent, Brian Nietfeld, Hunter Outten, Kaleb Jordan, Stan Williams</p><p data-rte-preserve-empty="true"><strong>Date image was taken:</strong> August 13, 2026</p><p data-rte-preserve-empty="true"><strong>Location:</strong> Laurel, Delaware<br>Brady, Texas<br>Houston, TX</p><p data-rte-preserve-empty="true"><strong>Data Acquisition Method:</strong> Shared Community Data</p><p data-rte-preserve-empty="true"><strong>Description and Details:</strong> GigaVeil: 1 billion pixels, 300 hours, 35 panels, and 5 contributors on the Veil Nebula<br>by GB Astronomy, Brian Nietfeld, Hunter Outten, Kaleb Jordan, Stan Williams<br><br>The Veil Nebula is a complex that can be beautiful at all focal lengths. With narrow FOVs, you can get beautifully detailed shots of small regions like the witch’s broom or Pickering’s triangle. At wider FOVs, you can capture the whole complex, another beautiful shot. However, one thing that is rarely done is to combine the two, creating a massive mosaic to get the whole complex in detail.<br><br>This project is the culmination of that idea: A 35 panel, 1 gigapixel mosaic of the whole Cygnus Loop to capture all that detail. Not only that, but it also includes over 200 hours of a 9 panel mosaic, a 2 panel mosaic, and single panels to fish out the background hydrogen structures found everywhere in Cygnus. It even includes additional time focused on a small planetary nebula - PA28 - that is nearby to the Veil Nebula, but rarely imaged.<br><br><br><br>Published: Aug 18, 2026<br><br>Total integration: 318h 20m<br><br>Integration per filter:<br>- Hα: 65h<br>- OIII: 79h<br>- Multiband: 174h 20m (2092 × 300")<br><br>Equipment:<br>- Optics: Celestron EdgeHD 8", Rokinon 135mm f/2.0 ED UMC, Sky-Watcher Evostar 80ED / Gold Series, Sky-Watcher Quattro 150P, SVBony SV503 102ED, SVBony SV545<br>- Cameras: QHYCCD miniCAM8M, ZWO ASI183MM, ZWO ASI2600MC DUO, ZWO ASI2600MC Pro, ZWO ASI533MC Pro<br>- Mounts: Celestron Advanced VX, Celestron CGX-L, Sky-Watcher EQ6-R Pro, Sky-Watcher HEQ5 PRO, Sky-Watcher Star Adventurer GTi<br>- Filters: Baader H-alpha Ultra-Narrowband 3.5nm (CMOS-Optimized) 2", Baader O-III Ultra-Narrowband 4nm (CMOS-Optimized) 2", Optolong L-eNhance 1.25", Optolong L-Ultimate 2", QHYCCD miniCAM8M H-alpha 3nm, QHYCCD miniCAM8M OIII 3nm, SVBony SV220 3nm H-alpha &amp; OIII 2"<br>- Software: Adobe Photoshop, Nikita Misiura DeepSNR, Pleiades Astrophoto PixInsight, Russell Croman Astrophotography BlurXTerminator, Russell Croman Astrophotography StarXTerminator<br><br>For more information, visit AstroBin:<br><a target="_blank" href="https://app.astrobin.com/i/l3k293">https://app.astrobin.com/i/l3k293</a></p><p data-rte-preserve-empty="true"><strong>Name:</strong> Hunter Outten</p><p data-rte-preserve-empty="true"><strong>Email:</strong> <a target="_blank" href="mailto:outtenastrophotography@gmail.com">outtenastrophotography@gmail.com</a></p><p data-rte-preserve-empty="true"><strong>Website or Facebook Profile:</strong> <a target="_blank" href="http://app.astrobin.com/u/OuttenAstrophotography">http://app.astrobin.com/u/OuttenAstrophotography</a></p>]]></content:encoded><media:content type="image/jpeg" url="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/f1081cc3-9470-4832-af12-dae79cfa40fa/Veil_Nebula_25_Magma.jpg?format=1500w" medium="image" isDefault="true" width="1500" height="1140"><media:title type="plain">GigaVeil: 1 billion pixels, 300 hours, 35 panels, and 5 contributors on the Veil Nebula</media:title></media:content></item><item><title>Collinder 399 - The Coathanger Cluste</title><category>2026</category><dc:creator>Charles Lillo</dc:creator><pubDate>Wed, 19 Aug 2026 04:00:47 +0000</pubDate><link>https://www.aapod2.com/blog/collinder-399-the-coathanger-cluster</link><guid isPermaLink="false">5debd4b16fcd7b02905712ff:5debd4f1c2fab6555bff00b5:6a848f64c8b3d4697a5cb039</guid><description><![CDATA[A striking capture of Collinder 399—the Coathanger Cluster—standing out 
against the rich background of the Milky Way, showcasing vivid star colors 
taken from Buttwil, Switzerland. Though long thought to be an open cluster, 
modern astrometry reveals it is an chance alignment—an asterism—of ten main 
stars ranging from 230 to 1,300 light-years away. Its distinctive 
coat-hanger shape remains one of the northern sky's most delightful 
binocular targets.]]></description><content:encoded><![CDATA[<figure class="
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                <img data-stretch="false" data-image="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/595ecd0e-3cd6-4e94-a63d-a14afa0d06b2/Cr399_AAPOD.jpg" data-image-dimensions="5907x3938" 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/595ecd0e-3cd6-4e94-a63d-a14afa0d06b2/Cr399_AAPOD.jpg?format=1000w" width="5907" height="3938" 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/595ecd0e-3cd6-4e94-a63d-a14afa0d06b2/Cr399_AAPOD.jpg?format=100w 100w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/595ecd0e-3cd6-4e94-a63d-a14afa0d06b2/Cr399_AAPOD.jpg?format=300w 300w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/595ecd0e-3cd6-4e94-a63d-a14afa0d06b2/Cr399_AAPOD.jpg?format=500w 500w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/595ecd0e-3cd6-4e94-a63d-a14afa0d06b2/Cr399_AAPOD.jpg?format=750w 750w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/595ecd0e-3cd6-4e94-a63d-a14afa0d06b2/Cr399_AAPOD.jpg?format=1000w 1000w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/595ecd0e-3cd6-4e94-a63d-a14afa0d06b2/Cr399_AAPOD.jpg?format=1500w 1500w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/595ecd0e-3cd6-4e94-a63d-a14afa0d06b2/Cr399_AAPOD.