<?xml version="1.0" encoding="UTF-8"?>
<!--Generated by Site-Server v@build.version@ (http://www.squarespace.com) on Thu, 06 Aug 2026 04:08:59 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, 04 Aug 2026 21:20:49 +0000</lastBuildDate><language>en-US</language><generator>Site-Server v@build.version@ (http://www.squarespace.com)</generator><description><![CDATA[]]></description><item><title>The Devil's Tower</title><category>2026</category><dc:creator>Charles Lillo</dc:creator><pubDate>Thu, 06 Aug 2026 04:00:20 +0000</pubDate><link>https://www.aapod2.com/blog/rcw-85</link><guid isPermaLink="false">5debd4b16fcd7b02905712ff:5debd4f1c2fab6555bff00b5:6a7256e2ad218c3184663122</guid><description><![CDATA[This image shows RCW 85, a faint Hα emission nebula in Centaurus shaped by 
strong stellar winds and radiation from nearby massive stars. The bright 
ionisation rim and hollowed cavity reveal active stellar feedback, while a 
compact star‑forming core sits just behind the shock front. RCW 85 is 
rarely imaged, but long integration exposes its tower‑like structure and 
the subtle architecture of the gas being carved out by young stars.]]></description><content:encoded><![CDATA[<figure class="
              sqs-block-image-figure
              intrinsic
            "
        >
          
        
        

        
          
            
          
            
                
                
                
                
                
                
                
                <img data-stretch="false" data-image="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/c04fcdf2-ccb0-4641-b2a1-8b5920f06f15/RCW85.jpg" data-image-dimensions="2507x2641" 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/c04fcdf2-ccb0-4641-b2a1-8b5920f06f15/RCW85.jpg?format=1000w" width="2507" height="2641" 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/c04fcdf2-ccb0-4641-b2a1-8b5920f06f15/RCW85.jpg?format=100w 100w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/c04fcdf2-ccb0-4641-b2a1-8b5920f06f15/RCW85.jpg?format=300w 300w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/c04fcdf2-ccb0-4641-b2a1-8b5920f06f15/RCW85.jpg?format=500w 500w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/c04fcdf2-ccb0-4641-b2a1-8b5920f06f15/RCW85.jpg?format=750w 750w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/c04fcdf2-ccb0-4641-b2a1-8b5920f06f15/RCW85.jpg?format=1000w 1000w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/c04fcdf2-ccb0-4641-b2a1-8b5920f06f15/RCW85.jpg?format=1500w 1500w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/c04fcdf2-ccb0-4641-b2a1-8b5920f06f15/RCW85.jpg?format=2500w 2500w" loading="lazy" decoding="async" data-loader="sqs">

            
          
        
          
        

        
      
        </figure>
      

    
  


  



  
  <p data-rte-preserve-empty="true"><strong>Image Title:</strong> The Devil's Tower</p><p data-rte-preserve-empty="true"><strong>Copyright:</strong> Katherine Miller</p><p data-rte-preserve-empty="true"><strong>Date image was taken:</strong> June 13, 2026</p><p data-rte-preserve-empty="true"><strong>Location:</strong> Caboolture, Queensland 4510</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 shows RCW 85, a faint Hα emission nebula in Centaurus shaped by strong stellar winds and radiation from nearby massive stars. The bright ionisation rim and hollowed cavity reveal active stellar feedback, while a compact star‑forming core sits just behind the shock front. RCW 85 is rarely imaged, but long integration exposes its tower‑like structure and the subtle architecture of the gas being carved out by young stars. Captured with the Sky-Watcher Quattro 150P Newtonian and Wave100i harmonic mount using ZWO ASI533MM pro camera and Antlia RGBHa filters.<br>Ha @ 300secs // 11 hours total<br>RGB @ 180 secs // 2 hours total</p><p data-rte-preserve-empty="true"><strong>Name:</strong> Katherine Miller</p><p data-rte-preserve-empty="true"><strong>Website or Facebook Profile:</strong> <a target="_blank" href="http://www.instagram.com/astrogirl.au">http://www.instagram.com/astrogirl.au</a></p>]]></content:encoded><media:content type="image/jpeg" url="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/c04fcdf2-ccb0-4641-b2a1-8b5920f06f15/RCW85.jpg?format=1500w" medium="image" isDefault="true" width="1500" height="1580"><media:title type="plain">The Devil's Tower</media:title></media:content></item><item><title>The Cygnus wall</title><category>2026</category><dc:creator>Charles Lillo</dc:creator><pubDate>Wed, 05 Aug 2026 04:00:30 +0000</pubDate><link>https://www.aapod2.com/blog/the-cygnus-wall-2026</link><guid isPermaLink="false">5debd4b16fcd7b02905712ff:5debd4f1c2fab6555bff00b5:6a7253fffe819939913a651f</guid><description><![CDATA[This image presents a striking view of a dense star-forming region within a 
giant molecular cloud, where turbulent gas and dust sculpt intricate 
structures across interstellar space. Dark, opaque dust lanes absorb 
visible light from background stars, producing dramatic silhouettes against 
luminous clouds of ionized gas. The blue-white glow traces energetic 
radiation from nearby massive young stars, whose ultraviolet emission 
ionizes surrounding hydrogen and drives powerful stellar winds that erode 
and compress the nebula.

The complex network of pillars, ridges, and cavities reflects the dynamic 
interaction between gravity, radiation pressure, magnetic fields, and 
supersonic turbulence. Dense pockets within the molecular cloud may 
collapse under their own gravity, giving rise to new generations of stars. 
As stellar feedback continues to reshape the environment, the nebula 
evolves over millions of years, simultaneously destroying and creating the 
conditions necessary for future star formation.]]></description><content:encoded><![CDATA[<figure class="
              sqs-block-image-figure
              intrinsic
            "
        >
          
        
        

        
          
            
          
            
                
                
                
                
                
                
                
                <img data-stretch="false" data-image="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/ca1bf9b1-dce5-40a9-bdfe-305b59ea516e/IMG_3886.jpeg" data-image-dimensions="3788x2168" 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/ca1bf9b1-dce5-40a9-bdfe-305b59ea516e/IMG_3886.jpeg?format=1000w" width="3788" height="2168" 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/ca1bf9b1-dce5-40a9-bdfe-305b59ea516e/IMG_3886.jpeg?format=100w 100w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/ca1bf9b1-dce5-40a9-bdfe-305b59ea516e/IMG_3886.jpeg?format=300w 300w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/ca1bf9b1-dce5-40a9-bdfe-305b59ea516e/IMG_3886.jpeg?format=500w 500w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/ca1bf9b1-dce5-40a9-bdfe-305b59ea516e/IMG_3886.jpeg?format=750w 750w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/ca1bf9b1-dce5-40a9-bdfe-305b59ea516e/IMG_3886.jpeg?format=1000w 1000w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/ca1bf9b1-dce5-40a9-bdfe-305b59ea516e/IMG_3886.jpeg?format=1500w 1500w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/ca1bf9b1-dce5-40a9-bdfe-305b59ea516e/IMG_3886.jpeg?format=2500w 2500w" loading="lazy" decoding="async" data-loader="sqs">

            
          
        
          
        

        
      
        </figure>
      

    
  


  



  
  <p data-rte-preserve-empty="true"><strong>Image Title:</strong> The Cygnus wall</p><p data-rte-preserve-empty="true"><strong>Copyright:</strong> stelios stergio</p><p data-rte-preserve-empty="true"><strong>Date image was taken:</strong> June 13, 2026</p><p data-rte-preserve-empty="true"><strong>Location:</strong> Veria 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> This was a new equipment setup test that came out very well.<br>Quattro 150 f/3,45<br>Qhy minicam8m with 3nm sho filters<br>Nyx88 mount<br>StellaVita controller<br>3hrs Ha and 3hrs of Oiii 180sec exposures</p><p data-rte-preserve-empty="true"><strong>Name:</strong> stelios stergiou</p><p data-rte-preserve-empty="true"><strong>Email:</strong> <a target="_blank" href="mailto:fast_stelios@yahoo.com">fast_stelios@yahoo.com</a></p><p data-rte-preserve-empty="true"><strong>Website or Facebook Profile:</strong></p><p data-rte-preserve-empty="true"><strong>Terms and conditions:</strong> I agree</p><p data-rte-preserve-empty="true"><a target="_blank" href="https://comms-sl-events.squarespace.info/?ref=HrwAADDZy3ebs6m4jb5ToQBatNhyko6FAQAAAK8igYSREdbrq0jDf67Hi7dFWuYmHbVnORZtGsQqQNf379jYzicLJVhYRjLByrTv4eLQtUyFGdbrR14o84jZIoH_Zu2dGjGGgNpv__XSOVkRus1BrzTdB0h507aTYKovKbtAJn00pVovynCYkbXEnSxB9GraeQDL_xLX6P-Ujr8chYTpxoy0Q05_3M1PP5rUrsqMy9_2Hml71w8YHLKDuI52v41Zyrj4p1qmvBp567lFe5GWE-3kuDPDmRwYI_jRF5Hq0oq3lyxW3kwpVED-J7U84NuPqyS81kHFp5S56NFv-yg6yU-y__cH5p5tVJghoBNI5dUAkAfDTgpadQYAFfw">Manage Submissions</a></p>]]></content:encoded><media:content type="image/jpeg" url="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/ca1bf9b1-dce5-40a9-bdfe-305b59ea516e/IMG_3886.jpeg?format=1500w" medium="image" isDefault="true" width="1500" height="859"><media:title type="plain">The Cygnus wall</media:title></media:content></item><item><title>M20 Trifid Nebula</title><category>2026</category><dc:creator>Charles Lillo</dc:creator><pubDate>Tue, 04 Aug 2026 04:00:01 +0000</pubDate><link>https://www.aapod2.com/blog/trifid-nebula-messier-20</link><guid isPermaLink="false">5debd4b16fcd7b02905712ff:5debd4f1c2fab6555bff00b5:6a6f5dbb61412d59ea703dbd</guid><description><![CDATA[This high-contrast image of the Trifid Nebula (Messier 20) captures a 
dynamic star-forming region in the constellation Sagittarius, showcasing 
the complex interplay between young, massive stars and interstellar matter. 
The distinct tri-lobed emission region shines vividly in characteristic 
reddish-pink tones, powered by intense ultraviolet radiation from a central 
massive star that ionizes surrounding hydrogen gas (H II region). Adjacent 
to the emission nebula, brilliant blue reflection regions illuminate dusty 
clouds of fine silicate and carbonaceous grains that scatter starlight. 
Cutting through the bright core are striking dark absorption lanes—dense, 
opaque filaments of cosmic dust blocking background light, where cold 
molecular gas continues to collapse to seed future generations of stars.]]></description><content:encoded><![CDATA[<figure class="
              sqs-block-image-figure
              intrinsic
            "
        >
          
        
        

        
          
            
          
            
                
                
                
                
                
                
                
