<?xml version="1.0" encoding="utf-8"?>
<?xml-stylesheet type="text/xsl" href="/assets/xml/rss.xsl" media="all"?><rss version="2.0" xmlns:dc="http://purl.org/dc/elements/1.1/" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>SpacePhoto.de (Posts about FN250)</title><link>https://spacephoto.de/</link><description></description><atom:link href="https://spacephoto.de/categories/fn250.xml" rel="self" type="application/rss+xml"></atom:link><language>en</language><copyright>Contents © 2026 &lt;a href="mailto:operator@spacephoto.de"&gt;Martin Timpe&lt;/a&gt; </copyright><lastBuildDate>Fri, 05 Jun 2026 14:30:14 GMT</lastBuildDate><generator>Nikola (getnikola.com)</generator><docs>http://blogs.law.harvard.edu/tech/rss</docs><item><title>Messier 101 – The Pinwheel Galaxy in Ursa Major</title><link>https://spacephoto.de/blog/M101/</link><dc:creator>Martin Timpe</dc:creator><description>&lt;div&gt;&lt;p&gt;Messier 101 (NGC 5457), better known as the Pinwheel Galaxy, is a face-on grand-design spiral galaxy
in the constellation Ursa Major. It lies at a distance of approximately 21 million light years (≈ 6.4 Mpc)
and shines at an apparent magnitude of about 7.9, which puts it within easy reach of a small telescope -
provided the sky is dark enough, as its light is spread over an apparent diameter of nearly 29 arc minutes,
close to the full Moon's. The galaxy was discovered by Pierre Méchain on 27 March 1781 and reported to Charles Messier,
who immediately included it among the very last entries of his famous catalogue
(&lt;a class="reference external" href="https://en.wikipedia.org/wiki/Pinwheel_Galaxy"&gt;Wikipedia: Pinwheel Galaxy&lt;/a&gt;).&lt;/p&gt;
&lt;div class="docutils container"&gt;
&lt;figure class="align-center" style="width: 80%"&gt;
&lt;a class="reference external image-reference" href="https://spacephoto.de/galleries/01_galaxies/201_M101_LRGB_22h20m_RC3_DT.jpg"&gt;
&lt;img alt="&amp;lt;/galleries/01_galaxies/201_M101_LRGB_22h20m_RC3_DT.jpg&amp;gt;" src="https://spacephoto.de/galleries/01_galaxies/201_M101_LRGB_22h20m_RC3_DT.jpg"&gt;
&lt;/a&gt;
&lt;figcaption&gt;
&lt;p&gt;The Pinwheel Galaxy M101 (NGC 5457) in Constellation Ursa Major, Telescope Newton f=1000mm f/4, Camera Atik 460Exm with Baader LRGB and Hα filters, Total Exposure Time 22h20min&lt;/p&gt;
&lt;/figcaption&gt;
&lt;/figure&gt;
&lt;/div&gt;
&lt;p&gt;&lt;a href="https://spacephoto.de/blog/M101/"&gt;Read more…&lt;/a&gt; (3 min remaining to read)&lt;/p&gt;&lt;/div&gt;</description><category>Atik460Exm</category><category>FN250</category><category>galaxy</category><category>M101</category><category>M101 Group</category><category>NGC 5457</category><category>Pinwheel Galaxy</category><category>SN 2011fe</category><category>Ursa Major</category><guid>https://spacephoto.de/blog/M101/</guid><pubDate>Fri, 24 Apr 2026 23:00:00 GMT</pubDate></item><item><title>The Merope Nebula in the Pleiades</title><link>https://spacephoto.de/blog/NGC%201435/</link><dc:creator>Martin Timpe</dc:creator><description>&lt;div&gt;&lt;p&gt;NGC 1435, commonly called the Merope Nebula, is a galactic nebula nestled within the Pleiades region in Taurus.
