<?xml version="1.0" encoding="utf-8" standalone="yes"?><rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>Emission Nebula on AstroT3k</title><link>https://astro.t3k.pl/en/tags/emission-nebula/</link><description>Recent content in Emission Nebula on AstroT3k</description><generator>Hugo -- gohugo.io</generator><language>en</language><lastBuildDate>Tue, 20 Jan 2026 21:00:00 +0100</lastBuildDate><atom:link href="https://astro.t3k.pl/en/tags/emission-nebula/index.xml" rel="self" type="application/rss+xml"/><item><title>IC 434 — Horsehead Nebula</title><link>https://astro.t3k.pl/en/post/2026/01/ic434_horsehead_nebula/</link><pubDate>Tue, 20 Jan 2026 21:00:00 +0100</pubDate><guid>https://astro.t3k.pl/en/post/2026/01/ic434_horsehead_nebula/</guid><description>&lt;img src="https://astro.t3k.pl/" alt="Featured image of post IC 434 — Horsehead Nebula" /&gt;&lt;p&gt;&lt;img class="gallery-image" data-flex-basis="358px" data-flex-grow="149" data-title-escaped="IC 434 — Horsehead Nebula" height="2003" loading="lazy" sizes="(max-width: 767px) calc(100vw - 30px), (max-width: 1023px) 700px, (max-width: 1279px) 950px, 1232px" src="https://astro.t3k.pl/post/2026/01/ic434_horsehead_nebula/images/ic434.png" srcset="https://astro.t3k.pl/post/2026/01/ic434_horsehead_nebula/images/ic434_hu_ce0ec6688e83e130.png 800w, https://astro.t3k.pl/post/2026/01/ic434_horsehead_nebula/images/ic434_hu_313b87d549a416ca.png 1600w, https://astro.t3k.pl/post/2026/01/ic434_horsehead_nebula/images/ic434_hu_32a0cdd3a4560232.png 2400w, https://astro.t3k.pl/post/2026/01/ic434_horsehead_nebula/images/ic434.png 2996w" title="IC 434 — Horsehead Nebula" width="2996"&gt;&lt;/p&gt;
&lt;p&gt;IC 434 is a bright curtain of hydrogen‑alpha emission in Orion, ionised mainly by the hot O‑type stars of the Sigma Orionis system. In front of this pinkish glow sits the famous Horsehead Nebula (Barnard 33), a compact pillar of dark dust sculpted by stellar winds and intense ultraviolet radiation. The complex lies about 1,350–1,500 light‑years away on the eastern edge of Orion’s Belt, close to the brilliant star Alnitak (Zeta Orionis).&lt;/p&gt;
&lt;p&gt;Visually, this area is challenging. The Horsehead itself is notoriously elusive in small telescopes because of its low contrast; under very dark skies and with a narrowband H‑alpha or UHC filter it can sometimes be hinted at in medium apertures. The wider IC 434 glow and the neighbouring Flame Nebula respond well to filters and long‑exposure imaging.&lt;/p&gt;
&lt;p&gt;The field is particularly rich in contrasting nebular types. Immediately east of Alnitak lies the Flame Nebula (NGC 2024), a bright emission and dark‑lane complex. Just south of the Horsehead is the bluish reflection nebula NGC 2023, while faint filaments of IC 434 extend across much of the frame. Bright field stars form striking halos and diffraction around the belt region, adding to the scene.&lt;/p&gt;
&lt;h4 id="what-else-is-in-this-image"&gt;What else is in this image?
&lt;/h4&gt;&lt;p&gt;&lt;img class="gallery-image" data-flex-basis="358px" data-flex-grow="149" data-title-escaped="IC 434 — annotated" height="1164" loading="lazy" sizes="(max-width: 767px) calc(100vw - 30px), (max-width: 1023px) 700px, (max-width: 1279px) 950px, 1232px" src="https://astro.t3k.pl/post/2026/01/ic434_horsehead_nebula/images/ic434_annotated.png" srcset="https://astro.t3k.pl/post/2026/01/ic434_horsehead_nebula/images/ic434_annotated_hu_849dbc98bdd7c4b3.png 800w, https://astro.t3k.pl/post/2026/01/ic434_horsehead_nebula/images/ic434_annotated_hu_2274fd1e250c2c5f.png 1600w, https://astro.t3k.pl/post/2026/01/ic434_horsehead_nebula/images/ic434_annotated.png 1741w" title="IC 434 — annotated" width="1741"&gt;&lt;/p&gt;
&lt;p&gt;In the image you can also see IC 434 as the background emission sheet, the Horsehead (B33) as a small, notched silhouette, NGC 2023 as a reflection patch below, and the Flame Nebula (NGC 2024) near Alnitak at the left edge. Several catalogued dark lanes thread the field along the Orion B molecular cloud.&lt;/p&gt;
&lt;p&gt;View this image on AstroBin: &lt;a class="link" href="https://app.astrobin.com/u/grodzik?i=iznra1#gallery" target="_blank" rel="noopener"
 &gt;https://app.astrobin.com/u/grodzik?i=iznra1#gallery&lt;/a&gt;&lt;/p&gt;
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 &lt;td&gt;Telescope&lt;/td&gt;
 &lt;td&gt;SkyWatcher 150/750P&lt;/td&gt;
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 &lt;td&gt;Mount&lt;/td&gt;
 &lt;td&gt;ZWO AM3N&lt;/td&gt;