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> Collinder 399 - The Coathanger Cluster</p><p data-rte-preserve-empty="true"><strong>Copyright:</strong> Jan Lindemann</p><p data-rte-preserve-empty="true"><strong>Date image was taken:</strong> July 23, 2026</p><p data-rte-preserve-empty="true"><strong>Location:</strong> Buttwil, Switzerland</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> Cr339 is a beautiful object that stands out wonderfully against the Milky Way. The different star colors are particularly appealing and make the image interesting.<br><br>Image:<br>ZWO ASI 2600mc duo<br>Sharpstar 94epdh<br>_ with Reducer auf 414mm f/4.4<br>Skywatcher EQ5 Pro<br>ASIAIR Plus<br>RGB 120x60“<br>Total 2h<br>Flats und Biases<br><br>Processing:<br>Siril, GIMP</p><p data-rte-preserve-empty="true"><strong>Name:</strong> Jan Lindemann</p><p data-rte-preserve-empty="true"><strong>Email:</strong> <a target="_blank" href="mailto:jan.lindemann@bluewin.ch">jan.lindemann@bluewin.ch</a></p><p data-rte-preserve-empty="true"><strong>Website or Facebook Profile:</strong> <a target="_blank" href="https://www.facebook.com/profile.php?id=61559515151868">https://www.facebook.com/profile.php?id=61559515151868</a></p>]]></content:encoded><media:content type="image/jpeg" url="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/595ecd0e-3cd6-4e94-a63d-a14afa0d06b2/Cr399_AAPOD.jpg?format=1500w" medium="image" isDefault="true" width="1500" height="1000"><media:title type="plain">Collinder 399 - The Coathanger Cluste</media:title></media:content></item><item><title>“Little Cocoon” and its dark nebulae</title><category>2026</category><dc:creator>Charles Lillo</dc:creator><pubDate>Tue, 18 Aug 2026 04:00:25 +0000</pubDate><link>https://www.aapod2.com/blog/little-cocoon-and-its-dark-nebula</link><guid isPermaLink="false">5debd4b16fcd7b02905712ff:5debd4f1c2fab6555bff00b5:6a830d6470b1395c9313d89b</guid><description><![CDATA[The "Little Cocoon" nebula, cataloged as SH2-82, is an active star-forming 
emission nebula embedded in a reflective region of dust and gas, set 
against the rich star clouds of the constellation Sagitta in the inner 
Milky Way. Glowing primarily via ionizing radiation from adjacent stellar 
activity, the nebula's vibrant core is framed by surrounding reflection 
dust and complex lanes of dark nebulae that obscure background starlight. 
Astrophotographic data captured across LRGB and narrow-band OIII 
wavelengths reveals intricate structural layers within these molecular 
clouds, highlighting the delicate interplay between hydrogen excitation, 
light scattering, and dense interstellar dust absorbing light across the 
region.]]></description><content:encoded><![CDATA[<figure class="
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                <img data-stretch="false" data-image="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/37773b6c-f56f-4108-aaea-acf87756030c/S_2.jpg" data-image-dimensions="5118x4091" 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/37773b6c-f56f-4108-aaea-acf87756030c/S_2.jpg?format=1000w" width="5118" height="4091" 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/37773b6c-f56f-4108-aaea-acf87756030c/S_2.jpg?format=100w 100w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/37773b6c-f56f-4108-aaea-acf87756030c/S_2.jpg?format=300w 300w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/37773b6c-f56f-4108-aaea-acf87756030c/S_2.jpg?format=500w 500w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/37773b6c-f56f-4108-aaea-acf87756030c/S_2.jpg?format=750w 750w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/37773b6c-f56f-4108-aaea-acf87756030c/S_2.jpg?format=1000w 1000w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/37773b6c-f56f-4108-aaea-acf87756030c/S_2.jpg?format=1500w 1500w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/37773b6c-f56f-4108-aaea-acf87756030c/S_2.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> “Little Cocoon” and its dark nebulae</p><p data-rte-preserve-empty="true"><strong>Copyright:</strong> Andrea Arbizzi</p><p data-rte-preserve-empty="true"><strong>Date image was taken:</strong> July 25, 2026</p><p data-rte-preserve-empty="true"><strong>Location:</strong> Agriturismo Vecchio Fontanile (GR) – Maremma – sqm21.1, Italy<br>Radici pass (MO) - 1540 m. – northern appennines - sqm 20.95, Italy<br>Modena (Sqm 18.5-18.8 Bortle 7,5-8), 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> Often called the “Little Cocoon”, SH2-82 is an emission nebula, ringed by a reflection nebula, surrounded by dark nebulae; it is set within the star clouds of Sagitta, in a rich part of the Milky Way.<br><br>Askar 160 F5,6 (897 mm)<br>Zwo Asi 2600 MC Duo<br>Zwo AM7<br>Zwo AsiAir Plus<br><br>jul 2026<br>no filter: 103X300”<br>Agriturismo Vecchio Fontanile (GR) – Maremma – sqm21.1, Italy<br>no filter: 64X300”<br>Radici pass (MO) - 1540 m. – northern appennines - sqm 20.95, Italy<br>Tot: 13h 55’<br><br>Antlia ALP-T Ha O3 3nm: 52X600”<br>Modena (Sqm 18.5-18.8 Bortle 7,5-8), Italy<br>Tot: 8h 40’<br><br>Tot: 22h 35’</p><p data-rte-preserve-empty="true"><strong>Name:</strong> Andrea Arbizzi</p>]]></content:encoded><media:content type="image/jpeg" url="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/37773b6c-f56f-4108-aaea-acf87756030c/S_2.jpg?format=1500w" medium="image" isDefault="true" width="1500" height="1199"><media:title type="plain">“Little Cocoon” and its dark nebulae</media:title></media:content></item><item><title>Beyond Totality: The Sun’s Chromosphere and Corona</title><dc:creator>Charles Lillo</dc:creator><pubDate>Mon, 17 Aug 2026 04:00:52 +0000</pubDate><link>https://www.aapod2.com/blog/beyond-totality-the-suns-chromosphere-and-corona</link><guid isPermaLink="false">5debd4b16fcd7b02905712ff:5debd4f1c2fab6555bff00b5:6a81f3c2494f52497fdbb40e</guid><description><![CDATA[A composite view of the eclipsed Sun combining two normally very different 
perspectives of our star: the H-alpha chromosphere and prominences, 
reconstructed through spectroheliography, and the faint outer corona, 
photographed during totality.