                <img data-stretch="false" data-image="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/9931545c-ed56-4d8c-bd7e-99cd09b49474/M20+FB+Image.jpg" data-image-dimensions="2048x1369" 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/9931545c-ed56-4d8c-bd7e-99cd09b49474/M20+FB+Image.jpg?format=1000w" width="2048" height="1369" 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/9931545c-ed56-4d8c-bd7e-99cd09b49474/M20+FB+Image.jpg?format=100w 100w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/9931545c-ed56-4d8c-bd7e-99cd09b49474/M20+FB+Image.jpg?format=300w 300w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/9931545c-ed56-4d8c-bd7e-99cd09b49474/M20+FB+Image.jpg?format=500w 500w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/9931545c-ed56-4d8c-bd7e-99cd09b49474/M20+FB+Image.jpg?format=750w 750w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/9931545c-ed56-4d8c-bd7e-99cd09b49474/M20+FB+Image.jpg?format=1000w 1000w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/9931545c-ed56-4d8c-bd7e-99cd09b49474/M20+FB+Image.jpg?format=1500w 1500w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/9931545c-ed56-4d8c-bd7e-99cd09b49474/M20+FB+Image.jpg?format=2500w 2500w" loading="lazy" decoding="async" data-loader="sqs">

            
          
        
          
        

        
      
        </figure>
      

    
  


  



  
  <p data-rte-preserve-empty="true"><strong>Image Title:</strong> M20 Trifid Nebula</p><p data-rte-preserve-empty="true"><strong>Copyright:</strong> Scott Horton</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> Backyard Berthoud Colorado</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> My first summer target of the "26 summer season. Ive always wanted to do a long FL acquisition on M20 with clean core details. M20 is a beautiful star nursery full of rich emission, birght refelction and contrasted by dark dust. Its also full of fascinating phenomea such as HH399 outflow<br><br>Completely unnecessary to shoot a target like this in narrowband, but i felt I was able to more control higher contrast color and luminance details in the emission portions of the nebula while keeping the refelction and stars LRGB.<br><br>Final Processing HOOLRGB<br>Total integration: 13h<br>Integration per filter:<br>- Lum/Clear: 4h (48 × 300")<br>- R: 1h (12 × 300")<br>- G: 1h (12 × 300")<br>- B: 1h (12 × 300")<br>- Hα: 3h (18 × 600")<br>- OIII: 3h (18 × 600")<br><br>Equipment:<br>- Telescope: Celestron EdgeHD 11"<br>- Camera: ZWO ASI2600MM Pro<br>- Mount: Sky-Watcher CQ350 Pro<br>- Filters: Antlia 3nm Narrowband H-alpha 2", Antlia 3nm Narrowband Oxygen III 2", Antlia Dark Blue 2", Antlia Dark Green 2", Antlia Dark Luminance 2", Antlia Dark Red 2"<br>- Accessories: PrimaLuceLab ARCO 2" rotator, PrimaLuceLab EAGLE6S, PrimaLuceLab ESATTO 2" LP low profile robotic focuser, ZWO EFW 7 x 2″<br>-Guiding: ZWO OAG-L, ASI174mm<br>- Software: Adobe Photoshop, Pleiades Astrophoto PixInsight, Stefan Berg Nighttime Imaging 'N' Astronomy (N.I.N.A. / NINA)<br><br>Full resolution, plate solved image on Astrobin:<br><a target="_blank" href="https://app.astrobin.com/i/0zjqze">https://app.astrobin.com/i/0zjqze</a></p><p data-rte-preserve-empty="true"><strong>Name:</strong> Scott Horton</p><p data-rte-preserve-empty="true"><strong>Website or Facebook Profile:</strong> <a target="_blank" href="http://app.astrobin.com/i/0zjqze">http://app.astrobin.com/i/0zjqze</a></p>]]></content:encoded><media:content type="image/jpeg" url="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/9931545c-ed56-4d8c-bd7e-99cd09b49474/M20+FB+Image.jpg?format=1500w" medium="image" isDefault="true" width="1500" height="1003"><media:title type="plain">M20 Trifid Nebula</media:title></media:content></item><item><title>Sea of Serenity in mineral detail</title><category>2026</category><dc:creator>Charles Lillo</dc:creator><pubDate>Mon, 03 Aug 2026 04:00:47 +0000</pubDate><link>https://www.aapod2.com/blog/mare-serenitatis-sea-of-serenity</link><guid isPermaLink="false">5debd4b16fcd7b02905712ff:5debd4f1c2fab6555bff00b5:6a6f5c94f8e0be78cd5fd65e</guid><description><![CDATA[This high-contrast mineral image of Mare Serenitatis (Sea of Serenity) 
captures the rich geological history of an ancient lunar impact basin 
flooded by volcanic basalt. The distinct tonal variations across the 
basaltic plains highlight regional differences in mineral chemistry, where 
darker, low-albedo deposits signify high concentrations of titanium dioxide 
and iron-rich minerals such as ilmenite and pyroxene. In contrast, bright 
impact features and crater rims—such as Posidonius and Bessel—display 
high-albedo ejecta blankets composed of pulverized, pristine silicate 
minerals like plagioclase feldspar (anorthosite) excavated from beneath the 
regolith, illustrating the interplay between volcanic effusion and impact 
cratering on the lunar surface.]]></description><content:encoded><![CDATA[<figure class="
              sqs-block-image-figure
              intrinsic
            "
        >
          
        
        

        
          
            
          
            
                
                
                
                
                
                
                
                <img data-stretch="false" data-image="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/7e53b029-5724-4c27-9d4b-7381b0885920/1001507438.jpg" data-image-dimensions="1569x1961" 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/7e53b029-5724-4c27-9d4b-7381b0885920/1001507438.jpg?format=1000w" width="1569" height="1961" 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/7e53b029-5724-4c27-9d4b-7381b0885920/1001507438.jpg?format=100w 100w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/7e53b029-5724-4c27-9d4b-7381b0885920/1001507438.jpg?format=300w 300w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/7e53b029-5724-4c27-9d4b-7381b0885920/1001507438.jpg?format=500w 500w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/7e53b029-5724-4c27-9d4b-7381b0885920/1001507438.jpg?format=750w 750w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/7e53b029-5724-4c27-9d4b-7381b0885920/1001507438.jpg?format=1000w 1000w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/7e53b029-5724-4c27-9d4b-7381b0885920/1001507438.jpg?format=1500w 1500w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/7e53b029-5724-4c27-9d4b-7381b0885920/1001507438.jpg?format=2500w 2500w" loading="lazy" decoding="async" data-loader="sqs">

            
          
        
          
        

        
      
        </figure>
      

    
  


  



  
  <p data-rte-preserve-empty="true"><strong>Image Title:</strong> Sea of Serenity in mineral detail</p><p data-rte-preserve-empty="true"><strong>Copyright:</strong> Nyêrdson Ferreira</p><p data-rte-preserve-empty="true"><strong>Date image was taken:</strong> June 28, 2026</p><p data-rte-preserve-empty="true"><strong>Location:</strong> Cajazeiras; Paraíba; 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> The Sea of Serenity is an ocean of petrified silence, where ancient rivers of lava shaped its plain. Its soil, rich in basalt and minerals, holds the memory of a volcanic past, reflecting the serene beauty of a Moon that transformed fire into tranquility.<br><br>The final image was the result of capturing 2,000 frames, with the 350 best ones being stacked.<br><br>SETUP:<br>TELESCOPE: SKY-WATCHER DOBSONIAN 250P FLEXTUBE<br>CAMERA: URANUS-C (IMX585)<br>BARLOW: 3x SVBONY ACHRO<br>FILTRO: UV/IR CUT SVBONY<br><br>SOFTWARES:<br>SHARPCAP; AUTOSTAKKERT!; ASTROSURFACE; LIGHTROOM.</p><p data-rte-preserve-empty="true"><strong>Name:</strong> Nyêrdson Ferreira</p><p data-rte-preserve-empty="true"><strong>Website or Facebook Profile:</strong> <a target="_blank" href="http://www.instagram.com/phot.astro?igsh=amV3ZGV4d3k0dGdx">http://www.instagram.com/phot.astro?igsh=amV3ZGV4d3k0dGdx</a></p>]]></content:encoded><media:content type="image/jpeg" url="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/7e53b029-5724-4c27-9d4b-7381b0885920/1001507438.jpg?format=1500w" medium="image" isDefault="true" width="1500" height="1875"><media:title type="plain">Sea of Serenity in mineral detail</media:title></media:content></item><item><title>Clusters in a Sea of Stars – M22 + M28</title><category>2026</category><dc:creator>Charles Lillo</dc:creator><pubDate>Sun, 02 Aug 2026 04:00:36 +0000</pubDate><link>https://www.aapod2.com/blog/messier-22-m22-and-messier-28</link><guid isPermaLink="false">5debd4b16fcd7b02905712ff:5debd4f1c2fab6555bff00b5:6a6cb5dab1ee864a20732280</guid><description><![CDATA[This wide-field deep-sky image captures two of the southern sky's finest 
globular clusters, Messier 22 (M22) and Messier 28 (M28), set against the 
dense star fields of the Milky Way's central bulge in the constellation 
Sagittarius.

Located approximately 10,600 light-years away, M22 is one of the closest 
and brightest globular clusters to Earth, containing hundreds of thousands 
of ancient stars. Nearby lies M28, a more compact cluster located roughly 
18,000 light-years away. Embedded across this field are several notable 
deep-sky objects, including the planetary nebulae NGC 6629, NGC 6644, and 
the intracluster planetary nebula GJJC 1, alongside numerous variable and 
carbon stars.]]></description><content:encoded><![CDATA[<figure class="
              sqs-block-image-figure
              intrinsic
            "
        >
          
        
        

        
          
            
          
            
                
                
                
                
                
                
                
                <img data-stretch="false" data-image="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/f14014b6-b5c3-4184-8563-86aa724327c0/M22%2BM28-reduced-0.25.jpg" data-image-dimensions="4732x3154" 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/f14014b6-b5c3-4184-8563-86aa724327c0/M22%2BM28-reduced-0.25.jpg?format=1000w" width="4732" height="3154" 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/f14014b6-b5c3-4184-8563-86aa724327c0/M22%2BM28-reduced-0.25.jpg?format=100w 100w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/f14014b6-b5c3-4184-8563-86aa724327c0/M22%2BM28-reduced-0.25.jpg?format=300w 300w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/f14014b6-b5c3-4184-8563-86aa724327c0/M22%2BM28-reduced-0.25.jpg?format=500w 500w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/f14014b6-b5c3-4184-8563-86aa724327c0/M22%2BM28-reduced-0.25.jpg?format=750w 750w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/f14014b6-b5c3-4184-8563-86aa724327c0/M22%2BM28-reduced-0.25.jpg?format=1000w 1000w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/f14014b6-b5c3-4184-8563-86aa724327c0/M22%2BM28-reduced-0.25.jpg?format=1500w 1500w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/f14014b6-b5c3-4184-8563-86aa724327c0/M22%2BM28-reduced-0.25.jpg?format=2500w 2500w" loading="lazy" decoding="async" data-loader="sqs">

            
          
        
          
        

        
      
        </figure>
      

    
  


  