German astronomer Wilhelm Tempel discovered this elusive object on October 19, 1859.&lt;/p&gt;
&lt;div class="docutils container"&gt;
&lt;figure class="align-center" style="width: 80%"&gt;
&lt;a class="reference external image-reference" href="https://spacephoto.de/galleries/03_starsclusters/NGC_1435_RGB_9x300s_DT.jpg"&gt;
&lt;img alt="&amp;lt;/galleries/03_starsclusters/NGC_1435_RGB_9x300s_DT.jpg&amp;gt;" src="https://spacephoto.de/galleries/03_starsclusters/NGC_1435_RGB_9x300s_DT.jpg"&gt;
&lt;/a&gt;
&lt;figcaption&gt;
&lt;p&gt;NGC 1435, the Merope Nebula in the Pleiades, image data: f=1000mm, f/4, 9x300s RGB, Atik460Exm&lt;/p&gt;
&lt;/figcaption&gt;
&lt;/figure&gt;
&lt;/div&gt;
&lt;p&gt;&lt;a href="https://spacephoto.de/blog/NGC%201435/"&gt;Read more…&lt;/a&gt; (3 min remaining to read)&lt;/p&gt;&lt;/div&gt;</description><category>Atik460Exm</category><category>FN250</category><category>IC 349</category><category>NGC 1435</category><category>open cluster</category><category>Pleiades</category><guid>https://spacephoto.de/blog/NGC%201435/</guid><pubDate>Tue, 30 Dec 2025 20:00:00 GMT</pubDate></item><item><title>Globular Cluster Messier 3 in Constellation Canis Venatici</title><link>https://spacephoto.de/blog/M%203/</link><dc:creator>Martin Timpe</dc:creator><description>&lt;div&gt;&lt;p&gt;Messier 3 (NGC 5272) stands as one of the finest globular clusters accessible to northern hemisphere imagers, offering both
visual splendor and technical challenge.
This densely packed stellar sphere in Canes Venatici contains approximately 500,000 stars
compressed into a volume roughly 180 light-years across.&lt;/p&gt;
&lt;div class="docutils container"&gt;
&lt;figure class="align-center" style="width: 80%"&gt;
&lt;a class="reference external image-reference" href="https://spacephoto.de/galleries/03_starsclusters/0140_M3_RGB_21_21_20x300s_f1000mm.jpg"&gt;
&lt;img alt="&amp;lt;/galleries/03_starsclusters/0140_M3_RGB_21_21_20x300s_f1000mm.jpg&amp;gt;" src="https://spacephoto.de/galleries/03_starsclusters/0140_M3_RGB_21_21_20x300s_f1000mm.jpg"&gt;
&lt;/a&gt;
&lt;figcaption&gt;
&lt;p&gt;Globular Cluster Messier 3: Newton 10" f/4, Atik 460EXM, Exposure Sum 5h10min, 9/2023-12/2025, Fuerfeld, Deutschland&lt;/p&gt;
&lt;/figcaption&gt;
&lt;/figure&gt;
&lt;/div&gt;
&lt;p&gt;&lt;a href="https://spacephoto.de/blog/M%203/"&gt;Read more…&lt;/a&gt; (2 min remaining to read)&lt;/p&gt;&lt;/div&gt;</description><category>Atik460Exm</category><category>Canis Venatici</category><category>FN250</category><category>globular cluster</category><category>Messier</category><category>Messier 3</category><category>NGC 5272</category><guid>https://spacephoto.de/blog/M%203/</guid><pubDate>Tue, 30 Dec 2025 19:00:00 GMT</pubDate></item><item><title>NGC 2264 – The Christmas Tree Cluster &amp; Cone Nebula</title><link>https://spacephoto.de/blog/NGC%202264/</link><dc:creator>Martin Timpe</dc:creator><description>&lt;div&gt;&lt;p&gt;NGC 2264 is one of the most rewarding winter targets for astrophotographers in the northern hemisphere.