The chromospheric data were acquired from Menorca, Balearic Islands, with 
the Sun only 12° above the western horizon, while the coronal images were 
obtained by Nicola Bizzotto from Madrid with the Sun 7° above the horizon.]]></description><content:encoded><![CDATA[<figure class="
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                <img data-stretch="false" data-image="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/9b7b0b40-f53b-4f37-844d-909b8801f6be/EclissiSoleNonEclissiRedWhiteLowLow.jpg" data-image-dimensions="5000x3541" 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/9b7b0b40-f53b-4f37-844d-909b8801f6be/EclissiSoleNonEclissiRedWhiteLowLow.jpg?format=1000w" width="5000" height="3541" 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/9b7b0b40-f53b-4f37-844d-909b8801f6be/EclissiSoleNonEclissiRedWhiteLowLow.jpg?format=100w 100w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/9b7b0b40-f53b-4f37-844d-909b8801f6be/EclissiSoleNonEclissiRedWhiteLowLow.jpg?format=300w 300w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/9b7b0b40-f53b-4f37-844d-909b8801f6be/EclissiSoleNonEclissiRedWhiteLowLow.jpg?format=500w 500w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/9b7b0b40-f53b-4f37-844d-909b8801f6be/EclissiSoleNonEclissiRedWhiteLowLow.jpg?format=750w 750w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/9b7b0b40-f53b-4f37-844d-909b8801f6be/EclissiSoleNonEclissiRedWhiteLowLow.jpg?format=1000w 1000w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/9b7b0b40-f53b-4f37-844d-909b8801f6be/EclissiSoleNonEclissiRedWhiteLowLow.jpg?format=1500w 1500w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/9b7b0b40-f53b-4f37-844d-909b8801f6be/EclissiSoleNonEclissiRedWhiteLowLow.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> Beyond Totality: The Sun’s Chromosphere and Corona</p><p data-rte-preserve-empty="true"><strong>Copyright:</strong> Alessandro Ravagnin &amp; Nicola Bizzotto</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> Menorca and Madrid</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> A composite view of the eclipsed Sun combining two normally very different perspectives of our star: the H-alpha chromosphere and prominences, reconstructed through spectroheliography, and the faint outer corona, photographed during totality.<br><br>The chromospheric data were acquired from Menorca, Balearic Islands, with the Sun only 12° above the western horizon, while the coronal images were obtained by Nicola Bizzotto from Madrid with the Sun 7° above the horizon.<br><br>The aim of the composition was to reveal different layers of the solar atmosphere in a single image, from the thin and highly structured chromosphere, with its prominences extending beyond the limb, to the much larger and fainter solar corona revealed by the natural occultation of the photosphere during totality.<br><br>To obtain an accurate geometrical match between the spectroheliographic solar disk and the eclipsed Sun, white-light images taken immediately after the beginning of totality and just before its end, close to the appearance/disappearance of Baily’s beads, were used as references for the exact apparent solar disk size relative to the Moon.<br><br>The chromosphere and corona were processed separately. The two datasets were then precisely registered using the prominences visible in both images as common reference features and finally blended into a single high-dynamic-range representation of the solar atmosphere.</p><p data-rte-preserve-empty="true"><strong>Name:</strong> Alessandro Ravagnin</p><p data-rte-preserve-empty="true"><strong>Website or Facebook Profile:</strong> <a target="_blank" href="https://astrotrex.wordpress.com/2026/08/16/total-eclipse-of-the-sun-12-08-2026/#english">https://astrotrex.wordpress.com/2026/08/16/total-eclipse-of-the-sun-12-08-2026/#english</a></p>]]></content:encoded><media:content type="image/jpeg" url="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/9b7b0b40-f53b-4f37-844d-909b8801f6be/EclissiSoleNonEclissiRedWhiteLowLow.jpg?format=1500w" medium="image" isDefault="true" width="1500" height="1062"><media:title type="plain">Beyond Totality: The Sun’s Chromosphere and Corona</media:title></media:content></item><item><title>ECLIPSE LANDSCAPE</title><category>2026</category><dc:creator>Charles Lillo</dc:creator><pubDate>Sun, 16 Aug 2026 04:00:34 +0000</pubDate><link>https://www.aapod2.com/blog/eclipse-landscape</link><guid isPermaLink="false">5debd4b16fcd7b02905712ff:5debd4f1c2fab6555bff00b5:6a7f4bf58d047a3a23f69073</guid><description><![CDATA[A unique composite captures the progression of the August 12, 2026 partial 
solar eclipse set against the countryside of Butser Hill in the South 
Downs, UK.

To properly balance the extreme brightness difference between the solar 
disk and the scenic foreground, this image was built using multiple 
exposures taken at various exposure lengths and ISO settings. Short, 
filtered exposures taken every 30 seconds across the 2.5-hour event 
captured the precise phases of the Sun, which were then composited onto a 
dedicated landscape exposure. This multi-exposure approach ensures both the 
fine detail of the Sun's path and the rich tones of the surrounding terrain 
remain perfectly exposed.]]></description><content:encoded><![CDATA[<figure class="
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                <img data-stretch="false" data-image="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/786c0995-d18d-4217-b167-8351b8487d99/EclipseLandscape-12Aug2026-Lowres.jpg" data-image-dimensions="7603x7462" 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/786c0995-d18d-4217-b167-8351b8487d99/EclipseLandscape-12Aug2026-Lowres.jpg?format=1000w" width="7603" height="7462" 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/786c0995-d18d-4217-b167-8351b8487d99/EclipseLandscape-12Aug2026-Lowres.jpg?format=100w 100w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/786c0995-d18d-4217-b167-8351b8487d99/EclipseLandscape-12Aug2026-Lowres.jpg?format=300w 300w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/786c0995-d18d-4217-b167-8351b8487d99/EclipseLandscape-12Aug2026-Lowres.jpg?format=500w 500w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/786c0995-d18d-4217-b167-8351b8487d99/EclipseLandscape-12Aug2026-Lowres.jpg?format=750w 750w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/786c0995-d18d-4217-b167-8351b8487d99/EclipseLandscape-12Aug2026-Lowres.jpg?format=1000w 1000w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/786c0995-d18d-4217-b167-8351b8487d99/EclipseLandscape-12Aug2026-Lowres.jpg?format=1500w 1500w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/786c0995-d18d-4217-b167-8351b8487d99/EclipseLandscape-12Aug2026-Lowres.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> Eclipse landscape</p><p data-rte-preserve-empty="true"><strong>Copyright:</strong> SteveFox</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> Butser Hill, South Downs, UK</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> A different take on the 12th Aug partial eclipse taken from Butser Hill in the South Downs.<br><br>Taken with Canon R6 with a solar filter at 1/320 sec, f/10, ISO 100 at 105mm focal length in a timelapse with a shot every 30 secs over about 2.5 hours. Every 5th frame (to get the required spacing) was then composited onto a landscape shot from the hill. Even the couple of clouds (they are real!) came along to the party.</p><p data-rte-preserve-empty="true"><strong>Name:</strong> Steve Fox</p>]]></content:encoded><media:content type="image/jpeg" url="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/786c0995-d18d-4217-b167-8351b8487d99/EclipseLandscape-12Aug2026-Lowres.jpg?format=1500w" medium="image" isDefault="true" width="1500" height="1472"><media:title type="plain">ECLIPSE LANDSCAPE</media:title></media:content></item><item><title>TOTAL SOLAR ECLIPSE 2026</title><category>2026</category><dc:creator>Charles Lillo</dc:creator><pubDate>Sat, 15 Aug 2026 04:00:10 +0000</pubDate><link>https://www.aapod2.com/blog/total-solar-eclipse-2026</link><guid isPermaLink="false">5debd4b16fcd7b02905712ff:5debd4f1c2fab6555bff00b5:6a7f4a9548d7953a9642e24b</guid><description><![CDATA[During totality of the August 12, 2026 solar eclipse over Guadalajara, 
Spain, the moon completely covered the solar disk, revealing the majestic 
structure of the Sun's outer atmosphere.