  
  <p data-rte-preserve-empty="true"><strong>Image Title:</strong> Clusters in a Sea of Stars - M22 + M28</p><p data-rte-preserve-empty="true"><strong>Copyright:</strong> Daniel Paull</p><p data-rte-preserve-empty="true"><strong>Date image was taken:</strong> July 14, 2026</p><p data-rte-preserve-empty="true"><strong>Location:</strong> Gidgegannup, Western Australia</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> Globular clusters are often photographed as isolated jewels against the darkness of space. Yet in reality, they are anything but isolated. This image places two of the southern sky's finest globular clusters, Messier 22 and Messier 28, in their natural environment: the extraordinarily rich star fields of the Milky Way's central bulge. Rather than standing apart from the background, the clusters are integrated seamlessly with the surrounding star field, reminding us that they are members of our own Galaxy, sharing the same cosmic neighbourhood.<br><br>Located in the constellation Sagittarius, M22 lies approximately 10,600 light-years from Earth and is one of the closest and brightest globular clusters in the night sky. It contains several hundred thousand ancient stars, many over 12 billion years old, making it a surviving relic from the earliest epochs of the Milky Way's formation.<br><br>Nearby lies Messier 28, a more compact and distant globular cluster roughly 18,000 light-years away. While often overshadowed by its famous neighbour, M28 is itself home to hundreds of thousands of stars and has become scientifically significant through the discovery of numerous millisecond pulsars within the cluster.<br><br>This image combines approximately six hours of exposure using a Celestron RASA 11 and QHY600C, followed by 2x drizzle integration to produce a final image of approximately 240 megapixels, with an effective sampling of around 0.6 arcseconds per pixel.<br><br>At f/2.2, the Celestron RASA 11 collects light extraordinarily quickly, making it ideal for revealing faint stars across the Galactic Bulge. The trade-off is that every optical imperfection becomes visible. Tiny errors in focus, sensor tilt, collimation or tracking quickly reveal themselves when nearly every pixel contains stellar data. With such an overwhelmingly dense field, there is nowhere for acquisition or processing mistakes to hide.<br><br>The result is an image that rewards exploration at full resolution, where countless faint stars and hidden gems continue to emerge as the viewer zooms deeper into the field.<br><br>This image is best viewed at full resolution on Astrometrical: <a target="_blank" href="https://astrometrical.com/works/clusters-in-a-sea-of-stars-m22-m28">https://astrometrical.com/works/clusters-in-a-sea-of-stars-m22-m28</a><br><br>The field includes several notable objects:<br><br>* Globular Clusters M22, M28, and NGC 6642<br>* Planetary Nebula NGC 6629<br>* Planetary Nebula NGC 6644<br>* Intracluster Planetary Nebula GJJC 1 (also known as PK 009-07.1)<br>* Numerous variable stars<br>* Numerous carbon stars<br>* Background galaxies and other fuzzies<br><br>Highrer resolution images can be supplied on request.</p><p data-rte-preserve-empty="true"><strong>Name:</strong> Daniel Paull</p><p data-rte-preserve-empty="true"><strong>Website or Facebook Profile:</strong> <a target="_blank" href="https://www.facebook.com/astrometrical">https://www.facebook.com/astrometrical</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/f14014b6-b5c3-4184-8563-86aa724327c0/M22%2BM28-reduced-0.25.jpg?format=1500w" medium="image" isDefault="true" width="1500" height="1000"><media:title type="plain">Clusters in a Sea of Stars – M22 + M28</media:title></media:content></item><item><title>Kokerboom Under the Namibian Milky Way</title><category>2026</category><dc:creator>Charles Lillo</dc:creator><pubDate>Sat, 01 Aug 2026 04:00:47 +0000</pubDate><link>https://www.aapod2.com/blog/kokerboom-under-the-namibian-milky-way</link><guid isPermaLink="false">5debd4b16fcd7b02905712ff:5debd4f1c2fab6555bff00b5:6a6cb2eebbbe5848b2a36d11</guid><description><![CDATA[Captured from the deep, dark skies of the Namib Desert at the Rooisand 
Desert Ranch in Namibia, this striking composite image highlights a native 
quiver tree (Aloe dichotoma) silhouetted against the core of the Milky Way. 
Known locally as the Kokerboom, these iconic desert aloe plants store water 
in their fleshy trunks to endure extreme heat and can live for hundreds of 
years.]]></description><content:encoded><![CDATA[<figure class="
              sqs-block-image-figure
              intrinsic
            "
        >
          
        
        

        
          
            
          
            
                
                
                
                
                
                
                
                <img data-stretch="false" data-image="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/24c89222-3b8d-4117-86c8-08af21dea27b/7F1A0033-C287-40AB-B440-375CB777D0E5.jpeg" data-image-dimensions="3500x2933" 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/24c89222-3b8d-4117-86c8-08af21dea27b/7F1A0033-C287-40AB-B440-375CB777D0E5.jpeg?format=1000w" width="3500" height="2933" 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/24c89222-3b8d-4117-86c8-08af21dea27b/7F1A0033-C287-40AB-B440-375CB777D0E5.jpeg?format=100w 100w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/24c89222-3b8d-4117-86c8-08af21dea27b/7F1A0033-C287-40AB-B440-375CB777D0E5.jpeg?format=300w 300w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/24c89222-3b8d-4117-86c8-08af21dea27b/7F1A0033-C287-40AB-B440-375CB777D0E5.jpeg?format=500w 500w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/24c89222-3b8d-4117-86c8-08af21dea27b/7F1A0033-C287-40AB-B440-375CB777D0E5.jpeg?format=750w 750w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/24c89222-3b8d-4117-86c8-08af21dea27b/7F1A0033-C287-40AB-B440-375CB777D0E5.jpeg?format=1000w 1000w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/24c89222-3b8d-4117-86c8-08af21dea27b/7F1A0033-C287-40AB-B440-375CB777D0E5.jpeg?format=1500w 1500w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/24c89222-3b8d-4117-86c8-08af21dea27b/7F1A0033-C287-40AB-B440-375CB777D0E5.jpeg?format=2500w 2500w" loading="lazy" decoding="async" data-loader="sqs">

            
          
        
          
        

        
      
        </figure>
      

    
  


  



  
  <p data-rte-preserve-empty="true"><strong>Image Title:</strong> Kokerboom</p><p data-rte-preserve-empty="true"><strong>Copyright:</strong> Marek Skowrone</p><p data-rte-preserve-empty="true"><strong>Date image was taken:</strong> June 14, 2026</p><p data-rte-preserve-empty="true"><strong>Location:</strong> Rooisand Desert Ranch<br>Namibia</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> Honestly, I look at the photo and I'm still in awe. Neither the description nor the video can adequately capture what it feels like to be in the absolute, piercing darkness of the Namib Desert. When you lift your head, millions of stars are uncountable, and the mighty ribbon of the Milky Way shines so brightly that it casts a delicate shadow on the ground. You automatically feel tiny, frozen in place, completely oblivious to the world around you.<br><br>In this cosmic medical spectacle, the raw elements of the quiver tree—sometimes called a tree—are actually gigantic, a desert aloe that stores water in its fleshy trunks, even through the fiercest African heat. It grows incredibly slowly, which is why the largest specimens visible in the photo can be as old as 200-300 years. For centuries, they have been silent witnesses to the history of these lands. It was from their dead, lightweight branches that the indigenous inhabitants – the Bushmen – carved out soft cores, creating perfect quivers for their arrows, hence their current name.<br><br>This journey to my great dreams. You with this view – I have a speech that will secure a fraction of the delight and magic that is controlled by that night.<br>Equipment used for capture:<br>* Camera: Canon 6D (Modified)<br>* Lens: Samyang 24mm f/2.8<br>* Tracker: Move Shoot Move Nomad<br><br>– Exposure parameters:<br>* Sky: 56 frames x 60 seconds, ISO 1600, f/2.8 (tracked)<br>* Foreground: 1 frame x 7 seconds, ISO 800, f/2.8 (untracked)</p><p data-rte-preserve-empty="true"><strong>Name:</strong> Marek Skowronek</p><p data-rte-preserve-empty="true"><strong>Website or Facebook Profile:</strong> <a target="_blank" href="https://www.facebook.com/share/1Lcr4uMLX8/?mibextid=wwXIfr">https://www.facebook.com/share/1Lcr4uMLX8/?mibextid=wwXIfr</a></p>]]></content:encoded><media:content type="image/jpeg" url="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/24c89222-3b8d-4117-86c8-08af21dea27b/7F1A0033-C287-40AB-B440-375CB777D0E5.jpeg?format=1500w" medium="image" isDefault="true" width="1500" height="1257"><media:title type="plain">Kokerboom Under the Namibian Milky Way</media:title></media:content></item><item><title>Rho Ophiuchi dancing in Hydrogen-alpha</title><category>2026</category><dc:creator>Charles Lillo</dc:creator><pubDate>Fri, 31 Jul 2026 04:01:19 +0000</pubDate><link>https://www.aapod2.com/blog/rho-ophiuchi-dancing-in-hydrogen-alpha</link><guid isPermaLink="false">5debd4b16fcd7b02905712ff:5debd4f1c2fab6555bff00b5:6a6a3429dd3847699fec111d</guid><description><![CDATA[Located approximately 460 light-years away in the constellation Ophiuchus, 
the Rho Ophiuchi cloud complex is one of the closest active star-forming 
regions to our solar system. Captured here in narrow-band Hydrogen-alpha 
(H$\alpha$) emission along with RGB broadband data, the image highlights 
the glowing ionized hydrogen gas ($\text{H II}$) energetic young stars 
carve out as intense ultraviolet radiation strips electrons from neutral 
hydrogen atoms. As these electrons recombine, they emit light at the 
characteristic Balmer-alpha wavelength of 656.3 nanometers, tracing the 
turbulent shock fronts, wispy filaments, and expanding cavity walls where 
radiation pressure and stellar winds sculpt the surrounding molecular 
cloud. Interspersed with dense lane structures of interstellar dust that 
absorb background starlight, this region provides a clear view into the 
early dynamic stages of stellar evolution and protostellar disk formation]]></description><content:encoded><![CDATA[<figure class="
              sqs-block-image-figure
              intrinsic
            "
        >
          
        
        

        
          
            
          
            
                
                
                
                
                
                
                
                <img data-stretch="false" data-image="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/bbd2211f-a6ee-4f0d-82b5-0d7450d2b2ba/Rho_Ophiuchi_V4+final-2.jpeg" data-image-dimensions="6219x7836" 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/bbd2211f-a6ee-4f0d-82b5-0d7450d2b2ba/Rho_Ophiuchi_V4+final-2.jpeg?format=1000w" width="6219" height="7836" 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/bbd2211f-a6ee-4f0d-82b5-0d7450d2b2ba/Rho_Ophiuchi_V4+final-2.jpeg?format=100w 100w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/bbd2211f-a6ee-4f0d-82b5-0d7450d2b2ba/Rho_Ophiuchi_V4+final-2.jpeg?format=300w 300w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/bbd2211f-a6ee-4f0d-82b5-0d7450d2b2ba/Rho_Ophiuchi_V4+final-2.jpeg?format=500w 500w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/bbd2211f-a6ee-4f0d-82b5-0d7450d2b2ba/Rho_Ophiuchi_V4+final-2.jpeg?format=750w 750w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/bbd2211f-a6ee-4f0d-82b5-0d7450d2b2ba/Rho_Ophiuchi_V4+final-2.jpeg?format=1000w 1000w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/bbd2211f-a6ee-4f0d-82b5-0d7450d2b2ba/Rho_Ophiuchi_V4+final-2.jpeg?format=1500w 1500w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/bbd2211f-a6ee-4f0d-82b5-0d7450d2b2ba/Rho_Ophiuchi_V4+final-2.jpeg?format=2500w 2500w" loading="lazy" decoding="async" data-loader="sqs">