The designation actually covers a complex of objects: the iconic &lt;strong&gt;Christmas Tree Cluster&lt;/strong&gt;,
the &lt;strong&gt;Cone Nebula&lt;/strong&gt;, the &lt;strong&gt;Fox Fur Nebula&lt;/strong&gt;,
and the &lt;strong&gt;Snowflake Cluster&lt;/strong&gt; – all embedded in a rich emission nebula in the constellation Monoceros.
The exposures were done in two nights on 28/29th and 30/31st December 2025. The image is a composit
of exposures taken trough H-apha and RGB filters.&lt;/p&gt;
&lt;div class="docutils container"&gt;
&lt;figure class="align-center" style="width: 80%"&gt;
&lt;a class="reference external image-reference" href="https://spacephoto.de/galleries/02_nebulas/190_NGC_2264_f1000mm_Ha_15x600s_3x300s_RGB_27_18_27x300s_DT.jpg"&gt;
&lt;img alt="&amp;lt;/galleries/02_nebulas/190_NGC_2264_f1000mm_Ha_15x600s_3x300s_RGB_27_18_27x300s_DT.jpg&amp;gt;" src="https://spacephoto.de/galleries/02_nebulas/190_NGC_2264_f1000mm_Ha_15x600s_3x300s_RGB_27_18_27x300s_DT.jpg"&gt;
&lt;/a&gt;
&lt;figcaption&gt;
&lt;p&gt;NGC 2264, Christmas Tree Cluster, image data: f=1000mm, f/4 Ha: 15x600s RGB: 27, 18, 27x300s Atik 460Exm&lt;/p&gt;
&lt;/figcaption&gt;
&lt;/figure&gt;
&lt;/div&gt;
&lt;p&gt;&lt;a href="https://spacephoto.de/blog/NGC%202264/"&gt;Read more…&lt;/a&gt; (2 min remaining to read)&lt;/p&gt;&lt;/div&gt;</description><category>Atik460Exm</category><category>FN250</category><category>Monoceros</category><category>nebula</category><category>NGC 2264</category><category>open cluster</category><guid>https://spacephoto.de/blog/NGC%202264/</guid><pubDate>Mon, 29 Dec 2025 23:00:00 GMT</pubDate></item><item><title>The Galaxy Cluster Abell 2151 in Constellation Hercules</title><link>https://spacephoto.de/blog/Abell%202151/</link><dc:creator>Martin Timpe</dc:creator><description>&lt;div&gt;&lt;p&gt;The galaxy cluster Abell 2151 in the constellation Hercules, therefore also known as the Hercules cluster,
has an extension of approx. 1° and is located at a distance of approx. 500 light years.
Unlike other clusters, it has no central galaxy, and contains several interacting galaxy systems.
It was first described by Harlow Shapley in 1933.&lt;/p&gt;
&lt;div class="docutils container"&gt;
&lt;figure class="align-center" style="width: 80%"&gt;
&lt;a class="reference external image-reference" href="https://spacephoto.de/galleries/01_galaxies/190_Hercules_Cluster_140L_15_14_29RGBx300s.jpg"&gt;
&lt;img alt="&amp;lt;/galleries/01_galaxies/190_Hercules_Cluster_140L_15_14_29RGBx300s.jpg&amp;gt;" src="https://spacephoto.de/galleries/01_galaxies/190_Hercules_Cluster_140L_15_14_29RGBx300s.jpg"&gt;
&lt;/a&gt;
&lt;figcaption&gt;
&lt;p&gt;The Galaxy Cluster Abell 2151 in Constellation Hercules,  Telescope Newton f=1000mm f/4,  Camera Atik 460Exm, Total Exposure Time 13h30min&lt;/p&gt;
&lt;/figcaption&gt;
&lt;/figure&gt;
&lt;/div&gt;
&lt;p&gt;&lt;a href="https://spacephoto.de/blog/Abell%202151/"&gt;Read more…&lt;/a&gt; (2 min remaining to read)&lt;/p&gt;&lt;/div&gt;</description><category>Abell 2151</category><category>Atik460Exm</category><category>FN250</category><category>galaxy</category><category>galaxy cluster</category><category>IC 1182</category><category>NGC 6040</category><category>NGC 6045</category><guid>https://spacephoto.de/blog/Abell%202151/</guid><pubDate>Sun, 12 May 2024 21:00:00 GMT</pubDate></item><item><title>NGC 225 - Open Cluster in Constellation Cassiopeia</title><link>https://spacephoto.de/blog/NGC%20225%2C%20LDN%201291%2C%20LBN%20604/</link><dc:creator>Martin Timpe</dc:creator><description>&lt;div&gt;&lt;p&gt;NGC 225 is an open cluster in the constellation Cassiopeia. It is located roughly 2,200 light-years from Earth. It is about 100 to 150 million years old.