To capture the vast dynamic range—from the intense brilliance of the solar 
prominences hugging the lunar limb to the delicate, faint streamers 
stretching far into the solar corona—this image was crafted using a 
composite of multiple exposures taken at varying exposure times and ISO 
settings. Blending these exposures allows the intricate details of the 
magnetic field lines frozen within the corona to shine through alongside 
the fiery, crimson prominences at the edge of the disk.]]></description><content:encoded><![CDATA[<figure class="
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                <img data-stretch="false" data-image="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/f47d67af-a72b-48c8-9587-e0315083493c/TOTAL+2026+FINAL4+V2.jpg" data-image-dimensions="1783x1545" 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/f47d67af-a72b-48c8-9587-e0315083493c/TOTAL+2026+FINAL4+V2.jpg?format=1000w" width="1783" height="1545" 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/f47d67af-a72b-48c8-9587-e0315083493c/TOTAL+2026+FINAL4+V2.jpg?format=100w 100w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/f47d67af-a72b-48c8-9587-e0315083493c/TOTAL+2026+FINAL4+V2.jpg?format=300w 300w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/f47d67af-a72b-48c8-9587-e0315083493c/TOTAL+2026+FINAL4+V2.jpg?format=500w 500w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/f47d67af-a72b-48c8-9587-e0315083493c/TOTAL+2026+FINAL4+V2.jpg?format=750w 750w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/f47d67af-a72b-48c8-9587-e0315083493c/TOTAL+2026+FINAL4+V2.jpg?format=1000w 1000w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/f47d67af-a72b-48c8-9587-e0315083493c/TOTAL+2026+FINAL4+V2.jpg?format=1500w 1500w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/f47d67af-a72b-48c8-9587-e0315083493c/TOTAL+2026+FINAL4+V2.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> TOTAL SOLAR ECLIPSE 2026</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 12, 2026</p><p data-rte-preserve-empty="true"><strong>Location:</strong> Guadalajara, 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> Canon 7d mkii - Canon 70-200 f4 lens - Handmade equatorIal mount</p><p data-rte-preserve-empty="true"><strong>Name:</strong> George Chatzifrantzis</p><p data-rte-preserve-empty="true"><strong>Website or Facebook Profile:</strong> <a target="_blank" href="http://www.facebook.com/GeorgeChatzifrantzis?locale=el_GR">http://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/f47d67af-a72b-48c8-9587-e0315083493c/TOTAL+2026+FINAL4+V2.jpg?format=1500w" medium="image" isDefault="true" width="1500" height="1300"><media:title type="plain">TOTAL SOLAR ECLIPSE 2026</media:title></media:content></item><item><title>Sunset Eclipse</title><category>2026</category><dc:creator>Charles Lillo</dc:creator><pubDate>Fri, 14 Aug 2026 04:00:20 +0000</pubDate><link>https://www.aapod2.com/blog/partial-solar-eclipse-ldinghausen-germany</link><guid isPermaLink="false">5debd4b16fcd7b02905712ff:5debd4f1c2fab6555bff00b5:6a7e285282992b081caec819</guid><description><![CDATA[On August 12, 2026, a magnificent partial solar eclipse unfolded across 
Western Europe, reaching an impressive 87% maximum solar obscuration as 
viewed from Lüdinghausen, Germany. Captured by photographer Michel Kroll 
using a Sony RX10 IV with sequential exposures taken every three minutes, 
this composite image illustrates the lunar limb progressively occulting the 
solar photosphere as the Sun descended toward the horizon. Even without 
achieving full totality, an 87% reduction in solar irradiance drastically 
alters ambient light, while atmospheric extinction and Rayleigh scattering 
near the horizon shift the Sun's spectral output toward deep amber hues, 
casting an eerie, twilight-like illumination over the terrestrial 
landscape.]]></description><content:encoded><![CDATA[<figure class="
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                <img data-stretch="false" data-image="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/9355b669-b0d2-4cba-b3fd-1234479bf1cb/SoFi_12-08-26_LH.jpg" data-image-dimensions="4373x3058" 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/9355b669-b0d2-4cba-b3fd-1234479bf1cb/SoFi_12-08-26_LH.jpg?format=1000w" width="4373" height="3058" 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/9355b669-b0d2-4cba-b3fd-1234479bf1cb/SoFi_12-08-26_LH.jpg?format=100w 100w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/9355b669-b0d2-4cba-b3fd-1234479bf1cb/SoFi_12-08-26_LH.jpg?format=300w 300w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/9355b669-b0d2-4cba-b3fd-1234479bf1cb/SoFi_12-08-26_LH.jpg?format=500w 500w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/9355b669-b0d2-4cba-b3fd-1234479bf1cb/SoFi_12-08-26_LH.jpg?format=750w 750w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/9355b669-b0d2-4cba-b3fd-1234479bf1cb/SoFi_12-08-26_LH.jpg?format=1000w 1000w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/9355b669-b0d2-4cba-b3fd-1234479bf1cb/SoFi_12-08-26_LH.jpg?format=1500w 1500w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/9355b669-b0d2-4cba-b3fd-1234479bf1cb/SoFi_12-08-26_LH.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> Sunset Eclipse</p><p data-rte-preserve-empty="true"><strong>Copyright:</strong> Michel Kroll</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> Lüdinghausen, Germany</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> Usually, clouds start rolling in as soon as any astronomical event begins at my place. This time, I got lucky! The partial eclipse was visible from start to sunset and offered truly incredible views for everyone equipped with a pair of eclipse glasses.<br><br>I had my Sony RX10 IV capturing an image every three minutes, which resulted in this stunning composite showing the changing position of the Sun and the degree of solar coverage throughout the eclipse.<br><br>We didn’t get to experience totality in Germany, but 87% solar coverage still made the lighting feel out of this world. I’ll remember this for a long time!</p><p data-rte-preserve-empty="true"><strong>Name:</strong> Michel Kroll</p>]]></content:encoded><media:content type="image/jpeg" url="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/9355b669-b0d2-4cba-b3fd-1234479bf1cb/SoFi_12-08-26_LH.jpg?format=1500w" medium="image" isDefault="true" width="1500" height="1049"><media:title type="plain">Sunset Eclipse</media:title></media:content></item><item><title>The Sun two weeks (July 27, 2026) before the total eclipse</title><category>2026</category><dc:creator>Charles Lillo</dc:creator><pubDate>Thu, 13 Aug 2026 04:00:48 +0000</pubDate><link>https://www.aapod2.com/blog/the-countdown-to-totality</link><guid isPermaLink="false">5debd4b16fcd7b02905712ff:5debd4f1c2fab6555bff00b5:6a7cd84e979d421ad33b5274</guid><description><![CDATA[Captured just two weeks ahead of the August 12 total solar eclipse, this 
striking full-disk H-alpha portrait highlights the Sun’s dynamic 
chromosphere in exceptional detail. A dense network of dark filaments spans 
across the solar disk, surrounded by brilliant active regions and prominent 
solar filaments extending from the limb.