            
          
        
          
        

        
      
        </figure>]]></content:encoded><media:content type="image/jpeg" url="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/bbd2211f-a6ee-4f0d-82b5-0d7450d2b2ba/Rho_Ophiuchi_V4+final-2.jpeg?format=1500w" medium="image" isDefault="true" width="1500" height="1890"><media:title type="plain">Rho Ophiuchi dancing in Hydrogen-alpha</media:title></media:content></item><item><title>Comet 10P-Temple</title><category>2026</category><dc:creator>Charles Lillo</dc:creator><pubDate>Thu, 30 Jul 2026 04:01:01 +0000</pubDate><link>https://www.aapod2.com/blog/comet-10p/tempel-2</link><guid isPermaLink="false">5debd4b16fcd7b02905712ff:5debd4f1c2fab6555bff00b5:6a6a32e37115230e4d01e8ab</guid><description><![CDATA[Comet 10P/Tempel 2 is a short-period, Jupiter-family comet with an orbital 
period of approximately 5.4 years. Captured in this telescopic exposure 
from July 21, 2026, the comet displays a bright, well-condensed nuclear 
region surrounded by a characteristic greenish coma, a hue primarily 
produced by the fluorescence of diatomic carbon and cyanogen gases as 
volatile ice sublimates under solar ultraviolet radiation. Extending across 
the nucleus is a thin, linear feature—not a typical radiation-driven dust 
tail, but a permanent debris trail composed of larger millimeter- to 
centimeter-sized particles deposited over past perihelion passages. Because 
Earth crossed the comet’s orbital plane around July 20, this edge-on 
viewing geometry enhanced the trail's apparent surface brightness, 
projecting it as a striking, narrow spike while the comet shone at 
magnitude 13.4 in the constellation Capricornus, roughly 64.4 million 
kilometers from Earth.]]></description><content:encoded><![CDATA[<figure class="
              sqs-block-image-figure
              intrinsic
            "
        >
          
        
        

        
          
            
          
            
                
                
                
                
                
                
                
                <img data-stretch="false" data-image="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/06c7590e-f7f7-40a5-b6b0-44209698eb80/10P-Temple.jpg" data-image-dimensions="12470x8011" 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/06c7590e-f7f7-40a5-b6b0-44209698eb80/10P-Temple.jpg?format=1000w" width="12470" height="8011" 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/06c7590e-f7f7-40a5-b6b0-44209698eb80/10P-Temple.jpg?format=100w 100w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/06c7590e-f7f7-40a5-b6b0-44209698eb80/10P-Temple.jpg?format=300w 300w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/06c7590e-f7f7-40a5-b6b0-44209698eb80/10P-Temple.jpg?format=500w 500w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/06c7590e-f7f7-40a5-b6b0-44209698eb80/10P-Temple.jpg?format=750w 750w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/06c7590e-f7f7-40a5-b6b0-44209698eb80/10P-Temple.jpg?format=1000w 1000w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/06c7590e-f7f7-40a5-b6b0-44209698eb80/10P-Temple.jpg?format=1500w 1500w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/06c7590e-f7f7-40a5-b6b0-44209698eb80/10P-Temple.jpg?format=2500w 2500w" loading="lazy" decoding="async" data-loader="sqs">

            
          
        
          
        

        
      
        </figure>
      

    
  


  



  
  <p data-rte-preserve-empty="true"><strong>Image Title:</strong> Comet 10P-Temple</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> July 21, 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> Orbita attorno al Sole una volta ogni 5,4 anni, attualmente visibile con binocoli o piccoli telescopi verso la costellazione del Capricorno. La cometa periodica immortalata in questa immagine telescopica del 21 Luglio 2026 alle ore 01:30 circa mostra una brillante regione nucleare e una chioma verdastra. Nello scatto si nota anche una sottile scia di polvere, non una tipica coda di polvere, che si estende sia a est che a ovest del nucleo cometario.<br>A differenza della coda di polvere di una cometa, che tende ad aprirsi temporaneamente in direzione opposta al Sole, questa scia di polvere è dovuta alla polvere residua rilasciata durante le numerose orbite passate lungo il piano orbitale da parte della cometa stessa.<br>Giorno 20 Luglio 2026 infatti la Terra ha attraversando il piano orbitale facendo risultare tale scia più sottile e luminosa per un gioco prospettico.<br>Il massimo avvicinamento della cometa 10P/Tempel alla Terra avverrà martedì 4 agosto 2026 a una distanza di 62.005.862 chilometri.<br>Al momento della ripresa brillava di una magnitudine di circa 13,40 e si trovava ad una distanza di circa 64.400.000 km dalla Terra e di circa 212.960.000 km dal Sole.<br><br>&nbsp;Light: 102 x 120 seconds<br>&nbsp;Filter: Optolong L-Qef<br>&nbsp;Camera: Asi 294 mc pro<br>&nbsp;Telescope: Sharpstar 94 EDPH<br>&nbsp;Mount: Skywatcher Eq 6-r Pro<br>&nbsp;Acquisition: Asiair Plus<br>&nbsp;Software: DSS - Pixinsight – Photoshop<br>&nbsp;Shots: 21/07/2026<br>&nbsp;Location: Torricella (TA) ITALY<br>&nbsp;Sky Bortle: 6<br>&nbsp;Author: PRO’ GIACOMO.</p><p data-rte-preserve-empty="true"><strong>Name:</strong> giacomo pro'</p><p data-rte-preserve-empty="true"><strong>Website or Facebook Profile:</strong> <a target="_blank" 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/06c7590e-f7f7-40a5-b6b0-44209698eb80/10P-Temple.jpg?format=1500w" medium="image" isDefault="true" width="1500" height="964"><media:title type="plain">Comet 10P-Temple</media:title></media:content></item><item><title>Flaming Skull Nebula SH2-68 with cometary like tail</title><category>2026</category><dc:creator>Charles Lillo</dc:creator><pubDate>Wed, 29 Jul 2026 04:00:21 +0000</pubDate><link>https://www.aapod2.com/blog/flaming-skull-nebula-sh2-68-with-cometary-like-tail</link><guid isPermaLink="false">5debd4b16fcd7b02905712ff:5debd4f1c2fab6555bff00b5:6a675ef5b669af12b83f8523</guid><description><![CDATA[Located roughly 1,100 light-years away in the constellation Serpens, 
Sh2-68—dramatically nicknamed the Flaming Skull Nebula—is an ancient, 
low-surface-brightness planetary nebula estimated to be at least 45,000 
years old.

What makes this target particularly fascinating is its strong interaction 
with the surrounding interstellar medium. As its high-proper-motion central 
white dwarf star travels through space, the expanding shell of ionized gas 
is stripped back, trailing an extended, cometary-like tail of hydrogen 
emission behind a glowing, blue oxygen-rich core.]]></description><content:encoded><![CDATA[<figure class="
              sqs-block-image-figure
              intrinsic
            "
        >
          
        
        

        
          
            
          
            
                
                
                
                
                
                
                
                <img data-stretch="false" data-image="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/1785159479307-KOG2EB4LQN4VTBY1QSAX/Foraxxbrighter.jpg" data-image-dimensions="7200x4524" 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/1785159479307-KOG2EB4LQN4VTBY1QSAX/Foraxxbrighter.jpg?format=1000w" width="7200" height="4524" 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/1785159479307-KOG2EB4LQN4VTBY1QSAX/Foraxxbrighter.jpg?format=100w 100w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/1785159479307-KOG2EB4LQN4VTBY1QSAX/Foraxxbrighter.jpg?format=300w 300w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/1785159479307-KOG2EB4LQN4VTBY1QSAX/Foraxxbrighter.jpg?format=500w 500w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/1785159479307-KOG2EB4LQN4VTBY1QSAX/Foraxxbrighter.jpg?format=750w 750w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/1785159479307-KOG2EB4LQN4VTBY1QSAX/Foraxxbrighter.jpg?format=1000w 1000w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/1785159479307-KOG2EB4LQN4VTBY1QSAX/Foraxxbrighter.jpg?format=1500w 1500w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/1785159479307-KOG2EB4LQN4VTBY1QSAX/Foraxxbrighter.jpg?format=2500w 2500w" loading="lazy" decoding="async" data-loader="sqs">

            
          
        
          
        

        
      
        </figure>
      

    
  


  



  
  <p data-rte-preserve-empty="true"><strong>Image Title:</strong> Flaming Skull Nebula SH2-68 with cometary like tail</p><p data-rte-preserve-empty="true"><strong>Copyright:</strong> Franklin Marek</p><p data-rte-preserve-empty="true"><strong>Date image was taken:</strong> July 11, 2026</p><p data-rte-preserve-empty="true"><strong>Location:</strong> Madisonville, LA</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> SH2-68 is a little studied ancient low surface brightness planetary nebula with an amazing name The Flaming Skull Nebula. What makes it really interesting is it is a confirmed case of PN-interstellar-medium interaction creating almost a cometary like tail. I hope you guys enjoy the image and the science below!<br><br>My Video on this object: <a target="_blank" href="https://youtu.be/tN6IzCNIQgs">https://youtu.be/tN6IzCNIQgs</a><br><br>My technical paper: <a target="_blank" href="https://www.setiastro.com/s/Calibrated-Emission-Line-Surface-Photometry-of-the-High-Proper-Motion-Planetary-Nebula-SH2-68.pdf">https://www.setiastro.com/s/Calibrated-Emission-Line-Surface-Photometry-of-the-High-Proper-Motion-Planetary-Nebula-SH2-68.pdf</a><br><br>Acquisition details:<br>Imaging Telescopes Or Lenses<br>iOptron 10-inch F/4 Imaging Newtonian<br>Imaging Cameras<br>ZWO ASI294MM Pro<br>Mounts<br>Sky-Watcher NEQ6-Pro<br>Filters<br>Antlia EDGE H-alpha 4.5nm 2" · Antlia EDGE OIII 4.5 nm 2" · Antlia EDGE SII 4.5 nm 2"<br>Accessories<br>Askar M54 OAG × · MoonLite CRL 2.5 inch Large Format Newtonian Focuser · Sharpstar 2" 0.95× coma corrector (CRC2095) × · WandererAstro WandererRotator Mini · ZWO EFW 7 x 2″<br><br>Dates:<br>June 9 - 11, 2026<br>June 28 - 29, 2026<br>July 3, 2026<br>July 7 - 11, 2026<br>Frames:<br>Antlia EDGE H-alpha 4.5nm 2": 30×900″(7h 30′) (gain: 121.00) f/3.8 -10°C bin 1×1<br>Antlia EDGE H-alpha 4.5nm 2": 13×900″(3h 15′) (gain: 121.00) f/3.8 -5°C bin 1×1<br>Antlia EDGE H-alpha 4.5nm 2": 31×900″(7h 45′) (gain: 121.00) f/3.8 -8°C bin 1×1<br>Antlia EDGE OIII 4.5 nm 2": 51×900″(12h 45′) (gain: 121.00) f/3.8 -10°C bin 1×1<br>Antlia EDGE OIII 4.5 nm 2": 21×900″(5h 15′) (gain: 121.00) f/3.8 -8°C bin 1×1<br>Antlia EDGE SII 4.5 nm 2": 18×900″(4h 30′) (gain: 121.00) f/3.8 -10°C bin 1×1<br>Antlia EDGE SII 4.5 nm 2": 31×900″(7h 45′) (gain: 121.00) f/3.8 -8°C bin 1×1<br>Antlia EDGE SII 4.5 nm 2": 4×900″(1h) (gain: 121.00) f/3.8 -9°C bin 1×1<br>Integration:<br>49h 45′<br>Avg. Moon age:<br>22.37 days<br>Avg. Moon phase:<br>48.40%<br>Bortle Dark-Sky Scale:<br>6.00<br>Temperature:<br>23.93°C</p><p data-rte-preserve-empty="true"><strong>Name:</strong> Franklin Marek</p><p data-rte-preserve-empty="true"><strong>Email:</strong><a target="_blank" href="mailto:frank@setiastro.com">frank@setiastro.com</a></p><p data-rte-preserve-empty="true"><strong>Website or Facebook Profile:</strong><a target="_blank" href="http://www.setiastro.com/">http://www.setiastro.com</a></p>