The binary fraction, or the fraction of stars that are multiple stars, is 0.52.
It is also known as sailboat cluster. But what's happening at the top of the mast? The boat is obviously being boarded by an octopus - the more
clearer, the longer you expose (or if you drink too much red wine)...
Beside the quite nice, probably not so well known star cluster you can see interesting dust clouds and a
reflection nebula, which are cataloged as LDN 1291 and LBN 604.&lt;/p&gt;
&lt;div class="docutils container"&gt;
&lt;figure class="align-center" style="width: 80%"&gt;
&lt;a class="reference external image-reference" href="https://spacephoto.de/galleries/03_starsclusters/0005_NGC225_61L_18R_26G_28Bx300s_DT2.jpg"&gt;
&lt;img alt="&amp;lt;/galleries/03_starsclusters/0005_NGC225_61L_18R_26G_28Bx300s_DT2.jpg&amp;gt;" src="https://spacephoto.de/galleries/03_starsclusters/0005_NGC225_61L_18R_26G_28Bx300s_DT2.jpg"&gt;
&lt;/a&gt;
&lt;figcaption&gt;
&lt;p&gt;NGC 225, the sailboat cluster in Constellation Cassiopeia, Telescope Newton 10" f/4,  Camera Atik 460EXM, Total Exposure Time 11h05min&lt;/p&gt;
&lt;/figcaption&gt;
&lt;/figure&gt;
&lt;/div&gt;
&lt;p&gt;&lt;a href="https://spacephoto.de/blog/NGC%20225%2C%20LDN%201291%2C%20LBN%20604/"&gt;Read more…&lt;/a&gt; (1 min remaining to read)&lt;/p&gt;&lt;/div&gt;</description><category>Atik460Exm</category><category>cluster</category><category>FN250</category><category>LBN 604</category><category>LDN 1291</category><category>NGC 225</category><category>reflection nebula</category><guid>https://spacephoto.de/blog/NGC%20225%2C%20LDN%201291%2C%20LBN%20604/</guid><pubDate>Thu, 14 Sep 2023 21:00:00 GMT</pubDate></item><item><title>The Iris Nebula NGC 7023</title><link>https://spacephoto.de/blog/NGC%207023/</link><dc:creator>Martin Timpe</dc:creator><description>&lt;div&gt;&lt;p&gt;The Iris nebula is a bright reflecion nebula in the constellation Cepheus.
It's appearance is caused by the very hot star HD 200775 in it's centre
whose light is partly reflected and partly absorbed by surrounding dust clouds.
As can be seen from the labeled image, the dust cloud itself can be found in
Lynd's cataologue of dark nebulae as entry LDN 1174.
The reflection nebula shines at magnitude +6.8.