Reconstructed from roughly 3,600 monochromatic frames, the image 
beautifully preserves the delicate fibrillar structures and complex 
magnetic pathways of our nearest star—promising a spectacular show for 
eclipse observers.]]></description><content:encoded><![CDATA[<figure class="
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  <p data-rte-preserve-empty="true"><strong>Image Title:</strong> The Sun two weeks before the total eclipse</p><p data-rte-preserve-empty="true"><strong>Copyright:</strong> Alessando Ravagnin</p><p data-rte-preserve-empty="true"><strong>Date image was taken:</strong> July 27, 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> The Countdown to Totality<br><br>With only two weeks remaining before the total solar eclipse of August 12, our nearest star continues to display remarkable chromospheric activity. This full-disk H-alpha image reveals a rich network of dark filaments suspended above the solar surface, bright active regions, and numerous prominences rising from the limb.<br><br>Such activity raises hopes that, if these magnetic structures persist, eclipse observers may witness an especially dynamic spectacle: a corona adorned with brilliant prominences extending beyond the silhouette of the Moon during totality.<br><br>The image was acquired with an MLAstro SHG700 slit spectroheliograph mounted on a 115 mm apochromatic refractor. The final image was reconstructed from approximately 3,600 monochromatic frames, preserving the delicate fibrilar texture of the chromosphere while revealing the Sun's complex magnetic architecture.<br><br>As eclipse day approaches, the Sun appears ready to deliver another unforgettable performance.</p><p data-rte-preserve-empty="true"><strong>Name:</strong> Alessandro Ravagnin</p><p data-rte-preserve-empty="true"><strong>Website or Facebook Profile:</strong> <a target="_blank" href="https://astrotrex.wordpress.com/2026/06/07/chasing-the-sun/#english">https://astrotrex.wordpress.com/2026/06/07/chasing-the-sun/#english</a></p>]]></content:encoded><media:content type="image/jpeg" url="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/54228410-8e2d-420d-91a7-9658e280e865/2026-07-27-0546.jpg?format=1500w" medium="image" isDefault="true" width="1500" height="1105"><media:title type="plain">The Sun two weeks (July 27, 2026) before the total eclipse</media:title></media:content></item><item><title> Deep in the Cosmic Ocean: The Heart of the Lagoon Nebula (M8)</title><dc:creator>Charles Lillo</dc:creator><pubDate>Wed, 12 Aug 2026 04:00:26 +0000</pubDate><link>https://www.aapod2.com/blog/lagoon-nebula-m8</link><guid isPermaLink="false">5debd4b16fcd7b02905712ff:5debd4f1c2fab6555bff00b5:6a7b5643198ae200bb6261d5</guid><description><![CDATA[Located roughly 4,100 light-years away in the constellation Sagittarius, 
this high-resolution deep-field view by Pasquale Mastroianni captures the 
intricate astrophysical dynamics of the Lagoon Nebula (M8). Acquired at the 
Domus Astrae Observatory using a broadband Optolong L-Quad filter, the 
image showcases an active star-forming region where powerful stellar winds 
carve through glowing ionized gas. The processing balances strict 
scientific fidelity and natural star color, highlighting dark Bok globules 
and dust lanes—such as the Hourglass region—alongside the vibrant 
interaction between gas ionization fronts and the embedded young open 
cluster NGC 6530.]]></description><content:encoded><![CDATA[<figure class="
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  <p data-rte-preserve-empty="true"><strong>Image Title:</strong>​ Deep in the Cosmic Ocean: The Heart of the Lagoon Nebula (M8)</p><p data-rte-preserve-empty="true"><strong>Copyright:</strong> Pasquale Mastroianni</p><p data-rte-preserve-empty="true"><strong>Date image was taken:</strong> July 08, 2026</p><p data-rte-preserve-empty="true"><strong>Location:</strong> Domus Astrae observatory,Liberi(CE)</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 is my version of the Lagoon Nebula. This high-resolution deep-field view captures the intricate astrophysical dynamics of one of the most active star-forming regions in Sagittarius, located roughly 4,100 light-years away.<br>​By leveraging a broadband enhancement filter (Optolong L-Quad), my primary goal during acquisition and processing was to achieve strict scientific fidelity, true-to-life star colors, and an exceptionally high dynamic range.<br>The processing pipeline was tailored to emphasize:<br>​The turbulent interface where stellar winds carve the glowing ionized gas, contrasting the core's intense brightness against the faint, diffuse outer filaments.<br>​The crisp structural definition of the dense, opaque Bok globules and dark dust lanes (such as the Hourglass region) where active star formation is currently occurring.<br>​The spatial relationship between the gas ionization fronts and the embedded young open cluster NGC 6530.<br>Technical Details:<br>​Target: Lagoon Nebula (M8 / NGC 6523)<br>​Location: Domus Astrae Observatory, Liberi (CE), Italy<br>​Acquisition Dates: July 8, 2026<br>​Total Integration: 5 hours (Sub-frames: 60 x 300s)<br>​Telescope: Sky-Watcher Newton 254/1000 f/4<br>​Coma Corrector: TS-Optics GPU Aplanatic Coma Corrector<br>​Camera: Omegon VeTEC 571 C (Gain 100)<br>​Filter: Optolong L-Quad Enhance Filter (L-QEF)<br>​Mount: Sky-Watcher EQ6-R Pro<br>​Guiding: Sky-Watcher 70/500 with ZWO ASI 224 MC<br>​Processing: PixInsight</p><p data-rte-preserve-empty="true"><strong>Name:</strong> Pasquale Mastroianni</p><p data-rte-preserve-empty="true"><strong>Website or Facebook Profile:</strong> <a target="_blank" href="https://www.instagram.com/pako_astrophotographer?igsh=dWlmcjFmMmdqcTI4">https://www.instagram.com/pako_astrophotographer?igsh=dWlmcjFmMmdqcTI4</a></p>


  









<p><a href="https://www.aapod2.com/blog/lagoon-nebula-m8">Permalink</a><p>]]></content:encoded><media:content type="image/jpeg" url="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/5f3ee217-586a-4bea-9083-02bc62df590d/164838.jpg?format=1500w" medium="image" isDefault="true" width="1500" height="2162"><media:title type="plain">Deep in the Cosmic Ocean: The Heart of the Lagoon Nebula (M8)</media:title></media:content></item><item><title>Saturn</title><category>2026</category><dc:creator>Charles Lillo</dc:creator><pubDate>Tue, 11 Aug 2026 04:00:09 +0000</pubDate><link>https://www.aapod2.com/blog/saturn-1</link><guid isPermaLink="false">5debd4b16fcd7b02905712ff:5debd4f1c2fab6555bff00b5:6a79d021f2d4081fced03bcd</guid><description><![CDATA[Captured under steady Italian skies, this vivid high-resolution capture 
reveals Saturn's ring system as it gradually begins to tilt back into view. 