  










  


  
    <iframe allow="accelerometer; autoplay; clipboard-write; encrypted-media; gyroscope; picture-in-picture; web-share" referrerpolicy="strict-origin-when-cross-origin" allowfullscreen src="https://www.youtube.com/embed/tN6IzCNIQgs?si=nIQalrt-z1TfFdZH" width="560" frameborder="0" title="YouTube video player" height="315"></iframe>]]></content:encoded><media:content type="image/jpeg" url="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/1785159479307-KOG2EB4LQN4VTBY1QSAX/Foraxxbrighter.jpg?format=1500w" medium="image" isDefault="true" width="1500" height="943"><media:title type="plain">Flaming Skull Nebula SH2-68 with cometary like tail</media:title></media:content></item><item><title>NGC 7129: Cosmic Rose in Cepheus</title><category>2026</category><dc:creator>Charles Lillo</dc:creator><pubDate>Tue, 28 Jul 2026 04:00:23 +0000</pubDate><link>https://www.aapod2.com/blog/4zbbxzusw0zz103e2weyjfx2u1krvs</link><guid isPermaLink="false">5debd4b16fcd7b02905712ff:5debd4f1c2fab6555bff00b5:6a67606725d0ca015cd6f9d4</guid><description><![CDATA[NGC 7129: Cosmic Rose in Cepheus

Nestled roughly 3,300 light-years away in the constellation Cepheus, NGC 
7129 is a striking reflection nebula illuminated by a young open cluster of 
stars. Glowing like a stellar rose amidst cosmic dust, this active 
star-forming region features vibrant blue light reflected off interstellar 
dust clouds surrounding a cluster of stars only a few million years old.

Captured over 11.6 hours of exposure using a broad-band LRGB setup from the 
backyard observatory "Videre Videnda" in Oisterwijk, Netherlands, this 
image reveals the delicate, intricate structures and ambient dust trailing 
through the rich field of Cepheus.]]></description><content:encoded><![CDATA[<figure class="
              sqs-block-image-figure
              intrinsic
            "
        >
          
        
        

        
          
            
          
            
                
                
                
                
                
                
                
                <img data-stretch="false" data-image="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/c124d434-78eb-4e9e-a37c-a02bc8e5a244/NGC7129_DEF.jpg" data-image-dimensions="3293x2464" 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/c124d434-78eb-4e9e-a37c-a02bc8e5a244/NGC7129_DEF.jpg?format=1000w" width="3293" height="2464" 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/c124d434-78eb-4e9e-a37c-a02bc8e5a244/NGC7129_DEF.jpg?format=100w 100w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/c124d434-78eb-4e9e-a37c-a02bc8e5a244/NGC7129_DEF.jpg?format=300w 300w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/c124d434-78eb-4e9e-a37c-a02bc8e5a244/NGC7129_DEF.jpg?format=500w 500w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/c124d434-78eb-4e9e-a37c-a02bc8e5a244/NGC7129_DEF.jpg?format=750w 750w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/c124d434-78eb-4e9e-a37c-a02bc8e5a244/NGC7129_DEF.jpg?format=1000w 1000w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/c124d434-78eb-4e9e-a37c-a02bc8e5a244/NGC7129_DEF.jpg?format=1500w 1500w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/c124d434-78eb-4e9e-a37c-a02bc8e5a244/NGC7129_DEF.jpg?format=2500w 2500w" loading="lazy" decoding="async" data-loader="sqs">

            
          
        
          
        

        
      
        </figure>
      

    
  


  



  
  <p data-rte-preserve-empty="true"><strong>Image Title:</strong> NGC7129</p><p data-rte-preserve-empty="true"><strong>Copyright:</strong> Jeroen Moonen</p><p data-rte-preserve-empty="true"><strong>Date image was taken:</strong> July 14, 2026</p><p data-rte-preserve-empty="true"><strong>Location:</strong> Oisterwijk, back yard observatory "Videre Videnda" - The Netherlands</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> In the dust of constellation Cepheus surrounding the famous Iris and Ghost nebula there's a small blue reflection nebula called NGC7129 and an open cluster called NGC7142. The nebula has many fine details. This image was taken using a 10" F4.7 Newton and STF8300M camera. Exposure times L 62x 5 min and RGB 26-25-27x 5 min.<br>Total exposure time 11 hours 40 min.</p><p data-rte-preserve-empty="true"><strong>Name:</strong> Jeroen Moonen</p>]]></content:encoded><media:content type="image/jpeg" url="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/c124d434-78eb-4e9e-a37c-a02bc8e5a244/NGC7129_DEF.jpg?format=1500w" medium="image" isDefault="true" width="1500" height="1122"><media:title type="plain">NGC 7129: Cosmic Rose in Cepheus</media:title></media:content></item><item><title>Ic 5146 HA RGB - The cocoon nebula</title><category>2026</category><dc:creator>Charles Lillo</dc:creator><pubDate>Mon, 27 Jul 2026 12:24:01 +0000</pubDate><link>https://www.aapod2.com/blog/ic-5146-ha-rgb-the-cocoon-nebula</link><guid isPermaLink="false">5debd4b16fcd7b02905712ff:5debd4f1c2fab6555bff00b5:6a674d5125d0ca015cd04052</guid><description><![CDATA[Located approximately 4,000 light-years away in the constellation Cygnus, 
IC 5146—famously known as the Cocoon Nebula—presents a striking cosmic 
display of emission, reflection, and absorption nebulae. Glowing softly at 
the end of a long dark dust cloud, this star-forming region shines with 
vibrant pinkish-red Hydrogen-alpha emissions surrounding a central cluster 
of young stars.

Captured over 11 hours of exposure using a broad-band RGB and dual-band 
narrowband filter setup, this image beautifully highlights the intricate 
dark dust lanes trailing into the dense, star-filled cosmic backdrop.]]></description><content:encoded><![CDATA[<figure class="
              sqs-block-image-figure
              intrinsic
            "
        >
          
        
        

        
          
            
          
            
                
                
                
                
                
                
                
                <img data-stretch="false" data-image="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/3d31037b-f481-42e7-ac15-e504cfd1685d/17136.jpg" data-image-dimensions="5899x4070" 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/3d31037b-f481-42e7-ac15-e504cfd1685d/17136.jpg?format=1000w" width="5899" height="4070" 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/3d31037b-f481-42e7-ac15-e504cfd1685d/17136.jpg?format=100w 100w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/3d31037b-f481-42e7-ac15-e504cfd1685d/17136.jpg?format=300w 300w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/3d31037b-f481-42e7-ac15-e504cfd1685d/17136.jpg?format=500w 500w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/3d31037b-f481-42e7-ac15-e504cfd1685d/17136.jpg?format=750w 750w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/3d31037b-f481-42e7-ac15-e504cfd1685d/17136.jpg?format=1000w 1000w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/3d31037b-f481-42e7-ac15-e504cfd1685d/17136.jpg?format=1500w 1500w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/3d31037b-f481-42e7-ac15-e504cfd1685d/17136.jpg?format=2500w 2500w" loading="lazy" decoding="async" data-loader="sqs">

            
          
        
          
        

        
      
        </figure>
      

    
  


  



  
  <p data-rte-preserve-empty="true"><strong>Image Title:</strong> Ic 5146 HA RGB - The cocoon nebula</p><p data-rte-preserve-empty="true"><strong>Copyright:</strong> Clément DANIEL</p><p data-rte-preserve-empty="true"><strong>Date image was taken:</strong> July 11, 2026</p><p data-rte-preserve-empty="true"><strong>Location:</strong> Pleine-Fougères, Brittany</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> 5146 ou la nébuleuse du cocon<br><br>Capturée en HA-RGB<br><br>Elle est située dans la constellation du Cygne à environ 4000 années lumières. Entre nébuleuse sombre, à réflexion et en émission, cette nébuleuse est gorgée de signal.<br><br>Équipement :<br><br>Skywatcher EQ6-R-PRO<br>Ts Hypergraph 150 f2.8 carbon<br>Zwo Asi 2600Mc Duo<br>Filtre Idas Nbz 2"<br>Asiair PLUS<br>Zwo CAA<br>Zwo EFW 7×2"<br><br>Exifs :<br><br>RGB : 85×300s (7h05)<br>IDAS NBZ : 26×600s (4h20)<br><br>Traitement : Pixinsight, BxT, NxT, SxT, Lightroom mobile<br><br>Astrobin : <a target="_blank" href="https://astrob.in/4tq1e4/0/">https://astrob.in/4tq1e4/0/</a></p><p data-rte-preserve-empty="true"><strong>Name:</strong> Clément Daniel</p><p data-rte-preserve-empty="true"><strong>Website or Facebook Profile:</strong> <a target="_blank" href="https://www.facebook.com/share/1JUueckdmq/">https://www.facebook.com/share/1JUueckdmq/</a></p>]]></content:encoded><media:content type="image/jpeg" url="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/3d31037b-f481-42e7-ac15-e504cfd1685d/17136.jpg?format=1500w" medium="image" isDefault="true" width="1500" height="1035"><media:title type="plain">Ic 5146 HA RGB - The cocoon nebula</media:title></media:content></item><item><title>OMEGA CENTAURI HALRGB</title><category>2026</category><dc:creator>Charles Lillo</dc:creator><pubDate>Sun, 26 Jul 2026 04:00:46 +0000</pubDate><link>https://www.aapod2.com/blog/omega-centauri-halrgb</link><guid isPermaLink="false">5debd4b16fcd7b02905712ff:5debd4f1c2fab6555bff00b5:6a64fb4f44644f1c0f9a73df</guid><description><![CDATA[Located roughly 17,000 light-years away in the constellation Centaurus, 
Omega Centauri (NGC 5139) is the largest and most luminous globular cluster 
in the Milky Way, housing over 10 million stars. This deep H-alpha and LRGB 
(HALRGB) composite reveals the brilliant, densely packed stellar core 
alongside subtle surrounding interstellar structures and faint atmospheric 
glow across the deep field.]]></description><content:encoded><![CDATA[<figure class="
              sqs-block-image-figure
              intrinsic
            "
        >
          