It lies 1,300 light-years away and is six light-years across&lt;/p&gt;
&lt;div class="docutils container"&gt;
&lt;figure class="align-center" style="width: 80%"&gt;
&lt;a class="reference external image-reference" href="https://spacephoto.de/galleries/02_nebulas/150_NGC_7023_LRGB_71_25_30_25_300s_DT.jpg"&gt;
&lt;img alt="&amp;lt;/galleries/02_nebulas/150_NGC_7023_LRGB_71_25_30_25_300s_DT.jpg&amp;gt;" src="https://spacephoto.de/galleries/02_nebulas/150_NGC_7023_LRGB_71_25_30_25_300s_DT.jpg"&gt;
&lt;/a&gt;
&lt;figcaption&gt;
&lt;p&gt;NGC 7023 in Constellation Cepheus, Telescope Newton 10" f/4,  Camera Atik 460EXM, Total Exposure Time 12h35min&lt;/p&gt;
&lt;/figcaption&gt;
&lt;/figure&gt;
&lt;/div&gt;
&lt;p&gt;&lt;a href="https://spacephoto.de/blog/NGC%207023/"&gt;Read more…&lt;/a&gt; (1 min remaining to read)&lt;/p&gt;&lt;/div&gt;</description><category>Atik460Exm</category><category>FN250</category><category>nebula</category><category>NGC7023</category><category>reflection nebula</category><guid>https://spacephoto.de/blog/NGC%207023/</guid><pubDate>Fri, 08 Sep 2023 20:00:00 GMT</pubDate></item><item><title>M 106 - Galaxy in Constellation Canes Venatici</title><link>https://spacephoto.de/blog/M%20106/</link><dc:creator>Martin Timpe</dc:creator><description>&lt;div&gt;&lt;p&gt;The galaxy Messier 106 (M 106) in the constellation Canes Venatici is one of our closer neighbour galaxies in roughly 23 million light years
distance from the Milkyway and the Earth.
The galaxy hosts an active nucleus with a black hole of approximately 40 million solar masses. The
galaxy core is known as a radio source since the 1950s. Further the galaxy undergoes a period of
increased star-formation (starburst galaxy).&lt;/p&gt;
&lt;div class="docutils container"&gt;
&lt;figure class="align-center" style="width: 80%"&gt;
&lt;a class="reference external image-reference" href="https://spacephoto.de/galleries/01_galaxies/170_M106_LRGB4_L159xR21xG18xB16x300s_Crop01_DT.jpg"&gt;
&lt;img alt="&amp;lt;//galleries/01_galaxies/170_M106_LRGB4_L159xR21xG18xB16x300s_Crop01_DT.jpg&amp;gt;" src="https://spacephoto.de/galleries/01_galaxies/170_M106_LRGB4_L159xR21xG18xB16x300s_Crop01_DT.jpg"&gt;
&lt;/a&gt;
&lt;figcaption&gt;
&lt;p&gt;Crop of M 106 in Constellation Canes Venatici, Telescope Newton 10" f/4,  Camera Atik 460EXM, Total Exposure Time 17h50min&lt;/p&gt;
&lt;/figcaption&gt;
&lt;/figure&gt;
&lt;/div&gt;
&lt;p&gt;&lt;a href="https://spacephoto.de/blog/M%20106/"&gt;Read more…&lt;/a&gt; (2 min remaining to read)&lt;/p&gt;&lt;/div&gt;</description><category>Atik460Exm</category><category>FN250</category><category>galaxy</category><category>M106</category><guid>https://spacephoto.de/blog/M%20106/</guid><pubDate>Sun, 23 Apr 2023 21:00:00 GMT</pubDate></item><item><title>NGC 1977 - The Running Man Nebula</title><link>https://spacephoto.de/blog/NGC%201977/</link><dc:creator>Martin Timpe</dc:creator><description>&lt;div&gt;&lt;p&gt;The reflection nebula NGC 1977 in the constellation Orion a slightly north of the Great Orion-Nebula.&lt;/p&gt;
&lt;div class="docutils container"&gt;
&lt;figure class="align-center" style="width: 80%"&gt;