Following the nearly edge-on ring plane alignment of 2025, Earth's changing 
perspective offers a fresh look at the gas giant's southern hemisphere and 
subtle atmospheric details. The changing angle of Saturn's rings from our 
vantage point on Earth comes down to two main orbital factors: Axial Tilt 
and the 29.5-Year Orbit.]]></description><content:encoded><![CDATA[<figure class="
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                <img data-stretch="false" data-image="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/397976ae-5d6c-4673-956b-89cb08645f41/1000184334.jpg" data-image-dimensions="950x670" 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/397976ae-5d6c-4673-956b-89cb08645f41/1000184334.jpg?format=1000w" width="950" height="670" 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/397976ae-5d6c-4673-956b-89cb08645f41/1000184334.jpg?format=100w 100w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/397976ae-5d6c-4673-956b-89cb08645f41/1000184334.jpg?format=300w 300w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/397976ae-5d6c-4673-956b-89cb08645f41/1000184334.jpg?format=500w 500w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/397976ae-5d6c-4673-956b-89cb08645f41/1000184334.jpg?format=750w 750w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/397976ae-5d6c-4673-956b-89cb08645f41/1000184334.jpg?format=1000w 1000w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/397976ae-5d6c-4673-956b-89cb08645f41/1000184334.jpg?format=1500w 1500w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/397976ae-5d6c-4673-956b-89cb08645f41/1000184334.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> Saturn</p><p data-rte-preserve-empty="true"><strong>Copyright:</strong> luigi morrone</p><p data-rte-preserve-empty="true"><strong>Date image was taken:</strong> July 21, 2026</p><p data-rte-preserve-empty="true"><strong>Location:</strong> Agerola -Amalfitan Coast- 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> Saturn July 21th 2026<br><br>Good seeing conditions with average transparency<br>Setup: C14 Edge HD, Fornax52 mount, Player One Uranus-M/C , Chroma L anr R filtes, Barlow FFC Baader, ADC Pietro Astro MK3. LRG.<br><br>Uranus-M for luminance with R filter. Uranus-C for colour.<br>Agerola -Amalfitan Coast-Italy<br>Full resolution:<br><a target="_blank" href="https://app.astrobin.com/u/Luigi_morrone_1979?i=lrltp5#fullscreen">https://app.astrobin.com/u/Luigi_morrone_1979?i=lrltp5#fullscreen</a><br>#PlayerOneAstronomy #astronomy #baader #celestron #astrophotography #edgehd</p><p data-rte-preserve-empty="true"><strong>Name:</strong> luigi morrone</p><p data-rte-preserve-empty="true"><strong>Email:</strong> <a target="_blank" href="mailto:luigi.astronomia.morrone1979@gmail.com">luigi.astronomia.morrone1979@gmail.com</a></p><p data-rte-preserve-empty="true"><strong>Website or Facebook Profile:</strong> <a target="_blank" href="http://www.astrobin.com/users/Luigi_morrone_1979/">http://www.astrobin.com/users/Luigi_morrone_1979/</a></p><p data-rte-preserve-empty="true"><strong>Terms and conditions:</strong> I agree</p>]]></content:encoded><media:content type="image/jpeg" url="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/397976ae-5d6c-4673-956b-89cb08645f41/1000184334.jpg?format=1500w" medium="image" isDefault="true" width="950" height="670"><media:title type="plain">Saturn</media:title></media:content></item><item><title>Markarian's Chain (LHRGB)</title><category>2026</category><dc:creator>Charles Lillo</dc:creator><pubDate>Mon, 10 Aug 2026 04:00:02 +0000</pubDate><link>https://www.aapod2.com/blog/markarians-chain-lhrgb</link><guid isPermaLink="false">5debd4b16fcd7b02905712ff:5debd4f1c2fab6555bff00b5:6a75e8ba6010cb3c947692b9</guid><description><![CDATA[Markarian's Chain is a prominent, gently curved stretch of galaxies 
situated near the heart of the Virgo Cluster, approximately 50 to 55 
million light-years away toward the constellation Virgo. Dominated by 
massive giant elliptical galaxies like M84 and M86 alongside interacting 
galactic pairs like "The Eyes" (NGC 4435 and NGC 4438), this dense 
structure forms a dynamic gravitational laboratory driven by tidal 
interactions and ram-pressure stripping as galaxies plunge through the 
intracluster medium. Deep narrowband and broadband imaging ($\text{LHRGB}$) 
reveals intricate extra-galactic ionized gas structures, including tenuous 
Hydrogen-alpha ($\text{H}\alpha$) bridges spanning between member galaxies, 
energetic relativistic jets from supermassive black holes like that of 
nearby M87, and faint diffuse foreground clouds across the intergalactic 
field.]]></description><content:encoded><![CDATA[<figure class="
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                <img data-stretch="false" data-image="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/5ed58272-1cdb-4aca-b24b-884488c8175c/Virgo_LRGB_Final.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/5ed58272-1cdb-4aca-b24b-884488c8175c/Virgo_LRGB_Final.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/5ed58272-1cdb-4aca-b24b-884488c8175c/Virgo_LRGB_Final.jpg?format=100w 100w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/5ed58272-1cdb-4aca-b24b-884488c8175c/Virgo_LRGB_Final.jpg?format=300w 300w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/5ed58272-1cdb-4aca-b24b-884488c8175c/Virgo_LRGB_Final.jpg?format=500w 500w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/5ed58272-1cdb-4aca-b24b-884488c8175c/Virgo_LRGB_Final.jpg?format=750w 750w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/5ed58272-1cdb-4aca-b24b-884488c8175c/Virgo_LRGB_Final.jpg?format=1000w 1000w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/5ed58272-1cdb-4aca-b24b-884488c8175c/Virgo_LRGB_Final.jpg?format=1500w 1500w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/5ed58272-1cdb-4aca-b24b-884488c8175c/Virgo_LRGB_Final.