        
        

        
          
            
          
            
                
                
                
                
                
                
                
                <img data-stretch="false" data-image="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/5983a8a6-42f8-4907-bfdb-e68f94822c86/1000342098.jpg" data-image-dimensions="6000x3956" 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/5983a8a6-42f8-4907-bfdb-e68f94822c86/1000342098.jpg?format=1000w" width="6000" height="3956" 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/5983a8a6-42f8-4907-bfdb-e68f94822c86/1000342098.jpg?format=100w 100w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/5983a8a6-42f8-4907-bfdb-e68f94822c86/1000342098.jpg?format=300w 300w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/5983a8a6-42f8-4907-bfdb-e68f94822c86/1000342098.jpg?format=500w 500w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/5983a8a6-42f8-4907-bfdb-e68f94822c86/1000342098.jpg?format=750w 750w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/5983a8a6-42f8-4907-bfdb-e68f94822c86/1000342098.jpg?format=1000w 1000w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/5983a8a6-42f8-4907-bfdb-e68f94822c86/1000342098.jpg?format=1500w 1500w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/5983a8a6-42f8-4907-bfdb-e68f94822c86/1000342098.jpg?format=2500w 2500w" loading="lazy" decoding="async" data-loader="sqs">

            
          
        
          
        

        
      
        </figure>]]></content:encoded><media:content type="image/jpeg" url="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/5983a8a6-42f8-4907-bfdb-e68f94822c86/1000342098.jpg?format=1500w" medium="image" isDefault="true" width="1500" height="989"><media:title type="plain">OMEGA CENTAURI HALRGB</media:title></media:content></item><item><title>Whispers of a Dying Star: Messier 27</title><category>2026</category><dc:creator>Charles Lillo</dc:creator><pubDate>Sat, 25 Jul 2026 04:00:04 +0000</pubDate><link>https://www.aapod2.com/blog/whispers-of-a-dying-star-messier-27</link><guid isPermaLink="false">5debd4b16fcd7b02905712ff:5debd4f1c2fab6555bff00b5:6a6372f75aae84664d9a444a</guid><description><![CDATA[Messier 27 is a prominent planetary nebula representing the late 
evolutionary stage of an intermediate-mass, Sun-like star. The object 
features a classic bipolar expansion geometry, driven by stellar wind 
ejection from the hot central white dwarf remnant. The image shows a 
bright, double-lobed central core surrounded by faint, 
low-surface-brightness outer halos, illustrating the dynamic mass-loss 
history during the asymptotic giant branch (AGB) phase.]]></description><content:encoded><![CDATA[<figure class="
              sqs-block-image-figure
              intrinsic
            "
        >
          
        
        

        
          
            
          
            
                
                
                
                
                
                
                
                <img data-stretch="false" data-image="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/8f0b1fd9-c458-4734-a101-6e3104c23b0e/1000094948.jpg" data-image-dimensions="2472x2806" 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/8f0b1fd9-c458-4734-a101-6e3104c23b0e/1000094948.jpg?format=1000w" width="2472" height="2806" 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/8f0b1fd9-c458-4734-a101-6e3104c23b0e/1000094948.jpg?format=100w 100w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/8f0b1fd9-c458-4734-a101-6e3104c23b0e/1000094948.jpg?format=300w 300w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/8f0b1fd9-c458-4734-a101-6e3104c23b0e/1000094948.jpg?format=500w 500w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/8f0b1fd9-c458-4734-a101-6e3104c23b0e/1000094948.jpg?format=750w 750w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/8f0b1fd9-c458-4734-a101-6e3104c23b0e/1000094948.jpg?format=1000w 1000w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/8f0b1fd9-c458-4734-a101-6e3104c23b0e/1000094948.jpg?format=1500w 1500w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/8f0b1fd9-c458-4734-a101-6e3104c23b0e/1000094948.jpg?format=2500w 2500w" loading="lazy" decoding="async" data-loader="sqs">

            
          
        
          
        

        
      
        </figure>
      

    
  


  



  
  <p data-rte-preserve-empty="true">M27 is one of the most remarkable planetary nebulae in the night sky, representing the final evolutionary stage of a Sun-like star. In this image, the cyan emission is dominated by doubly ionized oxygen (OIII), while the red regions trace ionized hydrogen (Hα), revealing the complex structure and physical composition of the expanding nebula.</p><p data-rte-preserve-empty="true">The image was captured from Marzamemi, Sicily (Italy) under Bortle 5 skies using the following equipment:</p><p data-rte-preserve-empty="true">Telescope: Modified Levenhuk Newtonian 200/1000</p><p data-rte-preserve-empty="true">Mount: Sky-Watcher CQ350 Pro</p><p data-rte-preserve-empty="true">Camera: ZWO ASI2600MC Pro</p><p data-rte-preserve-empty="true">Filter: Optolong L-Para</p><p data-rte-preserve-empty="true">Controller: ASIAIR Plus</p><p data-rte-preserve-empty="true">Integration: 104 × 300 seconds (8 hours 40 minutes)</p><p data-rte-preserve-empty="true">This image is the result of many hours of acquisition, careful calibration, and processing, with the goal of preserving the nebula's natural emission colors while revealing its faint outer structures.</p>]]></content:encoded><media:content type="image/jpeg" url="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/8f0b1fd9-c458-4734-a101-6e3104c23b0e/1000094948.jpg?format=1500w" medium="image" isDefault="true" width="1500" height="1703"><media:title type="plain">Whispers of a Dying Star: Messier 27</media:title></media:content></item><item><title>SNR G013.3-01.3 and its long, tightly grouped, glowing filaments</title><category>2026</category><dc:creator>Charles Lillo</dc:creator><pubDate>Fri, 24 Jul 2026 04:00:55 +0000</pubDate><link>https://www.aapod2.com/blog/snr-g0133-013</link><guid isPermaLink="false">5debd4b16fcd7b02905712ff:5debd4f1c2fab6555bff00b5:6a6225db4f2f845d8fe51885</guid><description><![CDATA[Tangled in the crowded starfields near M24 in Sagittarius, SNR G013.3-01.3 
showcases delicate, tightly grouped ribbons of glowing interstellar gas. 
Swept up and heated by an expanding supernova shockwave, these faint 
filaments offer a vivid window into the dramatic lifecycle of massive 
stars.]]></description><content:encoded><![CDATA[<figure class="
              sqs-block-image-figure
              intrinsic
            "
        >
          
        
        

        
          
            
          
            
                
                
                
                
                
                
                
                <img data-stretch="false" data-image="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/7007e28b-fb84-4009-b2ba-882463c3ef67/SNRG0133013_JYB_2026_10.jpg" data-image-dimensions="4500x3000" 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/7007e28b-fb84-4009-b2ba-882463c3ef67/SNRG0133013_JYB_2026_10.jpg?format=1000w" width="4500" height="3000" 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/7007e28b-fb84-4009-b2ba-882463c3ef67/SNRG0133013_JYB_2026_10.jpg?format=100w 100w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/7007e28b-fb84-4009-b2ba-882463c3ef67/SNRG0133013_JYB_2026_10.jpg?format=300w 300w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/7007e28b-fb84-4009-b2ba-882463c3ef67/SNRG0133013_JYB_2026_10.jpg?format=500w 500w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/7007e28b-fb84-4009-b2ba-882463c3ef67/SNRG0133013_JYB_2026_10.jpg?format=750w 750w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/7007e28b-fb84-4009-b2ba-882463c3ef67/SNRG0133013_JYB_2026_10.jpg?format=1000w 1000w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/7007e28b-fb84-4009-b2ba-882463c3ef67/SNRG0133013_JYB_2026_10.jpg?format=1500w 1500w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/7007e28b-fb84-4009-b2ba-882463c3ef67/SNRG0133013_JYB_2026_10.jpg?format=2500w 2500w" loading="lazy" decoding="async" data-loader="sqs">

            
          
        
          
        

        
      
        </figure>]]></content:encoded><media:content type="image/jpeg" url="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/7007e28b-fb84-4009-b2ba-882463c3ef67/SNRG0133013_JYB_2026_10.jpg?format=1500w" medium="image" isDefault="true" width="1500" height="1000"><media:title type="plain">SNR G013.3-01.3 and its long, tightly grouped, glowing filaments</media:title></media:content></item><item><title>Ptolemy's Cluster (M7)</title><category>2026</category><dc:creator>Charles Lillo</dc:creator><pubDate>Thu, 23 Jul 2026 04:00:49 +0000</pubDate><link>https://www.aapod2.com/blog/ptolemys-cluster-m7</link><guid isPermaLink="false">5debd4b16fcd7b02905712ff:5debd4f1c2fab6555bff00b5:6a60cd5f2dba747a89def95c</guid><description><![CDATA[Ptolemy's Cluster (Messier 7 / NGC 6475) is a prominent open cluster 
situated approximately 980 light-years away in the constellation Scorpius, 
near the tail of the celestial scorpion. Spanning an estimated diameter of 
25 light-years (with an angular size of 80 arcminutes), this 
gravitationally bound stellar grouping contains around 80 to 100 member 
stars that co-formed approximately 220 million years ago from the same 
interstellar gas and dust cloud. Projected directly against the rich star 
fields and dark absorption lanes of the inner Milky Way, the cluster is 
dominated by luminous, main-sequence stars, primarily spectral class A0, 
along with evolving yellow giants, the most massive of which will 
eventually terminate as supernovae while weaker gravitational pull slowly 
allows the remaining population to disperse into the galactic field over 
time.]]></description><content:encoded><![CDATA[<figure class="
              sqs-block-image-figure
              intrinsic
            "
        >
          
        
        

        
          
            
          
            
                
                
                
                
                
                
                
                <img data-stretch="false" data-image="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/5850d9a5-d40d-431d-8a02-cd5b3cc3d7c0/M7-AAPOD2.jpg" data-image-dimensions="2120x3180" 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/5850d9a5-d40d-431d-8a02-cd5b3cc3d7c0/M7-AAPOD2.jpg?format=1000w" width="2120" height="3180" 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/5850d9a5-d40d-431d-8a02-cd5b3cc3d7c0/M7-AAPOD2.jpg?format=100w 100w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/5850d9a5-d40d-431d-8a02-cd5b3cc3d7c0/M7-AAPOD2.jpg?format=300w 300w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/5850d9a5-d40d-431d-8a02-cd5b3cc3d7c0/M7-AAPOD2.jpg?format=500w 500w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/5850d9a5-d40d-431d-8a02-cd5b3cc3d7c0/M7-AAPOD2.jpg?format=750w 750w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/5850d9a5-d40d-431d-8a02-cd5b3cc3d7c0/M7-AAPOD2.jpg?format=1000w 1000w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/5850d9a5-d40d-431d-8a02-cd5b3cc3d7c0/M7-AAPOD2.jpg?format=1500w 1500w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/5850d9a5-d40d-431d-8a02-cd5b3cc3d7c0/M7-AAPOD2.jpg?format=2500w 2500w" loading="lazy" decoding="async" data-loader="sqs">

            
          
        
          
        

        
      
        </figure>]]></content:encoded><media:content type="image/jpeg" url="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/5850d9a5-d40d-431d-8a02-cd5b3cc3d7c0/M7-AAPOD2.jpg?format=1500w" medium="image" isDefault="true" width="1500" height="2250"><media:title type="plain">Ptolemy's Cluster (M7)</media:title></media:content></item><item><title>Garden of Nebulae</title><category>2026</category><dc:creator>Charles Lillo</dc:creator><pubDate>Wed, 22 Jul 2026 04:00:48 +0000</pubDate><link>https://www.aapod2.com/blog/rho-ophiuchi-cloud-complex-setting-behind-a-snow-capped-peak</link><guid isPermaLink="false">5debd4b16fcd7b02905712ff:5debd4f1c2fab6555bff00b5:6a5f6e1ce852773253a1afbf</guid><description><![CDATA[The Rho Ophiuchi dark and emission nebulae complex, featuring at least 
seven distinct nebulae, sets gracefully behind the snow-capped peaks of 
Padum, Zanskar, India.