&lt;a class="reference external image-reference" href="https://spacephoto.de/galleries/02_nebulas/140_NGC_1975_cOri_8x300s_RGB_DT_WM.jpg"&gt;
&lt;img alt="&amp;lt;/galleries/02_nebulas/140_NGC_1975_cOri_8x300s_RGB_DT_WM.jpg&amp;gt;" src="https://spacephoto.de/galleries/02_nebulas/140_NGC_1975_cOri_8x300s_RGB_DT_WM.jpg"&gt;
&lt;/a&gt;
&lt;figcaption&gt;
&lt;p&gt;Image Data: NGC 1977, the "Running Man Nebula", Telescope Newton 10" f/4, Camera Atik 460EXM, 8x300s per Channel, RGB&lt;/p&gt;
&lt;/figcaption&gt;
&lt;/figure&gt;
&lt;/div&gt;
&lt;p&gt;&lt;a href="https://spacephoto.de/blog/NGC%201977/"&gt;Read more…&lt;/a&gt; (1 min remaining to read)&lt;/p&gt;&lt;/div&gt;</description><category>Atik460Exm</category><category>FN250</category><category>nebula</category><category>reflection nebula</category><guid>https://spacephoto.de/blog/NGC%201977/</guid><pubDate>Sat, 11 Mar 2023 13:00:00 GMT</pubDate></item><item><title>Tadpoles in the Cosmic Pond: IC 410 and NGC 1893</title><link>https://spacephoto.de/blog/IC%20410%2C%20NGC%201893/</link><dc:creator>Martin Timpe</dc:creator><description>&lt;div&gt;&lt;p&gt;In the constellation Auriga on clear winter nights one can find the open cluster NGC 1893 embedded in the emission nebula IC 410.
While NGC 1893 can be observed visually using a telescope with proper aperture the faint nebula IC 410 is a real hard case for the visual
observer and much easier to catch by photography.
Due to some smaller but prominent star formation regions the nebula IC 410 is nicknamed as the "tadpole nebula".
IC 410 was discovered on September 25, 1892 by the (german) astronomer Max Wolf (June 21, 1863 - October 3, 1932) while the
open cluster NGC 1893 was discovered already earlier on January 22, 1827 by the (british) astronomer
John Herschel (Mar 7, 1792 - May 11, 1871).&lt;/p&gt;
&lt;div class="docutils container"&gt;
&lt;figure class="align-center" style="width: 80%"&gt;
&lt;a class="reference external image-reference" href="https://spacephoto.de/galleries/02_nebulas/131_IC410_NGC1893_SHO_NG_600s_10xHa_11xO3_15xS2_DT_WM.jpg"&gt;
&lt;img alt="&amp;lt;/galleries/02_nebulas/131_IC410_NGC1893_SHO_NG_600s_10xHa_11xO3_15xS2_DT_WM.jpg&amp;gt;" src="https://spacephoto.de/galleries/02_nebulas/131_IC410_NGC1893_SHO_NG_600s_10xHa_11xO3_15xS2_DT_WM.jpg"&gt;
&lt;/a&gt;
&lt;figcaption&gt;
&lt;p&gt;IC 410 and NGC 1893, camera Atik 460EXmono, optics Lacerta Newton f=1000mm f/4, 2023-02-08, Bad Kreuznach, Germany&lt;/p&gt;
&lt;/figcaption&gt;
&lt;/figure&gt;
&lt;/div&gt;
&lt;p&gt;What can be seen in the image is what cannot be seen visually through a telescope. The image
is presented in false colors resulting from an (amongst astro-photographers
widely known) image acquisition technique using narrow band filters.&lt;/p&gt;
&lt;p&gt;&lt;a href="https://spacephoto.de/blog/IC%20410%2C%20NGC%201893/"&gt;Read more…&lt;/a&gt; (4 min remaining to read)&lt;/p&gt;&lt;/div&gt;</description><category>Atik460Exm</category><category>emission nebula</category><category>FN250</category><category>open cluster</category><guid>https://spacephoto.de/blog/IC%20410%2C%20NGC%201893/</guid><pubDate>Sun, 19 Feb 2023 23:00:00 GMT</pubDate></item></channel></rss>