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> Markarian's Chain (LHRGB)</p><p data-rte-preserve-empty="true"><strong>Copyright:</strong> Brent Newton</p><p data-rte-preserve-empty="true"><strong>Date image was taken:</strong> June 19, 2026</p><p data-rte-preserve-empty="true"><strong>Location:</strong> Starfront Observatories, Rockwood, TX, US</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> This is a 104 hour integration covering the king of Galaxy Season targets. This is the first time I have captured it under the appreciably dark skies of a remote observatory, and as such I captured much more dim background nebulosity than before as well as the Hα bridge between The Eyes and M86.<br><br>As always, the relativistic jet from M87 is tenuously visible among its bright core, though it may be realistically harder to see due to 8bit JPG compression and without full zoom. One curious detail which appeared in the ~50 hours of Hα exposures was a second jet-like detail opposite the main blue electron beam we have all seen before. My best guess is that this is capturing outflow material from the Black Hole which has been captured in IR by Spitzer and in Radio by the VLA in past decades - though I have never seen this detail appear in amateur images until now.<br><br>TS86SDQ, 460mm, F/5.4, ZWO ASI6200MM-P, Antlia LRGB, Antlia 3nm Hα filters<br><br>L | 210×300″ | 17h 30′<br>R | 146×300″ | 12h 10′<br>G | 147×300″ | 12h 15′<br>B | 141×300″ | 11h 45′<br>Hα | 300×600″ | 50h</p><p data-rte-preserve-empty="true"><strong>Name:</strong> Brent Newton</p><p data-rte-preserve-empty="true"><strong>Website or Facebook Profile:</strong> <a target="_blank" href="http://astronewton.com/">http://astronewton.com</a></p>]]></content:encoded><media:content type="image/jpeg" url="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/5ed58272-1cdb-4aca-b24b-884488c8175c/Virgo_LRGB_Final.jpg?format=1500w" medium="image" isDefault="true" width="1500" height="1000"><media:title type="plain">Markarian's Chain (LHRGB)</media:title></media:content></item><item><title>Layers of the Cosmos in Ursa Major </title><category>2026</category><dc:creator>Charles Lillo</dc:creator><pubDate>Sun, 09 Aug 2026 04:00:14 +0000</pubDate><link>https://www.aapod2.com/blog/layers-of-the-cosmos-in-ursa-major-ifnhgalaxies</link><guid isPermaLink="false">5debd4b16fcd7b02905712ff:5debd4f1c2fab6555bff00b5:6a75e73406cedf13373300c7</guid><description><![CDATA[Layers of the Cosmos in Ursa Major presents a compelling multi-depth cosmic 
panorama, highlighting the complex interplay between galactic foreground 
structures and distant extragalactic deep space. Illuminated by the 
collective starlight of the Milky Way, delicate wisps of Integrated Flux 
Nebula (IFN)—high-latitude dust clouds floating far above our galaxy's 
plane—weave across the field alongside diffuse Hydrogen-alpha emissions 
from ionized interstellar gas. Embedded within and shining through these 
ghostly foreground filaments are numerous background galaxies millions of 
light-years away, demonstrating the incredible dynamic range and depth 
achievable through deep narrowband and broadband astrophotography.]]></description><content:encoded><![CDATA[<figure class="
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  <p data-rte-preserve-empty="true"><strong>Image Title:</strong> Layers of the Cosmos in Ursa Major (IFN+Hα+Galaxies)</p><p data-rte-preserve-empty="true"><strong>Copyright:</strong> Jordi Jofre</p><p data-rte-preserve-empty="true"><strong>Date image was taken:</strong> March 25, 2026</p><p data-rte-preserve-empty="true"><strong>Location:</strong> Àger, Catalonia</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, captured in the constellation of Ursa Major, is dominated by an extensive cloud of Galactic interstellar dust located only a few hundred light-years from Earth. Despite its faint appearance, these dust structures can be recorded with relatively modest integration times.<br><br>Projected behind this nearby foreground is a remarkably rich extragalactic field containing dozens of galaxies. Several of the most prominent members belong to a galaxy group located roughly 100–170 million light-years away, while countless fainter galaxies extend much deeper into the Universe.<br><br>Nearly 50 hours of Hα integration were required to reveal the extremely faint diffuse hydrogen emission associated with the Galactic dust, adding another subtle layer to this view of our local interstellar medium.<br><br>TSOptics 94EDPH<br>ZWO AM5<br>ASI 2600MM Pro<br>LRGB Baader + Ha Antlia 4.5nm<br>80h exposure time</p><p data-rte-preserve-empty="true"><strong>Name:</strong> Jordi Jofre</p><p data-rte-preserve-empty="true"><strong>Website or Facebook Profile:</strong> <a target="_blank" href="https://www.astrobin.com/users/JJofre/">https://www.astrobin.com/users/JJofre/</a></p><p data-rte-preserve-empty="true"><strong>Terms and conditions:</strong> I agree</p>]]></content:encoded><media:content type="image/png" url="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/ed5fd04b-b2f7-4ad5-86b0-d21491562fff/LRGBHa_AAPOD_2.png?format=1500w" medium="image" isDefault="true" width="1500" height="2230"><media:title type="plain">Layers of the Cosmos in Ursa Major</media:title></media:content></item><item><title>The Glancing Bat</title><category>2026</category><dc:creator>Charles Lillo</dc:creator><pubDate>Sat, 08 Aug 2026 04:00:39 +0000</pubDate><link>https://www.aapod2.com/blog/the-glancing-bat</link><guid isPermaLink="false">5debd4b16fcd7b02905712ff:5debd4f1c2fab6555bff00b5:6a75e5d1d41bc66c90b05559</guid><description><![CDATA[NGC 6992, a prominent segment of the Eastern Veil Nebula within the larger 
Cygnus Loop, is an expanding supernova remnant located approximately 2,400 
light-years from Earth in the constellation Cygnus. Originating from the 
catastrophic core-collapse explosion of a massive star between 10,000 and 
20,000 years ago, this energetic shockfront continues to travel through the 
surrounding interstellar medium at speeds exceeding 1.5 million kilometers 
per hour. The intricate, web-like filaments visible across the structure 