Captured using a Sony A7C II with a Samyang 135mm lens at f/1.8 mounted on 
a star tracker, a fast aperture proved essential for pulling out faint dust 
lanes and nebular glow, combining a tracked 200-frame sky stack with a 
sharp foreground exposure.]]></description><content:encoded><![CDATA[<figure class="
              sqs-block-image-figure
              intrinsic
            "
        >
          
        
        

        
          
            
          
            
                
                
                
                
                
                
                
                <img data-stretch="false" data-image="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/1d3c7079-1229-412c-b3e9-d40da4b99f50/Rho+Ophiuchi+wtih+Peak+ANushtup+Roy+Choudhury1.jpg" data-image-dimensions="5662x6468" 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/1d3c7079-1229-412c-b3e9-d40da4b99f50/Rho+Ophiuchi+wtih+Peak+ANushtup+Roy+Choudhury1.jpg?format=1000w" width="5662" height="6468" 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/1d3c7079-1229-412c-b3e9-d40da4b99f50/Rho+Ophiuchi+wtih+Peak+ANushtup+Roy+Choudhury1.jpg?format=100w 100w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/1d3c7079-1229-412c-b3e9-d40da4b99f50/Rho+Ophiuchi+wtih+Peak+ANushtup+Roy+Choudhury1.jpg?format=300w 300w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/1d3c7079-1229-412c-b3e9-d40da4b99f50/Rho+Ophiuchi+wtih+Peak+ANushtup+Roy+Choudhury1.jpg?format=500w 500w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/1d3c7079-1229-412c-b3e9-d40da4b99f50/Rho+Ophiuchi+wtih+Peak+ANushtup+Roy+Choudhury1.jpg?format=750w 750w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/1d3c7079-1229-412c-b3e9-d40da4b99f50/Rho+Ophiuchi+wtih+Peak+ANushtup+Roy+Choudhury1.jpg?format=1000w 1000w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/1d3c7079-1229-412c-b3e9-d40da4b99f50/Rho+Ophiuchi+wtih+Peak+ANushtup+Roy+Choudhury1.jpg?format=1500w 1500w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/1d3c7079-1229-412c-b3e9-d40da4b99f50/Rho+Ophiuchi+wtih+Peak+ANushtup+Roy+Choudhury1.jpg?format=2500w 2500w" loading="lazy" decoding="async" data-loader="sqs">

            
          
        
          
        

        
      
        </figure>
      

    
  


  



  
  <p data-rte-preserve-empty="true"><strong>Image Title:</strong> Garden of Nebulae</p><p data-rte-preserve-empty="true"><strong>Copyright:</strong> Anushtup Roy Choudhury</p><p data-rte-preserve-empty="true"><strong>Date image was taken:</strong> June 21, 2026</p><p data-rte-preserve-empty="true"><strong>Location:</strong> Padum, Zanskar, India</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> During a recent trip to Ladakh, I finally had the opportunity to test my Samyang 135mm lens on a deep-sky target. Although purchased specifically for astrophotography, it had previously only seen use as a wedding lens.<br>While in Padum, I planned a shot of the Rho Ophiuchi cloud complex setting behind a snow-capped peak. I quickly set up my star tracker and started the shooting. Compared to my previous attempt at f/5.6, shooting at f/1.8 highlighted just how critical a fast aperture is for pulling out faint details.<br>And more surprisingly, plate-solving and annotating the final image revealed at least seven distinct nebulae within this single field of view!<br>Exif :<br>Sky :<br>25 sec f/1.8 ISO 1600 135mm x 200<br>FG :<br>30 sec f/3.5 ISO 2000 135mm<br>Gear:<br>Sony A7C II | Samyang 135mm f/1.8 | Leofoto LS-285C<br>Software:<br>Adobe Lightroom | Siril | GraXpert | Starnet++ | Adobe Photoshop</p><p data-rte-preserve-empty="true"><strong>Name:</strong> Anushtup Roy Choudhury</p><p data-rte-preserve-empty="true"><strong>Website or Facebook Profile:</strong> <a target="_blank" href="http://www.lightnlens.co.in/anushtup-portfolio">http://www.lightnlens.co.in/anushtup-portfolio</a></p>]]></content:encoded><media:content type="image/jpeg" url="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/1d3c7079-1229-412c-b3e9-d40da4b99f50/Rho+Ophiuchi+wtih+Peak+ANushtup+Roy+Choudhury1.jpg?format=1500w" medium="image" isDefault="true" width="1500" height="1714"><media:title type="plain">Garden of Nebulae</media:title></media:content></item><item><title>C/2024 J3 Atlas &amp; NGC6819 in Cygnus</title><category>2026</category><dc:creator>Charles Lillo</dc:creator><pubDate>Tue, 21 Jul 2026 04:00:05 +0000</pubDate><link>https://www.aapod2.com/blog/c/2024-j3-atlas</link><guid isPermaLink="false">5debd4b16fcd7b02905712ff:5debd4f1c2fab6555bff00b5:6a5e22e7be0ab21c434cbd31</guid><description><![CDATA[Caught streaking across the northern sky, Comet C/2024 J3 (ATLAS) makes a 
fleeting appearance alongside the rich open star cluster NGC 6819 in the 
constellation Cygnus. Captured on July 10, 2026, from Gahberg, Austria, 
this deep-sky portrait showcases the icy visitor as it sweeps through our 
inner solar system. Traveling on a highly eccentric, hyperbolic orbit, this 
Oort cloud native has no return date; it is making a single, open-ended 
pass around the Sun before escaping into the permanent chill of 
interstellar space.]]></description><content:encoded><![CDATA[<figure class="
              sqs-block-image-figure
              intrinsic
            "
        >
          
        
        

        
          
            
          
            
                
                
                
                
                
                
                
                <img data-stretch="false" data-image="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/0b8b9e78-0fb5-4b81-bf64-a9bfb4325fab/20260710-2024-J3-Atlas-bei-NGC6819.jpg" data-image-dimensions="5000x3390" 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/0b8b9e78-0fb5-4b81-bf64-a9bfb4325fab/20260710-2024-J3-Atlas-bei-NGC6819.jpg?format=1000w" width="5000" height="3390" 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/0b8b9e78-0fb5-4b81-bf64-a9bfb4325fab/20260710-2024-J3-Atlas-bei-NGC6819.jpg?format=100w 100w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/0b8b9e78-0fb5-4b81-bf64-a9bfb4325fab/20260710-2024-J3-Atlas-bei-NGC6819.jpg?format=300w 300w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/0b8b9e78-0fb5-4b81-bf64-a9bfb4325fab/20260710-2024-J3-Atlas-bei-NGC6819.jpg?format=500w 500w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/0b8b9e78-0fb5-4b81-bf64-a9bfb4325fab/20260710-2024-J3-Atlas-bei-NGC6819.jpg?format=750w 750w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/0b8b9e78-0fb5-4b81-bf64-a9bfb4325fab/20260710-2024-J3-Atlas-bei-NGC6819.jpg?format=1000w 1000w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/0b8b9e78-0fb5-4b81-bf64-a9bfb4325fab/20260710-2024-J3-Atlas-bei-NGC6819.jpg?format=1500w 1500w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/0b8b9e78-0fb5-4b81-bf64-a9bfb4325fab/20260710-2024-J3-Atlas-bei-NGC6819.jpg?format=2500w 2500w" loading="lazy" decoding="async" data-loader="sqs">

            
          
        
          
        

        
      
        </figure>
      

    
  


  



  
  <p data-rte-preserve-empty="true"><strong>Image Title:</strong> C/2024 J3 Atlas &amp; NGC6819 in Cygnus</p><p data-rte-preserve-empty="true"><strong>Copyright:</strong> Günter Kerschhuber</p><p data-rte-preserve-empty="true"><strong>Date image was taken:</strong> July 10, 2026</p><p data-rte-preserve-empty="true"><strong>Location:</strong> Gahberg Austria</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> C 2024/J3 (Atlas) bei NGC6819 in Cygnus, Newton 8“ f3 DSPro2600C 35x5min, total 2,9h, ASA DDM85, Gahberg 20260710 UT23:39<br>Comet C/2024 J3 (ATLAS) has no known orbital period. Its orbit is hyperbolic and eccentric, which means that it moves in an open orbit around the Sun. It probably comes from the Oort cloud, comes once through our inner solar system and will then escape back into interstellar space</p><p data-rte-preserve-empty="true"><strong>Name:</strong> Günter Kerschhuber</p><p data-rte-preserve-empty="true"><strong>Website or Facebook Profile:</strong> <a target="_blank" href="http://www.astro-photo.at/">http://www.astro-photo.at</a></p>]]></content:encoded><media:content type="image/jpeg" url="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/0b8b9e78-0fb5-4b81-bf64-a9bfb4325fab/20260710-2024-J3-Atlas-bei-NGC6819.jpg?format=1500w" medium="image" isDefault="true" width="1500" height="1017"><media:title type="plain">C/2024 J3 Atlas &amp; NGC6819 in Cygnus</media:title></media:content></item><item><title>Squid Nebula</title><category>2026</category><dc:creator>Charles Lillo</dc:creator><pubDate>Mon, 20 Jul 2026 04:00:54 +0000</pubDate><link>https://www.aapod2.com/blog/squid-nebula-ou4</link><guid isPermaLink="false">5debd4b16fcd7b02905712ff:5debd4f1c2fab6555bff00b5:6a5cd0936597953356696754</guid><description><![CDATA[An elusive giant of the night sky, the mysterious Squid Nebula (Ou4) swims 
through a sea of ionized gas in the royal constellation Cepheus, appearing 
as an ethereal blue-green structure nestled within the deep reddish folds 
of the larger hydrogen emission region Sh2-129 (the Flying Bat Nebula). 
Discovered recently in 2011 by French amateur astronomer Nicolas Outters, 
this incredibly faint bipolar outflow stretches nearly 50 light-years 
across and shines with the unmistakable signature of emission from doubly 
ionized oxygen atoms ([O III]). Driven by a powerful triple system of hot, 
young, and massive stars cataloged as HR 8119 at its core, capturing this 
ghostly cosmic geometry required a true masterclass in patience from 
Zielona Góra, Poland. This spectacular deep-sky portrait represents an 
incredible 63 hours and 25 minutes of total integration time, with 47 hours 
and 45 minutes strictly to the ultra-faint [OIII] channel to pull the 
elusive Squid from the cosmic background.]]></description><content:encoded><![CDATA[<figure class="
              sqs-block-image-figure
              intrinsic
            "
        >
          