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 &lt;td&gt;Camera&lt;/td&gt;
 &lt;td&gt;ZWO ASI2600MC Pro&lt;/td&gt;
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 &lt;td&gt;Filters&lt;/td&gt;
 &lt;td&gt;Astronomik UHC 2&amp;quot;&lt;/td&gt;
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 &lt;td&gt;Exposure&lt;/td&gt;
 &lt;td&gt;94 × 120s (3h 8min)&lt;/td&gt;
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 &lt;td&gt;Bortle&lt;/td&gt;
 &lt;td&gt;5&lt;/td&gt;
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 &lt;td&gt;Moon&lt;/td&gt;
 &lt;td&gt;Waxing crescent (3.1%)&lt;/td&gt;
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 &lt;td&gt;Processing&lt;/td&gt;
 &lt;td&gt;Siril, Prism Deep, Axiom2, CosmicClarity&lt;/td&gt;
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&lt;/table&gt;</description></item><item><title>IC 1848 — Soul Nebula</title><link>https://astro.t3k.pl/en/post/2025/10/ic1848_soul_nebula/</link><pubDate>Fri, 03 Oct 2025 21:00:00 +0200</pubDate><guid>https://astro.t3k.pl/en/post/2025/10/ic1848_soul_nebula/</guid><description>&lt;img src="https://astro.t3k.pl/" alt="Featured image of post IC 1848 — Soul Nebula" /&gt;&lt;p&gt;&lt;img class="gallery-image" data-flex-basis="360px" data-flex-grow="150" data-title-escaped="IC 1848 — Soul Nebula" height="1523" loading="lazy" sizes="(max-width: 767px) calc(100vw - 30px), (max-width: 1023px) 700px, (max-width: 1279px) 950px, 1232px" src="https://astro.t3k.pl/post/2025/10/ic1848_soul_nebula/images/ic1848_s.png" srcset="https://astro.t3k.pl/post/2025/10/ic1848_soul_nebula/images/ic1848_s_hu_e6e41e394d04597c.png 800w, https://astro.t3k.pl/post/2025/10/ic1848_soul_nebula/images/ic1848_s_hu_abe3cc06c16c35ae.png 1600w, https://astro.t3k.pl/post/2025/10/ic1848_soul_nebula/images/ic1848_s.png 2287w" title="IC 1848 — Soul Nebula" width="2287"&gt;&lt;/p&gt;
&lt;p&gt;IC 1848, better known as the Soul Nebula, is a vast H II star‑forming complex in Cassiopeia and the eastern half of the famous Heart and Soul pair. It glows strongly in hydrogen‑alpha, threaded with dark dust lanes and sculpted pillars shaped by the radiation and winds of massive young stars. Embedded open clusters light up the nebulosity; the Index Catalogue designation IC 1848 historically refers to the stellar association within this region.&lt;/p&gt;
&lt;p&gt;From mid‑northern latitudes the Soul rises high in the autumn and winter sky, making October evenings a convenient time to image it. Visually it is a challenging, low‑contrast target requiring dark skies; narrowband or broadband UHC filters help bring out the emission. The field here fits well within an APS‑C sensor at 750 mm focal length, framing the brighter central structures along with surrounding filaments.&lt;/p&gt;
&lt;p&gt;&lt;img class="gallery-image" data-flex-basis="357px" data-flex-grow="148" data-title-escaped="IC 1848 — Soul Nebula (annotated)" height="1605" loading="lazy" sizes="(max-width: 767px) calc(100vw - 30px), (max-width: 1023px) 700px, (max-width: 1279px) 950px, 1232px" src="https://astro.t3k.pl/post/2025/10/ic1848_soul_nebula/images/annotated_ic1848.png" srcset="https://astro.t3k.pl/post/2025/10/ic1848_soul_nebula/images/annotated_ic1848_hu_afd0ce8ea1a57095.png 800w, https://astro.t3k.pl/post/2025/10/ic1848_soul_nebula/images/annotated_ic1848_hu_2be6c8a5ea4ffa4b.png 1600w, https://astro.t3k.pl/post/2025/10/ic1848_soul_nebula/images/annotated_ic1848.png 2391w" title="IC 1848 — Soul Nebula (annotated)" width="2391"&gt;&lt;/p&gt;
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 &lt;td&gt;Telescope&lt;/td&gt;
 &lt;td&gt;SkyWatcher 150/750P&lt;/td&gt;
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 &lt;td&gt;Mount&lt;/td&gt;
 &lt;td&gt;motorised EQ3-2&lt;/td&gt;
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 &lt;td&gt;Camera&lt;/td&gt;
 &lt;td&gt;Canon 600D (astro‑mod)&lt;/td&gt;
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 &lt;td&gt;Filters&lt;/td&gt;
 &lt;td&gt;Astronomik UHC 2&amp;quot;&lt;/td&gt;
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 &lt;td&gt;Exposure&lt;/td&gt;
 &lt;td&gt;59 × 120s (1h 58min)&lt;/td&gt;
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 &lt;td&gt;Bortle&lt;/td&gt;
 &lt;td&gt;5&lt;/td&gt;
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 &lt;td&gt;Moon&lt;/td&gt;
 &lt;td&gt;Waxing gibbous (84.4%)&lt;/td&gt;
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 &lt;td&gt;Processing&lt;/td&gt;
 &lt;td&gt;Siril, Prism Deep, CosmicClarity, Gimp&lt;/td&gt;
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