are created as high-velocity shockwaves compress and heat diffuse 
interstellar gas, exciting atoms to produce vivid characteristic line 
emissions—most notably from ionized hydrogen, oxygen, and sulfur.]]></description><content:encoded><![CDATA[<figure class="
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                <img data-stretch="false" data-image="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/37c572c5-a19f-488e-9508-c5a5c105b70b/VeilCrop1.jpg" data-image-dimensions="4961x3256" 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/37c572c5-a19f-488e-9508-c5a5c105b70b/VeilCrop1.jpg?format=1000w" width="4961" height="3256" 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/37c572c5-a19f-488e-9508-c5a5c105b70b/VeilCrop1.jpg?format=100w 100w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/37c572c5-a19f-488e-9508-c5a5c105b70b/VeilCrop1.jpg?format=300w 300w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/37c572c5-a19f-488e-9508-c5a5c105b70b/VeilCrop1.jpg?format=500w 500w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/37c572c5-a19f-488e-9508-c5a5c105b70b/VeilCrop1.jpg?format=750w 750w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/37c572c5-a19f-488e-9508-c5a5c105b70b/VeilCrop1.jpg?format=1000w 1000w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/37c572c5-a19f-488e-9508-c5a5c105b70b/VeilCrop1.jpg?format=1500w 1500w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/37c572c5-a19f-488e-9508-c5a5c105b70b/VeilCrop1.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> The Glancing Bat</p><p data-rte-preserve-empty="true"><strong>Copyright:</strong> Sara Harve</p><p data-rte-preserve-empty="true"><strong>Date image was taken:</strong> June 30, 2026</p><p data-rte-preserve-empty="true"><strong>Location:</strong> Cork</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> NGC 6992, remnants of a Supernova in the constellation Cygnus, located about 2,400 light-years from Earth. It is a glowing, lace-like filament of ionized hydrogen, oxygen, and sulfur, formed by a massive star that exploded 10,000 to 20,000 years ago. structure continues to expand at a massive speed of over 1.5 million kilometers per hour.<br><br>Telescope: Lacerta 10" f/4 Carbon Newton<br>Camera: ZWO ASI2600MC Pro<br>Mount: Sky-Watcher EQ6-R Pro<br>Filter: Optolong L-eXtreme 2"<br>Software: Adobe Photoshop, Aries Productions Astro Pixel Processor (APP)<br>Pleiades Astrophoto PixInsight, ZWO ASIAIR,<br><br>Dualband: 15h 45′<br>No filter (for stars): 20′</p><p data-rte-preserve-empty="true"><strong>Name:</strong> sara harvey</p><p data-rte-preserve-empty="true"><strong>Website or Facebook Profile:</strong> <a target="_blank" href="http://www.facebook.com/saraharveyastrophotography">http://www.facebook.com/saraharveyastrophotography</a></p>]]></content:encoded><media:content type="image/jpeg" url="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/37c572c5-a19f-488e-9508-c5a5c105b70b/VeilCrop1.jpg?format=1500w" medium="image" isDefault="true" width="1500" height="984"><media:title type="plain">The Glancing Bat</media:title></media:content></item><item><title>Into the Heart of Our Galaxy</title><category>2026</category><dc:creator>Charles Lillo</dc:creator><pubDate>Fri, 07 Aug 2026 04:00:28 +0000</pubDate><link>https://www.aapod2.com/blog/eart-of-our-galaxy</link><guid isPermaLink="false">5debd4b16fcd7b02905712ff:5debd4f1c2fab6555bff00b5:6a74d5534a7e7611f7518332</guid><description><![CDATA[Every tiny point of light in this image is a star within the Milky Way. 
Dominating the center of the frame is the most densely populated and 
visually spectacular region of our night sky: the Galactic Center, where 
billions of stars, vast clouds of interstellar gas, and intricate lanes of 
cosmic dust converge into an extraordinary celestial landscape.]]></description><content:encoded><![CDATA[<figure class="
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  <p data-rte-preserve-empty="true"><strong>Image Title:</strong> Into the Heart of Our Galaxy</p><p data-rte-preserve-empty="true"><strong>Copyright:</strong> Filippo Galati</p><p data-rte-preserve-empty="true"><strong>Date image was taken:</strong> July 18, 2026</p><p data-rte-preserve-empty="true"><strong>Location:</strong> Portopalo di CapoPassero - 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> Every tiny point of light in this image is a star within the Milky Way. Dominating the center of the frame is the most densely populated and visually spectacular region of our night sky: the Galactic Center, where billions of stars, vast clouds of interstellar gas, and intricate lanes of cosmic dust converge into an extraordinary celestial landscape.<br>Observing this region means looking directly toward the heart of the Milky Way, approximately 26,000 light-years from Earth, where the supermassive black hole Sagittarius A* resides.<br>To the naked eye, the Galactic Center appears as a faint milky band stretching across the sky, but long-exposure astrophotography reveals its remarkable structure and complexity—dense star fields, dark dust lanes, and luminous nebular regions—offering a profound reminder of the immense scale and beauty of the Universe we inhabit.<br>Sony ILCE-7M3 + Sony 85mm - 55x50s f/2.8 ISO 800</p><p data-rte-preserve-empty="true"><strong>Name:</strong> Filippo Galati</p><p data-rte-preserve-empty="true"><strong>Website or Facebook Profile:</strong> <a target="_blank" href="http://www.facebook.com/filippogalatifotografia/">http://www.facebook.com/filippogalatifotografia/</a></p><p data-rte-preserve-empty="true"><strong>Terms and conditions:</strong> I agree</p>]]></content:encoded><media:content type="image/jpeg" url="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/8f2c54bf-07aa-4ad0-8bb3-cb1f4bb75d55/CentroGalattico_FG_2026_1920.jpg?format=1500w" medium="image" isDefault="true" width="1500" height="1875"><media:title type="plain">Into the Heart of Our Galaxy</media:title></media:content></item></channel></rss>