        
        

        
          
            
          
            
                
                
                
                
                
                
                
                <img data-stretch="false" data-image="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/dd7f4abc-809f-488c-894e-02b9b399e817/squidvox.jpg" data-image-dimensions="6014x4062" 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/dd7f4abc-809f-488c-894e-02b9b399e817/squidvox.jpg?format=1000w" width="6014" height="4062" 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/dd7f4abc-809f-488c-894e-02b9b399e817/squidvox.jpg?format=100w 100w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/dd7f4abc-809f-488c-894e-02b9b399e817/squidvox.jpg?format=300w 300w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/dd7f4abc-809f-488c-894e-02b9b399e817/squidvox.jpg?format=500w 500w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/dd7f4abc-809f-488c-894e-02b9b399e817/squidvox.jpg?format=750w 750w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/dd7f4abc-809f-488c-894e-02b9b399e817/squidvox.jpg?format=1000w 1000w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/dd7f4abc-809f-488c-894e-02b9b399e817/squidvox.jpg?format=1500w 1500w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/dd7f4abc-809f-488c-894e-02b9b399e817/squidvox.jpg?format=2500w 2500w" loading="lazy" decoding="async" data-loader="sqs">

            
          
        
          
        

        
      
        </figure>
      

    
  


  



  
  <p data-rte-preserve-empty="true"><strong>Image Title:</strong> Squid Nebula</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 05, 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> otal integration time of 63h 25' (Ha: 15h 40', OIII: 47h 45') across 17 days. Equipment used includes an Askar 65PHQ telescope, Player One Poseidon-M Pro camera, and a Pegasus Astro NYX-88 Harmonic Gear Mount. Captured using Antlia 3nm Narrowband 36 mm filters (H-alpha, Oxygen III, Sulfur II). Guided with an SVBony SV165 Mini 40mm f/4 and ToupTek G3M 290M camera.</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://app.astrobin.com/u/AlexFilothodoros">http://app.astrobin.com/u/AlexFilothodoros</a></p>]]></content:encoded><media:content type="image/jpeg" url="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/dd7f4abc-809f-488c-894e-02b9b399e817/squidvox.jpg?format=1500w" medium="image" isDefault="true" width="1500" height="1013"><media:title type="plain">Squid Nebula</media:title></media:content></item><item><title>IC 1396 - An Elephant´s Trunk</title><category>2026</category><dc:creator>Charles Lillo</dc:creator><pubDate>Sun, 19 Jul 2026 04:00:02 +0000</pubDate><link>https://www.aapod2.com/blog/ic-1396-an-elephants-trunk</link><guid isPermaLink="false">5debd4b16fcd7b02905712ff:5debd4f1c2fab6555bff00b5:6a5b78602020146782b6e8bd</guid><description><![CDATA[A stunning 2-panel mosaic of IC 1396, the iconic Elephant's Trunk Nebula 
in Cepheus. Captured by Oli B as a "first light" benchmark for a new 
equipment setup, this image beautifully highlights the intricate dance 
between vibrant, ionized gas and dense, dark interstellar dust lanes. The 
feature showcases the intense radiation from a massive central star 
compressing the surrounding molecular cloud, sculpting the distinctive, 
wind-sheared globules where a new generation of proto-stars is actively 
forming.]]></description><content:encoded><![CDATA[<figure class="
              sqs-block-image-figure
              intrinsic
            "
        >
          
        
        

        
          
            
          
            
                
                
                
                
                
                
                
                <img data-stretch="false" data-image="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/cc96fc26-e503-40f2-8d17-8534479c28d2/IC1396.jpg" data-image-dimensions="10051x7546" 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/cc96fc26-e503-40f2-8d17-8534479c28d2/IC1396.jpg?format=1000w" width="10051" height="7546" 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/cc96fc26-e503-40f2-8d17-8534479c28d2/IC1396.jpg?format=100w 100w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/cc96fc26-e503-40f2-8d17-8534479c28d2/IC1396.jpg?format=300w 300w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/cc96fc26-e503-40f2-8d17-8534479c28d2/IC1396.jpg?format=500w 500w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/cc96fc26-e503-40f2-8d17-8534479c28d2/IC1396.jpg?format=750w 750w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/cc96fc26-e503-40f2-8d17-8534479c28d2/IC1396.jpg?format=1000w 1000w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/cc96fc26-e503-40f2-8d17-8534479c28d2/IC1396.jpg?format=1500w 1500w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/cc96fc26-e503-40f2-8d17-8534479c28d2/IC1396.jpg?format=2500w 2500w" loading="lazy" decoding="async" data-loader="sqs">

            
          
        
          
        

        
      
        </figure>
      

    
  


  



  
  <p class=""><strong>Image Title:</strong> IC 1396 - An Elephant´s Trunk</p><p class=""><strong>Copyright:</strong> Oli B</p><p class=""><strong>Location:</strong> Imsbach, Germany<br>B4-5</p><p class=""><strong>Data Acquisition Method:</strong> Personal Telescope Setup</p><p class=""><strong>Description and Details:</strong> IC 1396, widely known as the Elephant's Trunk Nebula, is a classic emission nebula in Cepheus that remains a favorite for both beginners and experienced astrophotographers alike. Despite its popularity, its complex mix of bright, ionized gas and dense, dark interstellar dust lanes always makes it a pleasure to image. For me, this prominent star-forming region served as the perfect 'first light' benchmark to test the tracking precision, sampling, and overall performance of my new equipment setup under the night sky. To framing the region properly, the image was planned and executed as a 2-panel mosaic.<br><br>-Optics: Sky-Watcher Esprit 80ED<br>-Mount: Astrofrog FG17<br>-Camera: QHY 163M+FW<br>-Filters: Baader LRGB + Ha<br>-Software: Siril, Adobe Photoshop, RC-Astro Tools<br><br>Exposure details for each panel:<br>-Luminance: 40x 120sec<br>-RGB: 20x 120sec<br>-H-Alpha: 40x 300sec<br>Total Integration: 13h</p><p class=""><strong>Name:</strong> Oliver Betha</p>]]></content:encoded><media:content type="image/jpeg" url="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/cc96fc26-e503-40f2-8d17-8534479c28d2/IC1396.jpg?format=1500w" medium="image" isDefault="true" width="1500" height="1126"><media:title type="plain">IC 1396 - An Elephant´s Trunk</media:title></media:content></item><item><title>IC 4705 - distorted galaxy with 2 different neighbors</title><category>2026</category><dc:creator>Charles Lillo</dc:creator><pubDate>Sat, 18 Jul 2026 04:00:20 +0000</pubDate><link>https://www.aapod2.com/blog/ic-4704-and-the-fine-spiral-ic-4712</link><guid isPermaLink="false">5debd4b16fcd7b02905712ff:5debd4f1c2fab6555bff00b5:6a5a80668763d349524c3475</guid><description><![CDATA[Located in the southern constellation of Pavo, the peculiar barred spiral 
galaxy IC 4705 (type SB(s)a? pec) exhibits a heavily distorted structure. 
Discovered in 1900 by DeLisle Stewart, it features distinct tidal tails or 
"streamers" stretching from its core, vivid indicators of past 
gravitational interactions with its diverse neighbors, the elliptical IC 
4704 and the fine spiral IC 4712.]]></description><content:encoded><![CDATA[<figure class="
              sqs-block-image-figure
              intrinsic
            "
        >
          
        
        

        
          
            
          
            
                
                
                
                
                
                
                
                <img data-stretch="false" data-image="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/1b1e4403-3ed7-46e6-9534-bdb55b8409a1/ic4705_gemsbock_cdk_2048px.jpg" data-image-dimensions="2048x1366" 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/1b1e4403-3ed7-46e6-9534-bdb55b8409a1/ic4705_gemsbock_cdk_2048px.jpg?format=1000w" width="2048" height="1366" 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/1b1e4403-3ed7-46e6-9534-bdb55b8409a1/ic4705_gemsbock_cdk_2048px.jpg?format=100w 100w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/1b1e4403-3ed7-46e6-9534-bdb55b8409a1/ic4705_gemsbock_cdk_2048px.jpg?format=300w 300w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/1b1e4403-3ed7-46e6-9534-bdb55b8409a1/ic4705_gemsbock_cdk_2048px.jpg?format=500w 500w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/1b1e4403-3ed7-46e6-9534-bdb55b8409a1/ic4705_gemsbock_cdk_2048px.jpg?format=750w 750w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/1b1e4403-3ed7-46e6-9534-bdb55b8409a1/ic4705_gemsbock_cdk_2048px.jpg?format=1000w 1000w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/1b1e4403-3ed7-46e6-9534-bdb55b8409a1/ic4705_gemsbock_cdk_2048px.jpg?format=1500w 1500w, https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/1b1e4403-3ed7-46e6-9534-bdb55b8409a1/ic4705_gemsbock_cdk_2048px.jpg?format=2500w 2500w" loading="lazy" decoding="async" data-loader="sqs">

            
          
        
          
        

        
      
        </figure>
      

    
  


  



  
  <p data-rte-preserve-empty="true"><strong>Image Title:</strong> IC 4705 - distorted galaxy with 2 different neighbors</p><p data-rte-preserve-empty="true"><strong>Copyright:</strong> Franz Hofmann</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=1h-onHXenf_hpkK00pgqy8NYfzlURLqkO">https://drive.google.com/open?id=1h-onHXenf_hpkK00pgqy8NYfzlURLqkO</a></p><p data-rte-preserve-empty="true"><strong>Date image was taken:</strong> August 25, 2025</p><p data-rte-preserve-empty="true"><strong>Location:</strong> Gemsbock Observatory, Rooisand Desert Ranch, Namibia</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 cosmic meeting of three very different galaxies. In the center the distorted IC 4705 which is framed by the elliptic IC 4704 and the fine spiral IC 4712.<br><br>Planewave CDK14 on 10 Micron 2000HPS<br>QHY 268M with Baader filters<br>L:R:G:B 60:33:31:30 x 600s</p><p data-rte-preserve-empty="true"><strong>Name:</strong> Franz Hofmann</p><p data-rte-preserve-empty="true"><strong>Email:</strong> <a target="_blank" href="mailto:hofmannfranz@gmx.de">hofmannfranz@gmx.de</a></p><p data-rte-preserve-empty="true"><strong>Website or Facebook Profile:</strong> <a target="_blank" href="https://astroimages.bine-und-franz.de/en/bilder/galaxien/ic-4705-gemsbock-observatory/">https://astroimages.bine-und-franz.de/en/bilder/galaxien/ic-4705-gemsbock-observatory/</a></p>]]></content:encoded><media:content type="image/jpeg" url="https://images.squarespace-cdn.com/content/v1/5debd4b16fcd7b02905712ff/1b1e4403-3ed7-46e6-9534-bdb55b8409a1/ic4705_gemsbock_cdk_2048px.jpg?format=1500w" medium="image" isDefault="true" width="1500" height="1000"><media:title type="plain">IC 4705 - distorted galaxy with 2 different neighbors</media:title></media:content></item></channel></rss>